Joint European x-ray monitor (JEM-X): x-ray monitor for ESA's

H.W. Schnopper; C. Budtz-Joergensen; Niels Jørgen Stenfeldt Westergaard; Allan Hornstrup; V.J. Kamarainen; J. Huovelin; O. Vilhu; E. Costa; L. Piro; F. Frontera; G. Manzo; S. Giarrusso; A.J. Castro-Tirado; V. Reglero; R. Svensson; A.C. Fabian; A. Zdziarski

Joint European x-ray monitor (JEM-X): x-ray monitor for ESA's

H.W. Schnopper, C. Budtz-Joergensen, Niels Jørgen Stenfeldt Westergaard, Allan Hornstrup, V.J. Kamarainen, J. Huovelin, O. Vilhu, E. Costa, L. Piro, F. Frontera, G. Manzo, S. Giarrusso, A.J. Castro-Tirado, V. Reglero, R. Svensson, A.C. Fabian, A. Zdziarski

National Space Institute

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

Abstract

JEM-X will extend the energy range of the gamma ray instruments on ESA's INTEGRAL mission (SPI, IBIS) to include the x-ray band. JEM-X will provide images with arcminute angular resolution in the 2 - 60 keV band. The baseline photon detection system consists of two identical, high pressure, imaging microstrip gas chambers, each with a collecting area of 500 cm(superscript 2). They view the sky through a coded aperture mask (0.5 mm tungsten) at a separation of 3.4 m. The two detector boxes are formed from 2 mm thick stainless steel plate and are filled with 5 bar Xe. The field of view is defined by the collimator mounted on top of the detector. Each collimator consists of an array of bonded square tubes of Mo. The internal surface of these tubes is covered by a graded shield. The collimator provide also the support for the detector windows which are made out of 250 micrometer thick beryllium foils. The detector sensor elements consists of microstrip plates shaped as regular octagons with a diameter of 292 mm. The basic microstrip pattern is similar to the one chosen for the HEPC/LEPC detector system on SRG. The detector position resolution will be sufficient to ensure an angular resolution for JEM-X of better than 3 arcmin throughout the 2 - 60 keV band.

Original language	English
Title of host publication	Proc. SPIE : Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions
Editors	Brian D. Ramsey, Thomas A. Parnell
Volume	2806
Publication date	1996
Pages	297-307
Publication status	Published - 1996
Event	SPIE'S 1996 International Symposium on Optical Science, Engineering, and Instrumentation - Denver, United States Duration: 4 Aug 1996 → 9 Aug 1996

Conference

Conference	SPIE'S 1996 International Symposium on Optical Science, Engineering, and Instrumentation
Country	United States
City	Denver
Period	04/08/1996 → 09/08/1996

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http://adsabs.harvard.edu/abs/1996SPIE.2806..297S

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Schnopper, H. W., Budtz-Joergensen, C., Westergaard, N. J. S., Hornstrup, A., Kamarainen, V. J., Huovelin, J., Vilhu, O., Costa, E., Piro, L., Frontera, F., Manzo, G., Giarrusso, S., Castro-Tirado, A. J., Reglero, V., Svensson, R., Fabian, A. C., & Zdziarski, A. (1996). Joint European x-ray monitor (JEM-X): x-ray monitor for ESA's. In B. D. Ramsey, & T. A. Parnell (Eds.), Proc. SPIE: Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions (Vol. 2806, pp. 297-307) http://adsabs.harvard.edu/abs/1996SPIE.2806..297S

Schnopper, H.W. ; Budtz-Joergensen, C. ; Westergaard, Niels Jørgen Stenfeldt ; Hornstrup, Allan ; Kamarainen, V.J. ; Huovelin, J. ; Vilhu, O. ; Costa, E. ; Piro, L. ; Frontera, F. ; Manzo, G. ; Giarrusso, S. ; Castro-Tirado, A.J. ; Reglero, V. ; Svensson, R. ; Fabian, A.C. ; Zdziarski, A. / Joint European x-ray monitor (JEM-X): x-ray monitor for ESA's. Proc. SPIE: Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions. editor / Brian D. Ramsey ; Thomas A. Parnell. Vol. 2806 1996. pp. 297-307

@inproceedings{5c678e5ad5cc4556bfb9e62107471387,

title = "Joint European x-ray monitor (JEM-X): x-ray monitor for ESA's",

abstract = "JEM-X will extend the energy range of the gamma ray instruments on ESA's INTEGRAL mission (SPI, IBIS) to include the x-ray band. JEM-X will provide images with arcminute angular resolution in the 2 - 60 keV band. The baseline photon detection system consists of two identical, high pressure, imaging microstrip gas chambers, each with a collecting area of 500 cm(superscript 2). They view the sky through a coded aperture mask (0.5 mm tungsten) at a separation of 3.4 m. The two detector boxes are formed from 2 mm thick stainless steel plate and are filled with 5 bar Xe. The field of view is defined by the collimator mounted on top of the detector. Each collimator consists of an array of bonded square tubes of Mo. The internal surface of these tubes is covered by a graded shield. The collimator provide also the support for the detector windows which are made out of 250 micrometer thick beryllium foils. The detector sensor elements consists of microstrip plates shaped as regular octagons with a diameter of 292 mm. The basic microstrip pattern is similar to the one chosen for the HEPC/LEPC detector system on SRG. The detector position resolution will be sufficient to ensure an angular resolution for JEM-X of better than 3 arcmin throughout the 2 - 60 keV band.",

author = "H.W. Schnopper and C. Budtz-Joergensen and Westergaard, {Niels J{\o}rgen Stenfeldt} and Allan Hornstrup and V.J. Kamarainen and J. Huovelin and O. Vilhu and E. Costa and L. Piro and F. Frontera and G. Manzo and S. Giarrusso and A.J. Castro-Tirado and V. Reglero and R. Svensson and A.C. Fabian and A. Zdziarski",

year = "1996",

language = "English",

volume = "2806",

pages = "297--307",

editor = "Ramsey, {Brian D.} and Parnell, {Thomas A.}",

booktitle = "Proc. SPIE",

note = "SPIE'S 1996 International Symposium on Optical Science, Engineering, and Instrumentation ; Conference date: 04-08-1996 Through 09-08-1996",

