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20132026
most citedTESS Eclipsing Binary Stars. I. Short cadence observations of 4584 eclipsing binaries in Sectors 1-26

205 citations · 705 across the 41 of their papers we have counts for

collaborators

42 papers

astro-ph.SR2026

BS Cassiopeiae: A Contact Binary with Starspot-Driven Variability and Evidence for Additional Components

Min-Ji Jeong, Chun-Hwey Kim, Kyeongsoo Hong +5

We present a comprehensive photometric and spectroscopic analysis of the contact eclipsing binary BS Cas, based on 22-yr multi-site light curves and 2-yr high-resolution spectra. T…

astro-ph.SR2026

The Double-lined Eclipsing Doradus System AX Draconis in a 0.568-day Orbit

Jae Woo Lee, Min-Ji Jeong, Kyeongsoo Hong +3

For the near-contact binary AX Dra, we present the first time-series spectroscopy collected with the echelle spectrograph BOES. From spectral analysis, we measured the projected ro…

astro-ph.SR2025

TIC 322208686: An Eclipsing System with Doradus Pulsations and a Third Component on a Wider Orbit

Jae Woo Lee, Kyeongsoo Hong, Min-Ji Jeong +3

TIC 322208686 is known to be a detached binary that exhibits two types of variability: pulsation and eclipse. We present the physical properties of the target star using the short-…

astro-ph.SR2025

KMTNet View of Blue Large-amplitude Pulsators Toward the Galactic Bulge: I. Discovery of Wide-orbit Companions in OGLE-BLAP-006

Seung-Lee Kim, Chung-Uk Lee, Kyeongsoo Hong +6

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. Howev…

astro-ph.SR2025

Pulsations and Pre-He White Dwarf in the Post-mass Transfer Eclipsing System WASP 1021-28

Jae Woo Lee, Min-Ji Jeong, Kyeongsoo Hong

We present results from VLT/UVES spectra and TESS photometric observations of the pulsating EL CVn binary WASP 1021-28, containing a He-core white dwarf precursor (pre-He WD). Doub…

astro-ph.SR2024★ 2 cited

WASP 0346-21: An EL CVn-Type Eclipsing Binary with Multiperiodic Pulsations in a Triple System

Jae Woo Lee, Kyeongsoo Hong, Min-Ji Jeong +1

VLT/UVES spectroscopic and TESS photometric observations for WASP 0346-21 allow the direct determination of its physical properties, along with the detection of a circumbinary obje…

astro-ph.SR2023

Absolute Properties of the Oscillating Eclipsing Algol XZ Ursae Majoris

Jae Woo Lee, Kyeongsoo Hong, Hye-Young Kim +3

It is known from archival TESS data that the semi-detached Algol system XZ UMa is one of the candidate binary stars exhibiting short-period oscillations. We secured new high-resolu…

astro-ph.SR2023★ 2 cited

Improved period variations of 32 contact binaries with rapidly decreasing periods in the Galactic Bulge

Kyeongsoo Hong, Jae Woo Lee, Dong-Jin Kim +4

We present detailed analyses of updated eclipse timing diagrams for 32 contact binary merger candidates in the Galactic bulge. The photometric data was obtained from 2016 to 2021 u…

astro-ph.SR2023

Photometric and Spectroscopic Properties of the Eclipsing System V864 Monocerotis

Jang-Ho Park, Jae Woo Lee, Kyeongsoo Hong

We present the orbital period variability and evolutionary status of the W UMa-type binary system V864 Mon from accurately measured fundamental parameters. New photometric obs…

astro-ph.SR2023★ 5 cited

Absolute Properties of the Oscillating Eclipsing Algol X Trianguli

Jae Woo Lee, Kyeongsoo Hong, Jang-Ho Park +2

We report results from the TESS photometric data and new high-resolution spectra of the Algol system X Tri showing short-period pulsations. From the echelle spectra, the radial vel…

astro-ph.SR2022

A Photometric and Spectroscopic Study of the Short-Period Algol EW Boötis with a Sct Pulsator

Hye-Young Kim, Kyeongsoo Hong, Chun-Hwey Kim +4

In this paper, we present TESS photometry and high-resolution spectra of the short-period Algol EW Boo. We obtained double-lined radial velocities (RVs) from the time-series spectr…

astro-ph.SR2022★ 10 cited

The Pre-He White Dwarfs in Eclipsing Binaries. IV. WASP 1814+48 with Multiperiodic Pulsations

