A minor merger scenario for the ultraluminous X-ray source ESO 243-49 HLX-1 - II. Constraints from photometry
A population of luminous accreting black holes with hidden mergers
A Young Massive Stellar Population around the Intermediate-mass Black Hole ESO 243-49 HLX-1
Combined analysis of Hubble and VLT photometry of the intermediate mass black hole ESO 243-49 HLX-1
Kinematics of the Intermediate-mass Black Hole Candidate HLX-1
Optical counterpart of HLX-1 during the 2010 outburst
Outbursts of the intermediate-mass black hole HLX-1: a wind-instability scenario
The accretion disc, jets and environment of the intermediate mass black hole candidate ESO 243-49 HLX-1
The impact of satellite trails on Hubble Space Telescope observations
Understanding the environment around the intermediate mass black hole candidate ESO 243-49 HLX-1
X-ray emission from galaxies - Shedding light on the nature of ESO 243-49 HLX-1
Instrument
ACS, ACS/SBC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-09-13T06:16:06Z/2010-09-23T17:19:22Z
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, Farrell et al., 2011, 'The Ultraviolet and Optical Counterparts of the Intermediate Mass Black Hole Candidate ESO 243-49 HLX-1', 1.0, European Space Agency, https://doi.org/10.5270/esa-wtdu54g