Extending analysis from MacLeod+2010, MacLeod+2011, and MacLeod+2012, by extending S82 light curves to larger baselines with PS1, CRTS and PTF data. This is based on the findings of Kozlowski+2017 that we confirmed, namely that a longer baseline significantly reduces the bias in retrieval of quasar characteristic timescale and variability amplitude.
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suberlak/PS1_SDSS_CRTS
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Extending analysis from MacLeod+2011 to larger baselines with PS1 and CRTS data
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