Proposal #286
| Proposer | (35799) Kalee Tock (kaleeg@stanford.edu) obscode: TKAA |
|---|---|
| Assigned To | (3663) Dirk Terrell |
| Date Submitted | Oct. 28, 2022 |
| Status | Allocated |
| Priority | Normal |
| Proposal | Hi! I would like to get some images of NGC 457 (the "Owl" or "ET cluster"). I understand that AAVSOnet is not designed for time-series image requests, so I am assuming that it will not be possible to take enough images to see the variation of V765 Cas (an Eclipsing Binary in the cluster). However, I would still be able to use as many images as it is possible to request in multiple filters to make a color-magnitude diagram of the cluster. The filters for which my software is designed to fit isochrones are SDSS uprime, gprime, rprime, iprime, zprime, B, and V. However, I can get a qualitative idea from other filters depending on availability. Note: I am filling in the form with the magnitudes for V765Cas (the EB). Thank you very much! |
| Target | RA (H.HH) | Dec (D.DD) | Magnitude | Telescope | Observation Frequency | Expiration Date | Proprietary Term |
|---|---|---|---|---|---|---|---|
| NGC 457 | 19.887000 | 58.27800 | 10.6–11.0 | BSM_NH2 | 1 | May 10, 2023 | No |
Comments
- (4726) Kenneth Menzies — Nov. 11, 2022, 10:11 p.m.
Committed to MPO61 and NH
- (4726) Kenneth Menzies — Nov. 11, 2022, 10:15 p.m.
IF you can define a future TOM for the EB, we could try a time series.
Comments on this proposal are closed.