Showing 1–20 of 101 results
/ Date/ Name
Oct 14, 2008LCDM predictions for galaxy protoclusters I: the relation between galaxies, protoclusters and quasars at z~6Nov 28, 2010Dust Attenuation in UV-selected Starbursts at High Redshift and their Local Counterparts: Implications for the Cosmic Star Formation Rate DensityJul 20, 2015The Systematic Properties of the Warm Phase of Starburst-Driven Galactic WindsMar 12, 2019Tracing the formation history of galaxy clusters into the epoch of reionizationDec 17, 2013Discovery of a large number of candidate proto-clusters traced by ~15 Mpc-scale galaxy overdensities in COSMOSOct 10, 2013Ancient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-ClustersJul 30, 2024The Fourth S-PLUS Data Release: 12-filter photometry covering $\sim3000$ square degrees in the southern hemisphereNov 9, 2021Conditions for direct black hole seed collapse near a radio-loud quasar 1 Gyr after the Big BangSep 12, 2005Clustering of Star-forming Galaxies Near a Radio Galaxy at z=5.2May 17, 2018The Fraction of Active Galactic Nuclei in the USS 1558-003 Protocluster at z = 2.53May 14, 2015Surveying Galaxy Proto-clusters in Emission: A Large-scale Structure at z=2.44 and the Outlook for HETDEXJul 9, 2014Discovery of an Overdensity of Lyman-alpha Emitters Around a $\mathrm{z}\sim4$ QSO with the Large Binocular TelescopeOct 13, 2014A Local Clue to the Reionization of the UniverseOct 30, 2006Witnessing the formation of a brightest cluster galaxy at z>2Jan 10, 2006Lyman break galaxies, Lya emitters and a radio galaxy in a protocluster at z=4.1Jul 17, 2006Clustering of i-dropout galaxies at z=6 in GOODS and the UDFMay 3, 2017Galaxy Protoclusters as Drivers of Cosmic Star-Formation History in the First 2 GyrSep 20, 2007HST morphologies of local Lyman break galaxy analogs I: Evidence for starbursts triggered by mergingMay 4, 2012Quantifying the role of bars in the build-up of central mass concentrations in disk galaxiesSep 15, 2011Confronting theoretical models with the observed evolution of the galaxy population out to z=4