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19972026
most citedWhat Powers Ultra-luminous IRAS Galaxies?

1.2k citations · 48.4k across the 319 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★ 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…

astro-ph.CO2011★ 175 cited

Herschel/PACS spectroscopy of NGC 4418 and Arp 220: H2O, H2^{18}O, OH, ^{18}OH, O I, HCN and NH3

E. González-Alfonso, J. Fischer, J. Graciá-Carpio +14

Herschel/PACS spectroscopy of the luminous infrared galaxies NGC4418 and Arp220 reveals high excitation in H2O, OH, HCN, and NH3. In NGC4418, absorption lines were detected with E_…

astro-ph.CO2011★ 63 cited

Enriched haloes at redshift with no star-formation: Implications for accretion and wind scenarios

N. Bouche, M. T. Murphy, C. Peroux +9

[Abridged] In order to understand which process (e.g. galactic winds, cold accretion) is responsible for the cool (T~10^4 K) halo gas around galaxies, we embarked on a program to s…

astro-ph.CO2011★ 13 cited

FIR measurements of Ly- emitters at z1.0: dust attenuation from PACS-\emph{Herschel}

I. Oteo, A. Bongiovanni, A. M. Pérez García +24

One remaining open question regarding the physical properties of Ly emitters (LAEs) is their dust content and its evolution with redshift. The variety of results is large and wi…

astro-ph.CO2011★ 867 cited

The lesser role of starbursts for star formation at z=2

G. Rodighiero, E. Daddi, I. Baronchelli +31

Two main modes of star formation are know to control the growth of galaxies: a relatively steady one in disk-like galaxies, defining a tight star formation rate (SFR)-stellar mass…