Observations of three young gamma-ray pulsars with the Gran Telescopio Canarias

Abstract

We report the analysis of the first deep optical observations of three isolated $\gamma$-ray pulsars detected by the {\em 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 \sim$40--60 kyrs), spin-down energy ($\dot{E}\sim 10^{35}$ erg s${}^{-1}$), and dipolar surface magnetic field ($B\sim 3$--$5\times 10^{12}$ G). These pulsars are promising targets for multi-wavelength 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 10.4m Gran Telescopio Canarias (GTC). We could not find any candidate optical counterpart to the three pulsars close to their most recent radio or {\em Chandra} positions down to $3\sigma$ limits of $g^{\prime }\sim 27.3$, $g^{\prime }\sim 27$, $g^{\prime }\sim 27.3$ 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 \chan\ but we did not detect the pulsar down to a 3$\sigma$ flux limit of $5\times 10^{-14}$ 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 multi-wavelength properties with those of other $\gamma$-ray pulsars of comparable age.

arXiv comment12 pages, 5 figures, accepted for publication in MNRAS

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• The first ultraviolet detection of the Large Magellanic Cloud pulsar PSR B0540-69 and its multi-wavelength properties
• XMM-Newton observations of a gamma-ray pulsar J0633+0632: pulsations, cooling and large-scale emission
• Efficiency of Synchrotron Radiation from Rotation-Powered Pulsars
• Multiwavelength observations of PSR J2021+4026 across a mode change reveal a phase shift in its X-ray emission
• Observations of one young and three middle-aged $\gamma$-ray pulsars with the Gran Telescopio Canarias
• Searching for the optical counterparts of two young gamma-ray pulsars
• Large Binocular Telescope observations of PSR J2043+2740
• Identification of radio and gamma-ray pulsars in X-rays using data from the SRG/eROSITA all-sky survey