Probing the Evolution of the Infrared Luminosity Function of Galaxies to z = 0.5

Details Probing the Evolution of the Infrared Luminosity Function of Galaxies to z = 0.5 Probing the Evolution of the Infrared Luminosity Function of Galaxies to z = 0.5

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21342417m&link_type=abstract

American Astronomical Society, AAS Meeting #213, #424.17; Bulletin of the American Astronomical Society, Vol. 41, p.248

Other

Scientific paper

We present preliminary results from our redshift survey of 836 infrared sources covering the redshift range z = 0 - 0.5 in two deep fields observed with the Spitzer Space Telescope and XMM: the Lockman Hole and the Subaru XMM Deep Field. This dataset, in conjunction with our published data in the First Look Survey, is used to compute the infrared luminosity function of galaxies overcoming the main limitations of other published studies with heavy reliance on photometric redshifts, AGN contamination, and cosmic variance.

Affiliated with

Also associated with

No associations

Rating

Probing the Evolution of the Infrared Luminosity Function of Galaxies to z = 0.5 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 Probing the Evolution of the Infrared Luminosity Function of Galaxies to z = 0.5, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Probing the Evolution of the Infrared Luminosity Function of Galaxies to z = 0.5 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1702922