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A Full Implementation of Spectro-perfectionism for Precise Radial Velocity Exoplanet Detection
by
Bolton, Adam S.
, Sliski, David H.
, Wang, Sharon X.
, Johnson, John Asher
, Wilson, Maurice L.
, Eastman, Jason D.
, Johnson, Samson A.
, Wittenmyer, Robert A.
, Plavchan, Peter
, McCrady, Nate
, Wright, Jason T.
, Cornachione, Matthew A.
, Horner, Jonathan
in
Astronomical Software, Data Analysis, and Techniques
2019
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A Full Implementation of Spectro-perfectionism for Precise Radial Velocity Exoplanet Detection
by
Bolton, Adam S.
, Sliski, David H.
, Wang, Sharon X.
, Johnson, John Asher
, Wilson, Maurice L.
, Eastman, Jason D.
, Johnson, Samson A.
, Wittenmyer, Robert A.
, Plavchan, Peter
, McCrady, Nate
, Wright, Jason T.
, Cornachione, Matthew A.
, Horner, Jonathan
in
Astronomical Software, Data Analysis, and Techniques
2019
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Do you wish to request the book?
A Full Implementation of Spectro-perfectionism for Precise Radial Velocity Exoplanet Detection
by
Bolton, Adam S.
, Sliski, David H.
, Wang, Sharon X.
, Johnson, John Asher
, Wilson, Maurice L.
, Eastman, Jason D.
, Johnson, Samson A.
, Wittenmyer, Robert A.
, Plavchan, Peter
, McCrady, Nate
, Wright, Jason T.
, Cornachione, Matthew A.
, Horner, Jonathan
in
Astronomical Software, Data Analysis, and Techniques
2019
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A Full Implementation of Spectro-perfectionism for Precise Radial Velocity Exoplanet Detection
Journal Article
A Full Implementation of Spectro-perfectionism for Precise Radial Velocity Exoplanet Detection
2019
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Overview
We present a computationally tractable implementation of spectro-perfectionism, a method which minimizes error imparted by spectral extraction. We develop our method in conjunction with a full raw reduction pipeline for the MINiature Exoplanet Radial Velocity Array (MINERVA), capable of performing both optimal extraction and spectro-perfectionism. Although spectro-perfectionism remains computationally expensive, our implementation can extract a MINERVA exposure in approximately 30 minutes. We describe our localized extraction procedure and our approach to point-spread function (PSF) fitting. We compare the performance of both extraction methods on a set of 119 exposures on HD 122064, an RV standard star. Both the optimal extraction and spectro-perfectionism pipelines achieve nearly identical RV precision under a six-exposure chronological binning. We discuss the importance of reliable calibration data for PSF fitting and the potential of spectro-perfectionism for future precise radial velocity exoplanet studies.
Publisher
IOP Publishing Limited
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