Sky Subtraction for the MUSE Data Reduction Pipeline

Details Sky Subtraction for the MUSE Data Reduction Pipeline Sky Subtraction for the MUSE Data Reduction Pipeline

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..442..257s&link_type=abstract

Astronomical Data Analysis Software and Systems XX. ASP Conference Proceedings, Vol. 442, proceedings of a Conference held at Se

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Methodology

Scientific paper

The Multi Unit Spectroscopic Explorer (MUSE) is a second-generation integral-field spectrograph currently in development for the Very Large Telescope (VLT), consisting of 24 Integral Field Units (IFU). This paper presents the methodology for sky subtraction to be used in the MUSE data reduction pipeline. The method is based on the parameterized simulation of the night sky emission processes and the instrument response. In most cases, this method makes a separate sky exposition obsolete. The approach is described and illustrated here using simulated data.

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