activity
20072013
most citedThe Herschel Space Observatory view of dust in M81

165 citations · 563 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2013★ 5 cited

Chronos: A NIR spectroscopic galaxy survey. From the formation of galaxies to the peak of activity

I. Ferreras, R. Sharples, J. S. Dunlop +30

Chronos is our response to ESA's call for white papers to define the science for the future L2, L3 missions. Chronos targets the formation and evolution of galaxies, by collecting…

astro-ph.CO2012★ 86 cited

The rise and fall of the star formation histories of blue galaxies at redshifts 0.2<z<1.4

Camilla Pacifici, Susan A. Kassin, Benjamin Weiner +2

Popular cosmological scenarios predict that galaxies form hierarchically from the merger of many progenitors, each with their own unique star formation history (SFH). We use a soph…

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.GA2010★ 34 cited

Herschel photometric observations of the low metallicity dwarf galaxy NGC 1705

B. O'Halloran, M. Galametz, S. C. Madden +57

We present Herschel SPIRE and PACS photometeric observations of the low metallicity (Z ~ 0.35 solar) nearby dwarf galaxy, NGC 1705, in six wavelength bands as part of the Dwarf Gal…

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…