}

Schnopper, HW, Budtz-Joergensen, C, Westergaard, NJS , Hornstrup, A, Kamarainen, VJ, Huovelin, J, Vilhu, O, Costa, E, Piro, L, Frontera, F, Manzo, G, Giarrusso, S, Castro-Tirado, AJ, Reglero, V, Svensson, R, Fabian, AC & Zdziarski, A 1996, Joint European x-ray monitor (JEM-X): x-ray monitor for ESA's. in BD Ramsey & TA Parnell (eds), Proc. SPIE: Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions. vol. 2806, pp. 297-307, SPIE'S 1996 International Symposium on Optical Science, Engineering, and Instrumentation, Denver, United States, 04/08/1996. <http://adsabs.harvard.edu/abs/1996SPIE.2806..297S>

Joint European x-ray monitor (JEM-X): x-ray monitor for ESA's. / Schnopper, H.W.; Budtz-Joergensen, C.; Westergaard, Niels Jørgen Stenfeldt ; Hornstrup, Allan; Kamarainen, V.J.; Huovelin, J.; Vilhu, O.; Costa, E.; Piro, L.; Frontera, F.; Manzo, G.; Giarrusso, S.; Castro-Tirado, A.J.; Reglero, V.; Svensson, R.; Fabian, A.C.; Zdziarski, A.

Proc. SPIE: Gamma-Ray and Cosmic-Ray Detectors, Techniques, and Missions. ed. / Brian D. Ramsey; Thomas A. Parnell. Vol. 2806 1996. p. 297-307.

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

TY - GEN

T1 - Joint European x-ray monitor (JEM-X): x-ray monitor for ESA's

AU - Schnopper, H.W.

AU - Budtz-Joergensen, C.

AU - Westergaard, Niels Jørgen Stenfeldt

AU - Hornstrup, Allan

AU - Kamarainen, V.J.

AU - Huovelin, J.

AU - Vilhu, O.

AU - Costa, E.

AU - Piro, L.

AU - Frontera, F.

AU - Manzo, G.

AU - Giarrusso, S.

AU - Castro-Tirado, A.J.

AU - Reglero, V.

AU - Svensson, R.

AU - Fabian, A.C.

AU - Zdziarski, A.

PY - 1996

Y1 - 1996

N2 - JEM-X will extend the energy range of the gamma ray instruments on ESA's INTEGRAL mission (SPI, IBIS) to include the x-ray band. JEM-X will provide images with arcminute angular resolution in the 2 - 60 keV band. The baseline photon detection system consists of two identical, high pressure, imaging microstrip gas chambers, each with a collecting area of 500 cm(superscript 2). They view the sky through a coded aperture mask (0.5 mm tungsten) at a separation of 3.4 m. The two detector boxes are formed from 2 mm thick stainless steel plate and are filled with 5 bar Xe. The field of view is defined by the collimator mounted on top of the detector. Each collimator consists of an array of bonded square tubes of Mo. The internal surface of these tubes is covered by a graded shield. The collimator provide also the support for the detector windows which are made out of 250 micrometer thick beryllium foils. The detector sensor elements consists of microstrip plates shaped as regular octagons with a diameter of 292 mm. The basic microstrip pattern is similar to the one chosen for the HEPC/LEPC detector system on SRG. The detector position resolution will be sufficient to ensure an angular resolution for JEM-X of better than 3 arcmin throughout the 2 - 60 keV band.

AB - JEM-X will extend the energy range of the gamma ray instruments on ESA's INTEGRAL mission (SPI, IBIS) to include the x-ray band. JEM-X will provide images with arcminute angular resolution in the 2 - 60 keV band. The baseline photon detection system consists of two identical, high pressure, imaging microstrip gas chambers, each with a collecting area of 500 cm(superscript 2). They view the sky through a coded aperture mask (0.5 mm tungsten) at a separation of 3.4 m. The two detector boxes are formed from 2 mm thick stainless steel plate and are filled with 5 bar Xe. The field of view is defined by the collimator mounted on top of the detector. Each collimator consists of an array of bonded square tubes of Mo. The internal surface of these tubes is covered by a graded shield. The collimator provide also the support for the detector windows which are made out of 250 micrometer thick beryllium foils. The detector sensor elements consists of microstrip plates shaped as regular octagons with a diameter of 292 mm. The basic microstrip pattern is similar to the one chosen for the HEPC/LEPC detector system on SRG. The detector position resolution will be sufficient to ensure an angular resolution for JEM-X of better than 3 arcmin throughout the 2 - 60 keV band.

M3 - Article in proceedings

VL - 2806

SP - 297

EP - 307

BT - Proc. SPIE

A2 - Ramsey, Brian D.

A2 - Parnell, Thomas A.

T2 - SPIE'S 1996 International Symposium on Optical Science, Engineering, and Instrumentation

Y2 - 4 August 1996 through 9 August 1996

ER -