Search catalogue
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
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), except as noted. Note (2): Flag on Lambda, defined as follows: c = SiIV wavelength from Morton (1991ApJS...77..119M). Morton (2003ApJS..149..205M) prefers SiIV wavelengths of 1393.760 and 1402.773Å. d = CIV wavelength from Morton (1991ApJS...77..119M). Morton (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
| 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 |
© UDS/CNRS