activity
20032023
most citedDust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

1.1k citations · 15.3k across the 193 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.COShow all

6 papers · 2 filters

astro-ph.CO2012★ 101 cited

Radio Continuum Surveys with Square Kilometre Array Pathfinders

Ray P. Norris, J. Afonso, D. Bacon +48

In the lead-up to the Square Kilometre Array (SKA) project, several next-generation radio telescopes and upgrades are already being built around the world. These include APERTIF (T…

astro-ph.CO2012★ 195 cited

GOODS-Herschel:dust attenuation properties of UV selected high redshift galaxies

V. Buat, S. Noll, D. Burgarella +9

We study dust attenuation at UV wavelengths at high redshift, where the UV is redshifted to the observed visible. In particular, we search for a UV bump and related implications fo…

astro-ph.CO2012★ 10 cited

Cool Dust in the Outer Ring of NGC 1291

J. L. Hinz, C. W. Engelbracht, R. Skibba +18

We examine Herschel Space Observatory images of one nearby prototypical outer ring galaxy, NGC 1291, and show that the ring becomes more prominent at wavelengths longer than 160um.…

astro-ph.CO2012★ 88 cited

Submillimeter Observations of Millimeter Bright Galaxies Discovered by the South Pole Telescope

T. R. Greve, J. D. Vieira, A. Weiss +65

We present APEX SABOCA 350micron and LABOCA 870micron observations of 11 representative examples of the rare, extremely bright (S_1.4mm > 15mJy), dust-dominated millimeter-selected…

astro-ph.CO2012★ 203 cited

Estimating the Star Formation Rate at 1 kpc Scales in Nearby Galaxies

Adam K. Leroy, Frank Bigiel, W. J. G. de Blok +9

Using combinations of Hα, ultraviolet (UV), and infrared (IR) emission, we estimate the star formation rate (SFR) surface density, Σ_SFR, at 1 kpc resolution for 30 disk galaxies t…

astro-ph.CO2012★ 104 cited

Resolving the Far-IR Line Deficit: Photoelectric Heating and Far-IR Line Cooling in NGC 1097 and NGC 4559

Kevin V. Croxall, J. D. Smith, M. G. Wolfire +30

The physical state of interstellar gas and dust is dependent on the processes which heat and cool this medium. To probe heating and cooling of the ISM over a large range of infrare…