diff -Nru debian-astro-0.3/debian/changelog debian-astro-0.4/debian/changelog --- debian-astro-0.3/debian/changelog 2016-04-15 15:15:17.000000000 +0000 +++ debian-astro-0.4/debian/changelog 2016-07-25 07:50:35.000000000 +0000 @@ -1,3 +1,14 @@ +debian-astro (0.4) unstable; urgency=medium + + [ Paul Sladen ] + * Add new metapackage 'virtual-observatory' + + [ Ole Streicher ] + * Add new metapackage "radioastronomy" + * Update for newly introduced and announced packages + + -- Ole Streicher Mon, 25 Jul 2016 09:50:08 +0200 + debian-astro (0.3) unstable; urgency=medium * Raise Priority to 'optional' diff -Nru debian-astro-0.3/debian/control debian-astro-0.4/debian/control --- debian-astro-0.3/debian/control 2016-04-15 15:16:29.000000000 +0000 +++ debian-astro-0.4/debian/control 2016-07-25 07:52:08.000000000 +0000 @@ -3,7 +3,8 @@ Section: science Priority: optional Maintainer: Debian Astro Team -Uploaders: Ole Streicher +Uploaders: Ole Streicher , + Paul Sladen Build-Depends-Indep: blends-dev (>= 0.6.15) Standards-Version: 3.9.8 Vcs-Browser: https://anonscm.debian.org/cgit/blends/projects/astro.git @@ -25,8 +26,7 @@ Package: astro-all Section: metapackages Architecture: all -Recommends: astro-catalogs, - astro-datareduction, +Recommends: astro-datareduction, astro-development, astro-education, astro-frameworks, @@ -34,12 +34,15 @@ astro-java, astro-publication, astro-python3, + astro-radioastronomy, astro-simulation, - astro-tcltk, astro-telescopecontrol, astro-tools, astro-viewers -Suggests: astro-python +Suggests: astro-catalogs, + astro-python, + astro-tcltk, + astro-virtual-observatory Description: Default selection of tasks for Debian Astro This package is part of the Debian Astro Pure Blend and installs all tasks for a default installation of this blend. @@ -64,11 +67,16 @@ Depends: astro-tasks (= ${binary:Version}) Recommends: astromatic, astrometry.net, + esorex, montage, - python3-cpl | python-cpl | esorex + python3-astroscrappy | python-astroscrappy, + python3-cpl | python-cpl, + python3-montage-wrapper | python-montage-wrapper Suggests: cpl-plugin-amber, cpl-plugin-fors, cpl-plugin-giraf, + crush, + munipack, theli Description: Data reduction pipelines for astronomy The term data reduction in astronomy means the data processing from the raw @@ -83,7 +91,9 @@ Section: metapackages Architecture: all Depends: astro-tasks (= ${binary:Version}) -Recommends: libastro-fits-cfitsio-perl, +Recommends: casacore-dev, + giza-dev, + libastro-fits-cfitsio-perl, libastrometry-dev, libatlas-dev, libccfits-dev, @@ -101,8 +111,7 @@ libstarlink-ast-dev, libstarlink-pal-dev, libwcstools-dev -Suggests: casacore-dev, - libnexstar-dev, +Suggests: libnexstar-dev, libpgsbox-dev, libsofa-c-dev, pgplot5, @@ -140,12 +149,12 @@ Section: metapackages Architecture: all Depends: astro-tasks (= ${binary:Version}) -Recommends: eso-midas, +Recommends: dpuser, + eso-midas, pdl, scilab, yorick-full -Suggests: dpuser, - iraf +Suggests: iraf Description: Astronomical data analysis frameworks This metapackage will install large astronomical data analysis frameworks, which usually provide their own script language. @@ -170,15 +179,17 @@ Section: metapackages Architecture: all Depends: astro-tasks (= ${binary:Version}) -Recommends: libfits-java +Recommends: libcds-moc-java, + libcds-savot-java, + libfits-java, + libhealpix-java, + libjsamp-java Suggests: libcds-astro-java, - libcds-moc-java, - libivoafits-java, - libjsamp-java, - libsavot-java + libivoafits-java Description: Java packages for astronomy This metapackage will install packages that are useful to develop Java - applications for astronomy. + applications for astronomy. Apart vom FITS file handling, this is mainly used + for VO applications. Package: astro-publication Section: metapackages @@ -214,31 +225,38 @@ python-astropy-affiliated, python-astroquery, python-astroscrappy, + python-casacore, python-emcee, python-ephem, + python-fitsio, python-gdl, + python-ginga, python-gyoto, python-healpy, python-matplotlib, python-numpy, python-pyavm, python-pyds9, + python-pyfftw, python-pysynphot, + python-reproject, python-scipy, python-sunpy, python-yt Suggests: python-astroplan, - python-fitsio, python-galpy, python-gammapy, python-pyfits, python-pywcs, - python-reproject, python-sherpa, python-sncosmo Description: Python 2 packages for astronomy This metapackage will install Python 2 packages for astronomy. The packages can be used for interactive analysis, or to create specific programs. + . + Note that Python 2 is legacy only, Python 3 is the present and future of the + language. The support for Python 2 will end in 2020. Please use Python 2 only + if you don't have a choice. Package: astro-python3 Section: metapackages @@ -249,33 +267,70 @@ python3-aplpy, python3-asdf, python3-astlib, + python3-astroml, python3-astropy, python3-astropy-affiliated, python3-astroquery, python3-astroscrappy, + python3-casacore, python3-emcee, python3-ephem, + python3-fitsio, + python3-ginga, python3-gyoto, python3-healpy, python3-matplotlib, python3-numpy, python3-pyavm, python3-pyds9, + python3-pyfftw, + python3-reproject, python3-scipy, + python3-sunpy, python3-yt -Suggests: python3-astroml, - python3-astroplan, - python3-fitsio, +Suggests: python3-astroplan, python3-galpy, python3-gammapy, python3-pyfits, - python3-reproject, python3-sherpa, python3-sncosmo Description: Python 3 packages for astronomy This metapackage will install Python 3 packages for astronomy. The packages can be used for interactive analysis, or to create specific programs. +Package: astro-radioastronomy +Section: metapackages +Architecture: all +Depends: astro-tasks (= ${binary:Version}) +Recommends: casacore-dev, + python3-casacore, + python3-spectral-cube +Suggests: aoflagger, + casarest, + casasynthesis, + cassbeam, + lofar, + meqtrees-timba, + mt-imager, + oskar, + parseltongue, + purify, + python-casacore, + python-meqtrees-cattery, + python-meqtrees-timba, + python-owlcat, + python-pymoresane, + python-pyxis, + python-spectral-cube, + python-tigger, + rpfits, + sagecal, + wsclean +Description: Radio Astronomy Software + This metapackage will install Debian Astro packages for radio astronomy. It + should contain most of the required tools that a radio astronomer require for + setting up a data reduction pipeline. + Package: astro-simulation Section: metapackages Architecture: all @@ -285,6 +340,8 @@ python-yt, splash, yorick-yao +Suggests: cloudy, + mocassin Description: Simulation packages for astronomy This metapackage will install packages for celectial, astronomical and cosmological simulations. @@ -293,7 +350,7 @@ Section: metapackages Architecture: all Depends: astro-tasks (= ${binary:Version}) -Recommends: blt, +Recommends: blt-dev, ftools-pow, skycat, tcl-fitstcl, @@ -301,6 +358,7 @@ tcl-xpa, tcl8.6, tk8.6, + tkblt-dev, tksao Description: Tcl/Tk packages for astronomy This metapackage will install packages that are useful to develop Tcl/Tk @@ -312,6 +370,7 @@ Depends: astro-tasks (= ${binary:Version}) Recommends: gcx, indi-bin, + kstars, lynkeos.app, wxastrocapture Suggests: audela, @@ -324,24 +383,24 @@ Section: metapackages Architecture: all Depends: astro-tasks (= ${binary:Version}) -Recommends: asdftool, +Recommends: alfa, + asdftool, astronomical-almanac, astropy-utils, - boinc-app-milkyway, boinc-app-seti, + casacore-tools, fitscut, + fitspng, fitsverify, funtools, + neat, qfits-tools, rawtran, siril, wcslib-tools, wcstools, xpa-tools -Suggests: alfa, - casacore-tools, - fitspng, - neat +Suggests: boinc-app-milkyway Description: Astronomy tools and utilities This metapackage will install small tools provided by Debian Astronomy packages. These tools handle smaller tasks, mainly dealing with FITS files. @@ -351,19 +410,47 @@ Architecture: all Depends: astro-tasks (= ${binary:Version}) Recommends: ftools-fv, + ginga, glueviz, ifrit, imagej, mayavi2, paraview, + qfitsview, saods9, skycat, yorick-cubeview, yorick-spydr -Suggests: qfitsview, - vo-aladin +Suggests: aladin Description: Interactive astronomical data viewers This metapackage will install software for the interactive visual inspection of astronomical data. Note that Python packages can be used for interactive inspection as well within the ipython environment. +Package: astro-virtual-observatory +Section: metapackages +Architecture: all +Depends: astro-tasks (= ${binary:Version}) +Recommends: libcds-moc-java, + libcds-savot-java, + libjsamp-java +Suggests: aladin, + splat-vo, + stilts, + tapsh, + topcat +Description: Tools and viewers for the Virtual Observatory + This metapackage will install commonly used interfaces for interacting with + datasets and archive data within the online distributed Virtual Observatory. + . + The Virtual Observatory allows astronomers to interrogate multiple data + centers in a seamless and transparent way, provides new powerful analysis and + visualization tools within that system, and gives data centers a standard + framework for publishing and delivering services using their data. This is + made possible by standardization of data and metadata, by standardization of + data exchange methods, and by the use of a registry, which lists available + services and what can be done with them. + . + When running, many of these tools can communicate with each other + using the Simple Application Messaging Protocol (SAMP) + diff -Nru debian-astro-0.3/debian/control.stub debian-astro-0.4/debian/control.stub --- debian-astro-0.3/debian/control.stub 2016-04-15 15:16:34.000000000 +0000 +++ debian-astro-0.4/debian/control.stub 2016-06-16 07:38:34.000000000 +0000 @@ -2,7 +2,8 @@ Section: science Priority: optional Maintainer: Debian Astro Team -Uploaders: Ole Streicher +Uploaders: Ole Streicher , + Paul Sladen Build-Depends-Indep: blends-dev (>= 0.6.15) Standards-Version: 3.9.8 Vcs-Browser: https://anonscm.debian.org/cgit/blends/projects/astro.git diff -Nru debian-astro-0.3/debian-astro-tasks.desc debian-astro-0.4/debian-astro-tasks.desc --- debian-astro-0.3/debian-astro-tasks.desc 2016-04-15 15:14:58.000000000 +0000 +++ debian-astro-0.4/debian-astro-tasks.desc 2016-07-25 07:52:08.000000000 +0000 @@ -11,7 +11,6 @@ This metapackage will install a selection astronomical catalogs. Please note that due to their size, most catalogs are not included in Debian. Check the CDS web service for additional catalogs if needed. -Test-new-install: mark show Key: astro-catalogs @@ -80,7 +79,8 @@ Section: debian-astro Description: Java packages for astronomy This metapackage will install packages that are useful to develop Java - applications for astronomy. + applications for astronomy. Apart vom FITS file handling, this is mainly used + for VO applications. Test-new-install: mark show Key: astro-java @@ -101,6 +101,10 @@ Description: Python 2 packages for astronomy This metapackage will install Python 2 packages for astronomy. The packages can be used for interactive analysis, or to create specific programs. + . + Note that Python 2 is legacy only, Python 3 is the present and future of the + language. The support for Python 2 will end in 2020. Please use Python 2 only + if you don't have a choice. Key: astro-python @@ -114,6 +118,17 @@ Key: astro-python3 +Task: astro-radioastronomy +Parent: debian-astro +Section: debian-astro +Description: Radio Astronomy Software + This metapackage will install Debian Astro packages for radio astronomy. It + should contain most of the required tools that a radio astronomer require for + setting up a data reduction pipeline. +Test-new-install: mark show +Key: + astro-radioastronomy + Task: astro-simulation Parent: debian-astro Section: debian-astro @@ -130,7 +145,6 @@ Description: Tcl/Tk packages for astronomy This metapackage will install packages that are useful to develop Tcl/Tk applications for astronomy. -Test-new-install: mark show Key: astro-tcltk @@ -165,3 +179,23 @@ Key: astro-viewers +Task: astro-virtual-observatory +Parent: debian-astro +Section: debian-astro +Description: Tools and viewers for the Virtual Observatory + This metapackage will install commonly used interfaces for interacting with + datasets and archive data within the online distributed Virtual Observatory. + . + The Virtual Observatory allows astronomers to interrogate multiple data + centers in a seamless and transparent way, provides new powerful analysis and + visualization tools within that system, and gives data centers a standard + framework for publishing and delivering services using their data. This is + made possible by standardization of data and metadata, by standardization of + data exchange methods, and by the use of a registry, which lists available + services and what can be done with them. + . + When running, many of these tools can communicate with each other + using the Simple Application Messaging Protocol (SAMP) +Key: + astro-virtual-observatory + diff -Nru debian-astro-0.3/tasks/astroconda debian-astro-0.4/tasks/astroconda --- debian-astro-0.3/tasks/astroconda 1970-01-01 00:00:00.000000000 +0000 +++ debian-astro-0.4/tasks/astroconda 2016-05-07 12:43:05.000000000 +0000 @@ -0,0 +1,378 @@ +Task: AstroConda +Install: false +Index: false +Leaf: false +Metapackage: false +Description: AstroConda packages + Here we list the status of the packages that belong to the + [AstroConda](http://astroconda.readthedocs.io) + distribution. AstroConda is a free software repository maintained by the + [Space Telescope Science Institute (STScI)](http://www.stsci.edu/) in + Baltimore, Maryland. AstroConda provides tools and utilities commonly used by + the astronomical community. + +Depends: acstools +Homepage: http://acstools.readthedocs.io/ +Pkg-Description: Python Tools for ACS (Advanced Camera for Surveys) Data + +Depends: wfpc2tools +Homepage: http://www.stsci.edu/resources/software_hardware/stsci_python +Pkg-Description: Tools for use with the Wide Field and Planetary Camera 2 + +Depends: