New Constraints on Simultaneous Optical Emission From GRBs Measured by the LOTIS Experiment
H. S. Park, G. G. Williams, E. Ables, D. L. Band, S. D. Barthelmy, R. Bionta, P. S. Butterworth, T. L. Cline, D. H. Ferguson, G. J. Fishman, N. Gehrels, D. Hartmann, K. Hurley, C. Kouveliotou, C. A. Meegan, L. Ott, E. Parker, R. Wurtz
Abstract
LOTIS is a gamma-ray burst optical counterpart search experiment located near Lawrence Livermore National Laboratory in California. Since operations began in October 1996, LOTIS has responded to five triggers as of July 30, 1997, which occurred during good weather conditions. GRB970223 (BATSE Trigger #6100) was an exceptionally strong burst lasting 30 s with a peak at 8 s. LOTIS began imaging the error box 11 s after the burst began, and achieved simultaneous optical coverage of 100% of the region enclosed by the BATSE 3σ error circle and the IPN annulus. No optical transients were observed brighter than the mV 11 completeness limit of the resulting images providing a new upper limit on the simultaneous optical to gamma-ray fluence ratio of RL < 1.1 × 10-4 and on the simultaneous optical (at 700 nm) to gamma-ray (at 100 keV) flux density ratio of RF < 305 for a B type spectrum and RF < 475 for an M type spectrum.
Create a lesson
Related papers
On binary pulsars and the force of gravity
Davor Palle
Tidal torques. A critical review of some techniques
Michael Efroimsky, James G. Williams
Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
Rodrigo Fernández, Christopher Thompson
Asymptotically FRW black holes
J. T. Firouzjaee, Reza Mansouri
Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger
Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic et al.
A Gamma-Ray Burst/Pulsar for Cosmic-Ray Positrons with a Dark Matter-like Spectrum
Kunihito Ioka