Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24673
DC Field | Value | Language |
---|---|---|
dc.contributor.author | MIGNANI, Roberto | en_US |
dc.contributor.author | TESTA, Vincenzo | en_US |
dc.contributor.author | Marelli, M. | en_US |
dc.contributor.author | DE LUCA, Andrea | en_US |
dc.contributor.author | Pierbattista, M. | en_US |
dc.contributor.author | Razzano, M. | en_US |
dc.contributor.author | Salvetti, D. | en_US |
dc.contributor.author | Belfiore, A. | en_US |
dc.contributor.author | Shearer, A. | en_US |
dc.contributor.author | Moran, P. | en_US |
dc.date.accessioned | 2020-05-11T08:03:28Z | - |
dc.date.available | 2020-05-11T08:03:28Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24673 | - |
dc.description.abstract | We report on the first deep optical observations of two γ-ray pulsars, both among the very first discovered by the Fermi Gamma-ray Space Telescope. The two pulsars are the radio-loud PSR J1907+0602 in the TeV pulsar wind nebula (PWN) MGRO J1908+06 and the radio-quiet PSR J1809-2332 in the `Taz' radio/X-ray PWN. These pulsars are relatively young and energetic and have been both detected in the X-rays by XMM-Newton, which makes them viable targets for optical observations. We observed the pulsar fields in the B and V bands with the Very Large Telescope (VLT) in 2015 June/July to search for their optical counterparts. Neither of the two pulsars has been detected down to 3σ limiting magnitudes of m<SUB>v</SUB> ∼ 26.9 and ∼27.6 for PSR J1907+0602 and PSR J1809-2332, respectively. We discuss these results in the framework of the multiwavelength emission properties of pulsars. | en_US |
dc.language.iso | eng | en_US |
dc.title | Searching for the optical counterparts of two young γ-ray pulsars | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw2226 | en_US |
dc.identifier.scopus | 2-s2.0-85015083074 | en_US |
dc.identifier.isi | 000393566000051 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/463/3/2932/2646629 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 463 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 2932 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | 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.463.2932M | 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.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0002-8685-583x | - |
crisitem.author.orcid | 0000-0003-1033-1340 | - |
crisitem.author.orcid | 0000-0001-6739-687X | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
stw2226.pdf | PDF editoriale | 2.85 MB | Adobe PDF | View/Open |
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