Abstract
We present an integrated end-end simulation of the spectral images that
will be obtained by the weave spectrograph, which aims to include full
modelling of all effects from the top of the atmosphere to the detector.
These data are based in input spectra from a combination of library
spectra and synthetic models, and will be used to provide inputs for an
endend test of the full weave data pipeline and archive systems, prior
to 1st light of the instrument.
Original language | English |
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Article number | 99132x |
Number of pages | 8 |
Journal | Proceedings of the Society of Photo-optical Instrumentation Engineers |
Volume | 9913 |
DOIs | |
Publication status | Published - 2-Aug-2016 |
Event | Software and Cyberinfrastructure for Astronomy IV - Edinburgh, United Kingdom Duration: 26-Jun-2016 → 30-Jun-2016 |