Six years of optical photometry of the blazar OT 355 show intra-night and long-term variability, and a simple Doppler-geometry derivation argues that additive models predict a negative rms-flux relation, which is not observed.
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Optical Photometric Monitoring of the Blazar OT 355 and Local Standard Stars' Calibration
Six years of optical photometry of the blazar OT 355 show intra-night and long-term variability, and a simple Doppler-geometry derivation argues that additive models predict a negative rms-flux relation, which is not observed.