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Related papers: A fast X-ray timing capability on XEUS

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We describe measurements of the X-ray reflectance in the range 2 to 10 keV of samples representative of coated silicon wafers that are proposed for the fabrication of the XEUS (X-ray Evolving Universe Spectrometer) mission. We compare the…

Astrophysics · Physics 2009-11-13 D. H. Lumb , F. E. Christensen , C. P. Jensen , M. Krumrey

The upcoming launch of the first space based X-ray polarimeter in $\sim 40$ years will provide powerful new diagnostic information to study accreting compact objects. In particular, analysis of rapid variability of the polarisation degree…

High Energy Astrophysical Phenomena · Physics 2017-08-30 Adam Ingram , Tom Maccarone

The Constellation X-ray Mission is a high throughput X-ray facility emphasizing observations at high spectral resolution (E/\Delta E \sim 300-3000), and broad energy bandpass (0.25-40 keV). Constellation-X will provide a factor of nearly…

Astrophysics · Physics 2009-10-31 Azita Valinia , Nicholas White , Harvey Tananbaum , the Constellation-X Team

The European X-ray Free Electron Laser (XFEL.EU) will provide unprecedented peak brilliance and ultra-short and spatially coherent X-ray pulses in an energy range of 0.25 to 25 keV . The pulse timing structure is unique with a burst of 2700…

LOFT, the Large Observatory for X-ray Timing, is a new space mission concept devoted to observations of Galactic and extra-Galactic sources in the X-ray domain with the main goals of probing gravity theory in the very strong field…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 E. Bozzo

The X-ray Timing and Polarization (XTP) is a mission concept for a future space borne X-ray observatory and is currently selected for early phase study. We present a new design of X-ray polarimeter based on the time projection gas chamber.…

Instrumentation and Methods for Astrophysics · Physics 2015-09-16 Hong Li , Hua Feng , Jianfeng Ji , Zhi Deng , Li He , Ming Zeng , Tenglin Li , Yinong Liu , Peiyin Heng , Qiong Wu , Dong Han , Yongwei Dong , Fangjun Lu , Shuangnan Zhang

We have developed an algorithm that, starting from the observed properties of the X-ray spectrum and fast variability of an X-ray binary allows the production of synthetic data reproducing observables such as power density spectra and time…

High Energy Astrophysical Phenomena · Physics 2015-05-19 Y. X. Wu , T. M. Belloni , L. Stella

Observations of thermonuclear X-ray bursts from accreting neutron stars (NSs) in low-mass X-ray binary systems can be used to constrain NS masses and radii. Most previous work of this type has set these constraints using Planck function…

High Energy Astrophysical Phenomena · Physics 2017-12-06 J. Nättilä , M. C. Miller , A. W. Steiner , J. J. E. Kajava , V. F. Suleimanov , J. Poutanen

Some tests of fundamental physics - the equation of state at supra-nuclear densities, the metric in strong gravity, the effect of magnetic fields above the quantum critical value - can only be measured using compact astrophysical objects:…

Astrophysics · Physics 2009-11-11 Martin Elvis

Polarimetry is widely considered a powerful observational technique in X-ray astronomy, useful to enhance our understanding of the emission mechanisms, geometry and magnetic field arrangement of many compact objects. However, the lack of…

Instrumentation and Methods for Astrophysics · Physics 2010-04-28 Ronaldo Bellazzini , Fabio Muleri

Supernova remnants serve as nearby laboratories relevant to many areas in Astrophysics, from stellar and galaxy evolution to extreme astrophysics and the formation of the heavy elements in the Universe. The Chandra X-ray mission has enabled…

High Energy Astrophysical Phenomena · Physics 2019-04-16 Samar Safi-Harb , Elena Amato , Eric V. Gotthelf , Satoru Katsuda , Manami Sasaki , Yasunobu Uchiyama , Naomi Tsuji , Benson Guest

