MOA 2011-BLG-322 , the SIMBAD biblio

MOA 2011-BLG-322 , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:26:53

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2014ApJ...780..123S 39           X         1 10 14 MOA-2008-BLG-379Lb: a massive planet from a high magnification event with a faint source. SUZUKI D., UDALSKI A., SUMI T., et al.
2014MNRAS.438.2466N 415     A     X C F     9 1 11 Signatures of rotating binaries in microlensing experiments. NUCITA A.A., GIORDANO M., DE PAOLIS F., et al.
2014MNRAS.439..604S 139     A     X         4 15 29
MOA-2011-BLG-322Lb: a `second generation survey' microlensing planet. 		SHVARTZVALD Y., MAOZ D., KASPI S., et al.
2015MNRAS.454..946R 39           X         1 7 12 MOA-2010-BLG-353Lb: a possible Saturn revealed. RATTENBURY N.J., BENNETT D.P., SUMI T., et al.
2016MNRAS.457.4089S viz 173       D     X   F     4 31 60 The frequency of snowline-region planets from four years of OGLE-MOA-Wise second-generation microlensing. SHVARTZVALD Y., MAOZ D., UDALSKI A., et al.
2016ApJ...827L..22T 16       D               2 44 4 An opportunistic search for extraterrestrial intelligence (SETI) with the murchison widefield array. TINGAY S.J., TREMBLAY C., WALSH A., et al.
2016ApJ...830..150P 16       D               1 38 33 Is the galactic bulge devoid of planets? PENNY M.T., HENDERSON C.B. and CLANTON C.
2016ApJ...833..145S 95       D     X         3 64 176 The exoplanet mass-ratio function from the MOA-II survey: discovery of a break and likely peak at a Neptune mass. SUZUKI D., BENNETT D.P., SUMI T., et al.
2017A&A...604A.103P 40         O X         1 14 10 A companion on the planet/brown dwarf mass boundary on a wide orbit discovered by gravitational microlensing. POLESKI R., UDALSKI A., BOND I.A., et al.
2018AJ....156..236Z 120           X C       2 20 5 KMT-2016-BLG-1397b: KMTNET-only discovery of a microlens giant planet. ZANG W., HWANG K.-H., KIM H.-W., et al.
2020ApJ...890...23L viz 16       D               1 4936 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2021AJ....162...17K viz 17       D               1 54 ~ KMT-2019-BLG-0371 and the limits of Bayesian analysis. KIM Y.H., CHUNG S.-J., YEE J.C., et al.
2021ApJ...918L...8K 42           X         1 13 11 No large dependence of planet frequency on Galactocentric distance. KOSHIMOTO N., BENNETT D.P., SUZUKI D., et al.
2022NatAs...6..121C 17       D               1 115 8 Microlensing mass measurement from images of rotating gravitational arcs. CASSAN A., RANC C., ABSIL O., et al.
2024ApJ...967...77N 45           X         1 8 ~ Measurement of Dependence of Microlensing Planet Frequency on the Host Star Mass and Galactocentric Distance by Using a Galactic Model. NUNOTA K., KOSHIMOTO N., SUZUKI D., et al.
2025ApJ...995L..55Z 65       D     X         2 18 ~ The Brown-dwarf Desert Persists as a Mass-ratio Desert around Low-mass Stars. ZHANG K.

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