Tue, 07/30/2024 - 14:14
PNV J19430751+2100204 is a nova candidate (9.8 V) that has been reported to the IAU CBAT Transient Object Confirmation Page (TOCP). Spectroscopic confirmation is needed.
Here's the link to the VSX entry: https://www.aavso.org/vsx/index.php?view=detail.top&oid=2389912
A sequence will be created as soon as possible.
Please report your observations to the AAVSO: photometry/visual observations to the AID using WebObs, spectroscopy to AVSpec.
Many thanks, and good observing,
Elizabeth Waagen, AAVSO HQ
Kenta Taguchi has posted an ATel based on a spectrum from the 3.8-m Seimei telescope:
https://www.astronomerstelegram.org/?read=16743
\Brian
Dear Sequence Team, help please with comp stars for BVRI observations of Nova!
30 min field is preferable, but for bright stage field may be larger.
20240730.888 PNV J19430751+2100204 spectrum R~900
https://britastro.org/specdb/data_graph.php?obs_id=16646
Cheers
Robin
It looks heavily reddened, not surprising.
Arne
I did a time series this night, about 2 hours. It was slowing down.
N Vul 2024 has been assigned the GCVS name V615 Vul (V0615 Vul).
Alert Notice 867 reports on this nova. Please see the notice for details and observing instructions.
Important Note: The Alert Notices are in transition, and the format of Alert Notice 867 is very different from preceding Alert Notices! Also, please note that Alert Notices 865 and 866 have not been issued yet.
Many thanks, and good observing,
Elizabeth O. Waagen, AAVSO HQ
Two hours of Ic photometry of V0615 Vul centered on JD 2460535.605 shows flickering of amplitude 0.015 mag with period 4.11 minutes (mean), 3.88 minutes (median) +/-1.57 min. (st. dev.).
Rich Schmidt
Burleith Observatory
V0615 Vul
A period search using Generalized Lomb-Scargle and DCDFT (Ferraz-Mellow) on the above 2 hrs Ic photometry gives a flicker period of 4.377 +/- 0.346 minutes. Observations have been uploaded to WebObs.
Rich Schmidt (SREB)