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Related papers: X-ray polarimetry on-board HXMT

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X-ray polarization should provide new probes of magnetic field geometry and acceleration physics near the base of blazar jets, but near-future missions will have limited sensitivity. We thus use existing lower energy data and X-ray…

High Energy Astrophysical Phenomena · Physics 2019-08-09 I. Liodakis , A. L. Peirson , R. W. Romani

We report the first results from an X-ray polarimeter with a micropattern gas proportional counter using an amorphous silicon active matrix readout. With 100% polarized X-rays at 4.5 keV, we obtain a modulation factor of 0.33 +/- 0.03,…

Instrumentation and Detectors · Physics 2015-06-26 J. K. Black , P. Deines-Jones , S. E. Ready , R. A. Street

IXPE is a Small Explorer mission that was launched at the end of 2021 to measure the polarization of X-ray emission from tens of astronomical sources. Its focal plane detectors are based on the Gas Pixel Detector, which measures the…

The Galactic plane scanning survey is one of the main scientific objectives of the Hard X-ray Modulation Telescope (known as Insight-HXMT). During the two-year operation of Insight-HXMT, more than 1000 scanning observations have been…

Instrumentation and Methods for Astrophysics · Physics 2020-03-18 Na Sai , JinYuan Liao , ChengKui Li , Ju Guan , Chen Wang , Yi Nang , Yuan Liu , ChengCheng Guo , Shu Zhang , ShuangNan Zhang

The study of magnetars is of particular relevance since these objects are the only laboratories where the physics in ultra-strong magnetic fields can be directly tested. Until now, spectroscopic and timing measurements at X-ray energies in…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Roberto Taverna , Fabio Muleri , Roberto Turolla , Paolo Soffitta , Sergio Fabiani , Luciano Nobili

X-Calibur is a balloon-borne telescope that measures the polarization of high-energy X-rays in the 15--50keV energy range. The instrument makes use of the fact that X-rays scatter preferentially perpendicular to the polarization direction.…

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

Context: Polarimetry is a very powerful tool to uncover various properties of astronomical objects that remain otherwise hidden in standard imaging or spectroscopic observations. However, the reliable measurement of the low polarization…

Instrumentation and Methods for Astrophysics · Physics 2020-02-12 S. González-Gaitán , A. M. Mourão , F. Patat , J. P. Anderson , A. Cikota , K. Wiersema , A. B. Higgins , K. Silva

The Galactic center (GC) holds the closest-to-Earth supermassive black hole (SMBH), which makes it the best laboratory to study the close environment of extremely massive compact objects. Polarimetry is sensitive to geometry of the source,…

High Energy Astrophysical Phenomena · Physics 2014-08-05 F. Marin , V. Karas , D. Kunneriath , F. Muleri , P. Soffitta

The Hard X-ray Modulation Telescope (HXMT) is a broad band X-ray astronomical satellite from 1 to 250 keV. Understanding the X-ray background in detail will help to achieve a good performance of the instrument. In this work, we make use of…

Instrumentation and Methods for Astrophysics · Physics 2015-11-11 Fei Xie , Juan Zhang , Li-Ming Song , Shao-Lin Xiong , Ju Guan

The Hard X-ray Modulation Telescope (Insight-HXMT), is China's first X-ray astronomy satellite launched on June 15, 2017. The anti-coincidence CsI detectors of the High Energy X-ray telescope (HE) onboard Insight-HXMT could serve as an…

The Hard X-ray Modulation Telescope ($Insight$-HXMT) was successfully launched on June 15th, 2017. It performs broad band X-ray scan survey of the Galactic Plane to detect new black holes and other objects in active states. It also observes…

Instrumentation and Methods for Astrophysics · Physics 2022-01-03 S. M. Jia , X. Ma , Y. Huang , W. Z. Zhang , G. Ou , L. M. Song , J. L. Qu , S. Zhang , L. Chen

Polarimetry is an area of high energy astrophysics which is still relatively unexplored, even though it is recognized that this type of measurement could drastically increase our knowledge of the physics and geometry of high energy sources.…

