GRB 050904: The oldest cosmic explosion ever observed in the Universe

G. Cusumano; V. Mangano; G. Chincarini; A. Panaitescu; D. N. Burrows; V. La Parola; T. Sakamoto; S. Campana; T. Mineo; G. Tagliaferri; L. Angelini; S. D. Barthelemy; A. P. Beardmore; P. T. Boyd; L. R. Cominsky; C. Gronwall; E. E. Fenimore; N. Gehrels; P. Giommi; M. Goad; K. Hurley; J. A. Kennea; K. O. Mason; F. Marshall; P. Mèszàros; J. A. Nousek; J. P. Osborne; D. M. Palmer; P. W.A. Roming; A. Wells; N. E. White; B. Zhang

doi:10.1063/1.2207955

GRB 050904: The oldest cosmic explosion ever observed in the Universe

G. Cusumano
, V. Mangano
, G. Chincarini
, A. Panaitescu
, D. N. Burrows
, V. La Parola
, T. Sakamoto
, S. Campana
, T. Mineo
, G. Tagliaferri
, L. Angelini
, S. D. Barthelemy
, A. P. Beardmore
, P. T. Boyd
, L. R. Cominsky
, C. Gronwall
, E. E. Fenimore
, N. Gehrels
, P. Giommi
, M. Goad

K. Hurley, J. A. Kennea, K. O. Mason, F. Marshall, P. Mèszàros, J. A. Nousek, J. P. Osborne, D. M. Palmer, P. W.A. Roming, A. Wells, N. E. White, B. Zhang

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

1 Scopus citations

Abstract

Swift discovered the high redshift (z=6.29) GRB 050904 with the Burst Alert Telescope and began observing with its narrow field instruments only 161 s after the burst onset. GRB 050904 was a long, multi-peaked, bright GRB with a presence of flaring activity lasting up to 1-2 hours after the burst onset. The spectral energy distribution shows a clear softening trend along the burst evolution with a photon index decreasing from -1.2 up to -1.9. The observed variability is more dramatic than the typical Swift afterglow, the amplitude and rise/fall times of the flares are consistent with the behavior of nearby (z ≤ 1) long GRBs and suggest the interpretation of the BAT and XRT data as a single continuous observation of long lasting prompt emission.

Original language	English (US)
Title of host publication	GAMMA-RAY BURSTS IN THE SWIFT ERA
Subtitle of host publication	Sixteenth Maryland Astrophysics Conference
Pages	564-569
Number of pages	6
DOIs	https://doi.org/10.1063/1.2207955
State	Published - May 19 2006
Event	GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference - Washington, D.C., United States Duration: Nov 29 2005 → Dec 2 2005

Publication series

Name	AIP Conference Proceedings
Volume	836
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

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

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

Access to Document

10.1063/1.2207955

Cite this

Cusumano, G., Mangano, V., Chincarini, G., Panaitescu, A., Burrows, D. N., La Parola, V., Sakamoto, T., Campana, S., Mineo, T., Tagliaferri, G., Angelini, L., Barthelemy, S. D., Beardmore, A. P., Boyd, P. T., Cominsky, L. R., Gronwall, C., Fenimore, E. E., Gehrels, N., Giommi, P., ... Zhang, B. (2006). GRB 050904: The oldest cosmic explosion ever observed in the Universe. In GAMMA-RAY BURSTS IN THE SWIFT ERA: Sixteenth Maryland Astrophysics Conference (pp. 564-569). (AIP Conference Proceedings; Vol. 836). https://doi.org/10.1063/1.2207955

@inproceedings{a28af6fba9ca46b79195ce281c8a5aea,

title = "GRB 050904: The oldest cosmic explosion ever observed in the Universe",

abstract = "Swift discovered the high redshift (z=6.29) GRB 050904 with the Burst Alert Telescope and began observing with its narrow field instruments only 161 s after the burst onset. GRB 050904 was a long, multi-peaked, bright GRB with a presence of flaring activity lasting up to 1-2 hours after the burst onset. The spectral energy distribution shows a clear softening trend along the burst evolution with a photon index decreasing from -1.2 up to -1.9. The observed variability is more dramatic than the typical Swift afterglow, the amplitude and rise/fall times of the flares are consistent with the behavior of nearby (z ≤ 1) long GRBs and suggest the interpretation of the BAT and XRT data as a single continuous observation of long lasting prompt emission.",

