Ceci Nest Pas a Globular Cluster: The Metallicity Distribution of the Stellar System Terzan 5
Halo intruders in the Galactic bulge revealed by HST and Gaia: the globular clusters Terzan 10 and Djorgovski 1
High-resolution Reddening Map in the Direction of the Stellar System Terzan 5
New Density Profile and Structural Parameters of the Complex Stellar System Terzan 5
Probing the MSP Prenatal Stage: The Optical Identification of the X-Ray Burster EXO 1745-248 in Terzan 5
Proper Motions in Terzan 5: Membership of the Multi-iron Subpopulations and First Constraint on the Orbit
Relative Ages of Nine Inner Milky Way Globular Clusters from Proper-motion-cleaned Color-Magnitude Diagrams
Structure and Internal Kinematics of Nine Inner Milky Way Globular Clusters
The Age of the Young Bulge-like Population in the Stellar System Terzan 5: Linking the Galactic Bulge to the High-z Universe
The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge
The globular cluster NGC 6642: evidence for a depleted mass function
The globular cluster NGC 6642: evidence for a depleted mass function in a very old cluster
The impact of satellite trails on Hubble Space Telescope observations
The MAVERIC Survey: A Transitional Millisecond Pulsar Candidate in Terzan 5
The near-IR counterpart of IGR J17480-2446 in Terzan 5
Uncloaking Globular Clusters in the Inner Galaxy
Using Long-term Millisecond Pulsar Timing to Obtain Physical Characteristics of the Bulge Globular Cluster Terzan 5
Instrument
ACS, ACS/WFC
Temporal Coverage
2003-07-21T13:58:20Z/2004-03-01T20:08:20Z
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, Rich comma R. Michael, 2004, 'A Snapshot Survey of Galactic Bulge Globular Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-5z1qgn6