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The Herschel Fornax Cluster Survey I: The Bright Galaxy Sample
J. I. Davies, S. Bianchi, M. Baes +18
We present Herschel observations of the Fornax cluster at 100, 160, 250, 350 and 500u with a spatial resolution of 7 - 36 arc sec (10" = 1 kpc at d_Fornax=17.9 Mpc). We define a sa…
The Herschel Virgo Cluster Survey XII: FIR properties of optically-selected Virgo Cluster galaxies
R. Auld, S. Bianchi, M. W. L. Smith +24
The Herschel Virgo Cluster Survey (HeViCS) is the deepest, confusion-limited survey of the Virgo Cluster at far-infrared (FIR) wavelengths. The entire survey at full depth covers $…
The dust energy balance in the edge-on spiral galaxy NGC 4565
Ilse De Looze, Maarten Baes, George J. Bendo +20
We combine new dust continuum observations of the edge-on spiral galaxy NGC 4565 in all Herschel/SPIRE (250, 350, 500 micron) wavebands, obtained as part of the Herschel Reference…
Spatially resolved stellar, dust and gas properties of the post-interacting Whirlpool Galaxy system
Erin Mentuch Cooper, Christine D. Wilson, Kelly Foyle +15
Using infrared imaging from the Herschel Space Observatory, observed as part of the VNGS, we investigate the spatially resolved dust properties of the interacting Whirlpool galaxy…
The Herschel Virgo Cluster Survey: X.The relationship between cold dust and molecular gas content in Virgo spirals
Edvige Corbelli, Simone Bianchi, Luca Cortese +16
Using the far-infrared emission, as observed by the Herschel Virgo Cluster Survey (HeViCS), and the integrated HI and CO brightness, we infer the dust and total gas mass for a magn…
Herschel and JCMT observations of the early-type dwarf galaxy NGC 205
I. De Looze, M. Baes, T. J. Parkin +18
We present Herschel dust continuum, James Clerk Maxwell Telescope CO(3-2) observations and a search for [CII] 158 micron and [OI] 63 micron spectral line emission for the brightest…
The gas-to-dust mass ratio of Centaurus A as seen by Herschel
T. J. Parkin, C. D. Wilson, K. Foyle +20
We present photometry of the nearby galaxy NGC 5128 (Centaurus A) observed with the PACS and SPIRE instruments on board the Herschel Space Observatory, at 70, 160, 250, 350 and 500…
The dust scaling relations of the Herschel Reference Survey
L. Cortese, L. Ciesla, A. Boselli +23
We combine new Herschel/SPIRE sub-millimeter observations with existing multiwavelength data to investigate the dust scaling relations of the Herschel Reference Survey, a magnitude…
Can dust emission be used to map the interstellar medium in high-redshift galaxies? Results from the Herschel Reference Survey
Stephen Eales, Matthew W. L. Smith, Robbie Auld +23
It has often been suggested that an alternative to the standard CO/21-cm method for estimating the mass of the interstellar medium (ISM) in a galaxy might be to estimate the mass o…
The IRX-beta relation on sub-galactic scales in star-forming galaxies of the Herschel Reference Survey
M. Boquien, V. Buat, A. Boselli +13
UV and optical surveys are essential to gain insight into the processes driving galaxy formation and evolution. The rest-frame UV emission is key to measure the cosmic SFR. However…
FIR colours of nearby late-type galaxies in the Herschel Reference Survey
A. Boselli, L. Ciesla, L. Cortese +21
We study the far infrared (60-500 m) colours of late-type galaxies in the Reference Survey, a K-band selected, volume limited sample of nearby galaxies. The far infra…
The Dust & Gas Properties of M83
K. Foyle, C. D. Wilson, E. Mentuch +17
We examine the dust and gas properties of the nearby, barred galaxy M83, which is part of the Very Nearby Galaxy Survey. Using images from the PACS and SPIRE instruments of Hersche…