A dataset provided by the European Space Agency

Proposal ID 1520009
Obs ID 15200090001, 15200090002, 15200090003, 15200090004, 15200090005, 15200090006, 15200090007, 15200090008, 15200090009, 15200090010
Title Peering through accretion-ejections mechanisms with an INTEGRAL/multi-wavelength GRS 1915+1015 monitoring program
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:1520009
DOI https://doi.org/10.57780/esa-1258h3g
Author Rodriguez
Abstract We propose to continue the renewed INTEGRAL-multiwavelengh monitoring of GRS 1915+105 with the goal to understand the tight connections that exist between the different emitting media, and placed in a broader context, understand accreting-ejecting sources in general. As for AO 14, we will take advantage of new facilities (the Sardinia radio telescope in the radio domain, and NICER at soft X-rays), while tentatively increasing the number of wavelengths covered by including infrared (ESO facilities), and gamma-ray (Fermi) observations. Other X-ray facilities will also be considered. We require 45 ks pointings taken every second revolution, in order to 1) probe the physics of accretion by studying the 0.5--500 keV emission of the source, 2) study the origin of the high variability of GRS 1915+105, 3) understand the connections between accretion and ejection processes, and 4) constrain physical models of emission processes. Points 1) and 2) can be done by looking into the interplay between the soft and hard X-ray emitters (therefore with JEM-X and IBIS), point 3) and 4) needs contemporaneous braod band coverages and timing studies. Besides these specific points this monitoring will allow us to accumulate more data and thus have a better view of the (rather unknown) behaviour of this source beyond 200 keV. It should be noted that GRS 1915+105 lies in a quite crowded field, with many variable sources such as X-ray binaries of all types, the enigmatic microquasar SS 433, and a couple of highly absorbed IGR sources. This survey will also permit all these sources to be studied in a regular manner. Such a monitoring will greatly participate to the INTEGRAL legacy by bringing new data on a dozen of exciting Galactic sources.
Publications
  • An infrared study of Galactic OH/IR stars - III. Variability properties of the Arecibo sample - Jimenez-Esteban, F. M., Engels, D.,Aguado, D. S.,Gonzalez, J. B.,Garcia-Lario, P. (2021-08-01) http://ui.adsabs.harvard.edu/#abs/2021MNRAS.505.6051J
  • 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
  • Gamma-Ray Emission of 60Fe and 26Al Radioactivity in Our Galaxy - Wang, W., Siegert, T.,Dai, Z. G.,Diehl, R.,Greiner, J.,Heger, A.,Krause, M.,Lang, M.,Pleintinger, M. M. M.,Zhang, X. L. (2020-02-01) http://ui.adsabs.harvard.edu/#abs/2020ApJ...889..169W
  • Gamma-ray observations of MAXI J1820+070 during the 2018 outburst - Abe, H., Abe, S.,Acciari, V. A.,Aniello, T.,Ansoldi, S.,Antonelli, L. A.,Arbet Engels, A.,Arcaro, C.,Artero, M.,Asano, K.,Baack, D.,Babic, A.,Baquero, A.,Barres de Almeida, U.,Barrio, J. A.,Batkovic, I.,Baxter, J.,Becerra Gonzalez, J.,Bednarek, W.,Bernardini, E.,Bernardos, M.,Berti, A.,Besenrieder, J.,Bhattacharyya, W.,Bigongiari, C.,Biland, A.,Blanch, O.,Bonnoli, G.,Bosnjak, Z.,Burelli, I.,Busetto, G.,Carosi, R.,Carretero-Castrillo, M.,Ceribella, G.,Chai, Y.,Chilingarian, A.,Cikota, S.,Colombo, E.,Contreras, J. L.,Cortina, J.,Covino, S.,D Amico, G.,D Elia, V.,da Vela, P.,Dazzi, F.,de Angelis, A.,de Lotto, B.,Del Popolo, A.,Delfino, M.,Delgado, J.,Delgado Mendez, C.,Depaoli, D.,di Pierro, F.,di Venere, L.,Dominis Prester, D.,Donini, A.,Dorner, D.,Doro, M.,Elsaesser, D.,Emery, G.,Fallah Ramazani, V.,Farina, L.,Fattorini, A.,Font, L.,Fruck, C.,Fukami, S.,Fukazawa, Y.,Garcia