Publications

 

Paper I: Sarajedini et al. 2007, "The ACS Survey of Galactic Globular Clusters. I. Overview and Clusters Without Previous HST Photometry," AJ, 133, 1658 (ps) (pdf)

Paper I data files: NGC 5466, NGC 6779, NGC 5053, NGC 6144, Palomar 2, E 3, Lynga 7, Palomar 1, NGC 6366, M92 fiducial, NGC 6752 fiducial, 47 Tuc fiducial (readme file)

 

Paper II: Dotter et al. 2007, "The ACS Survey of Galactic Globular Clusters. II. Stellar Evolution Tracks, Isochrones, Luminosity Functions, and Synthetic Horizontal-Branch Models," AJ, 134, 376 (ps) (pdf)

Paper II theoretical models are available here.

 

Paper III: Milone et al. 2007, "The ACS Survey of Galactic Globular Clusters. III. The Double Subgiant Branch of NGC 1851," ApJ, 673, 241 (pdf) (NGC 1851 Photometry File) (README) Please refer to Paper V for a full discussion of the data files and their contents.

 

Paper IV: Siegel et al. 2007, "The ACS Survey of Galactic Globular Clusters: M54 and Young Populations in the Sagittarius Dwarf Spheroidal Galaxy," ApJL, 667, L57 (ps) (pdf)

 

Paper V: Anderson et al. 2008, "The ACS Survey of Galactic Globular Clusters. V. Generating a Comprehensive Star Catalog for each Cluster," AJ, 135, 2055 (pdf)

 

Paper VI: Paust et al. 2009, "The ACS Survey of Galactic Globular Clusters. VI. NGC 6366: a Heavily Stripped Galactic Globular Cluster," AJ, 137, 246 (pdf) (NGC 6366 Photometry File) (README) Please refer to Paper V for a full discussion of the data files and their contents.

 

Paper VII: Marin-Franch et al. 2009, "The ACS Survey of Galactic Globular Clusters. VII. Relative Ages," ApJ, 694, 1498

 

Paper VIII: Paust et al. 2010, "The ACS Survey of Galactic Globular Clusters. VIII. Effects of Environment on Globular Cluster Global Mass Functions," AJ, 139, 476

 

Paper IX: Dotter et al. 2010, "The ACS Survey of Galactic Globular Clusters. IX. Horizontal Branch Morphology and the Second Parameter Phenomenon," ApJ, 708, 698

 

 

As a courtesy, please send an email to ata@astro.ufl.edu if you decide to download these data.