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Table 1.

Summary of the model parameters we fit to three separate observations of the Crab pulsar by IXPE.

Obs. αt β/α bIt bQt bUt δI δP χ2/d.o.f. (a)
[×10−2 cnt/s] [×10−2 cnt/s] [×10−2 cnt/s] [%] [%]
1st 0.930 ± 0.004 0 . 55 0.13 + 0.12 $ 0.55^{+0.12}_{-0.13} $ 72.00 ± 0.09 0 . 62 0.41 + 0.42 $ 0.62^{+0.42}_{-0.41} $ 16 . 54 0.41 + 0.41 $ -16.54^{+0.41}_{-0.41} $ 7 . 42 4.42 + 5.94 $ 7.42^{+5.94}_{-4.42} $ 0 . 67 0.63 + 0.51 $ -0.67^{+0.51}_{-0.63} $ 126.46/75
2nd 0.957 ± 0.003 0 . 53 0.10 + 0.10 $ 0.53^{+0.10}_{-0.10} $ 76.65 ± 0.08 0 . 55 0.32 + 0.32 $ -0.55^{+0.32}_{-0.32} $ 17 . 40 0.34 + 0.34 $ -17.40^{+0.34}_{-0.34} $ 21 . 23 2.74 + 3.52 $ 21.23^{+3.52}_{-2.74} $ 0 . 90 0.70 + 0.57 $ -0.90^{+0.57}_{-0.70} $ 95.65/75
3rd 0.913 ± 0.007 0 . 31 0.21 + 0.19 $ 0.31^{+0.19}_{-0.21} $ 76.93 ± 0.13 0 . 24 0.56 + 0.56 $ 0.24^{+0.56}_{-0.56} $ 16 . 98 0.55 + 0.54 $ -16.98^{+0.54}_{-0.55} $ 2 . 16 13.88 + 9.13 $ -2.16^{+9.13}_{-13.88} $ 1 . 13 2.24 + 1.61 $ -1.13^{+1.61}_{-2.24} $ 100.75/75

Model without phase shift

1st 0.930 ± 0.004 0 . 51 0.12 + 0.12 $ 0.51^{+0.12}_{-0.12} $ 72.00 ± 0.09 0 . 68 0.41 + 0.41 $ 0.68^{+0.41}_{-0.41} $ 16 . 66 0.42 + 0.40 $ -16.66^{+0.40}_{-0.42} $ 0 0 132.05/77
2nd 0.957 ± 0.003 0 . 42 0.10 + 0.10 $ 0.42^{+0.10}_{-0.10} $ 76.65 ± 0.08 0 . 48 0.34 + 0.33 $ -0.48^{+0.33}_{-0.34} $ 17 . 70 0.33 + 0.35 $ -17.70^{+0.35}_{-0.33} $ 0 0 96.71/77
3rd 0.913 ± 0.007 0 . 44 0.16 + 0.16 $ 0.44^{+0.16}_{-0.16} $ 76.93 ± 0.13 0 . 49 0.52 + 0.55 $ 0.49^{+0.55}_{-0.52} $ 16 . 82 0.52 + 0.52 $ -16.82^{+0.52}_{-0.52} $ 0 0 101.07/77

Model including 90% subtraction of DC component from the Stokes parameters in the optical band

1st 0.930 ± 0.004 0 . 61 0.14 + 0.14 $ 0.61^{+0.14}_{-0.14} $ 72.00 ± 0.09 0 . 47 0.41 + 0.40 $ 0.47^{+0.40}_{-0.41} $ 17 . 11 0.37 + 0.37 $ -17.11^{+0.37}_{-0.37} $ 2 . 91 2.22 + 1.36 $ 2.91^{+1.36}_{-2.22} $ 0 . 54 0.56 + 0.45 $ -0.54^{+0.45}_{-0.56} $ 123.59/75
2nd 0.957 ± 0.003 0 . 53 0.10 + 0.10 $ 0.53^{+0.10}_{-0.10} $ 76.65 ± 0.08 0 . 98 0.31 + 0.29 $ -0.98^{+0.29}_{-0.31} $ 17 . 93 0.31 + 0.30 $ -17.93^{+0.30}_{-0.31} $ 32 . 91 1.51 + 1.23 $ 32.91^{+1.23}_{-1.51} $ 0 . 99 0.65 + 0.57 $ -0.99^{+0.57}_{-0.65} $ 84.33/75
3rd 0.913 ± 0.007 0 . 54 0.20 + 0.18 $ 0.54^{+0.18}_{-0.20} $ 76.93 ± 0.13 0 . 42 0.54 + 0.53 $ 0.42^{+0.53}_{-0.54} $ 17 . 23 0.48 + 0.47 $ -17.23^{+0.47}_{-0.48} $ 4 . 51 7.17 + 4.41 $ -4.51^{+4.41}_{-7.17} $ 0 . 78 1.09 + 0.85 $ -0.78^{+0.85}_{-1.09} $ 95.96/75

Notes.

(a)

χ2 statistic reported for the set of parameters {β, bQ, bU, δI, δP}. The parameters {α, bI} are fitted separately to the IXPE Stokes I; they do not depend on the treatment of the polarized components of the Stokes vector. The quantity Δt is the exposure time divided by the number of phase bins (40).

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