Jets from accreting black holes appear remarkably similar over eight
orders of magnitude in black hole mass, with more massive black holes
generally launching more powerful jets. For example, there is an
observed correlation, termed the fundamental plane of black hole
accretion, between black hole mass, radio luminosity, and X-ray
luminosity. Here, we probe the high-mass tail
(108-109 Msolar) of
... [Show full abstract] the accreting black
hole distribution with BL Lac objects. We build SEDs for hundreds of
SDSS BL Lacs, and we use these SEDs to test the blazar sequence, a
proposed anti-correlation between jet power and peak frequency. We then
show our BL Lacs fit on the fundamental plane, supporting the non-linear
scaling of jet radiation with black hole mass. The subset of BL Lacs
considered here compose the largest sample yet used in the above types
of studies, reducing potential selection effects and biases.