Nova Sco 2011 No. 2
Active Dates: Sept. 6, 2011 – Sept. 10, 2011
Abstract:
A nova was discovered independently by John Seach and Yuji Nakamura in Scorpius. Spectra suggest it is a highly reddened Fe II-type classical nova, and it has been confirmed as a young galactic nova.
Justification:
To study the characteristics and evolution of this newly discovered nova.
Requested Data Types:
Photometry, Spectroscopy
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| PNV J21173768+2107359 | 16.80 | UG |
Cadence: Not Specified Precision: 100 |
Cadence: Not Specified Resolution: 250 Desired SNR: 100 |
| V1313 Sco | 10.40 | NA |
Cadence: Not Specified Precision: 100 |
Cadence: Not Specified 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: John Seach and Yuji Nakamura; Imported Campaign (Alert Notice #447)