Discovery of the very red near-infrared and optical afterglow of the short-duration GRB 070724A

E. Berger, S. B. Cenko, D. B. Fox, A. Cucchiara

Research output: Contribution to journalArticle

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Abstract

We report the discovery of the near-infrared and optical afterglow of the short-duration gamma-ray burst GRB070724A. The afterglow is detected in iJHKs observations starting 2.3 hr after the burst with Ks = 19.59 ± 0.16 mag and i = 23.79 ± 0.07 mag, but is absent in images obtained 1.3 yr later. Fading is also detected in the Ks band between 2.8 and 3.7 hr at a 4σ significance level. The optical/near-IR spectral index, βO,NIR ≈-2, is much redder than expected in the standard afterglow model, pointing to either significant dust extinction, A host V ≈ 2 mag, or a non-afterglow origin for the near-IR emission. The case for extinction is supported by a shallow optical to X-ray spectral index, consistent with the definition for "dark bursts," and a normal near-IR to X-ray spectral index. Moreover, a comparison to the optical discovery magnitudes of all short GRBs with optical afterglows indicates that the near-IR counterpart of GRB070724A is one of the brightest to date, while its observed optical emission is one of the faintest. In the context of a non-afterglow origin, the near-IR emission may be dominated by a mini-supernova (mini-SN), leading to an estimated ejected mass of M 10 -4 M and a radioactive energy release efficiency of f ∼ 5 × 10-3 (for v ∼ 0.3c). However, the mini-SN model predicts a spectral peak in the UV rather than near-IR, suggesting that this is either not the correct interpretation or that the mini-SN models need to be revised. Finally, the afterglow coincides with a star-forming galaxy at z = 0.457, previously identified as the host based on its coincidence with the X-ray afterglow position (2″ radius). Our discovery of the optical/near-IR afterglow makes this association secure, and furthermore localizes the burst to the outskirts of the galaxy, with an offset of 4.8 ± 0.1 kpc relative to the host center. At such a large offset, the possible large extinction points to a dusty environment local to the burst and rules out a halo or intergalactic origin.

Original languageEnglish (US)
Pages (from-to)877-882
Number of pages6
JournalAstrophysical Journal
Volume704
Issue number1
DOIs
StatePublished - Jan 1 2009

Fingerprint

afterglows
near infrared
extinction
bursts
supernovae
dust
galaxies
x rays
fading
energy
index
gamma ray bursts
light emission
halos
stars
radii

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Berger, E. ; Cenko, S. B. ; Fox, D. B. ; Cucchiara, A. / Discovery of the very red near-infrared and optical afterglow of the short-duration GRB 070724A. In: Astrophysical Journal. 2009 ; Vol. 704, No. 1. pp. 877-882.
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abstract = "We report the discovery of the near-infrared and optical afterglow of the short-duration gamma-ray burst GRB070724A. The afterglow is detected in iJHKs observations starting 2.3 hr after the burst with Ks = 19.59 ± 0.16 mag and i = 23.79 ± 0.07 mag, but is absent in images obtained 1.3 yr later. Fading is also detected in the Ks band between 2.8 and 3.7 hr at a 4σ significance level. The optical/near-IR spectral index, βO,NIR ≈-2, is much redder than expected in the standard afterglow model, pointing to either significant dust extinction, A host V ≈ 2 mag, or a non-afterglow origin for the near-IR emission. The case for extinction is supported by a shallow optical to X-ray spectral index, consistent with the definition for {"}dark bursts,{"} and a normal near-IR to X-ray spectral index. Moreover, a comparison to the optical discovery magnitudes of all short GRBs with optical afterglows indicates that the near-IR counterpart of GRB070724A is one of the brightest to date, while its observed optical emission is one of the faintest. In the context of a non-afterglow origin, the near-IR emission may be dominated by a mini-supernova (mini-SN), leading to an estimated ejected mass of M 10 -4 M and a radioactive energy release efficiency of f ∼ 5 × 10-3 (for v ∼ 0.3c). However, the mini-SN model predicts a spectral peak in the UV rather than near-IR, suggesting that this is either not the correct interpretation or that the mini-SN models need to be revised. Finally, the afterglow coincides with a star-forming galaxy at z = 0.457, previously identified as the host based on its coincidence with the X-ray afterglow position (2″ radius). Our discovery of the optical/near-IR afterglow makes this association secure, and furthermore localizes the burst to the outskirts of the galaxy, with an offset of 4.8 ± 0.1 kpc relative to the host center. At such a large offset, the possible large extinction points to a dusty environment local to the burst and rules out a halo or intergalactic origin.",
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Discovery of the very red near-infrared and optical afterglow of the short-duration GRB 070724A. / Berger, E.; Cenko, S. B.; Fox, D. B.; Cucchiara, A.

