We now have custom cloudy models working in our interactive spectral analysis dashboard. Overall the fits look really good and the intrinsic and extrinsic physical properties(Teff, logg, fsed, vsini, RV) are mostly consistent from spectral-order-to-spectral-order. Caroline and I examined the fits--- it's tricky to see the visit-to-visit variation by eye, but we flagged some locations that may be more variable than others. The next step is to quantify these changes and and quantify the degree to which spurious artifacts could mimic them. Below we list the specific takeaways from the meeting.
Tasks for the next week:
[x] 1. Label conspicuous spectral features
[x] 2. Overlay low-res spectrum with high-res cutouts
[x] 3. Label brightness temperature per echelle order (you can coarsely compute it with a scaling relation)
[x] 4. Refine the telluric correction (the default plp one leaves broad residuals)
We now have custom cloudy models working in our interactive spectral analysis dashboard. Overall the fits look really good and the intrinsic and extrinsic physical properties(Teff, logg, fsed, vsini, RV) are mostly consistent from spectral-order-to-spectral-order. Caroline and I examined the fits--- it's tricky to see the visit-to-visit variation by eye, but we flagged some locations that may be more variable than others. The next step is to quantify these changes and and quantify the degree to which spurious artifacts could mimic them. Below we list the specific takeaways from the meeting.
Tasks for the next week:
plpone leaves broad residuals)