The requirements of a gamma‐ray burst optical counterpart detector are reviewed. By taking advantage of real‐time notification of bursts, new instruments can make sensitive searches while the gamma‐ray transient is still in progress. A wide field of view camera at Livermore National Laboratories has recently been adapted for detecting GRB optical counterparts to a limiting magnitude of 8. A more sensitive camera, capable of reaching mv=14, is under development. © 1994 American Institute of Physics.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/87629/2/633_1.pd
Abstract. We are constructing a 0.6 meter telescope system to search for early time gamma-ray burstG...
We are in an exciting period of discovery for gamma-ray bursts. The Swift observatory is detecting 1...
Approximately three times per day a bright flash of high energy radiation from the depths of the uni...
GROCSE (Gamma-Ray Optical Counterpart Search Experiment) is a system of automated telescopes that se...
The GROCSE I experiment (Gamma-Ray Optical Counterpart Search Experiment) is a rapid slewing wide fi...
The Gamma-Ray Optical Counterpart Search Experiment (GROCSE) presents new experimental upper limits ...
GROCSE (Gamma-Ray Optical Counterpart Search Experiments) is a system of automated telescopes that s...
The GROCSE Collaboration (Gamma-Ray Optical Counterpart Search Experiment) has been operating a rapi...
The Robotic Optical Transient Search Experiment (ROTSE) seeks to measure contemporaneous and early a...
An overview is given of the Robotic Optical Transient Search Experiment, a ground-based observationa...
LOTIS is a gamma-ray burst optical counterpart search experiment located near Lawrence Livermore Nat...
The main scientific aim of the present GRO-proposal: Search for time-correlated optical counterparts...
This is a final report for a contract begun in Dec. 1987 and ended in Mar. 1989 to use the existing ...
We report the results of a 5 year CCD imaging program of small gamma-ray burst (GRB) error boxes fro...
The three gamma-ray burst source fields GBS1028+46, GBS1205+24, and GBS2252-03 have been monitored f...
Abstract. We are constructing a 0.6 meter telescope system to search for early time gamma-ray burstG...
We are in an exciting period of discovery for gamma-ray bursts. The Swift observatory is detecting 1...
Approximately three times per day a bright flash of high energy radiation from the depths of the uni...
GROCSE (Gamma-Ray Optical Counterpart Search Experiment) is a system of automated telescopes that se...
The GROCSE I experiment (Gamma-Ray Optical Counterpart Search Experiment) is a rapid slewing wide fi...
The Gamma-Ray Optical Counterpart Search Experiment (GROCSE) presents new experimental upper limits ...
GROCSE (Gamma-Ray Optical Counterpart Search Experiments) is a system of automated telescopes that s...
The GROCSE Collaboration (Gamma-Ray Optical Counterpart Search Experiment) has been operating a rapi...
The Robotic Optical Transient Search Experiment (ROTSE) seeks to measure contemporaneous and early a...
An overview is given of the Robotic Optical Transient Search Experiment, a ground-based observationa...
LOTIS is a gamma-ray burst optical counterpart search experiment located near Lawrence Livermore Nat...
The main scientific aim of the present GRO-proposal: Search for time-correlated optical counterparts...
This is a final report for a contract begun in Dec. 1987 and ended in Mar. 1989 to use the existing ...
We report the results of a 5 year CCD imaging program of small gamma-ray burst (GRB) error boxes fro...
The three gamma-ray burst source fields GBS1028+46, GBS1205+24, and GBS2252-03 have been monitored f...
Abstract. We are constructing a 0.6 meter telescope system to search for early time gamma-ray burstG...
We are in an exciting period of discovery for gamma-ray bursts. The Swift observatory is detecting 1...
Approximately three times per day a bright flash of high energy radiation from the depths of the uni...