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dc.contributor.authorMenéndez-Delmestre, Karínen_US
dc.contributor.authorBlain, Andrew W.en_US
dc.contributor.authorAlexander, Dave M.en_US
dc.contributor.authorSmail, Ianen_US
dc.contributor.authorArmus, Leeen_US
dc.contributor.authorChapman, Scott C.en_US
dc.contributor.authorFrayer, Daveen_US
dc.contributor.authorIvison, Rob J.en_US
dc.contributor.authorTeplitz, Harryen_US
dc.date.accessioned2014-03-12T19:20:57Z
dc.date.available2014-03-12T19:20:57Z
dc.date.issued2007-02-01en_US
dc.identifier.citationMenéndez-Delmestre, Karín, Andrew W. Blain, Dave M. Alexander, Ian Smail, et al. 2007. "Mid-Infrared Spectroscopy of High Redshift Submillimeter Galaxies: First Results." The Astrophysical Journal 655(2): 65-L68en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://dx.doi.org/10.1086/512038en_US
dc.identifier.urihttp://hdl.handle.net/10222/45397
dc.description.abstractWe present mid-infrared spectra of 5 submillimeter galaxies at z=0.65-2.38 taken with the Spitzer Space Telescope. Four of these sources, at z<1.5, have strong PAH features and their composite spectrum is well fitted by an M82-like spectrum with an additional power-law component consistent with that expected from AGN activity. Based on a comparison of the 7.7-micron PAH equivalent width and the PAH-to-infrared luminosity ratio of these galaxies with local templates, we conclude that these galaxies host both star-formation and AGN activity, with star-formation dominating the bolometric luminosity. The source at z=2.38 displays a Mrk231-type broad feature at restframe ~8 micron that does not conform to the typical 7.7/8.6 micron PAH complex in starburst galaxies, suggesting a more substantial AGN contribution.en_US
dc.titleMid-Infrared Spectroscopy of High Redshift Submillimeter Galaxies: First Resultsen_US
dc.title.alternativeThe Astrophysical Journalen_US
dc.typearticleen_US
dc.identifier.volume655en_US
dc.identifier.issue2en_US
dc.identifier.startpage65en_US
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