A Search for Short-period Rocky Planets around WDs with the Cosmic Origins Spectrograph (COS)
Doppler imaging of the planetary debris disc at the white dwarf SDSS J122859.93+104032.9
Non-LTE models for the gaseous metal component of circumstellar discs around white dwarfs
The chemical diversity of exo-terrestrial planetary debris around white dwarfs
The composition of a disrupted extrasolar planetesimal at SDSS J0845+2257 (Ton 345)
The gaseous debris disk of the white dwarf SDSS J1228+1040. HST/COS search for far-ultraviolet signatures
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2010-02-19T15:31:29Z/2010-04-12T19:31:55Z
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, Gaensicke et al., 2011, 'An intensive COS spectroscopic study of the planetary debris disks around two warm white dwarfs', 1.0, European Space Agency, https://doi.org/10.5270/esa-33v0re9