The 26.3-hr orbit and multi-wavelength properties of the "redback" millisecond pulsar PSR J1306-40

We present the discovery of the variable optical and X-ray counterparts to the radio millisecond pulsar (MSP) PSR J1306-40, recently discovered by Keane et al. We find that both the optical and X-ray fluxes are modulated with the same period, which allows us to measure for the first time the orbital period P${}_{\mathrm{o}\mathrm{r}\mathrm{b}}$=1.09716[6] d. The optical properties are consistent with a main sequence companion with spectral type G to mid K and, together with the X-ray luminosity (8.8$\times$10${}^{31}$ erg s${}^{-1}$ in the 0.5-10 keV band, for a distance of 1.2 kpc), confirm the redback classification of this pulsar. Our results establish the binary nature of PSR J1306-40, which has the longest P${}_{\mathrm{o}\mathrm{r}\mathrm{b}}$ among all known compact binary MSPs in the Galactic disk. We briefly discuss these findings in the context of irradiation and intrabinary shock emission in compact binary MSPs.