
2018 data update (36/n)
[Orig: September 19, 2018] Hello everyone, Data taken over the past week show a bit of increased scatter, perhaps caused by variability at smaller levels that our measurements can detect, but overall there is not much change to report. More later, ~Tabby and team Note from previous post that still applies: The gray vertical line indicates the time of the change in configuration. There are still some remaining issues that we need to address for data taken primarily during the

2018 data update (35/n)
[Orig: September 12, 2018] Hello all! Just wanted to share an update on how observations are going. The star has been a bit quite since March of this year, when we saw the two deepest dips since the Kepler mission (Caral-Supe and Evangeline). After March, the brightness has hovered slightly above normal (I define "normal" brightness as the brightness level just before Elsie in 2017 May. This is equal to unity on the graphs, and can be traced with the horizontal dotted line).