A late-time view of the progenitors of five Type IIP supernovae
A New Sample of Transient Ultraluminous X-Ray Sources Serendipitously Discovered by Swift/XRT
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Redetermination of the Hubble Constant
Chromodynamical analysis of lenticular galaxies using globular clusters and planetary nebulae
Discovery, photometry, and astrometry of 49 classical nova candidates in M 81 galaxy
Hubble Space Telescope imaging of the progenitor sites of six nearby core-collapse supernovae
Kinematics and host-galaxy properties suggest a nuclear origin for calcium-rich supernova progenitors
Long term optical variability of bright X-ray point sources in elliptical galaxies
Radially extended kinematics in the S0 galaxy NGC 2768 from planetary nebulae, globular clusters and starlight
The ATLAS3D Project - XXIII. Angular momentum and nuclear surface brightness profiles
The GHOSTS Survey. I. Hubble Space Telescope Advanced Camera for Surveys Data
The GHOSTS survey - II. The diversity of halo colour and metallicity profiles of massive disc galaxies
The impact of satellite trails on Hubble Space Telescope observations
The massive binary companion star to the progenitor of supernova 1993J
The Production Rate of SN Ia Events in Globular Clusters
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: the globular cluster systems of three early-type galaxies using wide-field imaging
The very young resolved stellar populations around stripped-envelope supernovae
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2002-05-28T06:28:15Z/2002-12-31T19:23:58Z
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, Smartt et al., 2004, 'Direct imaging of the progenitors of massive, core-collapse supernovae', 1.0, European Space Agency, https://doi.org/10.5270/esa-p9o3wud