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[ascl:1708.019] SINFONI Pipeline: Data reduction pipeline for the Very Large Telescope SINFONI spectrograph

The SINFONI pipeline reduces data from the Very Large Telescope's SINFONI (Spectrograph for INtegral Field Observations in the Near Infrared) instrument. It can evaluate the detector linearity and generate a corresponding non linear pixel map, create a master dark and a hot-pixel map, a master flat and a map of pixels which have intensities greater than a given threshold. It can also compute the optical distortions and slitlets distances, and perform wavelength calibration, PSF, telluric standard and other science data reduction, and can coadd bad pixel maps, collapse a cube to an image over a given wavelength range, perform cube arithmetics, among other useful tasks.

Code site:
https://www.eso.org/sci/software/pipelines/sinfoni/sinfoni-pipe-recipes.html
Appears in:
https://ui.adsabs.harvard.edu/#abs/2003SPIE.4841.1548E
Bibcode:
2017ascl.soft08019E
Preferred citation method:

https://ui.adsabs.harvard.edu/#abs/2003SPIE.4841.1548E and Bonnet, H. et al. 2004, The ESO Messenger 117, 17


ascl:1708.019
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