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Kepler-30d , the SIMBAD biblio (63 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.06.09CEST10:11:44 |
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...736L..25K ![]() |
15 | D | 1 | 92 | 58 | Exploring the habitable zone for Kepler planetary candidates. | KALTENEGGER L. and SASSELOV D. | ||
2011ApJS..197...12D | 15 | D | 1 | 124 | 110 | Lack of inflated radii for Kepler giant planet candidates receiving modest stellar irradiation. | DEMORY B.-O. and SEAGER S. | ||
2011A&A...536L...9T ![]() |
10 | 9 | Detection of transit timing variations in excess of one hour in the Kepler multi-planet candidate system KOI 806 with the GTC. | TINGLEY B., PALLE E., PARVIAINEN H., et al. | |||||
2012ApJ...750..114F ![]() |
1 | 50 | 139 | Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models. | FABRYCKY D.C., FORD E.B., STEFFEN J.H., et al. | ||||
2012Natur.487..449S | 15 | 4 | 120 | Alignment of the stellar spin with the orbits of a three-planet system. | SANCHIS-OJEDA R., FABRYCKY D.C., WINN J.N., et al. | ||||
2012ApJ...756..185F ![]() |
172 | D | X C | 4 | 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. | |
2011PASP..123..412W ![]() |
15 | D | 1 | 2897 | 358 | The Exoplanet Orbit Database. | WRIGHT J.T., KAKHOURI O., MARCY G.W., et al. | ||
2013ApJ...764...18L ![]() |
16 | D | 1 | 174 | 6 | Pulsation frequencies and modes of giant exoplanets. | LE BIHAN B. and BURROWS A. | ||
2013ApJS..204...24B ![]() |
16 | D | 1 | 3274 | 779 | 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...767...94S ![]() |
16 | D | 1 | 267 | 21 | A 1.1-1.9 GHz SETI survey of the Kepler field. I. A search for narrow-band emission from select targets. | SIEMION A.P.V., DEMOREST P., KORPELA E., et al. | ||
2013A&A...552A.119S ![]() |
16 | D | 1 | 1487 | 42 | Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. | SAUR J., GRAMBUSCH T., DULING S., et al. | ||
2013ApJ...769L...9B | 86 | S | 1 | 1 | 14 | Mass-radius relationships for very low mass gaseous planets. | BATYGIN K. and STEVENSON D.J. | ||
2013ApJ...771..107E ![]() |
16 | D | 1 | 756 | 47 | Spectroscopy of faint Kepler mission exoplanet candidate host stars. | EVERETT M.E., HOWELL S.B., SILVA D.R., et al. | ||
2013ApJ...775...80F | 81 | X | 2 | 22 | 98 | A framework for characterizing the atmospheres of low-mass low-density transiting planets. | FORTNEY J.J., MORDASINI C., NETTELMANN N., et al. | ||
2013AJ....146..122K | 16 | D | 1 | 42 | 4 | Solar system moons as analogs for compact exoplanetary systems. | KANE S.R., HINKEL N.R. and RAYMOND S.N. | ||
2013ApJ...778..110M | 118 | X | 3 | 23 | 0 | Eight planets in four multi-planet systems via transit timing variations in 1350 days. | MING Y., HUI-GEN L., HUI Z., et al. | ||
2014ApJS..210...19B ![]() |
16 | D | 1 | 5860 | 162 | Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). | BURKE C.J., BRYSON S.T., MULLALLY F., et al. | ||
2014A&A...561A.103O | 119 | X C | 2 | 28 | 28 | An independent planet search in the Kepler dataset. II. An extremely low-density super-earth mass planet around Kepler-87. | OFIR A., DREIZLER S., ZECHMEISTER M., et al. | ||
2014ApJ...784...45R ![]() |
16 | D | 1 | 1691 | 227 | 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. | ||
2014ApJ...785...15J ![]() |
40 | X | 1 | 33 | 59 | Kepler-79's low density planets. | JONTOF-HUTTER D., LISSAUER J.J., ROWE J.F., et al. | ||
2014A&A...564A..50L | 41 | X | 1 | 11 | 26 | Measuring stellar differential rotation with high-precision space-borne photometry. | LANZA A.F., DAS CHAGAS M.L. and DE MEDEIROS J.R. | ||
2014ApJ...790..146F ![]() |