calcos +Homepage: https://github.com/spacetelescope/calcos +Pkg-Description: Calibration for HST/COS + +Depends: hstcal +Homepage: https://github.com/spacetelescope/hstcal +Pkg-Description: Calibration for HST/WFC3, HST/ACS, and HST/STIS + +Depends: nictools +Homepage: https://github.com/spacetelescope/nictools +Pkg-Description: Tools for HST/NICMOS + +Depends: jwst-lib +Homepage: ssh://git@bitbucket.org/stsci_ssb/jwst.git +Pkg-Description: James Webb Space Telescope library + +Depends: jwst-pipeline +Homepage: http://ssb.stsci.edu/doc/jwst_dev/jwst_pipeline.pipeline.doc.user_guide.doc/html/index.html +Pkg-Description: James Webb Space Telescope pipeline + +Depends: jwst-tools +Homepage: ssh://git@bitbucket.org/stsci_ssb/jwst.git +Pkg-Description: James Webb Space Telescope tools + +Depends: wfc3tools +Homepage: http://ssb.stsci.edu/doc/stsci_python_2.15.1/wfc3tools.doc/html/index.html +Pkg-Description: Tools for the Hubble Space Telescope Wide Field Camera 3 + +Depends: reftools +Homepage: http://www.stsci.edu/institute/software_hardware/pyraf/stsci_python +Pkg-Description: Tools for HST reference files + +Depends: stistools +Homepage: http://www.stsci.edu/institute/software_hardware/pyraf/stsci_python +Pkg-Description: Tools for working with STIS data + +Depends: costools +Homepage: http://www.stsci.edu/institute/software_hardware +Pkg-Description: Tools for working with COS data + +Depends: crds +Homepage: http://www.stsci.edu/hst/observatory/crds/ +Pkg-Description: Calibration Reference Data System + +Depends: stsci.sphere +Homepage: http://ssb.stsci.edu/doc/stsci_python_x/stsci.sphere.doc/html/user.html +Pkg-Description: STScI's spherical geometry astropy package + Python package for handling spherical polygons that represent arbitrary + regions of the sky.sphere +Remark: + Package is outdated and replaced by Scipy + +Depends: stsci.skypac +Homepage: https://github.com/spacetelescope/stsci.skypac +Pkg-Description: Sky matching for image mosaic +Remark: + Package is outdated and replaced by Scipy + +Depends: stsci.convolve +Homepage: https://github.com/spacetelescope/stsci.convolve +Pkg-Description: Subset of SciPy functionality for convolving + Formerly included in SciPy as scipy.stsci.convolve. +Remark: + Package is outdated and replaced by Scipy + +Suggests: python3-stsci.distutils | python-stsci.distutils +Remark: + Package is outdated + +Depends: stsci.image +Homepage: https://github.com/spacetelescope/stsci.image +Pkg-Description: Image array manipulation functions +Remark: + Package is outdated and replaced by Scipy + +Depends: stsci.imagemanip +Homepage: https://github.com/spacetelescope/stsci.imagemanip +Pkg-Description: STScI general image manipulation tools +Remark: + Package is outdated and replaced by Scipy + +Depends: stsci.imagestats +Homepage: https://github.com/spacetelescope/stsci.imagestats +Pkg-Description: Compute various useful statistical values for array objects +Remark: + Package is outdated and replaced by Scipy + +Depends: stsci.ndimage +Homepage: https://github.com/spacetelescope/stsci.ndimage +Pkg-Description: Fork of scipy.ndimage +Remark: + Package is outdated and replaced by Scipy + +Depends: stsci.numdisplay +Homepage: http://stsdas.stsci.edu/numdisplay +Pkg-Description: Visualize numpy array objects + Visualize numpy array objects using image display tools like ds9 and ximtool +Remark: + Package is outdated and may be replaced by pyds9. + +Depends: stsci.stimage +Homepage: https://github.com/spacetelescope/stsci.stimage +Pkg-Description: Various functions for performing processing of images +Remark: + Package is outdated and replaced by Scipy + +Depends: stsci.tools +Homepage: https://github.com/spacetelescope/stsci.tools +Pkg-Description: STScI utility functions +Remark: + Package is outdated and replaced by Scipy + +Depends: asv +Homepage: http://asv.readthedocs.io/ +Pkg-Description: Simple Python benchmarking tool with web-based reporting + airspeed velocity (asv) is a tool for benchmarking Python packages over their + lifetime. Runtime, memory consumption and even custom-computed values may be + tracked. The results are displayed in an interactive web frontend that + requires only a basic static webserver to host. + +Depends: cube-tools +Homepage: https://github.com/spacetelescope/cube-tools +Pkg-Description: Data analysis package for cubes + +Depends: fitsblender +Homepage: http://ssb.stsci.edu/doc/stsci_python_dev/fitsblender.doc/html/index.html +Pkg-Description: FITS header merging from multiple images. + Given a list of FITS headers, aggregates values and creates a table made up + of values from a number of headers, according to the given specification. + +Depends: stwcs +Homepage: https://github.com/spacetelescope/stwcs +Pkg-Description: WCS based distortion models and coordinate transformation + Recomputes the WCS of an HST observation and puts all distortion + corrections in the headers. + +Depends: specview +Homepage: https://github.com/spacetelescope/specview +Pkg-Description: Java spectrum visualization, manipulation, and fitting + Specview is a tool for 1-D spectral visualization and analysis of + astronomical spectrograms. Written in Java, it is capable of reading all + the Hubble Space Telescope spectral data formats as well as data from + several other instruments (such as IUE, FUSE, ISO, FORS and SDSS), + preview spectra from MAST, and data from generic FITS and ASCII tables. + It can read data from Virtual Observatory servers, and read and write + spectrogram data in Virtual Observatory SED format. It can also read + files in the SPC Galactic format used in the chemistry field. Once + ingested, data can be plotted and examined with a large selection of + custom settings. Specview supports instrument-specific data quality + handling, flexible spectral units conversions, custom plotting + attributes, plot annotations, tiled plots, hardcopy to JPEG files and + PostScript file or printer, etc. Specview can be used to build wide-band + SEDs, overplotting or combining data from the same astronomical source + taken with different instruments and/or spectral bands. Data can be + further processed with averaging, splicing, detrending, and Fourier + filtering tools. Specview has a spectral model fitting capability that + enables the user to work with multi-component models (including user- + defined models) and fit models to data. + +Depends: stginga +Homepage: https://github.com/spacetelescope/stginga +Pkg-Description: Ginga products specific to STScI data analysis + +Depends: python3-pyregion | python-pyregion + +Depends: python3-asdf | python-asdf + +Depends: asdf-standard +Homepage: http://asdf-standard.readthedocs.io/ +Pkg-Description: Advanced Scientific Data Format documentation + Advanced Scientific Data Format is a proposed replacement to the FITS + standard for astronomical images and other astronomical data. The Metadata is + contained in a YAML header followed by binary or ascii data. + +Depends: astrolib.coords +Homepage: http://ssb.stsci.edu/doc/stsci_python_dev/astrolib.coords.doc/html/index.html +Pkg-Description: Astronomical coordinates & angular separations + This package aims to provide much of the IDL "astron" functionality that + pertains to coordinate manipulations in an OO framework. Our target user is a + typical astronomer who needs to analyze data, work with catalogs, prepare + observing proposals, and prepare for observing runs. +Remark: + This packages is obsolete and replaced by astrolib.coordinates. + +Depends: python3-photutils | python-photutils + +Depends: python3-pyds9 | python-pyds9 + +Depends: libxpa-dev + +Depends: libcfitsio-dev + +Depends: saods9 + +Depends: wcstools + +Depends: python-pysynphot + +Suggests: python-pywcs +Remark: + This package is obsoleted by python3-astropy. Please use + python3-astropy instead. + +Depends: pyraf +WNPP: 711038 +Homepage: https://github.com/spacetelescope/pyraf +Pkg-Description: Python replacement for IRAF cl from STScI + PyRAF is a command language for running IRAF tasks that is based on the + Python scripting language. It gives users the ability to run IRAF tasks + in an environment that has all the power and flexibility of Python. + PyRAF can be installed along with an existing IRAF installation; users + can then choose to run either PyRAF or the IRAF CL. + +Depends: iraf +WNPP: 690531 +Homepage: http://iraf.noao.edu +Pkg-Description: NOAO Image Reduction and Analysis Facility + IRAF includes a broad selection of programs for general image processing + and graphics, plus a large number of programs for the reduction and + analysis of optical and IR astronomy data. Other external or layered + packages are available for applications such as data acquisition or + handling data from other observatories and wavelength regimes such as + the Hubble Space Telescope (optical), EUVE (extreme ultra-violet), or + ROSAT and AXAF (X-ray). These external packages are distributed + separately from the main IRAF distribution but can be easily installed. + The IRAF system also includes a complete programming environment for + scientific applications, which includes a programmable Command Language + scripting facility, the IMFORT Fortran/C programming interface, and the + full SPP/VOS programming environment in which the portable IRAF system + and all applications are written. + +Depends: ginga +WNPP: 823598 +Homepage: https://github.com/ejeschke/ginga +Pkg-Description: The Ginga astronomical FITS file viewer + Ginga is a viewer for astronomical data FITS (Flexible Image Transport + System) files; the viewer centers around a FITS display widget which + supports zooming and panning, color and intensity mapping, a choice of + several automatic cut levels algorithms and canvases for plotting + scalable geometric forms. In addition to this widget, the FITS viewer + provides a flexible plugin framework for extending the viewer with many + different features. A fairly complete set of "standard" plugins are + provided for expected features of a modern viewer: panning and zooming + windows, star catalog access, cuts, star pick/fwhm, thumbnails, and + others. This viewer was written by software engineers at Subaru + Telescope, National Astronomical Observatory of Japan, and is in use at + that facility. + +Depends: python3-astropy | python-astropy + +Depends: imexam +Homepage: http://imexam.readthedocs.io +Pkg-Description: Simple image examination, and plotting, with similar functionality to IRAF's imexamine + imexam is an AstroPy affiliated package meant for quick image analysis, much + like the IRAF imexamine task. Image display is currently supported with + either DS9 or a Ginga widget from a python session. + +Depends: gwcs +Homepage: http://gwcs.readthedocs.io/ +Pkg-Description: Tools for managing the WCS in a general way + GWCS takes a general approach to WCS. It supports a data model which includes + the entire transformation pipeline from input coordinates (detector by + default) to world cooridnates. Transformations can be chained, joined or + combined with arithmetic operators using the flexible framework of compound + models in modeling. In the case of a celestial output frame coordinates + provides further transformations between standard coordinate frames. Spectral + output coordinates are instances of Quantity and are transformed to other + units with the tools in that package. The goal is to provide a flexible + toolkit which is easily extendable by adding new transforms and frames. + +Depends: astroimtools +Homepage: http://astroimtools.readthedocs.io +Pkg-Description: Astronomical Image Convenience Tools + Astroimtools is an open-source Python package to provide convenience tools + for working with astronomical images. + . + This work is driven by the JWST Data Analysis Development Forum at the Space + Telescope Science Institute. + +Depends: drizzlepac +Homepage: http://drizzlepac.stsci.edu/ +Pkg-Description: Align and combine HST images + DrizzlePac allows users to easily and accurately align and combine HST + images taken at multiple epochs, and even with different instruments. It + is a suite of supporting tasks for AstroDrizzle which + includes:astrodrizzle to align and combine imagestweakreg and tweakback + for aligning images in different visitspixtopix transforms an X,Y pixel + position to its pixel position after distortion correctionsskytopix + transforms sky coordinates to X,Y pixel positions. A reverse + transformation can be done using the task pixtosky. +Remark: + Depends on stsci.tools, stsci.convolve, stsci.image, stsci.imagemanip, + stsci.imagestats, stsci.ndimage, stsci.stimage, nictools, stwcs, fitsblender, + and astrolib.coords. + + +Depends: python3-numpy | python-numpy + +Depends: python3-scipy | python-scipy + +Depends: python3-pyfftw | python-pyfftw + +Depends: poppy +Homepage: https://github.com/mperrin/poppy +Pkg-Description: Physical Optics Propagation in Python + POPPY (Physical Optics Propagation in PYthon) simulates physical optical + propagation including diffraction. It implements a flexible framework + for modeling Fraunhofer and Fresnel diffraction and point spread + function formation, particularly in the context of astronomical + telescopes. POPPY provides the optical modeling framework for WebbPSF + (ascl:1504.007) and was developed as part of a simulation package for + JWST, but is available separately and is broadly applicable to many + kinds of imaging simulations. + +Depends: webbpsf +Homepage: http://www.stsci.edu/jwst/software/webbpsf/ +Pkg-Description: WebbPSF: Simulated PSF for the James Webb Space Telescope + WebbPSF provides a PSF simulation tool in a flexible and easy-to-use + software package implemented in Python. Functionality includes support + for spectroscopic modes of JWST NIRISS, MIRI, and NIRSpec, including + modeling of slit losses and diffractive line spread functions. + +Depends: libfftw3-dev + +Depends: htc-utils +Homepage: http://bitbucket.org/jhunkeler/htc_utils +Pkg-Description: Homebrew set of HTCondor wrappers + HTCondor is a specialized workload management system for compute-intensive + jobs. Like other full-featured batch systems, HTCondor provides a job + queueing mechanism, scheduling policy, priority scheme, resource monitoring, + and resource management. Users submit their serial or parallel jobs to + HTCondor, HTCondor places them into a queue, chooses when and where to run + the jobs based upon a policy, carefully monitors their progress, and + ultimately informs the user upon completion. + . + This package installs some home-rolled Condor utilities. + +Depends: python3-appdirs | python-appdirs + +Depends: python3-d2to1 | python-d2to1 + +Depends: recon +Homepage: http://github.com/jhunkeler/recon +Pkg-Description: Release control for git + RELIC stands for "Release I Control". This software attempts to automatically + maintain a git project's version information without the need for hardcoded + values in the source code. It is designed primarily for hardcore build + maintainers, and is best used with continuous integration services (i.e + Travis-CI, etc). + +Depends: python3-pytools | python-pytools + +Depends: purge-path +Homepage: http://bitbucket.org/jhunkeler/purge_path +Pkg-Description: Small PATH manipulator + +Depends: shunit2 diff -Nru debian-astro-0.3/tasks/catalogs debian-astro-0.4/tasks/catalogs --- debian-astro-0.3/tasks/catalogs 2016-04-03 12:54:12.000000000 +0000 +++ debian-astro-0.4/tasks/catalogs 2016-04-19 11:36:10.000000000 +0000 @@ -1,4 +1,5 @@ Task: Catalogs +Install: false Description: Astronomy catalogs This metapackage will install a selection astronomical catalogs. Please note that due to their size, most catalogs are not included in Debian. Check the diff -Nru debian-astro-0.3/tasks/datareduction debian-astro-0.4/tasks/datareduction --- debian-astro-0.3/tasks/datareduction 2016-04-04 13:40:51.000000000 +0000 +++ debian-astro-0.4/tasks/datareduction 2016-05-24 09:23:48.000000000 +0000 @@ -1,4 +1,5 @@ Task: Data Reduction +Install: true Description: Data reduction pipelines for astronomy The term data reduction in astronomy means the data processing from the raw exposures up to scientific usable data. This includes the basic CCD @@ -8,7 +9,7 @@ This metapackage will install astronomy data reduction pipelines that can be used universally, but also those for specific telescopes. -Depends: python3-cpl | python-cpl | esorex, +Depends: python3-cpl | python-cpl, esorex, eso-pipelines Suggests: cpl-plugin-amber, cpl-plugin-fors, cpl-plugin-giraf, cpl-plugin-hawki, cpl-plugin-sinfo, cpl-plugin-kmos, @@ -21,7 +22,11 @@ Depends: astrometry.net -Depends: montage +Depends: montage, python3-montage-wrapper | python-montage-wrapper + +Depends: python3-astroscrappy | python-astroscrappy, + python3-ccdproc | python-ccdproc, + python3-photutils | python-photutils Depends: theli WNPP: 780303 @@ -42,3 +47,24 @@ * Absolute flux calibration * Extensive documentation and online help Homepage: https://www.astro.uni-bonn.de/theli/index.html + +Depends: crush +WNPP: 815714 +Pkg-Description: Data reduction and imaging tool for astronomical cameras + CRUSH is an astronomical data reduction/imaging tool for certain + astronomical cameras. Currently, it supports SHARC, SHARC-2, LABOCA, + SABOCA, ASZCA, p-ArTeMiS, PolKa, GISMO, MAKO, MAKO-2, MUSTANG-2, and + SCUBA-2. +Homepage: http://www.submm.caltech.edu/~sharc/crush/ + +Depends: munipack +WNPP: 824746 +Pkg-Description: Astronomical photometry software package + Munipack is a general astronomical photometry software package + designed for both batch and interactive processing of large + amount of data. One currently implements functions for image + preprocessing, aperture and growth-curve photometry, astrometry + and photometry calibration, merge of images, light-curves, + partial support for Virtual observatory access, FITS files tool + and a graphical interface. +Homepage: http://munipack.physics.muni.cz/ diff -Nru debian-astro-0.3/tasks/development debian-astro-0.4/tasks/development --- debian-astro-0.3/tasks/development 2016-04-14 15:36:45.000000000 +0000 +++ debian-astro-0.4/tasks/development 2016-06-29 07:56:19.000000000 +0000 @@ -1,4 +1,5 @@ Task: Development +Install: true Description: C/C++ development packages for astronomy This metapackage will install Debian Astro packages which might be helpful for the development of (mainly C/C++) astronomical applications. Note @@ -27,8 +28,15 @@ Depends: libhdf5-dev -Suggests: pgplot5, libpgsbox-dev +Depends: giza-dev +Suggests: pgplot5 +Remark: + Giza-dev is a DFSG-free replacement for pgplot5. +Suggests: libpgsbox-dev +Remark: + In Debian Stretch, this package is integrated in wcslib-dev. + Suggests: libsofa-c-dev Remark: This package is included for reference only. It can be fully replaced @@ -48,3 +56,4 @@ SkyWatcher: EQ5, HEQ5, EQ6 (Pro), AZ-EQ5 GT, AZ-EQ6 GT, EQ8 etc. and the corresponding Orion mounts. Homepage: https://sourceforge.net/projects/libnexstar + diff -Nru debian-astro-0.3/tasks/education debian-astro-0.4/tasks/education --- debian-astro-0.3/tasks/education 2016-03-07 21:30:54.000000000 +0000 +++ debian-astro-0.4/tasks/education 2016-05-24 09:23:48.000000000 +0000 @@ -1,4 +1,5 @@ Task: Education +Install: true Description: Educational astronomy applications This metapackage depends on various applications that can be used to teach astronomy. diff -Nru debian-astro-0.3/tasks/fedora debian-astro-0.4/tasks/fedora --- debian-astro-0.3/tasks/fedora 1970-01-01 00:00:00.000000000 +0000 +++ debian-astro-0.4/tasks/fedora 2016-05-10 03:44:02.000000000 +0000 @@ -0,0 +1,173 @@ +Task: Fedora +Install: false +Index: false +Metapackage: false +Description: Fedora Astronomy Spin + Here we list the packages that belong to the + [Fedora Astronomy Spin](https://fedoraproject.org/wiki/Astronomy_Spin). + The goal is to create a Live media Fedora spin containing a set of tools for + astronomers and astrophysicists. This includes observatory control as well as + scientific data analysis and astrophotography. + +Depends: cdsclient +Homepage: http://cdsarc.u-strasbg.fr/doc/cdsclient.html +Pkg-Description: Tools to query databases at CDS + The cdsclient package is a set of C and shell routines which can be built on + Unix stations or PCs running Linux, which once compiled allow to query some + databases located at CDS or on mirrors over the network. + +Depends: libcfitsio-bin + +Depends: gcx + +Depends: psfex + +Depends: saods9 +Remark: + Fedora includes the predessor saoimage instead. + +Depends: scamp + +Depends: sextractor + +Depends: siril + +Depends: skyviewer +Homepage: http://lambda.gsfc.nasa.gov/toolbox/tb_skyviewer_ov.cfm +Pkg-Description: Program to display HEALPix-based skymaps in FITS files + SkyViewer is an OpenGL based program to display HEALPix-based skymaps, saved + in FITS format files. The loaded skymaps can be viewed either on a 3D sphere + or as a Mollweide projection. In either case, realtime panning and zooming + are supported, along with rotations for the 3D sphere view, assuming you have + a strong enough graphics card. + +Depends: swarp + +Depends: indi-plugins +Remark: + The Debian package includes the plugins that are separate packages on Fedora: + indi-sx, indi-gphoto, indi-eqmod, indi-apogee, indi-aagcloudwatcher + +Depends: indi-bin + +Depends: kstars + +Depends: skychart +Homepage: http://www.ap-i.net/skychart +Pkg-Description: Planetarium software for the advanced amateur astronomer + This program enables you to draw sky charts, making use of the data in 16 + catalogs of stars and nebulae. In addition the position of planets, asteroids + and comets are shown. + . + The purpose of this program is to prepare different sky maps for a particular + observation. A large number of parameters help you to choose specifically or + automatically which catalogs to use, the colour and the dimension of stars + and nebulae, the representation of planets, the display of labels and + coordinate grids, the superposition of pictures, the condition of visibility + and more. All these features make this celestial atlas more complete than a + conventional planetarium. + +Depends: stellarium + +Depends: celestia + +Depends: python3 | python + +Depends: idle3 | idle + +Depends: python3-matplotlib | python-matplotlib + +Depends: python3-scipy | python-scipy + +Depends: python3-numpy | python-numpy + +Depends: ipython3 | ipython + +Depends: ipython3-qtconsole | ipython-qtconsole + +Depends: ipython3-notebook | ipython3-qtconsole + +Depends: python3-sympy | python-sympy + +Depends: python3-networkx | python-networkx + +Depends: python3-pandas | python-pandas + +Depends: astropy-utils + +Depends: python3-astropy | python-astropy + +Depends: python3-astroml | python-astroml + +Depends: python3-astroml-addons | python-astroml-addons + +Depends: python3-astroquery | python-astroquery + +Depends: python3-aplpy | python-aplpy + +Depends: python3-atpy | python-atpy +Homepage: http://atpy.readthedocs.org/ +Pkg-Description: Astronomical Tables in Python + ATpy is a high-level Python package providing a way to manipulate tables of + astronomical data in a uniform way. It provides built-in support for NumPy + recarrays and common astronomical file/database formats (FITS, VO, HDF5, and + ASCII tables) with a very simple API. +Remark: + Much of ATpy’s functionality has now been incorporated into Astropy, and + there is no longer active development of new features in ATpy, instead + focusing efforts on Astropy. + +Depends: python3-ccdproc | python-ccdproc + +Depends: python3-gatspy | python-gatspy +Homepage: http://www.astroml.org/gatspy/ +Pkg-Description: General tools for Astronomical Time Series in Python + Gatspy contains efficient, well-documented implementations of several common + routines for Astronomical time series analysis, including the Lomb-Scargle + periodogram, the Supersmoother method, and others. + +Depends: python3-photutils | python-photutils + +Depends: python3-sep | python-sep +Homepage: http://sep.readthedocs.org/ +Pkg-Description: Astronomical source extraction and photometry in Python + SEP makes available some of the astronomical source extraction and photometry + algorithms in Source Extractor as stand-alone functions and classes. These + operate directly on in-memory numpy arrays (no FITS files, configuration + files, etc). It’s derived directly from (and tested against) the Source + Extractor code base. + +Depends: spyder3 | spyder + +Depends: rapidsvn, subversion + +Depends: git, git-gui + +Depends: mercurial + +Depends: dia + +Depends: gimp + +Depends: inkscape + +Depends: kst +Remark: + The Debian package includes the FITS reader that is a separate package on + Fedora. + +Depends: kst-doc + +Depends: labplot + +Depends: veusz + +Depends: icedtea-plugin + +Depends: imagemagick + +Depends: kate + +Depends: rlwrap + +Depends: screen diff -Nru debian-astro-0.3/tasks/frameworks debian-astro-0.4/tasks/frameworks --- debian-astro-0.3/tasks/frameworks 2016-04-14 15:36:45.000000000 +0000 +++ debian-astro-0.4/tasks/frameworks 2016-07-05 13:54:45.000000000 +0000 @@ -1,4 +1,5 @@ Task: Frameworks +Install: true Description: Astronomical data analysis frameworks This metapackage will install large astronomical data analysis frameworks, which usually provide their own script language. @@ -9,20 +10,13 @@ Depends: scilab +Depends: pdl + +Depends: dpuser + Depends: iraf WNPP: 690531 Remark: The development of the IRAF package is currently on hold because of the complicated source package structure and some major licensing issues. -Depends: pdl - -Depends: dpuser -WNPP: 472961 -Pkg-Description: Interactive language for (astronomical) data analysis - DPUSER is a command line program which provides an interactive language that - is capable of handling numbers (both real and complex), strings, and - matrices. Its main aim is to do astronomical image analysis, for which it - provides a comprehensive set of functions, but it can also be used for many - other applications. -Homepage: http://www.mpe.mpg.de/~ott/dpuser/ diff -Nru debian-astro-0.3/tasks/gdl debian-astro-0.4/tasks/gdl --- debian-astro-0.3/tasks/gdl 2016-01-19 10:42:02.000000000 +0000 +++ debian-astro-0.4/tasks/gdl 2016-05-24 09:23:48.000000000 +0000 @@ -1,4 +1,5 @@ Task: GDL +Install: true Description: IDL/GDL packages for astronomy GDL (GNU Data Language) is a free replacement for the commercial software IDL (Interactive Data Language). It has full syntax compatibility with IDL 7.1 diff -Nru debian-astro-0.3/tasks/java debian-astro-0.4/tasks/java --- debian-astro-0.3/tasks/java 2016-03-19 07:02:31.000000000 +0000 +++ debian-astro-0.4/tasks/java 2016-07-09 08:58:29.000000000 +0000 @@ -1,54 +1,17 @@ Task: Java +Install: true Description: Java packages for astronomy This metapackage will install packages that are useful to develop Java - applications for astronomy. + applications for astronomy. Apart vom FITS file handling, this is mainly used + for VO applications. Depends: libfits-java -Depends: libivoafits-java - -Depends: libjsamp-java -WNPP: 680475 -Pkg-Description: Java toolkit for the Simple Application Messaging Protocol - JSAMP provides a hub implementation for the Simple Application - Messaging Protocol (SAMP), suitable for standalone or embedded use. - . - Moreover, it offers a set of classes which can be used to implement - SAMP capabilities in client applications. JSAMP provides a hub test - and a benchmarking suite to examine the correctness and performance - of third-party hub implementations. The software includes hub and - client implementations of the standard and web profiles and a bridge - component, which allows clients on different hubs to talk to each - other. -Homepage: http://software.astrogrid.org/doc/p/jsamp/1.3-2/index.html +Depends: libhealpix-java -Depends: