First VLTI-GRAVITY near-infrared observations of blazars indicate possible detection of unresolved or partially resolved jet emission in Ton 599, though data cannot distinguish extended structure from instrumental coherence loss.
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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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VLTI-GRAVITY observations of blazars
First VLTI-GRAVITY near-infrared observations of blazars indicate possible detection of unresolved or partially resolved jet emission in Ton 599, though data cannot distinguish extended structure from instrumental coherence loss.
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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.