Photometry and astrometry with JWST - III. A NIRCam-Gaia DR3 analysis of the open cluster NGC 2506
Survey of Multiple Populations in Globular Clusters among Very-low-mass Stars
The HST large programme on NGC 6752 - III. Detection of the peak of the white dwarf luminosity function
The HST Large Programme on NGC 6752 - II. Multiple populations at the bottom of the main sequence probed in NIR
The HST Large Programme on NGC 6752. I. Serendipitous discovery of a dwarf Galaxy in background
The HST large programme on NGC 6752 - IV. The White Dwarf sequence
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS/WFC, WFC3/IR
Temporal Coverage
2018-09-07T02:02:54Z/2019-08-15T21:14:19Z
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., 2019, 'The end of the White Dwarf Cooling Sequence of NGC 6752', 1.0, European Space Agency, https://doi.org/10.5270/esa-hpgrdei