16 | D | 1 | 918 | 322 | Architecture of Kepler's multi-transiting systems. II. New investigations with twice as many candidates. | FABRYCKY D.C., LISSAUER J.J., RAGOZZINE D., et al. | ||
2014ApJ...796...48Z ![]() |
16 | D | 1 | 199 | 11 | The ground-based H-, K-, and L-band absolute emission spectra of HD 209458b. | ZELLEM R.T., GRIFFITH C.A., DEROO P., et al. | ||
2015ApJ...798...66D | 40 | X | 1 | 296 | 52 | 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...800L...9A | 40 | X | 1 | 15 | 7 | The well-aligned orbit of Wasp-84b: evidence for disk migration of a hot Jupiter. | ANDERSON D.R., TRIAUD A.H.M.J., TURNER O.D., et al. | ||
2015ApJS..217...16R ![]() |
16 | D | 1 | 8625 | 84 | Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). | ROWE J.F., COUGHLIN J.L., ANTOCI V., et al. | ||
2015ApJS..217...31M ![]() |
16 | D | 1 | 2033 | 146 | Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). | MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al. | ||
2015A&A...579A..55B | 17 | D | 1 | 21 | 25 | SOPHIE velocimetry of Kepler transit candidates. XVI. Tomographic measurement of the low obliquity of KOI-12b, a warm Jupiter transiting a fast rotator. | BOURRIER V., LECAVELIER DES ETANGS A., HEBRARD G., et al. | ||
2015ApJ...809....8B ![]() |
16 | D | 1 | 112329 | 139 | Terrestrial planet occurrence rates for the Kepler GK dwarf sample. | BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al. | ||
2015MNRAS.453.4089S | 16 | D | 1 | 103 | 3 | Tides alone cannot explain Kepler planets close to 2:1 MMR. | SILBURT A. and REIN H. | ||
2016ApJ...820...39J | 16 | D | 1 | 107 | 48 | Secure mass measurements from transit timing: 10 Kepler exoplanets between 3 and 8 M⊕ with diverse densities and incident fluxes. | JONTOF-HUTTER D., FORD E.B., ROWE J.F., et al. | ||
2016ApJ...823...29A | 16 | D | 1 | 117 | 7 | Spin-orbit alignment for three transiting hot jupiters: WASP-103b, WASP-87b, and WASP-66b. | ADDISON B.C., TINNEY C.G., WRIGHT D.J., et al. | ||
2016ApJ...825...98H | 16 | D | 1 | 166 | 45 | Warm jupiters are less lonely than hot jupiters: close neighbors. | HUANG C., WU Y. and TRIAUD A.H.M.J. | ||
2016ApJ...831...64T ![]() |
98 | D | C | 2 | 49 | 62 | The mass-metallicity relation for giant planets. | THORNGREN D.P., FORTNEY J.J., MURRAY-CLAY R.A., et al. | |
2016AJ....152..158T ![]() |
16 | D | 1 | 4387 | 18 | Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25). | TWICKEN J.D., JENKINS J.M., SEADER S.E., et al. | ||
2016AJ....152..181H ![]() |
16 | D | 2 | 9279 | 9 | SETI observations of exoplanets with the Allen Telescope Array. | HARP G.R., RICHARDS J., TARTER J.C., et al. | ||
2017ApJ...834...17C ![]() |
16 | D | 1 | 290 | 84 | Probabilistic forecasting of the masses and radii of other worlds. | CHEN J. and KIPPING D. | ||
2017ApJ...838L...9E | 85 | X | 2 | 6 | 19 | Metal enrichment leads to low atmospheric C/O ratios in transiting giant exoplanets. | ESPINOZA N., FORTNEY J.J., MIGUEL Y., et al. | ||
2017MNRAS.466.1868C ![]() |
16 | D | 1 | 176 | 16 | An overabundance of low-density Neptune-like planets. | CUBILLOS P., ERKAEV N.V., JUVAN I., et al. | ||
2017AJ....154..108J ![]() |
16 | D | 1 | 3237 | 46 | 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. | ||
2018AJ....155...48W ![]() |
17 | D | 1 | 911 | 22 | The California-Kepler survey. V. Peas in a pod: planets in a Kepler multi-planet system are similar in size and regularly spaced. | WEISS L.M., MARCY G.W., PETIGURA E.A., et al. | ||
2018AJ....155...94S | 125 | X | 3 | 51 | 23 | Identifying exoplanets with deep learning: a five-planet resonant chain around Kepler-80 and an eighth planet around Kepler-90. | SHALLUE C.J. and VANDERBURG A. | ||
2018AJ....155..206A ![]() |
