A data-driven Bayesian approach for finding young stellar populations in early-type galaxies from their ultraviolet-optical spectra
Hubble Space Telescope Observations and Photoionization Modeling of the LINER Galaxy NGC 1052
Integrated Ultraviolet Spectra and Line Indices of M31 Globular Clusters and the Cores of Elliptical Galaxies
Is the giant elliptical galaxy NGC 5018 a post-merger remnant?
The mid-UV population of the nucleus and the bulk of the post-merger NGC 3610
The star formation histories of elliptical galaxies across the Fundamental Plane
UV-extended E-MILES stellar population models: young components in massive early-type galaxies
Instrument
FOS/RD
Temporal Coverage
1996-07-05T20:46:59Z/1996-12-21T02:22:18Z
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, Burstein et al., 1997, 'UV SPECTRA OF REPRESENTATIVE STELLAR POPULATIONS OF AGE > 2 GYR', 1.0, European Space Agency, https://doi.org/10.5270/esa-zhth6ms