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MOA 2011-BLG-322 , the SIMBAD biblio (14 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST02:14:56 |
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 | 422 | 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 | 142 | 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 | 40 | 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 | 178 | 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 | 98 | 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 | 41 | 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 | 123 | 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 | 17 | D | 1 | 4935 | 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 | 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 | 44 | 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 | 18 | D | 1 | 115 | 8 | Microlensing mass measurement from images of rotating gravitational arcs. | CASSAN A., RANC C., ABSIL O., et al. |