author = "G. Cusumano and V. Mangano and G. Chincarini and A. Panaitescu and Burrows, \{D. N.\} and \{La Parola\}, V. and T. Sakamoto and S. Campana and T. Mineo and G. Tagliaferri and L. Angelini and Barthelemy, \{S. D.\} and Beardmore, \{A. P.\} and Boyd, \{P. T.\} and Cominsky, \{L. R.\} and C. Gronwall and Fenimore, \{E. E.\} and N. Gehrels and P. Giommi and M. Goad and K. Hurley and Kennea, \{J. A.\} and Mason, \{K. O.\} and F. Marshall and P. M{\`e}sz{\`a}ros and Nousek, \{J. A.\} and Osborne, \{J. P.\} and Palmer, \{D. M.\} and Roming, \{P. W.A.\} and A. Wells and White, \{N. E.\} and B. Zhang",

year = "2006",

month = may,

day = "19",

doi = "10.1063/1.2207955",

language = "English (US)",

isbn = "0735403260",

series = "AIP Conference Proceedings",

pages = "564--569",

booktitle = "GAMMA-RAY BURSTS IN THE SWIFT ERA",

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

}

Cusumano, G, Mangano, V, Chincarini, G, Panaitescu, A, Burrows, DN, La Parola, V, Sakamoto, T, Campana, S, Mineo, T, Tagliaferri, G, Angelini, L, Barthelemy, SD, Beardmore, AP, Boyd, PT, Cominsky, LR, Gronwall, C, Fenimore, EE, Gehrels, N, Giommi, P, Goad, M, Hurley, K, Kennea, JA, Mason, KO, Marshall, F, Mèszàros, P, Nousek, JA, Osborne, JP, Palmer, DM, Roming, PWA, Wells, A, White, NE & Zhang, B 2006, GRB 050904: The oldest cosmic explosion ever observed in the Universe. in GAMMA-RAY BURSTS IN THE SWIFT ERA: Sixteenth Maryland Astrophysics Conference. AIP Conference Proceedings, vol. 836, pp. 564-569, GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference, Washington, D.C., United States, 11/29/05. https://doi.org/10.1063/1.2207955

TY - GEN

T1 - GRB 050904

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

AU - Cusumano, G.

AU - Mangano, V.

AU - Chincarini, G.

AU - Panaitescu, A.

AU - Burrows, D. N.

AU - La Parola, V.

AU - Sakamoto, T.

AU - Campana, S.

AU - Mineo, T.

AU - Tagliaferri, G.

AU - Angelini, L.

AU - Barthelemy, S. D.

AU - Beardmore, A. P.

AU - Boyd, P. T.

AU - Cominsky, L. R.

AU - Gronwall, C.

AU - Fenimore, E. E.

AU - Gehrels, N.

AU - Giommi, P.

AU - Goad, M.

AU - Hurley, K.

AU - Kennea, J. A.

AU - Mason, K. O.

AU - Marshall, F.

AU - Mèszàros, P.

AU - Nousek, J. A.

AU - Osborne, J. P.

AU - Palmer, D. M.

AU - Roming, P. W.A.

AU - Wells, A.

AU - White, N. E.

AU - Zhang, B.

PY - 2006/5/19

Y1 - 2006/5/19

N2 - Swift discovered the high redshift (z=6.29) GRB 050904 with the Burst Alert Telescope and began observing with its narrow field instruments only 161 s after the burst onset. GRB 050904 was a long, multi-peaked, bright GRB with a presence of flaring activity lasting up to 1-2 hours after the burst onset. The spectral energy distribution shows a clear softening trend along the burst evolution with a photon index decreasing from -1.2 up to -1.9. The observed variability is more dramatic than the typical Swift afterglow, the amplitude and rise/fall times of the flares are consistent with the behavior of nearby (z ≤ 1) long GRBs and suggest the interpretation of the BAT and XRT data as a single continuous observation of long lasting prompt emission.

AB - Swift discovered the high redshift (z=6.29) GRB 050904 with the Burst Alert Telescope and began observing with its narrow field instruments only 161 s after the burst onset. GRB 050904 was a long, multi-peaked, bright GRB with a presence of flaring activity lasting up to 1-2 hours after the burst onset. The spectral energy distribution shows a clear softening trend along the burst evolution with a photon index decreasing from -1.2 up to -1.9. The observed variability is more dramatic than the typical Swift afterglow, the amplitude and rise/fall times of the flares are consistent with the behavior of nearby (z ≤ 1) long GRBs and suggest the interpretation of the BAT and XRT data as a single continuous observation of long lasting prompt emission.

UR - https://www.scopus.com/pages/publications/33845579086

UR - https://www.scopus.com/pages/publications/33845579086#tab=citedBy

U2 - 10.1063/1.2207955

DO - 10.1063/1.2207955

M3 - Conference contribution

AN - SCOPUS:33845579086

SN - 0735403260

SN - 9780735403260

T3 - AIP Conference Proceedings

SP - 564

EP - 569

BT - GAMMA-RAY BURSTS IN THE SWIFT ERA

Y2 - 29 November 2005 through 2 December 2005

ER -

GRB 050904: The oldest cosmic explosion ever observed in the Universe

Abstract

Publication series

Other

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this