GRB 071003

Broadband follow-up observations of a very bright gamma-ray burst in a galactic halo

D. A. Perley, W. Li, R. Chornock, J. X. Prochaska, N. R. Butler, P. Chandra, L. K. Pollack, J. S. Bloom, A. V. Fllippenko, H. Swan, F. Yuan, C. Akerlof, M. W. Auger, S. B. Cenko, H. W. Chen, C. D. Fassnacht, D. Fox, D. Frail, E. M. Johansson, T. McKay & 9 others D. Le Mignant, M. Modjaz, W. Rujopakarn, R. Russel, M. A. Skinner, G. H. Smith, I. Smith, M. A. Van Dam, S. Yost

    Research output: Contribution to journalArticle

    Abstract

    The optical afterglow of long-duration GRB 071003 is among the brightest yet to be detected from any GRB, with A ≈ 12 mag in KAIT observations starting 42 s after the GRB trigger, including filtered detections during prompt emission. However, our high-S/N afterglow spectrum displays only extremely weak absorption lines at what we argue is the host redshift of z = 1.60435, in contrast to the three other, much stronger Mg IT absorption systems observed at lower redshifts. Together with Keck adaptive optics observations, which fail to reveal a host galaxy coincident with the burst position, our observations suggest a halo progenitor and offer a cautionary tale about the use of Mg n for GRB redshift determination. We present early- through late-time observations spanning the electro-magnetic spectrum, constrain the connection between the prompt emission and early variations in the light curve (we observe no correlation), and discuss possible origins for an unusual, marked rebrightening that occurs a few hours after the burst: likely either a late-time refreshed shock or a wide-angle secondary jet. Analysis of the late-time afterglow is most consistent with a wind environment, suggesting a massive star progenitor. Together with GRB 070125, this may indicate that a small but significant portion of star formation in the early universe occurred far outside what we consider a normal galactic disk.

    Original languageEnglish (US)
    Pages (from-to)470-490
    Number of pages21
    JournalAstrophysical Journal
    Volume688
    Issue number1
    DOIs
    StatePublished - Nov 20 2008

    Fingerprint

    galactic halos
    gamma ray bursts
    afterglows
    broadband
    bursts
    electromagnetic spectra
    massive stars
    adaptive optics
    light curve
    star formation
    halos
    universe
    actuators
    shock
    galaxies

    Keywords

    • Gamma rays: bursts

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    Perley, D. A., Li, W., Chornock, R., Prochaska, J. X., Butler, N. R., Chandra, P., ... Yost, S. (2008). GRB 071003: Broadband follow-up observations of a very bright gamma-ray burst in a galactic halo. Astrophysical Journal, 688(1), 470-490. https://doi.org/10.1086/591961

    GRB 071003 : Broadband follow-up observations of a very bright gamma-ray burst in a galactic halo. / Perley, D. A.; Li, W.; Chornock, R.; Prochaska, J. X.; Butler, N. R.; Chandra, P.; Pollack, L. K.; Bloom, J. S.; Fllippenko, A. V.; Swan, H.; Yuan, F.; Akerlof, C.; Auger, M. W.; Cenko, S. B.; Chen, H. W.; Fassnacht, C. D.; Fox, D.; Frail, D.; Johansson, E. M.; McKay, T.; Le Mignant, D.; Modjaz, M.; Rujopakarn, W.; Russel, R.; Skinner, M. A.; Smith, G. H.; Smith, I.; Van Dam, M. A.; Yost, S.

    In: Astrophysical Journal, Vol. 688, No. 1, 20.11.2008, p. 470-490.

