activity
20072026
most citedA Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34

609 citations · 3.4k across the 49 of their papers we have counts for

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Showing 2010Show all

9 papers · 1 filter

astro-ph.CO2010★ 29 cited

On the origin of M81 group extended dust emission

J. I. Davies, C. D. Wilson, R. Auld +57

Galactic cirrus emission at far-infrared wavelengths affects many extragalactic observations. Separating this emission from that associated with extragalactic objects is both impor…

astro-ph.CO2010★ 59 cited

HerMES: SPIRE Science Demonstration Phase Maps

L. Levenson, G. Marsden, M. Zemcov +30

We describe the production and verification of sky maps of the five SPIRE fields observed as part of the Herschel Multi-tiered Extragalactic Survey (HerMES) during the Science Demo…

astro-ph.CO2010★ 67 cited

Radial distribution of gas and dust in the two spiral galaxies M99 and M100

M. Pohlen, L. Cortese, M. W. L. Smith +55

By combining Herschel-SPIRE data with archival Spitzer, HI, and CO maps, we investigate the spatial distribution of gas and dust in the two famous grand-design spirals M99 and M100…

astro-ph.CO2010★ 9 cited

HerMES: The Submillimeter Spectral Energy Distributions of Herschel/SPIRE-Detected Galaxies

B. Schulz, C. P. Pearson, D. L. Clements +75

We present colours of sources detected with the Herschel/SPIRE instrument in deep extragalactic surveys of the Lockman Hole, Spitzer-FLS, and GOODS-N fields in three photometric ba…

astro-ph.CO2010★ 92 cited

Probing the molecular interstellar medium of M82 with Herschel-SPIRE spectroscopy

P. Panuzzo, N. Rangwala, A. Rykala +60

We present the observations of the starburst galaxy M82 taken with the Herschel SPIRE Fourier Transform Spectrometer. The spectrum (194-671 μm) shows a prominent CO rotational ladd…

astro-ph.GA2010★ 17 cited

The central region of spiral galaxies as seen by Herschel. M81, M99 and M100

M. Sauvage, N. Sacchi, G. J. Bendo +57

With appropriate spatial resolution, images of spiral galaxies in thermal infrared (~10 micron and beyond) often reveal a bright central component, distinct from the stellar bulge,…