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Related papers: Science objectives of the Einstein Probe mission

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The hard X-ray emission from magnetars and other isolated neutron stars remains under-explored. An instrument with higher sensitivity to hard X-rays is critical to understanding the physics of neutron star magnetospheres and also the…

HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging ($<10"$ FWHM) and broad spectral coverage (0.2-80 keV) with an effective area far superior to current facilities' (including XMM-Newton and…

We present in detail the scientific objectives in fundamental physics of the Space-Time Explorer and QUantum Equivalence Space Test (STE-QUEST) space mission. STE-QUEST was pre-selected by the European Space Agency together with four other…

Gravitational waves (GWs) are expected to play a crucial role in the development of multimessenger astrophysics. The combination of GW observations with other astrophysical triggers, such as from gamma-ray and X-ray satellites,…

General Relativity and Quantum Cosmology · Physics 2011-01-28 Eric Chassande-Mottin , Martin Hendry , Patrick J. Sutton , Szabolcs Márka

Current constraints on Einstein's weak equivalence principle (WEP) utilize the observed time delay between correlated particles of astronomical sources. However, the intrinsic time delay due to particle emission time is impossible to…

High Energy Astrophysical Phenomena · Physics 2018-09-26 H. Yu , F. Y. Wang

We construct simulated galaxy data sets based on the High Energy X-ray Probe (HEX-P) mission concept to demonstrate the significant advances in galaxy science that will be yielded by the HEX-P observatory. The combination of high spatial…

Low-cost mass-produced sensors and optics have recently made it feasible to build telescope arrays which observe the entire accessible sky simultaneously. In this article we discuss the scientific motivation for these telescopes, including…

An extremely sensitive all-sky survey will be carried out in the millimetre/submillimetre waveband by the forthcoming ESA mission Planck Surveyor. The main scientific goal of the mission is to make very accurate measurements of the spatial…

Astrophysics · Physics 2009-10-30 Andrew W. Blain

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a…

Instrumentation and Methods for Astrophysics · Physics 2018-06-13 L. Amati , P. O'Brien , D. Goetz , E. Bozzo , C. Tenzer , F. Frontera , G. Ghirlanda , C. Labanti , J. P. Osborne , G. Stratta , N. Tanvir , R. Willingale , P. Attina , R. Campana , A. J. Castro-Tirado , C. Contini , F. Fuschino , A. Gomboc , R. Hudec , P. Orleanski , E. Renotte , T. Rodic , Z. Bagoly , A. Blain , P. Callanan , S. Covino , A. Ferrara , E. Le Floch , M. Marisaldi , S. Mereghetti , P. Rosati , A. Vacchi , P. D'Avanzo , P. Giommi , A. Gomboc , S. Piranomonte , L. Piro , V. Reglero , A. Rossi , A. Santangelo , R. Salvaterra , G. Tagliaferri , S. Vergani , S. Vinciguerra , M. Briggs , E. Campolongo , R. Ciolfi , V. Connaughton , B. Cordier , B. Morelli , M. Orlandini , C. Adami , A. Argan , J. -L. Atteia , N. Auricchio , L. Balazs , G. Baldazzi , S. Basa , R. Basak , P. Bellutti , M. G. Bernardini , G. Bertuccio , J. Braga , M. Branchesi , S. Brandt , E. Brocato , C. Budtz-Jorgensen , A. Bulgarelli , L. Burderi , J. Camp , S. Capozziello , J. Caruana , P. Casella , B. Cenko , P. Chardonnet , B. Ciardi , S. Colafrancesco , M. G. Dainotti , V. D'Elia , D. De Martino , M. De Pasquale , E. Del Monte , M. Della Valle , A. Drago , Y. Evangelista , M. Feroci , F. Finelli , M. Fiorini , J. Fynbo , A. Gal-Yam , B. Gendre , G. Ghisellini , A. Grado , C. Guidorzi , M. Hafizi , L. Hanlon , J. Hjorth , L. Izzo , L. Kiss , P. Kumar , I. Kuvvetli , M. Lavagna , T. Li , F. Longo , M. Lyutikov , U. Maio , E. Maiorano , P. Malcovati , D. Malesani , R. Margutti , A. Martin-Carrillo , N. Masetti , S. McBreen , R. Mignani , G. Morgante , C. Mundell , H. U. Nargaard-Nielsen , L. Nicastro , E. Palazzi , S. Paltani , F. Panessa , G. Pareschi , A. Pe'er , A. V. Penacchioni , E. Pian , E. Piedipalumbo , T. Piran , G. Rauw , M. Razzano , A. Read , L. Rezzolla , P. Romano , R. Ruffini , S. Savaglio , V. Sguera , P. Schady , W. Skidmore , L. Song , E. Stanway , R. Starling , M. Topinka , E. Troja , M. van Putten , E. Vanzella , S. Vercellone , C. Wilson-Hodge , D. Yonetoku , G. Zampa , N. Zampa , B. Zhang , B. B. Zhang , S. Zhang , S. -N. Zhang , A. Antonelli , F. Bianco , S. Boci , M. Boer , M. T. Botticella , O. Boulade , C. Butler , S. Campana , F. Capitanio , A. Celotti , Y. Chen , M. Colpi , A. Comastri , J. -G. Cuby , M. Dadina , A. De Luca , Y. -W. Dong , S. Ettori , P. Gandhi , E. Geza , J. Greiner , S. Guiriec , J. Harms , M. Hernanz , A. Hornstrup , I. Hutchinson , G. Israel , P. Jonker , Y. Kaneko , N. Kawai , K. Wiersema , S. Korpela , V. Lebrun , F. Lu , A. MacFadyen , G. Malaguti , L. Maraschi , A. Melandri , M. Modjaz , D. Morris , N. Omodei , A. Paizis , P. Pata , V. Petrosian , A. Rachevski , J. Rhoads , F. Ryde , L. Sabau-Graziati , N. Shigehiro , M. Sims , J. Soomin , D. Szecsi , Y. Urata , M. Uslenghi , L. Valenziano , G. Vianello , S. Vojtech , D. Watson , J. Zicha

