|Proposer||(33599) Clifford Kotnik (email@example.com) obscode: KCLA|
|Assigned To||(3663) Dirk Terrell|
|Date Submitted||July 6, 2020|
HIP 105217 was identified as variable by Hipparcos 30 years ago. Recent TESS full frame images allow this object to be identified as a GDOR with multiple periods of pulsation. The strongest periods are approximately 0.615 and 0.577 days. There are some indications from TESS of a period around 0.02 days (29 minutes).
|Target||RA (H.HH)||Dec (D.DD)||Magnitude||Telescope||Observation Frequency||Expiration Date||Proprietary Term|
|HIP 105217||21.312400||-23.80783||8.75–8.71||BSM_S||2||Jan. 17, 2021||No|
Time series plan generated and committed to BSM_S and BSM_Berry.
Comments on this proposal are closed.