An HST COS ultraviolet spectroscopic survey of 311 DA white dwarfs - I. Fundamental parameters and comparative studies
Carbon to oxygen ratios in extrasolar planetesimals
Circumstellar debris and pollution at white dwarf stars
Discovery of Molecular Hydrogen in White Dwarf Atmospheres
Evidence for Water in the Rocky Debris of a Disrupted Extrasolar Minor Planet
Evidence of rocky planetesimals orbiting two Hyades stars
The chemical diversity of exo-terrestrial planetary debris around white dwarfs
The frequency and infrared brightness of circumstellar discs at white dwarfs
The frequency of planetary debris around young white dwarfs
The Hyades Cluster: Identification of a Planetary System and Escaping White Dwarfs
The unbiased frequency of planetary signatures around single and binary white dwarfs using Spitzer and Hubble
Unified line profiles for hydrogen perturbed by collisions with protons: satellites and asymmetries
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2010-09-17T09:03:45Z/2011-08-30T01:12:35Z
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, Gaensicke comma Boris T., 2012, 'The frequency and chemical composition of planetary debris discs around young white dwarfs', 1.0, European Space Agency, https://doi.org/10.5270/esa-lih25hy