Cool White Dwarfs Selection with Pan-STARRS Proper Motions

M. C. Lam, N. C. Hambly

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The use of Reduced Proper Motion in identifying isolated white dwarfs has long been used as a proxy for the absolute magnitude in a population with known kinematics. This, however, introduces a proper motion detection limit on top of the existing photometric limit. How the survey volume is hampered by this extra parameter is discussed in Hambly et al (2012). In this work, we discuss some robust outlier rejection methods in order to minimise the proper motion limit and hence maximise the survey volume. The generalised volume, corrected for the distance of the Sun from the Galactic Plane, is integrated explicitly.
Original languageEnglish
Title of host publication19th European Workshop on White Dwarfs
EditorsPatrick Dufour, Pierre Bergeron, Gilles Fontaine
PublisherAstronomical Society of the Paific
Pages347
Volume493
Publication statusPublished - 1 Jun 2015
Event19th European Workshop on White Dwarfs - Université de Montréal, Montréal, Canada
Duration: 11 Aug 201415 Aug 2014

Publication series

NameASP Conference Series

Conference

Conference19th European Workshop on White Dwarfs
CountryCanada
CityMontréal
Period11/08/1415/08/14

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