COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
Probing the physicochemical properties of the Leo Ring and the Leo I group
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
Unraveling the Mysteries of the Leo Ring: An Absorption Line Study of an Unusual Gas Cloud
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2011-05-30T05:34:04Z/2011-07-02T12:52:10Z
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, Rosenberg, 2013, 'Unravelling the Mysteries of the Leo Ring: An Absorption Line Study of an Unusual Gas Cloud', 1.0, European Space Agency, https://doi.org/10.5270/esa-13hwv4n
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.