Published July 19, 2026 | Version v3

An empirical model of the Gaia DR3 selection function

  • 1. Max Planck Institute for Astronomy
  • 2. ROR icon Leiden University

Description

Precomputed maps of the M10 parameter used to predict the completeness of the Gaia DR3 source catalogue.

allsky_M10_hpx7.hdf5 is a tessellation of the whole sky in Galactic nested healpix scheme of order 7.

allsky_uniq_10.fits uses an adaptive resolution and is based on the 'uniq' numbering of healpix tiles. Regions of higher density use a finer resolution, up to order 10, chosen so that every tile contains a minimum of twenty sources to compute M10 from.

Paper: https://ui.adsabs.harvard.edu/abs/2023A%26A...669A..55C/abstract

Tutorial using the GaiaUnlimited python package to query these maps: https://github.com/gaia-unlimited/gaiaunlimited/blob/main/docs/notebooks/dr3-empirical-completeness.ipynb

Documentation for the GaiaUnlimited package: https://gaiaunlimited.readthedocs.io/en/latest/

Files

Files (41.1 MB)

Name Size Download all
md5:4d80621b40aead69ee6759954b7292b2
4.7 MB Download
md5:0e844651d20aee967b590664ef4ca83e
36.3 MB Download

Additional details

Related works

Is documented by
Journal article: 10.1051/0004-6361/202244784 (DOI)
Preprint: 10.48550/arXiv.2208.09335 (DOI)

Funding

European Commission
GaiaUnlimited - Who is In, and Who is Not? Determining the Gaia Survey Selection Function 101004110

Dates

Updated
2026-07-19
Changed UNIQ field to integer type in allsky_uniq_10.fits, re-uploaded hdf5 file

References

  • Cantat-Gaudin et al. (2023) bibcode:2023A&A...669A..55C arXiv:2208.09335