[vsnet-grb-info 13090] Skynet/GORT observations of GRB130420A

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Sun Apr 21 07:28:13 JST 2013


TITLE:   GCN CIRCULAR
NUMBER:  14427
SUBJECT: Skynet/GORT observations of GRB130420A
DATE:    13/04/20 22:28:05 GMT
FROM:    Adam S. Trotter at UNC-Chapel Hill/NC AnTPROMPT/Skynet  <atrotter at physics.unc.edu>

A. Trotter, N. Frank, A. LaCluyze, D. Reichart, K. McLin,  L. Cominsky, 
T. Berger, J. A. Crain, H. T. Cromartie,  R. Egger, A. Foster, J. 
Haislip, K. Ivarsen, M. Maples, J. Moore,   M. Nysewander, and E. 
Speckhard report:

Skynet observed the Swift/BAT localization of GRB 130420A (Page et al., 
GCN 14406, Swift trigger 553977) with the 14" GLAST Optical Robotic 
Telescope (GORT) at the Hume observatory in California, beginning ~100s 
after the trigger in RcIc, and continuing until the source set at 
t=4.9h. We detect the afterglow reported by Guidorzi et al. (GCN 14405) 
at RA 13:04:06.6, Dec +59:25:25.2 (J2000), within the error circle 
reported by the Swift XRT (GCN 14406). Photometry was calibrated to six 
SDSS stars in the field.
The afterglow exhibits a rising light curve in both Rc and Ic bands at 
early times, peaking at t=330s (peak Rc~16, Ic~15.5), after which it 
fades with an approximate temporal index alpha~-1.  There is some 
evidence for flattening of the Ic-band light curve at t>1h, at which 
time Ic~18.7.

Follow-up observations at GORT have been scheduled.

A preliminary light curve of the first night's data can be found at: 
http://skynet.unc.edu/grb/grb130420a.png


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