A Hubble Space Telescope Survey of H2 Emission in the Circumstellar Environments of Young Stars
Constraints to the magnetospheric properties of T Tauri stars - II. The Mg II ultraviolet feature
Direct Measurement of Interstellar Extinction toward Young Stars Using Atomic Hydrogen Lya Absorption
Empirically Estimated Far-UV Extinction Curves for Classical T Tauri Stars
High-resolution Ultraviolet Radiation Fields of Classical T Tauri Stars
Hot Gas Lines in T Tauri Stars
Lya Dominance of the Classical T Tauri Far-ultraviolet Radiation Field
Probing Protoplanetary Disk Winds with C II Absorption
Probing UV-sensitive Pathways for CN and HCN Formation in Protoplanetary Disks with the Hubble Space Telescope
Signatures of Hot Molecular Hydrogen Absorption from Protoplanetary Disks. I. Non-thermal Populations
SuperBoRG: Exploration of Point Sources at z ~ 8 in HST Parallel Fields
SuperBoRG: Search for the Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
The 1600 A Emission Bump in Protoplanetary Disks: A Spectral Signature of H2O Dissociation
The Evolution of Inner Disk Gas in Transition Disks
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
Instrument
COS, COS/FUV, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-07-20T06:53:29Z/2012-02-28T21:08:40Z
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, Green comma James Carswell, 2013, 'COS-GTO: Accretion Flows and Winds of Pre-Main Sequence Stars Part 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-k089wip