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Proceedings Paper

The VIRUS data reduction pipeline
Author(s): Claus A. Goessl; Niv Drory; Helena Relke; Karl Gebhardt; Frank Grupp; Gary Hill; Ulrich Hopp; Ralf Köhler; Phillip MacQueen
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Paper Abstract

The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) will measure baryonic acoustic oscillations, first discovered in the Cosmic Microwave Background (CMB), to constrain the nature of dark energy by performing a blind search for Ly-α emitting galaxies within a 200 deg2 field and a redshift bin of 1.8 < z < 3.7. This will be achieved by VIRUS, a wide field, low resolution, 145 IFU spectrograph. The data reduction pipeline will have to extract ≈ 35.000 spectra per exposure (≈5 million per night, i.e. 500 million in total), perform an astrometric, photometric, and wavelength calibration, and find and classify objects in the spectra fully automatically. We will describe our ideas how to achieve this goal.

Paper Details

Date Published: 30 June 2006
PDF: 11 pages
Proc. SPIE 6270, Observatory Operations: Strategies, Processes, and Systems, 627021 (30 June 2006); doi: 10.1117/12.671264
Show Author Affiliations
Claus A. Goessl, Univ.-Sternwarte München (Germany)
Niv Drory, The Univ. of Texas at Austin (United States)
Helena Relke, Max-Planck-Institut für extraterrestrische Physik (Germany)
Karl Gebhardt, The Univ. of Texas at Austin (United States)
Frank Grupp, Univ.-Sternwarte München (Germany)
Gary Hill, The Univ. of Texas at Austin (United States)
Ulrich Hopp, Univ.-Sternwarte München (Germany)
Max-Planck-Institut für extraterrestrische Physik (Germany)
Ralf Köhler, Univ.-Sternwarte München (Germany)
Phillip MacQueen, The Univ. of Texas at Austin (United States)

Published in SPIE Proceedings Vol. 6270:
Observatory Operations: Strategies, Processes, and Systems
David R. Silva; Rodger E. Doxsey, Editor(s)

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