Carl Budtz-Jørgensen,N. Lund,N. J. Westergaard,Søren Krinstian Brandt,Allan Hornstrup,I. L. Rasmussen,S. Laursen,Søren Møller Pedersen,Rene E. Kristansen,P. B. Mögensen,Kimberly Andersen,I. L. Rasmussen,Josef Polny,P Anker Jensen,Carol Anne Oxborrow,J. Chenevez,K. Omø,Veikko J. Kamarainen,Tor Andersson,Osmi R. Vilhu
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).