iraf-rvsao 2.8.3-1build3 source package in Ubuntu


iraf-rvsao (2.8.3-1build3) groovy; urgency=medium

  * No change rebuild against new cfitsio ABI.

 -- Dimitri John Ledkov <email address hidden>  Thu, 27 Aug 2020 23:47:29 +0100

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Uploaded by:
Dimitri John Ledkov on 2020-08-27
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Ubuntu Developers
Medium Urgency

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Series Pocket Published Component Section
Hirsute release 1 hour ago universe misc
Groovy release on 2020-09-04 universe misc


File Size SHA-256 Checksum
iraf-rvsao_2.8.3.orig.tar.gz 5.6 MiB 3ad85610ae571b9c0b963453fdbb6a8dc36fd413bfd4f021c66f2ce1b56b9bf0
iraf-rvsao_2.8.3-1build3.debian.tar.xz 4.0 KiB 1ba811a4f500ae8b099ebc081bb61a841ba942eae18d2d02d96f919985a2c5e2
iraf-rvsao_2.8.3-1build3.dsc 2.0 KiB b149ac043786d4cd3f8d6afdee4124fa610a9fa6e902413712c3dc13c80cd75c

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Binary packages built by this source

iraf-rvsao: IRAF package to obtain radial velocities from spectra

 This package obtains radial velocities and velocity dispersions using
 cross-correlation methods or emission line fits. It consists of
 several SPP tasks:
  * XCSAO and PXCSAO: cross-correlate spectra,
  * EMSAO and PEMSAO: find emission lines in spectra,
  * BCVCORR: solar system barycentric velocity correction,
  * SUMSPEC: add and/or modify spectra,
  * LINESPEC: synthetic emission line templates,
  * EQWIDTH: equivalent widths of lines in spectra,
  * WLRANGE: wavelength overlap range for a list of spectra,
  * LISTSPEC: list pixel, wavelength, delta wavelength, and/or pixel value for
    spectrum image,
  * PIX2WL: wavelength at a given pixel in a spectrum,
  * WL2PIX: pixel at a given wavelength in a spectrum,
  * VELSET Artificially change the redshift of (log-wavelength) spectra

iraf-rvsao-dbgsym: debug symbols for iraf-rvsao