OGLE-2015-BLG-1609Lb: A sub-Jovian planet orbiting a low-mass stellar or brown dwarf host

We present a comprehensive analysis of the planetary microlensing event OGLE-2015-BLG-1609. The planetary anomaly was detected by two survey telescopes, OGLE and MOA. Both surveys collected enough data over the planetary anomaly to enable an unambiguous planet detection. Such survey detections of planetary anomalies are needed to build a robust sample of planets, which could improve studies on the microlensing planetary occurrence rate by reducing biases and statistical uncertainties. In this work we examined different methods for modeling microlensing events using individual datasets. In particular, we incorporated a Galactic model prior to better constrain the poorly defined microlensing parallax. Ultimately, we fitted a comprehensive model to all available data, identifying three potential topologies, with two showing comparably high Bayesian evidence. Our analysis indicates that the host of the planet is either a brown dwarf, with a probability of 34%, or a low-mass stellar object (M dwarf), with a probability of 66%. The topology that provides the best fit to the data results in an extraordinary low host mass, M h = 0.025 +0.050 -0.012 M ⊙ , accompanied by an Earth-mass planet with M c = 1.9 +3.9 -1.0 M ⊕ .

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-05-01
DOI
https://doi.org/10.1051/0004-6361/202453454
Citations
1
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
1.15

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article

OGLE-2015-BLG-1609Lb: A sub-Jovian planet orbiting a low-mass stellar or brown dwarf host

M. Rabus, I. Soszyński, Yuki Satoh, Sean K. Terry et al.
1 citations
Astronomy and Astrophysics
Astro and Planetary Science
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article

OGLE-2015-BLG-1609Lb: A sub-Jovian planet orbiting a low-mass stellar or brown dwarf host

M. Rabus, I. Soszyński, Yuki Satoh, Sean K. Terry, Riku Hamada, M. Hundertmark, T. Nagai, M. Gromadzki, R. Poleski, Akihiko Fukui, Y. Muraki, Krzysztof A. Rybicki, D. P. Bennett, J. Skottfelt, M. K. Szymański, J. Skowron, S. Rahvar, Seiichi Hamada, Satoshi Miyazaki, T. Sumi, R. A. Street, C. Snodgrass, S. Ishitani Silva, J. Southworth, Naoki Koshimoto, Aikaterini Vandorou, G. D’Ago, R. Figuera Jaimes, V. Bozza, D. M. Skowron, T. C. Hinse, J. Menzies, Patryk Iwanek, H. Yama, D. Suzuki, I. A. Bond, P. Pietrukowicz, P. Mróz, I. A. Steele, Nicholas J. Rattenbury, E. Kerins, H. Korhonen, Greg Olmschenk, Michael Küffmeier, A. Bhattacharya, Yuki Hirao, P. Longa-Peña, P. J. Tristram, S. Kozłowski, Y. Tsapras, A. Udalski, M. Ratajczak, M. Dominik, E. Bachelet, Luigi Mancini, Marcin Wrona, Kansuke Nunota, Y. Itow, K. Ulaczyk, F. Abe, K. Horne, J. Wambsganss, C. Ranc, A. Cassan, Mateusz J. Mroz, Ulrik Jørgensen, Naotaka Hamasaki, Y. Matsubara, Koichi Bando, R. Schmidt
article en
1 citations

Abstract

We present a comprehensive analysis of the planetary microlensing event OGLE-2015-BLG-1609. The planetary anomaly was detected by two survey telescopes, OGLE and MOA. Both surveys collected enough data over the planetary anomaly to enable an unambiguous planet detection. Such survey detections of planetary anomalies are needed to build a robust sample of planets, which could improve studies on the microlensing planetary occurrence rate by reducing biases and statistical uncertainties. In this work we examined different methods for modeling microlensing events using individual datasets. In particular, we incorporated a Galactic model prior to better constrain the poorly defined microlensing parallax. Ultimately, we fitted a comprehensive model to all available data, identifying three potential topologies, with two showing comparably high Bayesian evidence. Our analysis indicates that the host of the planet is either a brown dwarf, with a probability of 34%, or a low-mass stellar object (M dwarf), with a probability of 66%. The topology that provides the best fit to the data results in an extraordinary low host mass, M h = 0.025 +0.050 -0.012 M ⊙ , accompanied by an Earth-mass planet with M c = 1.9 +3.9 -1.0 M ⊕ .

Astronomy and AstrophysicsVol. 698
Deutsche Forschungsgemeinschaft, Narodowa Agencja Wymiany Akademickiej, Agencia Nacional de Investigación y Desarrollo, Japan Society for the Promotion of Science
Openalex Percentile: Top 20%
Astro and Planetary Science
1.15
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