Abstract
We present a fast and portable reimplementation of Piskunov and Valenti's optimal-extraction algorithm (Piskunov & Valenti 2002) in C/C++ together with full uncertainty propagation, improved cosmicray removal, and an optimal background-subtraction algorithm. This reimplementation can be used with IRAF and most existing data-reduction packages and leads to signal-to-noise ratios close to the Poisson limit. The algorithm is very stable, operates on spectra from a wide range of instruments (slit spectra and fibre feeds), and has been extensively tested for VLT/UVES, ESO/CES, ESO/FEROS, NTT/EMMI, NOT/ALFOSC, STELLA/SES, SSO/ WiFeS, and finally, P60/SEDM-IFU data.
| Original language | English |
|---|---|
| Pages (from-to) | 170-179 |
| Number of pages | 10 |
| Journal | Publications of the Astronomical Society of the Pacific |
| Volume | 126 |
| Issue number | 936 |
| DOIs | |
| Publication status | Published - 2014 |
Keywords
- algorithms
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