activity
20062024
most citedThe Herschel-SPIRE instrument and its in-flight performance

2.2k citations · 4k across the 12 of their papers we have counts for

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Showing 2010Show all

10 papers · 1 filter

astro-ph.IM2010★ 2.2k cited

The Herschel-SPIRE instrument and its in-flight performance

M. J. Griffin, A. Abergel, A. Abreu +176

The Spectral and Photometric Imaging Receiver (SPIRE), is the Herschel Space Observatory`s submillimetre camera and spectrometer. It contains a three-band imaging photometer operat…

astro-ph.GA2010★ 60 cited

The Herschel view of star formation in the Rosette molecular cloud under the influence of NGC 2244

N. Schneider, F. Motte, S. Bontemps +43

The Rosette molecular cloud is promoted as the archetype of a triggered star-formation site. This is mainly due to its morphology, because the central OB cluster NGC 2244 has blown…

astro-ph.GA2010★ 41 cited

Small-scale structure in the Rosette molecular cloud revealed by Herschel

J. Di Francesco, S. Sadavoy, F. Motte +40

We present a preliminary analysis of the small-scale structure found in new 70-520 micron continuum maps of the Rosette molecular cloud (RMC), obtained with the SPIRE and PACS inst…

astro-ph.GA2010★ 47 cited

Herschel observations of embedded protostellar clusters in the Rosette Molecular Cloud

M. Hennemann, F. Motte, S. Bontemps +39

The Herschel OB young stellar objects survey (HOBYS) has observed the Rosette molecular cloud, providing an unprecedented view of its star formation activity. These new far-infrare…

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…