Infrared Surface Brightness Fluctuations of Magellanic Star Clusters
Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations
The host galaxy/AGN connection in nearby early-type galaxies. A new view of the origin of the radio-quiet/radio-loud dichotomy?
The host galaxy/AGN connection in nearby early-type galaxies. Sample selection and hosts brightness profiles
The Infrared Nuclear Emission of Seyfert Galaxies on Parsec Scales: Testing the Clumpy Torus Models
The Infrared Surface Brightness Fluctuation Hubble Constant
The supermassive black hole of FornaxA
Unravelling the nuclear dust morphology of NGC 1365: a two-phase polar-RAT model for the ultraviolet to infrared spectral energy distribution
Instrument
NICMOS/NIC1, NICMOS/NIC2
Temporal Coverage
1997-12-19T11:19:59Z/1998-04-01T08:14:54Z
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, Graham comma James R., 1999, 'IR Surface Brightness Fluctuations of Fornax Cluster Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-sciowz7