Deep Photometry of the Globular Cluster M5: Distance Estimates from White Dwarf and Main-Sequence Stars
Isochrone fitting of Galactic globular clusters - I. NGC 5904
The distance to NGC 5904 (M 5) via the subdwarf main sequence fitting method
Instrument
STIS/CCD, WFPC2, WFPC2/PC
Temporal Coverage
1999-07-17T10:00:39Z/1999-08-09T13:09:55Z
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, Layden comma Andrew C., 2007, 'White Dwarf Distances to Globular Clusters and the RR Lyrae Luminosity Calibration -- M5.', 1.0, European Space Agency, https://doi.org/10.5270/esa-mgv8whd