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@ARTICLE{Astropy:2018, | ||
author = {{Astropy Collaboration} and {Price-Whelan}, A.~M. and {Sip{\H o}cz}, B.~M. and | ||
{G{\"u}nther}, H.~M. and {Lim}, P.~L. and {Crawford}, S.~M. and | ||
{Conseil}, S. and {Shupe}, D.~L. and {Craig}, M.~W. and {Dencheva}, N. and | ||
{Ginsburg}, A. and {VanderPlas}, J.~T. and {Bradley}, L.~D. and | ||
{P{\'e}rez-Su{\'a}rez}, D. and {de Val-Borro}, M. and {Aldcroft}, T.~L. and | ||
{Cruz}, K.~L. and {Robitaille}, T.~P. and {Tollerud}, E.~J. and | ||
{Ardelean}, C. and {Babej}, T. and {Bach}, Y.~P. and {Bachetti}, M. and | ||
{Bakanov}, A.~V. and {Bamford}, S.~P. and {Barentsen}, G. and | ||
{Barmby}, P. and {Baumbach}, A. and {Berry}, K.~L. and {Biscani}, F. and | ||
{Boquien}, M. and {Bostroem}, K.~A. and {Bouma}, L.~G. and {Brammer}, G.~B. and | ||
{Bray}, E.~M. and {Breytenbach}, H. and {Buddelmeijer}, H. and | ||
{Burke}, D.~J. and {Calderone}, G. and {Cano Rodr{\'{\i}}guez}, J.~L. and | ||
{Cara}, M. and {Cardoso}, J.~V.~M. and {Cheedella}, S. and {Copin}, Y. and | ||
{Corrales}, L. and {Crichton}, D. and {D'Avella}, D. and {Deil}, C. and | ||
{Depagne}, {\'E}. and {Dietrich}, J.~P. and {Donath}, A. and | ||
{Droettboom}, M. and {Earl}, N. and {Erben}, T. and {Fabbro}, S. and | ||
{Ferreira}, L.~A. and {Finethy}, T. and {Fox}, R.~T. and {Garrison}, L.~H. and | ||
{Gibbons}, S.~L.~J. and {Goldstein}, D.~A. and {Gommers}, R. and | ||
{Greco}, J.~P. and {Greenfield}, P. and {Groener}, A.~M. and | ||
{Grollier}, F. and {Hagen}, A. and {Hirst}, P. and {Homeier}, D. and | ||
{Horton}, A.~J. and {Hosseinzadeh}, G. and {Hu}, L. and {Hunkeler}, J.~S. and | ||
{Ivezi{\'c}}, {\v Z}. and {Jain}, A. and {Jenness}, T. and {Kanarek}, G. and | ||
{Kendrew}, S. and {Kern}, N.~S. and {Kerzendorf}, W.~E. and | ||
{Khvalko}, A. and {King}, J. and {Kirkby}, D. and {Kulkarni}, A.~M. and | ||
{Kumar}, A. and {Lee}, A. and {Lenz}, D. and {Littlefair}, S.~P. and | ||
{Ma}, Z. and {Macleod}, D.~M. and {Mastropietro}, M. and {McCully}, C. and | ||
{Montagnac}, S. and {Morris}, B.~M. and {Mueller}, M. and {Mumford}, S.~J. and | ||
{Muna}, D. and {Murphy}, N.~A. and {Nelson}, S. and {Nguyen}, G.~H. and | ||
{Ninan}, J.~P. and {N{\"o}the}, M. and {Ogaz}, S. and {Oh}, S. and | ||
{Parejko}, J.~K. and {Parley}, N. and {Pascual}, S. and {Patil}, R. and | ||
{Patil}, A.~A. and {Plunkett}, A.~L. and {Prochaska}, J.~X. and | ||
{Rastogi}, T. and {Reddy Janga}, V. and {Sabater}, J. and {Sakurikar}, P. and | ||
{Seifert}, M. and {Sherbert}, L.~E. and {Sherwood-Taylor}, H. and | ||
{Shih}, A.~Y. and {Sick}, J. and {Silbiger}, M.~T. and {Singanamalla}, S. and | ||
{Singer}, L.~P. and {Sladen}, P.~H. and {Sooley}, K.~A. and | ||
{Sornarajah}, S. and {Streicher}, O. and {Teuben}, P. and {Thomas}, S.~W. and | ||
{Tremblay}, G.~R. and {Turner}, J.~E.~H. and {Terr{\'o}n}, V. and | ||
{van Kerkwijk}, M.~H. and {de la Vega}, A. and {Watkins}, L.~L. and | ||
{Weaver}, B.~A. and {Whitmore}, J.~B. and {Woillez}, J. and | ||
{Zabalza}, V. and {Astropy Contributors}}, | ||
title = "{The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package}", | ||
journal = {\aj}, | ||
archivePrefix = "arXiv", | ||
eprint = {1801.02634}, | ||
primaryClass = "astro-ph.IM", | ||
keywords = {methods: data analysis, methods: miscellaneous, methods: statistical, reference systems }, | ||
year = 2018, | ||
month = sep, | ||
volume = 156, | ||
eid = {123}, | ||
pages = {123}, | ||
doi = {10.3847/1538-3881/aabc4f}, | ||
