dc.contributor.author | Mignani, R. P. | |
dc.contributor.author | Rea, N. | |
dc.contributor.author | Testa, V. | |
dc.contributor.author | Marelli, M. | |
dc.contributor.author | De Luca, A. | |
dc.contributor.author | Pierbattista, M. | |
dc.contributor.author | Shearer, A. | |
dc.contributor.author | Torres, D. F. | |
dc.contributor.author | De Oña Wilhelmi, E. | |
dc.date.accessioned | 2018-09-20T16:17:47Z | |
dc.date.available | 2018-09-20T16:17:47Z | |
dc.date.issued | 2016-07-07 | |
dc.identifier.citation | Mignani, R. P. Rea, N.; Testa, V.; Marelli, M.; De Luca, A.; Pierbattista, M.; Shearer, A.; Torres, D. F.; De Oña Wilhelmi, E. (2016). Observations of three young γ-ray pulsars with the gran telescopio canarias. Monthly Notices of the Royal Astronomical Society 461 (4), 4317-4328 | |
dc.identifier.issn | 0035-8711,1365-2966 | |
dc.identifier.uri | http://hdl.handle.net/10379/12891 | |
dc.description.abstract | We report the analysis of the first deep optical observations of three isolated gamma-ray pulsars detected by the Fermi Gamma-ray Space Telescope: the radio-loud PSR J0248+6021 and PSR J0631+1036, and the radio-quiet PSR J0633+0632. The latter has also been detected in the X-rays. The pulsars are very similar in their spin-down age (tau similar to 40-60 kyr), spin-down energy (E similar to 10(35) erg s(-1)), and dipolar surface magnetic field (B similar to 3-5 x 10(12) G). These pulsars are promising targets for multiwavelength observations, since they have been already detected in gamma-rays and in radio or X-rays. None of them has been detected yet in the optical band. We observed the three pulsar fields in 2014 with the Spanish 10.4 m Gran Telescopio Canarias (GTC). We could not find any candidate optical counterpart to the three pulsars close to their most recent radio or Chandra positions down to 3 sigma limits of g' similar to 27.3, g' similar to 27, g' similar to 27.3 for PSR J0248+6021, J0631+1036, and J0633+0632, respectively. From the inferred optical upper limits and estimated distance and interstellar extinction, we derived limits on the pulsar optical luminosity. We also searched for the X-ray counterpart to PSR J0248+6021 with Chandra but we did not detect the pulsar down to a 3s flux limit of 5 x 10(-14) erg cm(-2) s(-1) (0.3-10 keV). For all these pulsars, we compared the optical flux upper limits with the extrapolations in the optical domain of the gamma-ray spectra and compared their multiwavelength properties with those of other gamma-ray pulsars of comparable age. | |
dc.publisher | Oxford University Press (OUP) | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Ireland | |
dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/3.0/ie/ | |
dc.subject | stars: neutron | |
dc.subject | large-area telescope | |
dc.subject | large-magellanic-cloud | |
dc.subject | wind nebula | |
dc.subject | optical observations | |
dc.subject | radio-quiet | |
dc.subject | supernova remnant | |
dc.subject | psr j2021+3651 | |
dc.subject | cta 1 | |
dc.subject | discovery | |
dc.subject | emission | |
dc.title | Observations of three young γ-ray pulsars with the gran telescopio canarias | |
dc.type | Article | |
dc.identifier.doi | 10.1093/mnras/stw1629 | |
dc.local.publishedsource | http://arxiv.org/pdf/1606.04711 | |
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