2015/03/04 by Igor Chilingarian, Yuri Beletsky, Sean Moran +3 · 39 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Background subtraction #Data reduction #Data set #Galaxies: Formation, Evolution, Phenomena #Infrared #Noise reduction #Pipeline (software) #Reduction (mathematics) #Sky #Spectrograph #Stellar, planetary, and galactic studies #astro-ph.IM
paper · pdf · doi:10.1086/680598
published in Publications of the Astronomical Society of the Pacific 127(950), 406-420 (Institute of Physics) · PASP in press, 14 pages, 6 figures
openalex publication_date 2015/03/04 · arxiv created 2015/03/25 · arxiv updated 2015/06/24 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We describe the new spectroscopic data reduction pipeline for the multi-object MMT/Magellan Infrared Spectrograph. The pipeline is implemented in idl as a stand-alone package and is publicly available in both stable and development versions. We describe novel algorithms for sky subtraction and correction for telluric absorption. We demonstrate that our sky subtraction technique reaches the Poisson limit set by the photon statistics. Our telluric correction uses a hybrid approach by first computing a correction function from an observed stellar spectrum, and then differentially correcting it using a grid of atmosphere transmission models for the target airmass value. The pipeline provides a sufficient level of performance for real time reduction and thus enables data quality control during observations. We reduce an example dataset to demonstrate the high data reduction quality.