An independent determination of Fomalhaut bs orbit and the dynamical effects on the outer dust belt
A planetary system as the origin of structure in Fomalhauts dust belt
Feasibility of transit photometry of nearby debris discs
First published ALMA Early Science Cycle 0 Result - Mapping of the Fomalhaut Debris Disc
Fomalhaut b could be massive and sculpting the narrow, eccentric debris disc, if in mean-motion resonance with it
Fomalhauts Debris Disk and Planet: Constraining the Mass of Fomalhaut b from disk Morphology
HST/STIS imaging of Fomalhaut: New main belt structure and confirmation of Fomalhaut bs eccentric orbit
JWST/NIRCam Imaging of Young Stellar Objects. III. Detailed Imaging of the Nebular Environment around the HL Tau Disk
Optical Images of an Exosolar Planet 25 Light-Years from Earth
Searching for Planets Orbiting Fomalhaut with JWST/NIRCam
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, ACS/HRC
Temporal Coverage
2004-01-01T07:08:23Z/2004-08-02T03:54:58Z
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 PAUL, 2005, 'ACS detection of sub-stellar companions around Vega, Fomalhaut and beta Pic via parallax & proper motion', 1.0, European Space Agency, https://doi.org/10.5270/esa-6su00cu