How to Install and Uninstall cpl-plugin-fors Package on Kali Linux

Last updated: November 05,2024

1. Install "cpl-plugin-fors" package

This is a short guide on how to install cpl-plugin-fors on Kali Linux

$ sudo apt update $ sudo apt install cpl-plugin-fors

2. Uninstall "cpl-plugin-fors" package

Here is a brief guide to show you how to uninstall cpl-plugin-fors on Kali Linux:

$ sudo apt remove cpl-plugin-fors $ sudo apt autoclean && sudo apt autoremove

3. Information about the cpl-plugin-fors package on Kali Linux

Package: cpl-plugin-fors
Source: cpl-plugin-fors (5.5.7+dfsg-2)
Version: 5.5.7+dfsg-2+b1
Installed-Size: 11325
Maintainer: Debian Astronomy Maintainers
Architecture: amd64
Depends: libc6 (>= 2.29), libcext0 (>= 5.3.1), libcplcore26 (>= 6.4), libcpldfs26 (>= 6.0), libcpldrs26 (>= 6.4), libcplui26 (>= 6.4), libgcc-s1 (>= 4.0), libgomp1 (>= 4.9), libgsl27 (>= 2.7.1), libstdc++6 (>= 11)
Recommends: esorex | python3-cpl, source-extractor
Suggests: cpl-plugin-fors-calib (= 5.5.7+dfsg-2+b1), cpl-plugin-fors-doc
Size: 1061104
SHA256: 4c4c48d83faaa318512b7fb8719f2280bc47602e0b861171eec84455bf1a0da1
SHA1: 11368465e30d1cf2dd9d7b6d9f99a2785963a002
MD5sum: 0e26e23d8af94470bb6e4f6235962b50
Description: ESO data reduction pipeline for the FORS1/2 instruments
FORS pipeline recipes for the reduction of data obtained with the FORS1 and
FORS2 instruments in the LSS, MOS, MXU, PMOS, and direct imaging instrument
modes.
.
FORS is the visual and near UV FOcal Reducer and low dispersion Spectrograph
for the Very Large Telescope (VLT) of the European Southern Observatory
(ESO). Two versions of FORS have been built, upgraded and moved to the
Cassegrain foci of different telescopes in the past years. In April 2009,
FORS1 was dismounted to make room for X-shooter, so only FORS2 is in
operation. FORS is designed as an all-dioptric instrument for the wavelength
range from 330 nm to 1100 nm and provides an image scale of 0".25/pixel (or
0".125/pixel with the high resolution collimator) in the standard readout
mode (2x2 binning). FORS2 is installed on UT1 (Antu) and is by default
equipped with a detector system that is optimised for the red with a very low
level of fringes thanks to a mosaic of two 2k x 4k MIT CCDs (with 15 μm
pixels). However, the blue-optimised detector system that was previously
available on FORS1 has been commissioned on FORS2 and can be requested for
Visitor Mode observation. The geometries of both detector systems are
similar, with the optical axis falling ~30" above the gap and offsets of a
few arc-seconds between the two chips. FORS2 has many modes, including
multi-object spectroscopy with exchangeable masks, long-slit spectroscopy,
imaging and spectro-polarimetry and high-time resolution imaging and
spectroscopy.
Description-md5: bc62d65505a7f0e2f157b1acbe092f8a
Multi-Arch: same
Homepage: https://www.eso.org/sci/software/pipelines/fors
Section: science
Priority: optional
Filename: pool/main/c/cpl-plugin-fors/cpl-plugin-fors_5.5.7+dfsg-2+b1_amd64.deb