Emission from blazar jets in the ultraviolet, optical, and infrared is polarized. If these low-energy photons were inverse-Compton scattered, the upscattered high-energy photons retain a fraction of the polarization. Current and future…

High Energy Astrophysical Phenomena · Physics 2015-02-03 Nachiketa Chakraborty , Vasiliki Pavlidou , Brian Fields

The Insight-Hard X-ray Modulation Telescope (Insight-HXMT) is a broad band X-ray and gamma-ray (1-3000 keV) astronomy satellite. The High Energy X-ray telescope (HE) is one of its three main telescopes. The main detector plane of HE is…

X-ray polarimetry, sometimes alone, and sometimes coupled to spectral and temporal variability measurements and to imaging, allows a wealth of physical phenomena in astrophysics to be studied. X-ray polarimetry investigates the acceleration…

High Energy Astrophysical Phenomena · Physics 2016-08-11 Paolo Soffitta , Xavier Barcons , Ronaldo Bellazzini , João Braga , Enrico Costa , George W. Fraser , Szymon Gburek , Juhani Huovelin , Giorgio Matt , Mark Pearce , Juri Poutanen , Victor Reglero , Andrea Santangelo , Rashid A. Sunyaev , Gianpiero Tagliaferri , Martin Weisskopf , Roberto Aloisio , Elena Amato , Primo Attiná , Magnus Axelsson , Luca Baldini , Stefano Basso , Stefano Bianchi , Pasquale Blasi , Johan Bregeon , Alessandro Brez , Niccoló Bucciantini , Luciano Burderi , Vadim Burwitz , Piergiorgio Casella , Eugene Churazov , Marta Civitani , Stefano Covino , Rui Miguel Curado da Silva , Giancarlo Cusumano , Mauro Dadina , Flavio D'Amico , Alessandra De Rosa , Sergio Di Cosimo , Giuseppe Di Persio , Tiziana Di Salvo , Michal Dovciak , Ronald Elsner , Chris J. Eyles , Andrew C. Fabian , Sergio Fabiani , Hua Feng , Salvatore Giarrusso , René W. Goosmann , Paola Grandi , Nicolas Grosso , Gianluca Israel , Miranda Jackson , Philip Kaaret , Vladimir Karas , Michael Kuss , Dong Lai , Giovanni La Rosa , Josefin Larsson , Stefan Larsson , Luca Latronico , Antonio Maggio , Jorge Maia , Frédéric Marin , Marco Maria Massai , Teresa Mineo , Massimo Minuti , Elena Moretti , Fabio Muleri , Stephen L. O'Dell , Giovanni Pareschi , Giovanni Peres , Melissa Pesce , Pierre-Olivier Petrucci , Michele Pinchera , Delphine Porquet , Brian Ramsey , Nanda Rea , Fabio Reale , Juana Maria Rodrigo , Agata Różańska , Alda Rubini , Pawel Rudawy , Felix Ryde , Marco Salvati , Valdivino Alexandre de Santiago Júnior , Sergey Sazonov , Carmelo Sgró , Eric Silver , Gloria Spandre , Daniele Spiga , Luigi Stella , Toru Tamagawa , Francesco Tamborra , Fabrizio Tavecchio , Teresa Teixeira Dias , Matthew van Adelsberg , Kinwah Wu , Silvia Zane

The Sun is the nearest astrophysical source with a very intense emission in the X-ray band. The study of energetic events, such as solar flares, can help us to understand the behaviour of the magnetic field of our star. There are in the…

eXTP is a science mission designed to study the state of matter under extreme conditions of density, gravity and magnetism. Primary targets include isolated and binary neutron stars, strong magnetic field systems like magnetars, and…

