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• W2079652688 endingPage "969" @default.
• W2079652688 startingPage "957" @default.
• W2079652688 abstract "We present mid-infrared spectra of 32 high-redshift ultraluminous infrared galaxies, selected via the stellar photospheric feature at rest-frame 1.6 μm, and an observed-frame 24 μm flux of >500 μJy. Nearly all the sample reside in a redshift range of ⟨ z⟩ = 1.71 ± 0.15 and have rest-frame 1-1000 μm luminosities of 1012.9-1013.8 L☉. Most of the spectra exhibit prominent polycyclic aromatic hydrocarbon emission features and weak silicate absorption, consistent with a starburst origin for the IR emission. Our selection method appears to be a straightforward and efficient way of finding distant, IR-luminous, star-forming galaxies in narrow redshift ranges. There is, however, evidence that the mid-IR spectra of our sample differ systematically from those of local ULIRGs; our sample have comparable PAH equivalent widths but weaker apparent silicate absorption, and (possibly) enhanced PAH 6.2 μm/7.7 μm and 6.2 μm/11.2 μm flux ratios. Furthermore, the composite mid-IR spectrum of our sample is almost identical to that of local starbursts with IR luminosities of 1010-1011 L☉, rather than that of local ULIRGs. These differences are consistent with a reduced dust column, which can plausibly be obtained via some combination of (1) star formation that is extended over spatial scales of 1-4 kpc and (2) star formation in unusually gas-rich regions." @default.
• W2079652688 created "2016-06-24" @default.
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• W2079652688 date "2008-04-20" @default.
• W2079652688 modified "2023-09-25" @default.
• W2079652688 title "The Nature of Star Formation in Distant Ultraluminous Infrared Galaxies Selected in a Remarkably Narrow Redshift Range" @default.
• W2079652688 cites W1492972489 @default.
• W2079652688 cites W1494366456 @default.
• W2079652688 cites W1681063222 @default.
• W2079652688 cites W1880006316 @default.
• W2079652688 cites W1929623410 @default.
• W2079652688 cites W1966320264 @default.
• W2079652688 cites W1971306567 @default.
• W2079652688 cites W1973939397 @default.
• W2079652688 cites W1977843574 @default.
• W2079652688 cites W1978188520 @default.
• W2079652688 cites W1978480760 @default.
• W2079652688 cites W1986486448 @default.
• W2079652688 cites W1986619956 @default.
• W2079652688 cites W1987400244 @default.
• W2079652688 cites W1989379779 @default.
• W2079652688 cites W1989738078 @default.
• W2079652688 cites W1990732800 @default.
• W2079652688 cites W1990923363 @default.
• W2079652688 cites W1994703407 @default.
• W2079652688 cites W1995030014 @default.
• W2079652688 cites W1995066861 @default.
• W2079652688 cites W1998759148 @default.
• W2079652688 cites W2003637061 @default.
• W2079652688 cites W2004032299 @default.
• W2079652688 cites W2004152002 @default.
• W2079652688 cites W2007741717 @default.
• W2079652688 cites W2014170433 @default.
• W2079652688 cites W2015267403 @default.
• W2079652688 cites W2016121098 @default.
• W2079652688 cites W2017569741 @default.
• W2079652688 cites W2018858432 @default.
• W2079652688 cites W2019274267 @default.
• W2079652688 cites W2020863669 @default.
• W2079652688 cites W2024301260 @default.
• W2079652688 cites W2027739765 @default.
• W2079652688 cites W2029193721 @default.
• W2079652688 cites W2029350534 @default.
• W2079652688 cites W2031203855 @default.
• W2079652688 cites W2038551325 @default.
• W2079652688 cites W2038897178 @default.
• W2079652688 cites W2041984258 @default.
• W2079652688 cites W2042692850 @default.
• W2079652688 cites W2044669640 @default.
• W2079652688 cites W2046312639 @default.
• W2079652688 cites W2047953583 @default.
• W2079652688 cites W2051128239 @default.
• W2079652688 cites W2056085571 @default.
• W2079652688 cites W2065155014 @default.
• W2079652688 cites W2069771108 @default.
• W2079652688 cites W207201400 @default.
• W2079652688 cites W2074987565 @default.
• W2079652688 cites W2083570008 @default.
• W2079652688 cites W2084061910 @default.
• W2079652688 cites W2085122822 @default.
• W2079652688 cites W2089442644 @default.
• W2079652688 cites W2090268762 @default.
• W2079652688 cites W2090459210 @default.
• W2079652688 cites W2093322326 @default.
• W2079652688 cites W2093811237 @default.
• W2079652688 cites W2095225003 @default.
• W2079652688 cites W2102519805 @default.
• W2079652688 cites W2105875544 @default.
• W2079652688 cites W2109104929 @default.
• W2079652688 cites W2110830624 @default.
• W2079652688 cites W2112685586 @default.
• W2079652688 cites W2115032180 @default.
• W2079652688 cites W2117271951 @default.
• W2079652688 cites W2117629212 @default.
• W2079652688 cites W2118955801 @default.
• W2079652688 cites W2122471784 @default.
• W2079652688 cites W2124572431 @default.
• W2079652688 cites W2127580887 @default.
• W2079652688 cites W2127581133 @default.
• W2079652688 cites W2128517068 @default.
• W2079652688 cites W2130190861 @default.
• W2079652688 cites W2132662311 @default.
• W2079652688 cites W2148804397 @default.
• W2079652688 cites W2149976691 @default.
• W2079652688 cites W2153887579 @default.
• W2079652688 cites W2154474449 @default.
• W2079652688 cites W2155122056 @default.
• W2079652688 cites W2155475085 @default.
• W2079652688 cites W2162926959 @default.
• W2079652688 cites W2163171108 @default.

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