A dataset provided by the European Space Agency

Proposal ID 1920005
Obs ID 19200050019, 19200050020, 19200050021, 19200050022, 19200050024, 19200050026, 19200050027, 19200050028, 19200050029, 19200050032, 19200050033, 19200050034, 19200050036, 19200050037, 19200050039, 19200050042, 19200050048, 19200050074, 19200050079, 19200050080, 19200050084, 19200050087, 19200050089, 19200050091, 19200050092, 19200050093, 19200050094, 19200050095, 19200050096, 19200050097, 19200050098, 19200050099, 19200050100, 19200050101, 19200050102, 19200050103, 19200050104, 19200050105, 19200050106, 19200050107, 19200050108, 19200050109, 19200050110, 19200050111, 19200050112, 19200050113, 19200050114, 19200050115, 19200050116, 19200050117, 19200050118, 19200050119, 19200050120, 19200050121, 19200050122, 19200050123, 19200050124, 19200050127, 19200050129, 19200050145, 19200050146, 19200050147, 19200050148, 19200050149, 19200050150, 19200050151, 19200050152, 19200050153, 19200050154, 19200050155, 19200050156, 19200050157, 19200050158, 19200050159, 19200050160, 19200050161, 19200050162, 19200050163, 19200050164, 19200050165, 19200050166, 19200050167, 19200050168, 19200050169, 19200050170, 19200050171, 19200050172, 19200050173, 19200050174, 19200050175, 19200050176, 19200050177, 19200050178, 19200050179, 19200050180
Title Keeping watch over our Galaxy - GPS7
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:1920005
DOI https://doi.org/10.57780/esa-ioll0yg
Author Bazzano
Abstract The survey of the Galactic Plane has continued as one of the main INTEGRAL scientific objectives because of the scientific potential of both new source discovery and detailed monitoring of already known sources that will provide a legacy archive and a basis for future missions. We propose for a total of 3.0 Ms of observations in AO18 and 3 Ms in AO19 to continue our KeyProgram covering areas of the Plane with regular scans every orbit. For these AOs we selected again the section of the Plane incorporating two sky regions centered at l=+/-30, that are both rich in galactic sources (LMXB and HMXB, SFXT inparticular) and potential MeV/TeV sources. Our purpose is to regularly monitor known systems as well as to dramatically enhance the chances of discovering new systems or new outbursts from known sources. This program will allow a rapid response to bright events and a detailed study of faint transients and their long-term activity. Such a programme will be of high value to avery large fraction of the high-energy astronomy community, stimulating science immediately, and furthermore contributing greatly to the INTEGRAL legacy. In order to maximise the engagement of the scientific community, we will continue to make the observations public immediately. The team will make, as it has been through AO8-17, the scw-resolution IBIS and JEM-X light curves (in two energy bands) and per revolution mosaic images publicly available through the web as soon as possible. Any interesting source behaviour that emerges from our observations will be announced promptly in the usual way through Atels, so that rapid follow-up by the community is possible, as has already been demonstrated.
Publications
  • A Multi-epoch, Multiwavelength Study of the Classical FUor V1515 Cyg Approaching Quiescence - Szabo, Zs. M., Kospal, A.,Abraham, P.,Park, S.,Siwak, M.,Green, J. D.,Pal, A.,Acosta-Pulido, J. A.,Lee, J. -E.,Ibrahimov, M.,Grankin, K.,Kovacs, B.,Bora, Zs.,Bodi, A.,Cseh, B.,Csornyei, G.,Drozdz, Marek,Hanyecz, O.,Ignacz, B.,Kalup, Cs.,Konyves-Toth, R.,Krezinger, M.,Kriskovics, L.,Ogloza, Waldemar,Ordasi, A.,Sarneczky, K.,Seli, B.,Szakats, R.,Sodor, A.,Szing, A.,Vida, K.,Vinko, J. (2022-09-01) http://ui.adsabs.harvard.edu/#abs/2022ApJ...936...64S
  • An asymmetrical model for high-energy radiation of Cassiopeia A - Zhan, Shihong, Wang, Wei,Mou, Guobin,Li, Zhuo (2022-06-01) http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.2471Z
  • CCD Observations and Period Change of the Type ab RR Lyrae Star DV Mon - Berdnikov, L. N., Kniazev, A. Yu.,Dambis, A. K.,Kravtsov, V. V.,Pastukhova, E. N.,Katkov, I. Y. (2019-04-01) http://ui.adsabs.harvard.edu/#abs/2019AstBu..74..183B
  • 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
  • INTEGRAL Observations of Magnetars - Pacholski, Dominik Patryk, Ducci, Lorenzo,Topinka, Martin,Mereghetti, Sandro (2025-01-01) http://ui.adsabs.harvard.edu/#abs/2025AN....34640109P
  • Jitter Radiation as an Alternative Mechanism for the Nonthermal X-Ray Emission of Cassiopeia A - Greco, Emanuele, Vink, Jacco,Ellien, Amael,Ferrigno, Carlo (2023-10-01) http://ui.adsabs.harvard.edu/#abs/2023ApJ...956..116G
  • Multi-wavelength study of 1eRASS J085039.9-421151 with eROSITA, NuSTAR, and X-shooter - Zainab, A., Avakyan, A.,Doroshenko, V.,Thalhammer, P.,Sokolova-Lapa, E.,Ballhausen, R.,Zalot, N.,Stierhof, J.,Hammerich, S.,Diez, C. M.,Weber, P.,Dauser, T.,Berger, K.,Kretschmar, P.,Pottschmidt, K.,Pradhan, P.,Islam, N.,Maitra, C.,Coley, J. B.,Blay, P.,Corbet, R. H. D.,Rothschild, R. E.,Wood, K.,Santangelo, A.,Heber, U.,Wilms, J. (2025-01-01) http://ui.adsabs.harvard.edu/#abs/2025A&A...693A.260Z
  • 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
  • Searching for redshifted 2.2 MeV neutron-capture lines from accreting neutron stars: Theoretical X-ray luminosity requirements and INTEGRAL/SPI observations - Ducci, L., Santangelo, A.,Tsygankov, S.,Mushtukov, A.,Ferrigno, C. (2024-10-01) http://ui.adsabs.harvard.edu/#abs/2024A&A...690A.309D
  • 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
  • Swift, NuSTAR, and INTEGRAL observations of the symbiotic X-ray binary IGR J16194-2810 - Bozzo, E., Romano, P.,Ferrigno, C.,Ducci, L. (2024-01-01) http://ui.adsabs.harvard.edu/#abs/2024MNRAS.527.3585B
Temporal Coverage 2022-01-03T15:41:19Z / 2023-01-01T13:45:33Z
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 2025-03-25T09:54:40Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Bazzano, 2025, 'Keeping watch over our Galaxy - GPS7', 1.0, European Space Agency, https://doi.org/10.57780/esa-ioll0yg