Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26792
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Dereli, H. | en_US |
dc.contributor.author | Boër, M. | en_US |
dc.contributor.author | Gendre, B. | en_US |
dc.contributor.author | AMATI, LORENZO | en_US |
dc.contributor.author | Dichiara, S. | en_US |
dc.contributor.author | Orange, N. B. | en_US |
dc.date.accessioned | 2020-08-25T11:10:15Z | - |
dc.date.available | 2020-08-25T11:10:15Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26792 | - |
dc.description.abstract | We present a sample composed of the 41 faintest X-ray afterglows of the population of long gamma-ray bursts (lGRBs) with known redshift. We study their intrinsic properties (spectral index, decay index, distance, luminosity, isotropic radiated energy, and peak energy) and their luminosity distribution functions to assess whether they belong to the same population as the brighter afterglow events. We find that these events belong to a population of nearby ones, different from the general population of lGRBs. In addition, these events are faint during their prompt phase, and include the few possible outliers of the Amati relation. | en_US |
dc.language.iso | eng | en_US |
dc.title | A Study of GRBs with Low-luminosity Afterglows | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/aa947d | en_US |
dc.identifier.scopus | 2-s2.0-85037706168 | en_US |
dc.identifier.isi | 000416005400007 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/aa947d | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 850 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 117 | 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 | FRA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017ApJ...850..117D | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | en_US |
dc.description.apc | sì | 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 | OAS Bologna | - |
crisitem.author.orcid | 0000-0001-5355-7388 | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Dereli_2017_ApJ_850_117.pdf | 1.27 MB | Adobe PDF | View/Open |
Page view(s)
36
checked on Apr 17, 2024
Download(s)
13
checked on Apr 17, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.