A comparative analysis of the observed white dwarf cooling sequence from globular clusters
A fast matching algorithm for sheared stellar samples: k-d match
Deep Near-IR Observations of the Globular Cluster M4: Hunting for Brown Dwarfs
Improved white dwarves constraints on inelastic dark matter and left-right symmetric models
The age of the Milky Way inner halo
The End of the White Dwarf Cooling Sequence in M4: An Efficient Approach
The Hubble Space Telescope UV legacy survey of galactic globular clusters - XVI. The helium abundance of multiple populations
The impact of satellite trails on Hubble Space Telescope observations
The M 4 Core Project with HST - II. Multiple stellar populations at the bottom of the main sequence
Instrument
ACS, ACS/WFC
Temporal Coverage
2004-07-25T09:07:12Z/2005-06-27T14:17:16Z
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.
European Space Agency, Bedin comma Luigi R., 2006, 'Solving the problem of the White Dwarf Cooling Sequence End in M4: an efficent approach', 1.0, European Space Agency, https://doi.org/10.5270/esa-rxef2m9