OGLE-2005-BLG-169 , the SIMBAD biblio

OGLE-2005-BLG-169 , the SIMBAD biblio (68 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST18:54:53

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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 11 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 4 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 1 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 39           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 37           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 60     A     X         2 2 1 Characterization of the resonant caustic perturbation. CHUNG S.-J.
2010ApJ...716.1408B 317       D S   X         8 19 52 An efficient method for modeling high-magnification planetary microlensing events. BENNETT D.P.
2010ApJ...720.1073G 170       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 42           X         1 4 35 Second-generation microlensing planet surveys: a realistic simulation. SHVARTZVALD Y. and MAOZ D.
2012NewAR..56...25B 114           X         3 30 1 The first extrasolar planet detected via gravitational microlensing. BOND I.A.
2012MNRAS.426.1496I 206       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 viz 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.
2014A&A...562A.108S viz 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...791...90C 15       D               1 14 15 Synthesizing exoplanet demographics from radial velocity and microlensing surveys. I. Methodology. CLANTON C. and GAUDI B.S.
2014ApJ...794...71H 15       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 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...808..169B 505 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 448 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 40           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 39           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 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.
2016AJ....152..181H viz 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 40           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 318           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 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.
2017AJ....154..210Z viz 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..223H 40           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 42           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 120           X         3 7 4 OGLE-2017-BLG-0329L: a microlensing binary characterized with dramatically enhanced precision using data from space-based observations. HAN C., CALCHI NOVATI S., UDALSKI A., et al.
2018ApJ...860...25W 41           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 120           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 40           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 40           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 123           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 42           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 97       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 365           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 81           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 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.
2019AJ....157..121C 42           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 41           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 viz 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..116Z viz 41           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 123           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 46           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 41           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 82           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 viz 42           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 viz 84             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 42           X         1 22 12 Three microlensing planets with no caustic-crossing features. HAN C., UDALSKI A., KIM D., et al.
2021AJ....162...60B 42           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 42           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 17       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 44           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 viz 44           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 44           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.
2024AJ....168...15B 179           X         4 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.
2024AJ....168..152J 18       D               1 16 ~ KMT-2023-BLG-2669: Ninth Free-floating Planet Candidate with θE Measurements. JUNG Y.K., HWANG K.-H., YANG H., et al.

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