A census of nuclear stellar discs in early-type galaxies
A population of luminous accreting black holes with hidden mergers
Connecting Infrared Surface Brightness Fluctuation Distances to Type Ia Supernova Hosts: Testing the Top Rung of the Distance Ladder
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
History and destiny of an emerging early-type galaxy. New IFU insights on the major-merger remnant NGC 7252
Identification of a new ultraluminous X-ray source in NGC 1316
Is the escape velocity in star clusters linked to extended star formation histories? Using NGC 7252: W3 as a test case
Luminosity profiles and sizes of massive star clusters in NGC 7252
Measuring Infrared Surface Brightness Fluctuation Distances with HST WFC3: Calibration and Advice
Mid-infrared dust in two nearby radio galaxies, NGC 1316 (Fornax A) and NGC 612 (PKS 0131-36)
Sizes, Half-mass Densities, and Mass Functions of Star Clusters in the Merger Remnant NGC 1316: Clues to the Fate of Second-generation Globular Clusters
The distance to NGC 1316 (Fornax A): yet another curious case
The impact of satellite trails on Hubble Space Telescope observations
The Nature of the Bright ULX X-2 in NGC 3921: A Chandra Position and HST Candidate Counterpart
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2009-11-09T05:00:10Z/2010-10-03T10:11:44Z
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, Goudfrooij comma Paul, 2011, 'Using Massive Star Clusters in Merger Remnants To Provide Reference Colors of Intermediate-Age Stellar Populations', 1.0, European Space Agency, https://doi.org/10.5270/esa-ofc07dz