Transformed photometry of young stars in Cha requested
Active Dates: Jan. 1, 2013 – Feb. 28, 2013
Abstract:
Dr. Péter Ábrahám (Konkoly Observatory, Budapest, Hungary) has requested the assistance of AAVSO observers in monitoring eight young stars in Chamaeleon in support of photometry he and his colleagues will be obtaining with the VLT/ISAAC (infrared) and Herschel Space Observatory (far-infrared) during January-February 2013.
Justification:
Calibrated, transformed VRI photometry is requested to precisely monitor changes in the optical brightness and colors of these objects. Calibration and transformation of the photometry is crucial - if all of the data are not on the same system and particularly if the colors are not transformed, it will be extremely difficult to correlate the data usefully.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| CR Cha | 10.92 | CTTS/ROT |
Cadence: Not Specified Precision: 100 |
Not Requested |
| CT Cha | 11.70 | CTTS |
Cadence: Not Specified Precision: 100 |
Not Requested |
| VW Cha | 12.40 | CTTS/ROT |
Cadence: Not Specified Precision: 100 |
Not Requested |
| VZ Cha | 12.10 | CTTS/ROT |
Cadence: Not Specified Precision: 100 |
Not Requested |
| WW Cha | 12.70 | CTTS |
Cadence: Not Specified Precision: 100 |
Not Requested |
| WX Cha | 13.40 | CTTS |
Cadence: Not Specified Precision: 100 |
Not Requested |
| XX Cha | 13.10 | CTTS |
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. Péter Ábrahám; Imported Campaign (Alert Notice #478)