J/ApJ/743/138   Spectroscopic survey of bright white dwarfs   (Gianninas+, 2011)

A spectroscopic survey and analysis of bright, hydrogen-rich white dwarfs. Gianninas A., Bergeron P., Ruiz M.T. <Astrophys. J., 743, 138 (2011)> =2011ApJ...743..138G 2011ApJ...743..138G
ADC_Keywords: Stars, white dwarf ; Spectral types ; Effective temperatures ; Surveys ; Spectroscopy Keywords: binaries: spectroscopic - stars: fundamental parameters - surveys - techniques: spectroscopic - white dwarfs Abstract: We have conducted a spectroscopic survey of over 1300 bright (V≤17.5), hydrogen-rich white dwarfs based largely on the last published version of the McCook & Sion (1999ApJS..121....1M 1999ApJS..121....1M, Cat. III/235) catalog. The complete results from our survey, including the spectroscopic analysis of over 1100 DA white dwarfs, are presented. High signal-to-noise ratio optical spectra were obtained for each star and were subsequently analyzed using our standard spectroscopic technique where the observed Balmer line profiles are compared to synthetic spectra computed from the latest generation of model atmospheres appropriate for these stars. First, we present the spectroscopic content of our sample, which includes many misclassifications as well as several DAB, DAZ, and magnetic white dwarfs. Next, we look at how the new Stark broadening profiles affect the determination of the atmospheric parameters. When necessary, specific models and analysis techniques are used to derive the most accurate atmospheric parameters possible. In particular, we employ M dwarf templates to obtain better estimates of the atmospheric parameters for those white dwarfs that are in DA+dM binary systems. Description: The goal of our survey was to observe all the white dwarfs listed as DA in McCook & Sion (1999ApJS..121....1M 1999ApJS..121....1M, Cat. III/235), including all subtypes (DAB, DAH/P, DAO, DAZ, DA+dM), with a visual magnitude V≤17.5. After nearly 8 years of observing, and a total of 19 observing runs in both the northern and southern hemispheres, we succeeded in securing spectra for 1360 of the 1503 white dwarfs we had selected. 726 spectra were obtained specifically for the purposes of this survey since it began in 2003. Of those 726 spectra, 568 were obtained between 2003 September and 2011 April at Steward Observatory's 2.3m telescope equipped with the Boller & Chivens spectrograph (spectral coverage from about 3000 to 5250Å at a resolution of ∼6Å (FWHM)). An additional 18 spectra were obtained in 2006 April and 2007 January at the 1.6m telescope of the Observatoire du Mont-Megantic. Furthermore, a total of 140 spectra from the southern hemisphere were secured during the course of two observing runs in 2007 March and 2007 October, respectively, at ESO's 3.6m telescope and at Carnegie Observatories' 2.5m Irenee du Pont Telescope. There are also 169 spectra that were kindly provided by C. Moran (1999, private comm.). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 46 68 Misclassified objects table3.dat 50 13 Parameters for magnetic white dwarfs table4.dat 51 10 Parameters for cool white dwarfs table5.dat 80 1265 Atmospheric parameters of DA white dwarfs from McCook & Sion (1999ApJS..121....1M 1999ApJS..121....1M, Cat. III/235) refs.dat 69 32 References -------------------------------------------------------------------------------- See also: III/235 : Spectroscopically Identified White Dwarfs (McCook+, 2008) III/137 : Spectroscopically Identified Hot Subdwarf Stars (Kilkenny+ 1988) II/207 : Palomar-Green catalog UV-excess stellar objects (Green+ 1986) J/ApJS/204/5 : SDSS DR7 white dwarf catalog (Kleinman+, 2013) J/ApJ/730/128 : Spectroscopy of DA WD from the SDSS-DR4 (Tremblay+, 2011) J/ApJS/197/38 : The