Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100658422> ?p ?o ?g. }
- W3100658422 endingPage "124101" @default.
- W3100658422 startingPage "124101" @default.
- W3100658422 abstract "Hot dust-obscured galaxies (Hot DOGs) are a new population recently discovered in the wise All-Sky survey. Multiwavelength follow-up observations suggest that they are luminous, dust-obscured quasars at high redshift. Here we present the JCMT SCUBA-2 850 $mu m$ follow-up observations of 10 Hot DOGs. Four out of ten Hot DOGs have been detected at $>3sigma$ level. Based on the IR SED decomposition approach, we derive the IR luminosities of AGN torus and cold dust components. Hot DOGs in our sample are extremely luminous with most of them having $L_{rm IR}^{rm tot}>10^{14} L_odot$. The torus emissions dominate the total IR energy output. However, the cold dust contribution is still non-negligible, with the fraction of the cold dust contribution to the total IR luminosity $(sim 8-24%)$ being dependent on the choice of torus model. The derived cold dust temperatures in Hot DOGs are comparable to those in UV bright quasars with similar IR luminosity, but much higher than those in SMGs. Higher dust temperatures in Hot DOGs may be due to the more intense radiation field caused by intense starburst and obscured AGN activities. Fourteen and five submillimeter serendipitous sources in the 10 SCUBA-2 fields around Hot DOGs have been detected at $>3sigma$ and $>3.5sigma$ levels, respectively. By estimating their cumulative number counts, we confirm the previous argument that Hot DOGs lie in dense environments. Our results support the scenario in which Hot DOGs are luminous, dust-obscured quasars lying in dense environments, and being in the transition phase between extreme starburst and UV-bright quasars." @default.
- W3100658422 created "2020-11-23" @default.
- W3100658422 creator A5003976784 @default.
- W3100658422 creator A5011869846 @default.
- W3100658422 creator A5038406883 @default.
- W3100658422 creator A5072218639 @default.
- W3100658422 date "2017-10-24" @default.
- W3100658422 modified "2023-10-16" @default.
- W3100658422 title "The SCUBA-2 850<i>μ</i>m Follow-up of<i>WISE</i>-selected, Luminous Dust-obscured Quasars" @default.
- W3100658422 cites W1482390384 @default.
- W3100658422 cites W1679458787 @default.
- W3100658422 cites W1839094326 @default.
- W3100658422 cites W1979252468 @default.
- W3100658422 cites W1994703407 @default.
- W3100658422 cites W2001852248 @default.
- W3100658422 cites W2004865359 @default.
- W3100658422 cites W2024319723 @default.
- W3100658422 cites W2025105301 @default.
- W3100658422 cites W2028213535 @default.
- W3100658422 cites W2028626541 @default.
- W3100658422 cites W2048316219 @default.
- W3100658422 cites W2049565733 @default.
- W3100658422 cites W2052937506 @default.
- W3100658422 cites W2054314318 @default.
- W3100658422 cites W2084830951 @default.
- W3100658422 cites W2086125693 @default.
- W3100658422 cites W2089375435 @default.
- W3100658422 cites W2106044588 @default.
- W3100658422 cites W2117322039 @default.
- W3100658422 cites W2131546154 @default.
- W3100658422 cites W2132759038 @default.
- W3100658422 cites W2135536375 @default.
- W3100658422 cites W2136576103 @default.
- W3100658422 cites W2137454077 @default.
- W3100658422 cites W2139681095 @default.
- W3100658422 cites W2141105013 @default.
- W3100658422 cites W2147875900 @default.
- W3100658422 cites W2152912297 @default.
- W3100658422 cites W2153449693 @default.
- W3100658422 cites W2153931839 @default.
- W3100658422 cites W2158198401 @default.
- W3100658422 cites W2162511570 @default.
- W3100658422 cites W2162680611 @default.
- W3100658422 cites W2164106029 @default.
- W3100658422 cites W2168495929 @default.
- W3100658422 cites W2171622449 @default.
- W3100658422 cites W2179382741 @default.
- W3100658422 cites W2197026494 @default.
- W3100658422 cites W2205033212 @default.
- W3100658422 cites W2269847210 @default.
- W3100658422 cites W2341734301 @default.
- W3100658422 cites W2346478428 @default.
- W3100658422 cites W2521878568 @default.
- W3100658422 cites W2530734350 @default.
- W3100658422 cites W2950472986 @default.
- W3100658422 cites W2963226493 @default.
- W3100658422 cites W3037981304 @default.
- W3100658422 cites W3099445393 @default.
- W3100658422 cites W3099537209 @default.
- W3100658422 cites W3100106758 @default.
- W3100658422 cites W3101742051 @default.
- W3100658422 cites W3102634630 @default.
- W3100658422 cites W3103051631 @default.
- W3100658422 cites W3103448631 @default.
- W3100658422 cites W3104188978 @default.
- W3100658422 cites W3104330986 @default.
- W3100658422 cites W3105360976 @default.
- W3100658422 cites W3105546747 @default.
- W3100658422 cites W3105755493 @default.
- W3100658422 cites W3121495298 @default.
- W3100658422 cites W3124164584 @default.
- W3100658422 cites W3125409350 @default.
- W3100658422 cites W4246099101 @default.
- W3100658422 cites W4292241407 @default.
- W3100658422 cites W4293003757 @default.
- W3100658422 cites W4300793255 @default.
- W3100658422 doi "https://doi.org/10.1088/1538-3873/aa8e91" @default.
- W3100658422 hasPublicationYear "2017" @default.
- W3100658422 type Work @default.
- W3100658422 sameAs 3100658422 @default.
- W3100658422 citedByCount "12" @default.
- W3100658422 countsByYear W31006584222018 @default.
- W3100658422 countsByYear W31006584222019 @default.
- W3100658422 countsByYear W31006584222020 @default.
- W3100658422 countsByYear W31006584222021 @default.
- W3100658422 countsByYear W31006584222022 @default.
- W3100658422 countsByYear W31006584222023 @default.
- W3100658422 crossrefType "journal-article" @default.
- W3100658422 hasAuthorship W3100658422A5003976784 @default.
- W3100658422 hasAuthorship W3100658422A5011869846 @default.
- W3100658422 hasAuthorship W3100658422A5038406883 @default.
- W3100658422 hasAuthorship W3100658422A5072218639 @default.
- W3100658422 hasBestOaLocation W31006584221 @default.
- W3100658422 hasConcept C121332964 @default.
- W3100658422 hasConcept C12287442 @default.
- W3100658422 hasConcept C1276947 @default.
- W3100658422 hasConcept C135041427 @default.
- W3100658422 hasConcept C144024400 @default.