| refcode |
metd |
author |
reference |
| Cti1971 |
- |
Conti, P.S. & Alschuler, W.R. |
1971ApJ...170..325C |
| Cti1971 |
|
ApJ 170, 325, 1971 |
|
| Msn1998a |
Sc j |
Mason, B.D., Gies, D.R., Hartkopf, W.I., Bagnuolo, Jr., W.G., |
1998AJ....115..821M |
| Msn1998a |
|
ten Brummelaar, T.A., & McAlister, H.A. |
|
| Msn1998a |
|
AJ 115, 821, 1998 |
|
| Trn2008 |
Ac j |
Turner, N.H., ten Brummelaar, T.A., Roberts, L.C., Mason, B.D., Hartkopf, W.I., & |
2008AJ....136..554T |
| Trn2008 |
+E2 |
Gies, D.R. |
|
| Trn2008 |
+A |
AJ 136, 554, 2008 |
|
| Trn2008 |
|
(Note: For some observations the image derotator was in an unknown state. In these |
|
| Trn2008 |
|
cases the theta value is either left blank or two possible values are listed - one |
|
| Trn2008 |
|
for zenith up and one for north up. For unresolved objects, the listed rho value |
|
| Trn2008 |
|
is the FWHM of the corrected stellar PSF. Larger FWHM values are indicative of |
|
| Trn2008 |
|
poorer seeing and/or non-optimal AO system tuning.) |
|
