Swift panchromatic observations of the bright gamma-ray burst GRB 050525a

A. J. Blustin, D. Band, S. Barthelmy, P. Boyd, M. Capalbi, S. T. Holland, F. E. Marshall, K. O. Mason, M. Perri, T. Poole, P. Roming, S. Rosen, P. Schady, M. Still, B. Zhang, L. Angelini, L. Barbier, A. Beardmore, A. Breeveld, D. N. Burrows & 45 others J. R. Cummings, J. Canizzo, S. Campana, M. M. Chester, G. Chincarini, L. R. Cominsky, A. Cucchiara, M. De Pasquale, E. E. Fenimore, N. Gehrels, P. Giommi, M. Goad, C. Gronwall, D. Grupe, J. E. Hill, D. Hinshaw, S. Hunsberger, K. C. Hurley, M. Ivanushkina, J. A. Kennea, H. A. Krimm, P. Kumar, W. Landsman, V. La Parola, C. B. Markwardt, K. McGowan, P. Mészáros, T. Mineo, A. Moretti, A. Morgan, J. Nousek, P. T. O'Brien, J. P. Osborne, K. Page, M. J. Page, D. M. Palmer, A. M. Parsons, J. Rhoads, P. Romano, T. Sakamoto, G. Sato, G. Tagliaferri, J. Tueller, A. A. Wells, N. E. White

Research output: Contribution to journalArticle

101 Citations (Scopus)

Abstract

The bright gamma-ray burst GRB 050525a has been detected with the Swift observatory, providing unique multi-wavelength coverage from the very earliest phases of the burst. The X-ray and optical/UV afterglow decay light curves both exhibit a steeper slope ∼0.15 days after the burst, indicative of a jet break. This jet break time combined with the total gamma-ray energy of the burst constrains the opening angle of the jet to be 3°.2. We derive an empirical "time-lag" redshift from the BAT data of ẑ = 0.69 ± 0.02, in good agreement with the spectroscopic redshift of 0.61. Prior to the jet break, the X-ray data can be modeled by a simple power law with index α = -1.2. However, after 300 s the X-ray flux brightens by about 30% compared to the power-law fit. The optical/UV data have a more complex decay, with evidence of a rapidly falling reverse shock component that dominates in the first minute or so, giving way to a flatter forward shock component at later times. The multiwavelength X-ray/UV/optical spectrum of the afterglow shows evidence for migration of the electron cooling frequency through the optical range within 25,000 s. The measured temporal decay and spectral indexes in the X-ray and optical/UV regimes compare favorably with the standard fireball model for gamma-ray bursts assuming expansion into a constant-density interstellar medium.

Original languageEnglish
Pages (from-to)901-913
Number of pages13
JournalAstrophysical Journal
Volume637
Issue number2 I
DOIs
Publication statusPublished - 2006 Feb 1

Fingerprint

gamma ray bursts
bursts
afterglows
x rays
Swift observatory
power law
decay
shock
fireballs
falling
light curve
optical spectrum
time lag
observatory
gamma rays
slopes
cooling
wavelength
electron
expansion

Keywords

  • Astrometry
  • Galaxies: distances and redshifts
  • Gamma rays: bursts
  • Shock waves
  • X-rays: individual (GRB 050525a)

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Blustin, A. J., Band, D., Barthelmy, S., Boyd, P., Capalbi, M., Holland, S. T., ... White, N. E. (2006). Swift panchromatic observations of the bright gamma-ray burst GRB 050525a. Astrophysical Journal, 637(2 I), 901-913. https://doi.org/10.1086/498425

Swift panchromatic observations of the bright gamma-ray burst GRB 050525a. / Blustin, A. J.; Band, D.; Barthelmy, S.; Boyd, P.; Capalbi, M.; Holland, S. T.; Marshall, F. E.; Mason, K. O.; Perri, M.; Poole, T.; Roming, P.; Rosen, S.; Schady, P.; Still, M.; Zhang, B.; Angelini, L.; Barbier, L.; Beardmore, A.; Breeveld, A.; Burrows, D. N.; Cummings, J. R.; Canizzo, J.; Campana, S.; Chester, M. M.; Chincarini, G.; Cominsky, L. R.; Cucchiara, A.; De Pasquale, M.; Fenimore, E. E.; Gehrels, N.; Giommi, P.; Goad, M.; Gronwall, C.; Grupe, D.; Hill, J. E.; Hinshaw, D.; Hunsberger, S.; Hurley, K. C.; Ivanushkina, M.; Kennea, J. A.; Krimm, H. A.; Kumar, P.; Landsman, W.; La Parola, V.; Markwardt, C. B.; McGowan, K.; Mészáros, P.; Mineo, T.; Moretti, A.; Morgan, A.; Nousek, J.; O'Brien, P. T.; Osborne, J. P.; Page, K.; Page, M. J.; Palmer, D. M.; Parsons, A. M.; Rhoads, J.; Romano, P.; Sakamoto, T.; Sato, G.; Tagliaferri, G.; Tueller, J.; Wells, A. A.; White, N. E.

