Proposer | (19565) Jamey Jenkins (jameyljenkins@gmail.com) obscode: JENJ |
---|---|
Assigned To | (3663) Dirk Terrell |
Date Submitted | March 29, 2023 |
Status | Allocated |
Priority | Normal |
Proposal | Hi, My name is Jamey Jenkins, observer code is JENJ.This is my first request for time on the AAVSOnet to obtain photometric data on several under observed LPVs and one Young Stellar Object (YSO). Following is my requested filter(s) and cadence for each. Three images per observation for stacking to improve SNR is preferred. Please upload calibrated images to my VPhot account. Any questions I can be contacted at jameyljenkins@gmail.com. V0373 Cep V 1 observation daily |
Target | RA (H.HH) | Dec (D.DD) | Magnitude | Telescope | Observation Frequency | Expiration Date | Proprietary Term |
---|---|---|---|---|---|---|---|
BG Cyg | 19.649300 | 28.51290 | 12.8–9.0 | BSM_NH2 | 5 | Oct. 3, 2023 | No |
R Cyg | 19.613700 | 50.19980 | 14.4–6.1 | BSM_NH2 | 5 | Oct. 3, 2023 | No |
U Her | 16.429800 | 18.89240 | 13.4–6.4 | BSM_NH2 | 5 | Oct. 3, 2023 | No |
W Per | 2.843800 | 56.98340 | 11.0–8.6 | BSM_NH2 | 5 | Oct. 3, 2023 | No |
V0373 Cep | 21.718500 | 66.11500 | 13.3–11.82 | BSM_NH2 | 1 | Oct. 3, 2023 | No |
The TAC suggests using multiple filters for V373 Cep as well.
My past observations of V373 Cep were V-only, and I didn't want to use more telescope time than necessary. If VBR is no problem then most certainly add those filters to the schedule. I would appreciate observations to begin when each star reaches a suitable (30+ degrees) in elevation this season and continue until they are unobservable later in the year. Thanks!!
Jamey Jenkins (JENJ)
Adding filters has a relatively minor impact on the observing time that is more than offset by the additional astrophysical information.
Sounds good...please let me know when we move to the next step in the proposal process.
Committed to NH. Pairs of exposures (long and short) for LPVs with large amplitude. Select exposure appropriate for photometry at different phase.
from email to BSM_NH2 : Summary of exposures is following
BG Cyg V-ok at 90s x 2, B-ok at 180s x 2, R-ok at 15s x 2
U Her V-change to 30s x 2 (90s is saturated), B-ok at 180s x 2, R-change to 5s x 6 (stacking 6 images for scintillation)
Ken Menzies, could you send me a note to my email? I have a question regarding transforming of AAVSOnet images... jameyljenkins@gmail.com
from email to BSM_NH2 : Summary of exposures is following
R Cyg V-ok at 90s x 2, B-ok at 180s x 2, R-ok at 15s x 2
Comments on this proposal are closed.