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Related papers: A Deep Proper Motion Catalog Within the Sloan Digi…

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We present 5,080 white dwarf (WD) candidates selected from stars matching between the multi-band imaging datasets of the Subaru Hyper Suprime-Cam (HSC) Survey and the Sloan Digital Sky Survey (SDSS) in the Stripe82 region covering about…

Astrophysics of Galaxies · Physics 2024-12-16 Tian Qiu , Masahiro Takada , Naoki Yasuda , Akira Tokiwa , Kazumi Kashiyama , Yoshihisa Suzuki , Kenta Hotokezaka

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…

We present a magnitude and proper motion limited catalogue of ~10,000 white dwarf candidates, obtained from the SuperCOSMOS Sky Survey by means of reduced proper motion selection. This catalogue extends to magnitudes r~19.75 and proper…

Astrophysics of Galaxies · Physics 2011-04-21 Nicholas Rowell , Nigel Hambly

We present the techniques and early results of our program to measure the luminosity function for White Dwarfs in the SuperCOSMOS Sky Survey. Our survey covers over three quarters of the sky to a mean depth of I~19.2, and finds ~9,500…

Solar and Stellar Astrophysics · Physics 2009-07-22 N. R. Rowell , N. C. Hambly , P. Bergeron

The SDSS Data Release 1 includes 1833 DA white dwarfs (WDs) and forms the largest homogeneous sample of WDs. This sample provides the best opportunity to study the statistical properties of WDs. We adopt a recently established theoretical…

Astrophysics · Physics 2009-11-13 Qi Hu , Chaolun Wu , Xue-Bing Wu

Using data from the Sloan Digital Sky Survey Early Data Release and SuperCOSMOS Sky Survey scans of POSS-I plates we identify a sample of 2600 subdwarfs using reduced proper motion methods and strict selection criteria. This forms one of…

Astrophysics · Physics 2008-11-26 Andrew P. Digby , Nigel C. Hambly , John A. Cooke , I. Neill Reid , Russell D. Cannon

We present the first phase in our ongoing work to use Sloan Digital Sky Survey (SDSS) data to create separate white dwarf (WD) luminosity functions for two or more different mass ranges. In this paper, we determine the completeness of the…

A large sample of white dwarfs is selected by both proper motion and colours from the Pan-STARRS 1 3{\pi} Steradian Survey Processing Version 2 to construct the White Dwarf Luminosity Functions of the discs and halo in the solar…

An initial assessment is made of white dwarf and hot subdwarf stars observed in the Sloan Digital Sky Survey. In a small area of sky (190 square degrees), observed much like the full survey will be, 269 white dwarfs and 56 hot subdwarfs are…

We present optical spectroscopy and near-infrared photometry of 126 cool white dwarfs in the Sloan Digital Sky Survey (SDSS). Our sample includes high proper motion targets selected using the SDSS and USNO-B astrometry and a dozen…

We have performed a search for halo white dwarfs as high proper motion objects in a second epoch WFPC2 image of the Groth-Westphal strip. We identify 24 high proper motion objects with mu > 0.014 ''/yr. Five of these high proper motion…

Astrophysics · Physics 2009-11-07 Cailin A. Nelson , Kem H. Cook , Tim S. Axelrod , Jeremy R. Mould , Charles Alcock

Although it a very narrow angle survey, the depth of the HDF results in its sampling a significant volume of the halo of our galaxy. Thus it is useful for the purposes of detecting (or placing upper limits on the distribution of)…

Astrophysics · Physics 2007-05-23 Steven D. Kawaler

We describe a new multi-colour proper motion survey for cool white dwarfs (CWDs). The observational database consists of ~300 digitally scanned Schmidt plates in ESO/SERC field 287. The entire survey procedure, from the raw Schmidt plate…

Astrophysics · Physics 2009-10-31 R. A. Knox , M. R. S. Hawkins , N. C Hambly

The reduced proper motion diagram (RPMD) for a complete sample of faint stars with high accuracy proper motions in the North Galactic Pole field SA57 is investigated. Eight stars with very large reduced proper motions are identified as…

Astrophysics · Physics 2009-11-07 S. R. Majewski , M. H. Siegel

We present optical spectroscopy and near-infrared photometry of 57 faint ($g= 19-22$) high proper motion white dwarfs identified through repeat imaging of $\approx3100$ square degrees of the Sloan Digital Sky Survey footprint by Munn et al.…

Solar and Stellar Astrophysics · Physics 2016-09-07 Kyra Dame , A. Gianninas , Mukremin Kilic , Jeffrey A. Munn , Warren R. Brown , Kurtis A. Williams , Ted von Hippel , Hugh C. Harris

We present the mass distribution for all S/N > 15 pure DA white dwarfs detected in the Sloan Digital Sky Survey up to Data Release 12, fitted with Koester models for ML2/alpha=0.8, and with Teff > 10 000 K, and for DBs with S/N >10, fitted…

Solar and Stellar Astrophysics · Physics 2016-10-04 S. O. Kepler , Detlev Koester , Alejandra Daniela Romero , Gustavo Ourique , Ingrid Pelisoli

We use three different techniques to identify hundreds of white dwarf (WD) candidates in the Next Generation Virgo Cluster Survey (NGVS) based on photometry from the NGVS and GUViCS, and proper motions derived from the NGVS and the Sloan…

We present a catalog of over 6.2 million stars with measured proper motions. All these stars are observed in the direction of the Magellanic Clouds within the brightness range 12 < I < 19 mag. Based on these proper motions about 440 000…

Astrophysics of Galaxies · Physics 2012-04-26 R. Poleski , I. Soszyński , A. Udalski , M. K. Szymański , M. Kubiak , G. Pietrzyński , Ł. Wyrzykowski , K. Ulaczyk

Wide binaries made up of two white dwarfs (WDs) receive far less attention than their tight counterparts. However, our tests using the binary population synthesis code {\tt StarTrack} indicate that, for any set of reasonable initial…

Solar and Stellar Astrophysics · Physics 2015-06-11 Jeff J. Andrews , Marcel A. Agüeros , Krzysztof Belczynski , Saurav Dhital , S. J. Kleinman , Andrew A. West

We present a catalog of 531 white dwarf candidates that have large apparent transverse motions relative to the Sun ($v_{T} > 200$ km s$^{-1}$), thus making them likely members of the local Galactic halo population. The candidates were…

Solar and Stellar Astrophysics · Physics 2020-08-20 Bokyoung Kim , Sebastien Lépine , Ilija Medan
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