Searching for Low-Redshift Hot Dust-Obscured Galaxies
Guodong Li, Jingwen Wu, Chao-Wei Tsai, Daniel Stern, Roberto J. Assef,, Peter R. M. Eisenhardt, Kevin McCarthy, Hyunsung D. Jun, Tanio D\'iaz-Santos,, Andrew W. Blain, Trystan Lambert, Dejene Zewdie, Rom\'an Fern\'andez Aranda,, Cuihuan Li, Yao Wang, and Zeyu Tan

TL;DR
This study searches for low-redshift Hot Dust-Obscured Galaxies using WISE and Herschel data, identifying a few candidates and analyzing their properties to understand their role in galaxy evolution.
Contribution
It is the first to identify and spectroscopically confirm low-redshift Hot DOGs, expanding understanding of their evolution and properties at z<0.5.
Findings
Three low-redshift Hot DOGs confirmed spectroscopically.
Low-z Hot DOGs have black hole accretion near the Eddington limit.
Surface density of low-z Hot DOGs is an order of magnitude lower than high-z counterparts.
Abstract
Hot Dust-Obscured Galaxies (Hot DOGs), discovered by the "W1W2 dropout" selection at high redshifts ( 2-4), are a rare population of hyper-luminous obscured quasars. Their number density is comparable to similarly luminous type 1 quasars in the same redshift range, potentially representing a short, yet critical stage in galaxy evolution. The evolution in their number density towards low redshift, however, remains unclear as their selection function is heavily biased against objects at . We combine data from the WISE and Herschel archives to search for Hot DOGs at based on their unique spectral energy distributions. We find 68 candidates, and spectroscopic observations confirm that 3 of them are at . For those 3 we find their black hole accretion is close to the Eddington limit, with lower bolometric luminosities and black hole masses than those of…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Gamma-ray bursts and supernovae
