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20052026
most citedPHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxies

948 citations · 15.9k across the 176 of their papers we have counts for

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astro-ph.CO2011★ 136 cited

The GALEX Arecibo SDSS Survey V: The Relation between the HI Content of Galaxies and Metal Enrichment at their Outskirts

Sean M. Moran, Timothy M. Heckman, Guinevere Kauffmann +14

We have obtained long-slit spectra of 174 star-forming galaxies with stellar masses greater than 10^10 M_\odot from the GALEX Arecibo SDSS (GASS) survey. These galaxies have both H…

astro-ph.CO2011★ 3 cited

Multi-Wavelength Properties of Barred Galaxies in the Local Universe: Environment and evolution across the Hubble sequence

Lea Giordano, Kim-Vy H. Tran, Ben Moore +1

We investigate possible environmental and morphological trends in the bar fraction using two carefully selected samples representative of a low-density environment (the is…

astro-ph.CO2011★ 4 cited

Detection of Outflowing and Extraplanar Gas in Disks in an Assembling Galaxy Cluster at z=0.37

E. Freeland, K-V. Tran, T. Irwin +5

We detect ionized gas characteristics indicative of winds in three disk-dominated galaxies that are members of a super-group at z=0.37 that will merge to form a Coma-mass cluster.…

astro-ph.CO2011★ 63 cited

The GALEX Arecibo SDSS Survey. IV. Baryonic Mass-Velocity-Size Relations of Massive Galaxies

Barbara Catinella, Guinevere Kauffmann, David Schiminovich +12

We present dynamical scaling relations for a homogeneous and representative sample of ~500 massive galaxies, selected only by stellar mass (>10^10 Msun) and redshift (0.025<z<0.05)…

astro-ph.CO2011★ 5 cited

Caught in the Act: The Assembly of Massive Cluster Galaxies at z=1.62

J. M. Lotz, C. Papovich, S. M. Faber +13

We present the recent merger history of massive galaxies in a spectroscopically-confirmed proto-cluster at z=1.62. Using HST WFC3 near-infrared imaging from the Cosmic Assembly Nea…

astro-ph.CO2011★ 66 cited

The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel

P. Popesso, A. Biviano, G. Rodighiero +40

Star formation in massive galaxies is quenched at some point during hierarchical mass assembly. To understand where and when the quenching processes takes place, we study the evolu…