GM Aur being observed by HST and TESS
Abstract:
Part V of the ODYSSEUS pre-main sequence star program starts this month. 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. The HST will monitor the pre-main sequence star GM Aur for 3 stellar rotation periods (about 18 days) starting 13 October. It is being observed simultaneously with TESS.
Justification:
It is the color changes that will help us determine the cause for any changes in the UV line fluxes, or in the overall brightness.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| 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 #756)