The X-ray luminosity function of short gamma-ray bursts.
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| Title: | The X-ray luminosity function of short gamma-ray bursts. |
|---|---|
| Authors: | Liu, Zhi-Ying1 (AUTHOR), Zhang, Fu-Wen1,2 (AUTHOR) fwzhang@pmo.ac.cn, Zhu, Si-Yuan1 (AUTHOR) |
| Source: | Astrophysics & Space Science. Apr2021, Vol. 366 Issue 4, p1-7. 7p. |
| Subjects: | Stellar luminosity function, Luminosity, Gamma ray bursts, X-rays |
| Abstract: | We present for the first time the X-ray luminosity function of short gamma-ray bursts (sGRBs) estimated from 22 Fermi sGRBs. We find that the cumulative distribution of X-ray emission at rest frame 200 s is well described by a broken power law function, which is ϕ (L X , 0) ∝ L X , 0 − 0.20 ± 0.04 for dim bursts and ϕ (L X , 0) ∝ L X , 0 − 1.05 ± 0.11 for bright bursts, with the break luminosity is 2.57 × 10 46 erg s − 1 , where the cosmological evolution of luminosity is taken into account. We also find that the early X-ray luminosity of sGRBs is correlated with the isotropic energy/luminosity of prompt emission. These results are need to confirm with large observed data of sGRBs. [ABSTRACT FROM AUTHOR] |
| Copyright of Astrophysics & Space Science is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
| Database: | Engineering Source |
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| Items | – Name: Title Label: Title Group: Ti Data: The X-ray luminosity function of short gamma-ray bursts. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Liu%2C+Zhi-Ying%22">Liu, Zhi-Ying</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Zhang%2C+Fu-Wen%22">Zhang, Fu-Wen</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<i> fwzhang@pmo.ac.cn</i><br /><searchLink fieldCode="AR" term="%22Zhu%2C+Si-Yuan%22">Zhu, Si-Yuan</searchLink><relatesTo>1</relatesTo> (AUTHOR) – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Astrophysics+%26+Space+Science%22">Astrophysics & Space Science</searchLink>. Apr2021, Vol. 366 Issue 4, p1-7. 7p. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Stellar+luminosity+function%22">Stellar luminosity function</searchLink><br /><searchLink fieldCode="DE" term="%22Luminosity%22">Luminosity</searchLink><br /><searchLink fieldCode="DE" term="%22Gamma+ray+bursts%22">Gamma ray bursts</searchLink><br /><searchLink fieldCode="DE" term="%22X-rays%22">X-rays</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: We present for the first time the X-ray luminosity function of short gamma-ray bursts (sGRBs) estimated from 22 Fermi sGRBs. We find that the cumulative distribution of X-ray emission at rest frame 200 s is well described by a broken power law function, which is ϕ (L X , 0) ∝ L X , 0 − 0.20 ± 0.04 for dim bursts and ϕ (L X , 0) ∝ L X , 0 − 1.05 ± 0.11 for bright bursts, with the break luminosity is 2.57 × 10 46 erg s − 1 , where the cosmological evolution of luminosity is taken into account. We also find that the early X-ray luminosity of sGRBs is correlated with the isotropic energy/luminosity of prompt emission. These results are need to confirm with large observed data of sGRBs. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Astrophysics & Space Science is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.) |
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| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1007/s10509-021-03945-3 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 7 StartPage: 1 Subjects: – SubjectFull: Stellar luminosity function Type: general – SubjectFull: Luminosity Type: general – SubjectFull: Gamma ray bursts Type: general – SubjectFull: X-rays Type: general Titles: – TitleFull: The X-ray luminosity function of short gamma-ray bursts. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Liu, Zhi-Ying – PersonEntity: Name: NameFull: Zhang, Fu-Wen – PersonEntity: Name: NameFull: Zhu, Si-Yuan IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 04 Text: Apr2021 Type: published Y: 2021 Identifiers: – Type: issn-print Value: 0004640X Numbering: – Type: volume Value: 366 – Type: issue Value: 4 Titles: – TitleFull: Astrophysics & Space Science Type: main |
| ResultId | 1 |