Table 1.
Summary of the model parameters we fit to three separate observations of the Crab pulsar by IXPE.
Obs. | α/Δt | β/α | bI/Δt | bQ/Δt | bU/Δt | δI | δP | χ2/d.o.f. (a) |
---|---|---|---|---|---|---|---|---|
[×10−2 cnt/s] | [×10−2 cnt/s] | [×10−2 cnt/s] | [%] | [%] | ||||
1st | 0.930 ± 0.004 | ![]() |
72.00 ± 0.09 | ![]() |
![]() |
![]() |
![]() |
126.46/75 |
2nd | 0.957 ± 0.003 | ![]() |
76.65 ± 0.08 | ![]() |
![]() |
![]() |
![]() |
95.65/75 |
3rd | 0.913 ± 0.007 | ![]() |
76.93 ± 0.13 | ![]() |
![]() |
![]() |
![]() |
100.75/75 |
Model without phase shift | ||||||||
1st | 0.930 ± 0.004 | ![]() |
72.00 ± 0.09 | ![]() |
![]() |
0 | 0 | 132.05/77 |
2nd | 0.957 ± 0.003 | ![]() |
76.65 ± 0.08 | ![]() |
![]() |
0 | 0 | 96.71/77 |
3rd | 0.913 ± 0.007 | ![]() |
76.93 ± 0.13 | ![]() |
![]() |
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 | ![]() |
72.00 ± 0.09 | ![]() |
![]() |
![]() |
![]() |
123.59/75 |
2nd | 0.957 ± 0.003 | ![]() |
76.65 ± 0.08 | ![]() |
![]() |
![]() |
![]() |
84.33/75 |
3rd | 0.913 ± 0.007 | ![]() |
76.93 ± 0.13 | ![]() |
![]() |
![]() |
![]() |
95.96/75 |
Notes.
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).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.