GRB 060614
Time: 12:43:49
Trigger Number: 214805
Burst Advocate: Ann Parsons
BAT Data:
| RA: a | 320.877 21:23:30.5 |
| Dec: a | -53.027 -53:01:37.2 |
| 90% Error Radius: b | 1.0 |
| T90: c | 108.700 |
| Fluence: d | 204.00 (3.63) |
| 1s Peak Photon Flux: e | 11.50 (0.74) |
| Photon Index: f | 2.02, PL (0.04) |
90% error in parentheses,
a J2000;
b arcmin;
c seconds;
d 10-7 erg/cm2 (15-150 keV);
e ph/cm2/sec (15-150 keV);
f PL = simple power-law, CPL = cutoff power-law (15-150 keV)
BAT Light Curve:
XRT Data:
| RA: a | 21:23:32.12 |
| Dec: a | -53:01:36.6 |
| 90% Error Radius: b | 1.4 |
| Time to First Observation: c | 91.40 |
| Early Flux: d | 6000 |
| 11 Hour Flux: d | 0.550962 |
| 24 Hour Flux: d | 0.20174922 |
| Initial Temporal Index: | 1.5 |
| Spectral Index (Gamma): | 1.89544 |
| Column Density (NH): e | 0.325209 |
Note: Please be aware that only the very basic temporal and spectral quantities are reported here. You are strongly encouraged to see the referenced GCN circulars for full details.
a J2000;
b arcsec;
c seconds;
d 10-11 erg/cm2/s (0.3-10 keV);
e 1021 cm-2
» XRT GRB Live Catalogue
» XRT Light Curves
» XRT Spectra
UVOT Data:
| RA: a | 21:23:32.08 |
| Dec: a | -53:01:36.2 |
| 90% Error Radius: b | 0.56 |
| Time to First Observation: c | 101 |
| V Magnitude: | V=19.54 |
| Other Filter Magnitudes: | B=19.91 U=18.81 UVW1=18.35 UVM2=18.06 UVW2=18.26 White=18.30 |
a J2000; b arcsec; c seconds
Other Burst Info:
Redshift:0.13 (Gemini: emission)Host Galaxy:
0.125 (VLT: emission)
R-band (Danish 1.54m)Other Observatory Detections:
I = 21.9 (SMARTS)
Watcher (0.4m), Siding Spring Observatory (1m), CTIO (1.3m), VLT-UT1, Konus-Wind, VLT-UT2, La Silla (Danish 1.54m), Gemini South
Comments:
UVOT: possible, late-time rebrightening
References:
BAT: GCN 5252; GCN 5256; GCN 5262; arXiv:0707.4626
XRT: GCN 5252; GCN 5254; GCN 5262; Evans et al., 2009, MNRAS, 397, 1177
UVOT: GCN 5252; GCN 5255; GCN 5262; GCN 5281; GCN 5286
Radio:
Redshift: GCN 5275 (Gemini); GCN 5276 (VLT)
Host: GCN 5277 (Danish 1.54m); GCN 5282 (SMARTS)
Other: