Characterizing Extreme Emission-line Galaxies. I. A Four-zone Ionization Model for Very High-ionization Emission
Characterizing Extreme Emission Line Galaxies. II. A Self-consistent Model of Their Ionizing Spectrum
Using Ne V/Ne III to Understand the Nature of Extreme-ionization Galaxies
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2018-06-21T03:12:17Z/2018-08-07T22:02:48Z
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, Berg et al., 2018, 'Resolving Extreme High-Ionization UV Emission-Line Diagnostics in Preparation for JWST', 1.0, European Space Agency, https://doi.org/10.5270/esa-kvu03w5