A Deep Keck/NIRC2 Search for Thermal Emission from Planetary Companions Orbiting Fomalhaut
An independent determination of Fomalhaut bs orbit and the dynamical effects on the outer dust belt
Direct Imaging Confirmation and Characterization of a Dust-enshrouded Candidate Exoplanet Orbiting Fomalhaut
First published ALMA Early Science Cycle 0 Result - Mapping of the Fomalhaut Debris Disc
Fomalhaut b as A Cloud of Dust: Testing Aspects of Planet Formation Theory
Fomalhaut b could be massive and sculpting the narrow, eccentric debris disc, if in mean-motion resonance with it
Fomalhaut b: Independent Analysis of the Hubble Space Telescope Public Archive Data
HST/STIS imaging of Fomalhaut: New main belt structure and confirmation of Fomalhaut bs eccentric orbit
Optical Images of an Exosolar Planet 25 Light-Years from Earth
STIS Coronagraphic Imaging of Fomalhaut: Main Belt Structure and the Orbit of Fomalhaut b
The companion candidate near Fomalhaut - a background neutron star?
Instrument
ACS/HRC
Temporal Coverage
2006-07-14T18:43:24Z/2006-07-20T03:03:10Z
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, Kalas comma Paul George, 2007, 'ACS Imaging of Fomalhaut: A Rosetta Stone for Debris Disks Sculpted by Planets', 1.0, European Space Agency, https://doi.org/10.5270/esa-s60bwmy