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SKA-Athena Synergy White Paper

Authors :
Cassano, R.
Fender, R.
Ferrari, C.
Merloni, A.
Akahori, T.
Akamatsu, H.
Ascasibar, Y.
Ballantyne, D.
Brunetti, G.
Corbelli, E.
Croston, J.
Donnarumma, I.
Ettori, S.
Ferdman, R.
Feretti, L.
Forbrich, J.
Gheller, C.
Ghirlanda, G.
Govoni, F.
Ingallinera, A.
Johnston-Hollitt, M.
Markevitch, M.
Mesinger, A.
Moss, V.
Nicastro, F.
Padovani, P.
Panessa, F.
Piro, L.
Ponti, G.
Pratt, G.
Rossi, E.M.
Sadler, E.
Sasaki, M.
Soria, R.
Stevens, I.
Van Weeren, R.
Vazza, F.
Webb, N.
Observatoire de la Côte d'Azur (OCA)
Centre National de la Recherche Scientifique (CNRS)
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Université Paris Diderot - Paris 7 (UPD7)
Institut de recherche en astrophysique et planétologie (IRAP)
Université Toulouse III - Paul Sabatier (UT3)
Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP)
Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)
Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3)
Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
Source :
arXiv.org e-Print Archive
Publication Year :
2018
Publisher :
arXiv, 2018.

Abstract

The Advanced Telescope for High Energy Astrophysics (Athena) is the X-ray observatory large mission selected by the European Space Agency (ESA), within its Cosmic Vision 2015-2025 programme, to address the "Hot and Energetic Universe" scientific theme (Nandra et al. 2013), and it is provisionally due for launch in the early 2030s. The Square Kilometer Array (SKA) is the next generation radio observatory and consists of two telescopes, one comprised of dishes operating at mid frequencies (SKA1-MID) and located in South Africa, and the other comprised of Log-Periodic antennas operating at low radio frequencies (SKA1-LOW), which will be located in Australia (Braun et al. 2017). The scientific commissioning of the radio telescope is planned to begin in 2021-2022. The SKA-Athena Synergy Team (SAST) has been tasked to single out the potential scientific synergies between Athena and SKA. The astrophysical community was involved in this exercise primarily through a dedicated SKA-Athena Synergy Workshop, which took place on April 24-25, 2017 at SKAO, Jodrell Bank, Manchester. The final result of the synergy exercise, this White Paper, describes in detail a number of scientific opportunities that will be opened up by the combination of Athena and SKA, these include: 1. the Cosmic Dawn; 2. the Evolution of black holes and galaxies; 3. Active galaxy feedback in galaxy clusters; 4. Non-thermal phenomena in galaxy clusters; 5. Detecting the cosmic web; 6. Black-hole accretion physics and astrophysical transients; 7. Galactic astronomy: stars, planets, pulsars and supernovae.<br />Comment: 79 pages, 28 figures. A high resolution version of the White Paper is available here: https://drive.google.com/open?id=1HpuGUlDGl2oWHV7j7fQPDYnkZZ15af2I

Details

Database :
OpenAIRE
Journal :
arXiv.org e-Print Archive
Accession number :
edsair.doi.dedup.....0aa14a880aef8a4cb064602610c145cc
Full Text :
https://doi.org/10.48550/arxiv.1807.09080