other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
EWS 2005-BLG-169 , the SIMBAD biblio (66 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST02:21:16 |
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 |
---|---|---|---|---|---|---|---|---|---|
2006ApJ...643L.131R | 1 | 8 | 31 | The search for other earths: limits on the giant planet orbits that allow habitable terrestrial planets to form. | RAYMOND S.N. | ||||
2006ApJ...644L..37G | 17 | 8 | 275 | Microlens OGLE-2005-BLG-169 implies that cool Neptune-like planets are common. | GOULD A., UDALSKI A., AN D., et al. | ||||
2006ApJ...647L.171B | 6 | 8 | 104 | Identification of the OGLE-2003-BLG-235/MOA-2003-BLG-53 planetary host star. | BENNETT D.P., ANDERSON J., BOND I.A., et al. | ||||
2007ApJ...660..781B | 2 | 8 | 43 | Characterization of gravitational microlensing planetary host stars. | BENNETT D.P., ANDERSON J. and GAUDI B.S. | ||||
2007ApJ...660..823M | 110 | 111 | Formation of earth-like planets during and after giant planet migration. | MANDELL A.M., RAYMOND S.N. and SIGURDSSON S. | |||||
2007AcA....57..281S | 16 | 16 | Binary lenses in OGLE III EWS database. Season 2005. | SKOWRON J., JAROSZYNSKI M., UDALSKI A., et al. | |||||
2007Msngr.128...33B | 5 | 2 | Hunting for Frozen Super-Earths via Microlensing. | BEAULIEU J.-P., ALBROW M., BENNETT D., et al. | |||||
2008ApJ...687.1339K | 237 | 103 | Extrasolar giant planets and X-ray activity. | KASHYAP V.L., DRAKE J.J. and SAAR S.H. | |||||
2009ApJ...690.1772P | 40 | X | 1 | 16 | 80 | Extended-source effect and chromaticity in two-point-mass microlensing. | PEJCHA O.R. and HEYROVSKY D. | ||
2009AN....330....4T | 4 | 7 | 59 | RoboNet-II: Follow-up observations of microlensing events with a robotic network of telescopes. | TSAPRAS Y., STREET R., HORNE K., et al. | ||||
2009AcA....59..255N | 38 | X | 1 | 21 | 4 | Finding the brightest Galactic Bulge microlensing events with a small aperture telescope and image subtraction. | NATAF D.M., STANEK K.Z. and BAKOS G.A. | ||
2009ApJ...705..386C | 61 | A | X | 2 | 2 | 1 | Characterization of the resonant caustic perturbation. | CHUNG S.-J. | |
2010ApJ...716.1408B | 321 | D | S X | 8 | 19 | 52 | An efficient method for modeling high-magnification planetary microlensing events. | BENNETT D.P. | |
2010ApJ...720.1073G | 172 | D | X | 5 | 30 | 287 | 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. | |
2010AcA....60..197J | 38 | X | 1 | 63 | 12 | Binary lenses in OGLE-III EWS database. Seasons 2006-2008. | JAROSZYNSKI M., SKOWRON J., UDALSKI A., et al. | ||
2012MNRAS.419.3631S | 43 | X | 1 | 4 | 35 | Second-generation microlensing planet surveys: a realistic simulation. | SHVARTZVALD Y. and MAOZ D. | ||
2012NewAR..56...25B | 116 | X | 3 | 30 | 1 | The first extrasolar planet detected via gravitational microlensing. | BOND I.A. | ||
2012MNRAS.426.1496I | 209 | D | X C | 5 | 22 | 20 | Polarization in microlensing events towards the Galactic bulge. | INGROSSO G., CALCHI NOVATI S., DE PAOLIS F., et al. | |
2013A&A...552A.119S | 16 | D | 1 | 1487 | 118 | Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. | SAUR J., GRAMBUSCH T., DULING S., et al. | ||
2014A&A...562A.108S | 16 | 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...791...90C | 16 | D | 1 | 14 | 15 | Synthesizing exoplanet demographics from radial velocity and microlensing surveys. I. Methodology. | CLANTON C. and GAUDI B.S. | ||
