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We have copious photometry data! Let's make a figure with these elements:
K2 data from 3 campaigns, vertically registered to K2 zero-points.
ASASSN data
Vertical bar of IGRINS epoch
Celerite model fit threading through both the K2 and ASASSN data.
We've already done this for posters, so we should translate that work into a paper-sized version. We also need to describe in the text what we have done to create this figure and what we learn from it. In particular:
Can we assign the starspot coverage fraction at the global peak-and-valley?
The text was updated successfully, but these errors were encountered:
We have copious photometry data! Let's make a figure with these elements:
We've already done this for posters, so we should translate that work into a paper-sized version. We also need to describe in the text what we have done to create this figure and what we learn from it. In particular:
Can we assign the starspot coverage fraction at the global peak-and-valley?
The text was updated successfully, but these errors were encountered: