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J/MNRAS/392/1539 Metal absorption systems in pairs of QSOs (Tytler+, 2009)
Metal absorption systems in spectra of pairs of QSOs: how absorbers cluster around QSOs and other absorbers. Tytler D., Gleed M., Melis C., Chapman A., Kirkman D., Lubin D., Paschos P., Jena T., Crotts A.P.S. <Mon. Not. R. Astron. Soc., 392, 1539-1572 (2009)> =2009MNRAS.392.1539T
ADC_Keywords: QSOs ; Redshifts Keywords: intergalactic medium - quasars: absorption lines - quasars: general - cosmology: observations Abstract: We present the first large sample of metal absorption systems in pairs of QSOs with sightlines separated by about 1Mpc at z=2. We found 690 absorption systems in the spectra of 310 QSOs in 170 pairings. Most systems show CIV or MgII absorption. Description: We use spectra of the 310 QSOs which include 140 pairs and 10 triplets. We use spectra that we obtained with LRIS on the Keck I telescope, the Kast spectrograph on the Lick 3-m Shane telescope and from CTIO and KPNO. We also use spectra from the SDSS data release 5 (DR5). We obtained spectra with LRIS from 2001 to 2004 September. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 43 310 QSO targets, in order of QSO pair label number, not RA. table4.dat 115 996 The 690 metal-line absorption systems in the spectra of the 310 QSOs
See also: J/AJ/126/2579 : SDSS quasar catalog. II. First data release (Schneider+, 2003) http://www.sdss.org : SDSS Home Page Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh Right ascension (J2000) 4- 5 I2 min RAm Right ascension (J2000) 7- 11 F5.2 s RAs Right ascension (J2000) 13 A1 --- DE- Declination sign (J2000) 14- 15 I2 deg DEd Declination (J2000) 17- 18 I2 arcmin DEm Declination (J2000) 20- 24 F5.2 arcsec DEs Declination (J2000) 26- 30 F5.3 --- zem Emission redshift 32 A1 --- --- [P] 33- 35 I3 --- Pair [1,155] QSO pair number 36 A1 --- m_Pair [abc] Multiplicity index for pairs/triplets 38- 43 F6.2 arcsec Sep Separation between pairs
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1 A1 --- --- [P] 2- 4 I3 --- Pair [1,155] QSO pair number 5 A1 --- m_Pair [abc] Multiplicity index for pairs/triplets 7- 13 F7.5 --- z Redshift (1) 15- 78 A64 --- Ions Ions or zem (2) 80-101 A22 --- Notes Notes and system classifications (3) 104-108 F5.2 0.1nm Wrest ? Rest frame equivalent width for one of the stronger doublet lines (1548, 2796 or 1238) in order of preference 109 A1 --- f_Wrest [?] ? Wrest value for CIV 1550 or NV 1242 111-115 F5.2 0.1nm Wpm ? Wpm is the minimum Wrest that we could have seen for the same line in the spectrum of the partner QSO at the same z
Note (1): We give 5 decimal places for the redshifts of the coincident absorption systems, and 4 decimals for most other absorbers. Note (2): # indicates significantly blended absorption line. Note (3): Abbreviations used: EA = emission-absorption coincident absorbers are close to the emission redshift of the partner QSO, with -0.005<DzEA<0.005 EAV = coincident absorbers (V for velocity) are like EA coincidences but with have vEA<1000km/s and |DzEA|>0.005 AA = absorption-absorption) coincident systems have a partner in the paired QSO with -0.005<DzAA<0.005 AAV = coincident systems (V for velocity) have vAA<1000km/s but |DvAA|>0.005 AAA = associated absorber-absorber coincident systems have |vAA|<1000km/s and one or both absorbers at vabs<3000km/s from their QSO
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 24-Aug-2009
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