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 Energy Astrophysical Phenomena · Physics 2018-12-12 Jean J. M. in 't Zand , Enrico Bozzo , Jinlu 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 , Xuefeng 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 , Jérôme Chenevez , Maria Chernyakova , Jin Chichuan , Riccardo Ciolfi , Elisa Costantini , Andrew Cumming , Antonino D'Aı , Zi-Gao Dai , Filippo D'Ammando , Massimiliano De Pasquale , Nathalie Degenaar , Melania Del Santo , Valerio D'Elia , Tiziana Di Salvo , Gerry Doyle , Maurizio Falanga , Xilong Fan , Robert D. Ferdman , Marco Feroci , Federico Fraschetti , Duncan K. Galloway , Angelo F. Gambino , Poshak Gandhi , Mingyu Ge , Bruce Gendre , Ramandeep Gill , Diego Götz , Christian Gouiffès , Paola Grandi , Jonathan Granot , Manuel Güdel , Alexander Heger , Craig O. Heinke , Jeroen Homan , Rosario Iaria , Kazushi Iwasawa , Luca Izzo , Long Ji , Peter G. Jonker , Jordi José , Jelle S. Kaastra , Emrah Kalemci , Oleg Kargaltsev , Nobuyuki Kawai , Laurens Keek , Stefanie Komossa , Ingo Kreykenbohm , Lucien Kuiper , Devaky Kunneriath , Gang Li , En-Wei Liang , Manuel Linares , Francesco Longo , Fangjun Lu , Alexander A. Lutovinov , Denys Malyshev , Julien Malzac , Antonios Manousakis , Ian McHardy , Missagh Mehdipour , Yunpeng Men , Mariano Méndez , Roberto P. Mignani , Romana Mikusincova , M. Coleman Miller , Giovanni Miniutti , Christian Motch , Joonas Nättilä , Emanuele Nardini , Torsten Neubert , Paul T. O'Brien , Mauro Orlandini , Julian P. Osborne , Luigi Pacciani , Stéphane Paltani , Maurizio Paolillo , Iossif E. Papadakis , Biswajit Paul , Alberto Pellizzoni , Uria Peretz , Miguel A. Pérez Torres , Emanuele Perinati , Chanda Prescod-Weinstein , Pablo Reig , Alessandro Riggio , Jerome Rodriguez , Pablo Rodrıguez-Gil , Patrizia Romano , Agata Różańska , Takanori Sakamoto , Tuomo Salmi , Ruben Salvaterra , Andrea Sanna , Andrea Santangelo , Tuomas Savolainen , Stéphane Schanne , Hendrik Schatz , Lijing Shao , Andy Shearer , Steven N. Shore , Ben W. Stappers , Tod E. Strohmayer , Valery F. Suleimanov , Jirı Svoboda , F. -K. Thielemann , Francesco Tombesi , Diego F. Torres , Eleonora Torresi , Sara Turriziani , Andrea Vacchi , Stefano Vercellone , Jacco Vink , Jian-Min Wang , Junfeng Wang , Anna L. Watts , Shanshan Weng , Nevin N. Weinberg , Peter J. Wheatley , Rudy Wijnands , Tyrone E. Woods , Stan E. Woosley , Shaolin Xiong , Yupeng Xu , Zhen Yan , George Younes , Wenfei Yu , Feng Yuan , Luca Zampieri , Silvia Zane , Andrzej A. Zdziarski , Shuang-Nan Zhang , Shu Zhang , Shuo Zhang , Xiao Zhang , Michael Zingale

The X-ray emission of neutron stars enables a probe of their temperatures, geometries, and magnetospheric properties. The current number of X-ray emitting pulsars is insufficient to rule out observational biases that may arise from poorly…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Armin Vahdat , Bettina Posselt , Andrea Santangelo , George G. Pavlov

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of high-mass X-ray binaries and ultra-luminous…

The NeXT mission has been proposed to study high-energy non-thermal phenomena in the universe. The high-energy response of the super mirror will enable us to perform the first sensitive imaging observations up to 80 keV. The focal plane…

We are entering a new era for high energy astrophysics with the use of new technology to increase our ability to both survey and monitor the sky. The Soft X-ray Imager (SXI) instrument on the THESEUS mission will revolutionize transient…

The maturity of current detectors based on technologies that range from solid state to gases renewed the interest for X-ray polarimetry, raising the enthusiasm of a wide scientific community to improve the performance of polarimeters as…

Instrumentation and Methods for Astrophysics · Physics 2018-05-14 Sergio Fabiani

Analysis of XRD diffraction patterns is one of the keystones of materials science and materials research. With the advancement of data-driven methods for materials design, candidate materials can be quickly screened for the study of a…

The European X-ray Free Electron Laser (XFEL.EU) will provide as-yet-unrivaled peak brilliance and ultra-short pulses of spatially coherent X-rays with a pulse length of less than 100 fs in the energy range between 0.25 and 25 keV. The high…

Instrumentation and Detectors · Physics 2015-06-15 Jolanta Sztuk-Dambietz , Steffen Hauf , Andreas Koch , Markus Kuster , Monica Turcato
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