libsavot-java -WNPP: 818375 -Pkg-Description: Java-based VO-Table (Virtual Observatory) library - Simple Access to VOTable (SAVOT) is a Java library for VO-Tables which lives - under the 'cds.savot' namespace. - . - SAVOTv4 is a library written in Java, and maintined by the Strasbourg - astronomical Data Center (CDS). -Homepage: https://github.com/aschaaff/savot/ +Depends: libjsamp-java, libcds-savot-java, libcds-moc-java Depends: libcds-astro-java WNPP: 818376 -Pkg-Description: CDS Astronomical Units conversions - CDS Astro is a units conversion library that provides library - functionality under the 'cds.astro' namespace. It is one of the - dependencies of the Aladin Virtual Observatory (VO) client. - . - The library was written by the Strasbourg astronomical Data Center (CDS). -Homepage: http://cds.u-strasbg.fr/resources/doku.php?id=units -Depends: libcds-moc-java -WNPP: 818378 -Pkg-Description: Multi-Order Coverage Virtual Observatory library - The Multi-Order Coverage (MOC) library provides access to - functionality under the 'cds.moc' namespace. - . - The library is maintained by the Strasbourg astronomical Data Center - (CDS) and published by the International Virtual Observatory Alliance - (IVOA). -Homepage: http://wiki.ivoa.net/twiki/bin/view/IVOA/MocInfo +Depends: libivoafits-java diff -Nru debian-astro-0.3/tasks/publication debian-astro-0.4/tasks/publication --- debian-astro-0.3/tasks/publication 2016-03-10 16:13:59.000000000 +0000 +++ debian-astro-0.4/tasks/publication 2016-05-24 09:23:48.000000000 +0000 @@ -1,4 +1,5 @@ Task: Publication +Install: true Description: Packages for the publication and presentation of astronomical data This metapackage will install software for the preparation of astronomical data to publish them in journals or on the web. diff -Nru debian-astro-0.3/tasks/pulsar debian-astro-0.4/tasks/pulsar --- debian-astro-0.3/tasks/pulsar 1970-01-01 00:00:00.000000000 +0000 +++ debian-astro-0.4/tasks/pulsar 2016-07-22 10:11:21.000000000 +0000 @@ -0,0 +1,50 @@ +Task: Pulsar analysis +Install: false +Index: false +Leaf: false +Metapackage: false +Description: Pulsar analysis packages + These are taken from the "kernsuite" repository. + +Depends: dspsr +Homepage: http://dspsr.sourceforge.net/ +Vcs-Browser: https://github.com/kernsuite-debian/dspsr +Pkg-Description: Library for digital signal processing of pulsar astronomical timeseries + +Depends: tempo +Homepage: https://sourceforge.net/projects/tempo/ +Vcs-Browser: https://github.com/kernsuite-debian/tempo +Pkg-Description: Pulsar timing data analysis package + +Depends: multinest +Homepage: https://github.com/JohannesBuchner/MultiNest +Vcs-Browser: https://github.com/kernsuite-debian/multinest +Pkg-Description: Bayesian inference tool + MultiNest is a Bayesian inference tool which calculates the evidence and + explores the parameter space which may contain multiple posterior modes + and pronounced (curving) degeneracies in moderately high dimensions. + +Depends: psrchive +Homepage: http://psrchive.sourceforge.net/ +Vcs-Browser: https://github.com/kernsuite-debian/psrchive +Pkg-Description: C++ development library for the analysis of pulsar astronomical data + +Depends: sigproc +Homepage: https://github.com/SixByNine/sigproc +Vcs-Browser: https://github.com/kernsuite-debian/sigproc +Pkg-Description: Pulsar search and analysis software + +Depends: tempo2 +Homepage: https://bitbucket.org/psrsoft/tempo2/ +Vcs-Browser: https://github.com/kernsuite-debian/tempo2 +Pkg-Description: Pulsar timing package + +Depends: presto +Homepage: https://github.com/scottransom/presto/ +Vcs-Browser: https://github.com/kernsuite-debian/presto +Pkg-Description: Large suite of pulsar search and analysis software + +Depends: psrcat +Homepage: http://www.atnf.csiro.au/people/pulsar/psrcat/ +Vcs-Browser: https://github.com/kernsuite-debian/psrcat +Pkg-Description: The ATNF Pulsar Catalogue diff -Nru debian-astro-0.3/tasks/python debian-astro-0.4/tasks/python --- debian-astro-0.3/tasks/python 2016-04-14 15:36:45.000000000 +0000 +++ debian-astro-0.4/tasks/python 2016-07-25 07:52:08.000000000 +0000 @@ -3,6 +3,10 @@ Description: Python 2 packages for astronomy This metapackage will install Python 2 packages for astronomy. The packages can be used for interactive analysis, or to create specific programs. + . + Note that Python 2 is legacy only, Python 3 is the present and future of the + language. The support for Python 2 will end in 2020. Please use Python 2 only + if you don't have a choice. Depends: python, ipython @@ -25,7 +29,7 @@ python-spectral-cube, python-wcsaxes, python-specutils Depends: python-aplpy, python-astroml, python-galpy, - python-ginga, python-glue, python-imexam, python-omnifit, + python-glue, python-imexam, python-omnifit, python-pyregion, python-cpl, python-pyvo, python-spherical-geometry Why: Astropy affiliated packages @@ -36,6 +40,9 @@ Depends: python-reproject WNPP: 803741 +Depends: python-ginga +WNPP: 823598 + Depends: python-asdf Depends: python-pyavm @@ -56,8 +63,13 @@ Depends: python-emcee +Depends: python-fitsio + Depends: python-pysynphot +Depends: python-pyfftw +Why: From AstroConda + Depends: python-sherpa WNPP: 795370 Pkg-Description: Modeling and fitting in Python @@ -91,5 +103,12 @@ using an object-oriented interface. Homepage: https://sncosmo.github.io/ -Depends: python-fitsio -WNPP: 820811 +Depends: python-casacore +Pkg-Description: Python 2 bindings to the casacore library + The casacore package contains the core libraries of the old AIPS++/CASA + package. This split was made to get a better separation of core + libraries and applications. CASA is now built on top of casacore. + . + This is the Python 3 wrapper around the library. +Homepage: http://casacore.github.io/python-casacore/ +WNPP: 830118 diff -Nru debian-astro-0.3/tasks/python3 debian-astro-0.4/tasks/python3 --- debian-astro-0.3/tasks/python3 2016-04-14 15:36:45.000000000 +0000 +++ debian-astro-0.4/tasks/python3 2016-07-06 13:40:23.000000000 +0000 @@ -1,4 +1,5 @@ Task: Python3 +Install: true Description: Python 3 packages for astronomy This metapackage will install Python 3 packages for astronomy. The packages can be used for interactive analysis, or to create specific programs. @@ -24,7 +25,7 @@ python3-spectral-cube, python3-wcsaxes, python3-specutils Depends: python3-aplpy, python3-astroml, python3-galpy, - python3-ginga, python3-glue, python3-imexam, python3-omnifit, + python3-glue, python3-imexam, python3-omnifit, python3-pyregion, python3-cpl, python3-pyvo, python3-spherical-geometry Why: Astropy affiliated packages @@ -35,6 +36,9 @@ Depends: python3-reproject WNPP: 803741 +Depends: python3-ginga +WNPP: 823598 + Depends: python3-asdf Depends: python3-pyavm @@ -45,10 +49,17 @@ Depends: python3-gyoto +Depends: python3-sunpy + Depends: python3-ephem Depends: python3-emcee +Depends: python3-fitsio + +Depends: python3-pyfftw +Why: From AstroConda + Depends: python3-sherpa WNPP: 795370 Pkg-Description: Modeling and fitting in Python 3 @@ -82,5 +93,12 @@ using an object-oriented interface. Homepage: https://sncosmo.github.io/ -Depends: python3-fitsio -WNPP: 820811 +Depends: python3-casacore +Pkg-Description: Python 3 bindings to the casacore library + The casacore package contains the core libraries of the old AIPS++/CASA + package. This split was made to get a better separation of core + libraries and applications. CASA is now built on top of casacore. + . + This is the Python 3 wrapper around the library. +Homepage: http://casacore.github.io/python-casacore/ +WNPP: 830118 diff -Nru debian-astro-0.3/tasks/radioastronomy debian-astro-0.4/tasks/radioastronomy --- debian-astro-0.3/tasks/radioastronomy 1970-01-01 00:00:00.000000000 +0000 +++ debian-astro-0.4/tasks/radioastronomy 2016-07-22 10:09:57.000000000 +0000 @@ -0,0 +1,191 @@ +Task: Radio Astronomy +Install: true +Description: Radio Astronomy Software + This metapackage will install Debian Astro packages for radio astronomy. It + should contain most of the required tools that a radio astronomer require for + setting up a data reduction pipeline. + +Depends: casacore-dev + +Depends: python3-casacore +Suggests: python-casacore + +Depends: python3-spectral-cube +Suggests: python-spectral-cube + +Depends: aoflagger +Pkg-Description: RFI detector for astronomical radio observations + The AOFlagger is a flagger framework that implements several methods to deal + with radio-frequency interference or RFI. Some of the implemented algorithms + are the SumThreshold method, background fitting techniques (smoothing, + sliding window, median filters, high-pass filters) and morphological + operators. These are combined into one default strategy that performs very + well on almost any observation. +Homepage: https://sourceforge.net/p/aoflagger/wiki/Home/ +WNPP: 830120 + +Depends: wsclean +Pkg-Description: Fast widefield interferometric imager + WSClean (w-stacking clean) is a fast generic widefield imager. It uses the + w-stacking algorithm and can make use of the w-snapshot algorithm. As of + Feb 2014, it is 2-12 times faster than CASA's w-projection, depending on + the array configuration. It supports full-sky imaging and proper beam + correction for homogeneous dipole arrays such as the MWA. + . + WSClean allows Hogbom and Cotton-Schwab cleaning and has wideband, multiscale, + compressed sensing and joined-polarization deconvolution modes. All operations + are performed on the CPU. +Homepage: https://sourceforge.net/projects/wsclean/ +WNPP: 830124 + +Depends: casasynthesis +Pkg-Description: CASA modules needed for processing synthesis data + Aperture synthesis or synthesis imaging is a type of interferometry that + mixes signals from a collection of telescopes to produce images having the + same angular resolution as an instrument the size of the entire + collection. At each separation and orientation, the lobe-pattern of the + interferometer produces an output which is one component of the Fourier + transform of the spatial distribution of the brightness of the observed + object. The image (or "map") of the source is produced from these + measurements. Astronomical interferometers are commonly used for + high-resolution optical, infrared, submillimetre and radio astronomy + observations. + . + This is a fork of some of the synthesis submodule (combined with inter + project dependencies) of CASA 4.4. +Homepage: https://github.com/radio-astro/casasynthesis +WNPP: 830122 +Vcs-Browser: https://github.com/kernsuite-debian/casasynthesis + +Depends: casarest +Pkg-Description: Old AIPS++ code not included in casacore + This is the casarest package, the remainder of the AIPS++ libraries which are + not included in casacore. The program lwimager is the main deliverable. +Homepage: https://github.com/casacore/casarest/ +WNPP: 830123 +Vcs-Browser: https://github.com/kernsuite-debian/casarest + +Depends: oskar +Pkg-Description: Oxford's Square Kilometre Array Radio-telescope simulator + The OSKAR package consists of a number of open source libraries and + applications for the simulation of astronomical radio interferometers. + OSKAR has been designed primarily to produce simulated visibility data from + large aperture arrays, such as those envisaged for the SKA. +Homepage: http://www.oerc.ox.ac.uk/~ska/oskar2/ +WNPP: 830125 +Vcs-Browser: https://github.com/kernsuite-debian/oskar + +Depends: purify +Pkg-Description: Next-generation radio interferometric imaging + PURIFY is an open-source code that provides functionality to perform radio + interferometric imaging, i.e. to recover images from the incomplete Fourier + measurements taken by radio interferometric telescopes. PURIFY leverages + recent developments in the field of compressive sensing and convex + optimization. + . + PURIFY is written in C and contains the high-level functionality required for + adio interferometric imaging, such as modelling radio telescopes and posing + imaging as a convex optimisation problem. Low-level functionality to solve + the resulting convex optimisation is factored into the open-source companion + code, SOPT, also written by the authors of PURIFY. For further background + please see the following papers. +Homepage: http://basp-group.github.io/purify/ +WNPP: 830126 +Vcs-Browser: https://github.com/kernsuite-debian/purify + +Depends: sagecal +Pkg-Description: GPU/MIC accelerated radio interferometric calibration program + SAGECal is a very fast, memory efficient and GPU accelerated radio + interferometric calibration program. It can handle all source models + including points, Gaussians and Shapelets. It can calibrate along + hundreds of directions without running out of memory in almost real + time. Intel Xeon Phi acceleration is also available. Distributed + calibration using MPI and consensus optimization is enabled. Also + tools to build/restore sky models are included. +Homepage: https://sourceforge.net/projects/sagecal/ +WNPP: 830127 +Vcs-Browser: https://github.com/kernsuite-debian/sagecal + +Depends: lofar +Pkg-Description: LOFAR software suite + The LOFAR repository contains some of the software packages to operate + the LOFAR radio telescope and process its measurement output. + . + LOFAR is operated by ASTRON, the Netherlands Institute for Radio Astronomy. + For more information, see http://www.astron.nl/ and http://www.lofar.org/ +Homepage: http://www.lofar.org/ +Vcs-Browser: https://github.com/kernsuite-debian/lofar + +Depends: parseltongue +Homepage: http://www.jive.nl/jivewiki/doku.php?id=parseltongue:parseltongue +Vcs-Browser: https://github.com/kernsuite-debian/parseltongue +Pkg-Description: Python scripting interface for classic AIPS + ParselTongue is a Python interface to classic AIPS, Obit and possibly + other task-based data reduction packages. It serves as the software + infrastructure for some of the ALBUS implementation. It allows you to + run AIPS tasks, and access AIPS