VizieR Online Data Catalog: Large-scale structure of M31 halo. II. PAndAS (McConnachie+, 2018)

The primary observing goal of the Pan-Andromeda Archaeological Survey (PAndAS) was to provide contiguous mapping of the resolved stellar content of the halo of M31 out to approximately half of its halo virial radius (in projection; R_vir~300kpc), and it ran from 2008 to 2011. In addition, the aim was to map M33 out to a broadly equivalent radius (~50kpc), accounting for the difference in mass between these galaxies. PAndAS used the CFHT/MegaCam wide field camera in g- and i-band filters. Table 2 contains the observing log (spanning 2008 August to 2011 February) for the 2985 CFHT/MegaCam exposures.

(3 data files).