activity
20082026
most citedOne or more bound planets per Milky Way star from microlensing observations

588 citations · 5.8k across the 140 of their papers we have counts for

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Showing 2020Show all

11 papers · 1 filter

astro-ph.GA2020★ 45 cited

Time Delay of MgII Emission Response for the Luminous Quasar HE 0435-4312: Towards Application of High-Accretor Radius-Luminosity Relation in Cosmology

Michal Zajaček, Bożena Czerny, Mary Loli Martinez-Aldama +21

Using the six years of the spectroscopic monitoring of the luminous quasar HE 0435-4312 () with the Southern African Large Telescope (SALT), in combination with the photo…

astro-ph.EP2020★ 70 cited

A terrestrial-mass rogue planet candidate detected in the shortest-timescale microlensing event

P. Mroz, R. Poleski, A. Gould +27

Some low-mass planets are expected to be ejected from their parent planetary systems during early stages of planetary system formation. According to planet-formation theories, such…

astro-ph.SR2020★ 7 cited

OGLE-GAL-ACEP-091 -- The First Known Multi-Mode Anomalous Cepheid

I. Soszyński, R. Smolec, A. Udalski +12

Anomalous Cepheids (ACs) are metal-deficient, core-helium-burning pulsating stars with masses in the range 1.2-2.2 M_S. Until recently, all known ACs were pure single-mode pulsator…

astro-ph.HE2020★ 8 cited

Dynamical Modeling of CXOGBS J175553.2-281633: A 10 Hour Long Orbital Period Cataclysmic Variable

Sebastian Gomez, Manuel A. P. Torres, Peter G. Jonker +8

We present modeling of the long-term optical light curve and radial velocity curve of the binary stellar system CXOGBS J175553.2-281633, first detected in X-rays in the \textit{Cha…

astro-ph.SR2020★ 9 cited

OGLE-2018-BLG-1269Lb: A Jovian Planet With A Bright, Host

Youn Kil Jung, Andrew Gould, Andrzej Udalski +54

We report the discovery of a planet in the microlensing event OGLE-2018-BLG-1269, with planet-host mass ratio , i.e., times smaller than the Jupiter/Su…

astro-ph.GA2020★ 44 cited

Time-delay measurement of MgII broad line response for the highly-accreting quasar HE 0413-4031: Implications for the MgII-based radius-luminosity relation

Michal Zajaček, Bożena Czerny, Mary Loli Martinez-Aldama +16

We present the monitoring of the AGN continuum and MgII broad line emission for the quasar HE 0413-4031 () based on the six-year monitoring by the South African Large Teles…

astro-ph.EP2020★ 16 cited

A Gas Giant Planet in the OGLE-2006-BLG-284L Stellar Binary System

David P. Bennett, Andrzej Udalski, Ian A. Bond +32

We present the analysis of microlensing event OGLE-2006-BLG-284, which has a lens system that consists of two stars and a gas giant planet with a mass ratio of $q_p = (1.26\pm 0.19…

astro-ph.GA2020★ 30 cited

Microlensing optical depth and event rate in the OGLE-IV Galactic plane fields

Przemek Mroz, Andrzej Udalski, Michal K. Szymanski +10

Searches for gravitational microlensing events are traditionally concentrated on the central regions of the Galactic bulge but many microlensing events are expected to occur in the…

astro-ph.EP2020★ 8 cited

KMT-2019-BLG-1339L: an M Dwarf with a Giant Planet or a Companion Near the Planet/Brown Dwarf Boundary

Cheongho Han, Doeon Kim, Andrzej Udalski +31

We analyze KMT-2019-BLG-1339, a microlensing event with an obvious but incompletely resolved brief anomaly feature around the peak of the light curve. Although the origin of the an…

astro-ph.EP2020★ 34 cited

A free-floating or wide-orbit planet in the microlensing event OGLE-2019-BLG-0551

P. Mroz, R. Poleski, C. Han +30

High-cadence observations of the Galactic bulge by the microlensing surveys led to the discovery of a handful of extremely short-timescale microlensing events that can be attribute…

astro-ph.SR2020★ 34 cited

The Cluster Ages Experiment (CASE). VIII. Age and Distance of the Globular Cluster 47 Tuc from the Analysis of Two Detached Eclipsing Binaries

I. B. Thompson, A. Udalski, A. Dotter +20

We use photometric and spectroscopic observations of the eclipsing binary E32 in the globular cluster 47 Tuc to derive the masses, radii, and luminosities of the component stars. T…