Mathematics – Logic
Scientific paper
Mar 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005phdt.........2b&link_type=abstract
PhD Thesis, Padova University, I, 2005.
Mathematics
Logic
5
Galaxy, Spitzer, Infrared, Counts, Spectroscopy, Iso, Ulirg, Sed, Iras, Rdcs
Scientific paper
This Thesis follows a chronological outline, covering the development of infrared space facilities in the last decades: IRAS, ISO and Spitzer galaxies are studied.
Optical, near- and mid-IR spectroscopy, optical spectropolarimetry and broad-band UV to sub-mm analysis of nearby Ultra Luminous Infrared Galaxies are used as ``local laboratory'' for studying distant IR, active, dusty galaxies.
Optical and near-IR spectroscopy of 15 microns ISO sources is analysed; a comparison of the broad-band spectral energy distributions of such objects to those of intermediate-redshift early-type galaxies and distant Lyman-break sources follows.
Early Spitzer/SWIRE data are used here to study the optical to near-IR restframe SEDs of galaxies up to redshift ~3, exploiting both near- and mid-IR observations by IRAC and MIPS. The evolution of actively star-forming sources is analyzed through modeling of differential mid-IR source counts. A subsample of field galaxies from the GOODS survey is finally compared to the members of the RDCS 1252.9-2927 cluster, lying at a redshift z=1.237.
No associations
LandOfFree
Multiwavelength analyses of faint infrared galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Multiwavelength analyses of faint infrared galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multiwavelength analyses of faint infrared galaxies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1567108