activity
19962023
most citedUnveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field

1.3k citations · 19.2k across the 239 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.COShow all

24 papers · 2 filters

astro-ph.CO2013★ 285 cited

The evolution of the dust and gas content in galaxies

P. Santini, R. Maiolino, B. Magnelli +36

We use deep Herschel PACS and SPIRE observations in GOODSS, GOODSN and COSMOS to estimate the average dust mass (Mdust) of galaxies on a redshift-stellar mass (Mstar)-SFR grid. We…

astro-ph.CO2013★ 264 cited

The evolution of the dust temperatures of galaxies in the SFR plane up to

B. Magnelli, D. Lutz, A. Saintonge +38

[Abridged] We study the evolution of the dust temperatures of galaxies in the SFR-M* plane up to z~2 using observations from the Herschel Space Observatory. Starting from a sample…

astro-ph.CO2013★ 117 cited

HerMES: Candidate High-Redshift Galaxies Discovered with Herschel/SPIRE

C. Darren Dowell, A. Conley, J. Glenn +63

We present a method for selecting dusty, star forming galaxies (DSFGs) using Herschel/SPIRE 250/350/500 flux densities to search for red sources. We apply this method to…

astro-ph.CO2013★ 208 cited

The suppression of star formation by powerful active galactic nuclei

M. J. Page, M. Symeonidis, J. D. Vieira +75

The old, red stars which constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at…

astro-ph.CO2013★ 216 cited

Gravitational Lens Models Based on Submillimeter Array Imaging of Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z>1.5

R. S. Bussmann, I. Perez-Fournon, S. Amber +46

Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub)millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution im…

astro-ph.CO2013★ 129 cited

HerMES: dust attenuation and star formation activity in UV-selected samples from z~4 to z~1.5

S. Heinis, V. Buat, M. Bethermin +16

We study the link between observed ultraviolet luminosity, stellar mass, and dust attenuation within rest-frame UV-selected samples at z~ 4, 3, and 1.5. We measure by stacking at 2…