Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31858
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Tanvir, N. R. | en_US |
dc.contributor.author | Le Floc'h, E. | en_US |
dc.contributor.author | Christensen, L. | en_US |
dc.contributor.author | Caruana, J. | en_US |
dc.contributor.author | SALVATERRA, Ruben | en_US |
dc.contributor.author | GHIRLANDA, Giancarlo | en_US |
dc.contributor.author | Ciardi, B. | en_US |
dc.contributor.author | Maio, U. | en_US |
dc.contributor.author | D'ODORICO, Valentina | en_US |
dc.contributor.author | Piedipalumbo, E. | en_US |
dc.contributor.author | CAMPANA, Sergio | en_US |
dc.contributor.author | Noterdaeme, P. | en_US |
dc.contributor.author | Graziani, L. | en_US |
dc.contributor.author | AMATI, LORENZO | en_US |
dc.contributor.author | Bagoly, Z. | en_US |
dc.contributor.author | Balázs, L. G. | en_US |
dc.contributor.author | Basa, S. | en_US |
dc.contributor.author | Behar, E. | en_US |
dc.contributor.author | De Cia, A. | en_US |
dc.contributor.author | DELLA VALLE, Massimo | en_US |
dc.contributor.author | De Pasquale, M. | en_US |
dc.contributor.author | Frontera, F. | en_US |
dc.contributor.author | Gomboc, A. | en_US |
dc.contributor.author | Götz, D. | en_US |
dc.contributor.author | Horvath, I. | en_US |
dc.contributor.author | Hudec, R. | en_US |
dc.contributor.author | MEREGHETTI, Sandro | en_US |
dc.contributor.author | O'Brien, P. T. | en_US |
dc.contributor.author | Osborne, J. P. | en_US |
dc.contributor.author | Paltani, S. | en_US |
dc.contributor.author | Rosati, P. | en_US |
dc.contributor.author | Sergijenko, O. | en_US |
dc.contributor.author | Stanway, E. R. | en_US |
dc.contributor.author | Szécsi, D. | en_US |
dc.contributor.author | Toth, L. V. | en_US |
dc.contributor.author | Urata, Y. | en_US |
dc.contributor.author | Vergani, S. | en_US |
dc.contributor.author | Zane, S. | en_US |
dc.date.accessioned | 2022-03-24T11:36:56Z | - |
dc.date.available | 2022-03-24T11:36:56Z | - |
dc.date.issued | 2021 | en_US |
dc.identifier.issn | 0922-6435 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31858 | - |
dc.description.abstract | At 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.iso | eng | en_US |
dc.title | Exploration of the high-redshift universe enabled by THESEUS | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s10686-021-09778-w | en_US |
dc.identifier.scopus | 2-s2.0-85111671470 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007/s10686-021-09778-w | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85111671470 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 52 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 219 | en_US |
dc.relation.lastpage | 244 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | 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....52..219T | 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.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0002-9393-8078 | - |
crisitem.author.orcid | 0000-0001-5876-9259 | - |
crisitem.author.orcid | 0000-0003-3693-3091 | - |
crisitem.author.orcid | 0000-0001-6278-1576 | - |
crisitem.author.orcid | 0000-0001-5355-7388 | - |
crisitem.author.orcid | 0000-0003-3142-5020 | - |
crisitem.author.orcid | 0000-0003-3259-7801 | - |
crisitem.journal.journalissn | 0922-6435 | - |
crisitem.journal.ance | E061604 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
Tanvir2021_Article_ExplorationOfTheHigh-redshiftU.pdf | Pdf editoriale | 1.85 MB | Adobe PDF | Visualizza/apri |
2104.09532.pdf | preprint | 2.16 MB | Adobe PDF | Visualizza/apri |
Page view(s)
56
controllato il 18-apr-2024
Download(s)
31
controllato il 18-apr-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.