AMUSE-Field. II. Nucleation of Early-type Galaxies in the Field versus Cluster Environment
A trail of the invisible: blue globular clusters trace the radial density distribution of the dark matter - case study of NGC 4278
Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe
Filling the gap: a new class of old star cluster.
Long term optical variability of bright X-ray point sources in elliptical galaxies
Low-mass X-Ray Binaries and Globular Clusters Streamers and Arcs in NGC 4278
Recoiling Supermassive Black Holes: A Search in the Nearby Universe
The impact of satellite trails on Hubble Space Telescope observations
The SLUGGS survey: calcium triplet-based spectroscopic metallicities for over 900 globular clusters
The SLUGGS Survey: kinematics for over 2500 globular clusters in 12 early-type galaxies
The SLUGGS Survey: wide field imaging of the globular cluster system of NGC 4278
X-ray and multiwavelength view of NGC 4278. A LINER-Seyfert connection?
Instrument
ACS, ACS/WFC
Temporal Coverage
2006-12-20T09:59:58Z/2007-01-05T21:40:40Z
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, Sivakoff et al., 2008, 'Probing The Globular Cluster / Low Mass X-ray Binary Connection in Early-type Galaxies At Low X-ray Luminosities', 1.0, European Space Agency, https://doi.org/10.5270/esa-r2az23m
