Publications |
- A photometric study of two neglected eclipsing binaries - Kudak, V., Fedurco, M.,Perig, V.,Parimucha, S. (2021-08-01) http://ui.adsabs.harvard.edu/#abs/2021RAA....21..174K
- Multiwavelength observation of 1A 0535+262=HD 245770 from 2010 to 2021 - Liu, Wei, Yan, Jingzhi,Xiao, Guangcheng,Li, Xiukun,Gao, Bo,Liu, Qingzhong (2024-01-01) http://ui.adsabs.harvard.edu/#abs/2024A&A...681A..10L
- Study of changes in the pulsation period of 148 Galactic Cepheid variables - Csornyei, G., Szabados, L.,Molnar, L.,Cseh, B.,Egei, N.,Kalup, Cs,Kecskemethy, V.,Konyves-Toth, R.,Sarneczky, K.,Szakats, R. (2022-04-01) http://ui.adsabs.harvard.edu/#abs/2022MNRAS.511.2125C
- 26Al gamma rays from the Galaxy with INTEGRAL/SPI - Pleintinger, Moritz M. M., Diehl, Roland,Siegert, Thomas,Greiner, Jochen,Krause, Martin G. H. (2023-04-01) http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..53P
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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. |