Observatory science with eXTP

Tarih
2019
Yazar
Svoboda, Jirai
Vink, Jacco
Wang, Jian-Min
Wang, JunFeng
Watts, Anna L.
Weng, ShanShan
Weinberg, Nevin N.
Wheatley, Peter J.
Wijnands, Rudy
Woods, Tyrone E.
Woosley, Stan E.
Xiong, ShaoLin
Xu, YuPeng
Yan, Zhen
Younes, George
Yu, WenFei
Yuan, Feng
Zampieri, Luca
Zane, Silvia
Zdziarski, Andrzej A.
Zhang, Shuang-Nan
Zhang, Shu
Zhang, Shuo
Zhang, Xiao
Zingale, Michael
De Pasquale, Massimiliano
in't Zand, Jean J. M.
Bozzo, Enrico
Qu, JinLu
Li, Xiang-Dong
Amati, Lorenzo
Chen, Yang
Donnarumma, Immacolata
Doroshenko, Victor
Drake, Stephen A.
Hernanz, Margarita
Jenke, Peter A.
Maccarone, Thomas J.
Mahmoodifar, Simin
de Martino, Domitilla
De Rosa, Alessandra
Rossi, Elena M.
Rowlinson, Antonia
Sala, Gloria
Stratta, Giulia
Tauris, Thomas M.
Wilms, Joern
Wu, XueFeng
Zhou, Ping
Agudo, Ivan
Altamirano, Diego
Atteia, Jean-Luc
Andersson, Nils A.
Baglio, M. Cristina
Ballantyne, David R.
BAYKAL, ALTAN
Behar, Ehud
Belloni, Tomaso
Bhattacharyya, Sudip
Bianchi, Stefano
Bilous, Anna
Blay, Pere
Braga, Joao
Brandt, Soren
Brown, Edward F.
Bucciantini, Niccolo
Burderi, Luciano
Cackett, Edward M.
Campana, Riccardo
Campana, Sergio
Casella, Piergiorgio
Cavecchi, Yuri
Chambers, Frank
Chen, Liang
Chen, Yu-Peng
Chenevez, Jerome
Chernyakova, Maria
Jin, ChiChuan
Ciolfi, Riccardo
Costantini, Elisa
Cumming, Andrew
D'Ai, Antonino
Dai, Zi-Gao
D'Ammando, Filippo
Degenaar, Nathalie
Del Santo, Melania
D'Elia, Valerio
Di Salvo, Tiziana
Doyle, Gerry
Falanga, Maurizio
Fan, XiLong
Ferdman, Robert D.
Feroci, Marco
Fraschetti, Federico
Galloway, Duncan K.
Gambino, Angelo F.
Gandhi, Poshak
Ge, MingYu
Gendre, Bruce
Gill, Ramandeep
Gotz, Diego
Gouiffes, Christian
Grandi, Paola
Granot, Jonathan
Guedel, Manuel
Heger, Alexander
Heinke, Craig O.
Homan, Jeroen
Iaria, Rosario
Iwasawa, Kazushi
Izzo, Luca
Ji, Long
Jonker, Peter G.
Jose, Jordi
Kaastra, Jelle S.
KALEMCİ, EMRAH
Kargaltsev, Oleg
Kawai, Nobuyuki
Keek, Laurens
Komossa, Stefanie
Kreykenbohm, Ingo
Kuiper, Lucien
Kunneriath, Devaky
Li, Gang
Liang, En-Wei
Linares, Manuel
Longo, Francesco
Lu, FangJun
Lutovinov, Alexander A.
Malyshev, Denys
Malzac, Julien
Manousakis, Antonios
McHardy, Ian
Mehdipour, Missagh
Men, YunPeng
Mendez, Mariano
Mignani, Roberto P.
Mikusincova, Romana
Miller, M. Coleman
Miniutti, Giovanni
Motch, Christian
Nattila, Joonas
Nardini, Emanuele
Neubert, Torsten
O'Brien, Paul T.
Orlandini, Mauro
Osborne, Julian P.
Pacciani, Luigi
Paltani, Stephane
Paolillo, Maurizio
Papadakis, Iossif E.
Paul, Biswajit
Pellizzoni, Alberto
Peretz, Uria
Perez Torres, Miguel A.
Perinati, Emanuele
Prescod-Weinstein, Chanda
Reig, Pablo
Riggio, Alessandro
Rodriguez, Jerome
Rodriguez-Gil, Pablo
Romano, Patrizia
Rozanska, Agata
Sakamoto, Takanori
Salmi, Tuomo
Salvaterra, Ruben
Sanna, Andrea
Santangelo, Andrea
Savolainen, Tuomas
Schanne, Stephane
Schatz, Hendrik
Shao, LiJing
Shearer, Andy
Shore, Steven N.
Stappers, Ben W.
Strohmayer, Tod E.
Suleimanov, Valery F.
Thielemann, F. -K.
Tombesi, Francesco
Torres, Diego F.
Torresi, Eleonora
Turriziani, Sara
Vacchi, Andrea
Vercellone, Stefano
Üst veri
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Özet
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.
Bağlantı
http://hdl.handle.net/20.500.12627/27693
https://doi.org/10.1007/s11433-017-9186-1
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