- libc6 (>= 2.29)
- libcext0 (>= 5.3.1)
- libcplcore26 (>= 7.2.2)
- libcpldfs26 (>= 6.5)
- libcpldrs26 (>= 6.4)
- libcplui26 (>= 6.3)
- libgomp1 (>= 4.9)
- libgsl27 (>= 2.7.1)
This is the data reduction pipeline for the Muse instrument of the
Very Large Telescope (VLT) from the European Southern Observatory (ESO).
.
MUSE, the Multi-Unit Spectroscopic Explorer, is an Integral Field
Spectrograph located at the Nasmyth B focus of Yepun, the VLT UT4
telescope. It has a modular structure composed of 24 identical IFU modules
that together sample, in Wide Field Mode (WFM), a near-contiguous 1 squared
arcmin field of view. Spectrally the instrument samples almost the full
optical domain with a mean resolution of 3000. Spatially, the instrument
samples the sky with 0.2 arcseconds spatial pixels in the currently offered
Wide Field Mode with natural seeing (WFM-noAO).
Installed Size: 15.6 MB
Architectures: arm64 amd64