GRB 100814A: not optical observations, GRB Coordinates Networks, Circular Servicen
Research output: Other contribution › Research
We observed the optical afterglow of GRB 100814A (Schaefer et al., GCN
11086; Beardmore et al., GCN 11087) with the NOT equipped with ALFOSC.
Observations were carried out in the R band, with a mean time August
17.13 UT (2.97 days after the burst).
The optical afterglow is well detected, with R=19.5 compared to several
USNO stars in the field. The error is about 0.3 mag, completely due to
the scatter in the calibration stars.
11086; Beardmore et al., GCN 11087) with the NOT equipped with ALFOSC.
Observations were carried out in the R band, with a mean time August
17.13 UT (2.97 days after the burst).
The optical afterglow is well detected, with R=19.5 compared to several
USNO stars in the field. The error is about 0.3 mag, completely due to
the scatter in the calibration stars.
| Original language | English |
|---|---|
| Publication date | 17 Aug 2010 |
| Number of pages | 1 |
| Publication status | Published - 17 Aug 2010 |
| Series | GRB Coordinates Networks, Circular Service |
|---|---|
| Number | 1 |
| Volume | 11121 |
ID: 32931548