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| Kepler-289 , the SIMBAD biblio (94 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST07:06:08 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2011ApJ...736...19B |
15 | D | 1 | 1507 | 867 | Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data. | BORUCKI W.J., KOCH D.G., BASRI G., et al. | ||
|
2011ApJ...738..170M |
15 | D | 1 | 997 | 230 | On the low false positive probabilities of Kepler planet candidates. | MORTON T.D. and JOHNSON J.A. | ||
|
2011ApJS..197....2F |
15 | D | 1 | 980 | 66 | Transit timing observations from Kepler. I. Statistical analysis of the first four months. | FORD E.B., ROWE J.F., FABRYCKY D.C., et al. | ||
|
2012ApJ...752...72D |
15 | D | 1 | 229 | 7 | A correlation between the eclipse depths of Kepler gas giant candidates and the metallicities of their parent stars. | DODSON-ROBINSON S.E. | ||
|
2012ApJ...756..185F |
15 | D | 2 | 1856 | 44 | Transit timing observations from Kepler. V. Transit timing variation candidates in the first sixteen months from polynomial models. | FORD E.B., RAGOZZINE D., ROWE J.F., et al. | ||
|
2012ApJ...756..186S |
15 | D | 1 | 811 | 35 | Transit timing observations from Kepler. VI. Potentially interesting candidate systems from fourier-based statistical tests. | STEFFEN J.H., FORD E.B., ROWE J.F., et al. | ||
|
2013ApJS..204...24B |
15 | D | 1 | 3274 | 922 | Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data. | BATALHA N.M., ROWE J.F., BRYSON S.T., et al. | ||
|
2013ApJ...774L..12S |
15 | D | 1 | 469 | 25 | A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42. | STEFFEN J.H. and FARR W.M. | ||
|
2013ApJ...775L..11M |
15 | D | 1 | 2010 | 189 | Stellar rotation periods of the Kepler Objects of Interest: a dearth of close-in planets around fast rotators. | McQUILLAN A., MAZEH T. and AIGRAIN S. | ||
|
2013ApJS..208...16M |
15 | D | 2 | 1518 | 139 | Transit timing observations from Kepler. VIII. Catalog of transit timing measurements of the first twelve quarters. | MAZEH T., NACHMANI G., HOLCZER T., et al. | ||
|
2013MNRAS.436.1883W |
15 | D | 1 | 961 | 136 | Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. | WALKOWICZ L.M. and BASRI G.S. | ||
|
2013A&A...560A...4R |
15 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
|
2014ApJS..210...19B |
15 | D | 2 | 5860 | 211 | Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). | BURKE C.J., BRYSON S.T., MULLALLY F., et al. | ||
|
2014ApJ...784...45R |
15 | D | 1 | 1691 | 388 | Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems. | ROWE J.F., BRYSON S.T., MARCY G.W., et al. | ||
|
2014AJ....147..119C |
15 | D | 1 | 8013 | 91 | Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. | COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al. | ||
|
2014A&A...566A.103L |
15 | D | 4 | 359 | 102 | High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. | LILLO-BOX J., BARRADO D. and BOUY H. | ||
|
2014ApJ...795..167S |
1045 | T A | D | S X C | 25 | 30 | 33 |
Planet hunters. VII. Discovery of a new low-mass, low-density planet ( PH3 c) orbiting Kepler-289 with mass measurements of two additional planets ( PH3 b and d). |
SCHMITT J.R., AGOL E., DECK K.M., et al. |
|
2015ApJ...801....3M |
16 | D | 1 | 3357 | 109 | Photometric amplitude distribution of stellar rotation of KOIs–Indication for spin-orbit alignment of cool stars and high obliquity for hot stars. | MAZEH T., PERETS H.B., McQUILLAN A., et al. | ||
