Clustering Of Starforming Galaxies And Agn At z˜3; In Musyc

Details Clustering Of Starforming Galaxies And Agn At z˜3; In Musyc Clustering Of Starforming Galaxies And Agn At z˜3; In Musyc

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.3503f&link_type=abstract

American Astronomical Society, AAS Meeting #211, #35.03; Bulletin of the American Astronomical Society, Vol. 39, p.787

Other

Scientific paper

The MUltiwavelength Survey by Yale/Chile (MUSYC; Gawiser et al. 2006, ApjS 162, 1) covers 1.2 square degrees of sky to U,B,V,R˜26; and K˜22; (AB). The deep imaging with broad wavelength coverage of this survey (UBVRIzJHK+NB5000) is especially suited for selecting starforming galaxies at z˜3. Using UVR, BV+NB5000, X-rays and spectroscopy, we have selected LBG (Lyman Break Galaxies), LAE (Lyman Alpha Emitters) and AGN at z˜3. We present results on the clustering properties of these protogalaxies over the whole survey, where we found the dark matter halos of LAEs, LBGs and AGN to have masses of log10(M/M_&sun;) = 10.9+0.5/-0.9, 11.8+/-0.1 and 12.6+0.5/-0.8 respectively. This shows, on one side, consistency with AGN downsizing, namely that SMBH tend to be in galaxies more massive than the typical population. On the other side, LAEs seem to sit in relatively low mass halos, which might contain L* galaxies today.

Affiliated with

Also associated with

No associations

Rating

Clustering Of Starforming Galaxies And Agn At z˜3; In Musyc 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 Clustering Of Starforming Galaxies And Agn At z˜3; In Musyc, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clustering Of Starforming Galaxies And Agn At z˜3; In Musyc will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1476553