Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24890
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Burlon, D. | en_US |
dc.contributor.author | Murphy, T. | en_US |
dc.contributor.author | GHIRLANDA, Giancarlo | en_US |
dc.contributor.author | Hancock, P. J. | en_US |
dc.contributor.author | Parry, R. | en_US |
dc.contributor.author | SALVATERRA, Ruben | en_US |
dc.date.accessioned | 2020-05-15T15:11:22Z | - |
dc.date.available | 2020-05-15T15:11:22Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24890 | - |
dc.description.abstract | Current models suggest gamma-ray bursts could be used as a way of probing Population-III stars - the first stars in the early Universe. In this paper, we use numerical simulations to demonstrate that late-time radio observations of gamma-ray burst afterglows could provide a means of identifying bursts that originate from Population-III stars, if these were highly massive, independently from their redshift. We then present the results from a pilot study using the Australia Telescope Compact Array at 17 GHz, designed to test the hypothesis that there may be Population-III gamma-ray bursts amongst the current sample of known events. We observed three candidates plus a control gamma-ray burst, and make no detections with upper limits of 20-40 μJy at 500-1300 d post-explosion. | en_US |
dc.language.iso | eng | en_US |
dc.title | Gamma-ray bursts from massive Population-III stars: clues from the radio band | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw905 | en_US |
dc.identifier.scopus | 2-s2.0-84975045817 | en_US |
dc.identifier.isi | 000379840900081 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/459/3/3356/2595257 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 459 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 3356 | en_US |
dc.relation.lastpage | 3362 | en_US |
dc.relation.numberofpages | 8 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 6 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | AUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016MNRAS.459.3356B | 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 | O.A. Brera | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0001-5876-9259 | - |
crisitem.author.orcid | 0000-0002-9393-8078 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
stw905.pdf | PDF editoriale | 1.29 MB | Adobe PDF | View/Open |
1604.03946.pdf | postprint | 2.87 MB | Adobe PDF | View/Open |
Page view(s)
58
checked on Apr 20, 2024
Download(s)
30
checked on Apr 20, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.