A multi-wavelength test of the FR I-BL Lac unifying model
A NICMOS Survey of Early-Type Galaxy Centers: The Relation Between Core Properties, Gas and Dust Content, and Environment
Central Structural Parameters of Early-Type Galaxies as Viewed with Nicmos on the Hubble Space Telescope
Correlations between Supermassive Black Holes, Velocity Dispersions, and Mass Deficits in Elliptical Galaxies with Cores
Hubble Space Telescope Near-infrared Snapshot Survey of 3CR Radio Source Counterparts. II. An Atlas and Inventory of the Host Galaxies, Mergers, and Companions
Hubble Space Telescope Near-infrared Snapshot Survey of 3CR Radio Source Counterparts. III. Radio Galaxies and Quasars in Context
Hydrostatic Gas Constraints on Supermassive Black Hole Masses: Implications for Hydrostatic Equilibrium and Dynamical Modeling in a Sample of Early-type Galaxies
Infrared Surface Brightness Fluctuations of Magellanic Star Clusters
M84: A Warp Caused by Jet-induced Pressure Gradients?
Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations
Molecular gas and nuclear activity in early-type galaxies: any link with radio loudness?
Radio AGN in the local universe: unification, triggering and evolution
Recoiling Supermassive Black Holes: A Search in the Nearby Universe
Revisiting the dichotomy of early-type galaxies
Spectral energy distributions of five FR I radio galaxies
Spectral energy distributions of FR I nuclei and the FR I/BL Lac unifying model
Structure and Formation of Elliptical and Spheroidal Galaxies
The 1.6 mm Near-infrared Nuclei of 3C Radio Galaxies: Jets, Thermal Emission, or Scattered Light?
The connection between radio loudness and central surface brightness profiles in optically selected low-luminosity active galaxies
The host galaxy/AGN connection in nearby early-type galaxies. Sample selection and hosts brightness profiles
The Ionization Source in the Nucleus of M84
The Supermassive Black Hole in M84 Revisited
Virial models and anisotropy of velocity dispersion in E-galaxies
What Do the Hubble Space Telescope and Chandra Tell Us about the Jet and the Nuclear Region of the Radio Galaxy 3C 270?
Instrument
NICMOS, NICMOS/NIC1, NICMOS/NIC2, NICMOS/NIC3
Temporal Coverage
1998-04-23T12:25:15Z/1998-07-13T04:08:44Z
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, Quillen comma Alice, 1999, 'Near-IR Cores of Radio Galaxies, Are the AGN's Moving in the Galaxy?', 1.0, European Space Agency, https://doi.org/10.5270/esa-qrm3msk