The enhanced X-ray Timing and Polarimetry mission – eXTP. (arXiv:1812.04020v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_S/0/1/0/all/0/1">ShuangNan Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Santangelo_A/0/1/0/all/0/1">Andrea Santangelo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Feroci_M/0/1/0/all/0/1">Marco Feroci</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Xu_Y/0/1/0/all/0/1">YuPeng Xu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lu_F/0/1/0/all/0/1">FangJun Lu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_Y/0/1/0/all/0/1">Yong Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Feng_H/0/1/0/all/0/1">Hua Feng</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_S/0/1/0/all/0/1">Shu Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brandt_S/0/1/0/all/0/1">S&#xf8;ren Brandt</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hernanz_M/0/1/0/all/0/1">Margarita Hernanz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Baldini_L/0/1/0/all/0/1">Luca Baldini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bozzo_E/0/1/0/all/0/1">Enrico Bozzo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Campana_R/0/1/0/all/0/1">Riccardo Campana</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rosa_A/0/1/0/all/0/1">Alessandra De Rosa</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dong_Y/0/1/0/all/0/1">YongWei Dong</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Evangelista_Y/0/1/0/all/0/1">Yuri Evangelista</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Karas_V/0/1/0/all/0/1">Vladimir Karas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Meidinger_N/0/1/0/all/0/1">Norbert Meidinger</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Meuris_A/0/1/0/all/0/1">Aline Meuris</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Nandra_K/0/1/0/all/0/1">Kirpal Nandra</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pan_T/0/1/0/all/0/1">Teng Pan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pareschi_G/0/1/0/all/0/1">Giovanni Pareschi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Orleanski_P/0/1/0/all/0/1">Piotr Orleanski</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Huang_Q/0/1/0/all/0/1">QiuShi Huang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Schanne_S/0/1/0/all/0/1">Stephane Schanne</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sironi_G/0/1/0/all/0/1">Giorgia Sironi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Spiga_D/0/1/0/all/0/1">Daniele Spiga</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Svoboda_J/0/1/0/all/0/1">Jiri Svoboda</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tagliaferri_G/0/1/0/all/0/1">Gianpiero Tagliaferri</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tenzer_C/0/1/0/all/0/1">Christoph Tenzer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vacchi_A/0/1/0/all/0/1">Andrea Vacchi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zane_S/0/1/0/all/0/1">Silvia Zane</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Walton_D/0/1/0/all/0/1">Dave Walton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wang_Z/0/1/0/all/0/1">ZhanShan Wang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Winter_B/0/1/0/all/0/1">Berend Winter</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wu_X/0/1/0/all/0/1">Xin Wu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zand_J/0/1/0/all/0/1">Jean J.M. in &#x27;t Zand</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ahangarianabhari_M/0/1/0/all/0/1">Mahdi Ahangarianabhari</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ambrosi_G/0/1/0/all/0/1">Giovanni Ambrosi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ambrosino_F/0/1/0/all/0/1">Filippo Ambrosino</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barbera_M/0/1/0/all/0/1">Marco Barbera</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Basso_S/0/1/0/all/0/1">Stefano Basso</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bayer_J/0/1/0/all/0/1">J&#xf6;rg Bayer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bellazzini_R/0/1/0/all/0/1">Ronaldo Bellazzini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bellutti_P/0/1/0/all/0/1">Pierluigi Bellutti</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertucci_B/0/1/0/all/0/1">Bruna Bertucci</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertuccio_G/0/1/0/all/0/1">Giuseppe Bertuccio</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Borghi_G/0/1/0/all/0/1">Giacomo Borghi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cao_X/0/1/0/all/0/1">XueLei Cao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cadoux_F/0/1/0/all/0/1">Franck Cadoux</a>, et al. (100 additional authors not shown)

In this paper we present the enhanced X-ray Timing and Polarimetry mission –
eXTP. eXTP is a space science mission designed to study fundamental physics
under extreme conditions of density, gravity and magnetism. The mission aims at
determining the equation of state of matter at supra-nuclear density, measuring
effects of QED, and understanding the dynamics of matter in strong-field
gravity. In addition to investigating fundamental physics, eXTP will be a very
powerful observatory for astrophysics that will provide observations of
unprecedented quality on a variety of galactic and extragalactic objects. In
particular, its wide field monitoring capabilities will be highly instrumental
to detect the electro-magnetic counterparts of gravitational wave sources. The
paper provides a detailed description of: (1) the technological and technical
aspects, and the expected performance of the instruments of the scientific
payload; (2) the elements and functions of the mission, from the spacecraft to
the ground segment.

In this paper we present the enhanced X-ray Timing and Polarimetry mission –
eXTP. eXTP is a space science mission designed to study fundamental physics
under extreme conditions of density, gravity and magnetism. The mission aims at
determining the equation of state of matter at supra-nuclear density, measuring
effects of QED, and understanding the dynamics of matter in strong-field
gravity. In addition to investigating fundamental physics, eXTP will be a very
powerful observatory for astrophysics that will provide observations of
unprecedented quality on a variety of galactic and extragalactic objects. In
particular, its wide field monitoring capabilities will be highly instrumental
to detect the electro-magnetic counterparts of gravitational wave sources. The
paper provides a detailed description of: (1) the technological and technical
aspects, and the expected performance of the instruments of the scientific
payload; (2) the elements and functions of the mission, from the spacecraft to
the ground segment.

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