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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/31858
DC FieldValueLanguage
dc.contributor.authorTanvir, N. R.en_US
dc.contributor.authorLe Floc'h, E.en_US
dc.contributor.authorChristensen, L.en_US
dc.contributor.authorCaruana, J.en_US
dc.contributor.authorSALVATERRA, Rubenen_US
dc.contributor.authorGHIRLANDA, Giancarloen_US
dc.contributor.authorCiardi, B.en_US
dc.contributor.authorMaio, U.en_US
dc.contributor.authorD'ODORICO, Valentinaen_US
dc.contributor.authorPiedipalumbo, E.en_US
dc.contributor.authorCAMPANA, Sergioen_US
dc.contributor.authorNoterdaeme, P.en_US
dc.contributor.authorGraziani, L.en_US
dc.contributor.authorAMATI, LORENZOen_US
dc.contributor.authorBagoly, Z.en_US
dc.contributor.authorBalázs, L. G.en_US
dc.contributor.authorBasa, S.en_US
dc.contributor.authorBehar, E.en_US
dc.contributor.authorDe Cia, A.en_US
dc.contributor.authorDELLA VALLE, Massimoen_US
dc.contributor.authorDe Pasquale, M.en_US
dc.contributor.authorFrontera, F.en_US
dc.contributor.authorGomboc, A.en_US
dc.contributor.authorGötz, D.en_US
dc.contributor.authorHorvath, I.en_US
dc.contributor.authorHudec, R.en_US
dc.contributor.authorMEREGHETTI, Sandroen_US
dc.contributor.authorO'Brien, P. T.en_US
dc.contributor.authorOsborne, J. P.en_US
dc.contributor.authorPaltani, S.en_US
dc.contributor.authorRosati, P.en_US
dc.contributor.authorSergijenko, O.en_US
dc.contributor.authorStanway, E. R.en_US
dc.contributor.authorSzécsi, D.en_US
dc.contributor.authorToth, L. V.en_US
dc.contributor.authorUrata, Y.en_US
dc.contributor.authorVergani, S.en_US
dc.contributor.authorZane, S.en_US
dc.date.accessioned2022-03-24T11:36:56Z-
dc.date.available2022-03-24T11:36:56Z-
dc.date.issued2021en_US
dc.identifier.issn0922-6435en_US
dc.identifier.urihttp://hdl.handle.net/20.500.12386/31858-
dc.description.abstractAt peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star formation and star-forming galaxies over the whole of cosmic history. Their bright power-law afterglows provide ideal backlights for absorption studies of the interstellar and intergalactic medium back to the reionization era. The proposed THESEUS mission is designed to detect large samples of GRBs at z > 6 in the 2030s, at a time when supporting observations with major next generation facilities will be possible, thus enabling a range of transformative science. THESEUS will allow us to explore the faint end of the luminosity function of galaxies and the star formation rate density to high redshifts; constrain the progress of re-ionisation beyond z ≳6 ; study in detail early chemical enrichment from stellar explosions, including signatures of Population III stars; and potentially characterize the dark energy equation of state at the highest redshifts.en_US
dc.language.isoengen_US
dc.titleExploration of the high-redshift universe enabled by THESEUSen_US
dc.typeArticle-
dc.identifier.doi10.1007/s10686-021-09778-wen_US
dc.identifier.scopus2-s2.0-85111671470en_US
dc.identifier.urlhttps://link.springer.com/article/10.1007/s10686-021-09778-wen_US
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85111671470en_US
dc.relation.mediumSTAMPAen_US
dc.relation.volume52en_US
dc.relation.issue3en_US
dc.relation.firstpage219en_US
dc.relation.lastpage244en_US
dc.type.refereeREF_1en_US
dc.description.internationalsìen_US
dc.relation.scientificsectorFIS/05 - ASTRONOMIA E ASTROFISICAen_US
dc.relation.journalEXPERIMENTAL ASTRONOMYen_US
dc.type.miur262 Articolo in rivista-
dc.identifier.adsbibcode2021ExA....52..219Ten_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.openairetypeArticle-
item.languageiso639-1en-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.journal.journalissn0922-6435-
crisitem.journal.anceE061604-
crisitem.author.deptIASF Milano-
crisitem.author.deptO.A. Brera-
crisitem.author.deptO.A. Trieste-
crisitem.author.deptO.A. Brera-
crisitem.author.deptOAS Bologna-
crisitem.author.deptO.A. Capodimonte-
crisitem.author.deptIASF Milano-
crisitem.author.orcid0000-0002-9393-8078-
crisitem.author.orcid0000-0001-5876-9259-
crisitem.author.orcid0000-0003-3693-3091-
crisitem.author.orcid0000-0001-6278-1576-
crisitem.author.orcid0000-0001-5355-7388-
crisitem.author.orcid0000-0003-3142-5020-
crisitem.author.orcid0000-0003-3259-7801-
Appears in Collections:1.01 Articoli in rivista
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Tanvir2021_Article_ExplorationOfTheHigh-redshiftU.pdfPdf editoriale1.85 MBAdobe PDFView/Open
2104.09532.pdfpreprint2.16 MBAdobe PDFView/Open
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