Jae Woo Lee, Kyeongsoo Hong, Hye-Young Kim +1

For the EL CVn candidate 1SWASPJ181417.43+481117.0 (WASP 1814+48), we secured the first spectroscopic observations between 2015 April and 2021 March. Using the echelle spectra, the…

astro-ph.SR2022★ 8 cited

Period Changes of 14,127 Contact Eclipsing Binaries in the Galactic Bulge

Kyeongsoo Hong, Jae Woo Lee, Jang-Ho Park +5

We present the orbital period variations of 14,127 contact eclipsing binaries (CEBs) based on the OGLE-III\&IV observations in the Galactic bulge. New times of minimum lights for t…

astro-ph.SR2022★ 9 cited

The Pre-He White Dwarfs in Eclipsing Binaries. III. WASP 1625-04

Jae Woo Lee, Kyeongsoo Hong, Jang-Ho Park

1SWASP J162545.15-043027.9 (WASP 1625-04) has been announced as one of EL CVn candidates showing total primary eclipses and ellipsoidal variations. This paper presents the absolute…

astro-ph.SR2021★ 205 cited

TESS Eclipsing Binary Stars. I. Short cadence observations of 4584 eclipsing binaries in Sectors 1-26

Andrej Prsa, Angela Kochoska, Kyle E. Conroy +44

In this paper we present a catalog of 4584 eclipsing binaries observed during the first two years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binar…

astro-ph.SR2021

Pulsation and Rotation of the EL CVn-type Eclipsing Binary 1SWASP J024743.37-251549.2

Seung-Lee Kim, Jae Woo Lee, Chung-Uk Lee +6

EL CVn-type eclipsing binaries are composed of a massive A-type main-sequence primary star and a hotter B-type secondary star. This paper presents the time-series photometric and a…

astro-ph.SR2020★ 9 cited

Tidally Excited Modes and Scuti Pulsations in the Eclipsing Triple Star IM Persei

Jae Woo Lee, Kyeongsoo Hong, Hye-Young Kim

IM Per is a triple star system whose eclipsing pair masses and radii are accurate to within 1 \%. The TESS light curve of the program target exhibits partial eclipses and multiple…

astro-ph.SR2020★ 11 cited

Cephei Pulsations in the High-mass Eclipsing System CW Cephei

Jae Woo Lee, Kyeongsoo Hong

CW Cep is an early B-type eclipsing binary with mass measurement precisions better than 1 \%. We report the discovery of pulsation signatures in the TESS time-series data of the sy…

astro-ph.SR2020★ 6 cited

Physical Nature of the Eclipsing δ Scuti Star AO Serpentis

Jang-Ho Park, Jae Woo Lee, Kyeongsoo Hong +2

We present the absolute properties of the eclipsing binary AO Ser with a pulsating component from our photometric and high-resolution spectroscopic observations, which were pe…

astro-ph.SR2020★ 19 cited

The Pre-He White Dwarfs in Eclipsing Binaries. I. WASP 0131+28

Jae Woo Lee, Jae-Rim Koo, Kyeongsoo Hong +1

We report the first light curves and high-resolution spectra of the post-mass transfer binary star WASP 0131+28 to study the absolute properties of extremely low-mass white dw…

astro-ph.SR2020★ 8 cited

TESS Photometry of the Eclipsing Scuti Star AI Hydrae

Jae Woo Lee, Kyeongsoo Hong, Martti H. Kristiansen

AI Hya has been known as an eclipsing binary with a monoperiodic Sct pulsator. We present the results from its {\it TESS} photometry observed during Sector 7. Including our fiv…

astro-ph.SR2019★ 14 cited

Absolute Properties of the Eclipsing Dor Star V404 Lyrae

Jae Woo Lee, Kyeongsoo Hong, Jae-Rim Koo +1

We present the first high-resolution spectra for the eclipsing binary V404 Lyr showing Dor pulsations, which we use to study its absolute properties. By fitting models to the d…

astro-ph.EP2019★ 34 cited

OGLE-2018-BLG-1011L\lowercase{b,c}: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star

Cheongho Han, David P. Bennett, Andrzej Udalski +70

We report a multiplanetary system found from the analysis of microlensing event OGLE-2018-BLG-1011, for which the light curve exhibits a double-bump anomaly around the peak. We fin…

astro-ph.EP2019★ 20 cited

Spectroscopic Mass and Host-star Metallicity Measurements for Newly Discovered Microlensing Planet OGLE-2018-BLG-0740Lb

Cheongho Han, Jennifer C. Yee, Andrzej Udalski +63

We report the discovery of the microlensing planet OGLE-2018-BLG-0740Lb. The planet is detected with a very strong signal of , but the interpretation of the signal s…