Monitoring of V338 Boo
Abstract:
Monitoring of the double-mode RR Lyr variable V338 Boo to fully characterize the long-term changes of this RR Lyrae variable star.
Justification:
Follow-up observations are needed to more fully characterize the long-term changes of V338 Boo, a double-mode (RRd) RR Lyrae variable star. Previous observations, including from TESS, showed major changes in the star's pulsation properties over tens of days. Longer monitoring is required due to the insufficient observation window of TESS, which was only about 54 days.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| R Boo | 6.00 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
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: Dr. Kenneth Carrell, Ron Wilhelm, Horace Smith; Imported Campaign (Alert Notice #786)