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| Kepler-412 , the SIMBAD biblio (73 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:21:34 |
| 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 | 1 | 997 | 230 | On the low false positive probabilities of Kepler planet candidates. | MORTON T.D. and JOHNSON J.A. | ||
|
2011ApJS..197....2F |
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. | ||
|
2012AJ....143...39C |
15 | D | 1 | 90 | 34 | A uniform search for secondary eclipses of hot Jupiters in Kepler Q2 light curves. | COUGHLIN J.L. and LOPEZ-MORALES M. | ||
|
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...752...72D |
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 |
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 |
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. | ||
| 2012A&A...545A..76S | 16 | D | 1 | 69 | 149 | SOPHIE velocimetry of Kepler transit candidates. VII. A false-positive rate of 35% for Kepler close-in giant candidates. | SANTERNE A., DIAZ R.F., MOUTOU C., et al. | ||
|
2013A&A...552A.119S |
15 | D | 1 | 1487 | 118 | Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. | SAUR J., GRAMBUSCH T., DULING S., et al. | ||
|
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 | 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. | ||
|
2013A&A...556A.150S |
15 | D | 1 | 635 | 211 | SWEET-Cat: a catalogue of parameters for Stars With ExoplanETs. I. New atmospheric parameters and masses for 48 stars with planets. | SANTOS N.C., SOUSA S.G., MORTIER A., et al. | ||
|
2013MNRAS.436.1883W |
15 | D | 1 | 961 | 136 | Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. | WALKOWICZ L.M. and BASRI G.S. | ||
|
2013A&A...560A...4R |
15 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
| 2013A&A...560A.112M | 169 | D | X | 5 | 60 | 34 | High-precision stellar limb-darkening measurements. A transit study of 38 Kepler planetary candidates. | MUELLER H.M., HUBER K.F., CZESLA S., et al. | |
|
2014ApJS..210...19B |
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. | ||
|
2014A&A...562A.108S |
15 | D | 1 | 196 | 44 | Search for 150 MHz radio emission from extrasolar planets in the TIFR GMRT Sky Survey. | SIROTHIA S.K., LECAVELIER DES ETANGS A., GOPAL-KRISHNA, 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. | ||
| 2014A&A...564A..56D | 62 | A | X | 2 | 27 | 14 | SOPHIE velocimetry of Kepler transit candidates XI. Kepler-412 system: probing the properties of a new inflated hot Jupiter. | DELEUIL M., ALMENARA J.-M., SANTERNE A., et al. | |
|
2015A&A...574A..39D |
16 | D | 1 | 113 | 33 | Evolution of angular-momentum-losing exoplanetary systems. Revisiting Darwin stability. | DAMIANI C. and LANZA A.F. | ||
|
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. | ||
| 2015ApJ...804..150E | 18 | D | 2 | 32 | 158 | Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry. | ESTEVES L.J., DE MOOIJ E.J.W. and JAYAWARDHANA R. | ||
| 2015ApJ...806...97K | 16 | D | 1 | 93 | 15 | Polarization in exoplanetary systems caused by transits, grazing transits, and starspots. | KOSTOGRYZ N.M., YAKOBCHUK T.M. and BERDYUGINA S.V. | ||
|
2015ApJ...807..170H |
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 |
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. | ||
| 2015AJ....150..112S | 39 | X | 1 | 20 | 29 | Studying atmosphere-dominated hot Jupiter Kepler phase curves: evidence that inhomogeneous atmospheric reflection is common. | SHPORER A. and HU R. | ||
|
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 | 1 | 2846 | 162 | An increase in the mass of planetary systems around lower-mass stars. | MULDERS G.D., PASCUCCI I. and APAI D. | ||
| 2015PASP..127.1113A | 16 | D | 5 | 59 | 102 | A comprehensive study of Kepler phase curves and secondary eclipses: temperatures and Albedos of confirmed Kepler giant planets. | ANGERHAUSEN D., DELARME E. and MORSE J.A. | ||
|
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. | ||
| 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 |
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 | 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...602A.107B |
16 | D | 2 | 476 | 185 | The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. | BONOMO A.S., DESIDERA S., BENATTI S., et al. | ||
|
2018ApJS..234....9O |
16 | D | 1 | 436 | 14 | A spectral approach to transit timing variations. | OFIR A., XIE J.-W., JIANG C.-F., et al. | ||
| 2018AJ....156...91M | 522 | A | D | S X C | 12 | 24 | 9 | Robust transiting exoplanet radii in the presence of starspots from ingress and egress durations. | MORRIS B.M., AGOL E., HEBB L., et al. |
