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J/ApJ/640/579      Near-infrared spectra of 27 SDSS quasars     (Glikman+, 2006)

A near-infrared spectral template for quasars. Glikman E., Helfand D.J., White R.L. <Astrophys. J., 640, 579-591 (2006)> =2006ApJ...640..579G
ADC_Keywords: QSOs ; Spectra, infrared Keywords: quasars: emission lines - quasars: general Abstract: We present a near-infrared quasar composite spectrum spanning the wavelength range 0.58-3.5um. The spectrum has been constructed from observations of 27 quasars obtained at the NASA IRTF telescope and satisfying the criteria Ks<14.5 and Mi←23; the redshift range is 0.118<z<0.418. The signal-to-noise ratio is moderate, reaching a maximum of 150 between 1.6 and 1.9um. While a power-law fit to the continuum of the composite spectrum requires two breaks, a single power-law slope of alpha=-0.92 plus a 1260K blackbody provides an excellent description of the spectrum from Hα to 3.5um, strongly suggesting the presence of significant quantities of hot dust in this blue-selected quasar sample. We measure intensities and line widths for 10 lines, finding that the Paschen line ratios rule out case B recombination. We compute K-corrections for the J, H, K, and Spitzer 3.6um bands, which will be useful in analyzing observations of quasars up to z=10. Description: We obtained near-infrared spectra for 27 of the quasars. All spectra but one were obtained at the NASA Infrared Telescope Facility (IRTF), a 3.0m telescope optimized for infrared observations on the summit of Mauna Kea, Hawaii. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file list.dat 74 27 List of studied QSOs table3.dat 31 7740 Composite quasar spectrum, arithmetic and geometric means table7.dat 31 10944 Optical-to-infrared composite quasar spectrum, arithmetic and geometric means table8.dat 31 100 Quasar K-corrections sp/* 33 27 Individual spectra
See also: VII/252 : SDSS-DR5 quasar catalog (Schneider+, 2007) http://www.sdss.org : SDSS Home Page Byte-by-byte Description of file: list.dat
Bytes Format Units Label Explanations
1- 4 A4 --- --- [SDSS] 6- 24 A19 --- SDSS SDSS name (JHHMMSS.ss+DDMMSS.s) 26- 27 I2 h RAh Right ascension (J2000) 29- 30 I2 min RAm Right ascension (J2000) 32- 36 F5.2 s RAs Right ascension (J2000) 38 A1 --- DE- Declination sign (J2000) 39- 40 I2 deg DEd Declination (J2000) 42- 43 I2 arcmin DEm Declination (J2000) 45- 48 F4.1 arcsec DEs Declination (J2000) 52- 74 A23 --- FileName Name of the spectra file in sp subdirectory
Byte-by-byte Description of file: table[37].dat
Bytes Format Units Label Explanations
1- 7 F7.1 0.1nm Lambda Wavelength in Angstroms 9- 15 F7.4 --- Flux Arithmetic mean flux in arbitrary units 17- 23 F7.4 --- e_Flux Error in Flux 25- 31 F7.4 --- GFlux Geometric mean flux in arbitrary units
Byte-by-byte Description of file: table8.dat
Bytes Format Units Label Explanations
1- 4 F4.1 --- z Redshift 6- 10 F5.3 mag Kc(J) ? 2MASS J band K-correction 12- 17 F6.3 mag Kc(H) ? 2MASS H band K-correction 19- 24 F6.3 mag Kc(K) ? 2MASS KS band K-correction 26- 31 F6.3 mag Kc(3.6) Spitzer IRAC 3.6 micron band K-correction
Byte-by-byte Description of file: sp/*
Bytes Format Units Label Explanations
1- 8 F8.6 um Lambda Wavelength 10- 21 E12.5 --- Flux Flux in arbitrary units 23- 33 E11.5 --- e_Flux Error in Flux in arbitrary units
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 26-Sep-2008
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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