|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| MOA 2011-BLG-293 , the SIMBAD biblio (30 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST11:02:43 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2012ApJ...755..102Y | 812 | X C | 20 | 7 | 161 | MOA-2011-BLG-293Lb: a test of pure survey microlensing planet detections. | YEE J.C., SHVARTZVALD Y., GAL-YAM A., et al. | ||
|
2013A&A...552A.119S |
15 | D | 1 | 1487 | 118 | Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. | SAUR J., GRAMBUSCH T., DULING S., et al. | ||
| 2013MNRAS.431.2975A | 38 | X | 1 | 6 | 6 | Extending the planetary mass function to Earth mass by microlensing at moderately high magnification. | ABE F., AIREY C., BARNARD E., et al. | ||
| 2013ApJ...769...77Y | 77 | X | 2 | 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...780...54B | 507 | S X C | 11 | 5 | 47 | MOA-2011-BLG-293Lb: first microlensing planet possibly in the habitable zone. | BATISTA V., BEAULIEU J.-P., GOULD A., et al. | ||
| 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.439..604S | 39 | X | 1 | 15 | 29 | MOA-2011-BLG-322Lb: a `second generation survey' microlensing planet. | SHVARTZVALD Y., MAOZ D., KASPI S., et al. | ||
|
2014A&A...562A.108S |
15 | D | 1 | 196 | 44 | Search for 150 MHz radio emission from extrasolar planets in the TIFR GMRT Sky Survey. | SIROTHIA S.K., LECAVELIER DES ETANGS A., GOPAL-KRISHNA, et al. | ||
| 2014ApJ...788..128K | 93 | D | X | 3 | 20 | 18 | OGLE-2008-BLG-355Lb: a massive planet around a late-type star. | KOSHIMOTO N., UDALSKI A., SUMI T., et al. | |
| 2014ApJ...790...14Y | 77 | X | 2 | 6 | 8 | MOA-2013-BLG-220Lb: massive planetary companion to galactic-disk host. | YEE J.C., HAN C., GOULD A., et al. | ||
| 2015ApJ...802..108S | 156 | 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. |
| 2015ApJ...804...20C | 40 | X | 1 | 30 | 68 | Pathway to the galactic distribution of planets: combined Spitzer and ground-based microlens parallax measurements of 21 single-lens events. | CALCHI NOVATI S., GOULD A., UDALSKI A., 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 |
212 | D | X F | 5 | 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. | ||
| 2016AJ....152..140B | 39 | X | 1 | 10 | 5 | Discovery of a gas giant planet in microlensing event OGLE-2014-BLG-1760. | BHATTACHARYA A., BENNETT D.P., BOND I.A., et al. | ||
| 2016ApJ...833..145S | 40 | X | 1 | 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....1H | 40 | X | 1 | 10 | 6 | OGLE-2013-BLG-1761Lb: a massive planet around an M/K dwarf. | HIRAO Y., UDALSKI A., SUMI T., et al. | ||
| 2017AJ....154...59B | 79 | X | 2 | 30 | 10 | The star blended with the MOA-2008-BLG-310 source is not the exoplanet host star. | BHATTACHARYA A., BENNETT D.P., ANDERSON J., et al. | ||
| 2017MNRAS.469.2434B | 40 | X | 1 | 16 | 24 | The lowest mass ratio planetary microlens: OGLE 2016-BLG-1195Lb. | BOND I.A., BENNETT D.P., SUMI T., et al. | ||
|
2017AJ....154..210Z |
119 | X C | 2 | 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. | ||
| 2017AJ....154..247R | 40 | X | 1 | 5 | 3 | OGLE-2016-BLG-0693LB: probing the brown dwarf desert with microlensing. | RYU Y.-H., UDALSKI A., YEE J.C., 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. | ||
| 2019ApJ...873...30S | 41 | X | 1 | 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. | ||
|
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..268K | 1688 | A | D | X C | 41 | 12 | ~ | Bayesian approach for determining microlens system properties with high-angular-resolution follow-up imaging. | KOSHIMOTO N., BENNETT D.P. and SUZUKI D. |
| 2020AJ....160..183R | 41 | X | 1 | 23 | ~ | OGLE-2018-BLG-0532Lb: cold Neptune with possible jovian sibling. | RYU Y.-H., UDALSKI A., YEE J.C., 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. | ||
|
2022AJ....163..254S |
43 | X | 1 | 10 | 3 | 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. |