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 | 159 | 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...808..169B | 514 | T A | X C | 11 | 4 | 113 |
Confirmation of the planetary microlensing signal and star and planet mass determinations for event OGLE-2005-BLG-169. |
BENNETT D.P., BHATTACHARYA A., ANDERSON J., et al. | |
2015ApJ...808..170B | 456 | T | X C | 9 | 3 | 117 |
Confirmation of the OGLE-2005-BLG-169 planet signature and its characteristics with lens-source proper motion detection. |
BATISTA V., BEAULIEU J.-P., BENNETT D.P., et al. | |
2015ApJ...814..111S | 41 | X | 1 | 9 | 26 | Spitzer microlens measurement of a massive remnant in a well-separated binary. | SHVARTZVALD Y., UDALSKI A., GOULD A., et al. | ||
2016ApJ...824..109C | 41 | X | 1 | 5 | 9 | Microlensing parallax for observers in heliocentric motion. | CALCHI NOVATI S. and SCARPETTA G. | ||
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 | 42 | 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. | ||
2016AJ....152..181H | 16 | D | 1 | 9279 | 22 | SETI observations of exoplanets with the Allen Telescope Array. | HARP G.R., RICHARDS J., TARTER J.C., et al. | ||
2017MNRAS.466.2710R | 41 | X | 1 | 8 | 3 | Faint-source-star planetary microlensing: the discovery of the cold gas-giant planet OGLE-2014-BLG-0676Lb. | RATTENBURY N.J., BENNETT D.P., SUMI T., et al. | ||
2017AJ....154...59B | 325 | X | 8 | 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. | ||
2017AJ....154...68B | 41 | 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. | ||
2017AJ....154..210Z | 122 | 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..223H | 42 | X | 1 | 11 | 13 | OGLE-2016-BLG-0613LABb: a microlensing planet in a binary system. | HAN C., UDALSKI A., GOULD A., et al. | ||
2018AJ....155...20H | 43 | X | 1 | 8 | 22 | OGLE-2017-BLG-0173Lb: low-mass-ratio planet in a "hollywood" microlensing event. | HWANG K.-H., UDALSKI A., SHVARTZVALD Y., et al. | ||
2018ApJ...859...82H | 123 | X | 3 | 7 | 4 | OGLE-2017-BLG-0329L: a microlensing binary characterized with dramatically enhanced precision using data from space-based observations. | HAN C., NOVATI S.C., UDALSKI A., et al. | ||
2018ApJ...860...25W | 42 | X | 1 | 3 | 4 | OGLE-2017-BLG-1130: the first binary gravitational microlens detected from Spitzer only. | WANG T., CALCHI NOVATI S., UDALSKI A., et al. | ||
2018ApJ...863...22J | 123 | X | 3 | 11 | 4 | OGLE-2017-BLG-0537: a microlensing event with a resolvable lens in <=5 years from high-resolution follow-up observations. | JUNG Y.K., HAN C., UDALSKI A., et al. | ||
2018AJ....156..236Z | 41 | X | 1 | 20 | 5 | KMT-2016-BLG-1397b: KMTNET-only discovery of a microlens giant planet. | ZANG W., HWANG K.-H., KIM H.-W., et al. | ||
2018ApJ...867..136H | 41 | X | 1 | 21 | 4 | OGLE-2017-BLG-0039: microlensing event with light from a lens identified from mass measurement. | HAN C., JUNG Y.K., UDALSKI A., et al. | ||
2018AcA....68...43S | 1 | 7 | 10 | OGLE-2017-BLG-0373Lb: a Jovian mass-ratio planet exposes a new accidental microlensing degeneracy. | SKOWRON J., RYU Y.-H., HWANG K.-H., et al. | ||||
2018AJ....156..289B | 126 | X | 3 | 7 | 26 | WFIRST exoplanet mass-measurement method finds a planetary mass of 39 ± 8 M⊕ for OGLE-2012-BLG-0950Lb. | BHATTACHARYA A., BEAULIEU J.-P., BENNETT D.P., et al. | ||
