JEM-X: the x-ray monitor on INTEGRAL

Carl Budtz-Jorgensen; N. Lund; Niels J. Westergaard; S. Brandt; Allan Hornstrup; Ib Lundgaard Rasmussen; S. Laursen; S. M. Pedersen; Rene Engel Kristansen; P. B. Mogensen; K. Harpo Andersen; I. Rasmussen; Josef Polny; P. A. Jensen; C. A. Oxborrow; J. Chenevez; K. Omoe; Veikko J. Kamarainen; Tor Andersson; Osmi R. Vilhu; J. Huovelin; Enrico Costa; Marco Feroci; Alda Rubini; E. Morelli; A. Morbidini; Filippo Frontera; Carlo Pelliciari; G. Loffredo; Guido Zavattini; Vittore Carassiti; M. Morawski; G. Juchnikowski; Victor Reglero; J. Peris; V. Collado; Juana Maria Rodrigo; F. Perez; Jose-Luis Requena; S. Larsson; R. Svensson; A. Zdziarski; A. J. Castro-Tirado; Herbert W. Schnopper

doi:10.1117/12.506791

3 February 2004 JEM-X: the x-ray monitor on INTEGRAL

Carl Budtz-Jorgensen, N. Lund, Niels J. Westergaard, S. Brandt, Allan Hornstrup, Ib Lundgaard Rasmussen, S. Laursen, S. M. Pedersen, Rene Engel Kristansen, P. B. Mogensen, K. Harpo Andersen, I. Rasmussen, Josef Polny, P. A. Jensen, C. A. Oxborrow, J. Chenevez, K. Omoe, Veikko J. Kamarainen, Tor Andersson, Osmi R. Vilhu, J. Huovelin, Enrico Costa, Marco Feroci, Alda Rubini, E. Morelli, A. Morbidini, Filippo Frontera, Carlo Pelliciari, G. Loffredo, Guido Zavattini, Vittore Carassiti, M. Morawski, G. Juchnikowski, Victor Reglero, J. Peris, V. Collado, Juana Maria Rodrigo, F. Perez, Jose-Luis Requena, S. Larsson, R. Svensson, A. Zdziarski, A. J. Castro-Tirado, Herbert W. Schnopper

Author Affiliations +

Proceedings Volume 5165, X-Ray and Gamma-Ray Instrumentation for Astronomy XIII; (2004) https://doi.org/10.1117/12.506791
Event: Optical Science and Technology, SPIE's 48th Annual Meeting, 2003, San Diego, California, United States

Abstract

The INTEGRAL X-ray monitor, JEM-X, (together with the two gamma ray instruments, SPI and IBIS) provides simultaneous imaging with arcminute angular resolution in the 3-35 keV band. The good angular resolution and low energy response of JEM-X plays an important role in the detection and identification of gamma ray sources as well as in the analysis and scientific interpretation of the combined X-ray and gamma ray data. JEM-X is a coded aperture X-ray telescope consisting of two identical detectors. Each detector has a sensitive area of 500 cm², and views the sky through its own coded aperture mask. The coded masks are located 3.4 m above the detector windows. The detector field of view is constrained by X-ray collimators (6.6° FOV, FWHM).

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Carl Budtz-Jorgensen, N. Lund, Niels J. Westergaard, S. Brandt, Allan Hornstrup, Ib Lundgaard Rasmussen, S. Laursen, S. M. Pedersen, Rene Engel Kristansen, P. B. Mogensen, K. Harpo Andersen, I. Rasmussen, Josef Polny, P. A. Jensen, C. A. Oxborrow, J. Chenevez, K. Omoe, Veikko J. Kamarainen, Tor Andersson, Osmi R. Vilhu, J. Huovelin, Enrico Costa, Marco Feroci, Alda Rubini, E. Morelli, A. Morbidini, Filippo Frontera, Carlo Pelliciari, G. Loffredo, Guido Zavattini, Vittore Carassiti, M. Morawski, G. Juchnikowski, Victor Reglero, J. Peris, V. Collado, Juana Maria Rodrigo, F. Perez, Jose-Luis Requena, S. Larsson, R. Svensson, A. Zdziarski, A. J. Castro-Tirado, and Herbert W. Schnopper "JEM-X: the x-ray monitor on INTEGRAL", Proc. SPIE 5165, X-Ray and Gamma-Ray Instrumentation for Astronomy XIII, (3 February 2004); https://doi.org/10.1117/12.506791

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