|
2018A&A...616A...7S |
16 | D | 1 | 4792 | 112 | Gaia Data Release 2. The catalogue of radial velocity standard stars. | SOUBIRAN C., JASNIEWICZ G., CHEMIN L., et al. | ||
|
2018A&A...616A..39M |
122 | X C | 2 | 19 | 54 | Comparison of the power-2 limb-darkening law from the STAGGER-grid to Kepler light curves of transiting exoplanets. | MAXTED P.F.L. | ||
|
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. | ||
|
2018ApJ...869...66H |
16 | D | 1 | 99 | ~ | The application of autocorrelation SETI search techniques in an ATA survey. | HARP G.R., ACKERMANN R.F., ASTORGA A., et al. | ||
|
2019AJ....158..190H |
16 | D | 1 | 343 | 61 | Hot Jupiters are destroyed by tides while their host stars are on the main sequence. | HAMER J.H. and SCHLAUFMAN K.C. | ||
| 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. | ||
| 2020MNRAS.491.3137K | 41 | X | 1 | 12 | ~ | Stability of exoplanetary systems retrieved from scalar time series. | KOVACS T. | ||
|
2020ApJ...890...23L |
16 | D | 1 | 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. | ||
| 2020A&A...638A.143A | 16 | D | 1 | 193 | ~ | Variability of transit light curves of Kepler objects of interest. | ARKHYPOV O.V., KHODACHENKO M.L. and HANSLMEIER A. | ||
|
2020AJ....160..108B |
16 | 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. | ||
|
2021A&A...645A...7K |
17 | D | 1 | 1569 | 17 | Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. | KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al. | ||
| 2021A&A...646A.136A | 17 | D | 1 | 43 | ~ | Revealing peculiar exoplanetary shadows from transit light curves. | ARKHYPOV O.V., KHODACHENKO M.L. and HANSLMEIER A. | ||
|
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.503.4092B | 17 | D | 2 | 124 | ~ | Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data. | BATTLEY M.P., KUNIMOTO M., ARMSTRONG D.J., 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. | ||
| 2021ApJ...914...56A | 17 | D | 1 | 55 | 13 | On a possible solution to the tidal realignment problem for hot Jupiters. | ANDERSON K.R., WINN J.N. and PENEV K. | ||
|
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. | ||
|
2022MNRAS.512L..60H |
17 | D | 1 | 1974 | 9 | The flaring TESS Objects of Interest: flare rates for all two-minute cadence TESS planet candidates. | HOWARD W.S. | ||
|
2022MNRAS.513..102C |
17 | D | 1 | 961 | 6 | The TESS Triple-9 Catalog: 999 uniformly vetted exoplanet candidates. | CACCIAPUOTI L., KOSTOV V.B., KUCHNER M., et al. | ||
|
2022ApJS..261...26S |
17 | D | 1 | 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. | ||
| 2022ApJ...939...79C | 102 | D | C | 2 | 13 | ~ | Analysis of Thermal Emissions of Exoplanets with Axially Symmetric Temperature Gradients. | CARTER J.L. | |
|
2023ApJS..264...17Z |
17 | D | 1 | 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. | ||
| 2023AJ....165..171W | 392 | S X | 8 | 42 | 7 | Evidence for Hidden Nearby Companions to Hot Jupiters. | WU D.-H., RICE M. and WANG S. | ||
| 2023MNRAS.519.3723M | 17 | D | 2 | 48 | 1 | Limb darkening measurements from TESS and Kepler light curves of transiting exoplanets. | MAXTED P.F.L. | ||
|
2023NatAs...7..900C |
17 | D | 1 | 1054 | ~ | On the behaviour of spin-orbit connection of exoplanets. | CANTO MARTINS B.L., MESSIAS Y.S., ARRUDA GONCALVES M.I., et al. | ||
| 2023A&A...679A..65L | 17 | D | 1 | 18 | ~ | Effects of magnetic fields on the center-to-limb variation in solar-type stars. | LUDWIG H.-G., STEFFEN M. and FREYTAG B. | ||
|
2023A&A...679L..12G |
17 | D | 1 | 796 | ~ | Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars Architecture of Kepler confirmed single-exoplanet systems compared to star-planet evolution models. | GARCIA R.A., GOURVES C., SANTOS A.R.G., et al. | ||
| 2024ApJ...960...50W | 18 | D | 1 | 46 | ~ | Orbital Decay of Hot Jupiters due to Weakly Nonlinear Tidal Dissipation. | WEINBERG N.N., DAVACHI N., ESSICK R., et al. | ||
|
2024A&A...689A.250C |
18 | D | 1 | 3075 | ~ | Mapping the exo-Neptunian landscape A ridge between the desert and savanna. | CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al. | ||
| 2024MNRAS.534.3893V | 18 | D | 1 | 43 | ~ | A regularization technique to precisely infer limb darkening using transit measurements: can we estimate stellar surface magnetic fields? | VERMA K., MAXTED P.F.L., SINGH A., 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. | ||
| 2025ApJ...988L...4H | 19 | D | 1 | 301 | ~ | Hundreds of TESS Exoplanets Might Be Larger than We Thought. | HAN T., ROBERTSON P., BRANDT T.D., et al. |