A Model of the C IV l l1548, 1550 Doublet Line in T Tauri Stars
A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. I. HST Far-UV and Near-UV Spectra
A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. III. Optical Spectra
A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. II. Photometric Light Curves
An Ultraviolet Study of CO Chemistry in the Magellanic Clouds
Evidence of a Disk Wind Origin for Fluorescent H2 in Classical T Tauri Stars
PENELLOPE: VII. Revisiting empirical relations to measure accretion luminosity
The ODYSSEUS Survey. Characterizing Magnetospheric Geometries and Hotspot Structures in T Tauri Stars
The ODYSSEUS Survey. Spatial Correlation of Magnetospheric Inclinations Points to Parsec-scale Star-Cloud Connection
The ODYSSEUS Survey. Using Accretion and Stellar Rotation to Reveal the Star-Disk Connection in T Tauri Stars
The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Directors Discretionary Program with Hubble. I. Goals, Design, and Initial Results
The wind properties of O-type stars at sub-SMC metallicity
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2021-04-01T11:11:12Z/2021-04-05T04:36:26Z
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, Roman-Duval, 2021, 'ULLYSES Monitoring Observations of the T Tauri Star TW Hya: First Epoch', 1.0, European Space Agency, https://doi.org/10.57780/esa-o1yh3kl