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MOA 2007-BLG-400b , the SIMBAD biblio (33 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.03.23CET08:29:56 |
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 |
---|---|---|---|---|---|---|---|---|---|
2008ApJ...689.1084K | 8 | 2 | Limits of binaries that can be characterized by gravitational microlensing. | KIM D., RYU Y.-H., PARK B.-G., et al. | |||||
2009ApJ...691..452H | 76 | X | 2 | 9 | 8 | Microlensing zone of planets detectable through the channel of high-magnification events. | HAN C. | ||
2009ApJ...693.1835H | 41 | X | 1 | 2 | 12 | Planetary lensing signals of high-magnification events under the severe finite-source effect. | HAN C. and KIM D. | ||
2009ApJ...698.1826D | 523 | T A | X C F | 11 | 9 | 86 |
Microlensing event MOA-2007-BLG-400: exhuming the buried signature of a cool, Jovian-mass planet. |
DONG S., BOND I.A., GOULD A., et al. | |
2009A&A...508..467B | 38 | X | 1 | 17 | 17 | Mass measurement of a single unseen star and planetary detection efficiency. for OGLE 2007-BLG-050. | BATISTA V., DONG S., GOULD A., et al. | ||
2010ApJ...710.1641S | 83 | X | 2 | 12 | 147 | A cold neptune-mass planet OGLE-2007-BLG-368Lb: cold neptunes are common. | SUMI T., BENNETT D.P., BOND I.A., et al. | ||
2010ApJ...711..731J | 119 | X | 3 | 10 | 89 | Sub-Saturn planet MOA-2008-BLG-310Lb: likely to Be in the Galactic Bulge. | JANCZAK J., FUKUI A., DONG S., et al. | ||
2010ApJ...713..837B | 42 | X | 1 | 10 | 89 | Masses and orbital constraints for the OGLE-2006-BLG-109Lb,c Jupiter/Saturn analog planetary system. | BENNETT D.P., RHIE S.H., NIKOLAEV S., et al. | ||
2010ApJ...713..865C | 38 | X | 1 | 3 | 4 | Properties of microlensing central perturbations by planets in binary stellar systems under the strong finite-source effect. | CHUNG S.-J. and PARK B.-G. | ||
2010ApJ...716.1408B | 78 | X | 2 | 19 | 52 | An efficient method for modeling high-magnification planetary microlensing events. | BENNETT D.P. | ||
2010ApJ...720.1073G | 134 | D | X | 4 | 30 | 211 | Frequency of solar-like systems and of ice and gas giants beyond the snow line from high-magnification microlensing events in 2005-2008. | GOULD A., DONG S., GAUDI B.S., et al. | |
2010MNRAS.406.1918D | 15 | D | 1 | 404 | 29 | The Hill stability of the possible moons of extrasolar planets. | DONNISON J.R. | ||
2010A&A...518A..51F | 77 | X | 2 | 20 | 14 | OGLE 2008-BLG-290: an accurate measurement of the limb darkening of a galactic bulge K giant spatially resolved by microlensing. | FOUQUE P., HEYROVSKY D., DONG S., et al. | ||
2010A&A...520A..68L | 41 | X | 1 | 3 | 22 | Detectability of extrasolar moons as gravitational microlenses. | LIEBIG C. and WAMBSGANSS J. | ||
2011ApJ...728..120M | 94 | D | C | 2 | 14 | 31 | A Sub-Saturn mass planet, MOA-2009-BLG-319Lb. | MIYAKE N., SUMI T., DONG S., et al. | |
2011MNRAS.411....2D | 39 | X | 1 | 11 | 8 | Planetary mass function and planetary systems. | DOMINIK M. | ||
2012Natur.481..167C ![]() |
201 | 265 | One or more bound planets per Milky Way star from microlensing observations. | CASSAN A., KUBAS D., BEAULIEU J.-P., et al. | |||||
2012NewAR..56...25B | 16 | D | X | 1 | 30 | 1 | The first extrasolar planet detected via gravitational microlensing. | BOND I.A. | |
2012ApJ...751...41C | 78 | X | 2 | 23 | 23 | Characterizing lenses and lensed stars of high-magnification single-lens gravitational microlensing events with lenses passing over source stars. | CHOI J.-Y., SHIN I.-G., PARK S.-Y., et al. | ||
2012RAA....12..947M | 94 | D | C | 3 | 23 | 36 | Astrophysical applications of gravitational microlensing. | MAO S. | |
2013A&A...549A.109B ![]() |
1 | 172 | 346 | The HARPS search for southern extra-solar planets. XXXI. The M-dwarf sample. | BONFILS X., DELFOSSE X., UDRY S., et al. | ||||
2013A&A...552A.119S ![]() |
16 | D | 1 | 1487 | 42 | Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. | SAUR J., GRAMBUSCH T., DULING S., et al. | ||
2013ApJ...769...77Y | 39 | X | 1 | 10 | 15 | MOA-2010-BLG-311: a planetary candidate below the threshold of reliable detection. | YEE J.C., HUNG L.-W., BOND I.A., et al. | ||
2014ApJ...788...73Z | 16 | D | 1 | 28 | 24 | Predictions for microlensing planetary events from core accretion theory. | ZHU W., PENNY M., MAO S., et al. | ||
2014ApJ...794...71H | 16 | D | 1 | 24 | 11 | Candidate gravitational microlensing events for future direct lens imaging. | HENDERSON C.B., PARK H., SUMI T., et al. | ||
2015ApJ...802..108S | 161 | A | D | X | 5 | 12 | 1 | Constraint on additional planets in planetary systems discovered through the channel of high-magnification gravitational microlensing events. | SHIN I.-G., HAN C., CHOI J.-Y., et al. |
2016ApJ...833..145S | 41 | X | 1 | 64 | 43 | 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. | ||
2017AJ....153..143M | 16 | D | 1 | 53 | 10 | OGLE-2016 a high-mass planet from a high-magnification pure-survey microlensing event. | MROZ P., HAN C., UDALSKI A., et al. | ||
2017A&A...604A.103P | 41 | X | 1 | 14 | 6 | 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. | ||
2017AJ....154..203B | 100 | D | X | 3 | 6 | 6 | PyLIMA: an open-source package for microlensing modeling. I. Presentation of the software and analysis of single-lens models. | BACHELET E., NORBURY M., BOZZA V., et al. | |
2021AJ....162...60B | 90 | X | 2 | 9 | ~ | MOA-2007-BLG-400 a super-Jupiter-mass planet orbiting a Galactic bulge K-dwarf revealed by Keck adaptive optics imaging. | BHATTACHARYA A., BENNETT D.P., BEAULIEU J.P., et al. | ||
2021AJ....162..163Z ![]() |
90 | C | 1 | 20 | ~ | Systematic KMTNet planetary anomaly search. I. OGLE-2019-BLG-1053Lb, a buried terrestrial planet. | ZANG W., HWANG K.-H., UDALSKI A., et al. | ||
2022AJ....163..254S ![]() |
47 | X | 1 | 10 | ~ | OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in the Galactic Bulge. | SHIN I.-G., YEE J.C., HWANG K.-H., et al. |
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