Accurate photometric light curves of the lensed components of Q2237+0305 derived with an optimal image subtraction technique: Evidence for microlensing in image A
A Chandra High Resolution Camera Observation of X-Ray Point Sources in M31
Ages of M33 Star Clusters Based on the Hubble Space Telescope/WFPC2 Photometry
AGN feedback and multiphase gas in giant elliptical galaxies
An updated survey of globular clusters in M 31. I. Classification and radial velocity for 76 candidate clusters
A Possible Detection of M31* with Chandra
Assessing Formation Scenarios for the Double Nucleus of M31 Using Two-Dimensional Image Decomposition
A Wide-Field Survey of the Globular Cluster Systems of Elliptical and Spiral Galaxies
Calibration of the Surface Brightness Fluctuation Method for use with the Hubble Space Telescope.
Counting the Unseen. I. Nuclear Density Scaling Relations for Nucleated Galaxies
Detailed Structural Decomposition of Galaxy Images
Do Nuclear Star Clusters and Supermassive Black Holes Follow the Same Host-Galaxy Correlations?
Dynamical modeling of the stellar nucleus of M 31
Eccentric-Disk Models for the Nucleus of M31
Global properties of ordinary early-type galaxies: photometry and spectroscopy of stars and globular clusters in NGC 4494
High Spatial Resolution Near-Infrared Imaging of the Central Regions of M31
HST STIS Spectroscopy of the Triple Nucleus of M31: Two Nested Disks in Keplerian Rotation around a Supermassive Black Hole
Kinematics of Star Clusters in M33: Distinct Populations
M31 Globular Clusters in the Hubble Space Telescope Archive. I. Cluster Detection and Completeness
M31 Globular Clusters in the Hubble Space Telescope Archive. II. Structural Parameters
M31s Undisturbed Thin Disk of Globular Clusters
M32 +/- 1
M33: A Galaxy with No Supermassive Black Hole
Nearby Early-type Galactic Nuclei at High Resolution: Dynamical Black Hole and Nuclear Star Cluster Mass Measurements
New Insights from HST Studies of Globular Cluster Systems. I. Colors, Distances, and Specific Frequencies of 28 Elliptical Galaxies
Nonlinear Color-Metallicity Relations of Globular Clusters. IX. Different Radial Number Density Profiles between Blue and Red Clusters
On the Nuclear Rotation Curve of M31
On the Size Difference between Red and Blue Globular Clusters
Properties of Globular Cluster Systems in Nearby Early-Type Galaxies
Resolved Nuclear Kinematics Link the Formation and Growth of Nuclear Star Clusters with the Evolution of Their Early- and Late-type Hosts
SBF distances to Leo and Virgo using the HST
Self-Gravitating Eccentric Disk Models for the Double Nucleus of M31
Sizing up Partially Depleted Galaxy Cores
Star clusters in M 33. IV. A new survey from deep HST images
Stellar populations and surface brightness fluctuations: new observations and models
Supersoft X-Ray Sources in M31. I. A Chandra Survey and an Extension to Quasi-soft Sources
The Age Difference between the Globular Cluster Subpopulations in NGC 4472
The Centers of Early-Type Galaxies with HST. IV. Central Parameter Relations.
The Centers of Early-Type Galaxies with Hubble Space Telescope. V. New WFPC2 Photometry
The Central Gas Systems of Early-Type Galaxies Traced by Dust Features, Based on the Hubble Space Telescope WFPC2 Archival Images
The Cluster of Blue Stars Surrounding the M31 Nuclear Black Hole
The Double Nucleus and Central Black Hole of M31
The Fundamental Plane and the evolution of the M/L ratio of early-type field galaxies up to z~ 1
The Fundamental Plane of Gravitational Lens Galaxies and The Evolution of Early-Type Galaxies in Low-Density Environments
The Globular Cluster System in the Inner Region of the Giant Elliptical Galaxy NGC 4472
The Globular Cluster System in the Outer Regions of NGC 4472
The Low-Mass X-Ray Binary-Globular Cluster Connection. II. NGC 4472 X-Ray Source Properties and Source Catalogs
The Low-Mass X-Ray Binary-Globular Cluster Connection in NGC 4472
The M 31 double nucleus probed with OASIS. A natural vec m = 1 mode?
The M31 Globular Cluster Luminosity Function
The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes
The Optical Gravitational Lensing Experiment Monitoring of QSO 2237+0305
The Structure of the Virgo Cluster from Surface Brightness Fluctuations in Hubble Space Telescope Images
Three-dimensional Keplerian orbit-superposition models of the nucleus of M31
WFPC2 Observations of Compact Star Cluster Nuclei in Low-Luminosity Spiral Galaxies
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-12-26T12:16:16Z/1995-06-23T23:41:37Z
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, Westphal et al., 1996, 'NUCLEI OF NEARLY NORMAL GALAXIES (WC12): CYCLE 4 REVISED', 1.0, European Space Agency, https://doi.org/10.5270/esa-4cbszmg
