THE ACS VIRGO CLUSTER SURVEY XVI. SELECTION PROCEDURE AND CATALOGS OF GLOBULAR CLUSTER CANDIDATES

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THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE SURVEY (2012, methodology): “In the NGVS, it will therefore be possible to extend the study of nuclei (e.g., frequency of nucleation, luminosity functions, mass fractions, CMRs, etc.) to galaxies hundreds of times fainter than the lowest-luminosity galaxies in the ACSVCS, and to explore possible dependencies of nuclear properti”
Families of dynamically hot stellar systems over 10 orders of magnitude in mass (2011, background): “This is the task of large imaging surveys (e.g. SDSS), or dedicated cluster surveys (e.g. ACSVCS).”
THE RELATIONSHIPS AMONG COMPACT STELLAR SYSTEMS: A FRESH VIEW OF ULTRACOMPACT DWARFS (2011, background): “We will also be comparing our spectroscopicallyconfirmed sample to a larger sample of photometricallyidentified GCs from a central ACS pointing on M87 (Jordán et al. 2009).”
WIDE-FIELD PRECISION KINEMATICS OF THE M87 GLOBULAR CLUSTER SYSTEM (2011, methodology): “Unlike for our sizes, Jordán et al. (2009) do not assume a fixed King model concentration, but (i) moderate variations in the concentration affect the half-light radius very little, and (ii) the S/N of the majority of GCs is insufficient to constrain this parameter in any case.”