BrownDwarf welter issues

BrownDwarf / welter

Inferring starspot properties in the IGRINS spectrum of LkCa 4

MIT License

5 stars 0 forks source link

issues

Newest

Newest Most commented Recently updated Oldest Least commented Least recently updated

Post processing on the proofs

#56 gully opened 7 years ago
0
Comments from Covey re-read

#55 gully closed 7 years ago
1
Chat with GJH on my last day in Beijing

#54 gully closed 7 years ago
1
Referee report

#53 gully closed 7 years ago
9
Comments from collaborators to be addressed along with referee comments

#52 gully closed 7 years ago
4
Idea for new section: "Minimum possible starspot coverage assuming absolute zero Tspot"

#51 gully closed 7 years ago
4
Feedback from Gaitee on v0.6 paper draft

#50 gully opened 8 years ago
0
Tasks for Garrett when he is in Beijing

#49 gully opened 8 years ago
1
Tasks for GJH

#48 gully opened 8 years ago
3
Feedback from GJH on v0.6 paper draft

#47 gully closed 7 years ago
3
Feedback from Covey on v0.6+ paper draft

#46 gully opened 8 years ago
3
Feedback from MATYESSE team members on v0.6 paper draft

#45 gully closed 8 years ago
1
Feedback from ASAS-SN team members on v0.6+ paper draft

#44 gully closed 8 years ago
0
Feedback from IGRINS internal referee process on v0.6 paper draft

#43 gully closed 8 years ago
1
Feedback from Mace on v0.6 paper draft

#42 gully closed 8 years ago
1
Feedback from Konstantin on v0.6 paper draft

#41 gully closed 8 years ago
3
Feedback from Garrett on v0.6 paper draft

#40 gully closed 8 years ago
1
Feedback from Ian on v0.6 paper draft

#39 gully closed 8 years ago
0
Make pre-main sequence HR diagram animation

#38 gully closed 8 years ago
1
Version 0.7 roadmap: feedback from coauthors

#37 gully closed 7 years ago
1
Brainstorming ideas for discussion topics

#36 gully closed 8 years ago
0
Figure of postage stamps of spectral features

#35 gully closed 8 years ago
1
Version 0.6 roadmap: Fill in the missing content

#34 gully closed 8 years ago
0
Version 0.5 roadmap: version to send to collaborators

#33 gully closed 8 years ago
0
Shorten Section 3.2

#32 gully closed 8 years ago
0
Writing: rewrite tense and active voice

#31 gully closed 7 years ago
2
What symbol to use for fill factor?

#30 gully closed 8 years ago
1
Write up the Discussion section.

#29 gully closed 8 years ago
0
Modify star_mix.py to include priors on [Fe/H] and log g

#28 gully closed 8 years ago
1
Re-run all the H-band spectra with expanded Teff range.

#27 gully closed 8 years ago
4
Text and analysis for the results section

#26 gully closed 8 years ago
1
Determine best fit logOmega1 and logOmega2, forcing all other stellar parameters to some values

#25 gully closed 7 years ago
1
A plot of all the spectra arrayed into a single figure?

#24 gully closed 8 years ago
1
We need a line list to label spectral lines and reference them in text.

#23 gully closed 8 years ago
1
I used an ESPaDoNs spectrum to make the Teff vs wavelength plot. Which epoch was it taken at?

#22 gully closed 8 years ago
1
Improvements to the introduction- fact checking, references, develop lines of thought.

#21 gully closed 8 years ago
1
Make figures for Cool Stars 19 poster

#20 gully closed 8 years ago
1
Figure for paper: Trade-off matrix for various approaches

#19 gully closed 8 years ago
1
At what phase of variability were the spectra acquired?

#18 gully closed 8 years ago
2
Make LaTeX tables for stellar properties as a function of order

#17 gully closed 8 years ago
0
The "Evan Kirby experiment"-- coadd the data lines to show signal strength

#16 gully closed 8 years ago
2
Replicate O'Neal and Neff figures for OH lines and TiO lines

#15 gully closed 8 years ago
1
Figure of absolute flux ratio of hot and cool photosphere (as a function of wavelength)

#14 gully closed 8 years ago
1
Quality assurance of input spectra

#13 gully closed 8 years ago
1
Need to commit the config files for all orders so they are the same across machines.

#12 gully closed 8 years ago
2
How good is the spectral fit? Do the model spectra look reasonable?

#11 gully closed 8 years ago
1
Plot of starspot Teff versus starspot fill factor.

#10 gully closed 8 years ago
0
Generate synthetic, noised-up two-temperature model spectra, then naively fit a single temperature model to it.

#9 gully closed 8 years ago
0
Perform order-by-order analysis on the optical spectrum (ESPaDOnS)

#8 gully closed 8 years ago
1
Go order-by-order for the K-band.

#7 gully closed 8 years ago
1