17 | D | 3 | 183 | ~ | Systematic search for rings around Kepler planet candidates: constraints on ring size and occurrence rate. | AIZAWA M., MASUDA K., KAWAHARA H., et al. | ||
2018MNRAS.478.2480P | 669 | A | D | X C | 16 | 27 | 2 | The architecture and formation of the Kepler-30 planetary system. | PANICHI F., GOZDZIEWSKI K., MIGASZEWSKI C., et al. |
2018A&A...615A..79V ![]() |
83 | 1 | Kepler Object of Interest Network. I. First results combining ground- and space-based observations of Kepler systems with transit timing variations. | VON ESSEN C., OFIR A., DREIZLER S., et al. | |||||
2018AJ....156...96W | 59 | D | X | 2 | 31 | 1 | TTV-determined masses for warm Jupiters and their close planetary companions. | WU D.-H., WANG S., ZHOU J.-L., et al. | |
2018ApJ...866...99B ![]() |
17 | D | 1 | 7129 | 101 | Revised radii of Kepler stars and planet's using Gaia Data Release 2. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
2018AJ....156..254W ![]() |
17 | D | 1 | 1269 | ~ | The California-Kepler Survey. VI. Kepler multis and singles have similar planet and stellar properties indicating a common origin. | WEISS L.M., ISAACSON H.T., MARCY G.W., et al. | ||
2018AJ....156..264F ![]() |
17 | D | 1 | 1909 | 112 | The California-Kepler Survey. VII. Precise planet radii leveraging Gaia DR2 reveal the stellar mass dependence of the Planet radius gap. | FULTON B.J. and PETIGURA E.A. | ||
2019MNRAS.484.3233B | 85 | F | 1 | 35 | ~ | HARPS-N radial velocities confirm the low densities of the Kepler-9 planets. | BORSATO L., MALAVOLTA L., PIOTTO G., et al. | ||
2019ApJ...874L..31T ![]() |
17 | D | 1 | 403 | ~ | Connecting giant planet atmosphere and interior modeling: constraints on atmospheric metal enrichment. | THORNGREN D. and FORTNEY J.J. | ||
2019ApJ...875...29M ![]() |
17 | D | 1 | 2918 | ~ | 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. | ||
2019AJ....157..171K ![]() |
17 | D | 1 | 4069 | ~ | Visual analysis and demographics of Kepler transit timing variations. | KANE M., RAGOZZINE D., FLOWERS X., et al. | ||
2019AJ....157..174O ![]() |
17 | D | 1 | 176 | ~ | Discovery of a third transiting planet in the Kepler-47 circumbinary system. | OROSZ J.A., WELSH W.F., HAGHIGHIPOUR N., et al. | ||
2020AJ....159...41T ![]() |
17 | D | 1 | 564 | ~ | Estimating planetary mass with deep learning. | TASKER E.J., LANEUVILLE M. and GUTTENBERG N. | ||
2020AJ....160..108B ![]() |
17 | D | 1 | 6855 | ~ | 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. | ||
2020ApJ...903..147M | 44 | X | 1 | 23 | ~ | Theoretical versus observational uncertainties: composition of giant exoplanets. | MULLER S., BEN-YAMI M. and HELLED R. | ||
2021AJ....161...70P ![]() |
90 | F | 1 | 17 | ~ | WASP-107b's density is even lower: a case study for the physics of planetary gas envelope accretion and orbital migration. | PIAULET C., BENNEKE B., RUBENZAHL R.A., et al. | ||
2021AJ....161..246J ![]() |
376 | D | X | 9 | 204 | ~ | 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...650A..40D | 179 | X | 4 | 6 | ~ | Multiscale behaviour of stellar activity and rotation of the planet host Kepler-30. | DE FREITAS D.B., LANZA A.F., DA SILVA GOMES F.O., et al. | ||
2021AJ....162..166M | 18 | D | 2 | 22 | ~ | Evidence for a nondichotomous solution to the Kepler dichotomy: mutual inclinations of Kepler planetary systems from transit duration variations. | MILLHOLLAND S.C., HE M.Y., FORD E.B., et al. | ||
2022AJ....164...42J | 205 | D | X | 5 | 79 | ~ | TESS Observations of Kepler Systems with Transit Timing Variations. | JONTOF-HUTTER D., DALBA P.A. and LIVINGSTON J.H. | |
2023AJ....165..171W | 20 | D | 1 | 42 | ~ | Evidence for Hidden Nearby Companions to Hot Jupiters. | WU D.-H., RICE M. and WANG S. |
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