Z
Zachary I. Edwards
Researcher at Columbus State University
Publications - 8
Citations - 11825
Zachary I. Edwards is an academic researcher from Columbus State University. The author has contributed to research in topics: Stars & Large Magellanic Cloud. The author has an hindex of 7, co-authored 8 publications receiving 7314 citations. Previous affiliations of Zachary I. Edwards include Louisiana State University.
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Journal ArticleDOI
Astropy: A community Python package for astronomy
Thomas P. Robitaille,Erik Tollerud,Perry Greenfield,Michael Droettboom,Erik Bray,Tom Aldcroft,Matt Davis,Adam Ginsburg,Adrian M. Price-Whelan,Wolfgang Kerzendorf,A. Conley,Neil H. M. Crighton,Kyle Barbary,Demitri Muna,Henry C. Ferguson,Frédéric Grollier,Madhura Parikh,Prasanth H. Nair,Hans Moritz Günther,Christoph Deil,Julien Woillez,Simon Conseil,Roban Kramer,J. Turner,Leo Singer,R. T. Fox,Benjamin A. Weaver,Victor Zabalza,Zachary I. Edwards,K. Azalee Bostroem,Douglas Burke,Andrew R. Casey,Steven M. Crawford,Nadia Dencheva,Justin Ely,Tim Jenness,Kathleen Labrie,Pey Lian Lim,Francesco Pierfederici,Andrew Pontzen,Andy Ptak,Brian L. Refsdal,Mathieu Servillat,Ole Streicher +43 more
TL;DR: Astropy as discussed by the authors is a Python package for astronomy-related functionality, including support for domain-specific file formats such as flexible image transport system (FITS) files, Virtual Observatory (VO) tables, common ASCII table formats, unit and physical quantity conversions, physical constants specific to astronomy, celestial coordinate and time transformations, world coordinate system (WCS) support, generalized containers for representing gridded as well as tabular data, and a framework for cosmological transformations and conversions.
Journal ArticleDOI
Astropy: A Community Python Package for Astronomy
Thomas P. Robitaille,Erik Tollerud,Perry Greenfield,Michael Droettboom,Erik Bray,Tom Aldcroft,Matt Davis,Adam Ginsburg,Adrian M. Price-Whelan,Wolfgang Kerzendorf,A. Conley,Neil H. M. Crighton,Kyle Barbary,Demitri Muna,Henry C. Ferguson,Frédéric Grollier,Madhura Parikh,Prasanth H. Nair,Hans Moritz Günther,Christoph Deil,Julien Woillez,Simon Conseil,Roban Kramer,J. Turner,Leo Singer,R. T. Fox,Benjamin A. Weaver,Victor Zabalza,Zachary I. Edwards,K. Azalee Bostroem,Douglas Burke,Andrew R. Casey,Steven M. Crawford,Nadia Dencheva,Justin Ely,Tim Jenness,Kathleen Labrie,Pey Lian Lim,Francesco Pierfederici,Andrew Pontzen,Andy Ptak,Brian L. Refsdal,Mathieu Servillat,Ole Streicher +43 more
TL;DR: Astropy as mentioned in this paper provides core astronomy-related functionality to the community, including support for domain-specific file formats such as Flexible Image Transport System (FITS) files, Virtual Observatory (VO) tables, and common ASCII table formats, unit and physical quantity conversions, physical constants specific to astronomy, celestial coordinate and time transformations, world coordinate system (WCS) support, generalized containers for representing gridded as well as tabular data, and a framework for cosmological transformations and conversions.
Journal ArticleDOI
THE PROGENITOR OF THE TYPE Ia SUPERNOVA THAT CREATED SNR 0519-69.0 IN THE LARGE MAGELLANIC CLOUD
TL;DR: In this paper, the results of a search for an ex-companion star in SNR 0519-69.0, located in the Large Magellanic Cloud, based on images taken with the Hubble Space Telescope with a limiting magnitude of V = 26.05.
Journal ArticleDOI
DEM L241, a Supernova Remnant containing a High-Mass X-ray Binary
F. D. Seward,P. A. Charles,P. A. Charles,Deatrick Foster,John R. Dickel,P. S. Romero,Zachary I. Edwards,M. R. Perry,R. M. Williams +8 more
TL;DR: In this paper, Chandra observations of the Large Magellanic Cloud supernova remnant DEM L241 reveal an interior unresolved source which is probably an accretion-powered binary with an orbital period of tens of days.
Journal ArticleDOI
DEM L241, a Supernova Remnant containing a High-Mass X-ray Binary
F. D. Seward,P. A. Charles,P. A. Charles,Deatrick Foster,John R. Dickel,P. S. Romero,Zachary I. Edwards,M. R. Perry,R. M. Williams +8 more
TL;DR: In this article, Chandra observations of the Large Magellanic Cloud supernova remnant DEM L241 reveal an interior unresolved source which is probably an accretion-powered binary, making this a High-Mass X-ray Binary (HMXB) with orbital period likely to be of order tens of days.