Clusterix 2.0

Clusterix 2.0 is an interactive web-based application to calculate the grouping probability of a list of objects using proper motions and the non parametric method in the approach described in Balaguer-Nuñez et al (2020). It also allows the possibility of gathering physical parameters (parallaxes, radial velocities, proper motions,...) from Vizier and estimating effective temperatures, surface gravities and metallicities using VOSA.
An step-by-step example on how to use Clusterix can be found here
NOTE: When working with Clusterix, it is recommendable to open a private window to avoid caching problems.

Step 1/3: Information gathering (coordinates and physical parameters)

Search by Id


Q-Filter?
Filters from eqs. C.1 and C.2 from Lindegren et al (2018) for an
astrometrically clean subset. More information about spurious
astrometric solutions in Gaia DR2 can also be found in Arenou et al (2018).



Search by Coordinates


Q-Filter?



Search in Webda ?
ID is the merge of the Data source reference and the star number: Ref_Star

Search by file?
File format example:
ID,RAJ2000,DEJ2000,pmRAcosdelta,epmRAcosdelta,pmDEC,epmDEC
0001,132.584,11.8197,-1.70,1.00,+1.60,0.50
0002,132.613,11.8088,+0.10,0.50,+1.50,0.30
0003,132.641,11.7742,-1.90,0.20,+0.60,0.40
0004,132.651,11.7217,-1.90,0.40,+1.10,0.60
0005,132.653,11.8153,-1.60,0.40,+1.10,0.40
0006,132.67,11.7961,,,,
0007,132.669,11.7032,-1.70,0.80,+0.90,1.30



Download example 1
Download example 2
Download example 3


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