K-Band Red Clump Distance to the Large Magellanic Cloud
MACHO 96-LMC-2: Lensing of a Binary Source in the Large Magellanic Cloud and Constraints on the Lensing Object
Photometric Confirmation of MACHO Large Magellanic Cloud Microlensing Events
Properties of RR Lyrae stars in the inner regions of the Large Magellanic Cloud
Resolution of the MACHO-LMC-5 Puzzle: The Jerk-Parallax Microlens Degeneracy
Resolving the Nature of the Large Magellanic Cloud Microlensing Event MACHO-LMC-5
Spitzer Space Telescope Observations of the Aftermath of Microlensing Event MACHO-LMC-5
The MACHO Project Hubble Space Telescope Follow-Up: Preliminary Results on the Location of the Large Magellanic Cloud Microlensing Source Stars
The Mass of the MACHO-LMC-5 Lens Star
The origin of the LMC stellar bar: clues from the SFH of the bar and inner disc
Topics in microlensing and dark energy
Using Optical and Near-Infrared Photometry to Test MACHO Lens Candidates
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-03-12T11:08:13Z/1999-10-16T13:56:33Z
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, Cook comma Kem, 2000, 'Halo Microlens Source Systems and their Underlying Stellar Backgrounds', 1.0, European Space Agency, https://doi.org/10.5270/esa-kligetk