|RA:||18h 10m 05.42s||LC breaks:||0|
|Dec:||+58° 09′ 18.9′′||LC type:||No breaks|
This light curve comes from the light curve repository (if you use it, please cite Evans et al [2007, 2009]. Flares, marked by cross-hatched regions, are identified automatically, but may have been manually corrected. These are excluded from the fit. Any power-law breaks added to the fit must be required at the 3-σ level (according to an f-test) to be included in the best-fit. Details of all fits attempted are given below the plot. For more information see the light curve fitting documentation.
|1||5.6||7||Break significance <4-σ |
(43.10 % probability of chance improvement)
|2||3.5||5||Break significance <4-σ |
(38.85 % probability of chance improvement)
There are no flares ignored from this fit.
The best-fitting light curve has 0 breaks.
Click on the number of breaks in the table to the right to change which fit is plotted above and detailed below.
Currently showing the best fit.
|α1||0.99 (+0.37, -0.32)|
|Flux11hr||1.47e-12 erg cm-2 s-1|
Since there are no breaks in the light curve, only the time-averaged spectra are shown below. Times of flaring have not been removed, however this makes little difference to most spectra (see Fig 7/8c of Evans et al. 2009). For more information see the time-resolved spectroscopy documentation.
No spectra are available for this object.