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
Constraints on Remnant Planetary Systems as a Function of Main-sequence Mass with HST/COS
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
Measurements of three exo-planetesimal compositions: a planetary core, a chondritic body, and an icy Kuiper belt analogue
The chemical diversity of exo-terrestrial planetary debris around white dwarfs
The dearth of high-mass hydrogen-atmosphere metal-polluted white dwarfs within 40 pc
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
Ultraviolet extinction correlation with 3D dust maps using white dwarfs
Unified line profiles for hydrogen perturbed by collisions with protons: satellites and asymmetries
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2010-09-17T09:18:54Z/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, 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