학술논문

Observatory science with eXTP
Document Type
Working Paper
Author
Zand, Jean J. M. in 'tBozzo, EnricoQu, JinluLi, Xiang-DongAmati, LorenzoChen, YangDonnarumma, ImmacolataDoroshenko, VictorDrake, Stephen A.Hernanz, MargaritaJenke, Peter A.Maccarone, Thomas J.Mahmoodifar, Siminde Martino, DomitillaDe Rosa, AlessandraRossi, Elena M.Rowlinson, AntoniaSala, GloriaStratta, GiuliaTauris, Thomas M.Wilms, JoernWu, XuefengZhou, PingAgudo, IvánAltamirano, DiegoAtteia, Jean-LucAndersson, Nils A.Baglio, M. CristinaBallantyne, David R.Baykal, AltanBehar, EhudBelloni, TomasoBhattacharyya, SudipBianchi, StefanoBilous, AnnaBlay, PereBraga, JoãoBrandt, SørenBrown, Edward F.Bucciantini, NiccolòBurderi, LucianoCackett, Edward M.Campana, RiccardoCampana, SergioCasella, PiergiorgioCavecchi, YuriChambers, FrankChen, LiangChen, Yu-PengChenevez, JérômeChernyakova, MariaChichuan, JinCiolfi, RiccardoCostantini, ElisaCumming, AndrewD'Aı, AntoninoDai, Zi-GaoD'Ammando, FilippoDe Pasquale, MassimilianoDegenaar, NathalieDel Santo, MelaniaD'Elia, ValerioDi Salvo, TizianaDoyle, GerryFalanga, MaurizioFan, XilongFerdman, Robert D.Feroci, MarcoFraschetti, FedericoGalloway, Duncan K.Gambino, Angelo F.Gandhi, PoshakGe, MingyuGendre, BruceGill, RamandeepGötz, DiegoGouiffès, ChristianGrandi, PaolaGranot, JonathanGüdel, ManuelHeger, AlexanderHeinke, Craig O.Homan, JeroenIaria, RosarioIwasawa, KazushiIzzo, LucaJi, LongJonker, Peter G.José, JordiKaastra, Jelle S.Kalemci, EmrahKargaltsev, OlegKawai, NobuyukiKeek, LaurensKomossa, StefanieKreykenbohm, IngoKuiper, LucienKunneriath, DevakyLi, GangLiang, En-WeiLinares, ManuelLongo, FrancescoLu, FangjunLutovinov, Alexander A.Malyshev, DenysMalzac, JulienManousakis, AntoniosMcHardy, IanMehdipour, MissaghMen, YunpengMéndez, MarianoMignani, Roberto P.Mikusincova, RomanaMiller, M. ColemanMiniutti, GiovanniMotch, ChristianNättilä, JoonasNardini, EmanueleNeubert, TorstenO'Brien, Paul T.Orlandini, MauroOsborne, Julian P.Pacciani, LuigiPaltani, StéphanePaolillo, MaurizioPapadakis, Iossif E.Paul, BiswajitPellizzoni, AlbertoPeretz, UriaTorres, Miguel A. PérezPerinati, EmanuelePrescod-Weinstein, ChandaReig, PabloRiggio, AlessandroRodriguez, JeromeRodrıguez-Gil, PabloRomano, PatriziaRóżańska, AgataSakamoto, TakanoriSalmi, TuomoSalvaterra, RubenSanna, AndreaSantangelo, AndreaSavolainen, TuomasSchanne, StéphaneSchatz, HendrikShao, LijingShearer, AndyShore, Steven N.Stappers, Ben W.Strohmayer, Tod E.Suleimanov, Valery F.Svoboda, JirıThielemann, F. -K.Tombesi, FrancescoTorres, Diego F.Torresi, EleonoraTurriziani, SaraVacchi, AndreaVercellone, StefanoVink, JaccoWang, Jian-MinWang, JunfengWatts, Anna L.Weng, ShanshanWeinberg, Nevin N.Wheatley, Peter J.Wijnands, RudyWoods, Tyrone E.Woosley, Stan E.Xiong, ShaolinXu, YupengYan, ZhenYounes, GeorgeYu, WenfeiYuan, FengZampieri, LucaZane, SilviaZdziarski, Andrzej A.Zhang, Shuang-NanZhang, ShuZhang, ShuoZhang, XiaoZingale, Michael
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
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.
Comment: Accepted for publication on Sci. China Phys. Mech. Astron. (2019)