T CrB photometry and spectroscopy requested for HST and XMM-Newton observations
Active Dates: Aug. 3, 2021 – Sept. 30, 2021
Abstract:
Monitoring the symbiotic recurrent nova T CrB in support of multiwavelength observations scheduled with HST and XMM-Newton in August and September.
Justification:
The campaign's goal is to observe the rate of accretion through the disk and onto the white dwarf and the rate of wind mass loss, leading up to the next nova eruption in a few years' time. This data will complement upcoming HST and XMM-Newton observations.
Requested Data Types:
Photometry, Spectroscopy
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| T CrB | 2.00 | NR+ELL |
Cadence: Nightly Precision: 100 |
Cadence: Nightly Resolution: 250 Desired SNR: 100 |
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. Koji Mukai (NASA-GSFC, University of Maryland); Imported Campaign (Alert Notice #750)