In: Astrophysical Journal, Vol. 637, No. 2 I, 01.02.2006, p. 901-913.

Research output: Contribution to journalArticle

Blustin, AJ, Band, D, Barthelmy, S, Boyd, P, Capalbi, M, Holland, ST, Marshall, FE, Mason, KO, Perri, M, Poole, T, Roming, P, Rosen, S, Schady, P, Still, M, Zhang, B, Angelini, L, Barbier, L, Beardmore, A, Breeveld, A, Burrows, DN, Cummings, JR, Canizzo, J, Campana, S, Chester, MM, Chincarini, G, Cominsky, LR, Cucchiara, A, De Pasquale, M, Fenimore, EE, Gehrels, N, Giommi, P, Goad, M, Gronwall, C, Grupe, D, Hill, JE, Hinshaw, D, Hunsberger, S, Hurley, KC, Ivanushkina, M, Kennea, JA, Krimm, HA, Kumar, P, Landsman, W, La Parola, V, Markwardt, CB, McGowan, K, Mészáros, P, Mineo, T, Moretti, A, Morgan, A, Nousek, J, O'Brien, PT, Osborne, JP, Page, K, Page, MJ, Palmer, DM, Parsons, AM, Rhoads, J, Romano, P, Sakamoto, T, Sato, G, Tagliaferri, G, Tueller, J, Wells, AA & White, NE 2006, 'Swift panchromatic observations of the bright gamma-ray burst GRB 050525a', Astrophysical Journal, vol. 637, no. 2 I, pp. 901-913. https://doi.org/10.1086/498425
Blustin AJ, Band D, Barthelmy S, Boyd P, Capalbi M, Holland ST et al. Swift panchromatic observations of the bright gamma-ray burst GRB 050525a. Astrophysical Journal. 2006 Feb 1;637(2 I):901-913. https://doi.org/10.1086/498425
Blustin, A. J. ; Band, D. ; Barthelmy, S. ; Boyd, P. ; Capalbi, M. ; Holland, S. T. ; Marshall, F. E. ; Mason, K. O. ; Perri, M. ; Poole, T. ; Roming, P. ; Rosen, S. ; Schady, P. ; Still, M. ; Zhang, B. ; Angelini, L. ; Barbier, L. ; Beardmore, A. ; Breeveld, A. ; Burrows, D. N. ; Cummings, J. R. ; Canizzo, J. ; Campana, S. ; Chester, M. M. ; Chincarini, G. ; Cominsky, L. R. ; Cucchiara, A. ; De Pasquale, M. ; Fenimore, E. E. ; Gehrels, N. ; Giommi, P. ; Goad, M. ; Gronwall, C. ; Grupe, D. ; Hill, J. E. ; Hinshaw, D. ; Hunsberger, S. ; Hurley, K. C. ; Ivanushkina, M. ; Kennea, J. A. ; Krimm, H. A. ; Kumar, P. ; Landsman, W. ; La Parola, V. ; Markwardt, C. B. ; McGowan, K. ; Mészáros, P. ; Mineo, T. ; Moretti, A. ; Morgan, A. ; Nousek, J. ; O'Brien, P. T. ; Osborne, J. P. ; Page, K. ; Page, M. J. ; Palmer, D. M. ; Parsons, A. M. ; Rhoads, J. ; Romano, P. ; Sakamoto, T. ; Sato, G. ; Tagliaferri, G. ; Tueller, J. ; Wells, A. A. ; White, N. E. / Swift panchromatic observations of the bright gamma-ray burst GRB 050525a. In: Astrophysical Journal. 2006 ; Vol. 637, No. 2 I. pp. 901-913.
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TY - JOUR

T1 - Swift panchromatic observations of the bright gamma-ray burst GRB 050525a

AU - Blustin, A. J.

AU - Band, D.

AU - Barthelmy, S.

AU - Boyd, P.

