A2 Vertaisarvioitu katsausartikkeli tieteellisessä lehdessä
Observatory science with eXTP
Tekijät: in't Zand JJM, Bozzo E, Qu JL, Li XD, Amati L, Chen Y, Donnarumma I, Doroshenko V, Drake SA, Hernanz M, Jenke PA, Maccarone TJ, Mahmoodifar S, de Martino D, De Rosa A, Rossi EM, Rowlinson A, Sala G, Stratta G, Tauris TM, Wilms J, Wu XF, Zhou P, Agudo I, Altamirano D, Atteia JL, Andersson NA, Baglio MC, Ballantyne DR, Baykal A, Behar E, Belloni T, Bhattacharyya S, Bianchi S, Bilous A, Blay P, Braga J, Brandt S, Brown EF, Bucciantini N, Burderi L, Cackett EM, Campana R, Campana S, Casella P, Cavecchi Y, Chambers F, Chen L, Chen YP, Chenevez J, Chernyakova M, Jin CC, Ciolfi R, Costantini E, Cumming A, D'Ai A, Dai ZG, D'Ammando F, De Pasquale M, Degenaar N, Del Santo M, D'Elia V, Di Salvo T, Doyle G, Falanga M, Fan XL, Ferdman RD, Feroci M, Fraschetti F, Galloway DK, Gambino AF, Gandhi P, Ge MY, Gendre B, Gill R, Gotz D, Gouiffes C, Grandi P, Granot J, Gudel M, Heger A, Heinke CO, Homan J, Iaria R, Iwasawa K, Izzo L, Ji L, Jonker PG, Jose J, Kaastra JS, Kalemci E, Kargaltsev O, Kawai N, Keek L, Komossa S, Kreykenbohm I, Kuiper L, Kunneriath D, Li G, Liang EW, Linares M, Longo F, Lu FJ, Lutovinov AA, Malyshev D, Malzac J, Manousakis A, McHardy I, Mehdipour M, Men YP, Mendez M, Mignani RP, Mikusincova R, Miller MC, Miniutti G, Motch C, Nattila J, Nardini E, Neubert T, O'Brien PT, Orlandini M, Osborne JP, Pacciani L, Paltani S, Paolillo M, Papadakis IE, Paul B, Pellizzoni A, Peretz U, Torres MAP, Perinati E, Prescod-Weinstein C, Reig P, Riggio A, Rodriguez J, Rodriguez-Gil P, Romano P, Rozanska A, Sakamoto T, Salmi T, Salvaterra R, Sanna A, Santangelo A, Savolainen T, Schanne S, Schatz H, Shao LJ, Shearer A, Shore SN, Stappers B, Strohmayer TE, Suleimanov VF, Svoboda J, Thielemann FK, Tombesi F, Torres DF, Torresi E, Turriziani S, Vacchi A, Vercellone S, Vink J, Wang JM, Wang JF, Watts AL, Weng SS, Weinberg NN, Wheatley PJ, Wijnands R, Woods TE, Woosley SE, Xiong SL, Xu YP, Yan Z, Younes G, Yu WF, Yuan F, Zampieri L, Zane S, Zdziarski AA, Zhang SN, Zhang S, Zhang S, Zhang X, Zingale M, Zingale M, Zhang S, Zhang X
Kustantaja: SCIENCE PRESS
Julkaisuvuosi: 2019
Lehti:SCIENCE CHINA Physics, Mechanics and Astronomy
Tietokannassa oleva lehden nimiSCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
Lehden akronyymi: SCI CHINA PHYS MECH
Artikkelin numero: ARTN 029506
Vuosikerta: 62
Numero: 2
Sivujen määrä: 42
ISSN: 1674-7348
eISSN: 1869-1927
DOI: https://doi.org/10.1007/s11433-017-9186-1
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.
