The Mass-Luminosity Relation of Galaxies in the Deep Lens Survey

Details The Mass-Luminosity Relation of Galaxies in the Deep Lens Survey The Mass-Luminosity Relation of Galaxies in the Deep Lens Survey

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21733532c&link_type=abstract

American Astronomical Society, AAS Meeting #217, #335.32; Bulletin of the American Astronomical Society, Vol. 43, 2011

Mathematics

Logic

Scientific paper

Characterization of the redshift-dependence of the total mass to light and stellar mass to total mass relationships is an important probe of galaxy evolution. Recent theoretical progress has been made using statistical models such as abundance matching, but observational studies have been primarily limited to galaxies at low redshifts or very massive galaxies at higher redshifts. We present results from the Deep Lens Survey using galaxy-galaxy weak lensing to directly constrain total galaxy masses over several decades of mass out to z 0.7. We investigate the correlation of the M/L with color and environment as well as the possibility of evolution with cosmological time.

Affiliated with

Also associated with

No associations

Rating

The Mass-Luminosity Relation of Galaxies in the Deep Lens Survey 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 The Mass-Luminosity Relation of Galaxies in the Deep Lens Survey, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Mass-Luminosity Relation of Galaxies in the Deep Lens Survey will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1402005