Swift observations of GRB050712

T. S. Poole; M. De Pasquale; D. Grupe; A. A. Breeveld; S. Zane; S. R. Rosen; M. J. Page; K. O. Mason; D. N. Burrows; H. A. Krimm; N. Gehrels; J. A. Nousek; P. W.A. Roming; S. Kobayashi; B. Zhang

doi:10.1393/ncb/i2007-10321-y

Swift observations of GRB050712

T. S. Poole, M. De Pasquale, D. Grupe, A. A. Breeveld, S. Zane, S. R. Rosen, M. J. Page, K. O. Mason, D. N. Burrows, H. A. Krimm, N. Gehrels, J. A. Nousek, P. W.A. Roming, S. Kobayashi, B. Zhang

Astronomy & Astrophysics

Research output: Contribution to journal › Article › peer-review

Abstract

Swift observations of GRB050712 show that the X-ray light curve of this burst exhibits flaring activity in the first 500 s. We find that the initial flares can be due to "inner engine" activity, where the later flare may be explained in terms of the interaction of the ejecta with the surrounding medium. An optical counterpart was detected in the U and V band of UVOT up to 15000 s after the trigger.

Original language	English (US)
Pages (from-to)	1567-1568
Number of pages	2
Journal	Nuovo Cimento della Societa Italiana di Fisica B
Volume	121
Issue number	12
DOIs	https://doi.org/10.1393/ncb/i2007-10321-y
State	Published - Dec 2006

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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10.1393/ncb/i2007-10321-y

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title = "Swift observations of GRB050712",

abstract = "Swift observations of GRB050712 show that the X-ray light curve of this burst exhibits flaring activity in the first 500 s. We find that the initial flares can be due to {"}inner engine{"} activity, where the later flare may be explained in terms of the interaction of the ejecta with the surrounding medium. An optical counterpart was detected in the U and V band of UVOT up to 15000 s after the trigger.",

author = "Poole, {T. S.} and {De Pasquale}, M. and D. Grupe and Breeveld, {A. A.} and S. Zane and Rosen, {S. R.} and Page, {M. J.} and Mason, {K. O.} and Burrows, {D. N.} and Krimm, {H. A.} and N. Gehrels and Nousek, {J. A.} and Roming, {P. W.A.} and S. Kobayashi and B. Zhang",

year = "2006",

month = dec,

doi = "10.1393/ncb/i2007-10321-y",

language = "English (US)",

volume = "121",

pages = "1567--1568",

journal = "Nuovo Cimento della Societa Italiana di Fisica B",

issn = "1594-9982",

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TY - JOUR

T1 - Swift observations of GRB050712

AU - Poole, T. S.

AU - De Pasquale, M.

AU - Grupe, D.

AU - Breeveld, A. A.

AU - Zane, S.

AU - Rosen, S. R.

AU - Page, M. J.

AU - Mason, K. O.

AU - Burrows, D. N.

AU - Krimm, H. A.

AU - Gehrels, N.

AU - Nousek, J. A.

AU - Roming, P. W.A.

AU - Kobayashi, S.

AU - Zhang, B.

PY - 2006/12

Y1 - 2006/12

N2 - Swift observations of GRB050712 show that the X-ray light curve of this burst exhibits flaring activity in the first 500 s. We find that the initial flares can be due to "inner engine" activity, where the later flare may be explained in terms of the interaction of the ejecta with the surrounding medium. An optical counterpart was detected in the U and V band of UVOT up to 15000 s after the trigger.

AB - Swift observations of GRB050712 show that the X-ray light curve of this burst exhibits flaring activity in the first 500 s. We find that the initial flares can be due to "inner engine" activity, where the later flare may be explained in terms of the interaction of the ejecta with the surrounding medium. An optical counterpart was detected in the U and V band of UVOT up to 15000 s after the trigger.

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JF - Nuovo Cimento della Societa Italiana di Fisica B

IS - 12

ER -

Swift observations of GRB050712

Abstract

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