Add to ORKGAn astrophysics application of a low noise Double-sided Silicon Strip De-tector (DSSD) is described. A Semiconductor Multiple-Compton Telescope (SMCT) is being developed to explore the gamma-ray universe in the 0.1– 20 MeV energy band. Excellent energy resolution and polarization sensitiv-ity are key features of the SMCT. We have developed prototype modules for a low noise DSSD system, which reached an energy resolution of 1.3 keV (FWHM) for 122 keV at 0◦C. Results of a gamma-ray imaging test are also presented
While the scientific potential of high-energy X-ray and gamma-ray polarimetry has long been recogniz...
Gamma-ray observations in the low and medium energy range (0.1-100 MeV) with sufficiently sensitive ...
We describe the development and tests of the prototype for a new telescope for Medium Energy Gamma-r...
A Semiconductor Multiple-Compton Telescope (SMCT) is being developed to explore the gamma-ray univer...
Double-sided silicon strip detectors (DSSD) provide a very promising technology for constructing a C...
A Compton camera has been developed based on Si and CdTe semiconductor detectors with high spatial a...
International audienceGamma-ray astronomy in the MeV energy range shows a lack of sensitivity compar...
The Soft Gamma-ray Detector (SGD) on board the NeXT (Japanese future high energy astrophysics missio...
A future mission in medium-energy gamma-ray astrophysics would allow for many scientific advancement...
We are developing a Compton telescope based on high resolution Si and CdTe detectors for astrophysic...
The Soft Gamma-ray Detector (SGD) on board NeXT (Japanese future high energy astrophysics mission) i...
Abstract — We are developing a Compton camera based on Si and CdTe semiconductor imaging devices wit...
Abstract — We are developing a Compton camera based on Si and CdTe semiconductor imaging devices wit...
We present a concept for an imaging gamma-ray polarimeter operating from ~50 MeV to ~1 GeV. Such an ...
We have been developing a semiconductor Compton telescope to explore the universe in the energy band...
While the scientific potential of high-energy X-ray and gamma-ray polarimetry has long been recogniz...
Gamma-ray observations in the low and medium energy range (0.1-100 MeV) with sufficiently sensitive ...
We describe the development and tests of the prototype for a new telescope for Medium Energy Gamma-r...
A Semiconductor Multiple-Compton Telescope (SMCT) is being developed to explore the gamma-ray univer...
Double-sided silicon strip detectors (DSSD) provide a very promising technology for constructing a C...
A Compton camera has been developed based on Si and CdTe semiconductor detectors with high spatial a...
International audienceGamma-ray astronomy in the MeV energy range shows a lack of sensitivity compar...
The Soft Gamma-ray Detector (SGD) on board the NeXT (Japanese future high energy astrophysics missio...
A future mission in medium-energy gamma-ray astrophysics would allow for many scientific advancement...
We are developing a Compton telescope based on high resolution Si and CdTe detectors for astrophysic...
The Soft Gamma-ray Detector (SGD) on board NeXT (Japanese future high energy astrophysics mission) i...
Abstract — We are developing a Compton camera based on Si and CdTe semiconductor imaging devices wit...
Abstract — We are developing a Compton camera based on Si and CdTe semiconductor imaging devices wit...
We present a concept for an imaging gamma-ray polarimeter operating from ~50 MeV to ~1 GeV. Such an ...
We have been developing a semiconductor Compton telescope to explore the universe in the energy band...
While the scientific potential of high-energy X-ray and gamma-ray polarimetry has long been recogniz...
Gamma-ray observations in the low and medium energy range (0.1-100 MeV) with sufficiently sensitive ...
We describe the development and tests of the prototype for a new telescope for Medium Energy Gamma-r...