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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 3 CONTRIBUTI IN ATTI DI CONVEGNO (Proceedings)
  4. 3.01 Contributi in Atti di convegno
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/31385
DC FieldValueLanguage
dc.contributor.authorLABANTI, CLAUDIOen_US
dc.contributor.authorAMATI, LORENZOen_US
dc.contributor.authorFrontera, F.en_US
dc.contributor.authorMEREGHETTI, Sandroen_US
dc.contributor.authorGasent-Blesa, J. L.en_US
dc.contributor.authorTenzer, C.en_US
dc.contributor.authorOrleanski, P.en_US
dc.contributor.authorKuvvetli, I.en_US
dc.contributor.authorCAMPANA, RICCARDOen_US
dc.contributor.authorFUSCHINO, FABIOen_US
dc.contributor.authorTERENZI, LUCAen_US
dc.contributor.authorVirgilli, E.en_US
dc.contributor.authorMORGANTE, GIANLUCAen_US
dc.contributor.authorORLANDINI, MAUROen_US
dc.contributor.authorButler, R. C.en_US
dc.contributor.authorSTEPHEN, JOHN BUCHANen_US
dc.contributor.authorAURICCHIO, NATALIAen_US
dc.contributor.authorDe Rosa, A.en_US
dc.contributor.authorDa Ronco, V.en_US
dc.contributor.authorEvangelisti, F.en_US
dc.contributor.authorMelchiorri, M.en_US
dc.contributor.authorSquerzanti, S.en_US
dc.contributor.authorFIORINI, MAUROen_US
dc.contributor.authorBertuccio, G.en_US
dc.contributor.authorMele, F.en_US
dc.contributor.authorGandola, M.en_US
dc.contributor.authorMalcovati, P.en_US
dc.contributor.authorGrassi, M.en_US
dc.contributor.authorBellutti, P.en_US
dc.contributor.authorBorghi, G.en_US
dc.contributor.authorFicorella, F.en_US
dc.contributor.authorPicciotto, A.en_US
dc.contributor.authorZANINI, Valeriaen_US
dc.contributor.authorZorzi, N.en_US
dc.contributor.authorDemenev, E.en_US
dc.contributor.authorRashevskaya, I.en_US
dc.contributor.authorRachevski, A.en_US
dc.contributor.authorZampa, G.en_US
dc.contributor.authorVacchi, A.en_US
dc.contributor.authorZampa, N.en_US
dc.contributor.authorBaldazzi, G.en_US
dc.contributor.authorLA ROSA, GIOVANNIen_US
dc.contributor.authorSOTTILE, Giuseppeen_US
dc.contributor.authorVolpe, A.en_US
dc.contributor.authorWinkler, M.en_US
dc.contributor.authorReglero, V.en_US
dc.contributor.authorConnell, P. H.en_US
dc.contributor.authorPinazo-Herrero, B.en_US
dc.contributor.authorNavarro-González, J.en_US
dc.contributor.authorRodríguez-Martínez, P.en_US
dc.contributor.authorCastro-Tirado, A. J.en_US
dc.contributor.authorSantangelo, A.en_US
dc.contributor.authorHedderman, P.en_US
dc.contributor.authorLorenzi, P.en_US
dc.contributor.authorSarra, P.en_US
dc.contributor.authorPedersen, S. M.en_US
dc.contributor.authorTcherniak, D.en_US
dc.contributor.authorGuidorzi, C.en_US
dc.contributor.authorRosati, P.en_US
dc.contributor.authorTROIS, ALESSIOen_US
dc.contributor.authorPIAZZOLLA, RAFFAELEen_US
dc.date.accessioned2022-02-11T11:24:46Z-
dc.date.available2022-02-11T11:24:46Z-
dc.date.issued2020en_US
dc.identifier.isbn9781510636750en_US
dc.identifier.isbn9781510636767en_US
dc.identifier.issn0277-786Xen_US
dc.identifier.urihttp://hdl.handle.net/20.500.12386/31385-
dc.description.abstractTHESEUS (Transient High Energy Sky and Early Universe Surveyor) is one of the three missions selected by ESA as fifth medium class mission (M5) candidates in its Cosmic Vision science program, currently under assessment in a phase A study with a planned launch date in 2032. THESEUS is designed to carry on-board two wide and deep sky monitoring instruments for X/gamma-ray transients detection: a wide-field soft X-ray monitor with imaging capability (Soft X-ray Imager, SXI, 0.3 - 5 keV), a hard X-ray, partially-imaging spectroscopic instrument (X and Gamma Imaging Spectrometer, XGIS, 2 keV - 10 MeV), and an optical/near-IR telescope with both imaging and spectroscopic capability (InfraRed Telescope, IRT, 0.7 - 1.8 μm). The spacecraft will be capable of performing fast repointing of the IRT to the error region provided by the monitors, thus allowing it to detect and localize the transient sources down to a few arcsec accuracy, for immediate identification and redshift determination. The prime goal of the XGIS will be to