Evolution of IR-luminous SED from 0.1 < z < 0.6

Details Evolution of IR-luminous SED from 0.1 < z < 0.6 Evolution of IR-luminous SED from 0.1 < z < 0.6

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sptz.prop50245b&link_type=abstract

Spitzer Proposal ID #50245

Physics

Scientific paper

Luminous Infrared Galaxies (LIRGs) are primary contributors to the energy production at redshift ~1. They are responsible for the dramatic increase of the star formation density from z=0 to z=1. Establishing proper spectral energy distribution for this class of sources to characterize the physics of the high star formation activity is one of the challenge of the coming decade. We have obtained IRS low resolution spectra of a sample of 40 LIRGs at 0.1

Affiliated with

Also associated with

No associations

Rating

Evolution of IR-luminous SED from 0.1 < z < 0.6 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 Evolution of IR-luminous SED from 0.1 < z < 0.6, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of IR-luminous SED from 0.1 < z < 0.6 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-884871