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| Kepler-192 , the SIMBAD biblio (72 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:45:04 |
| 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 | 2 | 997 | 230 | On the low false positive probabilities of Kepler planet candidates. | MORTON T.D. and JOHNSON J.A. | ||
|
2011ApJS..197....2F |
15 | D | 2 | 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....8L |
16 | D | 1 | 177 | 608 | Architecture and dynamics of Kepler's candidate multiple transiting planet systems. | LISSAUER J.J., RAGOZZINE D., FABRYCKY D.C., et al. | ||
|
2012MNRAS.420L..23V |
15 | D | 1 | 94 | 22 | Identifying non-resonant Kepler planetary systems. | VERAS D. and FORD E.B. | ||
|
2012ApJS..199...24T |
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...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 | 2 | 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. | ||
|
2013MNRAS.429.2001H |
15 | D | 1 | 140 | 33 | 150 new transiting planet candidates from Kepler Q1-Q6 data. | HUANG X., BAKOS G.A. and HARTMAN J.D. | ||
|
2013A&A...555A..58O |
92 | D | S | 4 | 171 | 53 | An independent planet search in the Kepler dataset. I. One hundred new candidates and revised Kepler objects of interest. | OFIR A. and DREIZLER S. | |
|
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. | ||
|
2014ApJS..210...19B |
15 | D | 3 | 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...783..123C |
15 | D | 1 | 221 | 18 | Limits on surface gravities of Kepler planet-candidate host stars from non-detection of solar-like oscillations. | CAMPANTE T.L., CHAPLIN W.J., LUND M.N., 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. | ||
| 2014ApJ...795...85W | 40 | X | 1 | 6 | 20 | Near 3:2 and 2:1 mean motion resonance formation in the systems observed by Kepler. | WANG S. and JI J. | ||
|
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. | ||
| 2015MNRAS.448.1956S | 78 | F | 1 | 84 | 51 | The period ratio distribution of Kepler's candidate multiplanet systems. | STEFFEN J.H. and HWANG J.A. | ||
|
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...809....8B |
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...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 | 3 | 2846 | 162 | An increase in the mass of planetary systems around lower-mass stars. | MULDERS G.D., PASCUCCI I. and APAI D. | ||
|
2016ApJ...821...47B |
16 | D | 1 | 217 | 14 | Efficient geometric probabilities of multi-transiting exoplanetary systems from CORBITS. | BRAKENSIEK J. and RAGOZZINE D. | ||
|
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. | ||
|
2016AJ....152...18B |
16 | D | 2 | 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 |
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. | ||
|
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 | 3 | 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...602A.101R | 40 | X | 1 | 69 | 10 | Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in exoplanets. | RAMOS X.S., CHARALAMBOUS C., BENITEZ-LLAMBAY P., et al. | ||
|
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. | ||
| 2017AJ....154..236W | 95 | D | X | 3 | 34 | 7 | Near mean-motion resonances in the system observed by Kepler: affected by mass accretion and Type I migration. | WANG S. and JI J. | |
| 2018AJ....155...57C | 41 | X | 1 | 34 | 51 | The K2-138 system: a near-resonant chain of five sub-Neptune planets discovered by citizen scientists. | CHRISTIANSEN J.L., CROSSFIELD I.J.M., BARENTSEN G., et al. | ||
|
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. | ||
|
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. | ||
|
2018ApJS..237...38B |
16 | D | 2 | 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. | ||
|
2018AJ....156..292T |
16 | D | 2 | 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. | ||
|
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. | ||
|
2020ApJ...890...23L |
16 | D | 3 | 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. | ||
|
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. | ||
|
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.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. | ||
|
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. | ||
|
2022AJ....163...91J |
85 | X | 2 | 504 | ~ | Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. | JUDKOVSKY Y., OFIR A. and AHARONSON O. | ||
|
2022AJ....163..128W |
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 |
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. | ||
|
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. | ||
|
2022ApJS..259...35A |
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...60S |
17 | D | 3 | 854 | 2 | Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? | SWASTIK C., BANYAL R.K., NARANG M., et al. | ||
|
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. | ||
|
2023ApJS..265...50C |
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 |
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 | 1 | 165 | ~ | Differences between Stable and Unstable Architectures of Compact Planetary Systems. | VOLK K. and MALHOTRA R. | ||
|
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. | ||
|
2024AJ....168..129S |
18 | D | 3 | 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. | ||
| 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..154V | 18 | D | 4 | 210 | ~ | Modeling Multiple Radius Valley Emergence Mechanisms with Multitransiting Systems. | VANWYNGARDEN M. and CLOUTIER R. | ||
|
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. | ||
| 2025ApJS..277...15J | 19 | D | 2 | 136 | ~ | Half a Million Binary Stars Identified from the Low-resolution Spectra of LAMOST. | JING Y., MAO T.-X., WANG J., et al. | ||
|
2025A&A...699A.100D |
19 | D | 1 | 2580 | ~ | The Gaia spectroscopic catalogue of exoplanets and host stars. | DE LAVERNY P., LIGI R., CRIDA A., et al. | ||
| 2026ApJ...998..301G | 20 | D | 1 | 561 | ~ | A Comprehensive Study of the Relations between the Properties of Planetary Systems and the Chemical Compositions of Their Host Stars. | GHEZZI L., COSTA-ALMEIDA E., LOAIZA-TACURI V., et al. |