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- Publications
- Influence
Evolution of asymptotic giant branch stars. II. Optical to far-infrared isochrones with improved TP-
- P. Marigo, L. Girardi, +14 authors Astronomical Observatory of Trieste
- Physics
- 30 November 2007
We present a large set of theoretical isochrones, whose distinctive features mostly reside on the greatly-improved treatment of the thermally-pulsing asymptotic giant branch (TP-AGB) phase.… Expand
AMAZE - I. The evolution of the mass–metallicity relation at z $>$ 3
- R. Maiolino, T. Nagao, +16 authors L. Silva
- Physics
- 15 June 2008
We present initial results of an ESO-VLT large programme (AMAZE) aimed at determining the evolution of the mass-metallicity relation at z > 3 by means of deep near-IR spectroscopy. Gas metallicities… Expand
Modeling the Effects of Dust on Galactic Spectral Energy Distributions from the Ultraviolet to the Millimeter Band
- L. Silva, G. L. Granato, A. Bressan, L. Danese
- Physics
- 10 December 1998
We present models of photometric evolution of galaxies in which the effects of a dusty interstellar medium have been included with particular care. A chemical evolution code follows the star… Expand
Can the faint submillimetre galaxies be explained in the Λ cold dark matter model
We present predictions for the abundance of submillimetre galaxies (SMGs) and Lyman-break galaxies (LBGs) in the Λ cold dark matter cosmology. A key feature of our model is the self-consistent… Expand
Predictions for high-frequency radio surveys of extragalactic sources
- G. Zotti, R. Ricci, +4 authors J. González-Nuevo
- Physics
- 28 October 2004
We present detailed predictions of the contributions of the various source populations to the counts at frequen- cies of tens of GHz. New evolutionary models are worked out for flat-spectrum radio… Expand
The evolution of the dust and gas content in galaxies
- P. Santini, R. Maiolino, +36 authors K. Xu
- Physics
- 14 November 2013
We use deep Herschel observations taken with both PACS and SPIRE imaging cameras to estimate the dust mass of a sample of galaxies extracted from the GOODS-S, GOODS-N and the COSMOS fields. We divide… Expand
Dust and nebular emission. I. Models for normal galaxies
- P. Panuzzo, A. Bressan, +7 authors O. Trieste
- Physics
- 4 July 2003
Received ; accepted Abstract. We present a model for nebular emission in star forming galaxies, which takes into account the effects of dust reprocessing. The nebular emissions (continuum emission,… Expand
Astrophysical and cosmological information from large-scale submillimetre surveys of extragalactic sources
- M. Negrello, F. Perrotta, +5 authors L. Danese
- Physics
- 9 March 2007
We present a quantitative analysis of the astrophysical and cosmological information that can be extracted from the many important wide-area, shallow surveys that will be carried out in the next few… Expand
Far infrared and radio emission in dusty starburst galaxies
- A. Bressan, L. Silva, G. L. Granato
- Physics
- 3 June 2002
We revisit the nature of the far infrared (FIR)/radio correlation by means of the most recent models of star forming galaxies, focusing in particular on the case of obscured starbursts. We model the… Expand
Modeling the spectral energy distribution of ULIRGs - I. The radio spectra
- M. Clemens, O. Vega, A. Bressan, G. L. Granato, L. Silva, P. Panuzzo
- Physics
- 1 August 2007
Aims. We aim to constrain new starburst/AGN models of IRAS bright galaxies via their spectral energy distribution from the nearinfrared to the radio. To this end, we determine the radio spectra for a… Expand