V386 Ser HST observations rescheduled
Active Dates: June 21, 2019 – Aug. 10, 2019
Abstract:
The HST observations of the cataclysmic variable V386 Ser have been rescheduled to August 1 - 3, 2019. AAVSO observations are crucial to determine the system's state, ensuring it is not in outburst during HST observation.
Justification:
AAVSO observations are essential to know the state of the V386 Ser system to ensure it is not in outburst when observed with HST. Observations made 24 hours before the HST observing time will be used to make a go/no-go decision and aid in the analysis of the HST data.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| V0404 Ser | 12.20 | 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. Paula Szkody; Imported Campaign (Alert Notice #669)