deb_control_files:
- control
- md5sums
deb_fields:
Architecture: amd64
Depends: libc6 (>= 2.35), libcext0 (>= 5.3.1), libcfitsio10 (>= 4.2.0~), libcplcore26
(>= 6.4), libcpldfs26 (>= 6.0), libcpldrs26 (>= 6.4), libcplui26 (>= 6.4), libgomp1
(>= 4.9), libgsl27 (>= 2.7.1), libqfits0
Description: |-
ESO data reduction pipeline for the UVES instrument
This is the data reduction pipeline for the UVES instrument of the Very
Large Telescope (VLT) from the European Southern Observatory (ESO).
.
UVES is a cross-dispersed echelle spectrograph designed to operate with
high efficiency from the atmospheric cut-off at 300 nm to the long
wavelength limit of the CCD detectors (about 1100 nm). The light beam
from the telescope is split in two arms (UV to Blue, and Visual to Red)
within the instrument. The two arms can be operated separately, or in
parallel via a dichroic beam splitter. The resolving power is about
40,000 when a 1-arcsec slit is used. The maximum (two-pixel) resolution
is 80,000 or 110,000 in the Blue- and the Red Arm, respectively.
Homepage: https://www.eso.org/sci/software/pipelines/uves
Installed-Size: '3723'
Maintainer: Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
Multi-Arch: same
Package: cpl-plugin-uves
Priority: optional
Recommends: esorex | python3-cpl
Section: science
Source: cpl-plugin-uves (6.1.8+dfsg-2)
Suggests: cpl-plugin-uves-calib, cpl-plugin-uves-doc
Version: 6.1.8+dfsg-2+b1
srcpkg_name: cpl-plugin-uves
srcpkg_version: 6.1.8+dfsg-2