Observatory science with eXTP
Date Issued
2018
Author(s)
in ’t Zand, Jean J. M.
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Bozzo, Enrico
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Qu, JinLu
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Li, Xiang-Dong
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Donnarumma, Immacolata
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Doroshenko, Victor
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Drake, Stephen A.
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Hernanz, Margarita
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Jenke, Peter A.
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Kunneriath, Devaky
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Li, Gang
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Liang, En-Wei
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Mehdipour, Missagh
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Men, YunPeng
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Maccarone, Thomas J.
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Méndez, Mariano
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Mignani, Roberto P.
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Miller, M. Coleman
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Zhang, Shuo
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Miniutti, Giovanni
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Motch, Christian
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Nättilä, Joonas
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Neubert, Torsten
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O’Brien, Paul T.
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Mahmoodifar, Simin
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Osborne, Julian P.
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Zhang, Xiao
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Paltani, Stéphane
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Papadakis, Iossif E.
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Paul, Biswajit
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Peretz, Uria
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Pérez Torres, Miguel A.
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Perinati, Emanuele
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Prescod-Weinstein, Chanda
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Zingale, Michael
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Reig, Pablo
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Rodriguez, Jerome
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Rodríguez-Gil, Pablo
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Różańska, Agata
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Sakamoto, Takanori
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Salmi, Tuomo
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Tauris, Thomas M.
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Santangelo, Andrea
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Savolainen, Tuomas
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Schanne, Stéphane
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Schatz, Hendrik
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Shao, LiJing
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Shearer, Andy
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Shore, Steven N.
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Stappers, Ben W.
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Rossi, Elena M.
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Wilms, Joern
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Strohmayer, Tod E.
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Suleimanov, Valery F.
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Svoboda, Jir̆í
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Thielemann, F.-K.
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Torres, Diego F.
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Turriziani, Sara
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Vacchi, Andrea
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Wu, XueFeng
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Rowlinson, Antonia
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Vink, Jacco
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Wang, Jian-Min
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Wang, JunFeng
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Watts, Anna L.
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Weng, ShanShan
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Weinberg, Nevin N.
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Wheatley, Peter J.
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Wijnands, Rudy
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Woods, Tyrone E.
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Zhou, Ping
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Woosley, Stan E.
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Sala, Gloria
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Xiong, ShaoLin
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Xu, YuPeng
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Yan, Zhen
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Younes, George
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Yu, WenFei
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Yuan, Feng
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Zane, Silvia
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Agudo, Iván
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Zdziarski, Andrzej A.
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Zhang, Shuang-Nan
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Zhang, Shu
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Altamirano, Diego
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Atteia, Jean-Luc
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Linares, Manuel
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Andersson, Nils A.
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Baglio, M. Cristina
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Ballantyne, David R.
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Baykal, Altan
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Behar, Ehud
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Bhattacharyya, Sudip
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BIANCHI, STEFANO
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Bilous, Anna
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Blay, Pere
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Longo, Francesco
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Braga, João
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Brandt, Søren
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Brown, Edward F.
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Cackett, Edward M.
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Lu, FangJun
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Chambers, Frank
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Chen, Liang
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Chen, Yu-Peng
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Chenevez, Jérôme
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Chernyakova, Maria
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Jin, ChiChuan
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Costantini, Elisa
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Cumming, Andrew
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Lutovinov, Alexander A.
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Dai, Zi-Gao
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De Pasquale, Massimiliano
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Degenaar, Nathalie
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D’Elia, Valerio
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Doyle, Gerry
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Falanga, Maurizio
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Fan, XiLong
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Malyshev, Denys
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Ferdman, Robert D.
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Fraschetti, Federico
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Galloway, Duncan K.
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Gambino, Angelo F.
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Gandhi, Poshak
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Ge, MingYu
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Gendre, Bruce
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Gill, Ramandeep
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Götz, Diego
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Malzac, Julien
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Gouiffès, Christian
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Granot, Jonathan
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Güdel, Manuel
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Heger, Alexander
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Heinke, Craig O.
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Homan, Jeroen
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Iwasawa, Kazushi
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Manousakis, Antonios
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Ji, Long
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Jonker, Peter G.
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José, Jordi
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Kaastra, Jelle S.
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Kalemci, Emrah
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Kargaltsev, Oleg
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Kawai, Nobuyuki
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Keek, Laurens
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Komossa, Stefanie
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Kreykenbohm, Ingo
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McHardy, Ian
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Kuiper, Lucien
Abstract
In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring stars, supernova remnants, accreting white dwarfs, low and high mass X-ray binaries, radio quiet and radio loud active galactic nuclei, tidal disruption events, and gamma-ray bursts. eXTP will be excellently suited to study one common aspect of these objects: their often transient nature. Developed by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Science, the eXTP mission is expected to be launched in the mid 2020s.
Volume
62
Issue
2
Start page
29506
Issn Identifier
1674-7348
Ads BibCode
2019SCPMA..6229506I
Rights
open.access
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