adsurl = {http://adsabs.harvard.edu/abs/2018AJ....156..123A}, | ||
adsnote = {Provided by the SAO/NASA Astrophysics Data System} | ||
} | ||
|
||
@ARTICLE{Numpy:2011, | ||
author={S. {van der Walt} and S. C. {Colbert} and G. {Varoquaux}}, | ||
journal={Computing in Science Engineering}, | ||
title={The NumPy Array: A Structure for Efficient Numerical Computation}, | ||
year={2011}, | ||
volume={13}, | ||
number={2}, | ||
pages={22-30}, | ||
keywords={data structures;high level languages;mathematics computing;numerical analysis;numerical computation;numpy array;numerical data;high level language;Python programming language;Arrays;Numerical analysis;Performance evaluation;Computational efficiency;Finite element methods;Vector quantization;Resource management;Python;NumPy;scientific programming;numerical computations;programming libraries}, | ||
doi={10.1109/MCSE.2011.37}, | ||
ISSN={1558-366X}, | ||
month={March} | ||
} | ||
|
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--- | ||
title: 'linea: Fast linear detrending for CHEOPS photometry' | ||
tags: | ||
- Python | ||
- astronomy | ||
- photometry | ||
authors: | ||
- name: Brett M. Morris | ||
orcid: 0000-0003-2528-3409 | ||
affiliation: "1" | ||
affiliations: | ||
- name: Center for Space and Habitability, University of Bern, | ||
Gesellschaftsstrasse 6, CH-3012, Bern, Switzerland | ||
index: 1 | ||
date: 18 June 2020 | ||
bibliography: paper.bib | ||
--- | ||
|
||
# Summary | ||
|
||
The CHaracterizing ExOPlanets Satellite (CHEOPS) is a 30 cm telescope in orbit | ||
around the Earth, which seeks to measure properties of exoplanets using | ||
photometry, or brightness measurements of the planets and their host stars. The | ||
photometry collected with CHEOPS arrives on users machines in the form of FITS | ||
files which contain photometry that inevitably contains trends as a function of | ||
several variables; for example, the photometry is often covariant with the | ||
stellar centroid position on the detector, the roll angle of the spacecraft, | ||
the flux of contaminants within the aperture, the background and the | ||
dark current. | ||
|
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We present ``linea``, a linear detrending toolkit for CHEOPS photometry. | ||
``linea`` features an efficient ``numpy`` implementation of linear least-squares | ||
regression [@Numpy:2011] which can be used to quickly remove trends from CHEOPS | ||
photometry. The core principle of ``linea`` is that the vector of observed | ||
fluxes observed by CHEOPS can be represented by a linear combination of some | ||
observational vectors, like the roll angle and stellar centroid position. | ||
|
||
The ``linea`` API has handy classes and methods for reading in the output files | ||
produced by the CHEOPS Data Reduction Pipeline (DRP), assembling a design matrix | ||
of the housekeeping vectors, regressing the design matrix against the observed | ||
fluxes, and visualizing the results. We built-in two realistic, simulated | ||
example light curves and tutorials on how to detrend them including the phase | ||
curve of 55 Cnc e and four eclipses of WASP-189 b. | ||
|
||
The mathematical formalism of the ``linea`` algorithms are detailed in the | ||
software's documentation. The ``linea`` package is built on the ``astropy`` | ||
package template [@Astropy:2018]. ``linea`` is open source and contributions are | ||
welcome. | ||
|
||
# References | ||
|
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