    Research output: Contribution to journalArticle

    Perley, DA, Li, W, Chornock, R, Prochaska, JX, Butler, NR, Chandra, P, Pollack, LK, Bloom, JS, Fllippenko, AV, Swan, H, Yuan, F, Akerlof, C, Auger, MW, Cenko, SB, Chen, HW, Fassnacht, CD, Fox, D, Frail, D, Johansson, EM, McKay, T, Le Mignant, D, Modjaz, M, Rujopakarn, W, Russel, R, Skinner, MA, Smith, GH, Smith, I, Van Dam, MA & Yost, S 2008, 'GRB 071003: Broadband follow-up observations of a very bright gamma-ray burst in a galactic halo', Astrophysical Journal, vol. 688, no. 1, pp. 470-490. https://doi.org/10.1086/591961
    Perley DA, Li W, Chornock R, Prochaska JX, Butler NR, Chandra P et al. GRB 071003: Broadband follow-up observations of a very bright gamma-ray burst in a galactic halo. Astrophysical Journal. 2008 Nov 20;688(1):470-490. https://doi.org/10.1086/591961
    Perley, D. A. ; Li, W. ; Chornock, R. ; Prochaska, J. X. ; Butler, N. R. ; Chandra, P. ; Pollack, L. K. ; Bloom, J. S. ; Fllippenko, A. V. ; Swan, H. ; Yuan, F. ; Akerlof, C. ; Auger, M. W. ; Cenko, S. B. ; Chen, H. W. ; Fassnacht, C. D. ; Fox, D. ; Frail, D. ; Johansson, E. M. ; McKay, T. ; Le Mignant, D. ; Modjaz, M. ; Rujopakarn, W. ; Russel, R. ; Skinner, M. A. ; Smith, G. H. ; Smith, I. ; Van Dam, M. A. ; Yost, S. / GRB 071003 : Broadband follow-up observations of a very bright gamma-ray burst in a galactic halo. In: Astrophysical Journal. 2008 ; Vol. 688, No. 1. pp. 470-490.
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    abstract = "The optical afterglow of long-duration GRB 071003 is among the brightest yet to be detected from any GRB, with A ≈ 12 mag in KAIT observations starting 42 s after the GRB trigger, including filtered detections during prompt emission. However, our high-S/N afterglow spectrum displays only extremely weak absorption lines at what we argue is the host redshift of z = 1.60435, in contrast to the three other, much stronger Mg IT absorption systems observed at lower redshifts. Together with Keck adaptive optics observations, which fail to reveal a host galaxy coincident with the burst position, our observations suggest a halo progenitor and offer a cautionary tale about the use of Mg n for GRB redshift determination. We present early- through late-time observations spanning the electro-magnetic spectrum, constrain the connection between the prompt emission and early variations in the light curve (we observe no correlation), and discuss possible origins for an unusual, marked rebrightening that occurs a few hours after the burst: likely either a late-time refreshed shock or a wide-angle secondary jet. Analysis of the late-time afterglow is most consistent with a wind environment, suggesting a massive star progenitor. Together with GRB 070125, this may indicate that a small but significant portion of star formation in the early universe occurred far outside what we consider a normal galactic disk.",
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    TY - JOUR

    T1 - GRB 071003

    T2 - Broadband follow-up observations of a very bright gamma-ray burst in a galactic halo

    AU - Perley, D. A.

    AU - Li, W.

    AU - Chornock, R.

    AU - Prochaska, J. X.

    AU - Butler, N. R.

    AU - Chandra, P.

    AU - Pollack, L. K.

    AU - Bloom, J. S.

    AU - Fllippenko, A. V.

    AU - Swan, H.

    AU - Yuan, F.

    AU - Akerlof, C.

    AU - Auger, M. W.

    AU - Cenko, S. B.

    AU - Chen, H. W.

    AU - Fassnacht, C. D.

    AU - Fox, D.

    AU - Frail, D.

    AU - Johansson, E. M.

    AU - McKay, T.

    AU - Le Mignant, D.

    AU - Modjaz, M.

    AU - Rujopakarn, W.

    AU - Russel, R.

    AU - Skinner, M. A.

    AU - Smith, G. H.

    AU - Smith, I.

    AU - Van Dam, M. A.

    AU - Yost, S.

    PY - 2008/11/20

    Y1 - 2008/11/20

    N2 - The optical afterglow of long-duration GRB 071003 is among the brightest yet to be detected from any GRB, with A ≈ 12 mag in KAIT observations starting 42 s after the GRB trigger, including filtered detections during prompt emission. However, our high-S/N afterglow spectrum displays only extremely weak absorption lines at what we argue is the host redshift of z = 1.60435, in contrast to the three other, much stronger Mg IT absorption systems observed at lower redshifts. Together with Keck adaptive optics observations, which fail to reveal a host galaxy coincident with the burst position, our observations suggest a halo progenitor and offer a cautionary tale about the use of Mg n for GRB redshift determination. We present early- through late-time observations spanning the electro-magnetic spectrum, constrain the connection between the prompt emission and early variations in the light curve (we observe no correlation), and discuss possible origins for an unusual, marked rebrightening that occurs a few hours after the burst: likely either a late-time refreshed shock or a wide-angle secondary jet. Analysis of the late-time afterglow is most consistent with a wind environment, suggesting a massive star progenitor. Together with GRB 070125, this may indicate that a small but significant portion of star formation in the early universe occurred far outside what we consider a normal galactic disk.

    AB - The optical afterglow of long-duration GRB 071003 is among the brightest yet to be detected from any GRB, with A ≈ 12 mag in KAIT observations starting 42 s after the GRB trigger, including filtered detections during prompt emission. However, our high-S/N afterglow spectrum displays only extremely weak absorption lines at what we argue is the host redshift of z = 1.60435, in contrast to the three other, much stronger Mg IT absorption systems observed at lower redshifts. Together with Keck adaptive optics observations, which fail to reveal a host galaxy coincident with the burst position, our observations suggest a halo progenitor and offer a cautionary tale about the use of Mg n for GRB redshift determination. We present early- through late-time observations spanning the electro-magnetic spectrum, constrain the connection between the prompt emission and early variations in the light curve (we observe no correlation), and discuss possible origins for an unusual, marked rebrightening that occurs a few hours after the burst: likely either a late-time refreshed shock or a wide-angle secondary jet. Analysis of the late-time afterglow is most consistent with a wind environment, suggesting a massive star progenitor. Together with GRB 070125, this may indicate that a small but significant portion of star formation in the early universe occurred far outside what we consider a normal galactic disk.

    KW - Gamma rays: bursts

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