|
2015ApJS..217...16R |
16 | D | 1 | 8625 | 149 | Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). | ROWE J.F., COUGHLIN J.L., ANTOCI V., et al. | ||
| 2015ApJ...802..116D | 274 | S X | 6 | 13 | 44 | Measurement of planet masses with transit timing variations due to synodic ''chopping'' effects. | DECK K.M. and AGOL E. | ||
|
2015ApJ...806..248W |
16 | D | 2 | 143 | 44 | Influence of stellar multiplicity on planet formation. III. Adaptive optics imaging of Kepler stars with gas giant planets. | WANG J., FISCHER D.A., HORCH E.P., et al. | ||
|
2015ApJ...807..170H |
16 | D | 2 | 2117 | 10 | Time variation of Kepler transits induced by stellar Spots–A way to distinguish between prograde and retrograde motion. II. Application to KOIs. | HOLCZER T., SHPORER A., MAZEH T., et al. | ||
|
2015ApJ...813..100O |
16 | D | 1 | 327 | 7 | Deep GALEX UV survey of the Kepler field. I. Point source catalog. | OLMEDO M., LLOYD J., MAMAJEK E.E., et al. | ||
|
2015ApJ...814..130M |
16 | D | 2 | 2846 | 162 | An increase in the mass of planetary systems around lower-mass stars. | MULDERS G.D., PASCUCCI I. and APAI D. | ||
|
2016A&A...587A..64S |
79 | C | 1 | 179 | 172 | SOPHIE velocimetry of Kepler transit candidates. XVII. The physical properties of giant exoplanets within 400 days of period. | SANTERNE A., MOUTOU C., TSANTAKI M., et al. | ||
|
2016ApJ...822...86M |
16 | D | 1 | 6130 | 337 | False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. | MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al. | ||
| 2016ApJ...825...98H | 16 | D | 1 | 166 | 128 | Warm jupiters are less lonely than hot jupiters: close neighbors. | HUANG C., WU Y. and TRIAUD A.H.M.J. | ||
|
2016ApJS..225....9H |
16 | D | 2 | 2132 | 124 | Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. | HOLCZER T., MAZEH T., NACHMANI G., et al. | ||
|
2016ApJS..225...32B |
16 | D | 1 | 1473 | 266 | Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars. | BREWER J.M., FISCHER D.A., VALENTI J.A., et al. | ||
|
2017AJ....153...71F |
16 | D | 1 | 3575 | 164 | The Kepler follow-up observation program. I. A catalog of companions to Kepler stars from high-resolution imaging. | FURLAN E., CIARDI D.R., EVERETT M.E., et al. | ||
|
2017MNRAS.465.2634A |
16 | D | 2 | 5400 | 21 | Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. | ARMSTRONG D.J., POLLACCO D. and SANTERNE A. | ||
|
2017AJ....154..107P |
16 | D | 1 | 1306 | 226 | The California-Kepler Survey. I. High-resolution spectroscopy of 1305 stars hosting Kepler transiting planets. | PETIGURA E.A., HOWARD A.W., MARCY G.W., et al. | ||
|
2017AJ....154..108J |
16 | D | 1 | 3237 | 137 | The California-Kepler Survey. II. Precise physical properties of 2025 Kepler planets and their host stars. | JOHNSON J.A., PETIGURA E.A., FULTON B.J., et al. | ||
|
2017A&A...603A..30S |
16 | D | 6 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
|
2017A&A...605A..72L |
95 | D | C | 4 | 130 | 88 | AMD-stability and the classification of planetary systems. | LASKAR J. and PETIT A.C. | |
| 2017AJ....154..270W | 16 | D | 2 | 70 | 21 | Constraints on the obliquities of Kepler planet-hosting stars. | WINN J.N., PETIGURA E.A., MORTON T.D., et al. | ||
|
2018ApJS..234....9O |
