gherczeg
commented
8 years ago Figure 9 caption: The observed optical colors of LkCa 4 from Grankin et al. [32], compared with predictions from converting V -band brightness to a cool spot filling factor and subsequently calculating colors from main sequence colors and bolometric corrections of Kenyon & Hartmann [50](purple lines).
change KH95 to \citet{Pecaut13}.
Section 4.2, para 1, immediately following "pre-main sequence colors": The photometry is obtained from the colors of 4100 K and 2750 K photospheres, as obtained from main-sequence colors listed in \citet{Pecaut13}. The time-dependent color is then calculated by combining these two components based on their visible areas, as inferred from the $V$-band brightness.
On Fri, Sep 16, 2016 at 3:53 PM, gully notifications@github.com wrote:
From I. Czekala:
- Fig 10: What is the difference between red and blue spectra? If this information isn't obvious, it would be nice to have in the caption or as a legend on the plot.
From G. Somers:
- Fig 10: consider error bars on the TiO indices
- Fig 11: Plot legend for the various datapoints and lines?
- Put an unique entries for L in the "historical" table for our two different estimates for the cool component.
- Re: Fig. 9: How exactly did you construct the models you are comparing them to? ... Issues w/ PMS bolometric corrections might also come into play. ... contribution of plages/faculae (hot spots). Perhaps these are messing up your derived T's in a 2 zone model, and thus your prediction for what the cooler spots should look like is off.
- Explain why luminosity stays about the same in HR diagram
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gully
From I. Czekala:
From G. Somers: