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X-rays are particularly suited to probe the physics of extreme objects. However, despite the enormous improvements of X-ray Astronomy in imaging, spectroscopy and timing, polarimetry remains largely unexplored. We propose the photoelectric…

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…

高能天体物理现象 · 物理学 2023-09-22 Riccardo Ferrazzoli

Due to be launched in late 2021, the Imaging X-Ray Polarimetry Explorer (IXPE) is a NASA Small Explorer mission designed to perform polarization measurements in the 2-8 keV band, complemented with imaging, spectroscopy and timing…

The Gas Pixel Detector, recently developed and continuously improved by Pisa INFN in collaboration with IASF-Roma of INAF, can visualize the tracks produced within a low Z gas by photoelectrons of few keV. By reconstructing the impact point…

天体物理仪器与方法 · 物理学 2014-11-20 F. Muleri , R. Bellazzini , A. Brez , E. Costa , F. Lazzarotto , M. Minuti , M. Pinchera , A. Rubini , P. Soffitta , G. Spandre

This paper discusses issues encountered during the early development of the instrument on the Imaging X-ray Polarimetry Explorer (IXPE), a NASA ASI Small Explorer mission launched on 9 December 2021. IXPE has observed about 100 sources,…

The Gas Pixel Detector (GPD) is a new generation device which, thanks to its 50 um pixels, is capable of imaging the photoelectrons tracks produced by photoelectric absorption in a gas. Since the direction of emission of the photoelectrons…

The gas pixel detector (GPD) dedicated for photoelectric X-ray polarimetry is selected as the focal plane detector for the ESA medium-class mission concept X-ray Imaging and Polarimetry Explorer (XIPE). Here we show the design, assembly,…

天体物理仪器与方法 · 物理学 2015-12-09 H. Li , H. Feng , F. Muleri , R. Bellazzini , M. Minuti , P. Soffitta , A. Brez , G. Spandre , M. Pinchera , C. Sgro , L. Baldini , R. She , E. Costa

We report on the results of a new, sealed, Gas Pixel Detector. The very compact design and the absence of the gas flow system, make this detector substantially ready for use as focal plane detector for future X-ray space telescopes. The…

The gas pixel detector (GPD) is designed and developed for high-sensitivity astronomical X-ray polarimetry, which is a new window about to open in a few years. Due to the small mass, low power, and compact geometry of the GPD, we propose a…

The Gas Pixel Detector was designed and built as a focal plane instrument for X-ray polarimetry of celestial sources, the last unexplored subtopics of X-ray astronomy. It promises to perform detailed and sensitive measurements resolving…

Since the birth of X-ray Astronomy, spectacular advances have been seen in the imaging, spectroscopic and timing studies of the hot and violent X-ray Universe, and further leaps forward are expected in the future. On the other hand,…

The Gas Pixel Detector is an X-ray polarimeter to fly on-board IXPE and other missions. To correctly measure the source polarization, the response of IXPE's GPDs to unpolarized radiation has to be calibrated and corrected. In this paper we…

X-ray polarimetry, based on Gas Pixel Detectors (GPDs), have reached a high level of maturity with the Imaging X-ray Polarimeter Explorer (IXPE) leading to the first ever spatially resolved polarimetric measures. However, being this a new…

天体物理仪器与方法 · 物理学 2023-04-05 N. Bucciantini , N. Di Lalla , R. W. R. Romani , S. Silvestri , M. Negro , L. Baldini , A. F. Tennant , A. Manfreda

We discuss a new class of Micro Pattern Gas Detectors, the Gas Pixel Detector (GPD), in which a complete integration between the gas amplification structure and the read-out electronics has been reached. An Application-Specific Integrated…

Gaseous X-ray polarimetry refers to a class of detectors used for measuring the polarization of soft X-rays. The systematic effects of such detectors introduce residual modulation, leading to systematic biases in the polarization detection…

天体物理仪器与方法 · 物理学 2024-07-22 Difan Yi , Qian Liu , Hongbang Liu , Fei Xie , Huanbo Feng , Zuke Feng , Jin Li , Enwei Liang , Yangheng Zheng

While X-ray Spectroscopy, Timing and Imaging have improved verymuch since 1962, when the first astronomical non-solar source was discovered, especially with the launch of Newton/X-ray Multi-Mirror Mission, Rossi/X-ray Timing Explorer and…

The Low Energy Polarization Detector (LPD) is a key component of the next-generation large-scale Gamma-Ray Burst polarimeter, POLAR-2. It is designed for polarization observations of transient sources in the soft X-ray energy range with a…