16 | D | 1 | 436 | 14 | A spectral approach to transit timing variations. | OFIR A., XIE J.-W., JIANG C.-F., et al. | ||
| 2017MNRAS.472.3692A | 119 | X F | 2 | 25 | 17 | Moderately eccentric warm Jupiters from secular interactions with exterior companions. | ANDERSON K.R. and LAI D. | ||
|
2018ApJ...855..115B |
16 | D | 1 | 1305 | 5 | Identifying young Kepler planet host stars from Keck-HIRES spectra of lithium. | BERGER T.A., HOWARD A.W. and BOESGAARD A.M. | ||
|
2018MNRAS.474.2094A |
16 | D | 1 | 1073 | 143 | Inferring probabilistic stellar rotation periods using Gaussian processes. | ANGUS R., MORTON T., AIGRAIN S., et al. | ||
|
2018AJ....155..161Z |
80 | X | 2 | 1274 | 24 | Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. | ZIEGLER C., LAW N.M., BARANEC C., et al. | ||
|
2018ApJ...861..149F |
16 | D | 1 | 2261 | 6 | The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. | FURLAN E., CIARDI D.R., COCHRAN W.D., et al. | ||
| 2018AJ....156...50G | 16 | D | 1 | 54 | ~ | The best planets to harbor detectable exomoons. | GUIMARAES A. and VALIO A. | ||
| 2018AJ....156...96W | 40 | X | 1 | 31 | 3 | TTV-determined masses for warm Jupiters and their close planetary companions. | WU D.-H., WANG S., ZHOU J.-L., et al. | ||
|
2018ApJS..237...38B |
16 | D | 1 | 1111 | 42 | Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. | BREWER J.M. and FISCHER D.A. | ||
|
2018ApJ...866...99B |
16 | D | 1 | 7129 | 233 | Revised radii of Kepler stars and planet's using Gaia Data Release 2. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
| 2018A&A...618A.116P | 40 | X | 1 | 22 | 10 | Mass determination of the 1:3:5 near-resonant planets transiting GJ 9827 (K2-135). | PRIETO-ARRANZ J., PALLE E., GANDOLFI D., et al. | ||
|
2018AJ....156..292T |
16 | D | 1 | 647 | 8 | The effects of stellar companions on the observed transiting exoplanet radius distribution. | TESKE J.K., CIARDI D.R., HOWELL S.B., et al. | ||
|
2019AJ....157..143B |
16 | D | 1 | 423 | 5 | Re-evaluating small long-period confirmed planets from Kepler. | BURKE C.J., MULLALLY F., THOMPSON S.E., et al. | ||
|
2019ApJ...875...29M |
16 | D | 1 | 2918 | 72 | A spectroscopic analysis of the California-Kepler Survey sample. I. Stellar parameters, planetary radii, and a slope in the radius gap. | MARTINEZ C.F., CUNHA K., GHEZZI L., et al. | ||
| 2019A&A...625A...7P | 162 | X C | 3 | 18 | ~ | The role of dissipative evolution for three-planet, near-resonant extrasolar systems. | PICHIERRI G., BATYGIN K. and MORBIDELLI A. | ||
|
2020ApJ...890...23L |
16 | D | 4 | 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. | ||
|
2020ApJ...893...67M |
16 | D | 1 | 533 | 31 | A relationship between stellar age and spot coverage. | MORRIS B.M. | ||
| 2020AJ....159..207B | 16 | D | 1 | 150 | ~ | Transit duration variations in multiplanet systems. | BOLEY A.C., VAN LAERHOVEN C. and GRANADOS CONTRERAS A.P. | ||
|
2020AJ....160..108B |
16 | D | 3 | 6855 | 109 | The Gaia-Kepler stellar properties catalog. II. Planet radius demographics as a function of stellar mass and age. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
|
2020A&A...640A..48L |
41 | X | 1 | 27 | 17 | Masses for the seven planets in K2-32 and K2-233. Four diverse planets in resonant chain and the first young rocky worlds. | LILLO-BOX J., LOPEZ T.A., SANTERNE A., et al. | ||
