| Observatory | Telescopes | Community Access | Capabilities | Application Due Dates | Time Allocation Contact |
|---|---|---|---|---|---|
| Mount Laguna Observatory | 1m and 0.6m | direct imager, photoelect photometer | Paul Etzel | ||
| Lowell Observatory | Perkins 1.8m | 17% research time available to astronomical community | PRISM, a wide-field optical imager, polarimeter and spectrometer | Feb. 1, May 1, Aug. 1, Nov. 1 | Ken Janes |
| Michigan State University Observatory | 0.6m | 20% research time available to astronomical comunity | BVI imaging and differential photometry | by arrangement | Horace Smith |
| UNC (PROMPT) | six 0.4m robotic | 10% time available through peer evaluation to astronomical community; 30% time available to local consortia institutions | Optical and NIR imaging and optical polarimetry | Daniel Reichart | |
| FHIRE | 1.3m | Caty Pilachowski | |||
| Ritter Observatory, University of Toledo | 1.1m | 25% research time available to community, Service observing; hands on training of visiting grad, undergrad students; public data archive | Two fiber-fed spectrographs, low-resolution (R = 6,000) and high-resolution (R = 26,000) | Aplications accepted any time | Nancy Morrison |