Monitoring requested for developing planetary systems dust production study
Active Dates: March 13, 2015 – Dec. 31, 2017
Abstract:
Dr. George Rieke (University of Arizona) and colleagues have requested AAVSO assistance in monitoring four stars with developing planetary systems. This campaign is similar to the one conducted in 2013.
Justification:
A key part of our program is to obtain optical photometry of the same stars that we are observing in the infrared under the Spitzer program. The optical data are needed to verify that any changes we see in the infrared are not just driven by changes in the brightness of the star, but are truly due to changes in the structure or dust content of the debris disk.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| HD 15407A | 6.95 | CST |
Cadence: Not Specified Precision: 100 |
Not Requested |
| HD 23514 | 9.43 | VAR |
Cadence: Not Specified Precision: 100 |
Not Requested |
| RZ Psc | 11.25 | UXOR |
Cadence: Not Specified Precision: 100 |
Not Requested |
| BMAM-V488 | 18.20 | UG |
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. George Rieke; Imported Campaign (Alert Notice #511)