249 citations · 984 across the 11 of their papers we have counts for
11 papers
Hidden depths in the local Universe: The Stellar Stream Legacy Survey
David Martinez-Delgado, Andrew P. Cooper, Javier Roman +26
Mergers and tidal interactions between massive galaxies and their dwarf satellites are a fundamental prediction of the Lambda-Cold Dark Matter cosmology. These events are thought t…
Comparison of star formation rates from Halpha and infrared luminosities as seen by Herschel
H. Domínguez, M. Mignoli, F. Pozzi +55
We empirically test the relation between the SFR(LIR) derived from the infrared luminosity, LIR, and the SFR(Ha) derived from the Ha emission line luminosity using simple conversio…
The effect of environment on star forming galaxies at redshift 1 - First insight from PACS
P. Popesso, G. Rodighiero, A. Saintonge +4
We use deep 70, 100 and 160 um observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS Evolutionary Probe (PEP) guar…
Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel
H. S. Hwang, D. Elbaz, G. E. Magdis +112
We study the dust properties of galaxies in the redshift range 0.1<z<2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-Nort…
Herschel FIR counterparts of selected Ly-alpha emitters at z~2.2. Fast evolution since z~3 or missed obscured AGNs?
A. Bongiovanni, I. Oteo, J. Cepa +58
Ly-alpha emitters (LAEs) are seen everywhere in the redshift domain from local to z~7. Far-infrared (FIR) counterparts of LAEs at different epochs could provide direct clues on dus…
A First Glimpse into the far-IR properties of high-z UV-selected Galaxies: Herschel/PACS observations of z~3 LBGs
G. E. Magdis, D. Elbaz, H. S. Hwang +33
We present first insights into the far-IR properties for a sample of IRAC and MIPS-24um detected Lyman Break Galaxies (LBGs) at z ~ 3, as derived from observations in the northern…
Unveiling Far-Infrared Counterparts of Bright Submillimeter Galaxies Using PACS Imaging
H. Dannerbauer, E. Daddi, G. E. Morrison +35
We present a search for Herschel-PACS counterparts of dust-obscured, high-redshift objects previously selected at submillimeter and millimeter wavelengths in the Great Observatorie…
Herschel deep far-infrared counts through the Abell 2218 cluster-lens
B. Altieri, S. Berta, D. Lutz +35
Gravitational lensing by massive galaxy clusters allows study of the population of intrinsically faint infrared galaxies that lie below the sensitivity and confusion limits of curr…
Herschel unveils a puzzling uniformity of distant dusty galaxies
D. Elbaz, H. S. Hwang, B. Magnelli +106
The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their…
Herschel PEP: The star-formation rates of 1.5<z<2.5 massive galaxies
R. Nordon, D. Lutz, L. Shao +31
The star formation rate (SFR) is a key parameter in the study of galaxy evolution. The accuracy of SFR measurements at z~2 has been questioned following a disagreement between obse…
The far-infrared/radio correlation as probed by Herschel
R. J. Ivison, B. Magnelli, E. Ibar +100
We set out to determine the ratio, q(IR), of rest-frame 8-1000um flux, S(IR), to monochromatic radio flux, S(1.4GHz), for galaxies selected at far-IR and radio wavelengths, to sear…