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Table 1

Fitting results of Swift/XRT observations of PKS 1424418.

Time Time Net Exp. Time Photon Index Fluxa 0.310.0 keV (d.o.f.)/Cash
(UT) (MJD) (sec) (10-12 erg cm-2 s-1)

2005-Apr.-19 53 479 2249 1.35 ± 0.22 3.34 ± 0.62 Cash
2005-Apr.-23 53 483 1543 1.54 ± 0.41 1.73 ± 0.47 Cash
2006-Jun.-18 53 904 3784 1.37 ± 0.17 4.28 ± 0.49 0.727 (11)
2010-Feb.-11 55 238 3646 1.49 ± 0.24 3.77 ± 0.75 0.762(9)
2010-May-12 55 328 1958 1.70 ± 0.21 5.80 ± 0.90 0.796 (9)
2010-May-13 55 329 1279 1.75 ± 0.24 4.25 ± 0.84 Cash
2010-May-14 55 330.5 1963 1.99 ± 0.20 5.25 ± 0.63 0.803 (10)
2010-May-14 55 330.6 951 1.78 ± 0.20 7.89 ± 0.72 Cash
2010-May-15 55 331 1938 1.68 ± 0.21 4.45 ± 0.71 Cash
2010-May-16 55 332 3833 1.82 ± 0.18 4.29 ± 0.54 0.868 (13)
2010-Sep.-30 55 469 5152 1.47 ± 0.15 3.80 ± 0.41 1.008 (15)
2011-May-07 55 688 3913 1.80 ± 0.24 3.41 ± 0.55 0.920 (10)
2011-May-10 55 691 3932 1.61 ± 0.23 3.93 ± 0.46 1.080 (9)

Notes. Columns report, from left to right: observation time, net exposure time, observed photon index and flux. The last column indicates the method used to perform the spectral analysis: reduced χ2 and, in parentheses, the degrees of freedom, or the Cash method when the statistics were low. Results were obtained considering an absorbed power-law model with NH fixed to Galactic absorption in the direction of the source.

(a)

Observed flux.

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