A dataset provided by the European Space Agency

Proposal ID 1540005
Obs ID 15400050001
Title High energy emission from Galactic black hole transients when the compact jet turns on
Download Data Associated to the proposal https://isla.esac.esa.int/tap/download/bundle?format=ascii_curl&product_id=prop_id:1540005
DOI https://doi.org/10.57780/esa-o2i9ahg
Author Kalemci
Abstract One of the most active areas in black hole research currently is understanding the role of jets in the overall emission properties of black holes, from radio all the way to gamma-rays. Thanks to the daily monitoring campaigns in X-rays, radio and optical/IR (OIR) facilities, we have a solid understanding of the relation between jet emission in the OIR, radio and X-rays up to 25 keV. Yet, our understanding about the formation of compact jets and high energy emission is still not well established due to low number of dedicated INTEGRAL observations during the outburst decays. Most archival data do not have the statistical quality where we can study properties of Comptonizing corona (which is required for the formation of compact jets), and how jets consequently may affect electron energy distribution and perhaps directly contribute to hard X-ray emission. Our previous multiwavelength campaigns revealed secondary maxima, a brightening in X-rays and OIR late in outburst decay. The nature of these secondary maxima is also still debated. We propose for two 170 ks TOO observations of a GBHT. We will trigger the first observation at the transition to the hard state as the jet turns on to investigate the relation between the Gamma-ray emission and jet formation. We will trigger the second observation if a secondary outburst is observed, close to the peak to investigate its nature. Multiwavelength coverage exists in radio and in OIR to achieve objectives of this proposal, and an additional 10ks SWIFT time is requested to cover soft X-rays.
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
  • A search for period changes of eight short-period Type II Cepheids - Yacob, Alemiye M., Berdnikov, Leonid N.,Pastukhova, Elena N.,Kniazev, Alexei Y.,Whitelock, Patricia A. (2022-10-01) http://ui.adsabs.harvard.edu/#abs/2022MNRAS.516.2095Y
  • 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 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
  • INTEGRAL Observations of Magnetars - Pacholski, Dominik Patryk, Ducci, Lorenzo,Topinka, Martin,Mereghetti, Sandro (2025-01-01) http://ui.adsabs.harvard.edu/#abs/2025AN....34640109P
  • 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
  • Multiwavelength observations of MAXI J1820+070 during its outburst decay and subsequent mini-outburst - Ozbey Arabaci, M., Kalemci, E.,Dincer, T.,Bailyn, C. D.,Altamirano, D.,Ak, T. (2022-08-01) http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514.3894O
  • 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
  • 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
Temporal Coverage 2018-10-02T14:51:34Z / 2018-10-06T15:38:15Z
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, Kalemci, 2025, 'High energy emission from Galactic black hole transients when the compact jet turns on', 1.0, European Space Agency, https://doi.org/10.57780/esa-o2i9ahg