An Excess of Submillimeter Sources near 4C 41.17: A Candidate Protocluster at Z = 3.8?
A Star-forming Shock Front in Radio Galaxy 4C+41.17 Resolved with Laser-assisted Adaptive Optics Spectroscopy
Disentangling star formation and AGN activity in powerful infrared luminous radio galaxies at 1 < z < 4
Giant Lya Nebulae Associated with High-Redshift Radio Galaxies
The morphology of extremely red objects
VLBI imaging of high-redshift galaxies and protoclusters at low radio frequencies with the International LOFAR Telescope
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-10-30T11:03:17Z/1994-11-06T15:43:17Z
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, van Breugel comma Wil J.M., 1996, 'DETAILED STUDY OF 4C41.17, THE MOST DISTANT GALAXY CYCLE 4, MEDIUM. -- PART I: EARLY ACQUISITION IMAGING.', 1.0, European Space Agency, https://doi.org/10.5270/esa-kua85ek