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astro-ph2008

Bars driven by the Cosmology in stellar-gaseous disks

Anna Curir, Paola Mazzei, Giuseppe Murante

We present the first attempt to analyse the growth of the bar instability in stellar-gaseous disks evolving in a fully consistent cosmological scenario. We explored the role of the…

astro-ph2001

Formation of Spheroidal Galaxies: The Sub-MM View

G. De Zotti, G. L. Granato, C. Baccigalupi +4

The intensity of the Cosmic Far-IR Background and the strong evolution of galaxies in the far-IR to mm wavelength range demonstrate that the bulk of starlight emitted during the ea…

astro-ph2000

The Effect of Dust on Photometric Redshift Measurement; A Self-consistent Technique

Bahram Mobasher, Paola Mazzei

A new method is developed for estimating photometric redshifts to galaxies, using realistic template SEDs, extending over four decades in wavelength (i.e. from 0.05 micron to 1 mm)…

astro-ph1999

A Self-consistent Method for Estimating Photometric Redshifts

B. Mobasher, P. Mazzei

A new method is developed for estimating photometric redshifts, using realistic template SEDs, extending over four decades in wavelength (i.e from 0.05 to 1 mm). The SEDs are…

astro-ph1997

Dust in high-z radio-loud AGN

Andrea Cimatti, Wolfram Freudling, Huub Roettgering +2

We present continuum observations of a small sample of high-redshift, radio-loud AGN (radio galaxies and quasars) aimed at the detection of thermal emission from dust. Seven AGN we…

astro-ph1997

Source Counts and Background Radiation

A. Franceschini, H. Aussel, A. Bressan +7

Our present understanding of the extragalactic source counts and background radiation at infrared and sub-mm wavelengths is reviewed. Available count data are used to constrain evo…