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J/ApJ/669/791         Quasar black hole masses            (Wilhite+, 2007)

The effect of variability on the estimation of quasar black hole masses. Wilhite B.C., Brunner R.J., Schneider D.P., Vanden Berk D.E. <Astrophys. J., 669, 791-800 (2007)> =2007ApJ...669..791W
ADC_Keywords: Active gal. nuclei ; QSOs ; Spectroscopy ; Ultraviolet Keywords: galaxies: active - quasars: general - techniques: spectroscopic Abstract: We investigate the time-dependent variations of ultraviolet (UV) black hole mass estimates of quasars in the Sloan Digital Sky Survey (SDSS). From SDSS spectra of 615 high-redshift (1.69<z<4.75) quasars with spectra from two epochs, we estimate black hole masses using a single-epoch technique, which employs an additional, automated night-sky line removal and relies on UV continuum luminosity and CIV λ1549 emission-line dispersion. Mass estimates show variations between epochs at about the 30% level for the sample as a whole. We determine that for our full sample, measurement error in the line dispersion likely plays a larger role than the inherent variability in terms of contributing to variations in mass estimates between epochs. However, we use the variations in quasars with r-band spectral signal-to-noise ratio greater than 15 to estimate that the contribution to these variations from inherent variability is roughly 20%. We conclude that these differences in black hole mass estimates between epochs indicate that variability does not make a large contribution to the current factor of 2 scatter between mass estimates derived from low- and high-ionization emission lines. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 68 615 Variable quasar sample table2.dat 62 615 The 1450Å luminosity, CIV line dispersion, and estimated black hole mass at both epochs for all objects
See also: J/ApJ/613/682 : AGN central masses & broad-line region sizes (Peterson+, 2004) http://www.sdss.org : SDSS Home Page Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [WBS2007] Running quasar identification number 5- 22 A18 --- SDSS The SDSS identification (HHMMSS.ss+DDMMSS.s) 24- 28 I5 d MJDh Modified Julian Date of high-S/N ratio epoch 30- 34 I5 d MJDl Modified Julian Date of low-S/N ratio epoch 36- 40 F5.3 --- zh Redshift of high-S/N ratio epoch 42- 46 F5.3 --- e_zh Uncertainty in z-HSN 48- 52 F5.3 --- zl Redshift of low-S/N ratio epoch 54- 58 F5.3 --- e_zl Uncertainty in z-LSN 60- 63 F4.1 --- S/Nh Signal-to-Noise of high-S/N ratio epoch 65- 68 F4.1 --- S/Nl Signal-to-Noise of low-S/N ratio epoch
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [WBS2007] Running quasar identification number 5- 8 I4 10+37W Lh High-S/N ratio epoch 1450Å luminosity (1) 10- 12 I3 10+37W e_Lh Uncertainty in Lh (1) 14- 17 I4 10+37W Ll Low-S/N ratio epoch 1450Å luminosity (1) 19- 21 I3 10+37W e_Ll Uncertainty in Ll (1) 23- 26 I4 km/s sig.h High-S/N ratio epoch CIV 1550Å line dispersion 28- 31 I4 km/s e_sig.h Uncertainty in sig.h 33- 37 I5 km/s sig.l Low-S/N ratio epoch CIV 1550Å line dispersion 39- 42 I4 km/s e_sig.l Uncertainty in sig.l 44- 47 F4.2 [solMass] MBHh High-S/N ratio epoch log of Black hole mass 49- 52 F4.2 [solMass] e_MBHh Uncertainty in MBHh 54- 57 F4.2 [solMass] MBHl Low-S/N ratio epoch log of Black hole mass 59- 62 F4.2 [solMass] e_MBHl Uncertainty in MBHl
Note (1): In units of 10+44erg/s.
History: From electronic version of the journal References: Wandel et al., Paper I 1999ApJ...526..579W Peterson et al., Paper II 2004ApJ...613..682P, Cat. J/ApJ/613/682
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 27-Jan-2010
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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