| 2020MNRAS.499.1854M | 58 | D | X | 2 | 31 | ~ | Understanding the origin of white dwarf atmospheric pollution by dynamical simulations based on detected three-planet systems. | MALDONADO R.F., VILLAVER E., MUSTILL A.J., et al. | |
|
2021ApJ...909..115C |
17 | D | 1 | 2176 | 13 | Planets Across Space and Time (PAST). I. Characterizing the memberships of Galactic components and stellar ages: revisiting the kinematic methods and applying to planet host stars. | CHEN D.-C., XIE J.-W., ZHOU J.-L., et al. | ||
| 2021MNRAS.503.4092B | 17 | D | 2 | 124 | ~ | Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data. | BATTLEY M.P., KUNIMOTO M., ARMSTRONG D.J., et al. | ||
|
2021AJ....161..246J |
393 | D | X C | 9 | 204 | 12 | Following up the Kepler field: masses of targets for transit timing and atmospheric characterization. | JONTOF-HUTTER D., WOLFGANG A., FORD E.B., et al. | |
| 2021A&A...649L...5B | 42 | X | 1 | 41 | 19 | Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line. | BITSCH B., RAYMOND S.N., BUCHHAVE L.A., et al. | ||
| 2021MNRAS.504.5327A | 17 | D | 1 | 7000 | 19 | Exoplanet validation with machine learning: 50 new validated Kepler planets. | ARMSTRONG D.J., GAMPER J. and DAMOULAS T. | ||
|
2021ApJS..255...17S |
17 | D | 1 | 39591 | 57 | Surface rotation and photometric activity for Kepler targets. II. G and F main-sequence stars and cool subgiant stars. | SANTOS A.R.G., BRETON S.N., MATHUR S., et al. | ||
|
2021AJ....162...98B |
17 | D | 1 | 2175 | ~ | Seeking echoes of circumstellar disks in Kepler light curves. | BROMLEY B.C., LEONARD A., QUINTANILLA A., et al. | ||
|
2021ApJ...919..138T |
17 | D | 1 | 531 | 12 | Further evidence for tidal spin-up of hot Jupiter host stars. | TEJADA AREVALO R.A., WINN J.N. and ANDERSON K.R. | ||
|
2021ApJ...920...19G |
17 | D | 1 | 807 | 5 | A spectroscopic analysis of the California-Kepler Survey sample. II. Correlations of stellar metallicities with planetary architectures. | GHEZZI L., MARTINEZ C.F., WILSON R.F., et al. | ||
|
2021ApJ...921...24S |
17 | D | 4 | 328 | 1 | The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. | SCHLAUFMAN K.C. and HALPERN N.D. | ||
| 2022A&A...658A.107O | 145 | D | X F | 3 | 48 | 4 | The similarity of multi-planet systems. | OTEGI J.F., HELLED R. and BOUCHY F. | |
|
2022AJ....163..179P |
17 | D | 1 | 2962 | 39 | The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age. | PETIGURA E.A., ROGERS J.G., ISAACSON H., et al. | ||
| 2022AJ....163..225T | 17 | D | 1 | 13 | 5 | TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration. | TRAN Q.H., BOWLER B.P., ENDL M., et al. | ||
| 2022AJ....164...42J | 383 | A | D | X C | 9 | 79 | 3 | TESS Observations of Kepler Systems with Transit Timing Variations. | JONTOF-HUTTER D., DALBA P.A. and LIVINGSTON J.H. |
|
2022ApJS..261...26S |
17 | D | 4 | 1893 | 2 | Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. | SU T., ZHANG L.-Y., LONG L., et al. | ||
|
2022A&A...663A...4S |
17 | D | 1 | 14206 | 7 | Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. | SOUBIRAN C., BROUILLET N. and CASAMIQUELA L. | ||
| 2022ApJ...937L..41C | 85 | F | 1 | 51 | 5 | Life on Exoplanets in the Habitable Zone of M Dwarfs? | CHILDS A.C., MARTIN R.G. and LIVIO M. | ||
|
2023MNRAS.518.2068G |
17 | D | 1 | 179 | 2 | Chaos in multiplanetary extrasolar systems. | GAJDOS P. and VANKO M. | ||
|
2023AJ....165...48G |
