7 papers
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…
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)…
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…
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…
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…
Observability of Early Evolutionary Phases of Galaxies at mm Wavelengths
G. De Zotti, P. Mazzei, A. Franceschini +1
Several lines of evidence and theoretical arguments suggest that a large fraction of starlight is absorbed by interstellar dust and re-radiated at far-IR wavelengths, particularly…