Ultradeep Spectroscopy with the Spitzer^1 IRS^2

Details Ultradeep Spectroscopy with the Spitzer^1 IRS^2 Ultradeep Spectroscopy with the Spitzer^1 IRS^2

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..381..357t&link_type=abstract

The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution. ASP Conference Series, Vol. 381,

Astronomy and Astrophysics

Astronomy

Scientific paper

Mid-IR spectroscopy has detected the signatures of star-formation (PAH emission) in high redshift (z>1) ultra- and hyper-luminous infrared galaxies. However, the study of the dominant population of IR-luminous galaxies (10^{11} - 10^{12} Lsun at 1

Affiliated with

Also associated with

No associations

Rating

Ultradeep Spectroscopy with the Spitzer^1 IRS^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 Ultradeep Spectroscopy with the Spitzer^1 IRS^2, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultradeep Spectroscopy with the Spitzer^1 IRS^2 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-952603