All Tables

Table 1: Formal function decribing the pulse period during the outburst. The reference for the third order polinomial fit is MJD 53 618. From MJD 53 629 the period is essentially constant.
Table 2: Best-fit values for the available observations during the pre-outburst flare, where the CRSF energy is measured at a higher position, for the sum of the observations during the flare, and for one observation close to the maximum of the main outburst. L is the luminosity in units of $10^{37}~{\rm erg~s^{-1}}\xspace$ in the $5{-}50~{\rm keV}\xspace$ range. Errors are $90\%$ confidence for one parameter of interest ( $\chi^{2}_{\min}+2.7$ ).