KOI-3444 , the SIMBAD biblio

KOI-3444 , the SIMBAD biblio (45 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST05:16:00


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Title First 3 Authors
2012ApJS..199...24T viz 15       D               1 5394 66 Detection of potential transit signals in the first three quarters of Kepler mission data. TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al.
2014MNRAS.437.3473A viz 15       D               1 2614 45 A catalogue of temperatures for Kepler eclipsing binary stars. ARMSTRONG D.J., GOMEZ MAQUEO CHEW Y., FAEDI F., et al.
2014AJ....147..119C viz 15       D               2 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.
2014ApJS..213....5M viz 15       D               1 111 51 Characterizing the cool KOIs. VI. H- and K-band spectra of Kepler M dwarf planet-candidate hosts. MUIRHEAD P.S., BECKER J., FEIDEN G.A., et al.
2014A&A...566A.103L viz 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.
2015ApJS..217...16R viz 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.
2015MNRAS.448.3608B viz 39           X         1 156 6 Using the inclinations of Kepler systems to prioritize new Titius-Bode-based exoplanet predictions. BOVAIRD T., LINEWEAVER C.H. and JACOBSEN S.K.
2015ApJS..218...26S viz 55       D     X         2 275 13 Characterizing the cool KOIs. VIII. Parameters of the planets orbiting Kepler's coolest dwarfs. SWIFT J.J., MONTET B.T., VANDERBURG A., et al.
2015ApJ...806..248W viz 94       D     X         3 143 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 viz 16       D               1 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...807...45D viz 94       D     X         3 2707 726 The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity. DRESSING C.D. and CHARBONNEAU D.
2015ApJ...814..130M viz 16       D               3 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2016AJ....151...68K viz 16       D               1 2915 316 Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. KIRK B., CONROY K., PRSA A., et al.
2016ApJ...821...47B viz 16       D               1 217 14 Efficient geometric probabilities of multi-transiting exoplanetary systems from CORBITS. BRAKENSIEK J. and RAGOZZINE D.
2016ApJ...822...86M viz 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.
2016MNRAS.457.2877G viz 94       D     X         3 4245 141 They are small worlds after all: revised properties of Kepler M dwarf stars and their planets. GAIDOS E., MANN A.W., KRAUS A.L., et al.
2016AJ....152....8K viz 16       D               1 389 203 The impact of stellar multiplicity on planetary systems. I. The ruinous influence of close binary companions. KRAUS A.L., IRELAND M.J., HUBER D., et al.
2016AJ....152...18B viz 16       D               3 1167 34 Robo-AO Kepler planetary candidate survey. II. Adaptive optics imaging of 969 Kepler exoplanet candidate host stars. BARANEC C., ZIEGLER C., LAW N.M., et al.
2016ApJS..225....9H viz 16       D               1 2132 124 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2017AJ....153...71F viz 56       D     X         2 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.
2017AJ....153..117H viz 135       D     X C       3 170 51 Assessing the effect of stellar companions from high-resolution imaging of Kepler Objects of Interest. HIRSCH L.A., CIARDI D.R., HOWARD A.W., et al.
2017MNRAS.465.2634A viz 16       D               4 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..250L viz 16       D               1 2281 72 Tidal synchronization and differential rotation of Kepler eclipsing binaries. LURIE J.C., VYHMEISTER K., HAWLEY S.L., et al.
2018ApJ...861..149F viz 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.
2018ApJ...866...99B viz 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.
2019A&A...630A.106G viz 16       D               1 308 39 Systematic search for stellar pulsators in the eclipsing binaries observed by Kepler. GAULME P. and GUZIK J.A.
2020ApJ...890...23L viz 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...892...31B viz 16       D               1 14873 35 Temperatures and metallicities of M dwarfs in the APOGEE Survey. BIRKY J., HOGG D.W., MANN A.W., et al.
2020ApJ...892...58H 222       D     X C       5 16 ~ M-dwarf eclipsing binaries with flare activity. HUANG L.-C., IP W.-H., LIN C.-L., et al.
2020AJ....160..120J viz 16       D               1 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2020AJ....160..253L viz 16       D               1 3432 12 An increase in small-planet occurrence with metallicity for late-type dwarf stars in the Kepler field and its implications for planet formation. LU C.X., SCHLAUFMAN K.C. and CHENG S.
2021AJ....161..246J viz 42           X         1 204 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.
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.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022MNRAS.512..648D 341           X         8 40 9 Orbital architectures of planet-hosting binaries - II. Low mutual inclinations between planetary and stellar orbits. DUPUY T.J., KRAUS A.L., KRATTER K.M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2023ApJS..264...17Z viz 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.
2023ApJS..265...50C viz 17       D               1 2291 ~ Characterization of Low-mass Companions to Kepler Objects of Interest Observed with APOGEE-N. CANAS C.I., BENDER C.F., MAHADEVAN S., et al.
2024AJ....167...55H viz 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.
2024A&A...685A..62I viz 18       D               1 2906 ~ Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability. IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al.
2024AJ....168..109S viz 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.
2024AJ....168..129S viz 18       D               1 350 ~ Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation. SULLIVAN K., KRAUS A.L., BERGER T.A., et al.
2024MNRAS.534..575E 735       D     X C       16 51 ~ Orbital architectures of planet-hosting binaries - III. Testing mutual inclinations of stellar and planetary orbits in triple-star systems. EVANS E.L., DUPUY T.J., SULLIVAN K., et al.
2024A&A...689A.250C viz 18       D               2 3075 ~ Mapping the exo-Neptunian landscape A ridge between the desert and savanna. CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al.
2026AJ....171..110B 20       D               1 41 ~ Modeling the Impact of Unresolved Stellar Companions on Detection Sensitivity in Kepler's Small-planet Occurrence Rates. BERGSTEN G.J., CIARDI D.R., CHRISTIANSEN J.L., et al.

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