INTEGRAL TOO observations of the Rapid Burster in coordination with Swift and the Very Large Array to observe, strictly simultaneously, an outburst of the Rapid Burster
Searching for orbital period modulation in X-ray observations of the symbiotic X-ray binary GX 1+4 - Klawin, Moritz, Ducci, Lorenzo,Mirac Serim, M.,Santangelo, Andrea,Ferrigno, Carlo,Bozzo, Enrico (2024-12-01) http://ui.adsabs.harvard.edu/#abs/2024A&A...692A..19K
Sgr B2 hard X-ray emission with INTEGRAL after 2009: still detectable? - Kuznetsova, Ekaterina, Krivonos, Roman,Lutovinov, Alexander,Clavel, Maica (2022-01-01) http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.1605K
The variable radio jet of the accreting neutron star the Rapid Burster - van den Eijnden, J., Robins, D.,Sharma, R.,Sanchez-Fernandez, C.,Russell, T. D.,Degenaar, N.,Miller-Jones, J. C. A.,Maccarone, T. (2024-09-01) http://ui.adsabs.harvard.edu/#abs/2024MNRAS.533..756V
Temporal Coverage
2020-03-19T10:23:12Z / 2020-03-19T18:05:39Z
Version
1.0
Mission Description
The INTEGRAL (International Gamma-Ray Astrophysics Laboratory) mission, launched by the European Space Agency (ESA) on October 17, 2002, was designed to study high-energy phenomena in the universe. INTEGRAL was operating until february 2025 and it was equipped with three high-energy instruments: the Imager on Board the INTEGRAL Satellite (IBIS), the Spectrometer on INTEGRAL (SPI), and the JEM-X (Joint European Monitor for X-rays). Its Optical Monitoring Camera (OMC) provided optical V-band magnitude measurements, complementing the high-energy observations.
European Space Agency, van den Eijnden, 2025, 'INTEGRAL TOO observations of the Rapid Burster', 1.0, European Space Agency, https://doi.org/10.57780/esa-hz4k4fn
