Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100456603> ?p ?o ?g. }
- W3100456603 endingPage "21" @default.
- W3100456603 startingPage "21" @default.
- W3100456603 abstract "The exact relationship between the long gamma-ray burst (LGRB) rate and the cosmic star formation rate (CSFR) is essential for using LGRBs as cosmological probes. In this work, we collect a large sample composed of 371 Swift LGRBs with known redshifts and prompt emission properties. We first compare the rest-frame prompt properties of these bursts in different redshift bins, finding negligible redshift evolution of the luminosity of LGRBs with between z ∼ 1 and z ∼ 4. Then, by utilizing the CSFR obtained from the large-scale cosmological hydrodynamical simulation, the Illustris simulation, we calculate the cumulative redshift distribution of LGRBs under different metallicity thresholds. After comparing with our sample, we find that the predictions with a moderate threshold between are consistent with the sample between redshift 0 < z < 3, while at higher redshifts, between 3 < z < 5, all metallicity thresholds fit the data well. When changing to an empirical model based on observations, the predictions show similar results as well. After comparing with the metallicity distribution of the observed LGRB host galaxies between 0 < z < 1, we confirm that the production of LGRBs in galaxies with super-solar metallicity is suppressed. Nevertheless, considering that a significant fraction of stars are born in sub-solar metallicity environments at z ≳ 3, we suggest that, as a first approximation, LGRBs can be used as direct tracers of the CSFR in this redshift range." @default.
- W3100456603 created "2020-11-23" @default.
- W3100456603 creator A5001607790 @default.
- W3100456603 creator A5003680488 @default.
- W3100456603 creator A5020824627 @default.
- W3100456603 creator A5041283221 @default.
- W3100456603 creator A5052171580 @default.
- W3100456603 creator A5052598859 @default.
- W3100456603 creator A5055890975 @default.
- W3100456603 date "2020-05-15" @default.
- W3100456603 modified "2023-10-15" @default.
- W3100456603 title "Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample" @default.
- W3100456603 cites W1494146418 @default.
- W3100456603 cites W1911876284 @default.
- W3100456603 cites W1962465754 @default.
- W3100456603 cites W1975498920 @default.
- W3100456603 cites W1980277978 @default.
- W3100456603 cites W1985814919 @default.
- W3100456603 cites W1991506407 @default.
- W3100456603 cites W1992570077 @default.
- W3100456603 cites W1995594498 @default.
- W3100456603 cites W2021389441 @default.
- W3100456603 cites W2042331304 @default.
- W3100456603 cites W2042561599 @default.
- W3100456603 cites W2059302115 @default.
- W3100456603 cites W2072878892 @default.
- W3100456603 cites W2073424199 @default.
- W3100456603 cites W2074094455 @default.
- W3100456603 cites W2074259895 @default.
- W3100456603 cites W2075103542 @default.
- W3100456603 cites W2086199187 @default.
- W3100456603 cites W2089609573 @default.
- W3100456603 cites W2107002261 @default.
- W3100456603 cites W2107521467 @default.
- W3100456603 cites W2114800671 @default.
- W3100456603 cites W2117642017 @default.
- W3100456603 cites W2131661760 @default.
- W3100456603 cites W2137473859 @default.
- W3100456603 cites W2163798619 @default.
- W3100456603 cites W2204815181 @default.
- W3100456603 cites W2616150543 @default.
- W3100456603 cites W2736368318 @default.
- W3100456603 cites W2761024890 @default.
- W3100456603 cites W2951900035 @default.
- W3100456603 cites W2963487011 @default.
- W3100456603 cites W3023001381 @default.
- W3100456603 cites W3098508287 @default.
- W3100456603 cites W3098615625 @default.
- W3100456603 cites W3098870111 @default.
- W3100456603 cites W3099438994 @default.
- W3100456603 cites W3099444979 @default.
- W3100456603 cites W3099575410 @default.
- W3100456603 cites W3100136250 @default.
- W3100456603 cites W3100514957 @default.
- W3100456603 cites W3100829134 @default.
- W3100456603 cites W3101638350 @default.
- W3100456603 cites W3101917313 @default.
- W3100456603 cites W3102820987 @default.
- W3100456603 cites W3102826375 @default.
- W3100456603 cites W3102859222 @default.
- W3100456603 cites W3103788609 @default.
- W3100456603 cites W3103893093 @default.
- W3100456603 cites W3104059039 @default.
- W3100456603 cites W3104337150 @default.
- W3100456603 cites W3104728800 @default.
- W3100456603 cites W3105676301 @default.
- W3100456603 cites W3105808464 @default.
- W3100456603 cites W3106333081 @default.
- W3100456603 cites W3121472738 @default.
- W3100456603 cites W3123980727 @default.
- W3100456603 cites W3124333200 @default.
- W3100456603 cites W3125649778 @default.
- W3100456603 cites W4293166328 @default.
- W3100456603 doi "https://doi.org/10.3847/1538-4365/ab88da" @default.
- W3100456603 hasPublicationYear "2020" @default.
- W3100456603 type Work @default.
- W3100456603 sameAs 3100456603 @default.
- W3100456603 citedByCount "3" @default.
- W3100456603 countsByYear W31004566032021 @default.
- W3100456603 countsByYear W31004566032022 @default.
- W3100456603 crossrefType "journal-article" @default.
- W3100456603 hasAuthorship W3100456603A5001607790 @default.
- W3100456603 hasAuthorship W3100456603A5003680488 @default.
- W3100456603 hasAuthorship W3100456603A5020824627 @default.
- W3100456603 hasAuthorship W3100456603A5041283221 @default.
- W3100456603 hasAuthorship W3100456603A5052171580 @default.
- W3100456603 hasAuthorship W3100456603A5052598859 @default.
- W3100456603 hasAuthorship W3100456603A5055890975 @default.
- W3100456603 hasBestOaLocation W31004566031 @default.
- W3100456603 hasConcept C121332964 @default.
- W3100456603 hasConcept C12287442 @default.
- W3100456603 hasConcept C125857072 @default.
- W3100456603 hasConcept C1276947 @default.
- W3100456603 hasConcept C150846664 @default.
- W3100456603 hasConcept C17599544 @default.
- W3100456603 hasConcept C33024259 @default.
- W3100456603 hasConcept C44870925 @default.
- W3100456603 hasConcept C59375849 @default.