Sang-Mok Cha
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View article: A Comprehensive Analysis of Three Microlensing Planet Candidates with the Planet/Binary Degeneracy
A Comprehensive Analysis of Three Microlensing Planet Candidates with the Planet/Binary Degeneracy Open
We present observations and analyses of three high-magnification microlensing events: KMT-2022-BLG-0954, KMT-2024-BLG-0697, and MOA-2024-BLG-018. All three exhibit the “Planet/Binary” degeneracy, with planetary solutions corresponding to m…
View article: Six microlensing planets detected via sub-day signals during the 2023 -- 2024 season
Six microlensing planets detected via sub-day signals during the 2023 -- 2024 season Open
We present analyses of six microlensing events: KMT-2023-BLG-0548, KMT-2023-BLG-0830, KMT-2023-BLG-0949, KMT-2024-BLG-1281, KMT-2024-BLG-2059, and KMT-2024-BLG-2242. These were identified in KMTNet data from the 2023 -- 2024 seasons, selec…
View article: KMT-2022-BLG-0086: Another Binary-lens Binary-source Microlensing Event
KMT-2022-BLG-0086: Another Binary-lens Binary-source Microlensing Event Open
We present the analysis of a microlensing event KMT-2022-BLG-0086 of which the overall light curve is not described by a binary-lens single-source (2L1S) model, which suggests the existence of an extra lens or an extra source. We found tha…
View article: HST pre-imaging of a free-floating planet candidate microlensing event
HST pre-imaging of a free-floating planet candidate microlensing event Open
High-cadence microlensing observations uncovered a population of very short-timescale microlensing events, which are believed to be caused by the population of free-floating planets (FFP) roaming the Milky Way. Unfortunately, the light cur…
View article: KMT-2022-BLG-0086: Another binary-lens binary-source microlensing event
KMT-2022-BLG-0086: Another binary-lens binary-source microlensing event Open
We present the analysis of a microlensing event KMT-2022-BLG-0086 of which the overall light curve is not described by a binary-lens single-source (2L1S) model, which suggests the existence of an extra lens or an extra source. We found tha…
View article: MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals
MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals Open
Aims . The light curves of the microlensing events MOA-2022-BLG-091 and KMT-2024-BLG-1209 exhibit anomalies with very similar features. These anomalies appear near the peaks of the light curves, where the magnifications are moderately high…
View article: MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals
MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals Open
The light curves of the microlensing events MOA-2022-BLG-091 and KMT-2024-BLG-1209 exhibit anomalies with very similar features. These anomalies appear near the peaks of the light curves, where the magnifications are moderately high, and a…
View article: Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source Events
Systematic Reanalysis of KMTNet Microlensing Events. II. Two New Planets in Giant-source Events Open
In this work, we continue to apply the updated KMTNet tender-love care photometric pipeline to historical microlensing events. We apply the pipeline to a subsample of events from the KMTNet database, which we refer to as the giant source s…
View article: Four Planets Found through Microlensing Events Involving Faint Source Stars
Four Planets Found through Microlensing Events Involving Faint Source Stars Open
To conduct a comprehensive demographic study of microlensing planets, it is essential to detect all planetary signals that exceed a predefined threshold through a detailed analysis of survey data. We reanalyzed previous data from the Korea…
View article: Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits
Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits Open
Exoplanets classified as super-Earths are commonly observed on short-period orbits, close to their host stars, but their abundance on wider orbits is poorly constrained. Gravitational microlensing is sensitive to exoplanets on wide orbits.…
View article: KMTNet View of Blue Large-amplitude Pulsators Toward the Galactic Bulge. I. Discovery of Wide-orbit Companions in OGLE-BLAP-006
KMTNet View of Blue Large-amplitude Pulsators Toward the Galactic Bulge. I. Discovery of Wide-orbit Companions in OGLE-BLAP-006 Open
Blue large-amplitude pulsators (BLAPs), a recently classified type of variable stars, are evolved objects likely formed through interactions between stars in a binary system. However, only two BLAPs with stellar companions have been discov…
View article: Analyses of anomalous lensing events detected from the UKIRT microlensing survey
Analyses of anomalous lensing events detected from the UKIRT microlensing survey Open
Aims. The United Kingdom Infrared Telescope (UKIRT) microlensing survey was conducted over four years, from 2016 to 2019, with the goal of serving as a precursor to future near-infrared microlensing surveys. Focusing on stars in the Galact…
View article: Analyses of anomalous lensing events detected from the UKIRT microlensing survey
Analyses of anomalous lensing events detected from the UKIRT microlensing survey Open
The United Kingdom Infrared Telescope (UKIRT) microlensing survey was conducted over four years, from 2016 to 2019, with the goal of serving as a precursor to future near-infrared microlensing surveys (Shvartzvald et al. 2017). Focusing on…
View article: <tt>LensNet</tt>: Enhancing Real-time Microlensing Event Discovery with Recurrent Neural Networks in the Korea Microlensing Telescope Network
LensNet: Enhancing Real-time Microlensing Event Discovery with Recurrent Neural Networks in the Korea Microlensing Telescope Network Open
Traditional microlensing event vetting methods require highly trained human experts, and the process is both complex and time consuming. This reliance on manual inspection often leads to inefficiencies and constrains the ability to scale f…
View article: Observations of Microlensed Images with Dual-field Interferometry: On-sky Demonstration and Prospects
Observations of Microlensed Images with Dual-field Interferometry: On-sky Demonstration and Prospects Open
