Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26590
DC Field | Value | Language |
---|---|---|
dc.contributor.author | RAMPAZZO, Roberto | en_US |
dc.contributor.author | D'ONOFRIO, MAURO | en_US |
dc.contributor.author | ZAGGIA, Simone | en_US |
dc.contributor.author | Djorgovski, Stanislav George | en_US |
dc.contributor.author | Elmegreen, Debra M. | en_US |
dc.contributor.author | POGGIANTI, Bianca Maria | en_US |
dc.contributor.author | Calzetti, Daniela | en_US |
dc.contributor.author | Combes, Françoise | en_US |
dc.contributor.author | Longair, Malcolm S. | en_US |
dc.contributor.author | Bromm, Volker | en_US |
dc.date.accessioned | 2020-07-23T13:22:19Z | - |
dc.date.available | 2020-07-23T13:22:19Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.isbn | 978-3-319-31004-6 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26590 | - |
dc.description.abstract | Some contributions in Chap. 1 have highlighted the impact of the discovery in the 1960s of a handful of radio galaxies and Quasars in the redshift range z ∼ 0.2-0.4. About 40 years later, at the end of the twentieth Century, the systematic exploration of galaxies reached z ∼ 1-3. The combination of HST deep imaging and the coming into operation of the 8-10 m class telescopes with their spectroscopic capabilities, move ahead the limits. At the same time, astronomers greatly improved their strategies to hunt high-redshift galaxies. Today, it is not infrequent the spectroscopic confirmation of galaxies at z ∼ 7-8, pushing the detection limits more or less to the end of the re-ionization era. The gauntlet to observe the so called "first galaxies", i.e. those assembling during the first billion years of the cosmic time, is throw down. | en_US |
dc.language.iso | eng | en_US |
dc.title | In Pursuit of High Redshift Galaxies | en_US |
dc.type | Book part | - |
dc.identifier.doi | 10.1007/978-3-319-31006-0_6 | en_US |
dc.identifier.isi | 000389190800008 | en_US |
dc.identifier.url | https://link.springer.com/chapter/10.1007%2F978-3-319-31006-0_6 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 435 | en_US |
dc.relation.firstpage | 479 | en_US |
dc.relation.lastpage | 508 | en_US |
dc.type.referee | REF_4 | en_US |
dc.description.international | sì | en_US |
dc.relation.allauthors | D'Onofrio, M.; Rampazzo, R.: Zaggia, S. | en_US |
dc.relation.ispartofbook | From the Realm of the Nebulae to Populations of Galaxies | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 268 Contributo in volume (Capitolo o Saggio) | - |
dc.relation.series | ASTROPHYSICS AND SPACE SCIENCE LIBRARY | en_US |
dc.identifier.adsbibcode | 2016ASSL..435..479R | 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 | Book part | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | reserved | - |
crisitem.journal.journalissn | 0067-0057 | - |
crisitem.journal.ance | E016260 | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0001-5318-9183 | - |
crisitem.author.orcid | 0000-0001-6081-379X | - |
crisitem.author.orcid | 0000-0001-8751-8360 | - |
Appears in Collections: | 2.01 Capitoli o saggi in libro |
Files in This Item:
File | Description | Size | Format | Existing users please |
---|---|---|---|---|
FromTheRealmOfThe Nebuale-2016_Chapter6.pdf | [Administrators only] | 491.27 kB | Adobe PDF |
Page view(s)
105
checked on Aug 5, 2024
Download(s)
3
checked on Aug 5, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.