MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph

We introduce a data-reduction package written in Interactive Data Language (IDL) for the Magellan Echellete Spectrograph (MAGE). MAGE is a medium-resolution (R 4100), cross-dispersed, optical spectrograph, with coverage from . The MAGE Spectral Extractor (MASE) incorporates the entire image reducti...

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Main Authors: Murphy, Michael T., Bernstein, Rebecca A., Burles, Scott, Prochaska, J. Xavier, Hennawi, Joseph F., Williams, Christopher Leigh, Simcoe, Robert A., Bochanski, John J., Burgasser, Adam J., West, A. A.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Astronomical Society of the Pacific 2010
Online Access:http://hdl.handle.net/1721.1/55354
https://orcid.org/0000-0001-7130-208X
https://orcid.org/0000-0003-3769-9559
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author Murphy, Michael T.
Bernstein, Rebecca A.
Burles, Scott
Prochaska, J. Xavier
Hennawi, Joseph F.
Williams, Christopher Leigh
Simcoe, Robert A.
Bochanski, John J.
Burgasser, Adam J.
West, A. A.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Murphy, Michael T.
Bernstein, Rebecca A.
Burles, Scott
Prochaska, J. Xavier
Hennawi, Joseph F.
Williams, Christopher Leigh
Simcoe, Robert A.
Bochanski, John J.
Burgasser, Adam J.
West, A. A.
author_sort Murphy, Michael T.
collection MIT
description We introduce a data-reduction package written in Interactive Data Language (IDL) for the Magellan Echellete Spectrograph (MAGE). MAGE is a medium-resolution (R 4100), cross-dispersed, optical spectrograph, with coverage from . The MAGE Spectral Extractor (MASE) incorporates the entire image reduction and calibration process, including bias subtraction, flat fielding, wavelength calibration, sky subtraction, object extraction, and flux calibration of point sources. We include examples of the user interface and reduced spectra. We show that the wavelength calibration is sufficient to achieve 5 km s-1 rms accuracy and relative flux calibrations better than 10%. A lightweight version of the full reduction pipeline has been included for real-time source extraction and signal-to-noise estimation at the telescope.
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spelling mit-1721.1/553542022-09-26T12:43:43Z MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph Murphy, Michael T. Bernstein, Rebecca A. Burles, Scott Prochaska, J. Xavier Hennawi, Joseph F. Williams, Christopher Leigh Simcoe, Robert A. Bochanski, John J. Burgasser, Adam J. West, A. A. Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research Burgasser, Adam J. Williams, Christopher Leigh West, Andrew A. Simcoe, Robert A. Bochanski, John J. Burgasser, Adam J. We introduce a data-reduction package written in Interactive Data Language (IDL) for the Magellan Echellete Spectrograph (MAGE). MAGE is a medium-resolution (R 4100), cross-dispersed, optical spectrograph, with coverage from . The MAGE Spectral Extractor (MASE) incorporates the entire image reduction and calibration process, including bias subtraction, flat fielding, wavelength calibration, sky subtraction, object extraction, and flux calibration of point sources. We include examples of the user interface and reduced spectra. We show that the wavelength calibration is sufficient to achieve 5 km s-1 rms accuracy and relative flux calibrations better than 10%. A lightweight version of the full reduction pipeline has been included for real-time source extraction and signal-to-noise estimation at the telescope. National Science Foundation (AST- 0215989) Massachusetts Institute of Technology. School of Science Carnegie Observatories 2010-05-28T19:48:42Z 2010-05-28T19:48:42Z 2009-11 2007-07 Article http://purl.org/eprint/type/SubmittedJournalArticle 1538-3873 0004-6280 http://hdl.handle.net/1721.1/55354 Bochanski, John J et al. “MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph.” Publications of the Astronomical Society of the Pacific 121.886 (2009): 1409-1418. © 2009 The Astronomical Society of the Pacific. https://orcid.org/0000-0001-7130-208X https://orcid.org/0000-0003-3769-9559 en_US http://dx.doi.org/10.1086/648597 Publications of the Astronomical Society of the Pacific Attribution-Noncommercial-Share Alike 3.0 Unported http://creativecommons.org/licenses/by-nc-sa/3.0/ application/pdf Astronomical Society of the Pacific author/dept web page
spellingShingle Murphy, Michael T.
Bernstein, Rebecca A.
Burles, Scott
Prochaska, J. Xavier
Hennawi, Joseph F.
Williams, Christopher Leigh
Simcoe, Robert A.
Bochanski, John J.
Burgasser, Adam J.
West, A. A.
MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph
title MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph
title_full MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph
title_fullStr MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph
title_full_unstemmed MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph
title_short MASE: A New Data-Reduction Pipeline for the Magellan Echellette Spectrograph
title_sort mase a new data reduction pipeline for the magellan echellette spectrograph
url http://hdl.handle.net/1721.1/55354
https://orcid.org/0000-0001-7130-208X
https://orcid.org/0000-0003-3769-9559
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