activity
20102025
most citedCIGALE: a python Code Investigating GALaxy Emission

1.3k citations · 8k across the 106 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

21 papers · 1 filter

astro-ph.CO2014★ 9 cited

The bivariate K-band-submillimetre luminosity functions of the local HRS galaxy sample

P. Andreani, L. Spinoglio, A. Boselli +6

We study the relationship between the K-band and the sub-millimetre (submm) emissions of nearby galaxies by computing the bivariate K-band-submm luminosity function (BLF) of the He…

astro-ph.CO2013★ 12 cited

Cold dust but warm gas in the unusual elliptical galaxy NGC 4125

C. D. Wilson, A. Cridland, K. Foyle +19

Data from the Herschel Space Observatory have revealed an unusual elliptical galaxy, NGC 4125, which has strong and extended submillimeter emission from cold dust but only very str…

astro-ph.CO2013★ 20 cited

The Herschel Virgo Cluster Survey XIV: transition-type dwarf galaxies in the Virgo cluster

Ilse De Looze, Maarten Baes, Alessandro Boselli +19

We use dust scaling relations to investigate the hypothesis that Virgo cluster transition-type dwarfs are infalling star-forming field galaxies, which is argued based on their opti…

astro-ph.CO2013★ 41 cited

Towards understanding the relation between the gas and the attenuation in galaxies at kpc scales

M. Boquien, A. Boselli, V. Buat +13

[abridged] Aims. The aim of the present paper is to provide new and more detailed relations at the kpc scale between the gas surface density and the face-on optical depth directly…

astro-ph.CO2012★ 29 cited

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…

astro-ph.CO2012★ 90 cited

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 $…

astro-ph.CO2012★ 83 cited

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…

astro-ph.CO2012★ 98 cited

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…

astro-ph.CO2012★ 127 cited

Submillimetre Photometry of 323 Nearby Galaxies from the Herschel Reference Survey

L. Ciesla, A. Boselli, M. W. L. Smith +23

The Herschel Reference Survey (HRS) is a guaranteed time Herschel key project aimed at studying the physical properties of the interstellar medium in galaxies of the nearby univers…

astro-ph.CO2012★ 213 cited

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…

astro-ph.CO2012★ 98 cited

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…

astro-ph.CO2012★ 140 cited

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…

astro-ph.CO2012★ 95 cited

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…

astro-ph.CO2011★ 198 cited

The Herschel Reference Survey: Dust in Early-Type Galaxies and Across the Hubble Sequence

M. W. L. Smith, H. L. Gomez, S. A. Eales +24

We present Herschel observations of 62 Early-Type Galaxies (ETGs), including 39 galaxies morphologically classified as S0+S0a and 23 galaxies classified as ellipticals using SPIRE…

astro-ph.CO2011★ 82 cited

The Herschel Virgo Cluster Survey - VIII. The Bright Galaxy Sample

J. I. Davies, S. Bianchi, L. Cortese +20

We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data that cover the complete survey area (four 4 x 4 deg2 regions). We use these data to measure and compare th…

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★ 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★ 28 cited

Herschel deep far-infrared counts through the Abell 2218 cluster-lens

B. Altieri, S. Berta, D. Lutz +35

Gravitational lensing by massive galaxy clusters allows study of the population of intrinsically faint infrared galaxies that lie below the sensitivity and confusion limits of curr…

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.CO2010★ 55 cited

The dust morphology of the elliptical Galaxy M86 with SPIRE

H. L. Gomez, M. Baes, L. Cortese +58

We present Herschel-SPIRE observations at 250-500um of the giant elliptical galaxy M86 and examine the distribution of the resolved cold dust emission and its relation with other g…

astro-ph.CO2010★ 90 cited

SPIRE imaging of M82: cool dust in the wind and tidal streams

H. Roussel, C. D. Wilson, L. Vigroux +57

M82 is a unique representative of a whole class of galaxies, starbursts with superwinds, in the Very Nearby Galaxy Survey with Herschel. In addition, its interaction with the M81 g…