AU - Capalbi, M.

AU - Holland, S. T.

AU - Marshall, F. E.

AU - Mason, K. O.

AU - Perri, M.

AU - Poole, T.

AU - Roming, P.

AU - Rosen, S.

AU - Schady, P.

AU - Still, M.

AU - Zhang, B.

AU - Angelini, L.

AU - Barbier, L.

AU - Beardmore, A.

AU - Breeveld, A.

AU - Burrows, D. N.

AU - Cummings, J. R.

AU - Canizzo, J.

AU - Campana, S.

AU - Chester, M. M.

AU - Chincarini, G.

AU - Cominsky, L. R.

AU - Cucchiara, A.

AU - De Pasquale, M.

AU - Fenimore, E. E.

AU - Gehrels, N.

AU - Giommi, P.

AU - Goad, M.

AU - Gronwall, C.

AU - Grupe, D.

AU - Hill, J. E.

AU - Hinshaw, D.

AU - Hunsberger, S.

AU - Hurley, K. C.

AU - Ivanushkina, M.

AU - Kennea, J. A.

AU - Krimm, H. A.

AU - Kumar, P.

AU - Landsman, W.

AU - La Parola, V.

AU - Markwardt, C. B.

AU - McGowan, K.

AU - Mészáros, P.

AU - Mineo, T.

AU - Moretti, A.

AU - Morgan, A.

AU - Nousek, J.

AU - O'Brien, P. T.

AU - Osborne, J. P.

AU - Page, K.

AU - Page, M. J.

AU - Palmer, D. M.

AU - Parsons, A. M.

AU - Rhoads, J.

AU - Romano, P.

AU - Sakamoto, T.

AU - Sato, G.

AU - Tagliaferri, G.

AU - Tueller, J.

AU - Wells, A. A.

AU - White, N. E.

PY - 2006/2/1

Y1 - 2006/2/1

N2 - The bright gamma-ray burst GRB 050525a has been detected with the Swift observatory, providing unique multi-wavelength coverage from the very earliest phases of the burst. The X-ray and optical/UV afterglow decay light curves both exhibit a steeper slope ∼0.15 days after the burst, indicative of a jet break. This jet break time combined with the total gamma-ray energy of the burst constrains the opening angle of the jet to be 3°.2. We derive an empirical "time-lag" redshift from the BAT data of ẑ = 0.69 ± 0.02, in good agreement with the spectroscopic redshift of 0.61. Prior to the jet break, the X-ray data can be modeled by a simple power law with index α = -1.2. However, after 300 s the X-ray flux brightens by about 30% compared to the power-law fit. The optical/UV data have a more complex decay, with evidence of a rapidly falling reverse shock component that dominates in the first minute or so, giving way to a flatter forward shock component at later times. The multiwavelength X-ray/UV/optical spectrum of the afterglow shows evidence for migration of the electron cooling frequency through the optical range within 25,000 s. The measured temporal decay and spectral indexes in the X-ray and optical/UV regimes compare favorably with the standard fireball model for gamma-ray bursts assuming expansion into a constant-density interstellar medium.

AB - The bright gamma-ray burst GRB 050525a has been detected with the Swift observatory, providing unique multi-wavelength coverage from the very earliest phases of the burst. The X-ray and optical/UV afterglow decay light curves both exhibit a steeper slope ∼0.15 days after the burst, indicative of a jet break. This jet break time combined with the total gamma-ray energy of the burst constrains the opening angle of the jet to be 3°.2. We derive an empirical "time-lag" redshift from the BAT data of ẑ = 0.69 ± 0.02, in good agreement with the spectroscopic redshift of 0.61. Prior to the jet break, the X-ray data can be modeled by a simple power law with index α = -1.2. However, after 300 s the X-ray flux brightens by about 30% compared to the power-law fit. The optical/UV data have a more complex decay, with evidence of a rapidly falling reverse shock component that dominates in the first minute or so, giving way to a flatter forward shock component at later times. The multiwavelength X-ray/UV/optical spectrum of the afterglow shows evidence for migration of the electron cooling frequency through the optical range within 25,000 s. The measured temporal decay and spectral indexes in the X-ray and optical/UV regimes compare favorably with the standard fireball model for gamma-ray bursts assuming expansion into a constant-density interstellar medium.

KW - Astrometry

KW - Galaxies: distances and redshifts

KW - Gamma rays: bursts

KW - Shock waves

KW - X-rays: individual (GRB 050525a)

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