661 citations · 3.6k across the 59 of their papers we have counts for
13 papers · 1 filter
The Herschel Virgo Cluster Survey XVI: a cluster inventory
J. I. Davies, S. Bianchi, M. Baes +12
Herschel FIR observations are used to construct Virgo cluster galaxy luminosity functions and to show that the cluster lacks the very bright and the numerous faint sources detected…
Integrated Spectroscopy of the Herschel Reference Survey. The spectral line properties of a volume-limited, K-band selected sample of nearby galaxies
A. Boselli, T. Hughes, L. Cortese +2
We present long-slit integrated spectroscopy of 238 late-type galaxies belonging to the Herschel Reference Survey, a volume limited sample representative of the nearby universe. Th…
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 role of cold gas and environment on the stellar mass - metallicity relation of nearby galaxies
T. M. Hughes, L. Cortese, A. Boselli +2
We investigate the relationship between stellar mass, metallicity and gas content for a magnitude- and volume-limited sample of 260 nearby late-type galaxies in different environme…
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…
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 Herschel Virgo Cluster Survey. IX. Dust-to-gas mass ratio and metallicity gradients in four Virgo spiral galaxies
Laura Magrini, Simone Bianchi, Edvige Corbelli +20
Using Herschel data from the Open Time Key Project the Herschel Virgo Cluster Survey (HeViCS), we investigated the relationship between the metallicity gradients expressed by metal…
The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). I: The UV luminosity function of the central 12 sq.deg
A. Boselli, S. Boissier, S. Heinis +50
The GALEX Ultraviolet Virgo Cluster Survey (GUViCS) is a complete blind survey of the Virgo cluster covering about 40 sq. deg. in the far UV (FUV, lambda_eff=1539A, Delta-lambda=44…
The far-infrared view of M87 as seen by the Herschel Space Observatory
M. Baes, M. Clemens, E. M. Xilouris +29
The origin of the far-infrared emission from the nearby radio galaxy M87 remains a matter of debate. Some studies find evidence of a far-infrared excess due to thermal dust emissio…
High mass star formation in normal late-type galaxies: observational constraints to the IMF
A. Boselli, S. Boissier, L. Cortese +3
We use Halpha and FUV GALEX data for a large sample of nearby objects to study the high mass star formation activity of normal late-type galaxies. The data are corrected for dust a…
Evolutionary paths to and from the red sequence: Star formation and HI properties of transition galaxies at z~0
L. Cortese, T. M. Hughes
(Abridged) We investigate the properties of galaxies between the blue and the red sequence (i.e., the transition region) by combining UV and NIR imaging to HI line observations for…
The migration of nearby spirals from the blue to red sequence: AGN feedback or environmental effects?
T. M. Hughes, L. Cortese
We combine ultraviolet to near-infrared photometry with HI 21cm line observations for a complete volume-limited sample of nearby galaxies in different environments (from isolated g…