| Issue |
A&A
Volume 561, January 2014
|
|
|---|---|---|
| Article Number | A59 | |
| Number of page(s) | 8 | |
| Section | Astronomical instrumentation | |
| DOI | https://doi.org/10.1051/0004-6361/201322746 | |
| Published online | 23 December 2013 | |
Flat-relative optimal extraction
A quick and efficient algorithm for stabilised spectrographs⋆
1
Institut für Astrophysik, Georg-August-Universität,
Friedrich-Hund-Platz 1,
37077
Göttingen,
Germany
e-mail:
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2
Astronomy Unit, Queen Mary University of London,
Mile End Road,
London
E1 4NS,
UK
Received:
24
September
2013
Accepted:
29
October
2013
Abstract
Context. Optimal extraction is a key step in processing the raw images of spectra as registered by two-dimensional detector arrays to a one-dimensional format. Previously reported algorithms reconstruct models for a mean one-dimensional spatial profile to assist a properly weighted extraction.
Aims. We outline a simple optimal extraction algorithm (including error propagation), which is very suitable for stabilised, fibre-fed spectrographs and does not model the spatial profile shape.
Methods. A high signal-to-noise ratio, master-flat image serves as reference image and is directly used as an extraction profile mask. Each extracted spectral value is the scaling factor relative to the cross-section of the unnormalised master flat that contains all information about the spatial profile, as well as pixel-to-pixel variations, fringing, and blaze. The extracted spectrum is measured relative to the flat spectrum.
Results. Using echelle spectra of the HARPS spectrograph we demonstrate a competitive extraction performance in terms of a signal-to-noise ratio and show that extracted spectra can be used for high precision radial velocity measurement.
Conclusions. Pre- or post-flat-fielding of the data is not necessary, since all spectrograph inefficiencies inherent to the extraction mask are automatically accounted for. Also the reconstruction of the mean spatial profile by models is not needed, thereby reducing the number of operations to extract spectra. Flat-relative optimal extraction is a simple, efficient, and robust method that can be applied easily to stabilised, fibre-fed spectrographs.
Key words: instrumentation: spectrographs / methods: data analysis / techniques: image processing / techniques: radial velocities
Based on data obtained from the ESO Science Archive Facility under request number ZECHMEISTER73978. Based on observations made with the HARPS instrument on the ESO 3.6 m telescope under programme ID 074.D-0380.
© ESO, 2013
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