Lopez, R. J.,Garczarczyk, M.,Gasparyan, S.,Gaug, M.,Giesbrecht Paiva, J. G.,Giglietto, N.,Giordano, F.,Gliwny, P.,Godinovic, N.,Grau, R.,Green, D.,Green, J. G.,Hadasch, D.,Hahn, A.,Hassan, T.,Heckmann, L.,Herrera, J.,Hoang, J.,Hrupec, D.,Hutten, M.,Imazawa, R.,Inada, T.,Iotov, R.,Ishio, K.,Jimenez Martinez, I.,Jormanainen, J.,Kerszberg, D.,Kobayashi, Y.,Kubo, H.,Kushida, J.,Lamastra, A.,Lelas, D.,Leone, F.,Lindfors, E.,Linhoff, L.,Lombardi, S.,Longo, F.,Lopez-Coto, R.,Lopez-Moya, M.,Lopez-Oramas, A.,Loporchio, S.,Lorini, A.,Lyard, E.,Machado de Oliveira Fraga, B.,Majumdar, P.,Makariev, M.,Maneva, G.,Mang, N.,Manganaro, M.,Mangano, S.,Mannheim, K.,Mariotti, M.,Martinez, M.,Mas Aguilar, A.,Mazin, D.,Menchiari, S.,Mender, S.,Micanovic, S.,Miceli, D.,Miener, T.,Miranda, J. M.,Mirzoyan, R.,Molina, E.,Mondal, H. A.,Moralejo, A.,Morcuende, D.,Moreno, V.,Nakamori, T.,Nanci, C.,Nava, L.,Neustroev, V.,Nievas Rosillo, M.,Nigro, C.,Nilsson, K.,Nishijima, K.,Njoh Ekoume, T.,Noda, K.,Nozaki, S.,Ohtani, Y.,Oka, T.,Okumura, A.,Otero-Santos, J.,Paiano, S.,Palatiello, M.,Paneque, D.,Paoletti, R.,Paredes, J. M. et al. (2022-12-01) http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.4736A
  • Hybrid Comptonization and Electron-Positron Pair Production in the Black-hole X-Ray Binary MAXI J1820+070 - Zdziarski, Andrzej A., Jourdain, Elisabeth,Lubinski, Piotr,Szanecki, Michal,Niedzwiecki, Andrzej,Veledina, Alexandra,Poutanen, Juri,Dzielak, Marta A.,Roques, Jean-Pierre (2021-06-01) http://ui.adsabs.harvard.edu/#abs/2021ApJ...914L...5Z
  • INTEGRAL Observations of Magnetars - Pacholski, Dominik Patryk, Ducci, Lorenzo,Topinka, Martin,Mereghetti, Sandro (2025-01-01) http://ui.adsabs.harvard.edu/#abs/2025AN....34640109P
  • INTEGRAL study of MAXI J1535-571, MAXI J1820+070, and MAXI J1348 - 630 outbursts. I. Detection and polarization properties of the high-energy emission - Cangemi, F., Rodriguez, J.,Belloni, T.,Gouiffes, C.,Grinberg, V.,Laurent, P.,Petrucci, P. -O.,Wilms, J. (2023-01-01) http://ui.adsabs.harvard.edu/#abs/2023A&A...669A..65C
  • Magnetars and axion-like particles: probes with the hard X-ray spectrum - Fortin, Jean-Francois, Guo, Huai-Ke,Harris, Steven P.,Sheridan, Elijah,Sinha, Kuver (2021-06-01) http://ui.adsabs.harvard.edu/#abs/2021JCAP...06..036F
  • 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 of the Classical Cepheid EV Aql - Berdnikov, L. N., (2020-06-01) http://ui.adsabs.harvard.edu/#abs/2020AstL...46..388B
  • 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 Broad-lined Ic Supernova ZTF18aaqjovh (SN 2018bvw): An Optically Discovered Engine-driven Supernova Candidate with Luminous Radio Emission - Ho, Anna Y. Q., Corsi, Alessandra,Cenko, S. Bradley,Taddia, Francesco,Kulkarni, S. R.,Adams, Scott,De, Kishalay,Dekany, Richard,Frederiks, Dmitry D.,Fremling, Christoffer,Golkhou, V. Zach,Graham, Matthew J.,Hung, Tiara,Kupfer, Thomas,Laher, Russ R.,Mahabal, Ashish,Masci, Frank J.,Miller, Adam A.,Neill, James D.,Reiley, Daniel,Riddle, Reed,Ridnaia, Anna,Rusholme, Ben,Sharma, Yashvi,Sollerman, Jesper,Soumagnac, Maayane T.,Svinkin, Dmitry S.,Shupe, David L. (2020-04-01) http://ui.adsabs.harvard.edu/#abs/2020ApJ...893..132H
  • 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
  • XTE J1906+090: a persistent low-luminosity Be X-ray binary - Sguera, V., Sidoli, L.,Bird, A. J.,La Palombara, N. (2023-07-01) http://ui.adsabs.harvard.edu/#abs/2023MNRAS.523.1192S
Temporal Coverage 2018-04-21T13:17:18Z / 2018-11-09T10:53:14Z
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, Rodriguez, 2025, 'Peering through accretion-ejections mechanisms with an INTEGRAL/multi-wavelength GRS 1915+1015 monitoring program', 1.0, European Space Agency, https://doi.org/10.57780/esa-1258h3g