Anticipated primary eclipse of b Per centered on November 28 2023 UT
Abstract:
High time-resolved photometry of the bright star b Persei during the upcoming predicted primary eclipse of the AB inner pair by the third star is requested.
Justification:
The observations are desired to study the ellipsoidal variation of b Persei and to obtain high-resolution time-series observations to calibrate the various offsets expected from different observing systems during the primary eclipse.
Requested Data Types:
Photometry
Spectroscopy Lines:
No spectroscopy lines provided
Photometry Filters:
No photometry filters provided
Comparison Stars:
No comparison stars provided
Co-Authorship
Observers are not eligible for co-authorship.
Additional Observer Input:
Not provided
Additional Submission Location:
Not provided
Forum URL
N/A
Notes:
Principal Investigator: Donald F. Collins, Robert Zavala, Jason Sanborn, Anatoly Miroshnichenko; Imported Campaign (Alert Notice #840)