A decade of optical monitoring of blazar OJ 287 reveals persistent bluer-when-brighter behavior, co-spatial BVRI emission, and a central black hole mass of at least 3.89 billion suns.
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Multi-band optical photometric variability of the blazar OJ 287 from 2015 to 2025
A decade of optical monitoring of blazar OJ 287 reveals persistent bluer-when-brighter behavior, co-spatial BVRI emission, and a central black hole mass of at least 3.89 billion suns.