WIYN Open Cluster Study: Deep Observations of Open Clusters

Details WIYN Open Cluster Study: Deep Observations of Open Clusters WIYN Open Cluster Study: Deep Observations of Open Clusters

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.5824j&link_type=abstract

American Astronomical Society, AAS Meeting #211, #58.24; Bulletin of the American Astronomical Society, Vol. 39, p.837

Astronomy and Astrophysics

Astronomy

Scientific paper

Open clusters provide the ideal environment for the calibration of the ages determined from main sequence evolution theory (via cluster isochrones) and those determined from white dwarf cooling theory. Additionally, it provides the unique opportunity to directly compare and refine our understanding of both theories. Because the coolest cluster white dwarfs are faint, they require observations made with large telescopes or the Hubble Space Telescope (HST). We present new deep observations of three clusters taken with ACS on HST, as well as archival data of one cluster taken with WFPC2. For our analysis, we employ a new Bayesian statistical technique.

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