The incidence of cool gas in ~ 1e13 Msun halos

Abstract

We present the first results of an ongoing spectroscopic follow-up of close luminous red galaxy (LRGs) and MgII λλ 2796,2803 absorber pairs for an initial sample of 15 photometrically selected LRGs at physical projected separations ρ \le 350 kpc/h from a QSO sightline. Our moderate-resolution spectra confirm a physical association between the cool gas (T ~ 1e4 K) revealed by the presence of MgII absorption features and the LRG halo in five cases. In addition, we report an empirical estimate of the maximum covering fraction (κ_max) of cool gas in massive, \ge 1e13 Msun/h dark matter halos hosting LRGs at z ~ 0.5. This study is performed using a sample of foreground LRGs that are located at ρ < 400 kpc/h from a QSO sightline. The LRGs are selected to have a robust photometric redshift σ_z/(1+z_ph) \approx 0.03. We determine κ_max based on the incidence of MgII absorption systems that occur within z_ph +/- 3sigma_z in the spectra of the background QSOs. Despite the large uncertainties in z_ph, this experiment provides a conservative upper limit to the covering fraction of cool gas in the halos of LRGs. We find that κ_max \approx 0.07 at W_r(2796) \ge 1.0 A and κ_max \approx 0.18 at W_r(2796) \ge 0.5 A, averaged over 400 kpc/h radius. Our study shows that while cool gas is present in \ge 1e13 Msun/h halos, the mean covering fraction of strong absorbers is no more than 7%.

Accepted for publication in the Astrophysical Journal. 8 pages, 3 figures.

References in corpus (12)

• The Sloan Digital Sky Survey Quasar Catalog IV. Fifth Data Release
• An Empirical Characterization of Extended Cool Gas Around Galaxies Using MgII Absorption Features
• Clustering of Low-Redshift (z <= 2.2) Quasars from the Sloan Digital Sky Survey
• Seeding the formation of cold gaseous clouds in Milky Way size halos
• Halo Gas Cross Sections And Covering Fractions of MgII Absorption Selected Galaxies
• New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equivalent width anti-correlated?
• What determines satellite galaxy disruption?
• MegaZ-LRG: A photometric redshift catalogue of one million SDSS Luminous Red Galaxies
• The Baryon Content of Dark Matter Halos: Empirical Constraints from MgII Absorbers
• The Clustering of MgII Absorption Systems at z=0.5 and Detection of Cold Gas in Massive Halos
• On the Halo Occupation of Dark Baryons
• On the Redshift Evolution of MgII Absorption Systems

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