Jet power estimates for FSRQs PKS 1441+25 and Ton 599 are insensitive to the choice of electron energy distribution model because of lower break energies and external Compton dominance.
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New multi-band optical monitoring of quasar 4C 29.45 finds variability amplitudes of 220%, 208%, and 209% in V, R, I; spectral indices 1.032-1.573; achromatic trends; and no short-term periodicity.
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Jet Power Estimates of FSRQs PKS 1441+25 and Ton 599 from Broadband SED Modeling
Jet power estimates for FSRQs PKS 1441+25 and Ton 599 are insensitive to the choice of electron energy distribution model because of lower break energies and external Compton dominance.
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Shortterm optical variability of 4C 29.45
New multi-band optical monitoring of quasar 4C 29.45 finds variability amplitudes of 220%, 208%, and 209% in V, R, I; spectral indices 1.032-1.573; achromatic trends; and no short-term periodicity.