Evidence for a bottom-light initial mass function in massive star clusters
Globular Clusters in the Outer Galactic Halo: New Hubble Space Telescope/Advanced Camera for Surveys Imaging of Six Globular Clusters and the Galactic Globular Cluster Age-metallicity Relation
Mass Segregation in the Globular Cluster Palomar 5 and its Tidal Tails
Multimass modelling of milky way globular clusters - II. Present-day black hole populations
Searching for multiple populations in Ruprecht 106
Stellar mass segregation as separating classifier between globular clusters and ultrafaint dwarf galaxies
The ACS Survey of Galactic Globular Clusters. VIII. Effects of Environment on Globular Cluster Global Mass Functions
The influence of black holes on the binary population of the globular cluster Palomar 5
The Main-Sequence Luminosity Function of Palomar 5 from THE HUBBLE SPACE TELESCOPE
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-08-10T09:24:13Z/1999-08-19T11:38:53Z
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, Smith et al., 2000, 'The Main Sequence Luminosity Function of Palomar 5', 1.0, European Space Agency, https://doi.org/10.5270/esa-lk2kq0n