detect transient sources, with monitoring timescales down to milliseconds, both independently of, or following up, SXI detections, and identify the sources performing localisation at <15 arcmin and characterize them over a broad energy band, thus providing also unique clues to their emission physics. The XGIS system consists of two independent but identical coded mask cameras, arranged to cover 2 steradians. The XGIS will exploit an innovative technology coupling Silicon Drift Detectors (SDD) with crystal scintillator bars and a very low-noise distributed front-end electronics (ORION ASICs), which will produce a position sensitive detection plane, with a large effective area over a huge energy band (from soft X-rays to soft gamma-rays) with timing resolution down to a few µs. Here is presented an overview of the XGIS instrument design, its configuration, and capabilities.en_US
dc.language.isoengen_US
dc.titleThe X/Gamma-ray Imaging Spectrometer (XGIS) on-board THESEUS: design, main characteristics, and concept of operationen_US
dc.typeConference paper-
dc.identifier.doi10.1117/12.2561012en_US
dc.identifier.scopus2-s2.0-85099276079en_US
dc.identifier.isiWOS:000674737700036en_US
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85099276079en_US
dc.identifier.urlhttps://www.spiedigitallibrary.org/conference-proceedings-of-spie/11444/2561012/The-X-Gamma-ray-Imaging-Spectrometer-XGIS-on-board-THESEUS/10.1117/12.2561012.fullen_US
dc.relation.mediumSTAMPAen_US
dc.relation.volume11444en_US
dc.relation.firstpage114442Ken_US
dc.type.refereeREF_0en_US
dc.description.internationalsìen_US
dc.contributor.countryITAen_US
dc.contributor.countryDEUen_US
dc.contributor.countryESPen_US
dc.contributor.countryDNKen_US
dc.contributor.countryPOLen_US
dc.relation.alleditorsden Herder, Jan-Willem A.; Nikzad, Shouleh; Nakazawa, Kazuhiroen_US
dc.relation.ispartofbookSpace Telescopes and Instrumentation 2020: Ultraviolet to Gamma Rayen_US
dc.publisher.nameSPIE, The International Society for Optical Engineeringen_US
dc.publisher.placeBELLINGHAM, WA 98227-0010 USAen_US
dc.relation.conferencenameSpace Telescopes and Instrumentation 2020: Ultraviolet to Gamma Rayen_US
dc.relation.conferenceplaceCalifornia, United Statesen_US
dc.relation.conferencedate14-18 December, 2020en_US
dc.relation.scientificsectorFIS/05 - ASTRONOMIA E ASTROFISICAen_US
dc.type.miur273 Contributo in Atti di convegno-
dc.relation.seriesPROCEEDINGS OF SPIEen_US
dc.identifier.adsbibcode2020SPIE11444E..2KLen_US
dc.description.apcnoen_US
dc.description.oa1 – prodotto con file in versione Open Access (allegare il file al passo  5-Carica)en_US
item.grantfulltextopen-
item.fulltextWith Fulltext-
item.openairetypeConference paper-
item.languageiso639-1en-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.journal.journalissn0277-786X-
crisitem.journal.anceE136238-
crisitem.author.deptOAS Bologna-
crisitem.author.deptIASF Milano-
crisitem.author.deptOAS Bologna-
crisitem.author.deptOAS Bologna-
crisitem.author.deptOAS Bologna-
crisitem.author.deptOAS Bologna-
crisitem.author.deptOAS Bologna-
crisitem.author.deptOAS Bologna-
crisitem.author.deptOAS Bologna-
crisitem.author.deptIASF Milano-
crisitem.author.deptO.A. Padova-
crisitem.author.deptIASF Palermo-
crisitem.author.deptO.A. Cagliari-
crisitem.author.orcid0000-0002-5086-3619-
crisitem.author.orcid0000-0001-5355-7388-
crisitem.author.orcid0000-0003-3259-7801-
crisitem.author.orcid0000-0002-4794-5453-
crisitem.author.orcid0000-0003-2139-3299-
crisitem.author.orcid0000-0001-9915-6379-
crisitem.author.orcid0000-0001-9234-7412-
crisitem.author.orcid0000-0003-0946-3151-
crisitem.author.orcid0000-0002-6017-0592-
crisitem.author.orcid0000-0003-4444-8651-
crisitem.author.orcid0000-0001-8297-1983-
crisitem.author.orcid0000-0001-5258-9994-
crisitem.author.orcid0000-0002-3931-2269-
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crisitem.author.orcid0000-0002-3180-6002-
crisitem.author.orcid0000-0002-4222-6919-
Appears in Collections:3.01 Contributi in Atti di convegno
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