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The hard x-ray (10-600 keV) sky is inherently time variable and yet has neither been surveyed nor monitored with a sensitive imaging telescope. The Energetic X-ray Imaging Survey Telescope (EXIST) is a mission concept, proposed for MIDEX,…

Thanks to IXPE , the X-ray spectro-polarimeter launched at the end of 2021, X-ray polarimetry has finally become an extraordinary tool in investigating the physics of accretion in low mass X-ray binaries. Similarly to what happened with…

High Energy Astrophysical Phenomena · Physics 2023-12-25 F. Capitanio , A. Gnarini , S. Fabiani , F. Ursini , R. Farinelli , M. Cocchi , N. Rodriguez Cavero , L. Marra

We report our complete database of X-ray eclipse timings of the low mass X-ray binary EXO0748-676 observed by the Rossi X-Ray Timing Explorer (RXTE) satellite. As of this writing we have accumulated 443 full X-ray eclipses, 392 of which…

Astrophysics · Physics 2009-07-22 Michael T. Wolff , Paul S. Ray , Kent S. Wood , Paul L. Hertz

We investigate the use of deep learning in the context of X-ray polarization detection from astrophysical sources as will be observed by the Imaging X-ray Polarimetry Explorer (IXPE), a future NASA selected space-based mission expected to…

Instrumentation and Methods for Astrophysics · Physics 2020-05-19 Nikita Moriakov , Ashwin Samudre , Michela Negro , Fabian Gieseke , Sydney Otten , Luc Hendriks

This thesis focuses on X-ray polarimetry and its recent resurgence due to the NASA/ASI Imaging X-ray Polarimetry Explorer (IXPE) mission launched in December 2021. It aims to address two critical tasks: in-orbit calibrations and observing…

High Energy Astrophysical Phenomena · Physics 2023-09-22 Riccardo Ferrazzoli

The extreme conditions found near black holes and neutron stars provide a unique opportunity for testing physical theories. Observations of both types of compact objects can be used to probe regions of strong gravity, allowing for tests of…

High Energy Astrophysical Phenomena · Physics 2009-02-25 John A. Tomsick , Andreas Quirrenbach , Shrinivas R. Kulkarni , Stuart B. Shaklan , Xiaopei Pan

Lately a new approach to Extended Reality (XR), denoted as XR-RF, has been proposed which is realized by combining Radio Frequency (RF) Imaging and programmable wireless environments (PWEs). RF Imaging is a technique that aims to detect…

(abridged) With most physicists and astrophysicists in agreement that black holes do indeed exist, the focus of astrophysical black hole research has shifted to the detailed properties of these systems. Nature has provided us with an…

Astrophysics · Physics 2009-11-07 Christopher S. Reynolds , Michael A. Nowak

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

This paper presents L-VITeX, a lightweight visual intuition system for terrain exploration designed for resource-constrained robots and swarms. L-VITeX aims to provide a hint of Regions of Interest (RoIs) without computationally expensive…

Robotics · Computer Science 2024-10-11 Antar Mazumder , Zarin Anjum Madhiha

The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS) and China National Space Administration (CNSA) currently performing an extended phase A study and proposed for a launch by…

The last two decades have seen a great improvement in our understand- ing of the complex phenomenology observed in transient black-hole binary systems, especially thanks to the activity of the Rossi X-Ray Timing Explorer satellite, com-…

High Energy Astrophysical Phenomena · Physics 2016-08-17 T. M. Belloni , S. E. Motta

We report on X-ray monitoring observations of the transient black hole candidate (BHC) XTE J1752-223 with the Rossi X-ray Timing Explorer (RXTE). The source was discovered on 2009 October 23 and during its low/hard state, which lasted for…

High Energy Astrophysical Phenomena · Physics 2011-03-23 H. Stiele , T. Munoz-Darias , S. Motta , T. Belloni

Cosmic Explorer (CE) is a next-generation ground-based gravitational-wave observatory that is being designed in the 2020s and is envisioned to begin operations in the 2030s together with the Einstein Telescope in Europe. The CE concept…

