The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed mission to conduct an all-sky imaging hard x-ray (HX) survey (~5–600 keV) with ~0.05mCrab sensitivity (5σ; 6mo.; ~5–100keV) comparable to the ROSAT soft x-ray survey, and to provide the maximum sensitivity and resolution (spatial and temporal) HX imager as the Next Generation GRB mission. Its primary science goals are to i) identify and measure obscured AGN and constrain the accretion luminosity of the universe as well as the cosmic IR background from Blazar spectra coincident with GeV-TeV observations, ii) measure spectra, variability and locations for the faintest GRBs to study the most energetic events in the universe and the earliest epoch of star formation, and iii) ...
A next generation Gamma Ray Burst (GRB) mission to follow the upcoming Swift mission is described. T...
Abstract. The Energetic X-ray Timing Survey Telescope (EXIST) mission concept is under study as the ...
With its large collection area, broad-band energy coverage from optical/NIR (0.3 to 2.2 µm) to soft/...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed mission to conduct an all-sky ima...
A deep all-sky imaging hard x-ray survey and wide-field monitor is needed to extend soft (ROSAT) and...
A deep all-sky imaging hard x-ray survey and wide-field monitor is needed to extend soft (ROSAT) and...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed very large area coded aperture te...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed very large area coded aperture te...
We describe the Energetic X-ray Imaging Survey Telescope EXIST, designed to carry out a sensitive al...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed very large area coded aperture te...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a sensitive, wide field of view hard X-ray (...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a sensitive, wide field of view hard X-ray (...
We have begun to study a mission to carry out the first high sensitivity imaging survey of the entir...
A next generation Gamma Ray Burst (GRB) mission to follow the upcoming Swift mission is described. T...
A next generation Gamma Ray Burst (GRB) mission to follow the upcoming Swift mission is described. T...
A next generation Gamma Ray Burst (GRB) mission to follow the upcoming Swift mission is described. T...
Abstract. The Energetic X-ray Timing Survey Telescope (EXIST) mission concept is under study as the ...
With its large collection area, broad-band energy coverage from optical/NIR (0.3 to 2.2 µm) to soft/...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed mission to conduct an all-sky ima...
A deep all-sky imaging hard x-ray survey and wide-field monitor is needed to extend soft (ROSAT) and...
A deep all-sky imaging hard x-ray survey and wide-field monitor is needed to extend soft (ROSAT) and...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed very large area coded aperture te...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed very large area coded aperture te...
We describe the Energetic X-ray Imaging Survey Telescope EXIST, designed to carry out a sensitive al...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a proposed very large area coded aperture te...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a sensitive, wide field of view hard X-ray (...
The Energetic X-ray Imaging Survey Telescope (EXIST) is a sensitive, wide field of view hard X-ray (...
We have begun to study a mission to carry out the first high sensitivity imaging survey of the entir...
A next generation Gamma Ray Burst (GRB) mission to follow the upcoming Swift mission is described. T...
A next generation Gamma Ray Burst (GRB) mission to follow the upcoming Swift mission is described. T...
A next generation Gamma Ray Burst (GRB) mission to follow the upcoming Swift mission is described. T...
Abstract. The Energetic X-ray Timing Survey Telescope (EXIST) mission concept is under study as the ...
With its large collection area, broad-band energy coverage from optical/NIR (0.3 to 2.2 µm) to soft/...