Accretion onto Planetary Mass Companions of Low-mass Young Stars
A library of near-infrared integral field spectra of young M-L dwarfs
A Mid-infrared Study of Directly Imaged Planetary-mass Companions Using Archival Spitzer/IRAC Images
Astrometric follow-up observations of directly imaged sub-stellar companions to young stars and brown dwarfs
Disk of 2MASS 15491331-3539118 = GQ Lup C as seen by HST and WISE
Peering into the young planetary system AB Pic. Atmosphere, orbit, obliquity, and second planetary candidate
The search for disks or planetary objects around directly imaged companions: a candidate around DH Tauri B
Three Wide Planetary-mass Companions to FW Tau, ROXs 12, and ROXs 42B
To v and beyond! The He I absorption variability across the 2014.6 periastron passage of e Carinae
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2012-01-10T18:50:42Z/2012-10-16T17:29:37Z
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, Kraus et al., 2013, 'The Formation and Fundamental Properties of Wide Planetary-Mass Companions', 1.0, European Space Agency, https://doi.org/10.5270/esa-5m19pnh
