A dataset provided by the European Space Agency

Proposal ID 1620001
Obs ID 16200010001, 16200010002, 16200010003, 16200010004, 16200010005, 16200010006, 16200010007, 16200010008, 16200010009, 16200010010, 16200010011, 16200010012, 16200010013, 16200010014, 16200010015, 16200010016, 16200010017, 16200010018, 16200010019, 16200010020, 16200010021, 16200010022, 16200010023, 16200010024, 16200010025, 16200010026, 16200010027, 16200010028, 16200010029, 16200010030, 16200010031, 16200010032
Title Regular and frequent INTEGRAL monitoring of the Galactic Bulge region
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:1620001
DOI https://doi.org/10.57780/esa-9a8xzyd
Author Kuulkers
Abstract The Galactic bulge region is a rich host of variable X-ray and gamma-ray point sources. Since AO-3 we are monitoring about 190 of them with one hexagonal pattern about every 3 days, whenever the region is visible by INTEGRAL. Due to the high scientific return and in order to preserve the continuity with respect to past observations of this ever-changing region, we propose to continue our successful program. Our main aim is to monitor and actively report on any (transient) activity; in the long run the program is providing regular and homogeneous inputs about the soft and hard-X-ray (transient) population, as well as on the accretion regimes in the various types of binary systems. As a service to the scientific community, the observations are to be made public. We will continue to make the IBIS/ISGRI and JEM-X quick-look results publicly available through the web soon after the data have been taken, to preserve the possibility for rapid follow-up by the community.
Publications
  • Diffuse Galactic emission spectrum between 0.5 and 8.0 MeV - Siegert, Thomas, Berteaud, Joanna,Calore, Francesca,Serpico, Pasquale D.,Weinberger, Christoph (2022-04-01) http://ui.adsabs.harvard.edu/#abs/2022A&A...660A.130S
  • High-energy Jet Emission from GRS 1758-258 and 1E 1740.7-2942 with INTEGRAL? - Rodi, James, Bazzano, Angela,Ubertini, Pietro (2025-04-01) http://ui.adsabs.harvard.edu/#abs/2025ApJ...982..145R
  • INTEGRAL Observations of Magnetars - Pacholski, Dominik Patryk, Ducci, Lorenzo,Topinka, Martin,Mereghetti, Sandro (2025-01-01) http://ui.adsabs.harvard.edu/#abs/2025AN....34640109P
  • 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
  • SRGA J181414.6-225604: A New Galactic Symbiotic X-Ray Binary Outburst Triggered by an Intense Mass-loss Episode of a Heavily Obscured Mira Variable - De, Kishalay, Mereminskiy, Ilya,Soria, Roberto,Conroy, Charlie,Kara, Erin,Anand, Shreya,Ashley, Michael C. B.,Boyer, Martha L.,Chakrabarty, Deepto,Grefenstette, Brian,Hankins, Matthew J.,Hillenbrand, Lynne A.,Jencson, Jacob E.,Karambelkar, Viraj,Kasliwal, Mansi M.,Lau, Ryan M.,Lutovinov, Alexander,Moore, Anna M.,Ng, Mason,Panagiotou, Christos,Pasham, Dheeraj R.,Semena, Andrey,Simcoe, Robert,Soon, Jamie,Srinivasaragavan, Gokul P.,Travouillon, Tony,Yao, Yuhan (2022-08-01) http://ui.adsabs.harvard.edu/#abs/2022ApJ...935...36D
  • The efficiency of nuclear burning during thermonuclear (Type I) bursts as a function of accretion rate - Cavecchi, Y., Galloway, D. K.,Goodwin, A. J.,Johnston, Z.,Heger, A. (2020-12-01) http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499.2148C
Temporal Coverage 2019-02-11T19:27:33Z / 2019-10-28T11:12:39Z
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.
Creator Contact https://www.cosmos.esa.int/web/integral/helpdesk
Date Published 2026-03-05T13:06:00Z
Keywords INTEGRAL gamma-ray data, ESA INTEGRAL mission dataset, gamma-ray astronomy observations, high-energy astrophysics data, IBIS imaging data, SPI spectrometer data, JEM-X X-ray monitoring data, OMC optical monitoring data, coded mask telescope observations, gamma-ray spectroscopy dataset, MeV astrophysics data, keV–MeV photon observations, gamma-ray burst observations dataset, black hole gamma-ray data, neutron star high-energy observations, positron annihilation 511 keV line data, Galactic Center gamma-ray emission dataset, supernova nucleosynthesis gamma-ray lines, active galactic nuclei high-energy data, transient astrophysical source monitoring, calibrated photon event lists, gamma-ray light curves, high-energy spectra data, sky maps gamma-ray, time-series astrophysical observations, long-term gamma-ray monitoring dataset
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Kuulkers, 2026, 'Regular and frequent INTEGRAL monitoring of the Galactic Bulge region', 1.0, European Space Agency, https://doi.org/10.57780/esa-9a8xzyd