Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100179612> ?p ?o ?g. }
- W3100179612 endingPage "112" @default.
- W3100179612 startingPage "112" @default.
- W3100179612 abstract "Hot dust-obscured galaxies (Hot DOGs) are among the most luminous galaxies in the universe. Powered by highly obscured, possibly Compton-thick, active galactic nuclei (AGNs), Hot DOGs are characterized by spectral energy distributions that are very red in the mid-infrared yet dominated by the host galaxy stellar emission in the UV and optical. An earlier study identified a subsample of Hot DOGs with significantly enhanced UV emission. One target, W0204–0506, was studied in detail and, based on Chandra observations, it was concluded that the enhanced emission was most likely due to either extreme unobscured star formation (star formation rate > 1000 M⊙ yr−1) or to light from the highly obscured AGN scattered by gas or dust into our line of sight. Here, we present a follow-up study of W0204–0506 as well as two more Hot DOGs with excess UV emission. For the two new objects we obtained Chandra/ACIS-S observations, and for all three targets we obtained Hubble Space Telescope/WFC3 F555W and F160W imaging. The analysis of these observations, combined with multiwavelength photometry and UV/optical spectroscopy suggests that UV emission is most likely dominated by light from the central highly obscured, hyperluminous AGN that has been scattered into our line of sight, by either gas or dust. We cannot decisively rule out, however, that star formation or a second AGN in the system may significantly contribute to the UV excess of these targets." @default.
- W3100179612 created "2020-11-23" @default.
- W3100179612 creator A5004709630 @default.
- W3100179612 creator A5019841491 @default.
- W3100179612 creator A5019923842 @default.
- W3100179612 creator A5025718836 @default.
- W3100179612 creator A5029222325 @default.
- W3100179612 creator A5030771447 @default.
- W3100179612 creator A5044199747 @default.
- W3100179612 creator A5053324463 @default.
- W3100179612 creator A5054495214 @default.
- W3100179612 creator A5071998850 @default.
- W3100179612 creator A5081767701 @default.
- W3100179612 creator A5087897086 @default.
- W3100179612 creator A5090992108 @default.
- W3100179612 date "2020-07-08" @default.
- W3100179612 modified "2023-10-17" @default.
- W3100179612 title "Hot Dust-obscured Galaxies with Excess Blue Light" @default.
- W3100179612 cites W1485888419 @default.
- W3100179612 cites W1964385238 @default.
- W3100179612 cites W1981452559 @default.
- W3100179612 cites W1982857458 @default.
- W3100179612 cites W1987319691 @default.
- W3100179612 cites W1992572559 @default.
- W3100179612 cites W1997779216 @default.
- W3100179612 cites W2002044265 @default.
- W3100179612 cites W2010627606 @default.
- W3100179612 cites W2021006944 @default.
- W3100179612 cites W2024319723 @default.
- W3100179612 cites W2027970060 @default.
- W3100179612 cites W2032674235 @default.
- W3100179612 cites W2038328108 @default.
- W3100179612 cites W2052937506 @default.
- W3100179612 cites W2058379217 @default.
- W3100179612 cites W2068340869 @default.
- W3100179612 cites W2075222279 @default.
- W3100179612 cites W2081265738 @default.
- W3100179612 cites W2083572051 @default.
- W3100179612 cites W2089375435 @default.
- W3100179612 cites W2092882252 @default.
- W3100179612 cites W2106044588 @default.
- W3100179612 cites W2106074821 @default.
- W3100179612 cites W2109909345 @default.
- W3100179612 cites W2142238829 @default.
- W3100179612 cites W2152505756 @default.
- W3100179612 cites W2155288520 @default.
- W3100179612 cites W2165356463 @default.
- W3100179612 cites W2171622449 @default.
- W3100179612 cites W2291265024 @default.
- W3100179612 cites W2341734301 @default.
- W3100179612 cites W2346478428 @default.
- W3100179612 cites W2521878568 @default.
- W3100179612 cites W2525578541 @default.
- W3100179612 cites W2581997630 @default.
- W3100179612 cites W2621633326 @default.
- W3100179612 cites W2774155353 @default.
- W3100179612 cites W2810910383 @default.
- W3100179612 cites W2895005148 @default.
- W3100179612 cites W2901421994 @default.
- W3100179612 cites W2998815163 @default.
- W3100179612 cites W3098217400 @default.
- W3100179612 cites W3098845432 @default.
- W3100179612 cites W3099155372 @default.
- W3100179612 cites W3099321129 @default.
- W3100179612 cites W3099418948 @default.
- W3100179612 cites W3099537209 @default.
- W3100179612 cites W3100019216 @default.
- W3100179612 cites W3100064752 @default.
- W3100179612 cites W3100265020 @default.
- W3100179612 cites W3100445047 @default.
- W3100179612 cites W3101070241 @default.
- W3100179612 cites W3101742051 @default.
- W3100179612 cites W3101982976 @default.
- W3100179612 cites W3102936492 @default.
- W3100179612 cites W3103614059 @default.
- W3100179612 cites W3104343073 @default.
- W3100179612 cites W3104416848 @default.
- W3100179612 cites W3105546747 @default.
- W3100179612 cites W3105755493 @default.
- W3100179612 cites W3124164584 @default.
- W3100179612 cites W3125096254 @default.
- W3100179612 cites W3125409350 @default.
- W3100179612 cites W4296142163 @default.
- W3100179612 doi "https://doi.org/10.3847/1538-4357/ab9814" @default.
- W3100179612 hasPublicationYear "2020" @default.
- W3100179612 type Work @default.
- W3100179612 sameAs 3100179612 @default.
- W3100179612 citedByCount "11" @default.
- W3100179612 countsByYear W31001796122020 @default.
- W3100179612 countsByYear W31001796122021 @default.
- W3100179612 countsByYear W31001796122022 @default.
- W3100179612 countsByYear W31001796122023 @default.
- W3100179612 crossrefType "journal-article" @default.
- W3100179612 hasAuthorship W3100179612A5004709630 @default.
- W3100179612 hasAuthorship W3100179612A5019841491 @default.
- W3100179612 hasAuthorship W3100179612A5019923842 @default.
- W3100179612 hasAuthorship W3100179612A5025718836 @default.
- W3100179612 hasAuthorship W3100179612A5029222325 @default.