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Proceedings Paper

A detector system for SPIDR, A mission to perform spectroscopy and photometry of the IGM's diffuse radiation
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Paper Abstract

The primary goal of the Spectroscopy and Photometry of the IGM's Diffuse Radiation (SPIDR) Mission is to detect and map the huge filamentary structures, the "cosmic web", predicted to be present in the IGM. The SPIDR instrument comprises six imaging spectrographs providing 8° x 8° and 2.5° x 2.5° high-resolution spatial maps of IGM features in the OVI and CIV wavelength bands. For simplicity and economy all six spectrographs utilize virtually identical detector systems. Each detector records a two-dimensional image whose axes represent spectral and one-dimensional spatial information, the second spatial axis being obtained by tomographic reconstruction. We describe the design of the prototype detector built for the SPIDR mission. The detector uses a conventional microchannel plate (MCP) arrangement with a charge division readout anode used in the image charge configuration. The image charge technique provides enhanced resolution, linearity and stability in a more compact mechanical design. The predictable distribution of the induced image charge footprint has allowed us to accurately simulate the readout performance in software. The conservative requirements of the SPIDR spectrograph allow the use of a conventional wedge and strip anode which benefits from the design improvements generated using our software simulation. Redesign of the boundary electrodes has enabled us to improve overall linearity and increase useful imaging area. We describe the integrated electronics system for the SPIDR prototype, designed for low mass and power consumption. A single printed circuit board is used to house analog signal processing, digital processing, and power systems.

Paper Details

Date Published: 24 February 2003
PDF: 9 pages
Proc. SPIE 4854, Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation, (24 February 2003); doi: 10.1117/12.459828
Show Author Affiliations
Jonathan S. Lapington, Boston Univ. (United States)
Supriya Chakrabarti, Boston Univ. (United States)
Timothy A. Cook, Boston Univ. (United States)
Robert F. Goeke, Massachusetts Institute of Technology (United States)
J. C. Gsell, Boston Univ. (United States)
V. T. Gsell, Boston Univ. (United States)

Published in SPIE Proceedings Vol. 4854:
Future EUV/UV and Visible Space Astrophysics Missions and Instrumentation
J. Chris Blades; Oswald H. W. Siegmund, Editor(s)

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