Name
The name of the open cluster
l
Galactic longitude (degree)
b
Galactic latitude (degree)
r
Equivalent radius (degree)
a
Semi-major axis (degree)
b
Semi-minor axis (degree)
e
Ellipticity
angle
Angle between semi-major axis to the direction of increasing galactic longitude. (degree)
rc_pc
King profile core radius (pc)
rc_min
King profile core radius (arcmin)
rc_min_e
King profile core radius error (arcmin)
d_min
Min distance (pc)
d_max
Max distance (pc)
dist
Average distance between d_min and d_max (pc)
dmod
Mode distance (pc)
dist_e
Distance error (pc)
pmra
Proper motion in right ascension (mas/yr)
pmra_e
pmra error (mas/yr)
pmdec
Proper motion in declination (mas/yr)
pmdec_e
pmdec error (mas/yr)
r_mu
Proper motion radius (mas/yr)
member
Number of member stars that are inner spatial ellipse, proper motion radius, and distance range
cal_mem
Calibrated number of member stars using luminosity function
age
Age of cluster
br
The brightest stars’ G magnitude
brbr
The brightest stars’ G_bp-G_rp color index
bl
The bluest stars’ G magnitude
blbr
The bluest stars’ G_bp-G_rp color index
Corresponding Clusters
Cluster name format: ‘Cluster name’__‘Catalog or publication identifier’__‘code number’.
Identifier
dias
Dias W., Alessi B., Moitinho A., et al., 2002, New catalogue of optically visible open clusters and candidates, Astronomy & Astrophysics, 389, 871. (DALM).khar
Kharchenko N., Piskunov A., Schilbach E., et al., 2013, Global survey of star clusters in the Milky Way-II. The catalogue of basic parameters, Astronomy & Astrophysics, 558, A53. (MWSC).cocd
Kharchenko N., Piskunov A., Röser S., \etal, 2004, Astrophysical supplements to the ASCC‐2.5. II. Membership probabilities in 520 Galactic open cluster sky areas, Astronomische Nachrichten: Astronomical Notes, 325, 740 (COCD).cgoc
Cantat-Gaudin T., Jordi C., Vallenari A., et al., 2018, A Gaia DR2 view of the open cluster population in the Milky Way, Astronomy & Astrophysics, 618, A93.coin
Cantat-Gaudin T., Krone-Martins A., Sedaghat N., et al., 2019, Gaia DR2 unravels incompleteness of nearby cluster population: New open clusters in the direction of Perseus, Astronomy & Astrophysics, 624, A126.ubc
Castro-Ginard A., Jordi C., Luri X., et al., 2018, A new method for unveiling open clusters in Gaia-New nearby open clusters confirmed by DR2, Astronomy & Astrophysics, 618, A59.rsg
Röser S., Schilbach E., Goldman B., 2016, Nine new open clusters within 500 pc from the Sun, Astronomy & Astrophysics, 595, A22.Code number
1 : Satisfy only location
2 : Satisfy location and one of distance and proper motion.
3 : Satisfy location, distance and proper motion.