Scheduled for launch in 2030, the enhanced X-ray Timing and Polarization (eXTP) telescope is a Chinese space-based mission aimed at studying extreme conditions and phenomena in astrophysics. eXTP will feature three main payloads:…

The Extreme-ultraviolet Stellar Characterization for Atmospheric Physics and Evolution (ESCAPE) mission is an astrophysics Small Explorer employing ultraviolet spectroscopy (EUV: 80 - 825 \AA\ and FUV: 1280 - 1650 \AA) to explore the…

Instrumentation and Methods for Astrophysics · Physics 2022-02-01 K. France , B. Fleming , A. Youngblood , J. Mason , J. Drake , the ESCAPE Science , Instrument Team

The Einstein Telescope (ET) is a proposed next-generation, underground gravitational-wave (GW) detector to be based in Europe. It will provide about an order of magnitude sensitivity increase with respect to currently operating detectors,…

Einstein Telescope (ET) is a planned third generation gravitational waves detector located in Europe. Its design will be different from currently build interferometers, because ET will consist of three interferometers rotated by a 60 deg…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-25 I. Kowalska-Leszczynska , T. Bulik

Long gamma-ray bursts (GRBs) are believed to originate from core collapse of massive stars. High-redshift GRBs can probe the star formation and reionization history of the early universe, but their detection remains rare. Here we report the…

