A Chandra X-Ray Study of NGC 1068. I. Observations of Extended Emission
A Comparison between the Narrow-Line Regions of Seyfert 1 and Seyfert 2 Galaxies
Biconical Radiation Field and Outflow in NGC 1068: Location of the Hidden Nucleus
Bi-Dimensional Spectrography at HST-Like Spatial Resolution: OIII Kinematics and Ionization in the NLR of NGC 1068
High-Resolution Mid-Infrared Imaging and Astrometry of the Nucleus of the Seyfert Galaxy NGC 1068
HST Imaging of the Inner 3 Arcseconds of NGC 1068 in the Light of O iii lambda 5007
Near-infrared adaptive optics dissection of the core of NGC 1068 with NAOS-CONICA
NGC 1068: Resolution of Nuclear Structure in the Optical Continuum
On the nature of the near-UV extended light in Seyfert galaxies
Seeing the Nuclei of Active Galaxies
The Location of the Nucleus of NGC 1068 from HST Imaging Polarimetry and Absolute Astrometry
The Nuclear Region of NGC 1068: High-Accuracy Alignment of the Optical and Radio Emission
The Subarcsecond Radio Structure in NGC 1068. II. Implications for the Central Engine and Unifying Schemes
Instrument
WFPC/PC
Temporal Coverage
1990-08-26T15:47:14Z/1990-08-26T16:14:14Z
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, Ford comma Holland, 1990, 'IMAGING AND SPECTROPHOTOMETRY OF NGC1068', 1.0, European Space Agency, https://doi.org/10.5270/esa-ik1iooc