headers and extension tables from + Python. There is also support for running Obit tasks and accessing + data in FITS files. Full access to the visibilities in AIPS UV data + is also available. ParselTongue allows you to script AIPS with a + modern programming language, making complex automated data reduction + possible. The excellent support for today's web standards in Python + facilitates the development of pipelines that interact easily with + the outside world. + +Depends: python-tigger +Homepage: https://github.com/ska-sa/tigger +Vcs-Browser: https://github.com/kernsuite-debian/tigger +Pkg-Description: FITS and MeqTrees LSM viewer + +Depends: rpfits +Homepage: http://www.atnf.csiro.au/computing/software/rpfits.html +Vcs-Browser: https://github.com/kernsuite-debian/rpfits +Pkg-Description: RPFITS data-recording format support library + RPFITS is used since the mid-1980s within the Australia Telescope National + Facility (ATNF). + +Depends: python-pyxis +Homepage: https://github.com/ska-sa/pyxis +Vcs-Browser: https://github.com/kernsuite-debian/pyxis +Pkg-Description: Python Extensions for Interferometry Scripting + +Depends: python-pymoresane +Homepage: https://github.com/ratt-ru/PyMORESANE +Vcs-Browser: https://github.com/kernsuite-debian/pymoresane +Pkg-Description: Python version of the MORESANE deconvolution algorithm + This is a Python and pyCUDA-accelerated implementation of the MORESANE + deconvolution algorithm. + +Depends: python-owlcat +Homepage: https://github.com/ska-sa/owlcat +Vcs-Browser: https://github.com/kernsuite-debian/owlcat +Pkg-Description: Scripts for manipulating radio interferometry data + Miscellaneous utility scripts for manipulating radio interferometry data + +Depends: mt-imager +Homepage: http://www.mtimager.com/ +Vcs-Browser: https://github.com/kernsuite-debian/mt-imager +Pkg-Description: High performance image synthesiser for radio interferometry + The Malta-imager (mt-imager for short) is a high performance image synthesiser + for radio interferometry. It is implemented in C++ and CUDA. With the help of + international collaborators, there will soon be further development as part of + Daniel's doctorate studies. + +Depends: python-meqtrees-timba, meqtrees-timba +Homepage: http://www.astron.nl/meqwiki/MeqTrees +Vcs-Browser: https://github.com/kernsuite-debian/meqtrees-timba +Pkg-Description: implementing and solving arbitrary Measurement Equations + +Depends: python-meqtrees-cattery +Homepage: https://github.com/ska-sa/meqtrees-cattery +Vcs-Browser: https://github.com/kernsuite-debian/meqtrees-cattery +Pkg-Description: MeqTrees-based frameworks for simulation and calibration of radio interferometers + +Depends: cassbeam +Homepage: https://github.com/ratt-ru/cassbeam +Vcs-Browser: https://github.com/kernsuite-debian/cassbeam +Pkg-Description: Cassegrain antenna ray tracer + Based on an input text file, it computes several properties of the antenna + including gain, zenith system temperature, and the beam, in full polarization. + All calculations are done in the {\it transmit sense} and use reciprocity to + relate to the equivalent receiving system. diff -Nru debian-astro-0.3/tasks/scisoft debian-astro-0.4/tasks/scisoft --- debian-astro-0.3/tasks/scisoft 1970-01-01 00:00:00.000000000 +0000 +++ debian-astro-0.4/tasks/scisoft 2016-07-06 20:19:25.000000000 +0000 @@ -0,0 +1,894 @@ +Task: Scisoft +Install: false +Index: false +Leaf: false +Metapackage: false +Description: Scisoft packages + Here we list the status of the packages that belong to the + [SciSoft](http://www.eso.org/sci/software/scisoft) + distribution. Scisoft is a project within [ESO](http://www.eso.org) to + provide a collection of astronomical software utilities in a uniform way at + all ESO sites and to make them available to the outside world. The current + version, Scisoft 8, December 2014, is only available for 64-bit Fedora 20 + Linux. + +Depends: iraf +WNPP: 690531 +Homepage: http://iraf.noao.edu/ +Pkg-Description: Image Reduction and Analysis Facility + IRAF includes a broad selection of programs for general image processing + and graphics, plus a large number of programs for the reduction and + analysis of optical and IR astronomy data. Other external or layered + packages are available for applications such as data acquisition or + handling data from other observatories and wavelength regimes such as + the Hubble Space Telescope (optical), EUVE (extreme ultra-violet), or + ROSAT and AXAF (X-ray). These external packages are distributed + separately from the main IRAF distribution but can be easily installed. + The IRAF system also includes a complete programming environment for + scientific applications, which includes a programmable Command Language + scripting facility, the IMFORT Fortran/C programming interface, and the + full SPP/VOS programming environment in which the portable IRAF system + and all applications are written. +Remark: + IRAF is hard to package for Debian (in fact for any distribution) because +of its old architecture. It also contains various routines from Numerical +Recipes which are illegal to distribute. + +Depends: iraf-ctio +Homepage: http://www.stecf.org/scripts/irafhelp?ctio +Pkg-Description: Utilities from CTIO + CTIO is an IRAF external package with some CTIO-specific tools as well + as some general purpose ones not included in the main IRAF + distribution. +Remark: + Depends on IRAF + +Depends: iraf-mxtools +Homepage: http://www.noao.edu/noao/staff/mighell/mxtools/ +Pkg-Description: Utilities from NOAO including QDPHOT + MXTOOLS is an IRAF package providing tools for image matching and + image coordinate manipulation. +Remark: + Depends on IRAF + +Depends: iraf-guiapps +Homepage: http://www.stecf.org/iraf/web/projects/guiapps/ +Pkg-Description: Graphical applications for IRAF + GUIAPPS is an IRAF external package providing some prototype GUI + applications for data reduction and analysis. +Remark: + Depends on IRAF + +Depends: iraf-xdimsum +Pkg-Description: Enhanced IR data reduction and mosaicing software + XDIMSUM is a package for creating accurate sky subtracted images from sets of + dithered observations. While the observations need not be in the infrared, the + dominance of the variable sky background in infrared data requires dithering of + many short exposures and recombination with careful sky subtraction to produce + deep images. Hence the package is called "Experimental Deep Infrared Mosaicing + Software" or XDIMSUM. + . + XDIMSUM is a variant of the DIMSUM package developed by P. Eisenhardt, M. + Dickensen, S.A. Stanford, and J. Ward. F. Valdes (IRAF group) modified DIMSUM + to support FITS format images, added the DIMSUM tutorial demos script, wrote + the original version of this document, and repackaged DIMSUM for distribution + as an IRAF external package. L. Davis (IRAF group) rewrote the the major + DIMSUM scripts to improve their clarity, robustness, and efficiency, added + new scripts for computing relative offsets, and documented the tasks. The new + package uses the same default algorithms as DIMSUM but is sufficiently + different in format that it has been renamed XDIMSUM. +Remark: + Depends on IRAF + +Depends: iraf-color +Homepage: http://www.stecf.org/scripts/irafhelp?color +Pkg-Description: Utilities for creating colour images + A prototype IRAF color image display package, COLOR, is now available. + Currently this package provides conversion of 3 bandpass IRAF images to a + Sun 24-bit RGB rasterfile format, a 24-bit to 8-bit compression algorithm + and Floyd-Steinberg dithering, and an RGB 8-bit pixel dithering algorithm. + The Sun rasterfiles are displayed using non-IRAF tools and the others use + only IRAF images and SAOimage or IMTOOL. These tasks are usable with the + currently common 8-bit color workstations and are provided for those users + which don't have more capable hardware such as 24-bit workstations, IIS + displays, and 24-bit addon cards. +Remark: + Depends on IRAF + +Depends: iraf-fitsutil +Homepage: http://www.stecf.org/scripts/irafhelp?fitsutil +Pkg-Description: FITS utilities + FITSUTIL is an IRAF external package providing some extra utilities + for manipulating FITS files, including multiextention FITS files. +Remark: + Depends on IRAF + +Depends: iraf-mscred +Homepage: http://www.stecf.org/scripts/irafref?mscred +Pkg-Description: Mosaic camera CCD reduction tasks from NOAO + MSCRED is the IRAF CCD Mosaic Reduction package and can be used to + reduce CCD mosaic data that is in the mosaic MEF data format. +Remark: + Depends on IRAF + +Depends: iraf-esowfi +Pkg-Description: ESO WFI Mosaic reduction package + The ESOWFI external package is used to reduce ESO WFI CCD mosaic data. + It provides a single task for converting the ESO headers to work with + the MSCRED package. It also sets the default instrument files and an + astrometry solution. The reductions are then done using the MSCRED + Mosaic reduction package. +Remark: + Depends on IRAF + +Depends: iraf-rvsao +Homepage: http://tdc-www.harvard.edu/iraf/rvsao/rvsao.html +Pkg-Description: Spectral Radial Velocity package from CfAi + RVSAO is a set of programs to obtain redshifts and radial velocities + from digital spectra. RVSAO operates in the IRAF (Tody 1986, 1993) + environment. The heart of the system is xcsao, which implements the + cross-correlation method, and is a direct descendant of the system built + by Tonry and Davis (1979). emsao uses intelligent heuristics to search + for emission lines in spectra, then fits them to obtain a redshift. + sumspec shifts and sums spectra to build templates for cross- + correlation. linespec builds synthetic spectra given a list of spectral + lines. bcvcorr corrects velocities for the motion of the earth. We + discuss in detail the parameters necessary to run xcsao and emsao + properly. We discuss the reliability and error associated with xcsao + derived redshifts. We develop an internal error estimator, and we show + how large, stable surveys can be used to develop more accurate error + estimators. We develop a new methodology for building spectral templates + for galaxy redshifts. We show how to obtain correlation velocities using + emission line templates. Emission line correlations are substantially + more efficient than the previous standard technique, automated emission + line fitting. We compare the use of RVSAO with new methods, which use + Singular Value Decomposition and $chi^2$ fitting techniques. +Remark: + Depends on IRAF + +Depends: iraf-stecf +Homepage: http://www.stecf.org/software/stecf-iraf/ +Pkg-Description: Utilities from ST-ECF + Utilities from ST-ECF, including polarimetry reduction and spectral + restoration packages. +Remark: + Depends on IRAF + +Depends: iraf-stsdas-tables +Homepage: http://www.stsci.edu/resources/software_hardware/stsdas +Pkg-Description: HST data analysis and tables systems + TABLES provides support for tabular data for STSDAS and other packages. Many + types of data are stored in tabular format, such as catalogs of astronomical + objects, spectral data (e.g. columns of wavelength and flux), and + coefficients of fit to data. TABLES provides a programming interface for + accessing tables, and it includes a collection of utility programs for + working with tables. FITS tables, STSDAS format, and simple text tables are + supported. The programming interface is used for the utility programs in + TABLES, by tasks in STSDAS, and by other external packages. The utility + programs are used for such tasks as plotting, selecting rows based on an + expression involving column values, sorting rows in a table, joining tables, + and performing arithmetic operations on column values. +Remark: + Depends on IRAF + +Depends: iraf-ecl +Homepage: http://iraf.noao.edu/iraf/web/new_stuff/ecl_beta.html +Pkg-Description: Enhanced CL + The primary goals of the ECL project were to + . + * add an error-handling capability to the existing IRAF CL, + * include other functionality which could improve the + * scripting environment (e.g. pre-defined language constants + such as 'PI') and add any other features we found lacking + (e.g. missing trig functions and string utilities), and + * add commonly requested features. +Remark: + Depends on IRAF + +Depends: eso-eclipse +Homepage: http://www.eso.org/sci/software/eclipse/ +Pkg-Description: C Library for an Image Processing Software Environment + Written in ANSI C, eclipse is a library offering numerous services + related to astronomical image processing: FITS data access, various + image and cube loading methods, binary image handling and filtering + (including convolution and morphological filters), 2-D cross- + correlation, connected components, cube and image arithmetic, dead pixel + detection and correction, object detection, data extraction, flat- + fielding with robust fit, image generation, statistics, photometry, + image-space resampling, image combination, and cube stacking. It also + contains support for mathematical tools like random number generation, + FFT, curve fitting, matrices, fast median computation, and point-pattern + matching. The main feature of this library is its ability to handle + large amounts of input data (up to 2GB in the current version) + regardless of the amount of memory and swap available on the local + machine. Another feature is the very high speed allowed by optimized C, + making it an ideal base tool for programming efficient number-crunching + applications, e.g., on parallel (Beowulf) systems. + +Depends: eso-midas + +Depends: pymidas +Homepage: http://www.eso.org/sampo/pymidas +Pkg-Description: Python interface for ESO-MIDAS + PyMidas is an interface between Python and MIDAS, the major ESO legacy + general purpose data processing system. PyMidas allows a user to exploit + both the rich legacy of MIDAS software and the power of Python scripting + in a unified interactive environment. PyMidas