2019AJ....157...23H | 43 | X | 1 | 6 | 8 | KMT-2016-BLG-1107: a new hollywood-planet close/wide degeneracy. | HWANG K.-H., RYU Y.-H., KIM H.-W., et al. | ||
2019AJ....157...72J | 100 | D | C | 2 | 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. | |
2018AcA....68....1U | 374 | X | 9 | 13 | 53 | OGLE-2017-BLG-1434Lb: eighth q<1×10–4 mass-ratio microlens planet confirms turnover in planet mass-ratio function. | UDALSKI A., RYU Y.-H., SAJADIAN S., et al. | ||
2019ApJ...872..175J | 84 | X | 2 | 6 | 2 | OGLE-2016-BLG-0156: microlensing event with pronounced microlens-parallax effects yielding a precise lens mass measurement. | JUNG Y.K., HAN C., BOND I.A., et al. | ||
2019ApJ...873...30S | 42 | 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. | ||
2019AJ....157..121C | 43 | X | 1 | 13 | 16 | Spitzer microlensing parallax for OGLE-2016-BLG-1067: a sub-Jupiter orbiting an M dwarf in the disk. | CALCHI NOVATI S., SUZUKI D., UDALSKI A., et al. | ||
2019AJ....158..151R | 42 | X | 1 | 9 | ~ | KMT-2018-BLG-1990Lb: a nearby Jovian planet from a low-cadence microlensing field. | RYU Y.-H., HWANG K.-H., GOULD A., 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. | ||
2020AJ....159..116Z | 43 | X | 1 | 18 | ~ | OGLE-2015-BLG-1771Lb: a microlens planet orbiting an ultracool dwarf? | ZHANG X., ZANG W., UDALSKI A., et al. | ||
2020AJ....160...64H | 128 | X | 3 | 10 | ~ | KMT-2019-BLG-1339L: an M dwarf with a giant planet or a companion near the Planet/Brown dwarf boundary. | HAN C., KIM D., UDALSKI A., et al. | ||
2020AJ....160..121V | 48 | X | 1 | 6 | 35 | Revisiting MOA 2013-BLG-220L: a solar-type star with a cold super-Jupiter companion. | VANDOROU A., BENNETT D.P., BEAULIEU J.-P., et al. | ||
2020A&A...641A.105H | 43 | X | 1 | 20 | ~ | KMT-2018-BLG-0748Lb: sub-Saturn microlensing planet orbiting an ultracool host. | HAN C., SHIN I.-G., JUNG Y.K., et al. | ||
2020AJ....160..183R | 85 | X | 2 | 23 | ~ | OGLE-2018-BLG-0532Lb: cold Neptune with possible jovian sibling. | RYU Y.-H., UDALSKI A., YEE J.C., et al. | ||
2021AJ....161...54T | 44 | X | 1 | 7 | ~ | MOA-2009-BLG-319Lb: a sub-Saturn planet inside the predicted mass desert. | TERRY S.K., BHATTACHARYA A., BENNETT D.P., et al. | ||
2021A&A...649A..90H | 87 | C | 1 | 22 | ~ | KMT-2018-BLG-1025Lb: microlensing super-Earth planet orbiting a low-mass star. | HAN C., UDALSKI A., LEE C.-U., et al. | ||
2021A&A...650A..89H | 44 | X | 1 | 22 | 12 | Three microlensing planets with no caustic-crossing features. | HAN C., UDALSKI A., KIM D., et al. | ||
2021AJ....162...60B | 44 | X | 1 | 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. | ||
2021A&A...652A.145H | 44 | X | 1 | 15 | ~ | KMT-2018-BLG-1743: planetary microlensing event occurring on two source stars. | HAN C., ALBROW M.D., CHUNG S.-J., 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. | ||
2023A&A...670A.172H | 47 | X | 1 | 23 | 1 | OGLE-2018-BLG-0584 and KMT-2018-BLG-2119: Two microlensing events with two lens masses and two source stars. | HAN C., UDALSKI A., JUNG Y.K., et al. | ||
2023AJ....165..103Z | 47 | X | 1 | 45 | 8 | Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10–4 Planets from the First 4 yr Survey. | ZANG W., JUNG Y.K., YANG H., et al. | ||
2023AJ....166..145G | 47 | X | 1 | 18 | ~ | OGLE-2016-BLG-1195 AO: Lens, Companion to Lens or Source, or None of the Above? | GOULD A., SHVARTZVALD Y., ZHANG J., et al. |