Proposal #171
Proposer | (38606) Gabriel Neagu (gabrielneagu874@gmail.com) obscode: NGCA |
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Assigned To | (3663) Dirk Terrell |
Date Submitted | Dec. 16, 2020 |
Status | Declined |
Priority | Normal |
Proposal | Hello |
Target | RA (H.HH) | Dec (D.DD) | Magnitude | Telescope | Observation Frequency | Expiration Date | Proprietary Term |
---|---|---|---|---|---|---|---|
HD 46089 | 6.530083 | 11.54442 | 5.25–5.21 | — | — | — | No |
Comments
- (3663) Dirk Terrell — Dec. 17, 2020, 1:02 p.m.
The VSX entry shows B and V data of amplitude 3-4%. There appears to be no difference in amplitude between B and V, so it is unclear how I data would help you better understand this star. Is the 5-hour request based on a preliminary period? A 5 or 10 hour period with the light curve shape and amplitude, along with a lack of color variation is suggestive of a low inclination W UMa variable. Such a system would have little scientific value.
- (38606) Gabriel Neagu — Dec. 17, 2020, 1:48 p.m.
Hi
The 5 hours data is needed to have a longer timeline for the observations. The period is around 72 minutes. The variable star is a DSCT, but again, to confirm this we need the I band data to show the chromaticity. The chances are high that's a DSCT because of the period and spectral type.
Also, it's normal that at the presented scatter, B-V index is hard to measure.
Comments on this proposal are closed.