also allows the usage of + other Python-based astronomical analysis systems such asPyRAF. +Remark: + PyMidas is outdated and no longer maintained. Does not support Python 2.7 or 3.x. + +Depends: gnudatalanguage + +Depends: gdl-astrolib + +Depends: idl-starfinder +Homepage: http://www.bo.astro.it/StarFinder/ +Pkg-Description: IDL adaptive optics photometry software. + StarFinder is an IDL code for the deep analysis of stellar fields, + designed for Adaptive Optics well-sampled images with high and low + Strehl ratio. The Point Spread Function is extracted directly from the + frame, to take into account the actual structure of the instrumental + response and the atmospheric effects. The code is written in IDL + language and organized in the form of a self-contained widget-based + application, provided with a series of tools for data visualization and + analysis. A description of the method and some applications to Adaptive + Optics data are presented. + +Depends: idl-jhuapl +Homepage: http://fermi.jhuapl.edu/s1r/idl/s1rlib/local_idl.html +Pkg-Description: IDL procedure collection from Johns Hopkins + The JHU/APL/S1R IDL library contains over 600 IDL routines providing a wide + range of functionality. These routines have been developed over the years in + support of our group's work. We make them available as an aid to the wider + IDL community. + +Depends: idl-atv +Homepage: http://www.astro.caltech.edu/~barth/atv/ +Pkg-Description: interactive display tool for IDL + ATV displays and analyses astronomical images using the IDL image- + processing language. It allows interactive control of the image scaling, + color table, color stretch, and zoom, with support for world coordinate + systems. It also does point-and-click aperture photometry, simple + spectral extractions, and can produce publication-quality postscript + output images. + +Depends: gildas +Homepage: http://iram.fr/IRAMFR/GILDAS/ +Pkg-Description: Radio astronomy applications from IRAM + GILDAS is a collection of software oriented toward (sub-)millimeter + radioastronomical applications (either single-dish or interferometer). + It has been adopted as the IRAM standard data reduction package and is + jointly maintained by IRAM & CNRS. GILDAS contains many facilities, most + of which are oriented towards spectral line mapping and many kinds of + 3-dimensional data. The code, written in Fortran-90 with a few parts in + C/C++ (mainly keyboard interaction, plotting, widgets), is easily + extensible. +Remark: + The license makes GILDAS not suitable for Debian yet (according to DFSG): + . + GILDAS is freely available to non-profit institutes on an "as-is" basis. No + warranty at all is expressed or implied. We are thinking about going to + LGPL. (2004) + +Depends: miriad +Homepage: http://bima.astro.umd.edu/miriad/ +Pkg-Description: Calibration, mapping, deconvolution and image analysis of interferometric data + MIRIAD is a radio interferometry data-reduction package, designed for + taking raw visibility data through calibration to the image analysis + stage. It has been designed to handle any interferometric array, with + working examples for BIMA, CARMA, SMA, WSRT, and ATCA. A separate + version for ATCA is available, which differs in a few minor ways from + the CARMA version. + +Depends: karma +Homepage: http://www.atnf.csiro.au/computing/software/karma/ +Pkg-Description: Toolkit for IPC, authentication, graphics display etc. + Karma is a toolkit for interprocess communications, authentication, + encryption, graphics display, user interface and manipulating the Karma + network data structure. It contains KarmaLib (the structured libraries + and API) and a large number of modules (applications) to perform many + standard tasks. A suite of visualisation tools are distributed with the + library. +Remark: + Not maintained any longer. + +Depends: crush +WNPP: 815709 +Homepage: http://www.submm.caltech.edu/~sharc/crush/ +Pkg-Description: Data Reduction and Imaging for Bolometer Array + CRUSH is an astronomical data reduction/imaging tool for certain imaging + cameras, especially at the millimeter, sub-millimeter, and far-infrared + wavelengths. It supports the SHARC-2, LABOCA, SABOCA, ASZCA, p-ArTeMiS, + PolKa, GISMO, MAKO and SCUBA-2 instruments. The code is written entirely + in Java, allowing it to run on virtually any platform. It is normally + run from the command-line with several arguments. + +Depends: casa +Homepage: http://casa.nrao.edu/ +Pkg-Description: Common Astronomy Software Application + CASA, the Common Astronomy Software Applications package, is being + developed with the primary goal of supporting the data post-processing + needs of the next generation of radio astronomical telescopes such as + ALMA and EVLA. The package can process both interferometric and single + dish data. The CASA infrastructure consists of a set of C++ tools + bundled together under an iPython interface as a set of data reduction + tasks. This structure provides flexibility to process the data via task + interface or as a python script. In addition to the data reduction + tasks, many post-processing tools are available for even more + flexibility and special purpose reduction needs. + +Depends: theli +WNPP: 780303 +Homepage: http://www.astro.uni-bonn.de/theli/ +Pkg-Description: A pipeline for astronomical image data reduction + THELI is an easy-to-use, end-to-end pipeline for the reduction of any + optical, near-IR and mid-IR imaging data. It combines a variety of + processing algorithms and third party software into a single, + homogeneous tool. Over 90 optical and infrared instruments at + observatories world-wide are pre-configured; more can be added by the + user. The code's online appendix contains three walk-through examples + using public data (optical, near-IR and mid-IR) and additional online + documentation is available for training and troubleshooting. + +Depends: difmap +Homepage: http://www.cv.nrao.edu/adass/adassVI/shepherdm.html +Pkg-Description: Interactive program for radio synthesis imaging from Caltech + Difmap is a program developed for synthesis imaging of visibility data + from interferometer arrays of radio telescopes world-wide. Its prime + advantages over traditional packages are its emphasis on interactive + processing, speed, and the use of Difference mapping techniques. + +Depends: x11iraf +Homepage: http://www.openastro.com/osx/x11iraf-info.html +Pkg-Description: Graphical tools to work with IRAF + XGterm provides a Tek 4012 compatible graphics terminal emulation plus, for + clients in the know, a datastream driven widget server capability using the + Object Manager to provide full access to the underlying toolkit and widget + set. The remote client application downloads a GUI file to the widget server + (xgterm) which executes the GUI. While the GUI is executing it exchanges + messages with the remote client application at runtime via interprocess + communication. In the case of Xgterm, this currently uses a serial (tty + based) protocol. + . + XImtool is an image display server. This provides an image display capability + to remote client applications using the standard imtool/iis image display + protocol. The image display server allows a number of image frame buffers to + be created and displayed. The client can read and write data in these frame + buffers. Any frame or combination of frames can be displayed. Various display + options are provided, e.g., zoom and pan, flip about either axis, frame + blink, windowing of the display, and colortable enhancement. + . + XTapemon is a conventional Xt/Athena application which allows the status of + an IRAF tape job to be monitored continuously while the tape is being + accessed. +Remark: + Depends on IRAF + +Depends: saoimage +Homepage: http://tdc-www.harvard.edu/software/saoimage.html +Pkg-Description: The original, needs 8bit Xserver + SAOimage (pronounced S-A-0-image) is a utility for displaying astronomical + images in the X11 window environment. It was written at the Smithsonian + Astrophysical Observatory by Mike Van Hilst in 1990 and hass been maintained + by Doug Mink. Image files can be read directly, or image data may be passed + through a named pipe (Unix) or a mailbox (VMS) from IRAF display + tasks. SAOimage provides a large selection of options for zooming, panning, + scaling, coloring, pixel readback, display blinking, and region + specification. User interactions are generally performed with the + mouse. Mouse tracking in an image's world coordinate system, usually sky + coordinates, was added in 1994. You can also plot catalogs over images with + WCS information in their headers. + . + The SAOimage desktop includes, a main image display window, a button menu + panel, a display magnifier, a pan and zoom reference image, and a color + bar. A color table graph window can be brought up by clicking on the color + bar. +Remark: + Outdated; use saods9 + +Depends: saods9 + +Depends: xpa-tools + +Depends: skycat + +Depends: ftools-fv + +Depends: starlink-gaia +Homepage: http://star-www.dur.ac.uk/~pdraper/gaia/gaia.html +Pkg-Description: Graphical Astronomy and Image Analysis Tool + GAIA is an image and data-cube display and analysis tool for astronomy. + It provides the usual facilities of image display tools, plus more + astronomically useful ones such as aperture and optimal photometry, + contouring, source detection, surface photometry, arbitrary region + analysis, celestial coordinate readout, calibration and modification, + grid overlays, blink comparison, defect patching and the ability to + query on-line catalogues and image servers. It can also display slices + from data-cubes, extract and visualize spectra as well as perform full + 3D rendering. GAIA uses the Starlink software environment (ascl:1110.012) + and is derived from the ESO SkyCat tool(ascl:1109.019). + +Depends: supermongo +Homepage: http://www.astro.princeton.edu/~rhl/sm/ +Pkg-Description: SuperMongo. + SM is an interactive plotting package for drawing graphs written by Robert + Lupton and Patricia Monger. It has some capability to handle image data, but + mostly works with vectors. The main features of the package are: + . + * one can generate a plot with a minimum number of simple commands, + * one can view the plot on the screen and then with a simple set of + commands send the same plot to a hardcopy device, + * one can build and save plot subroutines to be invoked with a single + user-defined command, + * the program keeps a history of plot commands which can be edited and + defined as a plot subroutine, to be reused, + * one can define the data to be plotted from within the program, or read + them from an ASCII file. +Remark: + Not free. + +Depends: pgplot5 +Remark: + Giza-dev is a DFSG-free replacement for pgplot5. + +Depends: gnuplot + +Depends: grace + +Depends: ggobi + +Depends: python3-matplotlib | python-matplotlib + +Depends: libplplot-dev + +Suggests: python-numeric +Homepage: http://sourceforge.net/projects/numpy/files/Old%20Numeric/ +Pkg-Description: Python module for high-performance, numeric computing + Numeric is a Python module for high-performance, numeric computing. It + provides much of the functionality and performance of commercial numeric + software such as Matlab; in some cases, it provides more functionality than + commercial software. +Remark: + Not maintained anymore, outdated by python3-numpy + +Suggests: python-scientific +Remark: + Not maintained anymore, outdated by python3-scipy + +Depends: python3-pil | python-pil + +Suggests: python-pmw + +Suggests: python-asciidata +Homepage: http://www.stecf.org/software/PYTHONtools/astroasciidata/ +Pkg-Description: Python module to handle ASCII tables + AstroAsciiData is a Python module to handle ASCII tables. Features: + . + * Imports all reasonably well-formed Ascii tables + * Column-first access + * Easy creation and manipulation of tables, columns, rows and attached + comments + * Retains formatting of data values + * Support for SExtractor style headers + * Column sorting + * Interchangeable comment character, column delimiter and null value + * Exports data to Ascii, Numpy/Numarray, FITS table, HTML table, LaTeX table +Remark: + Package is obsoleted by python3-astropy. Please use python3-astropy instead. + +Depends: python3-scipy | python-scipy + +Suggests: python-gnuplot + +Depends: python-ppgplot +Homepage: https://github.com/npat-efault/ppgplot +Pkg-Description: Pythonic Interface to PGPLOT + ppgplot is a python module (extension) providing bindings to the + PGPLOT graphics library. PGPLOT is a scientific visualization + (graphics) library written in Fortran by T. J. Pearson. C bindings + for PGPLOT are also available. ppgplot makes the library usable by + Python programs. It uses the numeric / numarray modules (nowadays + replaced by Numpy), to efficiently represent and manipulate vectors + and matrices. +Remark: + Must go to contrib since it depends on pgplot (non-free) + +Suggests: python-pybiggles + +Suggests: python-pygame + +Suggests: python-wxgtk3.0 + +Depends: stsci-python +Homepage: http://www.stsci.edu/resources/software_hardware/pyraf/stsci_python +Pkg-Description: STScI Python packages + stsci_python is a library of Python routines and C extensions that has been + developed to provide a general astronomical data analysis infrastructure. It + includes the following: + . + * PyRAF, an environment for running IRAF tasks without using the IRAF CL + * DrizzlePac, a task for combining dithered STScI images + * PyFITS, used to read FITS images and tables into numpy or numarray objects + and to manipulate FITS headers + * pysynphot is a synthetic photometry package (still in development) + designed to replace STSDAS.SYNPHOT. It is suitable for library or + interactive use. + * Numdisplay, used to visualize numpy array objects using image display + tools like ds9 and ximtool + +Depends: python-pyraf +Homepage: http://www.stsci.edu/resources/software_hardware/pyraf +Pkg-Description: Python replacement for IRAF cl from STScI + PyRAF is a command language for running IRAF tasks that is based on the + Python scripting language. It gives users the ability to run IRAF tasks + in an environment that has all the power and flexibility of Python. + PyRAF can be installed along with an existing IRAF installation; users + can then choose to run either PyRAF or the IRAF CL. +Remark: + Depends on IRAF + +Suggests: python3-pyfits | python-pyfits +Remark: + This package is obsoleted by python3-astropy. Please use + python3-astropy instead. + +Depends: python-pydrizzle +Homepage: http://www.stsci.edu/resources/software_hardware/pydrizzle +Pkg-Description: Drizzling software + PyDrizzle provides a semi-automated interface for computing the + parameters necessary for runningDrizzle. PyDrizzle performs the task of + determining the parameters necessary for aligning images based on the + WCS information in the input image headers, as well as any supplemental + alignment information provided in shift files, and combines the images + onto the same WCS. Though it does not identify cosmic rays, it has the + ability to ignore pixels flagged as bad, such as pixels identified by + other programs as affected by cosmic rays. + +Depends: python-multidrizzle +Homepage: http://stsdas.stsci.edu/multidrizzle/ +Pkg-Description: Automatic image combination drizzling software + MultiDrizzle automates and simplifies the detection of cosmic-rays and the + combination of dithered observations using the Python scripting language and + PyRAF, the Python-based interface to IRAF. MultiDrizzle was developed by the + Science Software Branch at the Space Telescope Science Institute. + +Depends: python3-numpy | python-numpy + +Depends: dpuser, qfitsview + +Depends: libgsl-dev + +Depends: dislin +Homepage: http://www.mps.mpg.de/1389229/dislin +Pkg-Description: Scientific Data Plotting software. + DISLIN is a high-level plotting library for displaying data as curves, polar + plots, bar graphs, pie charts, 3D-color plots, surfaces, contours and maps. + . + DISLIN is intended to be a powerful and easy to use software package for + scientists and programmers. There are only a few graphics routines with a + short parameter list needed to display the desired graphical output. A large + variety of parameter setting routines can then be called to create + individually customized graphics. +Remark: + Not DFSG-free + +Depends: libcfitsio-dev + +Depends: liblapack-dev + +Depends: libatlas-dev + +Depends: libfftw3-dev + +Depends: plotutils + +Suggests: python-jpype + +Depends: funtools + +Depends: wcstools + +Depends: astromatic + +Depends: sextractor + +Depends: swarp + +Depends: scamp + +Depends: astromatic-eye +Homepage: http://www.astromatic.net/software/eye +Pkg-Description: Enhance Your Extraction + In EyE (Enhance Your Extraction) an artificial neural network connected + to pixels of a moving window (retina) is trained to associate these + input stimuli to the corresponding response in one or several output + image(s). The resulting filter can be loaded inSExtractorto operate + complex, wildly non-linear filters on astronomical images. Typical + applications of EyE include adaptive filtering, feature detection and + cosmetic corrections. + +Depends: missfits + +Depends: stiff + +Depends: astromatic-stuff +Homepage: http://www.astromatic.net/software/stuff +Pkg-Description: Simulate 'perfect' astronomical catalogues + Stuff is a program that simulates 'perfect' astronomical catalogues. It + generate object lists in ASCII which can read by the SkyMaker program to + produce realistic astronomical fields. Stuff is part of + theEFIGIdevelopment project. + +Depends: weightwatcher + +Depends: tiny-tim +Homepage: http://www.stsci.edu/software/tinytim/tinytim.html +Pkg-Description: HST point-spread function simulation software + Tiny Tim generates simulated Hubble Space Telescope point spread + functions (PSFs). It is written in C and distributed as source code and + runs on a wide variety of UNIX and VMS systems. Tiny Tim includes mirror + zonal errors, time dependent aberrations (for the pre-repair + instruments), field dependent obscuration patterns (for WF/PC-1 and + WFPC2), and filter passband effects. It can produce a normally sampled + or subsampled PSF. Output is a FITS image file. +Remark: + Unknown, unspecified license + +Depends: xephem +Homepage: http://www.clearskyinstitute.com/xephem/ +Pkg-Description: Planetarium and ephemeris software + XEphem is a scientific-grade interactive astronomical ephemeris package + for UNIX-like systems. Written in C, X11 and Motif, it is easily ported + to systems. Among other things, XEphem:computes heliocentric, geocentric + and topocentric information for all objects;has built-in support for all + planets; the moons of Mars, Jupiter, Saturn, Uranus and Earth; central + meridian longitude of Mars and Jupiter; Saturn's rings; and Jupiter's + Great Red Spot;allows user-defined objects including stars, deepsky + objects, asteroids, comets and Earth satellites;provides special + efficient handling of large catalogs including Tycho, Hipparcos, + GSC;displays data in configurable tabular formats in conjunction with + several interactive graphical views;displays a night-at-a-glance 24 hour + graphic showing when any selected objects are up;displays 3-D stereo + Solar System views that are particularly well suited for visualizing + comet trajectories;quickly finds all close pairs of objects in the sky; + andsorts and prints all catalogs with very flexible criteria for + creating custom observing lists.Its capabilities are listed more fully + in theuser manual introduction. +Remark: + Not DFSG-Free. + +Depends: dss-dss2 +Homepage: http://archive.eso.org/cms/tools-documentation/the-eso-st-ecf-digitized-sky-survey-application.html +Pkg-Description: Digitized Sky Survey image extraction software + The ESO/ST-ECF Digitized Sky Survey [DSS] application is a remote client + program that extracts random sky section from the DSS image server installed + at ESO. The extracted images are delivered in standard FITS format and + contain all header keywords needed to visualize proper celestial coordinates + for any pixel position. A client to be installed on your local machine can be + downloaded here. +Remark: + Probably not DFSG-Free + +Depends: daophot +Homepage: http://www.star.bris.ac.uk/~mbt/daophot/ +Pkg-Description: Stellar Photometry and related packages from Peter Stetson at DAO/HIA + The DAOPHOT program exploits the capability of photometrically linear + image detectors to perform stellar photometry in crowded fields. Raw CCD + images are prepared prior to analysis, and following the obtaining of an + initial star list with the FIND program, synthetic aperture photometry + is performed on the detected objects with the PHOT routine. A local sky + brightness and a magnitude are computed for each star in each of the + specified stellar apertures, and for crowded fields, the empirical + point-spread function must then be obtained for each data frame. The + GROUP routine divides the star list for a given frame into optimum + subgroups, and then the NSTAR routine is used to obtain photometry for + all the stars in the frame by means of least- squares profile fits. +Remark: + Not DFSG-Free. + +Depends: fitsverify + +Depends: fitscut + +Depends: libcfitsio-bin + +Depends: cloudy +WNPP: 725891 +Homepage: http://www.nublado.org/ +Pkg-Description: Plasma simulation and spectral synthesis code + Cloudy is a large-scale spectral synthesis code designed to simulate + fully physical conditions within an astronomical plasma and then predict + the emitted spectrum. The code is freely available and is widely used in + the analysis and interpretation of emission-line spectra. + +Depends: hyperz +Homepage: http://webast.ast.obs-mip.fr/hyperz/ +Pkg-Description: Photometric Redshift Code + From a photometric catalogue, hyperz finds the redshift of each object + by means of a standard SED fitting procedure, i.e. comparing the + observed magnitudes with the expected ones, computed from template + Spectral Energy Distributions. The set of templates used in the + minimization procedure (age, metallicity, reddening, absorption in the + Lyman forest, ...) is studied in detail, through both real and simulated + data. The expected accuracy of photometric redshifts, as well as the + fraction of catastrophic identifications and wrong detections, is given + as a function of the redshift range, the set of filters considered, and + the photometric accuracy. Special attention is paid to the results + expected from real data. +Remark: + Last update: 2000-12-11 + +Depends: graphviz + +Depends: aladin +WNPP: 818373 +Homepage: http://aladin.u-strasbg.fr/ +Pkg-Description: Aladin Sky Atlas + Aladin is an interactive software sky atlas allowing the user to + visualize digitized astronomical images, superimpose entries from + astronomical catalogues or databases, and interactively access related + data and information from the Simbad database, the VizieR service and + other archives for all known sources in the field.Created in 1999, + Aladin has become a widely-used VO tool capable of addressing challenges + such as locating data of interest, accessing and exploring distributed + datasets, visualizing multi-wavelength data. Compliance with existing or + emerging VO standards, interconnection with other visualisation or + analysis tools, ability to easily compare heterogeneous data are key + topics allowing Aladin to be a powerful data exploration and integration + tool as well as a science enabler. + +Depends: vospec +Homepage: http://esavo.esa.int/vospec/ +Pkg-Description: tool for handling Virtual Observatory compliant Spectra + VOSpec is a multi-wavelength spectral analysis tool with access to + spectra, theoretical models and atomic and molecular line databases + registered in the VO. The standard tools of VOSpec include line and + continuum fitting, redshift and reddening correction, spectral + arithmetic and convolution between spectra, equivalent width and flux + calculations, and a best fitting algorithm for fitting selected SEDs to + a TSAP service. VOSpec offers several display modes (tree vs table) and + organising functionalities according to the available metadata for each + service, including distance from the observation position. + +Depends: voplot +Homepage: http://vo.iucaa.ernet.in/~voi/voplot.htm +Pkg-Description: VOTable plotting tool + VOPlot is a tool for visualizing astronomical data. It was developed in + Java and acts on data available in VOTABLE, ASCII and FITS formats. + VOPlot is available as a stand alone version, which is to be installed + on the user's machine, or as a web-based version fully integrated with + the VizieR database. + +Depends: plastic +Homepage: http://plastic.sourceforge.net/ +Pkg-Description: PLatform for AStronomical Tool InterConnection + PLASTIC is a protocol for communication between client-side astronomy + applications. It is very simple for application developers to adopt and is + easily extended. Through PLASTIC applications can do tasks such as instruct + each other to load VOTables, highlight a subset of rows or load an image of a + particular area of sky. Although such operations are quite simple, they + enable powerful collaborations between tools. The philosophy is that the + astronomer should have a suite of interoperating tools at his disposal, each + of which does one thing well and which can be composed according to his + particular needs. + +Depends: specview +Homepage: http://www.stsci.edu/resources/software_hardware/specview +Pkg-Description: 1-D spectral visualization and analysis of astronomical spectrograms + Specview is a tool for 1-D spectral visualization and analysis of + astronomical spectrograms. Written in Java, it is capable of reading all + the Hubble Space Telescope spectral data formats as well as data from + several other instruments (such as IUE, FUSE, ISO, FORS and SDSS), + preview spectra from MAST, and data from generic FITS and ASCII tables. + It can read data from Virtual Observatory servers, and read and write + spectrogram data in Virtual Observatory SED format. It can also read + files in the SPC Galactic format used in the chemistry field. Once + ingested, data can be plotted and examined with a large selection of + custom settings. Specview supports instrument-specific data quality + handling, flexible spectral units conversions, custom plotting + attributes, plot annotations, tiled plots, hardcopy to JPEG files and + PostScript file or printer, etc. Specview can be used to build wide-band + SEDs, overplotting or combining data from the same astronomical source + taken with different instruments and/or spectral bands. Data can be + further processed with averaging, splicing, detrending, and Fourier + filtering tools. Specview has a spectral model fitting capability that + enables the user to work with multi-component models (including user- + defined models) and fit models to data. + +Depends: splat-vo +WNPP: 827354 +Homepage: http://star-www.dur.ac.uk/~pdraper/splat/splat-vo/ +Pkg-Description: Spectral Analysis Tool + SPLAT is a graphical tool for displaying, comparing, modifying and + analyzing astronomical spectra stored in NDF, FITS and TEXT files as + well as in NDX format. It can read in many spectra at the same time and + then display these as line plots. Display windows can show one or + several spectra at the same time and can be interactively zoomed and + scrolled, centered on specific wavelengths, provide continuous + coordinate readout, produce printable hardcopy and be configured in many + ways. Analysis facilities include the fitting of a polynomial to + selected parts of a spectrum, the