A Correlation between Galaxy Morphology and Mg II Halo Absorption Strength
A Lyman limit system associated with galactic winds
Empirical constraints of supergalactic winds at z 0.5
Halo Gas and Galaxy Disk Kinematics Derived from Observations and LCDM Simulations of Mg II Absorption-selected Galaxies at Intermediate Redshift
Ha Spectroscopy of Galaxies at z > 2: Kinematics and Star Formation
Infrared Emission-Line Galaxies Associated with Dampened Ly alpha and Strong Metal Absorber Redshifts
MAGIICAT VI. The Mg II Intragroup Medium Is Kinematically Complex
Morphological properties of z~ 0.5 absorption-selected galaxies: the role of galaxy inclination
MUSE-ALMA haloes VI: coupling atomic, ionized, and molecular gas kinematics of galaxies
MUSE-ALMA haloes VII: survey science goals & design, data processing and final catalogues
MUSE-ALMA haloes V: physical properties and environment of z <= 1.4 H I quasar absorbers
MUSE-ALMA Haloes XI: gas flows in the circumgalactic medium
MUSE-ALMA Haloes X: the stellar masses of gas-rich absorbing galaxies
Observational signatures of a warped disk associated with cold-flow accretion
Si and Mn Abundances in Damped Lya Systems with Low Dust Content
SINS/zC-SINF Survey of z ~ 2 Galaxy Kinematics: Rest-frame Morphology, Structure, and Colors from Near-infrared Hubble Space Telescope Imaging
The Azimuthal Dependence of Outflows and Accretion Detected Using O VI Absorption
The Highly Ionized Circumgalactic Medium is Kinematically Uniform around Galaxies
The morphological, kinematic, and halo gas properties of magnesium II absorption selected galaxies at intermediate redshift
The VLT SINFONI Mg II Program for Line Emitters (SIMPLE). II. Background Quasars Probing Z ~ 1 Galactic Winds
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
1996-05-09T19:51:16Z/1999-04-26T16:53:53Z
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, Steidel comma Charles C., 2000, 'WFPC2 Imaging of Intermediate Redshift Absorption-Selected Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-grp2fyc