JEM-X: The X-ray monitor aboard INTEGRAL ?
By N. Lund, C. Budtz-Jørgensen, N. Westergaard, S. Brandt, I. Rasmussen, A. Hornstrup, C. A. Oxborrow, J. Chenevez, P. A. Jensen, S. Laursen and 44 more. 2003
364 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/948d8beb18d5cbcac0c4b09a34deb64b82518e35
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In Astronomy and Astrophysics
- Andrii Y. Neronov
- R. Sunyaev
- The Pierre Auger Collaboration
- J. Knoedlseder
- Nami Mowlavi
- M. Falanga
- A. Kienlin
- E. Bozzo
In Nuclear and High Energy Physics
- Andrii Y. Neronov
- R. Sunyaev
- The Pierre Auger Collaboration
- Pietro Ubertini
- J. Gladstone
- R. Sunyaev
- G. Sivakoff
- B. Tetarenko
Citations in the corpus
- WATCHDOG: A COMPREHENSIVE ALL-SKY DATABASE OF GALACTIC BLACK HOLE X-RAY BINARIES (2015, background): “The other two are the Joint European X-Ray Monitor (JEM-X; Lund et al. 2003) X-ray detectors, which have a primary energy range of 3–35 keV, an energy resolution of 9% and 13% at 30 keV, and a circular field of view of diameter 10 degrees.”
- INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational-wave Event GW170817 (2017, methodology): “We investigated the mosaicked images of the complete observation of IBIS/ISGRI, SPI, and JEM-X.”
- Unveiling Supergiant Fast X-Ray Transient Sources with INTEGRAL (2006, methodology): “In most cases, the source was outside or on the edge of the JEM-X field of view; no significant detection were obtained for those inside the FOV so we did not take into account JEM-X data for our analysis.”
- INTEGRAL observations of the cosmic X-ray background in the 5–100 keV range via occultation by the Earth (2006, background): “In addition INTEGRAL provides simultaneous monitoring of sources in the X-ray (3–35keV; JEM-X, see Lund et al. 2003) and optical (V-band, 550nm; OMC, see MasHesse et al., 2003) energy ranges.”
- The INTEGRAL Science Data Centre (ISDC) (2001, neutral): “Appropriate calibration data are selectedfrom the status of the instruments, gains previously derived areapplied and corrections related e.g. to the JEM-X anodes and to the status of the individual IBIS pixels are applied.”
- Multi-messenger observations of a binary neutron star merger (2017, background): “Wavelength References GROND/– 2017 Aug 20 04:49:21 2.67 optical, IR GCN 21608, Chen et al. (2017) VIRT/– 2017 Aug 20 05:27:49 2.7 optical GCN 21609, Gendre et al. (2017) SALT/– 2017 Aug 20 06:14:37 2.73 optical GCN 21610, Shara et al. (2017) Swift/XRT 2017 Aug 20 08:42:40 2.83 x-ray GCN 21612, Evans”
- INTEGRAL observations of recurrent fast X-ray transient sources (2005, methodology): “The X-Ray Monitor JEM-X (Lund et al. 2003) on board the INTEGRAL satellite makes observations simultaneously with IBIS/ISGRI, providing images in the energy band 3–35 keV with a 13.”