DIISC-III. Signatures of Stellar Disk Growth in Nearby Galaxies
DIISC-II: Unveiling the Connections between Star Formation and Interstellar Medium in the Extended Ultraviolet Disk of NGC 3344
DIISC-I: The Discovery of Kinematically Anomalous H I Clouds in M 100
Evidence for a Rotational Component in the Circumgalactic Medium of Nearby Galaxies
Probing Large Galaxy Halos at Z ~ 0 with Automated Lya-absorption Matching
Probing the physicochemical properties of the Leo Ring and the Leo I group
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2015-11-23T17:49:12Z/2016-11-04T02:55:28Z
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, Borthakur comma Sanchayeeta, 2016, 'How are HI Disks Fed? Probing Condensation at the Disk-Halo Interface', 1.0, European Space Agency, https://doi.org/10.5270/esa-xqk9tac