Kepler-730 , the SIMBAD biblio

Kepler-730 , the SIMBAD biblio (74 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST06:53:29

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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
2011ApJ...736...19B viz 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 viz 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 viz 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.
2011ApJS..197...12D 15       D               1 124 184 Lack of inflated radii for Kepler giant planet candidates receiving modest stellar irradiation. DEMORY B.-O. and SEAGER S.
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.
2012ApJ...752...53L 15       D               1 320 18 Debris disks in Kepler exoplanet systems. LAWLER S.M. and GLADMAN B.
2012ApJ...752...72D viz 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 viz 15       D               1 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 viz 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.
2013ApJ...775L..11M viz 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 viz 15       D               1 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.
2014ApJS..210...19B viz 15       D               1 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.
2014AJ....147..119C viz 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.
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.
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.
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 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.
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.
2019ApJ...870L..17C 1219 T   A D     X C       29 7 8
Kepler-730: a hot Jupiter system with a close-in, transiting, Earth-sized planet. 		CANAS C.I., WANG S., MAHADEVAN S., et al.
2019A&A...624A..46L 81           X         2 9 4 Co-orbital exoplanets from close-period candidates: the TOI-178 case. LELEU A., LILLO-BOX J., SESTOVIC M., et al.
2019ApJ...877L..29C 42           X         1 6 6 TOI-150: a transiting hot Jupiter in the TESS southern CVZ. CANAS C.I., STEFANSSON G., MONSON A.J., et al.
2019A&A...631A.152A 16       D               2 121 ~ Dusty phenomena in the vicinity of giant exoplanets. ARKHYPOV O.V., KHODACHENKO M.L. and HANSLMEIER A.
2020ApJ...890...23L viz 16       D               2 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...892L...7H 210           X         5 9 39 TESS spots a hot Jupiter with an inner transiting Neptune. HUANG C.X., QUINN S.N., VANDERBURG A., et al.
2020A&A...636A..98C viz 42           X         1 14 27 TraMoS. V. Updated ephemeris and multi-epoch monitoring of the hot Jupiters WASP-18Ab, WASP-19b, and WASP-77Ab. CORTES-ZULETA P., ROJO P., WANG S., et al.
2020PASP..132a4401M 41           X         1 9 ~ K2 looks toward WASP-28 and WASP-151. MOCNIK T., HELLIER C. and ANDERSON D.R.
2020AJ....160..108B viz 16       D               2 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.
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.
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.
2021MNRAS.505.2500P 1129     A D     X C F     26 25 12 In situ formation of hot Jupiters with companion super-Earths. POON S.T.S., NELSON R.P. and COLEMAN G.A.L.
2021ApJS..255...15W 42           X         1 82 15 Transiting exoplanet monitoring project (TEMP). VI. The homogeneous refinement of system parameters for 39 transiting hot Jupiters with 127 new light curves. WANG X.-Y., WANG Y.-H., WANG S., et al.
2021AJ....162..263H viz 84           X         2 346 17 A uniform search for nearby planetary companions to hot Jupiters in TESS data reveals hot Jupiters are still lonely. HORD B.J., COLON K.D., KOSTOV V., et al.
2021A&A...656A..88M viz 42           X         1 7 ~ Revisiting TrES-5 b: departure from a linear ephemeris instead of short-period transit timing variation. MACIEJEWSKI G., FERNANDEZ M., ACEITUNO F., et al.
2022AJ....163..128W viz 17       D               1 1570 6 The influence of 10 unique chemical elements in shaping the distribution of Kepler planets. WILSON R.F., CANAS C.I., MAJEWSKI S.R., et al.
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.
2022ApJ...926L...8W viz 44           X         1 15 20 The Aligned Orbit of WASP-148b, the Only Known Hot Jupiter with a nearby Warm Jupiter Companion, from NEID and HIRES. WANG X.-Y., RICE M., WANG S., 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.
2022AJ....164...13H 213           X C       4 11 10 The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 b. HORD B.J., COLON K.D., BERGER T.A., et al.
