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Profil bibliographique

M Gromadzki

Informations fournies par OpenAlex. Research Africa ne déduit ni nationalité, ni poste, ni coordonnées personnelles.

3Publications signalées
1Citations signalées
2Affiliations récentes

Les institutions déclarées

Les domaines associés

Stellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchGalaxies: Formation, Evolution, PhenomenaAstrophysics and Star Formation StudiesGamma-ray bursts and supernovae

Les publications récentes

Accès ouvert 2026 article OpenAlex

Four Cold Giant Planets Discovered by High-cadence Microlensing Surveys

Cheongho Han, Chung‐Uk Lee, A. Udalski, Ian A. Bond et autres

Abstract We report the discovery of four cold giant planets identified through the analysis of microlensing events detected by high-cadence surveys: OGLE-2016-BLG-0261, KMT-2025-BLG-0026, KMT-2025-BLG-0030, and KMT-2025-BLG-2272. The planetary signals appear as short-duration anomalies in the light curves and are well described by …

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0 citations The Astronomical Journal
Accès ouvert 2026 article OpenAlex

Mass Production of 2023 KMTNet Microlensing Planets. II. Two Planets and A Brown Dwarf

Zhixing Li, Hongyu Li, Weicheng Zang, Yoon-Hyun Ryu et autres

Abstract To expand the homogeneous microlensing planetary sample of the Korea Microlensing Telescope Network (KMTNet), we investigate six planetary candidates identified by the AnomalyFinder search in the 2023 prime-field data, namely KMT-2023-BLG-1592, OGLE-2023-BLG-0766, KMT-2023-BLG-0332, KMT-2023-BLG-0486, KMT-2023-BLG-0792, and OGLE-2023-BLG-1043. Light-curve modeling indicates that …

cn, kr, pl, jp, nz, de, us, ye, Zimbabwe, il, gb, es, fr (code pays fourni par la source)

1 citation The Astronomical Journal
Accès ouvert 2026 article OpenAlex

Early interaction signatures and an extended plateau phase in Type II SN 2020aze

B Ailawadhi, R Dastidar, K Misra, S Valenti et autres

ABSTRACT We present a photometric and spectroscopic analysis of the fast-declining Type II SN 2020aze, observed in optical bands from 2.2 to 137.4 d post-explosion. The V-band light curve reaches a peak absolute magnitude of $-16.97\ \pm$ 0.20 mag by 15 d, …

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0 citations Monthly Notices of the Royal Astronomical Society

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