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IRAC excess in distant star-forming galaxies: tentative evidence for the 3.3 μm polycyclic aromatic hydrocarbon feature?

Magnelli, B. and Chary, R. R. and Pope, A. and Elbaz, D. and Morrison, G. and Dickinson, M. (2008) IRAC excess in distant star-forming galaxies: tentative evidence for the 3.3 μm polycyclic aromatic hydrocarbon feature? Astrophysical Journal, 681 (1). pp. 258-268. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:MAGapj08

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Abstract

We present evidence for the existence of an IRAC excess in the spectral energy distribution (SED) of five galaxies at 0.6 < z < 0.9 and one galaxy at z = 1.7. These six galaxies, located in the Great Observatories Origins Deep Survey field (GOODS-N), are star-forming since they present strong 6.2, 7.7, and, 11.3 μm polycyclic aromatic hydrocarbon (PAH) lines in their Spitzer IRS mid-infrared spectra. We use a library of templates computed with PEGASE.2 to fit their multiwavelength photometry and derive their stellar continuum. Subtraction of the stellar continuum enables us to detect in five galaxies a significant excess in the IRAC band pass where the 3.3 μm PAH is expected (i.e., IRAC 5.8 μm for the range of redshifts considered here). We then assess if the physical origin of the IRAC excess is due to an obscured active galactic nucleus (AGN) or warm dust emission. For one galaxy evidence of an obscured AGN is found, while the remaining four do not exhibit any significant AGN activity. Possible contamination by warm dust continuum of unknown origin as found in the Galactic diffuse emission is discussed. The properties of such a continuum would have to be different from the local universe to explain the measured IRAC excess, but we cannot definitively rule out this possibility until its origin is understood. Assuming that the IRAC excess is dominated by the 3.3 μm PAH feature, we find good agreement with the observed 11.3 μm PAH line flux arising from the same C-H bending and stretching modes, consistent with model expectations. Finally, the IRAC excess appears to be correlated with the star formation rate in the galaxies. Hence it could provide a powerful diagnostic for measuring dusty star formation in z > 3 galaxies once the mid-infrared spectroscopic capabilities of the James Webb Space Telescope become available.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/588599DOIArticle
http://www.iop.org/EJ/abstract/0004-637X/681/1/258/PublisherArticle
ORCID:
AuthorORCID
Chary, R. R.0000-0001-7583-0621
Pope, A.0000-0001-8592-2706
Elbaz, D.0000-0002-7631-647X
Dickinson, M.0000-0001-5414-5131
Additional Information:© 2008 American Astronomical Society. Print publication: Issue 1 (2008 July 1); received 2007 August 28; accepted for publication 2008 March 25. We thank Stephanie Juneau for revisiting our analysis of the optical spectra of these galaxies. We thank Masa Imanishi and Aaron Steffen for useful discussions. A. P. acknowledges support provided by NASA through the Spitzer Space Telescope Fellowship Program, through a contract issued by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. SMART was developed by the IRS Team at Cornell University and is available through the Spitzer Science Center at Caltech.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASAUNSPECIFIED
Subject Keywords:galaxies: evolution; galaxies: starburst; infrared: galaxies
Issue or Number:1
Record Number:CaltechAUTHORS:MAGapj08
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:MAGapj08
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:13819
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:02 Apr 2009 22:40
Last Modified:03 Oct 2019 00:44

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