Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/23396
DC Field | Value | Language |
---|---|---|
dc.contributor.author | SALVATERRA, Ruben | en_US |
dc.date.accessioned | 2020-03-19T15:10:09Z | - |
dc.date.available | 2020-03-19T15:10:09Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 2214-4048 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/23396 | - |
dc.description | Acknowledgements This research was supported by the ASI-INAF contract ( 1/005/11/1 ). The author would like to thank A. Melandri for providing the X-ray light curve for the z > 6 sample, S. Campana for providing the measure of the N H , X for some of the high- z bursts, G. Ghirlanda for providing the E iso values and the expected rate of GRBs at z > 8 . | en |
dc.description.abstract | Ten years of operations of the Swift satellite have allowed us to collect a small sample of long Gamma-Ray Bursts (GRBs) at redshift larger than 6. I will review here the present status of this research field and discuss the possible use of GRBs as a fundamental new tool to explore the early Universe, complementary to quasar and galaxy surveys. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | High redshift Gamma-Ray Bursts | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.jheap.2015.03.001 | en_US |
dc.identifier.scopus | 2-s2.0-84941937751 | en_US |
dc.identifier.isi | 000213811200006 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/pii/S2214404815000051?via%3Dihub | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 7 | en_US |
dc.relation.firstpage | 35 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | no | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF HIGH ENERGY ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2015JHEAp...7...35S | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò 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.orcid | 0000-0002-9393-8078 | - |
crisitem.journal.journalissn | 2214-4048 | - |
crisitem.journal.ance | E227120 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
JHEA 2015 Salvaterra.pdf | 468.03 kB | Adobe PDF | View/Open | |
1-s2.0-S2214404815000051-main.pdf | [Administrators only] | 655.35 kB | Adobe PDF |
Page view(s)
63
checked on Apr 17, 2024
Download(s)
18
checked on Apr 17, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.