Clusterix 2.0
× This is a beta version. Clusterix is still in development which means you can encounter some bugs or experience some changes as we are constantly adjusting and improving the application.
If you want to know more about the project, submit feedback or report a bug, please contact us

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 proposed by Cabrera-Caño& Alfaro (1990) and described in Galadí-Enríquez et al. 1998. 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.
For more information visit the following link

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

Search by Id

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 also in Arenou et al (2018).

Search by Coordinates


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

Search by file?
File format example:

Download example 1
Download example 2
Download example 3

--> Access to user vosa files