An HST COS ultraviolet spectroscopic survey of 311 DA white dwarfs - I. Fundamental parameters and comparative studies
Constraints on Remnant Planetary Systems as a Function of Main-sequence Mass with HST/COS
The dearth of high-mass hydrogen-atmosphere metal-polluted white dwarfs within 40 pc
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
Instrument
COS, COS/FUV
Temporal Coverage
2015-10-16T06:48:58Z/2017-09-28T05:15:41Z
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, 2018, 'The frequency and chemical composition of rocky planetary debris around young white dwarfs: Plugging the last gaps', 1.0, European Space Agency, https://doi.org/10.5270/esa-hyf8i7q
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.