Dual Stellar Halos in the Standard Elliptical Galaxy M105 and Formation of Massive Early-type Galaxies
Hubble Space Telescope Photometry for the Halo Stars in the Leo Elliptical NGC 3377
Photometric Completeness Modelled with Neural Networks
The Extragalactic Distance Scale Without Cepheids. II. Surface Brightness Fluctuations
The halo of M 105 and its group environment as traced by planetary nebula populations. I. Wide-field photometric survey of planetary nebulae in the Leo I group
The impact of satellite trails on Hubble Space Telescope observations
The Leo Elliptical NGC 3379: A Metal-Poor Halo Emerges
The Tip of the Red Giant Branch Distances to Type Ia Supernova Host Galaxies. IV. Color Dependence and Zero-point Calibration
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2004-03-20T14:05:38Z/2004-04-19T16:22:42Z
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, HARRIS WILLIAM E., 2005, 'Establishing the Metallicity Distribution in Normal Giant Ellipticals', 1.0, European Space Agency, https://doi.org/10.5270/esa-12dj46p