WIRED survey. II. (Debes+, 2011) J/ApJ/712/585 : Apparent velocity measurements of DA WDs (Falcon+, 2010) J/ApJ/714/1037 : White dwarfs from the Kiso survey (Limoges+, 2010) J/ApJ/723/1072 : The ELM survey. I. Low-mass white dwarfs (Brown+, 2010) J/ApJS/190/77 : Detailed analysis of cool WDs in the SDSS (Kilic+, 2010) J/A+A/496/191 : Spectral analysis of 636 SDSS WD-M binaries (Heller+, 2009) J/A+A/505/441 : UVES/VLT spectra of white dwarfs (Koester+, 2009) J/AJ/135/1239 : Spectral distances to DA white dwarfs (Holberg+, 2008) J/ApJ/654/499 : H-rich white dwarfs spectropolarimetric survey (Kawka+, 2007) J/A+A/466/627 : Parameters of DA white dwarfs in SDSS-DR1 (Hu+, 2007) J/ApJS/167/40 : SDSS4 confirmed white dwarfs catalog (Eisenstein+, 2006) J/A+A/448/579 : Sample of confirmed WDs in GSC-II survey (Carollo+, 2006) J/ApJ/643/402 : Cool white dwarfs in the solar neighborhood (Kawka+, 2006) J/ApJ/631/1100 : Atmospheric parameters of DA white dwarfs (Gianninas+, 2005) J/ApJS/161/394 : Low-luminosity companions to white dwarfs (Farihi+, 2005) J/A+A/430/223 : Parameters of cool companions of sdB stars (Lisker+, 2005) J/ApJS/156/47 : DA white dwarfs from the Palomar Green Survey (Liebert+, 2005) J/AJ/130/734 : Magnetic WDs from SDSS DR2 and DR3 (Vanlandingham+, 2005) J/ApJ/607/426 : Catalog of white dwarfs in SDSS-DR1 (Kleinman+, 2004) J/ApJS/147/145 : IUE low-dispersion spectra of white dwarfs (Holberg+, 2003) J/ApJS/133/413 : BVRIJHK photometry of cool white dwarfs (Bergeron+, 2001) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WD Object name (HHMM+DDM.N) 12- 30 A19 --- OName Other designation 32- 36 A5 --- OSpT McCook & Sion (1999ApJS..121....1M 1999ApJS..121....1M, Cat. III/235) spectral type 38- 43 A6 --- SpT New spectral type from this work 45- 46 I2 --- Ref Reference (see refs.dat file) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- WD Object name (HHMM+DDM) 10- 23 A14 --- OName Other name 25- 30 F6.1 hT Bp Magnetic field strength (assuming a magnetic dipole), in MGauss (106Gauss) = 100Teslas 32- 36 I5 K Teff Effective temperature 38- 41 F4.2 [cm/s2] logg ? Log of the surface gravity 43- 50 A8 --- Ref Reference(s) to the original analyses (see refs.dat file) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- WD Object name (HHMM+DDMA) 11- 13 A3 --- f_WD DAZ indication for WD 1729+371 15- 23 A9 --- OName Other name 25- 29 I5 K Teff Effective temperature 31- 34 F4.2 [cm/s2] logg ? Log of the surface gravity 36- 39 F4.2 Msun Mass ? Mass of the white dwarf 41- 45 F5.2 mag VMag ? Absolute visual magnitude 47- 51 A5 --- Ref Reference(s) (see refs.dat file) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- WD Coordinate based identifier (HHMM+DDM.N) 12- 26 A15 --- OName Other name 28- 33 A6 --- SpT Spectral type 35- 40 I6 K Teff Effective temperature 42- 45 I4 K e_Teff Uncertainty in Teff 47- 50 F4.2 [cm/s2] logg Log of the surface gravity 52- 55 F4.2 [cm/s2] e_logg Uncertainty in logg 57- 60 F4.2 Msun Mass Mass of the white dwarf 62- 65 F4.2 Msun e_Mass Uncertainty in Mass 67- 71 F5.2 mag VMag Absolute V band magnitude 73- 76 I4 pc Dist Distance 78- 80 A3 --- Notes Notes (1) -------------------------------------------------------------------------------- Note (1): Notes numbered as follows: 1 = Photometrically constant; 2 = DA+dM binary; 3 = ZZ Ceti; 4 = Balmer-line problem; 5 = based on non-magnetic models; 6 = DA+DC binary; 7 = DA+DB binary; 8 = Suffers from interstellar reddening. -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ref Reference code 4- 22 A19 --- BibCode Bibcode 24- 49 A26 --- Aut Author's name(s) 51- 69 A19 --- Comm Comment -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 07-May-2013
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