2023AJ....165..171W 44           X         1 42 7 Evidence for Hidden Nearby Companions to Hot Jupiters. WU D.-H., RICE M. and WANG S.
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.
2023A&A...673A..42N viz 44           X         1 15 2 A new dynamical modeling of the WASP-47 system with CHEOPS observations. NASCIMBENI V., BORSATO L., ZINGALES T., et al.
2023MNRAS.524.1113S 17       D               2 85 ~ TESS spots a mini- interior to a hot saturn in the TOI-2000 system. SHA L., VANDERBURG A.M., HUANG C.X., et al.
2023A&A...675A.115K viz 87           X         2 24 ~ TOI-1130: A photodynamical analysis of a hot Jupiter in resonance with an inner low-mass planet. KORTH J., GANDOLFI D., SUBJAK J., et al.
2023MNRAS.525L..43M viz 44           X         1 13 ~ A hot super-Earth planet in the WASP-84 planetary system. MACIEJEWSKI G., GOLONKA J., LOBODA W., et al.
2023ApJ...956L..29Z 44           X         1 5 ~ Hot Jupiters Have Giant Companions: Evidence for Coplanar High-eccentricity Migration. ZINK J.K. and HOWARD A.W.
2023AJ....166..267W 44           X         1 4 ~ Hot Jupiters from Disruption of Resonant Chains in Postdisk Evolution. WU D.-H. and HE Y.
2024AJ....167...55H viz 18       D               2 586 ~ Kepler-discovered Multiple-planet Systems near Period Ratios Suggestive of Mean-motion Resonances Are Young. HAMER J.H. and SCHLAUFMAN K.C.
2024A&A...682A.129M viz 179     A D     X         5 21 ~ The GAPS programme at TNG XLIX. TOI-5398, the youngest compact multi-planet system composed of an inner sub-Neptune and an outer warm Saturn. MANTOVAN G., MALAVOLTA L., DESIDERA S., et al.
2024A&A...684L..17M viz 45           X         1 25 ~ Orbital obliquity of the young planet TOI-5398 b and the evolutionary history of the system. MANTOVAN G., MALAVOLTA L., LOCCI D., et al.
2024ApJ...971L..28K 45           X         1 13 ~ TOI-1408: Discovery and Photodynamical Modeling of a Small Inner Companion to a Hot Jupiter Revealed by Transit Timing Variations. KORTH J., CHATURVEDI P., PARVIAINEN H., 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.
2024ApJ...973..108B 63       D     X         2 7 ~ Dynamical and Secular Stability of Mutually Inclined Planetary Systems. BHASKAR H.G. and PERETS H.
2024A&A...689A..52B viz 45           X         1 21 ~ Characterisation of the warm-Jupiter TOI-1130 system with CHEOPS and a photo-dynamical approach. BORSATO L., DEGEN D., LELEU A., 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.
2024A&A...691A..53S viz 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.254H viz 134           X   F     2 20 ~ Hints of a close outer companion to the ultra-hot Jupiter TOI-2109 b. HARRE J.-V., SMITH A.M.S., BARROS S.C.C., et al.
2025AJ....169...91M 47           X         1 32 ~ Eight New Candidate Multiplanet Systems among TESS Objects of Interest. MUNAVAR HUSSAIN M.J. and KUNIMOTO M.
2025A&A...693A.144G viz 47           X         1 19 ~ Discovery of a cold giant planet and mass measurement of a hot super-Earth in the multi-planetary system WASP-132. GRIEVES N., BOUCHY F., ARMSTRONG D.J., et al.
2025A&A...693A.235S 47           X         1 35 ~ TOI-2458 b: A mini-Neptune consistent with in situ hot Jupiter formation. SUBJAK J., GANDOLFI D., GOFFO E., et al.
2025AJ....169..149H 93               F     1 222 ~ Architecture Classification for Extrasolar Planetary Systems. HOWE A.R., BECKER J.C., STARK C.C., et al.
2025AJ....169..189R 93           X         2 37 ~ Evidence for Primordial Alignment II: Insights from Stellar Obliquity Measurements for Hot Jupiters in Compact Multiplanet Systems. RADZOM B.T., DONG J., RICE M., et al.
2025ApJ...981..106M 47           X         1 12 ~ A Planet Candidate Orbiting near the Hot Jupiter TOI-2818 b Inferred through Transit Timing. McKEE B.J., MONTET B.T., YEE S.W., et al.
2025ApJ...982L..15W 47           X         1 14 ~ Formation of Ultra-short-period Planets in Hot Jupiter Systems: Application to WASP-47. WANG S., PAN M., DONG Y., et al.
2025ApJ...987...30M 159       D     X C       3 23 ~ Three-dimensional Orbital Architectures and Detectability of Adjacent Companions to Hot Jupiters. MacLEAN T. and BECKER J.
2025A&A...699A.100D viz 19       D               1 2580 ~ The Gaia spectroscopic catalogue of exoplanets and host stars. DE LAVERNY P., LIGI R., CRIDA A., et al.
2025ApJ...991..206Z 159       D     X         4 31 ~ The Formation of Ultra-short-period Planets under the Influence of the Nearby Planetary Companions. ZHU J., WANG S., JI J., et al.

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