STRONG POLYCYCLIC AROMATIC HYDROCARBON EMISSION FROM z {approx} 2 ULIRGs

Journal Article · Sat Aug 01 04:00:00 EDT 2009 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/700/2/1190; COUNTRY OF INPUT: INTERNATIONAL ATOMIC ENERGY AGENCY (IAEA)· OSTI ID:21313802

Desai, Vandana; Soifer, B T; Melbourne, Jason ^[1]; Dey, Arjun; Brand, Kate; Brodwin, Mark; Jannuzi, Buell T ^[2]; Le Floc'h, Emeric ^[3]; Armus, Lee; Teplitz, Harry ^[4]; Brown, Michael J. I. ^[5]; Houck, James R; Weedman, Daniel W ^[6]; Ashby, Matthew L. N.; Jiasheng, Huang; Smith, Howard A; Willner, Steve P ^[7]; Gonzalez, Anthony ^[8]

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1. Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA 91125 (United States)
2. National Optical Astronomy Observatory, Tucson, AZ 85726-6732 (United States)
3. Institute for Astronomy, University of Hawaii, Honolulu, HI 96822 (United States)
4. Spitzer Science Center, California Institute of Technology, Pasadena, CA 91125 (United States)
5. School of Physics, Monash University, Clayton, Victoria 3800 (Australia)
6. Astronomy Department, Cornell University, Ithaca, NY 14853 (United States)
7. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)
8. Department of Astronomy, University of Florida, Gainesville, FL 32611-2055 (United States)

Using the Infrared Spectrograph on board the Spitzer Space Telescope, we present low-resolution (64 < {lambda}/{delta}{lambda} < 124), mid-infrared (20-38 {mu}m) spectra of 23 high-redshift ULIRGs detected in the Booetes field of the NOAO Deep Wide-Field Survey. All of the sources were selected to have (1) f {sub {nu}}(24 {mu}m)>0.5 mJy; (2) R - [24]>14 Vega mag; and (3) a prominent rest frame 1.6 {mu}m stellar photospheric feature redshifted into Spitzer's 3-8 {mu}m IRAC bands. Of these, 20 show emission from polycyclic aromatic hydrocarbons (PAHs), usually interpreted as signatures of star formation. The PAH features indicate redshifts in the range 1.5 < z < 3.0, with a mean of (z) = 1.96 and a dispersion of 0.30. Based on local templates, these sources have extremely large infrared luminosities, comparable to that of submillimeter galaxies. Our results confirm previous indications that the rest-frame 1.6 {mu}m stellar bump can be efficiently used to select highly obscured star-forming galaxies at z {approx} 2, and that the fraction of starburst-dominated ULIRGs increases to faint 24 {mu}m flux densities. Using local templates, we find that the observed narrow redshift distribution is due to the fact that the 24 {mu}m detectability of PAH-rich sources peaks sharply at z = 1.9. We can analogously use observed spectral energy distributions to explain the broader redshift distribution of Spitzer-detected ULIRGs that are dominated by an active galactic nucleus (AGN). Finally, we conclude that z {approx} 2 sources with a detectable 1.6 {mu}m stellar opacity feature lack sufficient AGN emission to veil the 7.7 {mu}m PAH band.

• OSTI ID: 21313802
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 700; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

99 GENERAL AND MISCELLANEOUS
EMISSION
ENERGY SPECTRA
FLUX DENSITY
GALACTIC EVOLUTION
GALAXIES
LUMINOSITY
POLYCYCLIC AROMATIC HYDROCARBONS
RED SHIFT
STARS
TELESCOPES