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The Imaging X-ray Polarimetry Explorer (IXPE) [PDF]
Results in Physics, 2016 The Imaging X-ray Polarimetry Explorer (IXPE) expands observation space by simultaneously adding polarization to the array of X-ray source properties currently measured (energy, time, and location).Martin C. Weisskopf, Brian Ramsey, Stephen L. O’Dell, Allyn Tennant, Ronald Elsner, Paolo Soffita, Ronaldo Bellazzini, Enrico Costa, Jeffery Kolodziejczak, Victoria Kaspi, Fabio Mulieri, Herman Marshall, Giorgio Matt, Roger Romani +13 moredoaj +11 more sourcesXIPE: the x-ray imaging polarimetry explorer [PDF]
Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 2016 XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric ...Soffitta P., Bellazzini R., Bozzo E., Burwitz V., Castro-Tirado A. J., Costa E., Courvoisier T., Feng H., Gburek S., Goosmann R., Karas V., Matt G., Muleri F., Nandra K., Pearce M., Poutanen J., Reglero V., Sabau Maria D., Santangelo A., Tagliaferri G., Tenzer C., Vink J., Weisskopf M. C., Zane S., Agudo I., Antonelli A., Attina P., Baldini L., Bykov A., Carpentiero R., Cavazzuti E., Churazov E., Del Monte E., De Martino D., Donnarumma I., Doroshenko V., Evangelista Y., Ferreira I., Gallo E., Grosso N., Kaaret P., Kuulkers E., Laranaga J., Latronico L., Lumb D. H., Macian J., Malzac J., Marin F., Massaro E., Minuti M., Mundell C., Ness J. U., Oosterbroek T., Paltani S., Pareschi G., Perna R., Petrucci P. -O., Pinazo H. B., Pinchera M., Rodriguez J. P., Roncadelli M., Santovincenzo A., Sazonov S., Sgro C., Spiga D., Svoboda J., Theobald C., Theodorou T., Turolla R., Wilhelmi De Ona E., Winter B., Akbar A. M., Allan H., Aloisio R., Altamirano D., Amati L., Amato E., Angelakis E., Arezu J., Atteia J. -L., Axelsson M., Bachetti M., Ballo L., Balman S., Bandiera R., Barcons X., Basso S., Baykal A., Becker W., Behar E., Beheshtipour B., Belmont R., Berger E., Bernardini F., Bianchi S., Bisnovatyi-Kogan G., Blasi P., Blay P., Bodaghee A., Boer M., Boettcher M., Bogdanov S., Bombaci I., Bonino R., Braga J., Brandt W., Brez A., Bucciantini N., Burderi L., Caiazzo I., Campana R., Campana S., Capitanio F., Cappi M., Cardillo M., Casella P., Catmabacak O., Cenko B., Cerda-Duran P., Cerruti C., Chaty S., Chauvin M., Chen Y., Chenevez J., Chernyakova M., Cheung Teddy C. C., Christodoulou D., Connell P., Corbet R., Coti Zelati F., Covino S., Cui W., Cusumano G., D'Ai A., D'Ammando F., Dadina M., Dai Z., De Rosa A., De Ruvo L., Degenaar N., Del Santo M., Del Zanna L., Dewangan G., Di Cosimo S., Di Lalla N., Di Persio G., Di Salvo T., Dias T., Done C., Dovciak M., Doyle G., Ducci L., Elsner R., Enoto T., Escada J., Esposito P., Eyles C., Fabiani S., Falanga M., Falocco S., Fan Y., Fender R., Feroci M., Ferrigno C., Forman W., Foschini L., Fragile C., Fuerst F., Fujita Y., Gasent-Blesa J. L., Gelfand J., Gendre B., Ghirlanda G., Ghisellini G., Giroletti M., Goetz D., Gogus E., Gomez J. -L., Gonzalez D., Gonzalez-Riestra R., Gotthelf E., Gou L., Grandi P., Grinberg V., Grise F., Guidorzi C., Gurlebeck N., Guver T., Haggard D., Hardcastle M., Hartmann D., Haswell C., Heger A., Hernanz M., Heyl J., Ho L., Hoormann J., Horak J., Huovelin J., Huppenkothen D., Iaria R., Israel G., Izzo L., Kajava J. J. E., Kallman T., Kong A., Kowalinski M., Linares M., Lister M., Liu H., Lodato G., Lohfink A., Longo F., Luna G., Maia J., Mainieri V., Malyshev D., Manfreda A., Manousakis A., Marinucci A., Mehdipour M., Mignani R., Mineo T., Mingo B., Miniutti G., Morlino G., Nattila J., Neustroev V., Nicastro F., Nucita A., Olmi B., Omodei N., Orienti M., Orlandini M., Papadakis I., Papitto A., Pellizzoni A., Porquet D., Postnov K., Prandoni I., Produit N., Razzano M., Rea N., Reig P., Reiprich T., Risaliti G., Roberts T., Rozanska A., Rudak B., Russell D., Savolainen T., Scaringi S., Shearer A., Spandre G., Stamerra A., Stergioulas N., Suleimanov V., Slowikowska A., Tavecchio F., Tolos L., Tombesi F., Torok G., Tortosa A., Tramacere A., Tsygankov S., Turriziani S., Ursini F., Varniere P., Vurgun E., Wijnands R., Wilms J., Zanin R., Zdziarski A. A., Zhang H. +273 morecore +23 more sourcesX-ray Polarimetry-Timing