In: Astrophysical Journal, Vol. 704, No. 1, 01.01.2009, p. 877-882.

Research output: Contribution to journalArticle

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T1 - Discovery of the very red near-infrared and optical afterglow of the short-duration GRB 070724A

AU - Berger, E.

AU - Cenko, S. B.

AU - Fox, D. B.

AU - Cucchiara, A.

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N2 - We report the discovery of the near-infrared and optical afterglow of the short-duration gamma-ray burst GRB070724A. The afterglow is detected in iJHKs observations starting 2.3 hr after the burst with Ks = 19.59 ± 0.16 mag and i = 23.79 ± 0.07 mag, but is absent in images obtained 1.3 yr later. Fading is also detected in the Ks band between 2.8 and 3.7 hr at a 4σ significance level. The optical/near-IR spectral index, βO,NIR ≈-2, is much redder than expected in the standard afterglow model, pointing to either significant dust extinction, A host V ≈ 2 mag, or a non-afterglow origin for the near-IR emission. The case for extinction is supported by a shallow optical to X-ray spectral index, consistent with the definition for "dark bursts," and a normal near-IR to X-ray spectral index. Moreover, a comparison to the optical discovery magnitudes of all short GRBs with optical afterglows indicates that the near-IR counterpart of GRB070724A is one of the brightest to date, while its observed optical emission is one of the faintest. In the context of a non-afterglow origin, the near-IR emission may be dominated by a mini-supernova (mini-SN), leading to an estimated ejected mass of M 10 -4 M and a radioactive energy release efficiency of f ∼ 5 × 10-3 (for v ∼ 0.3c). However, the mini-SN model predicts a spectral peak in the UV rather than near-IR, suggesting that this is either not the correct interpretation or that the mini-SN models need to be revised. Finally, the afterglow coincides with a star-forming galaxy at z = 0.457, previously identified as the host based on its coincidence with the X-ray afterglow position (2″ radius). Our discovery of the optical/near-IR afterglow makes this association secure, and furthermore localizes the burst to the outskirts of the galaxy, with an offset of 4.8 ± 0.1 kpc relative to the host center. At such a large offset, the possible large extinction points to a dusty environment local to the burst and rules out a halo or intergalactic origin.

AB - We report the discovery of the near-infrared and optical afterglow of the short-duration gamma-ray burst GRB070724A. The afterglow is detected in iJHKs observations starting 2.3 hr after the burst with Ks = 19.59 ± 0.16 mag and i = 23.79 ± 0.07 mag, but is absent in images obtained 1.3 yr later. Fading is also detected in the Ks band between 2.8 and 3.7 hr at a 4σ significance level. The optical/near-IR spectral index, βO,NIR ≈-2, is much redder than expected in the standard afterglow model, pointing to either significant dust extinction, A host V ≈ 2 mag, or a non-afterglow origin for the near-IR emission. The case for extinction is supported by a shallow optical to X-ray spectral index, consistent with the definition for "dark bursts," and a normal near-IR to X-ray spectral index. Moreover, a comparison to the optical discovery magnitudes of all short GRBs with optical afterglows indicates that the near-IR counterpart of GRB070724A is one of the brightest to date, while its observed optical emission is one of the faintest. In the context of a non-afterglow origin, the near-IR emission may be dominated by a mini-supernova (mini-SN), leading to an estimated ejected mass of M 10 -4 M and a radioactive energy release efficiency of f ∼ 5 × 10-3 (for v ∼ 0.3c). However, the mini-SN model predicts a spectral peak in the UV rather than near-IR, suggesting that this is either not the correct interpretation or that the mini-SN models need to be revised. Finally, the afterglow coincides with a star-forming galaxy at z = 0.457, previously identified as the host based on its coincidence with the X-ray afterglow position (2″ radius). Our discovery of the optical/near-IR afterglow makes this association secure, and furthermore localizes the burst to the outskirts of the galaxy, with an offset of 4.8 ± 0.1 kpc relative to the host center. At such a large offset, the possible large extinction points to a dusty environment local to the burst and rules out a halo or intergalactic origin.

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