Nova in Perseus: N Per 2020
Active Dates: Nov. 25, 2020 – Nov. 27, 2020
Abstract:
Announcement of the discovery of Nova in Perseus: N Per 2020 by Seiji Ueda and Stanislav Korotkiy, Kirill Sokolovsky, and Olga Smolyankina, and recommendations for observations.
Justification:
The nova is evolving and spectra indicate it is close to maximum brightness. Monitoring its development will provide valuable insights.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| R Per | 8.10 | M |
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: Elizabeth O. Waagen; Imported Campaign (Alert Notice #726)