The wide field monitor and spectrometer instrument on board the ASTENA satellite mission concept
Date Issued
2018
Author(s)
•
•
•
•
•
•
•
Virgilli, E.
•
Rosati, P.
•
Frontera, F.
Abstract
The ASTENA mission concept under study in the framework of the H2020 AHEAD project includes a wide field monitor and spectrometer (WFM/S), mainly dedicated to GRBs. The instrument, composed by different units, is sensitive in the range 1 keV - 20 MeV. The total isotropic detection area will be 3.0 m2 with a FOV of about 1.35 sr. The WFM will allow the detection and spectroscopic and polarimetric characterization of all classes of GRBs. Each module is a coded mask telescope that will allow the source localization within few arcmin up to 50-100 keV. The detector core is based on the coupling of low-noise, solid-state Silicon Drift Detectors (SDDs) with CsI(Tl) scintillator bars. Low-energy and highenergy photons are discriminated using the on-board electronics. The instrument design and preliminary experimental characterizations are reported and discussed.
Coverage
Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
All editors
den Herder, Jan-Willem A.; Nikzad, Shouleh; Nakazawa, Kazuhiro
Series
Volume
10699
Start page
106995Z
Conferenece
Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
Conferenece place
Austin, Texas, United States
Conferenece date
10-15 June, 2018
Issn Identifier
0277-786X
Ads BibCode
2018SPIE10699E..5ZF
Rights
open.access
File(s)![Thumbnail Image]()
Loading...
Name
106995Z.pdf
Description
Pdf editoriale
Size
951.8 KB
Format
Adobe PDF
Checksum (MD5)
d2d75aef9d72c9e9aca8280cc62549f9