Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31585
DC Field | Value | Language |
---|---|---|
dc.contributor.author | SOFFITTA, PAOLO | en_US |
dc.contributor.author | BUCCIANTINI, NICCOLO' | en_US |
dc.contributor.author | Churazov, Eugene | en_US |
dc.contributor.author | COSTA, ENRICO | en_US |
dc.contributor.author | Dovciak, Michal | en_US |
dc.contributor.author | Feng, Hua | en_US |
dc.contributor.author | Heyl, Jeremy | en_US |
dc.contributor.author | Ingram, Adam | en_US |
dc.contributor.author | Jahoda, Keith | en_US |
dc.contributor.author | Kaaret, Philip | en_US |
dc.contributor.author | Kallman, Timothy | en_US |
dc.contributor.author | Karas, Vladimir | en_US |
dc.contributor.author | Khabibullin, Ildar | en_US |
dc.contributor.author | Krawczynski, Henric | en_US |
dc.contributor.author | Malzac, Julien | en_US |
dc.contributor.author | Marin, Frédéric | en_US |
dc.contributor.author | Marshall, Herman | en_US |
dc.contributor.author | Matt, Giorgio | en_US |
dc.contributor.author | MULERI, FABIO | en_US |
dc.contributor.author | Mundell, Carole | en_US |
dc.contributor.author | Pearce, Mark | en_US |
dc.contributor.author | Petrucci, Pierre-Olivier | en_US |
dc.contributor.author | Poutanen, Juri | en_US |
dc.contributor.author | Romani, Roger | en_US |
dc.contributor.author | Santangelo, Andrea | en_US |
dc.contributor.author | TAGLIAFERRI, Gianpiero | en_US |
dc.contributor.author | Taverna, Roberto | en_US |
dc.contributor.author | Turolla, Roberto | en_US |
dc.contributor.author | Vink, Jacco | en_US |
dc.contributor.author | Zane, Silvia | en_US |
dc.date.accessioned | 2022-03-15T14:52:11Z | - |
dc.date.available | 2022-03-15T14:52:11Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 0922-6435 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31585 | - |
dc.description.abstract | X-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. | en_US |
dc.language.iso | eng | en_US |
dc.title | A polarized view of the hot and violent universe | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s10686-021-09722-y | en_US |
dc.identifier.scopus | 2-s2.0-85105520229 | en_US |
dc.identifier.isi | WOS:000648846100002 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85105520229 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007/s10686-021-09722-y | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 51 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 1109 | en_US |
dc.relation.lastpage | 1141 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | DEU | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | EXPERIMENTAL ASTRONOMY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2021ExA....51.1109S | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0922-6435 | - |
crisitem.journal.ance | E061604 | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0002-7781-4104 | - |
crisitem.author.orcid | 0000-0002-8848-1392 | - |
crisitem.author.orcid | 0000-0003-4925-8523 | - |
crisitem.author.orcid | 0000-0003-3331-3794 | - |
crisitem.author.orcid | 0000-0003-0121-0723 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Soffitta2021_Article_APolarizedViewOfTheHotAndViole.pdf | Pdf editoriale | 2.18 MB | Adobe PDF | View/Open |
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