SIMBAD references

2013A&A...558A..56D - Astronomy and Astrophysics, volume 558A, 56-56 (2013/10-1)

The software package for astronomical reductions with KMOS: SPARK.

DAVIES R.I., AGUDO BERBEL A., WIEZORREK E., CIRASUOLO M., FOERSTER SCHREIBER N.M., JUNG Y., MUSCHIELOK B., OTT T., RAMSAY S., SCHLICHTER J., SHARPLES R. and WEGNER M.

Abstract (from CDS):

The K-band Multi Object Spectrograph (KMOS) is a multi-object near-infrared integral field spectrometer with 24 deployable cryogenic pick-off arms. Inevitably, data processing is a complex task that requires careful calibration and quality control. In this paper we describe all the steps involved in producing science-quality data products from the raw observations. In particular, we focus on the following issues: (i) the calibration scheme which produces maps of the spatial and spectral locations of all illuminated pixels on the detectors; (ii) our concept of minimising the number of interpolations, to the limiting case of a single reconstruction that simultaneously uses raw data from multiple exposures; (iii) a comparison of the various interpolation methods implemented, and an assessment of the performance of true 3D interpolation schemes; (iv) the way in which instrumental flexure is measured and compensated. We finish by presenting some examples of data processed using the pipeline.

Abstract Copyright:

Journal keyword(s): methods: data analysis - techniques: imaging spectroscopy - instrumentation: spectrographs - infrared: general

Simbad objects: 7

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