Correlative analysis of GRBs detected by Swift, Konus and HETE

H. A. Krimm; S. D. Barthelmy; N. Gehrels; D. Hullinger; T. Sakamoto; T. Donaghy; D. Q. Lamb; V. Pal'shin; S. Golenetskii; G. R. Ricker; J. L. Atteia; N. Kawai; G. Sato

doi:10.1063/1.2207876

Correlative analysis of GRBs detected by Swift, Konus and HETE

H. A. Krimm^*, S. D. Barthelmy, N. Gehrels, D. Hullinger, T. Sakamoto, T. Donaghy, D. Q. Lamb, V. Pal'shin, S. Golenetskii, G. R. Ricker, J. L. Atteia, N. Kawai, G. Sato

^*Corresponding author for this work

Waseda Research Institute for Science and Engineering

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

12 Citations (Scopus)

Abstract

Swift has now detected a large enough sample of gamma-ray bursts (GRBs) to allow correlation studies of burst parameters. Such studies of earlier data sets have yielded important results leading to further understanding of burst parameters and classifications. This work focusses on seventeen Swift bursts that have also been detected either by Konus-Wind or HETE-II, providing high energy spectra and fits to E_peak. Eight of these bursts have spectroscopic redshifts and for others we can estimate redshifts using the variability/luminosity relationship. We can also compare E_peak with E_iso, and for those bursts for which a jet break was observed in the afterglow we can derive Eg and test the relationship between E_peak and E_γ. For all bursts we can derive durations and hardness ratios from the prompt emission.

Original language	English
Title of host publication	AIP Conference Proceedings
Pages	145-148
Number of pages	4
Volume	836
DOIs	https://doi.org/10.1063/1.2207876
Publication status	Published - 2006 May 19
Event	GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference - Washington, D.C. Duration: 2005 Nov 29 → 2005 Dec 2

Other

Other	GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference
City	Washington, D.C.
Period	05/11/29 → 05/12/2

Keywords

Gamma-ray bursts
Gamma-ray telescopes

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1063/1.2207876

Cite this

Krimm, HA, Barthelmy, SD, Gehrels, N, Hullinger, D, Sakamoto, T, Donaghy, T, Lamb, DQ, Pal'shin, V, Golenetskii, S, Ricker, GR, Atteia, JL, Kawai, N & Sato, G 2006, Correlative analysis of GRBs detected by Swift, Konus and HETE. in AIP Conference Proceedings. vol. 836, pp. 145-148, GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference, Washington, D.C., 05/11/29. https://doi.org/10.1063/1.2207876

@inproceedings{a66943fe74c64311ad4942cf61f0499c,

title = "Correlative analysis of GRBs detected by Swift, Konus and HETE",

abstract = "Swift has now detected a large enough sample of gamma-ray bursts (GRBs) to allow correlation studies of burst parameters. Such studies of earlier data sets have yielded important results leading to further understanding of burst parameters and classifications. This work focusses on seventeen Swift bursts that have also been detected either by Konus-Wind or HETE-II, providing high energy spectra and fits to Epeak. Eight of these bursts have spectroscopic redshifts and for others we can estimate redshifts using the variability/luminosity relationship. We can also compare Epeak with Eiso, and for those bursts for which a jet break was observed in the afterglow we can derive Eg and test the relationship between Epeak and Eγ. For all bursts we can derive durations and hardness ratios from the prompt emission.",

keywords = "Gamma-ray bursts, Gamma-ray telescopes",

author = "Krimm, {H. A.} and Barthelmy, {S. D.} and N. Gehrels and D. Hullinger and T. Sakamoto and T. Donaghy and Lamb, {D. Q.} and V. Pal'shin and S. Golenetskii and Ricker, {G. R.} and Atteia, {J. L.} and N. Kawai and G. Sato",

year = "2006",

month = may,

day = "19",

doi = "10.1063/1.2207876",

language = "English",

isbn = "0735403260",

volume = "836",

pages = "145--148",

booktitle = "AIP Conference Proceedings",

note = "GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference ; Conference date: 29-11-2005 Through 02-12-2005",

}

TY - GEN

T1 - Correlative analysis of GRBs detected by Swift, Konus and HETE

AU - Krimm, H. A.

AU - Barthelmy, S. D.

AU - Gehrels, N.

AU - Hullinger, D.

AU - Sakamoto, T.

AU - Donaghy, T.

AU - Lamb, D. Q.

AU - Pal'shin, V.

AU - Golenetskii, S.

AU - Ricker, G. R.

AU - Atteia, J. L.

AU - Kawai, N.

AU - Sato, G.

PY - 2006/5/19

Y1 - 2006/5/19

N2 - Swift has now detected a large enough sample of gamma-ray bursts (GRBs) to allow correlation studies of burst parameters. Such studies of earlier data sets have yielded important results leading to further understanding of burst parameters and classifications. This work focusses on seventeen Swift bursts that have also been detected either by Konus-Wind or HETE-II, providing high energy spectra and fits to Epeak. Eight of these bursts have spectroscopic redshifts and for others we can estimate redshifts using the variability/luminosity relationship. We can also compare Epeak with Eiso, and for those bursts for which a jet break was observed in the afterglow we can derive Eg and test the relationship between Epeak and Eγ. For all bursts we can derive durations and hardness ratios from the prompt emission.

AB - Swift has now detected a large enough sample of gamma-ray bursts (GRBs) to allow correlation studies of burst parameters. Such studies of earlier data sets have yielded important results leading to further understanding of burst parameters and classifications. This work focusses on seventeen Swift bursts that have also been detected either by Konus-Wind or HETE-II, providing high energy spectra and fits to Epeak. Eight of these bursts have spectroscopic redshifts and for others we can estimate redshifts using the variability/luminosity relationship. We can also compare Epeak with Eiso, and for those bursts for which a jet break was observed in the afterglow we can derive Eg and test the relationship between Epeak and Eγ. For all bursts we can derive durations and hardness ratios from the prompt emission.

KW - Gamma-ray bursts

KW - Gamma-ray telescopes

UR - http://www.scopus.com/inward/record.url?scp=33845589763&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=33845589763&partnerID=8YFLogxK

U2 - 10.1063/1.2207876

DO - 10.1063/1.2207876

M3 - Conference contribution

AN - SCOPUS:33845589763

SN - 0735403260

SN - 9780735403260

VL - 836

SP - 145

EP - 148

BT - AIP Conference Proceedings

T2 - GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference

Y2 - 29 November 2005 through 2 December 2005

ER -

Correlative analysis of GRBs detected by Swift, Konus and HETE

Abstract

Other

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this