Tuning the hot WD LF

Details Tuning the hot WD LF Tuning the hot WD LF

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273...41k&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 41-43 (2010).

Statistics

Applications

White Dwarfs, Monte Carlo Methods, Brightness, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Applications Of Monte Carlo Methods, Luminosity And Mass Functions

Scientific paper

The recently presented [8] hot white dwarf (WD) luminosity function (LF) has been recalculated using a Monte Carlo method to obtain more realistic error estimates. New analysis of the SDSS hot standard WD completeness dependence on the SDSS g filter brightness and galactic latitude is shown and the results compared with a previously determined map of the hot standard completeness. A joined hot+cold LF is also presented as is the result of separation of the DA and non-DA LFs within -0.5 to 10 absolute bolometric magnitude range.

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