The short GRB 051210 observed by Swift

V. La Parola; V. Mangano; B. Zhang; G. Cusumano; T. Mineo; E. Troja; D. N. Burrows; S. Campana; M. Capalbi; G. Chincarini; P. Giommi; A. Moretti; M. Perri; P. Romano; G. Tagliaferri

doi:10.1393/ncb/i2007-10299-4

The short GRB 051210 observed by Swift

V. La Parola, V. Mangano, B. Zhang, G. Cusumano, T. Mineo, E. Troja, D. N. Burrows, S. Campana, M. Capalbi, G. Chincarini, P. Giommi, A. Moretti, M. Perri, P. Romano, G. Tagliaferri

Astronomy & Astrophysics

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

1 Scopus citations

Abstract

We report on the short GRB 051210 detected by the Swift-BAT. The light curve, on which we focus mainly, shows a hint of extended emission in the BAT energy range, a steep decay of the X-ray emission, without any flattening or break, and two small flares in the first 300 s. The emission fades out after ∼ 1000 s.

Original language	English (US)
Pages (from-to)	1505-1506
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/i2007-10299-4
State	Published - Dec 2006

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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10.1393/ncb/i2007-10299-4

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title = "The short GRB 051210 observed by Swift",

abstract = "We report on the short GRB 051210 detected by the Swift-BAT. The light curve, on which we focus mainly, shows a hint of extended emission in the BAT energy range, a steep decay of the X-ray emission, without any flattening or break, and two small flares in the first 300 s. The emission fades out after ∼ 1000 s.",

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T1 - The short GRB 051210 observed by Swift

AU - La Parola, V.

AU - Mangano, V.

AU - Zhang, B.

AU - Cusumano, G.

AU - Mineo, T.

AU - Troja, E.

AU - Burrows, D. N.

AU - Campana, S.

AU - Capalbi, M.

AU - Chincarini, G.

AU - Giommi, P.

AU - Moretti, A.

AU - Perri, M.

AU - Romano, P.

AU - Tagliaferri, G.

PY - 2006/12

Y1 - 2006/12

N2 - We report on the short GRB 051210 detected by the Swift-BAT. The light curve, on which we focus mainly, shows a hint of extended emission in the BAT energy range, a steep decay of the X-ray emission, without any flattening or break, and two small flares in the first 300 s. The emission fades out after ∼ 1000 s.

AB - We report on the short GRB 051210 detected by the Swift-BAT. The light curve, on which we focus mainly, shows a hint of extended emission in the BAT energy range, a steep decay of the X-ray emission, without any flattening or break, and two small flares in the first 300 s. The emission fades out after ∼ 1000 s.

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U2 - 10.1393/ncb/i2007-10299-4

DO - 10.1393/ncb/i2007-10299-4

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SN - 1594-9982

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EP - 1506

JO - Nuovo Cimento della Societa Italiana di Fisica B

JF - Nuovo Cimento della Societa Italiana di Fisica B

IS - 12

ER -

The short GRB 051210 observed by Swift

Abstract

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