Rest-Optical Spectroscopic Properties of Luminous Infrared Galaxies at z˜2

Details Rest-Optical Spectroscopic Properties of Luminous Infrared Galaxies at z˜2 Rest-Optical Spectroscopic Properties of Luminous Infrared Galaxies at z˜2

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..399..214y&link_type=abstract

Panoramic Views of Galaxy Formation and Evolution ASP Conference Series, Vol. 399, proceedings of the conference held 11-16 Dece

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present the results of a near-infrared multi-object spectroscopic (MOS) observation of sBzK color and Spitzer/MIPS 24μm selected galaxies, which are used to examine the rest-optical spectroscopic properties of infrared luminous galaxies at z˜2. Both dust-corrected Hα luminosity and MIPS flux show consistent star formation rate, but some galaxies have moderate excess of MIPS flux. Star-formation time scales from Hα star formation rates and the stellar mass of our sample shows that massive ultra-luminous red galaxies (ULIRGs) are forming most of their stars during the redshift range of our sample.

Affiliated with

Also associated with

No associations

Rating

Rest-Optical Spectroscopic Properties of Luminous Infrared Galaxies at z˜2 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 Rest-Optical Spectroscopic Properties of Luminous Infrared Galaxies at z˜2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rest-Optical Spectroscopic Properties of Luminous Infrared Galaxies at z˜2 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-772745