The pipeline for the GOSSS data reduction
Alfredo Sota, Jes\'us Ma\'iz Apell\'aniz

TL;DR
The paper presents an automated IDL pipeline for efficient reduction of spectroscopic data from the GOSSS project, enabling rapid and accurate processing of large volumes of stellar spectra.
Contribution
It introduces a new automated spectroscopic reduction pipeline that operates in both quicklook and full modes, streamlining data processing for the GOSSS survey.
Findings
Quicklook mode processes spectra within minutes after observation.
Pipeline automatically identifies image types and applies standard reductions.
It enhances data quality by merging spectra and correcting defects.
Abstract
The Galactic O-Star Spectroscopic Survey (GOSSS) is an ambitious project that is observing all known Galactic O stars with B < 13 in the blue-violet part of the spectrum with R-2500. It is based on version 2 of the most complete catalog to date of Galactic O stars with accurate spectral types (v1, Ma\'iz Apell\'aniz et al. 2004 ;v2, Sota et al. 2008). Given the large amount of data that we are getting (more than 150 nights of observations at three different observatories in the last 4 years) we have developed an automatic spectroscopic reduction pipeline. This pipeline has been programmed in IDL and automates the process of data reduction. It can operate in two modes: automatic data reduction (quicklook) or semi-automatic data reduction (full). In "quicklook", we are able to get rectified and calibrated spectra of all stars of a full night just minutes after the observations. The…
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Taxonomy
TopicsGeophysics and Gravity Measurements
