Matches in SemOpenAlex for { <https://semopenalex.org/work/W2009308093> ?p ?o ?g. }
- W2009308093 endingPage "L128" @default.
- W2009308093 startingPage "L124" @default.
- W2009308093 abstract "We present Herschel/PACS observations of the nearby (z = 0.1055) dwarf galaxy that has hosted the long gamma-ray burst (LGRB) 031203. Using the PACS data, we have been able to place constraints on the dust temperature, dust mass, total infrared (IR) luminosity and IR-derived star formation rate (SFR) for this object. We find that the GRB host galaxy (GRBH) 031203 has a total IR luminosity of 3 × 1010 L⊙ placing it in the regime of the IR-luminous galaxy population. Its dust temperature and specific SFR are comparable to that of many high-redshift (z = 0.3–2.5) IR-detected GRB hosts (Tdust > 40 K; sSFR > 10 Gyr−1); however, its dust-to-stellar mass ratio is lower than what is commonly seen in IR-luminous galaxies. Our results suggest that GRBH 031203 is undergoing a strong starburst episode and its dust properties are different to those of local dwarf galaxies within the same metallicity and stellar mass range. Furthermore, our measurements place it in a distinct class to the well-studied nearby host of GRB 980425 (z = 0.0085), confirming the notion that GRB host galaxies can span a large range in properties even at similar cosmological epochs, making LGRBs an ideal tool in selecting samples of star-forming galaxies up to high redshift." @default.
- W2009308093 created "2016-06-24" @default.
- W2009308093 creator A5000947923 @default.
- W2009308093 creator A5004498560 @default.
- W2009308093 creator A5021324146 @default.
- W2009308093 creator A5026145878 @default.
- W2009308093 creator A5035042727 @default.
- W2009308093 creator A5035843723 @default.
- W2009308093 creator A5052042810 @default.
- W2009308093 creator A5081265238 @default.
- W2009308093 creator A5083305122 @default.
- W2009308093 date "2014-07-18" @default.
- W2009308093 modified "2023-10-08" @default.
- W2009308093 title "Herschel/PACS observations of the host galaxy of GRB 031203★" @default.
- W2009308093 cites W1936271073 @default.
- W2009308093 cites W1979622417 @default.
- W2009308093 cites W1985403054 @default.
- W2009308093 cites W1990209373 @default.
- W2009308093 cites W2020250376 @default.
- W2009308093 cites W2043830471 @default.
- W2009308093 cites W2050324272 @default.
- W2009308093 cites W2052159329 @default.
- W2009308093 cites W2052937506 @default.
- W2009308093 cites W2056076677 @default.
- W2009308093 cites W2058724092 @default.
- W2009308093 cites W2072878892 @default.
- W2009308093 cites W2073868676 @default.
- W2009308093 cites W2077017611 @default.
- W2009308093 cites W2078309823 @default.
- W2009308093 cites W2103734507 @default.
- W2009308093 cites W2106748044 @default.
- W2009308093 cites W2117322039 @default.
- W2009308093 cites W2119335435 @default.
- W2009308093 cites W2120075609 @default.
- W2009308093 cites W2131911270 @default.
- W2009308093 cites W2133898867 @default.
- W2009308093 cites W2147223987 @default.
- W2009308093 cites W2167530485 @default.
- W2009308093 cites W2168971251 @default.
- W2009308093 cites W2949965626 @default.
- W2009308093 cites W3099575410 @default.
- W2009308093 cites W3100106758 @default.
- W2009308093 cites W3100768343 @default.
- W2009308093 cites W3101953018 @default.
- W2009308093 cites W3103913301 @default.
- W2009308093 cites W3104124612 @default.
- W2009308093 cites W3105233603 @default.
- W2009308093 cites W3106004780 @default.
- W2009308093 cites W3125611252 @default.
- W2009308093 cites W4293003757 @default.
- W2009308093 cites W4298841527 @default.
- W2009308093 cites W4300386627 @default.
- W2009308093 cites W4300932849 @default.
- W2009308093 doi "https://doi.org/10.1093/mnrasl/slu090" @default.
- W2009308093 hasPublicationYear "2014" @default.
- W2009308093 type Work @default.
- W2009308093 sameAs 2009308093 @default.
- W2009308093 citedByCount "10" @default.
- W2009308093 countsByYear W20093080932014 @default.
- W2009308093 countsByYear W20093080932015 @default.
- W2009308093 countsByYear W20093080932018 @default.
- W2009308093 countsByYear W20093080932020 @default.
- W2009308093 crossrefType "journal-article" @default.
- W2009308093 hasAuthorship W2009308093A5000947923 @default.
- W2009308093 hasAuthorship W2009308093A5004498560 @default.
- W2009308093 hasAuthorship W2009308093A5021324146 @default.
- W2009308093 hasAuthorship W2009308093A5026145878 @default.
- W2009308093 hasAuthorship W2009308093A5035042727 @default.
- W2009308093 hasAuthorship W2009308093A5035843723 @default.
- W2009308093 hasAuthorship W2009308093A5052042810 @default.
- W2009308093 hasAuthorship W2009308093A5081265238 @default.
- W2009308093 hasAuthorship W2009308093A5083305122 @default.
- W2009308093 hasBestOaLocation W20093080931 @default.
- W2009308093 hasConcept C121332964 @default.
- W2009308093 hasConcept C12287442 @default.
- W2009308093 hasConcept C125857072 @default.
- W2009308093 hasConcept C1276947 @default.
- W2009308093 hasConcept C144024400 @default.
- W2009308093 hasConcept C149923435 @default.
- W2009308093 hasConcept C168589115 @default.
- W2009308093 hasConcept C17599544 @default.
- W2009308093 hasConcept C2908647359 @default.
- W2009308093 hasConcept C33024259 @default.
- W2009308093 hasConcept C37119246 @default.
- W2009308093 hasConcept C44870925 @default.
- W2009308093 hasConcept C98444146 @default.
- W2009308093 hasConcept C99465377 @default.
- W2009308093 hasConceptScore W2009308093C121332964 @default.
- W2009308093 hasConceptScore W2009308093C12287442 @default.
- W2009308093 hasConceptScore W2009308093C125857072 @default.
- W2009308093 hasConceptScore W2009308093C1276947 @default.
- W2009308093 hasConceptScore W2009308093C144024400 @default.
- W2009308093 hasConceptScore W2009308093C149923435 @default.
- W2009308093 hasConceptScore W2009308093C168589115 @default.
- W2009308093 hasConceptScore W2009308093C17599544 @default.
- W2009308093 hasConceptScore W2009308093C2908647359 @default.
- W2009308093 hasConceptScore W2009308093C33024259 @default.
- W2009308093 hasConceptScore W2009308093C37119246 @default.