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Michael Albrow

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Associate Professor

University of Canterbury

New Zealand

Research Interests

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About

Michael Albrow is an Associate Professor at the University of Canterbury in New Zealand. His research areas focus on microlensing events and exoplanet detection, as highlighted in his recent articles including "Another Binary-lens Binary-source Microlensing Event" and "Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits." Additionally, he explores advanced imaging techniques and the frequency of binaries in young open clusters through various innovative methodologies.

Recent Grants

Grant: Open

Shedding light on the dark components of the Galaxy.

Open Date: 2026-01-01

Close Date: 2029-01-01

Grant: Close

Counting the number and distribution of planets in the Galaxy.

Open Date: 2017-01-01

Close Date: 2020-01-01

Articles (42)

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Collaborators (24)

Weicheng Zang

Assistant Professor

Westlake University

CHINA

Michael Albrow

Research Interests

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About

Recent Grants

Articles (42)

Predictions of the Nancy Grace Roman Space Telescope Galactic Exoplanet Survey. IV. Lens Mass and Distance Measurements

A free-floating-planet microlensing event caused by a Saturn-mass object

Two Low Mass-ratio Microlensing Planets and Two Types of Central-resonant Degeneracy

A comprehensive analysis of three microlensing planet candidates with the planet/binary degeneracy

Mass Production of 2023 KMTNet Microlensing Planets. III. Three Planets from the Subprime Field

Predictions of the Nancy Grace Roman Space Telescope Galactic Exoplanet Survey

Four Cold Giant Planets Discovered by High-cadence Microlensing Surveys

Four-body Gravitational Microlensing Events Involving Both a Binary Lens and a Binary Source

Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023–2025 Observing Seasons

Mass Production of 2023 KMTNet Microlensing Planets. I. Low Mass Ratio

KMT-2024-BLG-3237: Another Free-floating Planet Candidate with Angular Einstein Radius Measurement

Towards sub-milliarcsecond astrometric precision using high-cadence seeing-limited imaging

KMT-2022-BLG-0086: Another Binary-lens Binary-source Microlensing Event

Dazzle: Oversampled Image Reconstruction and Difference-imaging Photometry for the Nancy Grace Roman Space Telescope

Four Planets Found through Microlensing Events Involving Faint Source Stars

Systematic Search for FFPs in KMTNet Full-frame Images. I. Photometry Pipeline

Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits

Analyses of anomalous lensing events detected from the UKIRT microlensing survey

LensNet: Enhancing Real-time Microlensing Event Discovery with Recurrent Neural Networks in the Korea Microlensing Telescope Network

MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals

Six microlensing planets detected via sub-day signals during the 2023–2024 season

Systematic KMTNet Planetary Anomaly Search. XII. Complete Sample of 2017 Subprime Field Planets

Four microlensing giant planets detected through signals produced by minor-image perturbations

KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host

Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Subprime Field Planets

OGLE-2023-BLG-0836L: The sixth microlensing planet in a binary stellar system

OGLE-2017-BLG-0448Lb: A Low Mass–Ratio Wide-orbit Microlensing Planet?

Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets

Three sub-Jovian-mass microlensing planets: MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb

The frequency and mass-ratio distribution of binaries in clusters II: radial segregation in the nearby dissolving open clusters Hyades and Praesepe

The frequency and mass-ratio distribution of binaries in clusters – III. Probabilistic generative modelling of six young open clusters

Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-field Planets

Systematic KMTNet Planetary Anomaly Search. VIII. Complete Sample of 2019 Subprime Field Planets

KMT-2022-BLG-0440Lb: A new q &lt; 10−4 microlensing planet with the central-resonant caustic degeneracy broken

Mass Production of 2021 KMTNet Microlensing Planets II

Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10−4 Planets from the First 4 yr Survey

Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets

OGLE-2019-BLG-1180Lb: Discovery of a Wide-orbit Jupiter-mass Planet around a Late-type Star

Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets

Mass Production of 2021 KMTNet Microlensing Planets. I

KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: two microlensing planets in the KMTNet high-cadence fields with followup observations

OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system?

Collaborators (24)

Weicheng Zang

Natasha Abrams

Jan Skowron

Nicholas Rattenbury

Paolo Rota

Subo Dong

Chung-Uk Lee

Pawel Zielinski

Ian Bond

Hongjing Yang

Wei Zhu

Macy Huston

Milena Ratajczak

Shude Mao

Jennifer Yee

Thomas Bensby

Szymon Kozlowski

Martin Dominik

Lukasz Wyrzykowski

Giovanni Covone

Mariusz Gromadzki

Eamonn Kerins

Igor Soszyński

Yuki Satoh

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KMT-2022-BLG-0440Lb: A new q < 10−4 microlensing planet with the central-resonant caustic degeneracy broken