|Proposer||(35799) Kalee Tock (firstname.lastname@example.org) obscode: TKAA|
|Assigned To||(3663) Dirk Terrell|
|Date Submitted||Oct. 28, 2022|
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|
Committed to MPO61 and NH
IF you can define a future TOM for the EB, we could try a time series.
Comments on this proposal are closed.