A faint extended cluster in the outskirts of NGC 5128: evidence of a low mass accretion
Are small-scale substructures a universal property of galaxy haloes? The case of the giant elliptical NGC 5128
Deep ACS Imaging of the Halo of NGC 5128: Reaching the Horizontal Branch
How old are the stars in the halo of NGC 5128 (Centaurus A)?
Resolved Stellar Populations in Nearby Galaxy Halos
The Complex Star Formation History of the Halo of NGC 5128 (Cen A)
The impact of satellite trails on Hubble Space Telescope observations
The outer halo of the nearest giant elliptical: a VLT/VIMOS survey of the resolved stellar populations in Centaurus A to 85 kpc
The outermost stellar halo of NGC 5128 (Centaurus A): Radial structure
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2002-07-05T10:21:37Z/2002-07-09T12:45:39Z
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, Rejkuba comma Marina, 2003, 'Reaching the Horizontal Branch in NGC 5128: Deepest Probe of a Giant Elliptical', 1.0, European Space Agency, https://doi.org/10.5270/esa-ztsq94u