The White Dwarf Luminosity Function from SDSS Imaging Data
| dc.creator | Harris, Hugh C. | |
| dc.creator | Munn, Jeffrey A. | |
| dc.creator | Kilic, Mukremin | |
| dc.creator | Liebert, James | |
| dc.creator | Williams, Kurtis A. | |
| dc.creator | von Hippel, Ted | |
| dc.creator | Levine, Stephen E. | |
| dc.creator | Monet, David G. | |
| dc.creator | Eisenstein, Daniel J. | |
| dc.creator | Kleinman, S. J. | |
| dc.creator | Metcalfe, T. S. | |
| dc.creator | Nitta, Atsuko | |
| dc.creator | Winget, D. E. | |
| dc.creator | Brinkmann, J. | |
| dc.creator | Fukugita, Masataka | |
| dc.creator | Knapp, G. R. | |
| dc.creator | Lupton, Robert H. | |
| dc.creator | Smith, J. Allyn | |
| dc.creator | Schneider, Donald P. | |
| dc.date | 2005-10-29 | |
| dc.date.accessioned | 2026-07-07T11:24:55Z | |
| dc.date.available | 2026-07-07T11:24:55Z | |
| dc.description | A sample of white dwarfs is selected from SDSS DR3 imaging data using their reduced proper motions, based on improved proper motions from SDSS plus USNO-B combined data. Numerous SDSS and followup spectra (Kilic et al. 2005) are used to quantify completeness and contamination of the sample; kinematic models are used to understand and correct for velocity-dependent selection biases. A luminosity function is constructed covering the range 7 < M_bol < 16, and its sensitivity to various assumptions and selection limits is discussed. The white dwarf luminosity function based on 6000 stars is remarkably smooth, and rises nearly monotonically to M_bol = 15.3. It then drops abruptly, although the small number of low-luminosity stars in the sample and their unknown atmospheric composition prevent quantitative conclusions about this decline. Stars are identified that may have high tangential velocities, and a preliminary luminosity function is constructed for them. | |
| dc.description | Accepted for AJ (Jan 2006). 35 pages (includes 10 figures) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0510820 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0510820 | |
| dc.identifier | Astron.J.131:571-581,2006 | |
| dc.identifier | doi:10.1086/497966 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/195352 | |
| dc.subject | Astrophysics | |
| dc.title | The White Dwarf Luminosity Function from SDSS Imaging Data | |
| dc.type | text |