High Energy Astrophysical Phenomena · Physics 2024-04-26 Y. Liu , H. Sun , D. Xu , D. S. Svinkin , J. Delaunay , N. R. Tanvir , H. Gao , C. Zhang , Y. Chen , X. -F. Wu , B. Zhang , W. Yuan , J. An , G. Bruni , D. D. Frederiks , G. Ghirlanda , J. -W. Hu , A. Li , C. -K. Li , J. -D. Li , D. B. Malesani , L. Piro , G. Raman , R. Ricci , E. Troja , S. D. Vergani , Q. -Y. Wu , J. Yang , B. -B. Zhang , Z. -P. Zhu , A. de Ugarte Postigo , A. G. Demin , D. Dobie , Z. Fan , S. -Y. Fu , J. P. U. Fynbo , J. -J. Geng , G. Gianfagna , Y. -D. Hu , Y. -F. Huang , S. -Q. Jiang , P. G. Jonker , Y. Julakanti , J. A. Kennea , A. A. Kokomov , E. Kuulkers , W. -H. Lei , J. K. Leung , A. J. Levan , D. -Y. Li , Y. Li , S. P. Littlefair , X. Liu , A. L. Lysenko , Y. -N. Ma , A. Martin-Carrillo , P. O'Brien , T. Parsotan , J. Quirola-Vasquez , A. V. Ridnaia , S. Ronchini , A. Rossi , D. Mata-Sanchez , B. Schneider , R. -F. Shen , A. L. Thakur , A. Tohuvavohu , M. A. P. Torres , A. E. Tsvetkova , M. V. Ulanov , J. -J. Wei , D. Xiao , Y. -H. I. Yin , M. Bai , V. Burwitz , Z. -M. Cai , F. -S. Chen , H. -L. Chen , T. -X. Chen , W. Chen , Y. -F. Chen , Y. -H. Chen , H. -Q. Cheng , C. -Z. Cui , W. -W. Cui , Y. -F. Dai , Z. -G. Dai , J. Eder , D. -W. Fan , C. Feldman , H. Feng , Z. Feng , P. Friedrich , X. Gao , J. Guan , D. -W Han , J. Han , D. -J. Hou , H. -B. Hu , T. Hu , M. -H. Huang , J. Huo , I. Hutchinson , Z. Ji , S. -M. Jia , Z. -Q. Jia , B. -W. Jiang , C. -C. Jin , G. Jin , J. -J. Jin , A. Keereman , H. Lerman , J. -F. Li , L. -H. Li , M. -S. Li , W. Li , Z. -D. Li , T. -Y. Lian , E. -W. Liang , Z. -X. Ling , C. -Z. Liu , H. -Y. Liu , H. -Q. Liu , M. -J. Liu , Y. -R. Liu , F. -J. Lu , H. -J. LU , L. -D. Luo , F. L. Ma , J. Ma , J. -R. Mao , X. Mao , M. McHugh , N. Meidinger , K. Nandra , J. P. Osborne , H. -W. Pan , X. Pan , M. E. Ravasio , A. Rau , N. Rea , U. Rehman , J. Sanders , A. Santovincenzo , L. -M. Song , J. Su , L. -J. Sun , S. -L. Sun , X. -J. Sun , Y. -Y. Tan , Q. -J. Tang , Y. -H. Tao , J. -Z. Tong , H. Wang , J. Wang , L. Wang , W. -X. Wang , X. -F. Wang , X. -Y. Wang , Y. -L. Wang , Y. -S. Wang , D. -M. Wei , R. Willingale , S. -L. Xiong , H. -T. Xu , J. -J. Xu , X. -P. Xu , Y. -F. Xu , Z. Xu , C. -B. Xue , Y. -L. Xue , A. -L. Yan , F. Yang , H. -N. Yang , X. -T. Yang , Y. -J Yang , Y. -W. Yu , J. Zhang , M. Zhang , S. -N. Zhang , W. -D. Zhang , W. -J. Zhang , Y. -H. Zhang , Z. Zhang , Z. Zhang , Z. -L. Zhang , D. -H. Zhao , H. -S. Zhao , X. -F. Zhao , Z. -J. Zhao , L. -X. Zhou , Y. -L. Zhou , Y. -X. Zhu , Z. -C. Zhu , X. -X. Zuo

The Einstein Telescope is a proposed third generation gravitational wave detector that will operate in the region of 1 Hz to a few kHz. As well as the inspiral of compact binaries composed of neutron stars or black holes, the lower…

General Relativity and Quantum Cosmology · Physics 2011-01-28 Leone Bosi , Edward K. Porter

The Einstein Telescope (ET) is going to bring a revolution for the future of multi-messenger astrophysics. In order to detect the counterparts of binary neutron star (BNS) mergers at high redshift, the high-energy observations will play a…

We present the results of our multi-wavelength (X-ray to radio) follow-up campaign of the Einstein Probe transient EP240408a. The initial 10 s trigger displayed bright soft X-ray (0.5-4 keV) radiation with peak luminosity $L_\textrm{X}…

We report on the result of an extensive search for X-ray counterparts to Gamma Ray Bursts (GRB) using data acquired with the Imaging Proportional Counter (IPC) on-board the Einstein Observatory. We examine background sky fields from all…

Astrophysics · Physics 2009-10-28 E. V. Gotthelf , T. T. Hamilton , D. J. Helfand

Einstein's weak equivalence principle (WEP) states that any freely falling, uncharged test particle follows the same identical trajectory independent of its internal structure and composition. Since the polarization of a photon is…

High Energy Astrophysical Phenomena · Physics 2017-05-05 Xue-Feng Wu , Jun-Jie Wei , Mi-Xiang Lan , He Gao , Zi-Gao Dai , Peter Mészáros