GRB 070714B
 | |
| Event type | Gamma-ray burst |
|---|---|
| Date | c. 7.4 billion years ago (detected 14 July 2007, 4:59 UTC) |
| Duration | 3 seconds |
| Instrument | Swift |
| Constellation | Taurus |
| Right ascension | 03h 51m 22.29s |
| Declination | +28° 17′ 52.2″ |
| Distance | c. 7.4 billion ly |
| Redshift | 0.92 |
| Total energy output | 1.2×1051 ergs |
| Other designations | GRB 070714B |
[edit on Wikidata] | |
GRB 070714B was a gamma-ray burst (GRB) that was detected on 14 July 2007 at 4:59 UTC. A gamma-ray burst is a highly luminous flash associated with an explosion in a distant galaxy and producing gamma rays, the most energetic form of electromagnetic radiation, and often followed by a longer-lived "afterglow" emitted at longer wavelengths (X-ray, ultraviolet, optical, infrared, and radio).
At a total duration of only 3 seconds, GRB 070714B was classified as a short burst, a subclass of GRBs which is believed to be caused by the merger of two neutron stars. GRB 070714B had a redshift of z = 0.92, corresponding to a distance of about 7.4 billion light years, making it the most distant short burst detected as of 2007.
Observations
GRB 070714B was detected by the Swift satellite on 14 July 2007 at 04:59 UTC. The burst lasted only 3 seconds and reached its peak intensity 0.2 seconds after the initial detection.[1] The optical afterglow was detected by the Liverpool Telescope[2] and the William Herschel Telescope.[3]
Distance record
Spectroscopy of the optical afterglow and the burst's host galaxy revealed a single emission line of oxygen at a redshift of z = 0.92.[4] This corresponds to a distance of 7.4 billion light years, making it the oldest and most distant short burst ever detected.[5] The previous record holder had been GRB 051221A at a redshift of z = 0.546.[4][6] At a redshift of z = 0.92, the total energy released by GRB 070714B (assuming isotropic emission) was approximately 1.2×1051 ergs, which is several orders of magnitude higher than short-duration bursts with a redshift less than z = 0.5, but still significantly smaller than typical long-duration bursts.[7]
Notes
- ^ Barthelmy, Scott (14 July 2007). "GRB 070714: Swift detection of a bright burst, possibly short". GCN Circulars. 6620: 1. Bibcode:2007GCN..6620....1R.
- ^ Melandri, Andrea (14 July 2007). "GRB 070714 : Liverpool Telescope optical counterpart?". GCN Circulars. 6621: 1. Bibcode:2007GCN..6621....1M.
- ^ Levan, Andrew (14 July 2007). "GRB 070714B: confirmation of optical afterglow". GCN Circulars. 6630: 1.
- ^ a b Graham, J. F.; et al. (3 June 2009). "GRB 070714B—Discovery of the Highest Spectroscopically Confirmed Short Burst Redshift". The Astrophysical Journal. 698 (2): 1620–1629. arXiv:0808.2610. Bibcode:2009ApJ...698.1620G. doi:10.1088/0004-637X/698/2/1620.
- ^ Naeye, Robert (8 January 2008). "NASA and Gemini Probe Mysterious Distant Explosion". NASA Goddard Space Flight Center. Retrieved 14 July 2010.
- ^ Soderberg, A. M.; et al. (10 October 2006). "The Afterglow, Energetics, and Host Galaxy of the Short-Hard Gamma-Ray Burst 051221a". The Astrophysical Journal. 650 (1): 261–271. arXiv:astro-ph/0601455. Bibcode:2006ApJ...650..261S. doi:10.1086/506429.
- ^ Cenko, S. Bradley; et al. (7 February 2008). "GRBs 070429B and 070714B: The High End of the Short-Duration Gamma-Ray Burst Redshift Distribution". The Astrophysical Journal. arXiv:0802.0874. Bibcode:2008arXiv0802.0874C.