Interferometric observations of gravitational microlensing events offer an opportunity for precise, efficient, and direct mass and distance measurements of lensing objects, especially those of isolated neutron stars and black holes. Howeve…
View article: MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals
MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals Open
Aims . We examined the anomalies in the light curves of the lensing events MOA-2022-BLG-033, KMT-2023-BLG-0119, and KMT- 2023-BLG-1896. These anomalies share similar traits: they occur near the peak of moderately to highly magnified events…
View article: MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals
MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals Open
We examined the anomalies in the light curves of the lensing events MOA-2022-BLG-033, KMT-2023-BLG-0119, and KMT-2023-BLG-1896. We conducted detailed modeling of the light curves to uncover the nature of the anomalies. This modeling reveal…
View article: Geninpsection: Toward Generalizable Anomaly Detection
Geninpsection: Toward Generalizable Anomaly Detection Open
View article: KMT-2021-BLG-0284, KMT-2022-BLG-2480, and KMT-2024-BLG-0412: Three microlensing events involving two lens masses and two source stars
KMT-2021-BLG-0284, KMT-2022-BLG-2480, and KMT-2024-BLG-0412: Three microlensing events involving two lens masses and two source stars Open
We carried out a project involving the systematic analysis of microlensing data from the Korea Microlensing Telescope Network survey. The aim of this project is to identify lensing events with complex anomaly features that are difficult to…
View article: Analysis of the Full Spitzer Microlensing Sample. I. Dark Remnant Candidates and Gaia Predictions
Analysis of the Full Spitzer Microlensing Sample. I. Dark Remnant Candidates and Gaia Predictions Open
In the pursuit of understanding the population of stellar remnants within the Milky Way, we analyze the sample of ∼950 microlensing events observed by the Spitzer Space Telescope between 2014 and 2019. In this study we focus on a subsample…
View article: KMT-2023-BLG-2669: Ninth Free-floating Planet Candidate with θ <sub>E</sub> Measurements
KMT-2023-BLG-2669: Ninth Free-floating Planet Candidate with θ <sub>E</sub> Measurements Open
We report a free-floating planet (FFP) candidate identified from the analysis of the microlensing event KMT-2023-BLG-2669. The lensing light curve is characterized by a short duration (≲3 days) and a small amplitude (≲0.7 mag). From the an…
View article: Microlensing brown-dwarf companions in binaries detected during the 2022 and 2023 seasons
Microlensing brown-dwarf companions in binaries detected during the 2022 and 2023 seasons Open
Aims. Building on previous works to construct a homogeneous sample of brown dwarfs in binary systems, we investigate microlensing events detected by the Korea Microlensing Telescope Network (KMTNet) survey during the 2022 and 2023 seasons.…
View article: Microlensing brown-dwarf companions in binaries detected during the 2022 and 2023 seasons
Microlensing brown-dwarf companions in binaries detected during the 2022 and 2023 seasons Open
Building on previous works to construct a homogeneous sample of brown dwarfs in binary systems, we investigate microlensing events detected by the Korea Microlensing Telescope Network (KMTNet) survey during the 2022 and 2023 seasons. Given…
View article: KMT-2021-BLG-2609Lb and KMT-2022-BLG-0303Lb: Microlensing planets identified through signals produced by major-image perturbations
KMT-2021-BLG-2609Lb and KMT-2022-BLG-0303Lb: Microlensing planets identified through signals produced by major-image perturbations Open
Aims. We investigate microlensing data collected by the Korea Microlensing Telescope Network (KMTNet) survey during the 2021 and 2022 seasons to identify planetary lensing events displaying a consistent anomalous pattern. Our investigation…
View article: Analysis of the full Spitzer microlensing sample I: Dark remnant candidates and Gaia predictions
Analysis of the full Spitzer microlensing sample I: Dark remnant candidates and Gaia predictions Open
In the pursuit of understanding the population of stellar remnants within the Milky Way, we analyze the sample of $\sim 950$ microlensing events observed by the Spitzer Space Telescope between 2014 and 2019. In this study we focus on a sub…
View article: Systematic KMTNet Planetary Anomaly Search. XII. Complete Sample of 2017 Subprime Field Planets
Systematic KMTNet Planetary Anomaly Search. XII. Complete Sample of 2017 Subprime Field Planets Open
We report the analysis of four unambiguous planets and one possible planet from the subprime fields (Γ ≤ 1 hr −1 ) of the 2017 Korea Microlensing Telescope Network (KMTNet) microlensing survey, to complete the KMTNet AnomalyFinder planetar…
View article: KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host
KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host Open
Aims. We aim to investigate the nature of the short-term anomaly that appears in the lensing light curve of KMT-2023-BLG-1866. The anomaly was only partly covered due to its short duration of less than a day, coupled with cloudy weather co…
View article: Four microlensing giant planets detected through signals produced by minor-image perturbations
Four microlensing giant planets detected through signals produced by minor-image perturbations Open
Aims. We investigated the nature of the anomalies appearing in four microlensing events KMT-2020-BLG-0757, KMT-2022-BLG-0732, KMT-2022-BLG-1787, and KMT-2022-BLG-1852. The light curves of these events commonly exhibit initial bumps followe…
View article: Four microlensing giant planets detected through signals produced by minor-image perturbations
Four microlensing giant planets detected through signals produced by minor-image perturbations Open
We investigated the nature of the anomalies appearing in four microlensing events KMT-2020-BLG-0757, KMT-2022-BLG-0732, KMT-2022-BLG-1787, and KMT-2022-BLG-1852. The light curves of these events commonly exhibit initial bumps followed by s…
View article: Erratum: “Photometric Selection of Unobscured QSOs at the Ecliptic Poles: KMTNet in the South Field and Pan-STARRS in the North Field” (2023, ApJS, 268, 57)
Erratum: “Photometric Selection of Unobscured QSOs at the Ecliptic Poles: KMTNet in the South Field and Pan-STARRS in the North Field” (2023, ApJS, 268, 57) Open