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Astrophysics Source Code Library

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Searching for codes credited to 'Barclay, Thomas'

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[ascl:1601.009] K2fov: Field of view software for NASA's K2 mission
Mullally, Fergal; Barclay, Thomas; Barentsen, Geert

K2fov allows users to transform celestial coordinates into K2's pixel coordinate system for the purpose of preparing target proposals and field of view visualizations. In particular, the package, written in Python, adds the "K2onSilicon" and "K2findCampaigns" tools to the command line, allowing the visibility of targets to be checked in a user-friendly way.

[ascl:1903.012] DAVE: Discovery And Vetting of K2 Exoplanets
Mullally, Fergal; Coughlin, Jeffrey; Mullally, Susan; Barclay, Thomas; Barentsen, Geert; Burke, Christopher J.; Colón, Knicole D.; Quintana, Elisa V.

DAVE implements a pipeline to find and vet planets planets using data from NASA's K2 mission. The pipeline contains several modules tailored to particular aspects of the vetting procedures, using photocenter analysis to rule out background eclipsing binaries and flux time-series analysis to rule out odd–even differences, secondary eclipses, low-S/N events, variability other than a transit, and size of the transiting object.

[ascl:1807.028] ktransit: Exoplanet transit modeling tool in python
Barclay, Thomas

The routines in ktransit create and fit a transiting planet model. The underlying model is a Fortran implementation of the Mandel & Agol (2002) limb darkened transit model. The code calculates a full orbital model and eccentricity can be allowed to vary; radial velocity data can also be calculated via the model and included in the fit.

[ascl:1812.013] Lightkurve: Kepler and TESS time series analysis in Python
Lightkurve Collaboration; Cardoso, José Vinícius de Miranda; Hedges, Christina; Gully-Santiago, Michael; Saunders, Nicholas; Cody, Ann Marie; Barclay, Thomas; Hall, Oliver; Sagear, Sheila; Turtelboom, Emma; Zhang, Johnny; Tzanidakis, Andy; Mighell, Ken; Coughlin, Jeff; Bell, Keaton; Berta-Thompson, Zach; Williams, Peter; Dotson, Jessie; Barentsen, Geert

Lightkurve analyzes astronomical flux time series data, in particular the pixels and light curves obtained by NASA’s Kepler, K2, and TESS exoplanet missions. This community-developed Python package is designed to be user friendly to lower the barrier for students, astronomers, and citizen scientists interested in analyzing data from these missions. Lightkurve provides easy tools to download, inspect, and analyze time series data and its documentation is supported by a large syllabus of tutorials.

[ascl:2003.001] TESS-Point: High precision TESS pointing tool
Burke, Christopher J.; Levine, Alan; Fausnaugh, Michael; Vanderspek, Roland; Barclay, Thomas; Libby-Roberts, Jessica E.; Morris, Brett; Sipocz, Brigitta; Owens, Martin; Feinstein, Adina D.; Camacho, Joao

TESS-Point converts astronomical target coordinates given in right ascension and declination to detector pixel coordinates for the MIT-led NASA Transiting Exoplanet Survey Satellite (TESS) spacecraft. The program can also provide detector pixel coordinates for a star by TESS input catalog identifier number and common astronomical name. Tess-Point outputs the observing sector number, camera number, detector number, and pixel column and row.