A dataset provided by the European Space Agency

Proposal ID 1520025
Obs ID 15200250003, 15200250004, 15200250005, 15200250006, 15200250007, 15200250008, 15200250009, 15200250010, 15200250011, 15200250012, 15200250013, 15200250014, 15200250015, 15200250016, 15200250017, 15200250018, 15200250019, 15200250020, 15200250021, 15200250022, 15200250023, 15200250024, 15200250025, 15200250026, 15200250027, 15200250028, 15200250029, 15200250030, 15200250031, 15200250032, 15200250033, 15200250034, 15200250035, 15200250036, 15200250037, 15200250038, 15200250039, 15200250040, 15200250041, 15200250042, 15200250043, 15200250044, 15200250045, 15200250046, 15200250047, 15200250048, 15200250049, 15200250050, 15200250051, 15200250052, 15200250053, 15200250054, 15200250055, 15200250056, 15200250057, 15200250058, 15200250059, 15200250060, 15200250061, 15200250062, 15200250063, 15200250064, 15200250065, 15200250066, 15200250067, 15200250068, 15200250069, 15200250070
Title Broad view on high energy Galactic background: Galactic Plane at L=58 deg
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:1520025
DOI https://doi.org/10.57780/esa-1wmktwd
Author Mereminskiy
Abstract This proposal is aimed on obtaining legacy-level observational datasets on the Milky Way Galactic disk. The ultimate goal of the entire project is to have model independent and systematics free measurements of the fluxes in nuclear lines (511 keV annihilation emission and 1.8 MeV Al26) and a broad band spectrum of the Galactic background emission, which at different energies is provided either by cumulative emission of faint Galactic source or by interaction of low energy cosmic rays with interstellar medium. Taking into account the unique combination of properties of INTEGRAL instruments - broad band coverage, large fields of view and possibilities to eliminate the contribution of discrete sources from the total measured photon flux, the proposed strategy is the best possible usage of the valuable INTEGRAL time. Wide mapping of the Milky Way during the campaign of Galactic latitude scans also contributes to the legacy of the INTEGRAL observatory, giving the opportunity to study the population of Galactic sources at high latitudes.
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
  • INTEGRAL Observations of Magnetars - Pacholski, Dominik Patryk, Ducci, Lorenzo,Topinka, Martin,Mereghetti, Sandro (2025-01-01) http://ui.adsabs.harvard.edu/#abs/2025AN....34640109P
  • Potential origin of the state-dependent high-energy tail in the black hole microquasar Cygnus X-1 as seen with INTEGRAL - Cangemi, F., Beuchert, T.,Siegert, T.,Rodriguez, J.,Grinberg, V.,Belmont, R.,Gouiffes, C.,Kreykenbohm, I.,Laurent, P.,Pottschmidt, K.,Wilms, J. (2021-06-01) http://ui.adsabs.harvard.edu/#abs/2021A&A...650A..93C
  • 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
  • Search for Evolutionary Changes in the Period the Cepheid ET Vul - Berdnikov, L. N., Pastukhova, E. N. (2020-04-01) http://ui.adsabs.harvard.edu/#abs/2020AstL...46..235B
  • 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
  • The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years - Song, Xin-Ying, Xiong, Shao-Lin,Zhang, Shuang-Nan,Li, Cheng-Kui,Li, Xiao-Bo,Huang, Yue,Guidorzi, Cristiano,Frontera, Filippo,Liu, Cong-Zhan,Li, Xu-Fang,Li, Gang,Liao, Jin-Yuan,Cai, Ce,Luo, Qi,Xiao, Shuo,Yi, Qi-Bin,Zheng, Yao-Guang,Zhou, Deng-Ke,Liu, Jia-Cong,Xue, Wang-Chen,Zhang, Yan-Qiu,Zheng, Chao,Chang, Zhi,Li, Zheng-Wei,Lu, Xue-Feng,Zhang, Ai-Mei,Zhang, Yi-Fei,Jin, Yong-Jie,Li, Ti-Pei,Lu, Fang-Jun,Song, Li-Ming,Wu, Mei,Xu, Yu-Peng,Ma, Xiang,Ge, Ming-Yu,Jia, Shu-Mei,Li, Bing,Nie, Jian-Yin,Wang, Ling-Jun,Zhang, Juan,Zheng, Shi-Jie,Yang, Xue-Juan,Yang, Rong-Jia (2022-04-01) http://ui.adsabs.harvard.edu/#abs/2022ApJS..259...46S
Temporal Coverage 2018-11-16T02:03:36Z / 2018-12-03T12:58:22Z
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 2025-03-25T09:54:39Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Mereminskiy, 2025, 'Broad view on high energy Galactic background: "Galactic Plane at L=58 deg"', 1.0, European Space Agency, https://doi.org/10.57780/esa-1wmktwd