GROCSE (Gamma-Ray Optical Counterpart Search Experiments) is a system of automated telescopes that search for simultaneous optical activity associated with gamma ray bursts in response to real-time burst notifications provided by the BATSE/BACODINE network. The first generation system, GROCSE 1, is sensitive down to Mv {approximately} 8.5 and requires an average of 12 seconds to obtain the first images of the gamma ray burst error box defined by the BACODINE trigger. The collaboration is now constructing a second generation system which has a 4 second slewing time and can reach Mv {approximately} 14 with a 5 second exposure. GROCSE 2 consists of 4 cameras on a single mount. Each camera views the night sky through a commercial Canon lens (f/...
LOTIS (Livermore Optical Transient Imaging System) is a gamma-ray burst optical couterpart search ex...
Abstract: The study of cosmic gamma ray bursts (GRBs) is one of the main goals of the Lomonosov spac...
A brief overview is given of the three phases of our Gamma Ray Observatory (GRO) optical monitoring ...
GROCSE (Gamma-Ray Optical Counterpart Search Experiment) is a system of automated telescopes that se...
The GROCSE Collaboration (Gamma-Ray Optical Counterpart Search Experiment) has been operating a rapi...
The GROCSE I experiment (Gamma-Ray Optical Counterpart Search Experiment) is a rapid slewing wide fi...
The requirements of a gamma‐ray burst optical counterpart detector are reviewed. By taking advantage...
The Gamma-Ray Optical Counterpart Search Experiment (GROCSE) presents new experimental upper limits ...
The main scientific aim of the present GRO-proposal: Search for time-correlated optical counterparts...
Abstract. We are constructing a 0.6 meter telescope system to search for early time gamma-ray burstG...
We report on two alternative simple methods to detect counterparts of cosmic gamma-ray bursts (GRBs)...
schanne @ hep.saclay.cea.fr Preliminary version prior to conference Abstract: Gamma-ray bursts (GRB)...
I report on the results of six studies related to identifying low-energy counterparts of gamma-ray b...
This is a final report for a contract begun in Dec. 1987 and ended in Mar. 1989 to use the existing ...
Gamma-ray bursts (GRBs), are variable bursts of gamma-ray radiation, that lasts from milliseconds to...
LOTIS (Livermore Optical Transient Imaging System) is a gamma-ray burst optical couterpart search ex...
Abstract: The study of cosmic gamma ray bursts (GRBs) is one of the main goals of the Lomonosov spac...
A brief overview is given of the three phases of our Gamma Ray Observatory (GRO) optical monitoring ...
GROCSE (Gamma-Ray Optical Counterpart Search Experiment) is a system of automated telescopes that se...
The GROCSE Collaboration (Gamma-Ray Optical Counterpart Search Experiment) has been operating a rapi...
The GROCSE I experiment (Gamma-Ray Optical Counterpart Search Experiment) is a rapid slewing wide fi...
The requirements of a gamma‐ray burst optical counterpart detector are reviewed. By taking advantage...
The Gamma-Ray Optical Counterpart Search Experiment (GROCSE) presents new experimental upper limits ...
The main scientific aim of the present GRO-proposal: Search for time-correlated optical counterparts...
Abstract. We are constructing a 0.6 meter telescope system to search for early time gamma-ray burstG...
We report on two alternative simple methods to detect counterparts of cosmic gamma-ray bursts (GRBs)...
schanne @ hep.saclay.cea.fr Preliminary version prior to conference Abstract: Gamma-ray bursts (GRB)...
I report on the results of six studies related to identifying low-energy counterparts of gamma-ray b...
This is a final report for a contract begun in Dec. 1987 and ended in Mar. 1989 to use the existing ...
Gamma-ray bursts (GRBs), are variable bursts of gamma-ray radiation, that lasts from milliseconds to...
LOTIS (Livermore Optical Transient Imaging System) is a gamma-ray burst optical couterpart search ex...
Abstract: The study of cosmic gamma ray bursts (GRBs) is one of the main goals of the Lomonosov spac...
A brief overview is given of the three phases of our Gamma Ray Observatory (GRO) optical monitoring ...