, 2023 X-ray polarimetry-timing is the characterization of rapid variability in the X-ray polarization degree and angle. As for the case of spectral-timing, it provides causal information valuable for reconstructing indirect maps of the vicinity of compact objects. To call X-ray polarimetry-timing a young field is somewhat of an understatement, given that the Ingram, Adamopenaire +3 more sourcesX-ray polarimetry on-board of HXMT [PDF]
SPIE Proceedings, 2008 The development of micropixel gas detectors, capable to image tracks produced in a gas by photoelectrons, makes possible to perform polarimetry of X-ray celestial sources in the focus of grazing incidence X-ray telescopes. HXMT is a mission by the Chinese Space Agency aimed to survey the Hard X-ray Sky with Phoswich detectors, by exploitation of the ...Soffitta Paolo, Bellazzini Ronaldo, Tagliaferri Gianpiero, Costa Enrico, Pareschi Giovanni, Basso Stefano, Cotroneo Vincenzo, Frutti Massimo, Lazzarotto Francesco, Muleri Fabio, Rubini Alda, Spaiidre Gloria, Bez Alessandro, BALDINI, LUCA, Bregeon Jean, Minuti Massimo, Matt Giorgio, Frontera Fillipo, BE Turner MJL, Flanagan KA +19 moreopenaire +4 more sourcesixpeobssim: A simulation and analysis framework for the imaging X-ray polarimetry explorer
SoftwareX, 2022 ixpeobssim is a simulation and analysis framework specifically developed for the Imaging X-ray Polarimetry Explorer (IXPE). Given a source model and the response functions of the telescopes, it is designed to produce realistic simulated observations, in ...Luca Baldini, Niccolò Bucciantini, Niccolò Di Lalla, Steven Ehlert, Alberto Manfreda, Michela Negro, Nicola Omodei, Melissa Pesce-Rollins, Carmelo Sgrò, Stefano Silvestri +9 moredoaj +3 more sourcesThe Instrument of the Imaging X-Ray Polarimetry Explorer [PDF]
The Astronomical Journal, 2021 Abstract While X-ray spectroscopy, timing, and imaging have improved much since 1962 when the first astronomical nonsolar source was discovered, especially wi the launch of the Newton/X-ray Multi-Mirror Mission, Rossi/X-ray Timing Explorer, and Chandra/Advanced X-ray Astrophysics Facility, the progress of X-ray polarimetry has been ...Paolo Soffitta, Luca Baldini, Ronaldo Bellazzini, Enrico Costa, Luca Latronico, Fabio Muleri, Ettore Del Monte, Sergio Fabiani, Massimo Minuti, Michele Pinchera, Carmelo Sgro’, Gloria Spandre, Alessio Trois, Fabrizio Amici, Hans Andersson, Primo Attina’, Matteo Bachetti, Mattia Barbanera, Fabio Borotto, Alessandro Brez, Daniele Brienza, Ciro Caporale, Claudia Cardelli, Rita Carpentiero, Simone Castellano, Marco Castronuovo, Luca Cavalli, Elisabetta Cavazzuti, Marco Ceccanti, Mauro Centrone, Stefano Ciprini, Saverio Citraro, Fabio D’Amico, Elisa D’Alba, Sergio Di Cosimo, Niccolo’ Di Lalla, Alessandro Di Marco, Giuseppe Di Persio, Immacolata Donnarumma, Yuri Evangelista, Riccardo Ferrazzoli, Asami Hayato, Takao Kitaguchi, Fabio La Monaca, Carlo Lefevre, Pasqualino Loffredo, Paolo Lorenzi, Leonardo Lucchesi, Carlo Magazzu, Simone Maldera, Alberto Manfreda, Elio Mangraviti, Marco Marengo, Giorgio Matt, Paolo Mereu, Alfredo Morbidini, Federico Mosti, Toshio Nakano, Hikmat Nasimi, Barbara Negri, Seppo Nenonen, Alessio Nuti, Leonardo Orsini, Matteo Perri, Melissa Pesce-Rollins, Raffaele Piazzolla, Maura Pilia, Alessandro Profeti, Simonetta Puccetti, John Rankin, Ajay Ratheesh, Alda Rubini, Francesco Santoli, Paolo Sarra, Emanuele Scalise, Andrea Sciortino, Toru Tamagawa, Marcello Tardiola, Antonino Tobia, Marco Vimercati, Fei Xie +80 morecore +7 more sourcesX-RAY AND GAMMA-RAY POLARIMETRY OF GRBS [PDF]
EAS Publications Series, 2013 Polarimetry is expected to play a major role as a diagnostic tool for GRBs. Techniques and methods for X/Gamma ray polarimetry are reviewed including the specific problems related to the transient nature of the sources. Optical data do not encourage optimistic predictions on polarimetry of afterglows.E. Costaopenaire +2 more sources
