GM Aur and BP Tau monitoring for HST and TESS
Active Dates: Dec. 1, 2022 – Jan. 7, 2023
Abstract:
Dr. Frederick Walter (Stony Brook University) requests AAVSO observers' assistance in monitoring the classical T Tau stars GM Aur and BP Tau in support of observations with HST and TESS scheduled for now through mid-January 2023.
Justification:
ODYSSEUS is an international collaborative campaign to understand the processes involved in the formation of low mass stars, their circumstellar disks, and their planets, via the time-variability of these systems.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| BP Tau | 11.50 | CTTS/ROT |
Cadence: Not Specified Precision: 100 |
Not Requested |
| GM Aur | 11.80 | CTTS/ROT |
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. Frederick Walter; Imported Campaign (Alert Notice #801)