GW Lib time scheduled for first HST observation
Abstract:
This campaign focuses on the pulsating white dwarf-containing cataclysmic variable GW Lib. For the HST observations, AAVSO observations are essential to know the state of the system in order to ensure that the object is NOT in outburst when observed with HST.
Justification:
In order to ensure that the object is NOT in outburst when observed with HST. AAVSO observations made 24-30 hours before each HST observing time will be used to make a go/no-go decision, and will also be used in the analysis of the resulting data.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| GW Lib | 8.20 | UGWZ+ZZ/GWLIB |
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. Boris Gaensicke; Imported Campaign (Alert Notice #595)