A 9 Month Hubble Space Telescope Near-UV Survey of M87. I. Light and Color Curves of 94 Novae, and a Redetermination of the Nova Rate
A Displaced Supermassive Black Hole in M87
Age and metallicity gradients support hierarchical formation for M87
A Hubble Space Telescope survey for novae in M87 - III. Are novae good standard candles 15 d after maximum brightness?
A Hubble Space Telescope Survey for Novae in M87. II. Snuffing out the Maximum Magnitude-Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae
A Hubble Space Telescope Survey for Novae in M87. I. Light and Color Curves, Spatial Distributions, and the Nova Rate
A Hubble Space Telescope Survey for Novae in the Globular Clusters of M87
Color Bimodality in M87 Globular Clusters
Discovery of C IV Emission Filaments in M87
Globular cluster scale sizes in giant galaxies: orbital anisotropy and tidally underfilling clusters in M87, NGC 1399 and NGC 5128
Globular Cluster Scale Sizes in Giant Galaxies: The Case of M87 and the Role of Orbital Anisotropy and Tidal Filling
High resolution analysis of extragalactic globular clusters
How ^ated is the dynamical-to-stellar mass ratio of the ultracompact dwarf S999?
Keck Cosmic Web Imager (KCWI) spectra of globular clusters and ultracompact dwarfs in the halo of M87
Long term optical variability of bright X-ray point sources in elliptical galaxies
Measuring Star Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams. II. Applications to Nearby Elliptical Galaxies
Observational Biases Masquerading as Cosmological Effects? a Cautionary tale about Blue Tilts and Other Trends in Globular Cluster Systems
Recoiling Supermassive Black Holes: A Search in the Nearby Universe
Structural Parameters of the Messier 87 Globular Clusters
The Color-Magnitude Relation for Metal-Poor Globular Clusters in M87: Confirmation from Deep HST/ACS Imaging
The connection between radio loudness and central surface brightness profiles in optically selected low-luminosity active galaxies
The impact of satellite trails on Hubble Space Telescope observations
The inner halo of M 87: a first direct view of the red-giant population
The innermost globular clusters of M87
The Most Massive Galaxies with Large Depleted Cores: Structural Parameter Relations and Black Hole Masses
The Observational and Theoretical Tidal Radii of Globular Clusters in M87
The Size Difference between Red and Blue Globular Clusters is not due to Projection Effects
Ubiquitous time variability of integrated stellar populations
UV Insights into the Complex Populations of M87 Globular Clusters
Instrument
ACS, ACS/WFC, WFPC2, WFPC2/PC
Temporal Coverage
2005-12-24T01:22:13Z/2006-03-05T11:07:51Z
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, Baltz comma Edward A., 2007, 'Microlensing in M87 and the Virgo Cluster', 1.0, European Space Agency, https://doi.org/10.5270/esa-fn74n21