A Gas Giant Planet in the OGLE-2006-BLG-284L Stellar Binary System
Age and metallicity gradients in the Galactic Bulge. A differential study using HST/WFPC2
Blending in gravitational microlensing experiments: source confusion and related systematics
Four microlensing planets with faint-source stars identified in the 2016 and 2017 season data
Free-floating Planet Mass Function from MOA-II 9 yr Survey toward the Galactic Bulge
Hubble Space Telescope WFPC2 Proper Motions in Two Bulge Fields: Kinematics and Stellar Population of the Galactic Bulge
KMT-2018-BLG-1743: planetary microlensing event occurring on two source stars
KMT-2019-BLG-0797: Binary-lensing event occurring on a binary stellar system
KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal
KMT-2022-BLG-0440Lb: A new q < 10-4 microlensing planet with the central-resonant caustic degeneracy broken
KMT-2023-BLG-0416, KMT-2023-BLG-1454, KMT-2023-BLG-1642: Microlensing planets identified from partially covered signals
Mass Production of 2021 KMTNet Microlensing Planets. I
Microlensing Optical Depth toward the Galactic Bulge from Microlensing Observations in Astrophysics Group Observations during 2000 with Difference Image Analysis
MOA-bin-29b: A Microlensing Gas-giant Planet Orbiting a Low-mass Host Star
New giant planet beyond the snow line for an extended MOA exoplanet microlens sample
Observational Evidence for the Effect of Amplification Bias in Gravitational Microlensing Experiments
OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions
OGLE-2015-BLG-1649Lb: A Gas Giant Planet around a Low-mass Dwarf
OGLE-2015-BLG-1670Lb: A Cold Neptune beyond the Snow Line in the Provisional WFIRST Microlensing Survey Field
OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?
OGLE-2017-BLG-0448Lb: A Low Mass-Ratio Wide-orbit Microlensing Planet?
OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf
OGLE-2019-BLG-0825: Constraints on the Source System and Effect on Binary-lens Parameters Arising from a Five-day Xallarap Effect in a Candidate Planetary Microlensing Event
OGLE-2019-BLG-1180Lb: Discovery of a Wide-orbit Jupiter-mass Planet around a Late-type Star
OGLE-2023-BLG-0836L: The sixth microlensing planet in a binary stellar system
Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605
Systematic KMTNet planetary anomaly search. V. Complete sample of 2018 prime-field
Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10-4 Planets from the First 4 yr Survey
Systematic Korea Microlensing Telescope Network planetary anomaly search - III. One wide-orbit planet and two stellar binaries
Terrestrial- and Neptune-mass Free-Floating Planet Candidates from the MOA-II 9 yr Galactic Bulge Survey
The 2L1S/1L2S Degeneracy for Two Microlensing Planet Candidates Discovered by the KMTNet Survey in 2017
The Luminosity Function and Initial Mass Function in the Galactic Bulge
The MACHO Project: Microlensing Optical Depth toward the Galactic Bulge from Difference Image Analysis
Three faint-source microlensing planets detected via the resonant-caustic channel
Three sub-Jovian-mass microlensing planets: MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-08-12T19:12:16Z/1994-08-13T01:53:56Z
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, Westphal comma J. A., 1995, 'STELLAR POPULATION IN THE GALACTIC BULGE (WC02): CYCLE 4', 1.0, European Space Agency, https://doi.org/10.5270/esa-vke27a3
