The most luminous_galaxies_discovered_by_wise

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The Astrophysical Journal, in Press
Preprint typeset using LATEX style emulateapj v. 5/2/11
THE MOST LUMINOUS GALAXIES DIS...

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intense starburst induced by the gas cloud collisions is
quickly followed by an optically luminous quasar phase,
and eve...

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Table 1
Properties of WISE ELIRGs
Source WISE Coordinates z Qz
R.A. (J2000) Decl. (J2000)
W0116 0505 01:16:01.42 05:05:0...

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Table 2
Photometry of WISE ELIRGs
Source r0-band 3.6µm 4.5µm 12µm 22µm 70µm 160µm 250µm 350µm 500µm
(µJy) (µJy) (µJy) (m...

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Table 3
Properties of Optically Selected Quasars with Lbol > 1014L (Short Version)
Source WISE Coordinate Redshift Lbol
...

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Figure 2. Mid-IR colors of the hyperluminous (Lbol > 1014 L )
Hot DOGs and optically selected hyperluminous quasars. The...

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Figure 3. Normalized rest-frame SEDs of the hyperluminous (Lbol > 1014 L ) ELIRG Hot DOGs and optically-selected hyperlu...

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Table 5
Luminosities of WISE ELIRGs
Source Redshift Lbol LIR L0.1 1 µm L1 20 µm L>20 µm L5.8 µm L7.8 µm
(1013L ) (1013L ...

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Figure 6. Mass limit of unresolved lenses vs. redshift, assuming
a source at z = 3.2. The blue curve shows the upper lim...

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Figure 8. Normalized histogram of LMIR/Lbol for WISE Hot
DOGs and optically selected quasars with Lbol > 1014 L , where...

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Figure 9. Ratio of L5.8µm to Lbol (left) and L7.8µm to Lbol (right) of hyperluminous Hot DOGs and quasars. The dashed l...

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massive black holes at the present epoch is not easy to
explain when the abundance of Hot DOGs matches that
of powerful...

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the ¯✏ estimate signiﬁcantly due to the logarithmic scal-
ing (Equation 7). An order of magnitude uncertainty in
these ...

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Figure 10. Bolometric luminosity Lbol vs. redshift. The age of the SMBH since formation at z ⇠ 20 is plotted on the top...

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cently, 1HERMES X24 J161506.65+543846.9 at z =
4.952 was discovered by Herschel HerMES survey (Casey
et al. 2012a). Its...

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R. J. A. was supported by Gemini-CONICYT grant num-
ber 32120009.
Facilities: WISE, Spitzer (IRAC), Herschel (PACS,
SPI...

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Silk, J., & Rees, M. J. 1998, A&A, 331, L1
Skrutskie, M. F., Cutri, R. M., Stiening, R., et al. 2006, AJ, 131,
1163
Spr...

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