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20042023
most citedMicrolens OGLE-2005-BLG-169 Implies Cool Neptune-Like Planets are Common

336 citations · 791 across the 14 of their papers we have counts for

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7 papers · 1 filter

astro-ph.SR2023★ 4 cited

Strong Variability in AzV 493, an Extreme Oe-Type Star in the SMC

M. S. Oey, N. Castro, M. Renzo +11

We present 18 years of OGLE photometry together with spectra obtained over 12 years, revealing that the early Oe star AzV 493 shows strong photometric (Delta I < 1.2 mag) and spect…

astro-ph.SR2022

New Short-Period Delta Scuti Stars in OGLE-IV Fields toward the Galactic Bulge

P. Pietrukowicz, M. Ratajczak, I. Soszynski +12

We report the classification of 24 puzzling short-period variable stars located in OGLE-IV Galactic bulge fields. The stars are low-amplitude (<0.05 mag) multi-periodic objects wit…

astro-ph.SR2022★ 43 cited

The OGLE Collection of Variable Stars. Nearly 66,000 Mira stars in the Milky Way

Patryk Iwanek, Igor Soszyński, Szymon Kozłowski +12

We present a collection of 65,981 Mira-type variable stars found in the Optical Gravitational Lensing Experiment (OGLE) project database. Two-thirds of our sample (40,356 objects)…

astro-ph.SR2021★ 29 cited

Photometric and spectroscopic evolution of the interacting transient AT 2016jbu (Gaia16cfr)

S. J. Brennan, M. Fraser, J. Johansson +68

We present the results from a high cadence, multi-wavelength observation campaign of AT 2016jbu (aka Gaia16cfr), an interacting transient. This dataset complements the current lite…

astro-ph.SR2020★ 17 cited

A search for strong magnetic fields in massive and very massive stars in the Magellanic Clouds

S. Bagnulo, G. A. Wade, Y. Naze +13

Despite their rarity, massive stars dominate the ecology of galaxies via their strong, radiatively-driven winds throughout their lives and as supernovae in their deaths. However, t…

astro-ph.SR2017★ 77 cited

Blue large-amplitude pulsators as a new class of variable stars

P. Pietrukowicz, W. A. Dziembowski, M. Latour +13

Regular intrinsic brightness variations observed in many stars are caused by pulsations. These pulsations provide information on the global and structural parameters of the star. T…