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Figure 1:
The effect of anisotropic errors on the best fit parameters of the fundamental plane (Eq. (1)). The horizontal axis gives the anisotropy parameter ![]() ![]() ![]() ![]() ![]() |
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Figure 2: Sketch of the SED of a relativistic jet as for example observed in BL Lac objects. At lower photon energies synchrotron emission is dominant while the high energy spectrum is usually explained by inverse Compton processes. See text for details. |
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Figure 3:
Histogram of the scatter in the full KFC sample. The scatter can be well approximated by a Gaussian with the standard-deviation
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Figure 4:
On the left side we show the ![]() |
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Figure 5:
Best fit for the full KFC sample if one fixes
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