Observatory science with eXTP

DOI: 
10.1007/s11433-017-9186-1
Publication date: 
16/01/2019
Main author: 
in ’t Zand J.J.M.
IAA authors: 
Agudo, I.;Izzo, L.;Pérez Torres, M.A.
Authors: 
in ’t Zand J.J.M., Bozzo E., Qu J.L., Li X.-D., Amati L., Chen Y., Donnarumma I., Doroshenko V., Drake S.A., Hernanz M., Jenke P.A., Maccarone T.J., Mahmoodifar S., de Martino D., De Rosa A., Rossi E.M., Rowlinson A., Sala G., Stratta G., Tauris T.M., Wilms J., Wu X.F., Zhou P., Agudo I., Altamirano D., Atteia J.-L., Andersson N.A., Baglio M.C., Ballantyne D.R., Baykal A., Behar E., Belloni T., Bhattacharyya S., Bianchi S., Bilous A., Blay P., Braga J., Brandt S., Brown E.F., Bucciantini N., Burderi L., Cackett E.M., Campana R., Campana S., Casella P., Cavecchi Y., Chambers F., Chen L., Chen Y.-P., Chenevez J., Chernyakova M., Jin C.C., Ciolfi R., Costantini E., Cumming A., D’Aì A., Dai Z.-G., D’Ammando F., De Pasquale M., Degenaar N., Del Santo M., D’Elia V., Di Salvo T., Doyle G., Falanga M., Fan X.L., Ferdman R.D., Feroci M., Fraschetti F., Galloway D.K., Gambino A.F., Gandhi P., Ge M.Y., Gendre B., Gill R., Götz D., Gouiffès C., Grandi P., Granot J., Güdel M., Heger A., Heinke C.O., Homan J., Iaria R., Iwasawa K., Izzo L., Ji L., Jonker P.G., José J., Kaastra J.S., Kalemci E., Kargaltsev O., Kawai N., Keek L., Komossa S., Kreykenbohm I., Kuiper L., Kunneriath D., Li G., Liang E.-W., Linares M., Longo F., Lu F.J., Lutovinov A.A., Malyshev D., Malzac J., Manousakis A., McHardy I., Mehdipour M., Men Y.P., Méndez M., Mignani R.P., Mikusincova R., Miller M.C., Miniutti G., Motch C., Nättilä J., Nardini E., Neubert T., O’Brien P.T., Orlandini M., Osborne J.P., Pacciani L., Paltani S., Paolillo M., Papadakis I.E., Paul B., Pellizzoni A., Peretz U., Pérez Torres M.A., Perinati E., Prescod-Weinstein C., Reig P., Riggio A., Rodriguez J., Rodríguez-Gil P., Romano P., Różańska A., Sakamoto T., Salmi T., Salvaterra R., Sanna A., Santangelo A., Savolainen T., Schanne S., Schatz H., Shao L.J., Shearer A., Shore S.N., Stappers B.W., Strohmayer T.E., Suleimanov V.F., Svoboda J., Thielemann F.-K., Tombesi F., Torres D.F., Torresi E., Turriziani S., Vacchi A., Vercellone S., Vink J., Wang J.-M., Wang J.F., Watts A.L., Weng S.S., Weinberg N.N., Wheatley P.J., Wijnands R., Woods T.E., Woosley S.E., Xiong S.L., Xu Y.P., Yan Z., Younes G., Yu W.F., Yuan F., Zampieri L., Zane S., Zdziarski A.A., Zhang S.-N., Zhang S., Zhang S., Zhang X., Zingale M.
Journal: 
Science China: Physics, Mechanics and Astronomy
Refereed: 
Yes
Publication type: 
Article
Volume: 
62
Pages: 
29506
Number: 
29506
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. © 2018, Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature.
Database: 
SCOPUS
ADS
URL: 
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85052723351&doi=10.1007%2fs11433-017-9186-1&partnerID=40&md5=82c1eb8b76a202d285280dde1dc81823
ADS Bibcode: 
2019SCPMA..6229506I
Keywords: 
accretion and accretion disks; active galactic nuclei; cataclysmic binaries; flare stars; gamma-ray bursts; gravitational waves; mass loss and stellar winds; nuclear astrophysics; space research instruments; supernova remnants; X-ray binaries; X-ray bursts