activity
20132023
most citedThe Herschel Dwarf Galaxy Survey: I. Properties of the low-metallicity ISM from PACS spectroscopy

234 citations · 1.8k across the 30 of their papers we have counts for

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Showing 2016 · astro-ph.GAShow all

9 papers · 2 filters

astro-ph.GA2016★ 168 cited

The Radio Spectral Energy Distribution and Star Formation Rate Calibration in Galaxies

F. S. Tabatabaei, E. Schinnerer, M. Krause +17

We study the spectral energy distribution (SED) of the radio continuum emission from the KINGFISH sample of nearby galaxies to understand the energetics and origin of this emission…

astro-ph.GA2016★ 112 cited

The Spatially Resolved [CII] Cooling Line Deficit in Galaxies

J. D. T. Smith, Kevin Croxall, Bruce Draine +17

We present [CII] 158um measurements from over 15,000 resolved regions within 54 nearby galaxies of the KINGFISH program to investigate the so-called [CII] "line cooling deficit" lo…

astro-ph.GA2016★ 138 cited

DustPedia - A Definitive Study of Cosmic Dust in the Local Universe

J. I. Davies, M. Baes, S. Bianchi +20

The European Space Agency has invested heavily in two cornerstones missions; Herschel and Planck. The legacy data from these missions provides us with an unprecedented opportunity…

astro-ph.GA2016

The dust content of galaxies from z = 0 to z = 9

Gergö Popping, Rachel S. Somerville, Maud Galametz

We study the dust content of galaxies from to in semi-analytic models of galaxy formation that include new recipes to track the production and destruction of dust. We i…

astro-ph.GA2016

Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. I. N159W

Min-Young Lee, Suzanne Madden, Vianney Lebouteiller +25

We present Herschel SPIRE Fourier Transform Spectrometer (FTS) observations of N159W, an active star-forming region in the Large Magellanic Cloud (LMC). In our observations, a numb…

astro-ph.GA2016

Gone with the heat: A fundamental constraint on the imaging of dust and molecular gas in the early Universe

Zhi-Yu Zhang, Padelis P. Papadopoulos, R. J. Ivison +3

Images of dust continuum and carbon monoxide (CO) line emission are powerful tools for deducing structural characteristics of galaxies, such as disk sizes, H gas velocity field…