g at the original files, it seems that the authors use indifferently the two notations (with or without the "V" for all there stars). (MB) | Details on Acronym: [TS2018] | |
[TS2018] | ||
Write: | <<[TS2018] sw5 wfc1 NNNNNN>> <<[TS2018] sw5 wfc2 NNNNNN>> <<[TS2018] ne7 wfc1 NNNNNN>> <<[TS2018] ne7 wfc2 NNNNNN>> <<[TS2018] sw20a wfc1 NNNNNN>> <<[TS2018] sw20a wfc2 NNNNNN>> <<[TS2018] sw20b uvis1 NNNNNN>> <<[TS2018] sw20b uvis2 NNNNNN>> <<[TS2018] sw23a wfc1 NNNNNN>> <<[TS2018] sw23a wfc2 NNNNNN>> <<[TS2018] sw23b uvis1 NNNNNN>> <<[TS2018] sw23b uvis2 NNNNNN>> | |
N: | 41+135+16+14+15+5 | |
Object: | RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable) | |
Stat: | is completely incorporated in Simbad | |
Note: | Use of HST ACS/WFC3 archival observations of 6 disc fields in M31 to identify N=226 RR Lyrae stars. | |
in source: | M 31 = NGC 224 | |
Ref: | =2018MNRAS.478.4590T | |
by | TANAKUL N. , SARAJEDINI A. | |
Mon. Not. R. Astron. Soc., 478, 4590-4601 (2018) | ||
RR Lyrae variables in M31 and its satellites: an analysis of the galaxy's population. | ||
o | <[TS2018] ne7 wfc1 NNNNNN> N=21 among (Nos 22960-124515), <[TS2018] ne7 wfc2 NNNNNN> N=20 among (Nos 61943-122846), <[TS2018] sw5 wfc1 NNNNN> N=68 among (Nos 1641-17003), <[TS2018] sw5 wfc2 NNNNN> N=67 among (Nos 2228-27525), <[TS2018] sw20a wfc1 NNNNN> N=6 among (Nos 15559-21279), <[TS2018] sw20a wfc2 NNNNN> N=10 among (Nos 16332-22047), <[TS2018] sw20b uvis1 NNNNN> N=7 among (Nos 4917-10706), <[TS2018] sw20b uvis2i NNNNN> N=5 among (Nos 5965-11309), <[TS2018] sw23a wfc1 NNNNN> N=11 among (Nos 8274-18395), <[TS2018] sw23a wfc2 NNNNN> N=4 among (Nos 10420-14574), <[TS2018] sw23b uvis1 NNNN> (Nos 3026, 3407, 3536), <[TS2018] sw23b uvis2 NNNN> (Nos 3184, 3443). | |
=E= | Catalogue in electronic form as <J/MNRAS/478/4590/> | |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |