| PI |
Title |
Dark |
Gray |
Bright |
|
| David W. Latham |
How Do Hot Jupiters Form and Migrate
Inward? |
0 |
5 |
5 |
|
| Jason Dittmann |
MEarth Spectroscopic
Follow-up |
0 |
2 |
2 |
|
| David W.
Latham |
Spectroscopic
follow-up of K2 Planet Candidates |
0 |
3 |
2 |
|
| Guillermo
Torres |
Low-mass eclipsing
binaries |
0 |
4 |
8 |
|
| David W.
Latham |
Transiting Planet
Candidate Follow-Up - 60 inch |
0 |
10 |
10 |
|
| Guillermo
Torres |
Accurate masses for
evolved stars |
0 |
0 |
1 |
|
| Guillermo
Torres |
Accurate masses for
selected double-lined eclipsing binaries |
0 |
0 |
8 |
|
| Guillermo
Torres |
Pleiades binary
survey |
0 |
0 |
8 |
|
| Andrea Dupree |
Chromospheres of
Dwarf Stars |
0 |
0 |
3 |
|
| Guillermo
Torres |
Comfirming runaway
stars in the binary supernova scenario |
0 |
0 |
2 |
|
|
|
|
|
|
|