Compact Optical Counterparts of Ultraluminous X-Ray Sources
Distance to the galaxy IC 342
Luminous and Variable Stars in NGC 2403 and M81
New Hubble Space Telescope imaging of the counterparts to six ultraluminous X-ray sources
Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
Optical Counterparts of ULXs and Their Host Environments in NGC 4490/4485
Roche-lobe Overflow Systems Powered by Black Holes in Young Star Clusters: The Importance of Dynamical Exchanges
The ACS Nearby Galaxy Survey Treasury
The ACS Nearby Galaxy Survey Treasury. XI. The Remarkably Undisturbed NGC 2403 Disk
The Ages of High-mass X-Ray Binaries in NGC 2403 and NGC 300
The Chandra Local Volume Survey. I. The X-Ray Point Source Populations of NGC 55, NGC 2403, and NGC 4214
The impact of satellite trails on Hubble Space Telescope observations
The Spitzer Local Volume Legacy: Survey Description and Infrared Photometry
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2005-09-02T01:06:59Z/2006-02-25T19:54:36Z
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, Roberts comma Timothy Paul, 2007, 'ULX counterparts: the key to finding intermediate-mass black holes', 1.0, European Space Agency, https://doi.org/10.5270/esa-ti1dut2