We present an R- and J-band photometry of an optical transient that is likely to be associated with the gamma-ray burst event GRB 971214. Our first measurement took place 13 hr after the gamma-ray event. The brightness decayed with a power-law exponent α = -1.20 ± 0.02, which is similar to those of GRB 970228 and GRB 970508, which had exponents of α = -1.10 ± 0.04 and α = -1.141 ± 0.014, respectively. The transient decayed monotonically during the first 4 days following the gamma-ray event in contrast with the optical transient associated with GRB 970508, which increased in brightness, peaking 2 days after the burst, before settling to a power-law decay.
|Original language||English (US)|
|Issue number||2 PART II|
|State||Published - 1998|
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
- Gamma rays: bursts