J/ApJS/155/351      Absorption toward PG 1116+215               (Sembach+, 2004)

Physical properties and baryonic content of low-redshift intergalactic Lyα and O VI absorption line systems: the PG 1116+215 sight line. Sembach K.R., Tripp T.M., Savage B.D., Richter P. <Astrophys. J. Suppl. Ser., 155, 351-393 (2004)> =2004ApJS..155..351S 2004ApJS..155..351S
ADC_Keywords: QSOs ; Spectroscopy ; Spectra, ultraviolet Keywords: cosmology: observations - intergalactic medium - quasars: absorption lines - quasars: individual (PG 1116+215) Abstract: We present Hubble Space Telescope (HST) and Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the intergalactic absorption toward QSO PG 1116+215 in the 900-3000Å spectral region. Description: We observed PG 1116+215 with FUSE in 2000 April and 2001 April as part of the FUSE Team low-redshift OVI project. We observed PG 1116+215 with HST STIS in 2000 May and 2000 June as part of Guest Observer programs GO-8097 and GO-8165. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 11 19 08.7 +21 19 18 PG 1116+215 = QSO J1119+2119 ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 114 204 Interstellar line cross reference -------------------------------------------------------------------------------- See also: J/ApJ/508/200 : QSO low-z Lyα absorbers (Tripp+, 1998) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Ion Species name 15- 22 F8.3 0.1nm Lambda Wavelength in units of Angstroms (1) 24 A1 --- f_Lambda [cd] Flag on Lambda (2) 26- 31 F6.3 --- logfw Log of oscillator strength times the wavelength (1) 33- 38 A6 --- LineID Line identification number in Figures 2-4 39-112 A74 --- Comm Additional comments -------------------------------------------------------------------------------- Note (1): Wavelengths and f-values are from Morton (2003ApJS..149..205M 2003ApJS..149..205M), except as noted. Note (2): Flag on Lambda, defined as follows: c = SiIV wavelength from Morton (1991ApJS...77..119M 1991ApJS...77..119M). Morton (2003ApJS..149..205M 2003ApJS..149..205M) prefers SiIV wavelengths of 1393.760 and 1402.773Å. d = CIV wavelength from Morton (1991ApJS...77..119M 1991ApJS...77..119M). Morton (2003ApJS..149..205M 2003ApJS..149..205M) prefers CIV wavelengths of 1548.202 and 1550.781Å. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 11-Oct-2005
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