Scheduled to launch in late 2021, the Imaging X-ray Polarimetry Explorer (IXPE) is a NASA Small Explorer Mission in collaboration with the Italian Space Agency (ASI). The mission will open a new window of investigation - imaging X-ray…

天体物理仪器与方法 · 物理学 2021-12-22 Martin C. Weisskopf , Paolo Soffitta , Luca Baldini , Brian D. Ramsey , Stephen L. O'Dell , Roger W. Romani , Giorgio Matt , William D. Deininger , Wayne H. Baumgartner , Ronaldo Bellazzini , Enrico Costa , Jeffery J. Kolodziejczak , Luca Latronico , Herman L. Marshall , Fabio Muleri , Stephen D. Bongiorno , Allyn Tennant , Niccolo Bucciantini , Michal Dovciak , Frederic Marin , Alan Marscher , Juri Poutanen , Pat Slane , Roberto Turolla , William Kalinowski , Alessandro Di Marco , Sergio Fabiani , Massimo Minuti , Fabio La Monaca , Michele Pinchera , John Rankin , Carmelo Sgro' , Alessio Trois , Fei Xie , Cheryl Alexander , D. Zachery Allen , Fabrizio Amici , Jason Andersen , Angelo Antonelli , Spencer Antoniak , Primo Attina' , Mattia Barbanera , Matteo Bachetti , Randy M. Baggett , Jeff Bladt , Alessandro Brez , Raffaella Bonino , Christopher Boree , Fabio Borotto , Shawn Breeding , Daniele Brienza , H. Kyle Bygott , Ciro Caporale , Claudia Cardelli , Rita Carpentiero , Simone Castellano , Marco Castronuovo , Luca Cavalli , Elisabetta Cavazzuti , Marco Ceccanti , Mauro Centrone , Saverio Citraro , Fabio D' Amico , Elisa D'Alba , Laura Di Gesu , Ettore Del Monte , Kurtis L. Dietz , Niccolo' Di Lalla , Giuseppe Di Persio , David Dolan , Immacolata Donnarumma , Yuri Evangelista , Kevin Ferrant , Riccardo Ferrazzoli , MacKenzie Ferrie , Joseph Footdale , Brent Forsyth , Michelle Foster , Benjamin Garelick , Shuichi Gunji , Eli Gurnee , Michael Head , Grant Hibbard , Samantha Johnson , Erik Kelly , Kiranmayee Kilaru , Carlo Lefevre , Shelley Le Roy , Pasqualino Loffredo , Paolo Lorenzi , Leonardo Lucchesi , Tyler Maddox , Guido Magazzu , Simone Maldera , Alberto Manfreda , Elio Mangraviti , Marco Marengo , Alessandra Marrocchesi , Francesco Massaro , David Mauger , Jeffrey McCracken , Michael McEachen , Rondal Mize , Paolo Mereu , Scott Mitchell , Ikuyuki Mitsuishi , Alfredo Morbidini , Federico Mosti , Hikmat Nasimi , Barbara Negri , Michela Negro , Toan Nguyen , Isaac Nitschke , Alessio Nuti , Mitch Onizuka , Chiara Oppedisano , Leonardo Orsini , Darren Osborne , Richard Pacheco , Alessandro Paggi , Will Painter , Steven D. Pavelitz , Christina Pentz , Raffaele Piazzolla , Matteo Perri , Melissa Pesce-Rollins , Colin Peterson , Maura Pilia , Alessandro Profeti , Simonetta Puccetti , Jaganathan Ranganathan , Ajay Ratheesh , Lee Reedy , Noah Root , Alda Rubini , Stephanie Ruswick , Javier Sanchez , Paolo Sarra , Francesco Santoli , Emanuele Scalise , Andrea Sciortino , Christopher Schroeder , Tim Seek , Kalie Sosdian , Gloria Spandre , Chet O. Speegle , Toru Tamagawa , Marcello Tardiola , Antonino Tobia , Nicholas E. Thomas , Robert Valerie , Marco Vimercati , Amy L. Walden , Bruce Weddendorf , Jeffrey Wedmore , David Welch , Davide Zanetti , Francesco Zanetti

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.…

Launched on December 9, 2021, the Imaging X-ray Polarimetry Explorer (IXPE) is the first imaging polarimeter ever flown, providing sensitivity in the 2--8 keV range, and during the 2-year initial phase of the mission will sample tens of…

天体物理仪器与方法 · 物理学 2023-03-21 Stefano Silvestri
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