609 citations · 7.9k across the 96 of their papers we have counts for
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Inferring the mass of sub-millimetre galaxies by exploiting their gravitational magnification of background galaxies
H. Hildebrandt, L. van Waerbeke, D. Scott +25
Dust emission at sub-millimetre wavelengths allows us to trace the early phases of star formation in the Universe. In order to understand the physical processes involved in this mo…
The SCUBA-2 Cosmology Legacy Survey: blank-field number counts of 450um-selected galaxies and their contribution to the cosmic infrared background
J. E. Geach, E. L. Chapin, K. E. K. Coppin +50
The first deep blank-field 450um map (1-sigma~1.3mJy) from the SCUBA-2 Cosmology Legacy Survey (S2CLS), conducted with the James Clerk Maxwell Telescope (JCMT) is presented. Our ma…
The complex physics of dusty star-forming galaxies at high redshifts as revealed by Herschel and Spitzer
B. Lo Faro, A. Franceschini, M. Vaccari +29
We combine far-infrared photometry from Herschel (PEP/HERMES) with deep mid-infrared spectroscopy from Spitzer to investigate the nature and the mass assembly history of a sample o…
HerMES: Unveiling obscured star formation - the far infrared luminosity function of ultraviolet-selected galaxies at z~1.5
S. Heinis, V. Buat, M. Béthermin +22
We study the far-infrared (IR) and sub-millimeter properties of a sample of ultraviolet (UV) selected galaxies at z\sim1.5. Using stacking at 250, 350 and 500 um from Herschel Spac…
A Redshift Survey of Herschel Far-Infrared Selected Starbursts and Implications for Obscured Star Formation
C. M. Casey, S. Berta, M. Béthermin +30
We present Keck spectroscopic observations and redshifts for a sample of 767 Herschel-SPIRE selected galaxies (HSGs) at 250, 350, and 500um, taken with the Keck I Low Resolution Im…
Herschel-ATLAS: the far-infrared properties and star-formation rates of broad absorption line quasi-stellar objects
J. M. Cao Orjales, J. A. Stevens, M. J. Jarvis +20
We have used data from the Herschel-ATLAS at 250, 350 and 500 μm to determine the far-infrared (FIR) properties of 50 Broad Absorption Line Quasars (BAL QSOs). Our sample contains…