activity
19992026
most citedWarm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data

815 citations · 9.1k across the 104 of their papers we have counts for

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Showing 2011 · astro-ph.COShow all

5 papers · 2 filters

astro-ph.CO2011★ 78 cited

Iron and alpha-element Production in the First One Billion Years after the Big Bang

George D. Becker, Wallace L. W. Sargent, Michael Rauch +1

We present measurements of carbon, oxygen, silicon, and iron in quasar absorption systems existing when the universe was roughly one billion years old. We measure column densities…

astro-ph.CO2011★ 122 cited

Improved measurements of the intergalactic medium temperature around quasars: possible evidence for the initial stages of He-II reionisation at z~6

James S. Bolton, George D. Becker, Sudhir Raskutti +3

We present measurements of the intergalactic medium (IGM) temperature within ~5 proper Mpc of seven luminous quasars at z~6. The constraints are obtained from the Doppler widths of…

astro-ph.CO2011★ 70 cited

Filamentary Infall of Cold Gas and Escape of Lyman Alpha and Hydrogen Ionizing Radiation from an Interacting High-Redshift Galaxy

Michael Rauch, George D. Becker, Martin G. Haehnelt +3

We present observations of a peculiar Lyman alpha-emitting galaxy at redshift 3.344, discovered in a deep, blind spectroscopic survey for faint Lyman alpha emitters with the Magell…

astro-ph.CO2011★ 69 cited

The Physical Conditions of a Lensed Star-forming Galaxy at z=1.7

J. R. Rigby, E. Wuyts, M. D. Gladders +2

We report rest-frame optical Keck/NIRSPEC spectroscopy of the bright lensed galaxy RCSGA 032727-132609 at z=1.7037. From precise measurements of the nebular lines, we infer a numbe…

astro-ph.CO2011★ 83 cited

High-Redshift Metals. II. Probing Reionization Galaxies with Low-Ionization Absorption Lines at Redshift Six

George D. Becker, Wallace L. W. Sargent, Michael Rauch +1

We present a survey for low-ionization metal absorption line systems towards 17 QSOs at redshifts z_em=5.8-6.4. Nine of our objects were observed at high resolution with either Kec…