Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation

The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key par...
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Autor*in:	Chen Deng [verfasserIn] Yong-Feng Huang [verfasserIn] Fan Xu [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Gamma-ray bursts Magnetars Neutron stars Markov chain Monte Carlo

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 943(2023), 2, p 126
Übergeordnetes Werk:	volume:943 ; year:2023 ; number:2, p 126

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/acaefd

Katalog-ID:	DOAJ089163133

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520			\|a The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample.
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allfields	10.3847/1538-4357/acaefd doi (DE-627)DOAJ089163133 (DE-599)DOAJ6d05f1eeab794b55aa7fc06253b7c214 DE-627 ger DE-627 rakwb eng QB460-466 Chen Deng verfasserin aut Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample. Gamma-ray bursts Magnetars Neutron stars Markov chain Monte Carlo Astrophysics Yong-Feng Huang verfasserin aut Fan Xu verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 2, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:2, p 126 https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/article/6d05f1eeab794b55aa7fc06253b7c214 kostenfrei https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 2, p 126
spelling	10.3847/1538-4357/acaefd doi (DE-627)DOAJ089163133 (DE-599)DOAJ6d05f1eeab794b55aa7fc06253b7c214 DE-627 ger DE-627 rakwb eng QB460-466 Chen Deng verfasserin aut Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample. Gamma-ray bursts Magnetars Neutron stars Markov chain Monte Carlo Astrophysics Yong-Feng Huang verfasserin aut Fan Xu verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 2, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:2, p 126 https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/article/6d05f1eeab794b55aa7fc06253b7c214 kostenfrei https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 2, p 126
allfields_unstemmed	10.3847/1538-4357/acaefd doi (DE-627)DOAJ089163133 (DE-599)DOAJ6d05f1eeab794b55aa7fc06253b7c214 DE-627 ger DE-627 rakwb eng QB460-466 Chen Deng verfasserin aut Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample. Gamma-ray bursts Magnetars Neutron stars Markov chain Monte Carlo Astrophysics Yong-Feng Huang verfasserin aut Fan Xu verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 2, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:2, p 126 https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/article/6d05f1eeab794b55aa7fc06253b7c214 kostenfrei https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 2, p 126
allfieldsGer	10.3847/1538-4357/acaefd doi (DE-627)DOAJ089163133 (DE-599)DOAJ6d05f1eeab794b55aa7fc06253b7c214 DE-627 ger DE-627 rakwb eng QB460-466 Chen Deng verfasserin aut Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample. Gamma-ray bursts Magnetars Neutron stars Markov chain Monte Carlo Astrophysics Yong-Feng Huang verfasserin aut Fan Xu verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 2, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:2, p 126 https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/article/6d05f1eeab794b55aa7fc06253b7c214 kostenfrei https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 2, p 126
allfieldsSound	10.3847/1538-4357/acaefd doi (DE-627)DOAJ089163133 (DE-599)DOAJ6d05f1eeab794b55aa7fc06253b7c214 DE-627 ger DE-627 rakwb eng QB460-466 Chen Deng verfasserin aut Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample. Gamma-ray bursts Magnetars Neutron stars Markov chain Monte Carlo Astrophysics Yong-Feng Huang verfasserin aut Fan Xu verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 943(2023), 2, p 126 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:943 year:2023 number:2, p 126 https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/article/6d05f1eeab794b55aa7fc06253b7c214 kostenfrei https://doi.org/10.3847/1538-4357/acaefd kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 943 2023 2, p 126
language	English
source	In The Astrophysical Journal 943(2023), 2, p 126 volume:943 year:2023 number:2, p 126
sourceStr	In The Astrophysical Journal 943(2023), 2, p 126 volume:943 year:2023 number:2, p 126
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Gamma-ray bursts Magnetars Neutron stars Markov chain Monte Carlo Astrophysics
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container_title	The Astrophysical Journal
authorswithroles_txt_mv	Chen Deng @@aut@@ Yong-Feng Huang @@aut@@ Fan Xu @@aut@@
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callnumber-first	Q - Science
author	Chen Deng
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topic_title	QB460-466 Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation Gamma-ray bursts Magnetars Neutron stars Markov chain Monte Carlo
topic	misc QB460-466 misc Gamma-ray bursts misc Magnetars misc Neutron stars misc Markov chain Monte Carlo misc Astrophysics
topic_unstemmed	misc QB460-466 misc Gamma-ray bursts misc Magnetars misc Neutron stars misc Markov chain Monte Carlo misc Astrophysics
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title	Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation
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title_sort	pseudo-redshifts of gamma-ray bursts derived from the l–t–e correlation
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title_auth	Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation
abstract	The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample.
abstractGer	The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample.
abstract_unstemmed	The X-ray afterglow of many gamma-ray bursts (GRBs) exhibits a plateau phase before the normal power-law decay stage, which may be related to continued activities of the central engine. Tang et al. collected 174 such GRBs and confirmed the so-called L – T – E correlation which involves three key parameters, i.e., the isotropic γ -ray energy E _γ _,iso of the prompt phase, the end time T _a of the plateau phase, and the corresponding X-ray luminosity L _X . In this study, the L – T – E correlation is confirmed and updated as ${L}_{{\rm{X}}}\propto {T}_{{\rm{a}}}^{-0.99}{E}_{\gamma ,\mathrm{iso}}^{0.86}$ with a large sample consisting of 210 plateau GRBs with known redshifts. The tight correlation is then applied to derive the pseudo-redshift of other 130 plateau GRBs whose redshifts are not directly measured. Statistical analysis is also carried out on this pseudo-redshift sample.
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title_short	Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation
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score	7.401078

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Pseudo-redshifts of Gamma-Ray Bursts Derived from the L–T–E Correlation

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