|
|
|
|
LEADER |
02504 am a22003373u 4500 |
001 |
95501 |
042 |
|
|
|a dc
|
100 |
1 |
0 |
|a Kurczynski, Peter
|e author
|
100 |
1 |
0 |
|a Massachusetts Institute of Technology. Department of Physics
|e contributor
|
100 |
1 |
0 |
|a Cardamone, Carolin
|e contributor
|
700 |
1 |
0 |
|a Gawiser, Eric
|e author
|
700 |
1 |
0 |
|a Huynh, Minh
|e author
|
700 |
1 |
0 |
|a Ivison, Rob J.
|e author
|
700 |
1 |
0 |
|a Treister, Ezequiel
|e author
|
700 |
1 |
0 |
|a Smail, Ian
|e author
|
700 |
1 |
0 |
|a Blanc, Guillermo A.
|e author
|
700 |
1 |
0 |
|a Greve, Thomas R.
|e author
|
700 |
1 |
0 |
|a Schinnerer, Eva
|e author
|
700 |
1 |
0 |
|a Urry, Meg
|e author
|
700 |
1 |
0 |
|a van der Werf, Paul
|e author
|
700 |
1 |
0 |
|a Cardamone, Carolin
|e author
|
245 |
0 |
0 |
|a PANCHROMATIC ESTIMATION OF STAR FORMATION RATES IN BzK GALAXIES AT 1 < z < 3
|
260 |
|
|
|b IOP Publishing,
|c 2015-02-25T13:22:03Z.
|
856 |
|
|
|z Get fulltext
|u http://hdl.handle.net/1721.1/95501
|
520 |
|
|
|a We determine star formation rates (SFRs) in a sample of color-selected, star-forming (sBzK) galaxies (K [subscript AB] < 21.8) in the Extended Chandra Deep Field-South. To identify and avoid active galactic nuclei, we use X-ray, IRAC color, and IR/radio flux ratio selection methods. Photometric redshift-binned, average flux densities are measured with stacking analyses in Spitzer-MIPS IR, BLAST and APEX/LABOCA submillimeter, VLA and GMRT radio, and Chandra X-ray data. We include averages of aperture fluxes in MUSYC UBVRIz'JHK images to determine UV-through-radio spectral energy distributions. We determine the total IR luminosities and compare SFR calibrations from FIR, 24 μm, UV, radio, and X-ray wavebands. We find consistency with our best estimator, SFR[subscript IR + UV], to within errors for the preferred radio SFR calibration. Our results imply that 24 μm only and X-ray SFR estimates should be applied to high-redshift galaxies with caution. Average IR luminosities are consistent with luminous infrared galaxies. We find SFR[subscript IR + UV] for our stacked sBzKs at median redshifts 1.4, 1.8, and 2.2 to be 55 ± 6 (random error), 74 ± 8, and 154 ± 17 M [subscript ☉] yr[superscript -1], respectively, with additional systematic uncertainty of a factor of ~2.
|
520 |
|
|
|a National Science Foundation (U.S.) (Grant AST-0807570)
|
520 |
|
|
|a National Science Foundation (U.S.) (Grant AST-1055919)
|
520 |
|
|
|a United States. National Aeronautics and Space Administration
|
546 |
|
|
|a en_US
|
655 |
7 |
|
|a Article
|
773 |
|
|
|t The Astrophysical Journal
|