A polarized view of the hot and violent universe

dc.contributor.authorSoffitta Paolo
dc.contributor.authorBucciantini Niccolo’
dc.contributor.authorChurazov Eugene
dc.contributor.authorCosta Enrico
dc.contributor.authorDovciak Michal
dc.contributor.authorFeng Hua
dc.contributor.authorHeyl Jeremy
dc.contributor.authorIngram Adam
dc.contributor.authorJahoda Keith
dc.contributor.authorKaaret Philip
dc.contributor.authorKallman Timothy
dc.contributor.authorKaras Vladimir
dc.contributor.authorKhabibullin Ildar
dc.contributor.authorKrawczynski Henric
dc.contributor.authorMalzac Julien
dc.contributor.authorMarin Frédéric
dc.contributor.authorMarshall Herman
dc.contributor.authorMatt Giorgio
dc.contributor.authorMuleri Fabio
dc.contributor.authorMundell Carole
dc.contributor.authorPearce Mark
dc.contributor.authorPetrucci Pierre-Olivier
dc.contributor.authorPoutanen Juri
dc.contributor.authorRomani Roger
dc.contributor.authorSantangelo Andrea
dc.contributor.authorTagliaferri Gianpiero
dc.contributor.authorTaverna Roberto
dc.contributor.authorTurolla Roberto
dc.contributor.authorVink Jacco
dc.contributor.authorZane Silvia
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organization-code1.2.246.10.2458963.20.90670098848
dc.converis.publication-id59148943
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/59148943
dc.date.accessioned2022-10-27T11:55:39Z
dc.date.available2022-10-27T11:55:39Z
dc.description.abstractX-ray polarimetry has long been considered the 'holy grail' of X-ray astronomy. Fortunately, after a silence of more than 40 years, the field is now rejuvenating. In fact, an X-ray polarimeter onboard a Cube-sat nano-satellite has been recently successfully operated. IXPE, the Imaging X-ray Polarimetry Explorer, will be launched in 2021 while eXTP, containing a larger version of IXPE, is expected to be launched in 2027. Although at present it is difficult to predict the discoveries that, given their exploratory nature, IXPE and eXTP will obtain, the path for a follow-up mission can already be envisaged. In this paper we describe the scientific goals of such a follow-up mission, and present a medium-size mission profile that can accomplish this task.
dc.identifier.eissn1572-9508
dc.identifier.jour-issn0922-6435
dc.identifier.olddbid172856
dc.identifier.oldhandle10024/155950
dc.identifier.urihttps://www.utupub.fi/handle/11111/55000
dc.identifier.urlhttps://link.springer.com/article/10.1007/s10686-021-09722-y
dc.identifier.urnURN:NBN:fi-fe2021093047987
dc.language.isoen
dc.okm.affiliatedauthorPoutanen, Juri
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherSPRINGER
dc.publisher.countryNetherlandsen_GB
dc.publisher.countryAlankomaatfi_FI
dc.publisher.country-codeNL
dc.relation.doi10.1007/s10686-021-09722-y
dc.relation.ispartofjournalExperimental Astronomy
dc.source.identifierhttps://www.utupub.fi/handle/10024/155950
dc.titleA polarized view of the hot and violent universe
dc.year.issued2021

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