The Implementation of Binned Kernel Density Estimation to Determine Open Clusters' Proper Motions: Validation of the Method

Abstract

Stellar membership determination of an open cluster is an important process to do before further analysis. Basically, there are two classes of membership determination method: parametric and non-parametric. In this study, an alternative of non-parametric method based on Binned Kernel Density Estimation that accounts measurements errors (simply called BKDE-e) is proposed. This method is applied upon proper motions data to determine cluster's membership kinematically and estimate the average proper motions of the cluster. Monte Carlo simulations show that the average proper motions determination using this proposed method is statistically more accurate than ordinary Kernel Density Estimator (KDE). By including measurement errors in the calculation, the mode location from the resulting density estimate is less sensitive to non-physical or stochastic fluctuation as compared to ordinary KDE that excludes measurement errors. For the typical mean measurement error of 7 mas/yr, BKDE-e suppresses the potential of miscalculation by a factor of two compared to KDE. With median accuracy of about 93%, BKDE-e method has comparable accuracy with respect to parametric method (modified Sanders algorithm). Application to real data from The Fourth USNO CCD Astrograph Catalog (UCAC4), especially to NGC 2682 is also performed. The mode of member stars distribution on Vector Point Diagram is located at ${\mu }_{\alpha }\cos \delta =-9.94\pm 0.85$ mas/yr and ${\mu }_{\delta }=-4.92\pm 0.88$ mas/yr. Although the BKDE-e performance does not overtake parametric approach, it serves a new view of doing membership analysis, expandable to astrometric and photometric data or even in binary cluster search.

arXiv comment11 pages, 5 figures, accepted for publication in ApSS

References in corpus (15)

• The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)
• New catalogue of optically visible open clusters and candidates
• Astrophysical parameters of Galactic open clusters
• The second US Naval Observatory CCD Astrograph Catalog (UCAC2)
• Revisiting the population of Galactic open clusters
• Overlapping abundance gradients and azimuthal gradients related to the spiral structure of the Galaxy
• Open Clusters as Galactic Disk Tracers: I. Project Motivation, Cluster Membership and Bulk Three-Dimensional Kinematics
• Double or binary: on the multiplicity of open star clusters
• The Sun was not born in M 67
• Absolute proper motion of the Galactic open cluster M67
• Kinematic parameters and membership probabilities of open clusters in the Bordeaux PM2000 catalogue
• $uvby-H_{\beta }$ CCD photometry and membership segregation of the open cluster NGC2682 (M67)
• The Quest for the Sun's Siblings: an Exploratory Search in the Hipparcos Catalogue
• Cluster radius and sampling radius in the determination of cluster membership probabilities
• Open Cluster Evolutions in Binary System: How They Dissolved