1288 | T A | X C | 28 | 4 | 3 |
Constraining the Densities of the Three Kepler-289 Planets with Transit Timing Variations. |
GREKLEK-MCKEON M., KNUTSON H.A., VISSAPRAGADA S., et al. | |
|
2023ApJS..264...17Z |
17 | D | 3 | 31380 | 1 | Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. | ZHANG L.-Y., SU T., MISRA P., et al. | ||
| 2023AJ....165..217M | 44 | X | 1 | 6 | ~ | Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star. | MANN C., LAFRENIERE D., DRAGOMIR D., et al. | ||
|
2023NatAs...7..900C |
17 | D | 1 | 1054 | ~ | On the behaviour of spin-orbit connection of exoplanets. | CANTO MARTINS B.L., MESSIAS Y.S., ARRUDA GONCALVES M.I., et al. | ||
| 2024AJ....167...48M | 108 | D | C | 7 | 72 | ~ | Signs of Similar Stellar Obliquity Distributions for Hot and Warm Jupiters Orbiting Cool Stars. | MORGAN M., BOWLER B.P., TRAN Q.H., et al. | |
|
2024AJ....167...55H |
18 | D | 6 | 586 | ~ | Kepler-discovered Multiple-planet Systems near Period Ratios Suggestive of Mean-motion Resonances Are Young. | HAMER J.H. and SCHLAUFMAN K.C. | ||
|
2024AJ....167..271V |
18 | D | 2 | 165 | ~ | Differences between Stable and Unstable Architectures of Compact Planetary Systems. | VOLK K. and MALHOTRA R. | ||
|
2024MNRAS.533.1290S |
18 | D | 1 | 7737 | ~ | The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages. | SEE V., LU Y., AMARD L., et al. | ||
|
2024AJ....168..109S |
18 | D | 2 | 702 | ~ | Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution. | SCHMIDT S.P., SCHLAUFMAN K.C. and HAMER J.H. | ||
| 2024ApJ...973L...4R | 90 | F | 1 | 49 | ~ | The Distribution of Planet Radius in Kepler Multiplanet Systems Depends on Gap Complexity. | RICE D.R., STEFFEN J.H. and VAZAN A. | ||
|
2024AJ....168..177C |
18 | D | 1 | 260 | ~ | Detecting Exoplanet Transits with the Next Generation of X-Ray Telescopes. | CILLEY R., KING G.W. and CORRALES L. | ||
|
2024A&A...689A.250C |
18 | D | 3 | 3075 | ~ | Mapping the exo-Neptunian landscape A ridge between the desert and savanna. | CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al. | ||
|
2024A&A...691A..53S |
18 | D | 1 | 4078 | ~ | SWEET-Cat: A view on the planetary mass-radius relation. | SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al. | ||
| 2024A&A...692A.122M | 45 | X | 1 | 45 | ~ | Diversities and similarities exhibited by multi-planetary systems and their architectures I. Orbital spacings. | MURESAN A., PERSSON C.M. and FRIDLUND M. | ||
|
2025AJ....169...90O |
205 | D | S X | 4 | 194 | ~ | Planetary Mass Determinations from a Simplified Photodynamical Model-Application to the Complete Kepler Dataset. | OFIR A., YOFFE G. and AHARONSON O. | |
| 2025ApJ...978...18F | 19 | D | 1 | 41 | ~ | More Likely Than You Think: Inclination-driving Secular Resonances Are Common in Known Exoplanet Systems. | FARIDANI T.H., NAOZ S., LI G., et al. | ||
| 2025ApJ...978...46K | 19 | D | 1 | 49 | ~ | Separating Super-puffs versus Hot Jupiters among Young Puffy Planets. | KARALIS A., LEE E.J. and THORNGREN D.P. | ||
| 2025AJ....169..149H | 187 | X F | 3 | 222 | ~ | Architecture Classification for Extrasolar Planetary Systems. | HOWE A.R., BECKER J.C., STARK C.C., et al. | ||
| 2026AJ....171...97G | 50 | X | 1 | 10 | ~ | Validation of a Third Earth-sized Planet in the TOI-2267 Binary System. | GREKLEK-MCKEON M., GOMEZ BARRIENTOS J., KNUTSON H.A., et al. |