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A catalog of 159,238 white dwarf ages

Published online by Cambridge University Press:  09 October 2020

Ted von Hippel
Affiliation:
Embry-Riddle Aeronautical University, Daytona Beach, FL, USA
Adam Moss
Affiliation:
University of Oklahoma, Norman, OK, USA
Isabelle Kloc
Affiliation:
Embry-Riddle Aeronautical University, Daytona Beach, FL, USA
Natalie Moticska
Affiliation:
Embry-Riddle Aeronautical University, Daytona Beach, FL, USA
Jimmy Sargent
Affiliation:
Embry-Riddle Aeronautical University, Daytona Beach, FL, USA
Elliot Robinson
Affiliation:
Embry-Riddle Aeronautical University, Daytona Beach, FL, USA
David Stenning
Affiliation:
Imperial College, London, UK
David van Dyk
Affiliation:
Imperial College, London, UK
Elizabeth Jeffery
Affiliation:
California Polytechnic State University, San Luis Obispo, CA, USA
Morgan Fouesneau
Affiliation:
Max Planck Institute for Astronomy, Heidelberg, Germany
Coryn Bailer-Jones
Affiliation:
Max Planck Institute for Astronomy, Heidelberg, Germany
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Abstract

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We employ Pan-STARRS photometry, Gaia trigonometric parallaxes, modern stellar evolution and atmosphere models, and our Bayesian fitting approach to determine cooling and total ages for 159,238 white dwarfs. In many cases we are able to derive precise ages (better than 5%) for individual white dwarfs. These results are meant for broad use within the white dwarf and stellar astrophysics communities and we plan to make available on-line the posterior distributions for cooling age, total age, initial stellar mass, and other parameters.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

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