Concordance between Observations and Simulations in the Evolution of the Mass Relation between Supermassive Black Holes and Their Host Galaxies
Concurrent Starbursts in Molecular Gas Disks within a Pair of Colliding Galaxies at z = 1.52
From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ~ 1.5
Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
Opening the Era of Quasar-host Studies at High Redshift with JWST
Testing the Fidelity of Simulations of Black Hole-Galaxy Coevolution at z ~ 1.5 with Observations
The Mass Relations between Supermassive Black Holes and Their Host Galaxies at 1 < z < 2 HST-WFC3
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
Where Do Quasar Hosts Lie with Respect to the Size-Mass Relation of Galaxies?
Instrument
WFC3/IR
Temporal Coverage
2017-10-23T02:13:05Z/2019-03-16T21:49:29Z
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, Silverman comma John David, 2019, 'Emergence of the supermassive black hole - galaxy mass relations at z > 1', 1.0, European Space Agency, https://doi.org/10.5270/esa-n5md1xf
