Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity

Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contrad...
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Autor*in:	Arkhangelskaja, I. V. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Schlagwörter:	Uniform Sample Optical Range Standard Candle Lensing Effect Redshift Distribution

Übergeordnetes Werk:	Enthalten in: Bulletin of the Russian Academy of Sciences - New York, NY : Allerton Press, 2007, 79(2015), 3 vom: März, Seite 413-416
Übergeordnetes Werk:	volume:79 ; year:2015 ; number:3 ; month:03 ; pages:413-416

Links:	Volltext

DOI / URN:	10.3103/S1062873815030089

Katalog-ID:	SPR023173726

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520			\|a Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines.
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912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_120
912			\|a GBV_ILN_138
912			\|a GBV_ILN_150
912			\|a GBV_ILN_151
912			\|a GBV_ILN_152
912			\|a GBV_ILN_161
912			\|a GBV_ILN_170
912			\|a GBV_ILN_171
912			\|a GBV_ILN_187
912			\|a GBV_ILN_213
912			\|a GBV_ILN_224
912			\|a GBV_ILN_230
912			\|a GBV_ILN_250
912			\|a GBV_ILN_281
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_636
912			\|a GBV_ILN_702
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912			\|a GBV_ILN_2007
912			\|a GBV_ILN_2008
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allfields	10.3103/S1062873815030089 doi (DE-627)SPR023173726 (SPR)S1062873815030089-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Arkhangelskaja, I. V. verfasserin aut Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines. Uniform Sample (dpeaa)DE-He213 Optical Range (dpeaa)DE-He213 Standard Candle (dpeaa)DE-He213 Lensing Effect (dpeaa)DE-He213 Redshift Distribution (dpeaa)DE-He213 Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 413-416 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:413-416 https://dx.doi.org/10.3103/S1062873815030089 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 413-416
spelling	10.3103/S1062873815030089 doi (DE-627)SPR023173726 (SPR)S1062873815030089-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Arkhangelskaja, I. V. verfasserin aut Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines. Uniform Sample (dpeaa)DE-He213 Optical Range (dpeaa)DE-He213 Standard Candle (dpeaa)DE-He213 Lensing Effect (dpeaa)DE-He213 Redshift Distribution (dpeaa)DE-He213 Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 413-416 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:413-416 https://dx.doi.org/10.3103/S1062873815030089 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 413-416
allfields_unstemmed	10.3103/S1062873815030089 doi (DE-627)SPR023173726 (SPR)S1062873815030089-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Arkhangelskaja, I. V. verfasserin aut Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines. Uniform Sample (dpeaa)DE-He213 Optical Range (dpeaa)DE-He213 Standard Candle (dpeaa)DE-He213 Lensing Effect (dpeaa)DE-He213 Redshift Distribution (dpeaa)DE-He213 Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 413-416 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:413-416 https://dx.doi.org/10.3103/S1062873815030089 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 413-416
allfieldsGer	10.3103/S1062873815030089 doi (DE-627)SPR023173726 (SPR)S1062873815030089-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Arkhangelskaja, I. V. verfasserin aut Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines. Uniform Sample (dpeaa)DE-He213 Optical Range (dpeaa)DE-He213 Standard Candle (dpeaa)DE-He213 Lensing Effect (dpeaa)DE-He213 Redshift Distribution (dpeaa)DE-He213 Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 413-416 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:413-416 https://dx.doi.org/10.3103/S1062873815030089 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 413-416
allfieldsSound	10.3103/S1062873815030089 doi (DE-627)SPR023173726 (SPR)S1062873815030089-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Arkhangelskaja, I. V. verfasserin aut Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines. Uniform Sample (dpeaa)DE-He213 Optical Range (dpeaa)DE-He213 Standard Candle (dpeaa)DE-He213 Lensing Effect (dpeaa)DE-He213 Redshift Distribution (dpeaa)DE-He213 Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 413-416 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:413-416 https://dx.doi.org/10.3103/S1062873815030089 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 413-416
language	English
source	Enthalten in Bulletin of the Russian Academy of Sciences 79(2015), 3 vom: März, Seite 413-416 volume:79 year:2015 number:3 month:03 pages:413-416
sourceStr	Enthalten in Bulletin of the Russian Academy of Sciences 79(2015), 3 vom: März, Seite 413-416 volume:79 year:2015 number:3 month:03 pages:413-416
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Uniform Sample Optical Range Standard Candle Lensing Effect Redshift Distribution
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container_title	Bulletin of the Russian Academy of Sciences
authorswithroles_txt_mv	Arkhangelskaja, I. V. @@aut@@
publishDateDaySort_date	2015-03-01T00:00:00Z
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author	Arkhangelskaja, I. V.
spellingShingle	Arkhangelskaja, I. V. ddc 530 bkl 33.00 misc Uniform Sample misc Optical Range misc Standard Candle misc Lensing Effect misc Redshift Distribution Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity
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topic_title	530 ASE 33.00 bkl Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity Uniform Sample (dpeaa)DE-He213 Optical Range (dpeaa)DE-He213 Standard Candle (dpeaa)DE-He213 Lensing Effect (dpeaa)DE-He213 Redshift Distribution (dpeaa)DE-He213
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title	Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity
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title_full	Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity
author_sort	Arkhangelskaja, I. V.
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title_sort	redshift distribution of gamma-ray bursts: evidence for the long grbs sources population nonuniformity
title_auth	Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity
abstract	Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines.
abstractGer	Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines.
abstract_unstemmed	Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. Detailed investigation of the redshift distribution shows that the former has at least two maxima at the 95% significance level in contradiction with the similar distribution for uniform samples in our Metagalaxy. This pattern (demonstrating the nonuniformity of the long GRB sources population) persists even if short GRBs with durations of t90 < 2 s without redshift correction, which corresponds to the classical definition of short GRB events, are excluded from consideration and if the analysis uses any sample of a smaller size for previous years. Preliminary investigation of the GRBs distribution on redshift and duration also reveals another subgroup that can be interpreted as intermediate GRB events. This subgroup persists if the analysis is confined to the distribution of those GRBs whose redshifts z are determined using one method only, e.g., from analyzing afterglow absorption lines.
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title_short	Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity
url	https://dx.doi.org/10.3103/S1062873815030089
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doi_str	10.3103/S1062873815030089
up_date	2024-07-03T17:20:14.446Z
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V.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The results of redshifts distribution investigation for 275 γ-ray bursts (GRBs) with defined duration from the Swift experiment catalogue are discussed. 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Redshift distribution of gamma-ray bursts: Evidence for the long GRBs sources population nonuniformity

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