LPV Maser campaign extended through October 2020
Active Dates: Oct. 1, 2018 – Oct. 31, 2020
Abstract:
Dr. Michael Stroh (Northwestern University) informs us that his SiO maser study on long period variables is being extended through October 2020.
Justification:
The strengths of the SiO maser lines observed at 43 GHz in the radio are believed to be correlated with the phase of the stars in the sample and may allow us to probe the density in the stellar envelopes. VLA observations will likely occur about once every 3 weeks, and AAVSO sampling of targets ranging from 2 to 4 weeks through October 2020 will guide interpretation of the radio observations.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| R Cyg | 6.10 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| R Cas | 4.70 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| TY Cas | 10.10 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| FI Per | 12.90 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| SY Mon | 7.00 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| FX Mon | 10.20 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| NSVS 12572573 | 13.50 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| R Vul | 7.00 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| RT Aql | 7.60 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| SX Cyg | 8.20 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| AU Cyg | 8.20 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| V1655 Cyg | 12.00 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| NSVS J2041274+511326 | 14.20 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| DR Cyg | 8.70 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| W Cep | 7.02 | SRC |
Cadence: Not Specified Precision: 100 |
Not Requested |
| AL Cep | 9.90 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| VX Cep | 10.40 | M |
Cadence: Not Specified Precision: 100 |
Not Requested |
| BMAM-V657 | 13.48 | EA/RS |
Cadence: Not Specified Precision: 100 |
Not Requested |
| V Cas | 6.90 | 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. Michael Stroh; Imported Campaign (Alert Notice #687)