activity
20032016
most citedThe Herschel Space Observatory view of dust in M81

165 citations · 517 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2016★ 102 cited

Witnessing the birth of the red sequence: ALMA high-resolution imaging of [CII] and dust in two interacting ultra-red starbursts at z = 4.425

I. Oteo, R. J. Ivison, L. Dunne +19

Exploiting the sensitivity and spatial resolution of the Atacama Large Millimeter/submillimeter Array (ALMA), we have studied the morphology and the physical scale of the interstel…

astro-ph.CO2014★ 31 cited

Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing

J. González-Nuevo, A. Lapi, M. Negrello +25

We report a highly significant () spatial correlation between galaxies with mJy detected in the equatorial fields of the \textsl{Herschel} Astrophysica…

astro-ph.CO2012★ 63 cited

Herschel-ATLAS/GAMA: a difference between star-formation rates in strong-line and weak-line radio galaxies

M. J. Hardcastle, J. H. Y. Ching, J. S. Virdee +25

We have constructed a sample of radio-loud objects with optical spectroscopy from the Galaxy and Mass Assembly (GAMA) project over the Herschel-ATLAS Phase 1 fields. Classifying th…

astro-ph.CO2010★ 33 cited

Herschel-SPIRE observations of the disturbed galaxy NGC4438

L. Cortese, G. J. Bendo, A. Boselli +56

We present Herschel-SPIRE observations of the perturbed galaxy NGC4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the gala…

astro-ph.CO2010★ 37 cited

Mapping the interstellar medium in galaxies with Herschel/SPIRE

S. A. Eales, M. W. L. Smith, C. D. Wilson +57

The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with…

astro-ph.CO2010★ 165 cited

The Herschel Space Observatory view of dust in M81

G. J. Bendo, C. D. Wilson, M. Pohlen +57

We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 microns in the nearby spiral gala…