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• W2066233280 endingPage "L13" @default.
• W2066233280 startingPage "L13" @default.
• W2066233280 abstract "We report the detection of four IRAC sources in the GOODS-South field with an extremely red color of H − [3.6] > 4.5. The four sources are not detected in the deep Hubble Space Telescope WFC3 H-band image with Hlimit = 28.3 mag. We find that only three types of SED templates can produce such a red H − [3.6] color: a very dusty SED with the Calzetti extinction of AV = 16 mag at z = 0.8; a very dusty SED with the SMC extinction of AV = 8 mag at z = 2.0– 2.2; and an 1 Gyr SSP with AV ∼ 0.8 at z = 5.7. We argue that these sources are unlikely dusty galaxies at z ⩽ 2.2 based on absent strong MIPS 24 μm emission. The old stellar population model at z > 4.5 remains a possible solution for the 4 sources. At z > 4.5, these sources have stellar masses of log(M*/M☉) = 10.6–11.2. One source, ERS-1, is also a type-II X-ray QSO with L2 − 8 keV = 1.6 × 1044 erg s−1. One of the four sources is an X-ray QSO and another one is a HyperLIRG, suggesting a galaxy-merging scenario for the formation of these massive galaxies at high redshifts." @default.
• W2066233280 created "2016-06-24" @default.
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• W2066233280 date "2011-11-01" @default.
• W2066233280 modified "2023-10-18" @default.
• W2066233280 title "FOUR IRAC SOURCES WITH AN EXTREMELY RED H – [3.6] COLOR: PASSIVE OR DUSTY GALAXIES AT <i>z</i> > 4.5?" @default.
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• W2066233280 doi "https://doi.org/10.1088/2041-8205/742/1/l13" @default.
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