软件包：cpl-plugin-uves（6.1.8+dfsg-2 以及其他的） [debports]
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.
其他与 cpl-plugin-uves 有关的软件包
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- dep: libc6 (>= 2.33)
- GNU C 语言运行库：共享库
同时作为一个虚包由这些包填实： libc6-udeb
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- dep: libcext0 (>= 5.3.1)
- Commonly used utility functions for C programs
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- dep: libcfitsio10 (>= 4.2.0~)
- shared library for I/O with FITS format data files
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- dep: libcplcore26 (>= 6.4)
- Fundamental CPL data types and functions
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- dep: libcpldfs26 (>= 6.0)
- CPL functions for Data Flow System compatibility
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- dep: libcpldrs26 (>= 6.4)
- CPL higher level data processing algorithms
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- dep: libcplui26 (>= 6.4)
- CPL framework interface library
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- dep: libgomp1 (>= 4.9)
- GCC OpenMP（GOMP）支持库
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- dep: libgsl27 (>= 2.7.1)
- GNU Scientific Library (GSL) -- library package
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- dep: libqfits0
- Library offering easy access to FITS files
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- rec: esorex
- Execution Tool for European Southern Observatory pipelines
- 或者 python3-cpl
- Control pipeline recipes from the ESO (Python3)
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- sug: cpl-plugin-uves-calib
- 软件包暂时不可用
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- sug: cpl-plugin-uves-doc
- 软件包暂时不可用