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X-ray Polarimetry of X-ray Pulsars
GalaxiesRadiation from X-ray pulsars (XRPs) was expected to be strongly linearly polarized owing to a large difference in their ordinary and extraordinary mode opacities. The launch of IXPE allowed us to check this prediction. IXPE observed a dozen X-ray pulsars,Juri Poutanen, Sergey S. Tsygankov, Sofia V. Forsblom +2 moredoaj +4 more sourcesX-Ray Polarimetry as a Tool to Constrain Orbital Parameters in X-Ray Binaries
The Astrophysical JournalX-ray binary systems consist of a companion star and a compact object in close orbit. Thanks to their copious X-ray emission, these objects have been studied in detail using X-ray spectroscopy and timing.John Rankin, Vadim Kravtsov, Fabio Muleri, Juri Poutanen, Frédéric Marin, Fiamma Capitanio, Giorgio Matt, Enrico Costa, Alessandro Di Marco, Sergio Fabiani, Fabio La Monaca, Lorenzo Marra, Paolo Soffitta +12 moredoaj +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 +3 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 moreopenaire +10 more sourcesBroadband soft x-ray polarimetry [PDF]
SPIE Proceedings, 2010 We developed an instrument design capable of measuring linear X-ray polarization over a broad-band using conventional spectroscopic optics. A set of multilayer-coated flats reflects the dispersed X-rays to the instrument detectors. The intensity variation with position angle is measured to determine three Stokes parameters: I, Q, and U -- all as a ...Schulz, Norbert S., Murphy, Kendrah Dawn, Marshall, Herman, Heilmann, Ralf K +3 moreopenaire +4 more sourcesDeep ensemble analysis for Imaging X-ray Polarimetry [PDF]
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2021 18 pages, 9 figures.Peirson, A. L., Romani, R. W., Marshall, H. L., Steiner, J. F., Baldini, L. +4 moreopenaire +2 more sourcesEqualizing the Pixel Response of the Imaging Photoelectric Polarimeter Onboard the IXPE Mission
The Astronomical Journal, 2023 The Gas Pixel Detector is a gas detector, sensitive to the polarization of X-rays, currently flying onboard the Imaging X-ray Polarimetry Explorer (IXPE)—the first observatory dedicated to X-ray polarimetry.John Rankin, Fabio Muleri, Alessandro Di Marco, Sergio Fabiani, Fabio La Monaca, Paolo Soffitta, Matteo Bachetti, Luca Baldini, Enrico Costa, Niccolò Di Lalla, Alberto Manfreda, Stephen L. O’Dell, Matteo Perri, Simonetta Puccetti, Brian D. Ramsey, Carmelo Sgrò, Allyn F. Tennant, Antonino Tobia, Alessio Trois, Martin C. Weisskopf, Fei Xie +20 moredoaj +1 more source