activity
20142026
most citedNo large population of unbound or wide-orbit Jupiter-mass planets

336 citations · 2.5k across the 81 of their papers we have counts for

collaborators

91 papers

astro-ph.SR2026

Eppur binaria non è esclusa: Pulsations in CZ Tuc appear to be tidally excited by its veiled companion

Piotr A. Kołaczek-Szymański, Patryk Iwanek, Jim Fuller +3

Long secondary periods (LSPs), observed in about one-third of pulsating red giants, remain unexplained despite decades of study, with binarity and non-radial oscillations as the le…

astro-ph.SR2026

Multiplicity of Cool Stars and their Evolution

Matthew I. Swayne, Leen Decin, Theo Khouri +12

Making up a sizeable portion of the galactic census, stellar multiples are experiencing a renaissance. Enabling the study of multiple strands of the study of cool stars, stellar mu…

astro-ph.SR2026

Incorporating physical source parameters into microlensing modeling

Mateusz J. Mróz, Radosław Poleski, Andrzej Udalski +14

Modeling of complex microlensing events suffers from many difficult-to-disentangle degeneracies. This is especially the case for orbital motion of the source in a binary system, th…

astro-ph.SR2026

Eppur binaria non é esclusa: Gaia astrometry does not disfavor a binary origin for Long Secondary Periods

Patryk Iwanek, Piotr A. Kołaczek-Szymański, Dorota M. Skowron +2

We present an independent reassessment of the nearby long secondary period (LSP) stars analyzed by Shariat et al. (2026). By inspecting long-term All Sky Automated Survey (ASAS) li…

astro-ph.GA2026

Rogue Ones: Orbital census of Galactic Cepheids and their Anomalies

Shourya Khanna, Ronald Drimmel, Eloisa Poggio +2

Classical Cepheids (DCEPs) are excellent standard candles expected to trace the spatial and kinematic distribution of the Galaxy's young and dynamically cold stellar disc. Using th…

astro-ph.SR2026

Thirty Circumbinary Disk Occultation Systems (KH 15D-like stars) from the OGLE Project

M. A. Urbanowicz, I. Soszyński, P. Pietrukowicz +14

We present a catalog of 30 stars that are candidates for KH 15D-like binary systems, in which the observed brightness variations are caused by a circumbinary dusty disk that period…