KOI-3349 , the SIMBAD biblio

KOI-3349 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST18:23:59


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Title First 3 Authors
2013ApJ...776...10W 16       D               1 50 35 Planet hunters. V. A confirmed jupiter-size planet in the habitable zone and 42 planet candidates from the Kepler archive data. WANG J., FISCHER D.A., BARCLAY T., et al.
2014AJ....147..119C viz 16       D               1 8010 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.
2015ApJ...798...66D 40           X         1 296 60 The photoeccentric effect and proto-hot jupiters. III. A paucity of proto-hot jupiters on super-eccentric orbits. DAWSON R.I., MURRAY-CLAY R.A. and JOHNSON J.A.
2015ApJ...801....3M viz 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 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.
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...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2015ApJ...814..130M viz 16       D               1 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2015ApJ...815..127W 373       D     X         10 59 64 Planet hunters. VIII. Characterization of 41 long-period exoplanet candidates from Kepler archival data. WANG J., FISCHER D.A., BARCLAY T., et al.
2016ApJ...822....2U 177       D S     C       6 38 26 Transiting planet candidates beyond the snow line detected by visual inspection of 7557 Kepler Objects of Interest. UEHARA S., KAWAHARA H., MASUDA K., et al.
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.
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...66Z viz 16       D               1 1663 45 Robo-AO Kepler Planetary Candidate Survey. III. Adaptive optics imaging of 1629 Kepler exoplanet candidate host stars. ZIEGLER C., LAW N.M., MORTON T., et al.
2017AJ....153...71F viz 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.
2017AJ....153..117H viz 57       D     X         2 170 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               1 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.
2017A&A...603A..30S viz 16       D               2 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., 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.
2019AJ....157..218K viz 100       D     X         3 142 26 Transiting planets near the snow line from Kepler. I. Catalog. KAWAHARA H. and MASUDA K.
2020AJ....159...38M 231       D     X         6 23 34 Mutual orbital inclinations between cold Jupiters and inner super-Earths. MASUDA K., WINN J.N. and KAWAHARA H.
2020ApJ...890...23L viz 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....160..108B viz 17       D               1 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.

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