Nova in Scutum - N Sct 2018 = TCP J18292290-1430460
Abstract:
A nova in the constellation Scutum was discovered by Yukio Sakurai on 2018 June 29.5768 UT with an unfiltered CCD magnitude of 10.3. Spectroscopic analysis identified it as a classical nova in the optically thick (Fe-curtain) stage.
Justification:
Observations of all types (visual, CCD, DSLR, PEP, spectroscopy) and multiple bands as instrumentation permits are strongly encouraged as the nova evolves.
Requested Data Types:
Photometry, Spectroscopy
Targets
Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
---|---|---|---|---|
V0487 Sct | 15.70 | L: |
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: Yukio Sakurai; Imported Campaign (Alert Notice #638)