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J/MNRAS/382/1377 SDSS WD main-sequence binaries (Rebassa-Mansergas+, 2007)
Post-common-envelope binaries from SDSS. I. 101 white dwarf main-sequence binaries with multiple Sloan Digital Sky Survey spectroscopy. Rebassa-Mansergas A., Gansicke B.T., Rodriguez-Gil P., Schreiber M.R., Koester D. <Mon. Not. R. Astron. Soc., 382, 1377-1393 (2007)> =2007MNRAS.382.1377R
ADC_Keywords: Stars, double and multiple ; Stars, dwarfs ; Stars, white dwarf Keywords: accretion, accretion discs - binaries: close - novae, cataclysmic variables Abstract: We present a detailed analysis of 101 white dwarf main-sequence binaries (WDMS) from the Sloan Digital Sky Survey (SDSS) for which multiple SDSS spectra are available. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 62 261 WD-MS in our sample that did not show a significant RV variation between their different SDSS spectra (123 stars) table3.dat 105 258 WD masses, effective temperatures, surface gravities, spectral types and distances (112 stars)
See also: J/AJ/129/2428 : M dwarf-white dwarf binary systems (Silvestri+, 2005) J/ApJS/167/40 : SDSS4 confirmed white dwarfs catalog (Eisenstein+, 2006) II/282 : SDSS Photometric Catalog, Release 6 (Adelman-McCarthy+, 2007) http://www.sdss.org/ : SDSS Home Page Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 4 A4 --- --- [SDSS] 5- 23 A19 --- SDSS SDSS designation (JHHMMSS.ss+DDMMSS.s) of WD 25- 36 F12.4 d HJD Heliocentric Julian Date of the spectrum 38 A1 --- f_SDSS [y/n] composed spectrum (1) 40- 45 F6.1 km/s RV(Na) ? NaI (8183.27,8194.81) absorption double radial velocity 47- 50 F4.1 km/s e_RV(Na) ? rms uncertainty on RV(Na) 52- 57 F6.1 km/s RV(Ha) ? Hα emission radial velocity 59- 62 F4.1 km/s e_RV(Ha) ? rms uncertainty on RV(Ha)
Note (1): yes (y) or no (n) those spectra which are composed of subspectra taken in different nights
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 4 A4 --- --- [SDSS] 5- 23 A19 --- SDSS SDSS designation (JHHMMSS.ss+DDMMSS.s) 25- 29 I5 --- MJD SDSS MJD value 31- 34 I4 --- Plate SDSS Plate value 36- 39 I4 --- Fiber SDSS Fiber value 41- 45 I5 K Teff ?=- Wide dwarf effective temperature 47- 51 I5 K e_Teff ?=- rms uncertainty on Teff 53- 56 F4.2 --- logg ?=- Wide dwarf surface gravity 58- 61 F4.2 --- e_logg ?=- rms uncertainty on logg 63- 66 F4.2 solMass Mass ?=- Wide dwarf mass 68- 71 F4.2 solMass e_Mass ?=- rms uncertainty on Mass 73- 76 I4 pc Dist ?=- Distance to the wide dwarf 78- 81 I4 pc e_Dist ?=- rms uncertainty on Dist 83- 84 A2 --- Sp2 ?=- MK spectral type of the secondary star 86- 89 I4 pc Dist2 ?=- Distance to the secondary star 91- 93 I3 pc e_Dist2 ?=- rms uncertainty on Distsec 95-101 A7 --- n_SDSS System already studied or resolved (1) 103-105 A3 --- Notes Individual Notes (2)
Note (1): Flags as follows: e = systems which have been studied previously by Eisenstein et al (2006, Cat. J/ApJS/167/40) s = systems which have been studied previously by Silvestri et al. (2006, Cat. J/AJ/131/1674) re = systems whose binary components are resolved in their SDSS images Note (2): Notes as follows: 1 = Probably K secondary star 2 = Some blue excess, WD? 3 = Teff less than 6000k 4 = DC white dwarf 5 = magnetic WD? No clear evidence for secondary star 6 = Chance superposition of an M and a G stars. No WD 7 = Blue star close to a very bright red star in the SDSS image. Bad background/scattered light subtraction? 8 = Diffuse Halpha emission in the sky area (Eridanus shell), no clear evidence for secondary star 9 = DO white dwarf 10 = Extended emission 11 = Blue flux differ by a factor two between the spectra 12 = Blue flux differ by a factor five. Eclipsing? Calibration problems? 13 = Something wrong in the SDSS image on cas.sdss.org: too many apparently blue objects that have faint u magnitudes 14 = Resolved binary, fit depends on the fiber placement 15 = Single WD 16 = At least one broken spectrum
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 02-Feb-2009
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