Ubuntu
eso-pipelines package

eso-pipelines 1.2 source package in Ubuntu

Changelog

eso-pipelines (1.2) unstable; urgency=low

  * Use https for copyright format URL
  * Fix VCS URLs
  * Update Standards-Version to 3.9.8. No changes needed.
  * Remove cpl-plugin-sinfo from Recommends. Package is not in Testing anymore.
    (Closes: #860097)
  * Remove lintian override that is not needed anymore

 -- Ole Streicher <email address hidden>  Tue, 11 Apr 2017 15:07:07 +0200

Upload details

Uploaded by:
Debian Astronomy Maintainers
Uploaded to:
Sid
Original maintainer:
Debian Astronomy Maintainers
Architectures:
all
Section:
misc
Urgency:
Low Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Bionic release universe misc

Builds

Artful: [FULLYBUILT] amd64

Downloads

File Size SHA-256 Checksum
eso-pipelines_1.2.dsc 1.6 KiB 6ba5eb5cc47f3844a30eb1b76d2f74e0380d4e6e3be8f8d4e54365b0215d6b4b
eso-pipelines_1.2.tar.xz 1.7 KiB c2b842c842454a8eeb2d8571b2286e40225489cb689ccc5c8dc7291c705ed83e

Available diffs

No changes file available.

Binary packages built by this source

eso-pipelines: ESO VLT Instrument pipeline collection

 In collaboration with the various instrument consortia, the Pipeline Systems
 Department has undertaken to implement data reduction pipelines for the most
 commonly used VLT/VLTI instrument modes. These data reduction pipelines have
 three main purposes:
 .
  * Data quality control: Pipelines are used to produce the quantitative
    information necessary to monitor instrument performance.
 .
  * Master calibration product creation: pipelines are used to produce master
    calibration products (e.g. combined bias frames, super-flats, wavelength
    dispersion solutions).
 .
  * Science product creation: using pipeline-generated master calibration
    products, science products are produced for supported instrument modes
    (e.g. combined ISAAC jitter stacks; bias-corrected, flat-fielded FORS
    images, wavelength-calibrated UVES spectra). The accuracy of the science
    products can be limited both by the quality of the available master
    calibration products and by the algorithmic implementation of the
    pipelines themselves. In particular, adopted reduction strategies may not
    be suitable for all scientific goals.
 .
 This metapackage will install all ESO VLT pipelines along with the
 environments needed to run them (esorex, python-cpl).