Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/32868
DC Field | Value | Language |
---|---|---|
dc.contributor.author | GRUPPIONI, Carlotta | en_US |
dc.contributor.author | Ciesla, L. | en_US |
dc.contributor.author | Hatziminaoglou, E. | en_US |
dc.contributor.author | Pozzi, F. | en_US |
dc.contributor.author | Rodighiero, G. | en_US |
dc.contributor.author | SANTINI, Paola | en_US |
dc.contributor.author | Armus, L. | en_US |
dc.contributor.author | Baes, M. | en_US |
dc.contributor.author | Braine, J. | en_US |
dc.contributor.author | Charmandaris, V. | en_US |
dc.contributor.author | Clements, D. L. | en_US |
dc.contributor.author | Christopher, N. | en_US |
dc.contributor.author | Dannerbauer, H. | en_US |
dc.contributor.author | Efstathiou, A. | en_US |
dc.contributor.author | Egami, E. | en_US |
dc.contributor.author | FERNANDEZ ONTIVEROS, Juan Antonio | en_US |
dc.contributor.author | FONTANOT, Fabio | en_US |
dc.contributor.author | Franceschini, A. | en_US |
dc.contributor.author | González-Alfonso, E. | en_US |
dc.contributor.author | Griffin, M. | en_US |
dc.contributor.author | Kaneda, H. | en_US |
dc.contributor.author | Marchetti, L. | en_US |
dc.contributor.author | Monaco, P. | en_US |
dc.contributor.author | Nakagawa, T. | en_US |
dc.contributor.author | Onaka, T. | en_US |
dc.contributor.author | Papadopoulos, A. | en_US |
dc.contributor.author | Pearson, C. | en_US |
dc.contributor.author | Pérez-Fournon, I. | en_US |
dc.contributor.author | Peréz-González, P. | en_US |
dc.contributor.author | Roelfsema, P. | en_US |
dc.contributor.author | Scott, D. | en_US |
dc.contributor.author | Serjeant, S. | en_US |
dc.contributor.author | SPINOGLIO, Luigi Giuseppe Maria | en_US |
dc.contributor.author | Vaccari, M. | en_US |
dc.contributor.author | van der Tak, F. | en_US |
dc.contributor.author | Vignali, C. | en_US |
dc.contributor.author | Wang, L. | en_US |
dc.contributor.author | Wada, T. | en_US |
dc.date.accessioned | 2023-01-16T14:25:41Z | - |
dc.date.available | 2023-01-16T14:25:41Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 1448-6083 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32868 | - |
dc.description.abstract | Our current knowledge of star formation and accretion luminosity at high redshift (z > 3-4), as well as the possible connections between them, relies mostly on observations in the rest-frame ultraviolet, which are strongly affected by dust obscuration. Due to the lack of sensitivity of past and current infrared instrumentation, so far it has not been possible to get a glimpse into the early phases of the dust-obscured Universe. Among the next generation of infrared observatories, SPICA, observing in the 12-350 µm range, will be the only facility that can enable us to trace the evolution of the obscured star-formation rate and black-hole accretion rate densities over cosmic time, from the peak of their activity back to the reionisation epoch (i.e., 3 < z ≲ 6-7), where its predecessors had severe limitations. Here, we discuss the potential of photometric surveys performed with the SPICA mid-infrared instrument, enabled by the very low level of impact of dust obscuration in a band centred at 34 µm. These unique unbiased photometric surveys that SPICA will perform will fully characterise the evolution of AGNs and star-forming galaxies after reionisation. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1017/pasa.2017.49 | en_US |
dc.identifier.isi | 000415377400001 | en_US |
dc.identifier.url | https://www.cambridge.org/core/journals/publications-of-the-astronomical-society-of-australia/article/tracing-the-evolution-of-dust-obscured-star-formation-and-accretion-back-to-the-reionisation-epoch-with-spica/961676281960A7B0604B5F95D2916FBA | en_US |
dc.identifier.url | https://arxiv.org/pdf/1710.02353.pdf | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 34 | en_US |
dc.relation.firstpage | e055 | 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.contributor.country | ESP | en_US |
dc.contributor.country | CAN | en_US |
dc.contributor.country | DNK | en_US |
dc.contributor.country | JPN | en_US |
dc.contributor.country | GRC | en_US |
dc.contributor.country | ZAF | en_US |
dc.contributor.country | CHE | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017PASA...34...55G | 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.grantfulltext | open | - |
item.cerifentitytype | Publications | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.journal.journalissn | 1448-6083 | - |
crisitem.journal.ance | E211088 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Trieste | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0002-5836-4056 | - |
crisitem.author.orcid | 0000-0002-9334-8705 | - |
crisitem.author.orcid | 0000-0001-9490-899X | - |
crisitem.author.orcid | 0000-0003-4744-0188 | - |
crisitem.author.orcid | 0000-0001-8840-1551 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Gruppioni2017_1710.02353.pdf | Pdf editoriale | 9.03 MB | Adobe PDF | View/Open |
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