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| MOA 2010-BLG-328 , the SIMBAD biblio (14 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST01:00:19 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2013ApJ...779...91F | 271 | X C | 6 | 4 | 17 | MOA-2010-BLG-328Lb: a Sub-Neptune orbiting very late M dwarf? | FURUSAWA K., UDALSKI A., SUMI T., et al. | ||
| 2014ApJ...788..128K | 15 | D | 1 | 20 | 18 | OGLE-2008-BLG-355Lb: a massive planet around a late-type star. | KOSHIMOTO N., UDALSKI A., SUMI T., et al. | ||
| 2016ApJ...825..112S | 81 | X | 2 | 6 | 33 | The first Neptune analog or super-Earth with a Neptune-like orbit: MOA-2013-BLG-605Lb. | SUMI T., UDALSKI A., BENNETT D.P., 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 | 173 | D | X | 5 | 38 | 33 | Is the galactic bulge devoid of planets? | PENNY M.T., HENDERSON C.B. and CLANTON C. | |
| 2016ApJ...833..145S | 56 | D | X | 2 | 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. | |
| 2017AJ....154...68B | 40 | X | 1 | 11 | 2 | MOA data reveal a new mass, distance, and relative proper motion for planetary system OGLE-2015-BLG-0954L. | BENNETT D.P., BOND I.A., ABE F., et al. | ||
|
2018ApJS..239...14J |
16 | D | 1 | 1561 | 6 | Revised exoplanet radii and habitability using Gaia data release 2. | JOHNS D., MARTI C., HUFF M., et al. | ||
|
2020ApJ...890...23L |
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. | ||
| 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. | ||
| 2024AJ....168...15B | 224 | X | 5 | 23 | ~ | Keck and Hubble Observations Show that MOA-2008-BLG-379Lb is a Super-Jupiter Orbiting an M Dwarf. | BENNETT D.P., BHATTACHARYA A., BEAULIEU J.-P., et al. | ||
| 2025AJ....170..310V | 1194 | T A | S X C | 23 | 6 | ~ |
MOA-2010-BLG-328: Keck and HST Expose the Limits of Occams Razor in Microlensing. |
VANDOROU A., BENNETT D.P., BEAULIEU J.-P., et al. |