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J/ApJ/727/47        The MgII cross-section of red galaxies        (Bowen+, 2011)

The Mg II cross-section of luminous red galaxies. Bowen D.V., Chelouche D. <Astrophys. J., 727, 47 (2011)> =2011ApJ...727...47B
ADC_Keywords: Galaxies, spectra ; Redshifts ; QSOs ; Equivalent widths Keywords: galaxies: clusters: general - galaxies: elliptical and lenticular, cD - galaxies: groups: general - galaxies: halos - quasars: absorption lines Abstract: We describe a search for MgII(2796, 2803) absorption lines in Sloan Digital Sky Survey (SDSS) spectra of QSOs whose lines of sight pass within impact parameters ρ∼200kpc of galaxies with photometric redshifts of z=0.46-0.6 and errors Δz∼0.05. The galaxies selected have the same colors and luminosities as the Luminous Red Galaxy (LRG) population previously selected from the SDSS. A search for MgII lines within a redshift interval of ±0.1 of a galaxy's photometric redshift shows that absorption by these galaxies is rare: the covering fraction is f(ρ)∼10%-15% between ρ=20kpc and ρ=100kpc, for MgII lines with rest equivalent widths of Wr≥0.6Å, falling to zero at larger ρ. There is no evidence that Wr correlates with impact parameter or galaxy luminosity. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 131 593 Mg II absorption in QSO-galaxy pairs
See also: VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010) II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009) J/ApJS/194/42 : SDSS-DR3 MgII-based black hole masses (Rafiee+, 2011) J/ApJ/724/L176 : MgII absorbing gas around galaxies (Chen+, 2010) J/ApJ/698/819 : MgII and LRGs cross-correlation analysis (Lundgren+, 2009) J/ApJ/679/239 : Associated MgII absorbers (Vanden+, 2008) J/ApJ/660/1093 : Weak MgII absorbers at 0.4<z<2.4 (Narayanan+, 2007) J/ApJ/639/766 : SDSS-DR3 strong MgII absorbers (Prochter+, 2006) J/MNRAS/371/495 : Catalogue of MgII absorbers from SDSS DR3 (Bouche+, 2006) J/MNRAS/354/L25 : MgII absorbers in SDSS QSOs (Bouche+, 2004) J/A+A/410/33 : MgII/FeII absorbers in 2dF-quasar survey (Menard+, 2003) J/AJ/106/848 : QSO MgII absorption line systems (Drinkwater+, 1993) http://www.sdss.org/ : SDSS home page Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 19 A19 --- QSO Background SDSS QSO name (JHHMMSS.ss+DDMMSS.s) (1) 21- 24 I4 --- Plate ? SDSS-DR6 Plate 25 A1 --- --- [-] 26- 30 I5 --- MJD ? SDSS-DR6 Modified Julian Date 31 A1 --- --- [-] 32- 34 I3 --- Fib ? SDSS-DR6 Fiber 36- 40 F5.3 --- zQSO [0.766/2.095]? QSO emission redshift 42- 60 A19 --- Gal Galaxy SDSS name (JHHMMSS.ss+DDMMSS.s) 62- 66 F5.3 --- zCC2 [0.459/0.6] Galaxy photometry redshift 68- 72 F5.3 --- e_zCC2 Uncertainty in zCC2 74- 77 F4.1 mag rmag Galaxy r band model magnitude de-reddened for Milky Way dust absorption 79- 83 F5.1 mag rMag SDSS absolute r band magnitude (2) 85- 88 F4.1 arcsec ASep [3.4/30] QSO-galaxy angular separation 90- 94 F5.1 kpc rho [20/197.1] QSO-galaxy impact parameter 96-101 F6.4 --- zabs [0.3779/0.6509]? Mg II absorption redshift (if doublet detected within ±0.1 of zCC2) 103-109 F7.4 --- Dz ? Difference Δz between zabs and zCC2 111 A1 --- l_W2796 The 2σ upper limit flag on W2796 112-115 F4.2 0.1nm W2796 Rest MgII (2796) equivalent width 117-120 F4.2 0.1nm e_W2796 ? Uncertainty in W2796 122 A1 --- l_W2803 The 2σ upper limit flag on W2803 123-126 F4.2 0.1nm W2803 Rest MgII (2803) equivalent width 128-131 F4.2 0.1nm e_W2803 ? Uncertainty in W2803
Note (1): Entries are listed in order of increasing QSO-galaxy impact parameter. In some cases, multiple galaxies satisfying our selection criteria were found around a single sightline. These are also listed, but are kept together with a single QSO entry, even though they may have much larger impact parameters. Note (2): Based on zCC2, after applying a K-correction to measure the r-band luminosity at a redshift z=0.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 23-Aug-2012
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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