Details on Acronym: [SGK2017] | |
[SGK2017] | (Soraisam+Gilfanov+Kupfer+, 2017) |
Write: | <<[SGK2017] NNNN>> |
Object: | Poss. Nova (SIMBAD class: Nova_Candidate = Classical Nova Candidate) |
Note: | N=15 nova candidates detected in a systematic search for novae in the intermediate Palomar Transient Factory (iPTF) observations of the bulge part of M31 during the second half of 2013. |
in source: | M 31 = NGC 224 |
Ref: | =2017A&A...599A..48S |
by | SORAISAM M.D. , GILFANOV M., KUPFER T., MASCI F., SHAFTER A.W., PRINCE T.A., KULKARNI S.R., OFEK E.O., BELLM E. |
Astron. Astrophys., 599A, 48-48 (2017) | |
A novel method for transient detection in high-cadence optical surveys. Its application for a systematic search for novae in M 31. | |
o | Table 2: <[SGK2017] NNNN> N=15 among (Nos 89-3182). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |