A Deep Hubble Space Telescope and Keck Search for Definitive Identification of Lyman Continuum Emitters at z~3.1
An enhanced merger fraction within the galaxy population of the SSA22 protocluster at z = 3.1
A Refined Estimate of the Ionizing Emissivity from Galaxies at z ~= 3: Spectroscopic Follow-up in the SSA22a Field
Detections of Lyman Continuum from Star-Forming Galaxies at z ~ 3 through Subaru/Suprime-Cam Narrow-Band Imaging
Expanding the Search for Galaxies at z ~ 7-10 with New NICMOS Parallel Fields
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Molecular gas in submillimetre-faint, star-forming ultraluminous galaxies at z > 1
Narrowband Imaging of Escaping Lyman-continuum Emission in the SSA22 Field
Searching for candidates of Lyman continuum sources - revisiting the SSA22 field
Spitzer Identifications and Classifications of Submillimeter Galaxies in Giant, High-Redshift, Lya-Emission-Line Nebulae
The Chandra Deep Protocluster Survey: Lya Blobs are Powered by Heating, Not Cooling
The impact of satellite trails on Hubble Space Telescope observations
The KMOS Deep Survey (KDS) - I. Dynamical measurements of typical star-forming galaxies at z 3.5
Instrument
ACS, ACS/WFC, NICMOS, NICMOS/NIC3
Temporal Coverage
2005-08-04T08:54:47Z/2005-08-17T20:06:12Z
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, Chapman comma Scott C., 2006, 'Probing the establishment of galaxy morphologies in the best-studied high-redshift structure', 1.0, European Space Agency, https://doi.org/10.5270/esa-5fq92o9