| Publications |
- Apsidal motion and absolute parameters of GV Nor and V881 Sco based on mid-resolution spectroscopy and TESS photometry - Surgit, Derya, Zasche, Petr,Hadrava, Petr,Erdem, Ahmet,Engelbrecht, Chris A.,Marang, Fred,Masek, Martin,Stevens, Daniel J. (2023-03-01) http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.4699S
- Deep Hard X-ray Survey of the M81 Field Based on INTEGRAL1 Data - Krivonos, R. A., Mereminskiy, I. A.,Sazonov, S. Yu. (2024-05-01) http://ui.adsabs.harvard.edu/#abs/2024AstL...50...25K
- Primordial black hole dark matter in the context of extra dimensions - Friedlander, Avi, Mack, Katherine J.,Schon, Sarah,Song, Ningqiang,Vincent, Aaron C. (2022-05-01) http://ui.adsabs.harvard.edu/#abs/2022PhRvD.105j3508F
- Thermonuclear explosions on neutron stars reveal the speed of their jets - Russell, Thomas D., Degenaar, Nathalie,van den Eijnden, Jakob,Maccarone, Thomas,Tetarenko, Alexandra J.,Sanchez-Fernandez, Celia,Miller-Jones, James C. A.,Kuulkers, Erik,Del Santo, Melania (2024-03-01) http://ui.adsabs.harvard.edu/#abs/2024Natur.627..763R
|
| 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. |