Instrumentation and Methods for Astrophysics · Physics 2020-03-17 S. N. Zhang , M. Feroci , A. Santangelo , Y. W. Dong , H. Feng , F. J. Lu , K. Nandra , Z. S. Wang , S. Zhang , E. Bozzo , S. Brandt , A. De Rosa , L. J. Gou , M. Hernanz , M. van der Klis , X. D. Li , Y. Liu , P. Orleanski , G. Pareschi , M. Pohl , J. Poutanen , J. L. Qu , S. Schanne , L. Stella , P. Uttley , A. Watts , R. X. Xu , W. F. Yu , J. J. M. in 't Zand , S. Zane , L. Alvarez , L. Amati , L. Baldini , C. Bambi , S. Basso , S. Bhattacharyya , R. Bellazzini , T. Belloni , P. Bellutti , S. Bianchi , A. Brez , M. Bursa , V. Burwitz , C. Budtz-Jorgensen , I. Caiazzo , R. Campana , X. L. Cao , P. Casella , C. Y. Chen , L. Chen , T. X. Chen , Y. Chen , Y. Chen , Y. P. Chen , M. Civitani , F. Coti Zelati , W. Cui , W. W. Cui , Z. G. Dai , E. Del Monte , D. De Martino , S. Di Cosimo , S. Diebold , M. Dovciak , I. Donnarumma , V. Doroshenko , P. Esposito , Y. Evangelista , Y. Favre , P. Friedrich , F. Fuschino , J. L. Galvez , Z. L. Gao , M. Y. Ge , O. Gevin , D. Goetz , D. W. Han , J. Heyl , J. Horak , W. Hu , F. Huang , Q. S. Huang , R. Hudec , D. Huppenkothen , G. L. Israel , A. Ingram , V. Karas , D. Karelin , P. A. Jenke , L. Ji , T. Kennedy , S. Korpela , D. Kunneriath , C. Labanti , G. Li , X. Li , Z. S. Li , E. W. Liang , O. Limousin , L. Lin , Z. X. Ling , H. B. Liu , H. W. Liu , Z. Liu , B. Lu , N. Lund , D. Lai , B. Luo , T. Luo , B. Ma , S. Mahmoodifar , M. Marisaldi , A. Martindale , N. Meidinger , Y. P. Men , M. Michalska , R. Mignani , M. Minuti , S. Motta , F. Muleri , J. Neilsen , M. Orlandini , A T. Pan , A. Patruno , E. Perinati , A. Picciotto , C. Piemonte , M. Pinchera , A. Rachevski , M. Rapisarda , N. Rea , E. M. R. Rossi , A. Rubini , G. Sala , X. W. Shu , C. Sgro , Z. X. Shen , P. Soffitta , L. M. Song , G. Spandre , G. Stratta , T. E. Strohmayer , L. Sun , J. Svoboda , G. Tagliaferri , C. Tenzer , H. Tong , R. Taverna , G. Torok , R. Turolla , A. Vacchi , J. Wang , J. X. Wang , D. Walton , K. Wang , J. F. Wang , R. J. Wang , Y. F. Wang , S. S. Weng , J. Wilms , B. Winter , X. Wu , X. F. Wu , S. L. Xiong , Y. P. Xu , Y. Q. Xue , Z. Yan , S. Yang , X. Yang , Y. J. Yang , F. Yuan , W. M. Yuan , Y. F. Yuan , G. Zampa , N. Zampa , A. Zdziarski , C. Zhang , C. L. Zhang , L. Zhang , X. Zhang , Z. Zhang , W. D. Zhang , S. J. Zheng , P. Zhou , X. L. Zhou

X-ray polarimetry is still largely uncharted territory. With the upcoming launch of IXPE, we will learn a lot more about X-ray polarization at energies above 2 keV, but so far no current or accepted mission provides observational…

Instrumentation and Methods for Astrophysics · Physics 2020-12-01 Hans Moritz Günther , Herman L. Marshall , Alan Garner

The INFN and INAF Italian research institutes developed a space-borne X-Ray polarimetry experiment based on a X-Ray telescope, focussing the radiation on a Gas Pixel Detector (GPD). The instrument obtains the polarization angle of the…