AGN feedback and multiphase gas in giant elliptical galaxies
Circumnuclear Dust in Luminous Early-type Galaxies. I. Sample Properties and Stellar Luminosity Models
Detection of an Optical/UV Jet/Counterjet and Multiple Spectral Components in M84
Direct Detections of Young Stars in Nearby Elliptical Galaxies
Nonlinear Color-Metallicity Relations of Globular Clusters. III. On the Discrepancy in Metallicity between Globular Cluster Systems and Their Parent Elliptical Galaxies
Nonlinear Color-Metallicity Relations of Globular Clusters. IV. Testing the Nonlinearity Scenario for Color Bimodality via HST/WFC3 u-band Photometry of M84 (NGC 4374)
The impact of satellite trails on Hubble Space Telescope observations
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2009-11-23T18:28:39Z/2010-03-29T03:59:52Z
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, Bregman et al., 2011, 'The Star Formation Rate In Nearby Elliptical Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-l9o1im2