fitting of Gaussian, Lorentzian and + Voigt profiles to emission and absorption lines and the filtering of + spectra using average, median and line-shape window functions as well as + wavelet denoising. SPLAT also supports a full range of coordinate + systems for spectra, which allows coordinates to be displayed and + aligned in many different coordinate systems (wavelength, frequency, + energy, velocity) and transformed between these and different standards + of rest (topocentric, heliocentric, dynamic and kinematic local + standards of rest, etc). SPLAT is distributed as part of + theStarlink(ascl:1110.012) software collection. + +Depends: stilts +Homepage: http://www.star.bris.ac.uk/~mbt/stilts/ +Pkg-Description: Starlink Tables Infrastructure Library Tool Set + The STIL Tool Set is a set of command-line tools based on STIL, the + Starlink Tables Infrastructure Library. It deals with the processing of + tabular data; the package has been designed for, but is not restricted + to, astronomical tables such as object catalogues. Some of the tools are + generic and can work with multiple formats (including FITS, VOTable, + CSV, SQL and ASCII), and others are specific to the VOTable format. In + some ways, STILTS forms the command-line counterpart of the GUI table + analysis tool TOPCAT. The package is robust, fully documented, and + designed for efficiency, especially with very large datasets.Facilities + offered include:format conversioncrossmatchingplottingcolumn calculation + and rearrangementrow selectionsdata and metadata manipulation and + displaysortingstatistical calculationshistogram calculationdata + validationVO service accessA powerful and extensible expression language + is used for specifying data calculations. These facilities can be put + together in very flexible and efficient ways. For tasks in which the + data can be streamed, the size of table STILTS can process is + effectively unlimited. For other tasks, million-row tables usually do + not present a problem. STILTS is written in pure Java (J2SE1.5 or + later), and can be run from the command line or from Jython, or embedded + into java applications. It is released under the GPL. + +Depends: topcat +Homepage: http://www.star.bristol.ac.uk/~mbt/topcat/ +Pkg-Description: Tool for OPerations on Catalogues And Tables + TOPCAT is an interactive graphical viewer and editor for tabular data. + Its aim is to provide most of the facilities that astronomers need for + analysis and manipulation of source catalogues and other tables, though + it can be used for non-astronomical data as well. It understands a + number of different astronomically important formats (including FITS and + VOTable) and more formats can be added.It offers a variety of ways to + view and analyse tables, including a browser for the cell data + themselves, viewers for information about table and column metadata, and + facilities for 1-, 2-, 3- and higher-dimensional visualisation, + calculating statistics and joining tables using flexible matching + algorithms. Using a powerful and extensible Java-based expression + language new columns can be defined and row subsets selected for + separate analysis. Table data and metadata can be edited and the + resulting modified table can be written out in a wide range of output + formats.It is a stand-alone application which works quite happily with + no network connection. However, because it uses Virtual Observatory (VO) + standards, it can cooperate smoothly with other tools in the VO world + and beyond, such as VODesktop, Aladin and ds9. Between 2006 and 2009 + TOPCAT was developed within the AstroGrid project, and is offered as + part of a standard suite of applications on the AstroGrid web site, + where you can find information on several other VO tools.The program is + written in pure Java and available under the GNU General Public Licence. + It has been developed in the UK within theStarlinkand AstroGrid + projects, and under PPARC and STFC grants. Its underlying table + processing facilities are provided by STIL. + +Depends: virgo +Homepage: http://archive.eso.org/cms/tools-documentation/visual-archive-browser +Pkg-Description: Visual Browser for the ESO Science Archive Facility + VirGO is the next generation Visual Browser for the ESO Science Archive + Facility developed by the Virtual Observatory (VO) Systems Department. + It is a plug-in for the popular open source software Stellarium adding + capabilities for browsing professional astronomical data. VirGO gives + astronomers the possibility to easily discover and select data from + millions of observations in a new visual and intuitive way. Its main + feature is to perform real-time access and graphical display of a large + number of observations by showing instrumental footprints and image + previews, and to allow their selection and filtering for subsequent + download from the ESO SAF web interface. It also allows the loading of + external FITS files or VOTables, the superimposition of Digitized Sky + Survey (DSS) background images, and the visualization of the sky in a + `real life' mode as seen from the main ESO sites. All data interfaces + are based on Virtual Observatory standards which allow access to images + and spectra from external data centers, and interaction with the ESO SAF + web interface or any other VO applications supporting the PLASTIC + messaging system. diff -Nru debian-astro-0.3/tasks/simulation debian-astro-0.4/tasks/simulation --- debian-astro-0.3/tasks/simulation 2016-02-19 07:42:45.000000000 +0000 +++ debian-astro-0.4/tasks/simulation 2016-06-22 08:17:51.000000000 +0000 @@ -1,4 +1,5 @@ Task: Simulation +Install: true Description: Simulation packages for astronomy This metapackage will install packages for celectial, astronomical and cosmological simulations. @@ -13,3 +14,29 @@ Depends: geant321 Why: taken from ascl + +Depends: cloudy +WNPP: 725891 +Pkg-Description: Simulations of non-equilibrium plasmas and their spectra + Cloudy is a spectral synthesis code designed to simulate conditions + in interstellar matter under a broad range of conditions. +Homepage: http://www.nublado.org/ + +Depends: mocassin +WNPP: 827841 +Pkg-Description: Monte Carlo simulations of ionised nebulae + MOCASSIN is a fully 3D or 2D photoionisation and dust radiative + transfer code which employs a Monte Carlo approach to the transfer of + radiation through media of arbitrary geometry and density + distribution. It was originally developed for the modelling of + photoionised regions like HII regions and planetary nebulae and has + since expanded and been applied to a variety of astrophysical + problems, including modelling clumpy dusty supernova envelopes, star + forming galaxies, protoplanetary disks and inner shell fluorence + emission in the photospheres of stars and disk atmospheres. The code + can deal with arbitrary Cartesian grids of variable resolution, it + has successfully been used to model complex density fields from SPH + calculations and can deal with ionising radiation extending from + Lyman edge to the X-ray. The dust and gas microphysics is fully + coupled both in the radiation transfer and in the thermal balance. +Homepage: http://www.3d-mocassin.net diff -Nru debian-astro-0.3/tasks/tcltk debian-astro-0.4/tasks/tcltk --- debian-astro-0.3/tasks/tcltk 2016-01-19 10:42:02.000000000 +0000 +++ debian-astro-0.4/tasks/tcltk 2016-06-20 08:51:01.000000000 +0000 @@ -1,9 +1,10 @@ Task: Tcl/Tk +Install: false Description: Tcl/Tk packages for astronomy This metapackage will install packages that are useful to develop Tcl/Tk applications for astronomy. -Depends: tcl8.6, tk8.6, blt +Depends: tcl8.6, tk8.6, blt-dev Depends: tcl-fitstcl, ftools-pow @@ -11,3 +12,4 @@ Depends: skycat +Depends: tkblt-dev diff -Nru debian-astro-0.3/tasks/telescopecontrol debian-astro-0.4/tasks/telescopecontrol --- debian-astro-0.3/tasks/telescopecontrol 2016-04-06 18:19:29.000000000 +0000 +++ debian-astro-0.4/tasks/telescopecontrol 2016-05-26 08:34:04.000000000 +0000 @@ -1,4 +1,5 @@ Task: Telescope Control +Install: true Description: Telescope control and data processing This metapackage will install Debian Astro packages to control (mainly amateur) telescopes and do their data reduction. @@ -11,6 +12,8 @@ Depends: lynkeos.app +Depends: kstars + Depends: audela WNPP: 744236 Pkg-Description: Free and open source astronomy software diff -Nru debian-astro-0.3/tasks/tools debian-astro-0.4/tasks/tools --- debian-astro-0.3/tasks/tools 2016-04-14 15:36:45.000000000 +0000 +++ debian-astro-0.4/tasks/tools 2016-05-24 09:23:48.000000000 +0000 @@ -1,4 +1,5 @@ Task: Tools +Install: true Description: Astronomy tools and utilities This metapackage will install small tools provided by Debian Astronomy packages. These tools handle smaller tasks, mainly dealing with FITS files. diff -Nru debian-astro-0.3/tasks/viewers debian-astro-0.4/tasks/viewers --- debian-astro-0.3/tasks/viewers 2016-04-04 13:40:51.000000000 +0000 +++ debian-astro-0.4/tasks/viewers 2016-07-05 13:51:14.000000000 +0000 @@ -1,4 +1,5 @@ Task: Viewers +Install: true Description: Interactive astronomical data viewers This metapackage will install software for the interactive visual inspection of astronomical data. Note that Python packages can be used for interactive @@ -17,7 +18,11 @@ Depends: paraview, mayavi2, imagej, ifrit Why: taken from ascl -Depends: vo-aladin +Depends: ginga + +Depends: qfitsview + +Depends: aladin WNPP: 818373 Pkg-Description: Interactive sky atlas for astronomical images and datasets Aladin is an desktop client for viewing and analysis of Virtual Observatory @@ -26,11 +31,3 @@ and and data centres offering access using VO protocols. Homepage: http://aladin.u-strasbg.fr/ -Depends: qfitsview -WNPP: 472961 -Pkg-Description: FITS file viewer based on DPUSER - QFitsView is a FITS file viewer based on DPUSER. In addition to displaying - two-dimensional images, it also provides means to explore three-dimensional - data cubes. It integrates the functionality of DPUSER which can be accessed - directly out of QFitsView. -Homepage: http://www.mpe.mpg.de/~ott/QFitsView/ diff -Nru debian-astro-0.3/tasks/virtual-observatory debian-astro-0.4/tasks/virtual-observatory --- debian-astro-0.3/tasks/virtual-observatory 1970-01-01 00:00:00.000000000 +0000 +++ debian-astro-0.4/tasks/virtual-observatory 2016-07-14 14:02:19.000000000 +0000 @@ -0,0 +1,70 @@ +Task: Virtual Observatory +Install: false +Metapackage: true +Description: Tools and viewers for the Virtual Observatory + This metapackage will install commonly used interfaces for interacting with + datasets and archive data within the online distributed Virtual Observatory. + . + The Virtual Observatory allows astronomers to interrogate multiple data + centers in a seamless and transparent way, provides new powerful analysis and + visualization tools within that system, and gives data centers a standard + framework for publishing and delivering services using their data. This is + made possible by standardization of data and metadata, by standardization of + data exchange methods, and by the use of a registry, which lists available + services and what can be done with them. + . + When running, many of these tools can communicate with each other + using the Simple Application Messaging Protocol (SAMP) + +Depends: libjsamp-java, libcds-savot-java, libcds-moc-java + +Depends: aladin +WNPP: 818373 + +Depends: splat-vo +WNPP: 827354 +Homepage: http://www.g-vo.org/pmwiki/About/SPLAT +Pkg-Description: Spectral Analysis Tool (SPLAT) for Virtual Observatory + Splat-VO is an desktop client for viewing and analysis of Virtual + Observatory (VO) spectral data. This graphical tool can display, + analyse, compare and modify already extracted spectra stored in FITS, + TEXT, and NDF/NDX formats. It can also interact with the Virtual + Observatory registery and data-centres to dynamically query and + download data for a particular section of the sky on-demand. + . + Splat-VO can work in multiple coordinate systems and can plot and + overlay multiple spectra at the same time. Plots are displayed in a + visually rich format. Analysis can be performed by selecting and + zooming multiple, and fitting to emission and absorption lines. + +Recommends: stilts +Homepage: http://www.star.bris.ac.uk/~mbt/stilts/ +Pkg-Description: Starlink Tables Infrastructure Library Tool Set (STILTS) for Virtual Observatory + STILTS is a command-line tool for processing tabular data within the + Virtual Observatory. All tools can process data in VOTable format + and many of the tools can additional work with other astronomical + formats (FITS, VOTable, CDF, GBIN, CSV, SQL and ASCII). + . + This tool shares backend libraries and can be regarded as a command-line + companion to TOPCAT (Debian package: 'topcat'). + +Depends: topcat +Homepage: http://www.star.bris.ac.uk/~mbt/topcat/ +Pkg-Description: Tool for Operations on Catalogues and Tables (TOPCAT) for Virtual Observatory + TOPCAT is a graphical tool for analysing and processing tabular data + within the Virtual Observatory. It includes multiple methods to view + and analyse tables and tabular data. The tool can also be used on + local data in multiple astronomical formats. Data and be shared and + exchanged with other visualisation tools using Simple Application + Messaging Protcol (SAMP). + . + This tools shares backend libraries and can be regarded as a graphical + companion to STILTS (Debian package: 'stilts'). + +Depends: tapsh +Homepage: http://soft.g-vo.org/tapsh +Pkg-Description: Table Access Protocol (TAP) Shell for Virtual Observatory + TAP Shell is a command-line interface for transmitting and receiving + Astronomical Data Query Language (ADQL) requests to remote data-centres + within the Virtual Observatory (VO). TAP Shell includes completition + allowing the exploration of the format of remote datashets at a low-level.