Observatory science with eXTP

Jean J.M. in ’t Zand; Enrico Bozzo; Jin Lu Qu; Xiang Dong Li; Lorenzo Amati; Yang Chen; Immacolata Donnarumma; Victor Doroshenko; Stephen A. Drake; Margarita Hernanz; Peter A. Jenke; Thomas J. Maccarone; Simin Mahmoodifar; Domitilla de Martino; Alessandra De Rosa; Elena M. Rossi; Antonia Rowlinson; Gloria Sala; Giulia Stratta; Thomas M. Tauris; Joern Wilms; Xue Feng Wu; Ping Zhou; Iván Agudo; Diego Altamirano; Jean Luc Atteia; Nils A. Andersson; M. Cristina Baglio; David R. Ballantyne; Altan Baykal; Ehud Behar; Tomaso Belloni; Sudip Bhattacharyya; Stefano Bianchi; Anna Bilous; Pere Blay; João Braga; Søren Brandt; Edward F. Brown; Niccolò Bucciantini; Luciano Burderi; Edward M. Cackett; Riccardo Campana; Sergio Campana; Piergiorgio Casella; Yuri Cavecchi; Frank Chambers; Liang Chen; Yu Peng Chen; Tuomas Savolainen

doi:10.1007/s11433-017-9186-1

Observatory science with eXTP

Jean J.M. in ’t Zand^*, Enrico Bozzo, Jin Lu Qu, Xiang Dong Li, Lorenzo Amati, Yang Chen, Immacolata Donnarumma, Victor Doroshenko, Stephen A. Drake, Margarita Hernanz, Peter A. Jenke, Thomas J. Maccarone, Simin Mahmoodifar, Domitilla de Martino, Alessandra De Rosa, Elena M. Rossi, Antonia Rowlinson, Gloria Sala, Giulia Stratta, Thomas M. TaurisJoern Wilms, Xue Feng Wu, Ping Zhou, Iván Agudo, Diego Altamirano, Jean Luc Atteia, Nils A. Andersson, M. Cristina Baglio, David R. Ballantyne, Altan Baykal, Ehud Behar, Tomaso Belloni, Sudip Bhattacharyya, Stefano Bianchi, Anna Bilous, Pere Blay, João Braga, Søren Brandt, Edward F. Brown, Niccolò Bucciantini, Luciano Burderi, Edward M. Cackett, Riccardo Campana, Sergio Campana, Piergiorgio Casella, Yuri Cavecchi, Frank Chambers, Liang Chen, Yu Peng Chen, Tuomas Savolainen

^*Corresponding author for this work

Research output: Contribution to journal › Review Article › peer-review

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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.

Original language	English
Article number	029506
Number of pages	42
Journal	Science China: Physics, Mechanics and Astronomy
Volume	62
Issue number	2
DOIs	https://doi.org/10.1007/s11433-017-9186-1
Publication status	Published - 1 Feb 2019
MoE publication type	A2 Review article, Literature review, Systematic review

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

Access to Document

10.1007/s11433-017-9186-1

ELEC-savolainen-et-al-eXTP_WP_OS_vs8nov2017Accepted author manuscript, 5.35 MB

Cite this

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., ... Savolainen, T. (2019). Observatory science with eXTP. Science China: Physics, Mechanics and Astronomy, 62(2), Article 029506. https://doi.org/10.1007/s11433-017-9186-1

