English

A maximum volume density estimator generalized over a proper motion-limited sample

Astrophysics of Galaxies 2015-06-22 v3

Abstract

The traditional Schmidt density estimator has been proven to be unbiased and effective in a magnitude-limited sample. Previously, efforts have been made to generalize it for populations with non-uniform density and proper motion-limited cases. This work shows that the then-good assumptions for a proper motion-limited sample are no longer sufficient to cope with modern data. Populations with larger differences in the kinematics as compared to the local standard of rest are most severely affected. We show that this systematic bias can be removed by treating the discovery fraction inseparable from the generalized maximum volume integrand. The treatment can be applied to any proper motion-limited sample with good knowledge of the kinematics. This work demonstrates the method through application to a mock catalogue of a white dwarf-only solar neighbourhood for various scenarios and compared against the traditional treatment using a survey with Pan-STARRS-like characteristics.

Keywords

Cite

@article{arxiv.1504.04643,
  title  = {A maximum volume density estimator generalized over a proper motion-limited sample},
  author = {Marco C. Lam and Nicholas Rowell and Nigel C. Hambly},
  journal= {arXiv preprint arXiv:1504.04643},
  year   = {2015}
}

Comments

12 pages, 10 figures, 2 tables. v2: typo correction. Published in MNRAS

R2 v1 2026-06-22T09:18:09.376Z