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| MOA 2015-BLG-281 , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:49:04 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2015ApJ...814...92C |
133 | D | X | 4 | 171 | 31 | Spitzer IRAC photometry for time series in crowded fields. | CALCHI NOVATI S., GOULD A., YEE J.C., et al. | |
| 2016ApJ...819...93S | 593 | T | X C | 13 | 9 | 66 |
Spitzer parallax of OGLE-2015-BLG-0966: a cold Neptune in the galactic disk. |
STREET R.A., UDALSKI A., CALCHI NOVATI S., et al. | |
| 2016ApJ...824..109C | 39 | X | 1 | 5 | 9 | Microlensing parallax for observers in heliocentric motion. | CALCHI NOVATI S. and SCARPETTA G. | ||
| 2016ApJ...825...60Z | 41 | X | 1 | 7 | 34 | Mass measurements of isolated objects from space-based microlensing. | ZHU W., CALCHI NOVATI S., GOULD A., et al. | ||
| 2017PASP..129g4401J | 397 | T | X C | 8 | 3 | ~ |
The radial velocity of OGLE-2015-BLG-0966S. |
JOHNSON S.A. and YEE J.C. | |
|
2017AJ....154..210Z |
159 | X | 4 | 75 | 40 | Toward a Galactic distribution of planets. I. Methodology and planet sensitivities of the 2015 high-cadence Spitzer microlens sample. | ZHU W., UDALSKI A., CALCHI NOVATI S., et al. | ||
| 2018AJ....155...40R | 81 | C | 2 | 17 | 21 | OGLE-2016-BLG-1190Lb: the first Spitzer bulge planet lies near the planet/brown-dwarf boundary. | RYU Y.-H., YEE J.C., UDALSKI A., et al. | ||
| 2018ApJ...853...70U | 41 | X | 1 | 7 | 7 | OGLE-2014-BLG-0289: precise characterization of a quintuple-peak gravitational microlensing event. | UDALSKI A., HAN C., BOZZA V., et al. | ||
| 2018A&A...609A..55H | 41 | X | 1 | 4 | 4 | RoboTAP: Target priorities for robotic microlensing observations. | HUNDERTMARK M., STREET R.A., TSAPRAS Y., et al. | ||
| 2018AJ....155..261C | 16 | D | 1 | 15 | 8 | Spitzer opens new path to break classic degeneracy for Jupiter-mass microlensing planet OGLE-2017-BLG-1140Lb. | CALCHI NOVATI S., SKOWRON J., JUNG Y.K., et al. | ||
| 2018AJ....156..113B | 40 | X | 1 | 21 | 9 | A planetary microlensing event with an unusually red source star: MOA-2011-BLG-291. | BENNETT D.P., UDALSKI A., BOND I.A., et al. | ||
| 2019AJ....157...72J | 16 | D | 1 | 32 | 7 | KMT-2017-BLG-0165Lb: a super-Neptune-mass planet orbiting a Sun-like host star. | JUNG Y.K., GOULD A., ZANG W., et al. | ||
| 2019ApJ...873...30S | 16 | D | 2 | 19 | 3 | OGLE-2014-BLG-0962 and a comparison of Galactic model priors to microlensing data. | SHAN Y., YEE J.C., UDALSKI A., et al. | ||
| 2019MNRAS.487.4603T | 4 | ~ | An analysis of binary microlensing event OGLE-2015-BLG-0060. | TSAPRAS Y., CASSAN A., RANC C., et al. | |||||
| 2019MNRAS.488.3308L | 41 | X | 1 | 5 | 2 | OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing. | LI S.-S., ZANG W., UDALSKI A., 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. | ||
| 2020AJ....159..134H | 41 | X | 1 | 14 | ~ | Candidate brown-dwarf microlensing events with very short timescales and small angular Einstein radii. | HAN C., LEE C.-U., UDALSKI A., et al. | ||
|
2020AJ....160...74H |
41 | X | 1 | 29 | ~ | OGLE-2017-BLG-0406: Spitzer microlens parallax reveals Saturn-mass planet orbiting M-dwarf host in the inner Galactic disk. | HIRAO Y., BENNETT D.P., RYU Y.-H., 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. | ||
| 2022MNRAS.514.5952Z | 43 | X | 1 | 20 | 11 | OGLE-2018-BLG-0799Lb: a q ∼ 2.7 x 10–3 planet with Spitzer parallax. | ZANG W., SHVARTZVALD Y., UDALSKI A., et al. | ||
| 2023MNRAS.522.6055Z | 44 | X | 1 | 16 | 1 | KMT-2022-BLG-0440Lb: A new q < 10–4 microlensing planet with the central-resonant caustic degeneracy broken. | ZHANG J., ZANG W., JUNG Y.K., et al. | ||
| 2025A&A...696A..94D | 19 | D | 1 | 44 | ~ | Earth-like planet predictor: A machine learning approach. | DAVOULT J., ELTSCHINGER R. and ALIBERT Y. |