We have developed a design for a hard X-ray polarimeter operating in the energy range from 50 to 500 keV. This modular design, known as GRAPE (Gamma-Ray Polarimeter Experiment), has been successfully demonstrated in the lab using partially polarized gamma-ray sources and using fully polarized photon beams at Argonne National Laboratory. In June of 2007, a GRAPE engineering model, consisting of a single detector module, was flown on a high altitude balloon flight to further demonstrate the design and to collect background data. We are currently preparing a much larger balloon payload for a flight in the fall of 2011. Using a large (16-element) array of detector modules, this payload is being designed to search for polarization from known poi...
We present a concept for an imaging gamma-ray polarimeter operating from ~50 MeV to ~1 GeV. Such an ...
Currently, it is widely recognised that a measurement of the polarization status of cosmic sources ...
Polarimetry provides insights into the emission mechanisms of astrophysical sources by elucidating t...
The Gamma RAy Polarimeter Experiment (GRAPE) was first flown on a 26-hour balloon flight in the fall...
The Gamma-RAy Polarimeter Experiment (GRAPE) is a concept for an astronomical hard X-ray Compton pol...
We have developed a modular design for a hard X-ray and soft gamma-ray polrimeter that we call GRAPE...
This paper discusses the latest progress in the development of GRAPE (Gamma‐Ray Polarimeter Experime...
This paper discusses the latest progress in the development of GRAPE (Gamma-Ray Polarimeter Experime...
The measurement of hard X‐ray polarization in γ‐ray bursts (GRBs) would add yet another piece of inf...
We report on the development of a dedicated polarimeter design that is capable of studying the linea...
— This paper discusses the latest progress in the development of GRAPE (Gamma-Ray Polarimeter Experi...
This dissertation describes the development of the Gamma Ray Polarimeter Experiment (GRAPE), which i...
Abstract This paper reviews the development status of GRAPE (the Gamma-Ray Polarimeter Experiment), ...
The study of the polarization properties of the gamma‐ray bursts is the one remaining unexplored ave...
The Gamma-RAy Polarimeter Experiment (GRAPE) is a concept for an astronomical hard X-ray Compton pol...
We present a concept for an imaging gamma-ray polarimeter operating from ~50 MeV to ~1 GeV. Such an ...
Currently, it is widely recognised that a measurement of the polarization status of cosmic sources ...
Polarimetry provides insights into the emission mechanisms of astrophysical sources by elucidating t...
The Gamma RAy Polarimeter Experiment (GRAPE) was first flown on a 26-hour balloon flight in the fall...
The Gamma-RAy Polarimeter Experiment (GRAPE) is a concept for an astronomical hard X-ray Compton pol...
We have developed a modular design for a hard X-ray and soft gamma-ray polrimeter that we call GRAPE...
This paper discusses the latest progress in the development of GRAPE (Gamma‐Ray Polarimeter Experime...
This paper discusses the latest progress in the development of GRAPE (Gamma-Ray Polarimeter Experime...
The measurement of hard X‐ray polarization in γ‐ray bursts (GRBs) would add yet another piece of inf...
We report on the development of a dedicated polarimeter design that is capable of studying the linea...
— This paper discusses the latest progress in the development of GRAPE (Gamma-Ray Polarimeter Experi...
This dissertation describes the development of the Gamma Ray Polarimeter Experiment (GRAPE), which i...
Abstract This paper reviews the development status of GRAPE (the Gamma-Ray Polarimeter Experiment), ...
The study of the polarization properties of the gamma‐ray bursts is the one remaining unexplored ave...
The Gamma-RAy Polarimeter Experiment (GRAPE) is a concept for an astronomical hard X-ray Compton pol...
We present a concept for an imaging gamma-ray polarimeter operating from ~50 MeV to ~1 GeV. Such an ...
Currently, it is widely recognised that a measurement of the polarization status of cosmic sources ...
Polarimetry provides insights into the emission mechanisms of astrophysical sources by elucidating t...