2059+48 Nova Cygni 2001 No. 2 AND 2003+17 WZ Sagittae superoutburst continues - recovering from dramatic dip [V2275 Cyg]
Abstract:
This campaign covers observations of two celestially-interesting events: the nova Nova Cygni 2001 No. 2 discovered independently by Akihiko Tago and K. Hatayama, and the ongoing superoutburst of WZ Sagittae, a dwarf nova cataclysmic variable.
Justification:
Nova Cygni 2001 No. 2 is a newly discovered nova requiring follow-up observations to study its development. WZ Sagittae's superoutburst, characterized by dramatic variations in brightness, presents a rare opportunity to study the evolution of superhumps and disk structure in cataclysmic variables.
Requested Data Types:
Spectroscopy, Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| ASAS J203252+2001.6 | 11.24 | MISC |
Cadence: Not Specified Precision: 100 |
Cadence: Not Specified Resolution: 250 Desired SNR: 100 |
Spectroscopy Lines:
No spectroscopy lines provided
Photometry Filters:
V (Johnson), r (Sloan), i (Sloan)
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: A. Nakamura, K. Hatayama; Imported Campaign (Alert Notice #287)