Summary table |
Variable |
Value |
Source |
T0 |
20:06:56 UTC |
Swift |
ra |
147.4230° |
Swift |
decl |
71.9450° |
Swift |
pos_error |
2.33e-02° |
Swift |
fluence |
1.60e-07 erg/cm² |
Swift |
GBM_located |
False |
|
mjd |
56822.83814814815 |
Swift |
Swift table |
GRB_name |
GRB140614C |
t_trigger |
20:06:56 UTC |
ra |
147.4230° |
decl |
71.9450° |
pos_error |
2.33e-02° |
fluence |
1.60e-07 erg/cm² |
GCN 16408 table |
GRB_name |
GRB140614C |
GCN_number |
16408 |
Detection_method |
Swift-BAT Det |
ra |
147.4230° |
decl |
71.9450° |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 16408
SUBJECT: GRB 140614C found in ground analysis of BAT data
DATE: 14/06/15 14:51:46 GMT
FROM: Jay R. Cummings at NASA/GSFC/Swift
J. R. Cummings reports on behalf of the Swift-BAT team:
The IPN reported a burst at 20:06:56. It occurred near the end of a Swift
pointing on top of an approach to the SAA. No source was found onboard.
In ground analysis a significant source was found at RA, Dec 147.423, 71.945,
which is:
RA (J2000) 09h 49m 41.5s
Dec (J2000) 71d 56' 41"
with an estimated 90% uncertainty radius of 3 arcmin.
The burst was a single peak about 20 seconds long.
The spectrum during the peak 10 seconds of the burst is best fit by a
simple power law function with a photon index of 1.0 0.3. The fluence
from 15-150 keV in the 10 seconds was (1.6 0.5) x 10^-7 ergs/cm^2.
Errors quoted are 68% confidence.
A Swift TOO has been requested.
|
GCN 16410 table |
GRB_name |
GRB140614C |
GCN_number |
16410 |
Detection_method |
Swift-BAT Det |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 16410
SUBJECT: GRB 140614C: 1.23m CAHA (+EDIPO) observations
DATE: 14/06/15 23:17:26 GMT
FROM: Alberto Castro-Tirado at Inst.de Astro. de Andalucia
A. J. Castro-Tirado (IAA-CSIC, ISA-UMA), J. Gorosabel (IAA-CSIC, UPV-EHU),
S. Guziy (Univ. of Nikolaev), O. Rabaza (UGR), I. Syniavskyi, Y. Ivanov
(Kiev Main Astronomical Observatory), R. Cunniffe, A. Gonzalez-Rodriguez,
M. Jelinek, S. Jeong, O. Lara-Gil, S. R. Oates, R. Sanchez-Ramirez and J.
C. Tello (IAA-CSIC) report:
“Following the detection of GRB 140614C by Swift/BAT (Cummings et al. GCNC
16408) we obtained R-band images at the 1.23m telescope (+EDIPO) at Calar
Alto Observatory in southern Spain, starting on June 15, 20:27 UT (i.e.
24.4 hr postburst). In the coadded image (6 x 300s), we see no credible
optical candidate within the BAT error box when compared to the DSS-1 down
to R = 20.5. Further observations are ongoing.â€
|