@article{4510bf6d82fe4a6fb3c0f5802bd94ddf,

title = "Observatory science with eXTP",

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.",

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",

author = "{in {\textquoteright}t Zand}, {Jean J.M.} and Enrico Bozzo and Qu, {Jin Lu} and Li, {Xiang Dong} and Lorenzo Amati and Yang Chen and Immacolata Donnarumma and Victor Doroshenko and Drake, {Stephen A.} and Margarita Hernanz and Jenke, {Peter A.} and Maccarone, {Thomas J.} and Simin Mahmoodifar and {de Martino}, Domitilla and {De Rosa}, Alessandra and Rossi, {Elena M.} and Antonia Rowlinson and Gloria Sala and Giulia Stratta and Tauris, {Thomas M.} and Joern Wilms and Wu, {Xue Feng} and Ping Zhou and Iv{\'a}n Agudo and Diego Altamirano and Atteia, {Jean Luc} and Andersson, {Nils A.} and Baglio, {M. Cristina} and Ballantyne, {David R.} and Altan Baykal and Ehud Behar and Tomaso Belloni and Sudip Bhattacharyya and Stefano Bianchi and Anna Bilous and Pere Blay and Jo{\~a}o Braga and S{\o}ren Brandt and Brown, {Edward F.} and Niccol{\`o} Bucciantini and Luciano Burderi and Cackett, {Edward M.} and Riccardo Campana and Sergio Campana and Piergiorgio Casella and Yuri Cavecchi and Frank Chambers and Liang Chen and Chen, {Yu Peng} and Tuomas Savolainen",

year = "2019",

month = feb,

day = "1",

doi = "10.1007/s11433-017-9186-1",

language = "English",

volume = "62",

journal = "Science China: Physics, Mechanics and Astronomy",

issn = "1674-7348",

publisher = "Science in China Press",

number = "2",

}

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 & Savolainen, T 2019, 'Observatory science with eXTP', Science China: Physics, Mechanics and Astronomy, vol. 62, no. 2, 029506. https://doi.org/10.1007/s11433-017-9186-1

TY - JOUR

T1 - Observatory science with eXTP

AU - in ’t Zand, Jean J.M.

AU - Bozzo, Enrico

AU - Qu, Jin Lu

AU - Li, Xiang Dong

AU - Amati, Lorenzo

AU - Chen, Yang

AU - Donnarumma, Immacolata

AU - Doroshenko, Victor

AU - Drake, Stephen A.

AU - Hernanz, Margarita

AU - Jenke, Peter A.

AU - Maccarone, Thomas J.

AU - Mahmoodifar, Simin

AU - de Martino, Domitilla

AU - De Rosa, Alessandra

AU - Rossi, Elena M.

AU - Rowlinson, Antonia

AU - Sala, Gloria

AU - Stratta, Giulia

AU - Tauris, Thomas M.

AU - Wilms, Joern

AU - Wu, Xue Feng

AU - Zhou, Ping

AU - Agudo, Iván

AU - Altamirano, Diego

AU - Atteia, Jean Luc

AU - Andersson, Nils A.

AU - Baglio, M. Cristina

AU - Ballantyne, David R.

AU - Baykal, Altan

AU - Behar, Ehud

AU - Belloni, Tomaso

AU - Bhattacharyya, Sudip

AU - Bianchi, Stefano

AU - Bilous, Anna

AU - Blay, Pere

AU - Braga, João

AU - Brandt, Søren

AU - Brown, Edward F.

AU - Bucciantini, Niccolò

AU - Burderi, Luciano

AU - Cackett, Edward M.

AU - Campana, Riccardo

AU - Campana, Sergio

AU - Casella, Piergiorgio

AU - Cavecchi, Yuri

AU - Chambers, Frank

AU - Chen, Liang

AU - Chen, Yu Peng

AU - Savolainen, Tuomas

PY - 2019/2/1

Y1 - 2019/2/1

N2 - 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.

AB - 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.

KW - accretion and accretion disks

KW - active galactic nuclei

KW - cataclysmic binaries

KW - flare stars

KW - gamma-ray bursts

KW - gravitational waves

KW - mass loss and stellar winds

KW - nuclear astrophysics

KW - space research instruments

KW - supernova remnants

KW - X-ray binaries

KW - X-ray bursts

UR - http://www.scopus.com/inward/record.url?scp=85052723351&partnerID=8YFLogxK

U2 - 10.1007/s11433-017-9186-1

DO - 10.1007/s11433-017-9186-1

M3 - Review Article

AN - SCOPUS:85052723351

SN - 1674-7348

VL - 62

JO - Science China: Physics, Mechanics and Astronomy

JF - Science China: Physics, Mechanics and Astronomy

IS - 2

M1 - 029506

ER -

Observatory science with eXTP

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Observatory science with eXTP

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