A comparative analysis of the observed white dwarf cooling sequence from globular clusters, Campos, Fabíola,Bergeron, P.,Romero, A. D., Monthly Notices of the Royal Astronomical Society, 456, 2016-03-01 00:00:00, 2016MNRAS.456.3729C||A Deep, Wide-field, and Panchromatic View of 47 Tuc and the SMC with HST: Observations and Data Analysis Methods, Kalirai, Jason S.,Richer, Harvey B.,Anderson, Jay, The Astronomical Journal, 143, 2012-01-01 00:00:00, 2012AJ....143...11K||A Dynamical Signature of Multiple Stellar Populations in 47 Tucanae, Richer, Harvey B.,Heyl, Jeremy,Anderson, Jay, The Astrophysical Journal, 771, 2013-07-01 00:00:00, 2013ApJ...771L..15R||An age difference of two billion years between a metal-rich and a metal-poor globular cluster, Hansen, B. M. S.,Kalirai, J. S.,Anderson, J., Nature, 500, 2013-08-01 00:00:00, 2013Natur.500...51H||An Empirical Measure of the Rate of White Dwarf Cooling in 47 Tucanae, Goldsbury, R.,Heyl, J.,Richer, H. 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Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-01-15T05:11:16Z/2010-10-01T21:00:10Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