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is currently planned for between 2022 and 2024. LOFT is designed to…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 M. Feroci , J. W. den Herder , E. Bozzo , D. Barret , S. Brandt , M. Hernanz , M. van der Klis , M. Pohl , A. Santangelo , L. Stella , A. Watts , J. Wilms , S. Zane , M. Ahangarianabhari , A. Alpar , D. Altamirano , L. Alvarez , L. Amati , C. Amoros , N. Andersson , A. Antonelli , A. Argan , R. Artigue , P. Azzarello , G. Baldazzi , S. Balman , M. Barbera , T. Belloni , G. Bertuccio , S. Bianchi , A. Bianchini , P. Bodin , J. -M. Bonnet Bidaud , S. Boutloukos , J. Braga , E. Brown , N. Bucciantini , L. Burderi , M. Bursa , C. Budtz-Jørgensen , E. Cackett , F. R. Cadoux , P. Cais , G. A. Caliandro , R. Campana , S. Campana , P. Casella , D. Chakrabarty , J. Chenevez , J. Coker , R. Cole , A. Collura , T. Courvoisier , A. Cros , A. Cumming , G. Cusumano , A. D'Aì , V. D'Elia , E. Del Monte , D. De Martino , A. De Rosa , S. Di Cosimo , S. Diebold , T. Di Salvo , I. Donnarumma , A. Drago , M. Durant , D. Emmanoulopoulos , Y. Evangelista , A. Fabian , M. Falanga , Y. Favre , C. Feldman , C. Ferrigno , M. H. Finger , G. W. Fraser , F. Fuschino , D. K. Galloway , J. L. Galvez Sanchez , E. Garcia-Berro , B. Gendre , S. Gezari , A. B. Giles , M. Gilfanov , P. Giommi , G. Giovannini , M. Giroletti , A. Goldwurm , D. Götz , C. Gouiffes , M. Grassi , P. Groot C. Guidorzi , D. Haas , F. Hansen , D. H. Hartmann , C. A. Haswe , A. Heger , J. Homan , A. Hornstrup , R. Hudec , J. Huovelin , A. Ingram , J. J. M. in't Zand , J. Isern , G. Israe , L. Izzo , P. Jonker , P. Kaaret , V. Karas , D. Karelin , D. Kataria , L. Keek , T. Kennedy , D. Klochkov , W. Kluzniak , K. Kokkotas , S. Korpela , C. Kouveliotou , I. Kreykenbohm , L. M. Kuiper , I. Kuvvetli , C. Labanti , D. Lai , F. K. Lamb , F. Lebrun , D. Lin , D. Linder , G. Lodato , F. Longo , N. Lund , T. J. Maccarone , D. Macera , D. Maier , P. Malcovati , V. Mangano , A. Manousakis , M. Marisaldi , A. Markowitz , A. Martindale , G. Matt , I. M. McHardy , A. Melatos , M. Mendez , S. Migliari , R. Mignani , M. C. Miller , J. M. Miller , T. Mineo , G. Miniutti , S. Morsink , C. Motch , S. Motta , M. Mouchet , F. Muleri , A. J. Norton , M. Nowak , P. O'Brien , M. Orienti , M. Orio , M. Orlandini , P. Orleanski , J. P. Osborne , R. Osten , F. Ozel , L. Pacciani , A. Papitto , B. Paul , E. Perinati , V. Petracek , J. Portell , J. Poutanen , D. Psaltis , D. Rambaud , G. Ramsay , M. Rapisarda , A. Rachevski , P. S. Ray , N. Rea , S. Reddy , P. Reig , M. Reina Aranda , R. Remillard , C. Reynolds , P. Rodríguez-Gil , J. Rodriguez , P. Romano , E. M. R. Rossi , F. Ryde , L. Sabau-Graziati , G. Sala , R. Salvaterra , A. Sanna , S. Schanne , J. Schee , C. Schmid , A. Schwenk , A. D. Schwope , J. -Y. Seyler , A. Shearer , A. Smith , D. M. Smith , P. J. Smith , V. Sochora , P. Soffitta , P. Soleri , B. Stappers , B. Stelzer , N. Stergioulas , G. Stratta , T. E. Strohmayer , Z. Stuchlik , S. Suchy , V. Sulemainov , T. Takahashi , F. Tamburini , C. Tenzer , L. Tolos , G. Torok , J. M. Torrejon , D. F. Torres , A. Tramacere , A. Trois , S. Turriziani , P. Uter , P. Uttley , A. Vacchi , P. Varniere , S. Vaughan , S. Vercellone , V. Vrba , D. Walton , S. Watanabe , R. Wawrzaszek , N. Webb , N. Weinberg , H. Wende , P. Wheatley , R. Wijers , R. Wijnands , M. Wille , C. A. Wilson-Hodge , B. Winter , K. Wood , G. Zampa , N. Zampa , L. Zampieri , A. Zdziarski , B. Zhang

Future direct imaging missions such as HabEx and LUVOIR aim to catalog and characterize Earth-mass analogs around nearby stars. The exoplanet yield of these missions will be dependent on the frequency of Earth-like planets, and potentially…

We report on the discovery of a new pulsating X-ray source during Rossi X-ray Timing Explorer observations of a low galactic latitude field centered at RA (J2000) = 19 hr 05 m 43 s and Dec (J2000) = +08 deg 58 arcmin 48 arcsec. Significant…

Astrophysics · Physics 2009-10-30 D. Marsden , D. E. Gruber , W. A. Heindl , M. R. Pelling , R. E. Rothschild

We discuss the need for very large detection planes for the detection of hard X-ray transients in the multi-messenger era that started with the quasi-simultaneous detection of GRB~170817A by \textit{Fermi}/GBM and \textit{INTEGRAL}/SPI on…

Instrumentation and Methods for Astrophysics · Physics 2019-09-20 K. Lacombe , C. Amoros , J. -L. Atteia , A. Bajat , L. Bouchet , J. -P. Dezalay , P. Guillemot , B. Houret , F. Lebrun , S. Mate , R. Pons , H. Triou , V. Waegebaert

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 active galactic nuclei. For a summary, we…

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