Direct detection of quasar feedback via the Sunyaev-Zeldovich effect
H2 molecular gas absorption-selected systems trace CO molecular gas-rich galaxy overdensities
Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
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
Quasar Sightline and Galaxy Evolution (QSAGE) - III. The mass-metallicity and fundamental metallicity relation of z 2.2 galaxies
Quasar Sightline and Galaxy Evolution (QSAGE) survey - II. Galaxy overdensities around UV luminous quasars at z = 1-2
Quasar Sightline and Galaxy Evolution (QSAGE) survey - I. The galaxy environment of O VI absorbers up to z = 1.4 around PKS 0232-04
The Galaxy Environment of Extremely Massive Quasars. I. An Overdensity of Ha Emitters at z = 1.47
Instrument
WFC3, WFC3/IR
Temporal Coverage
2016-09-28T18:29:04Z/2017-08-06T22:24:58Z
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, Bielby comma Rich, 2017, 'QSAGE: QSO Sightline And Galaxy Evolution', 1.0, European Space Agency, https://doi.org/10.5270/esa-b3750gj