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| CoRoT-19 , the SIMBAD biblio (43 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:26:26 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2012A&A...537A.136G | 497 | O X C | 12 | 5 | 17 | Transiting exoplanets from the CoRoT space mission. XXI. CoRoT-19b: a low density planet orbiting an old inactive F9V-star. | GUENTHER E.W., DIAZ R.F., GAZZANO J.-C., et al. | ||
| 2012ApJ...757....7M | 76 | C | 1 | 26 | 21 | WISE detections of dust in the habitable zones of planet-bearing stars. | MORALES F.Y., PADGETT D.L., BRYDEN G., et al. | ||
|
2012ApJ...757...18A |
40 | X | 1 | 84 | 472 | Obliquities of hot Jupiter host stars: evidence for tidal interactions and primordial misalignments. | ALBRECHT S., WINN J.N., JOHNSON J.A., et al. | ||
|
2012MNRAS.426.1291S |
1373 | A | D | S X C | 35 | 81 | 121 | Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets. | SOUTHWORTH J. |
| 2013A&A...550A..67P | 15 | D | 1 | 44 | 15 | Secondary eclipses in the CoRoT light curves. A homogeneous search based on Bayesian model selection. | PARVIAINEN H., DEEG H.J. and BELMONTE J.A. | ||
|
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. | ||
|
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. | ||
|
2013A&A...558A..86B |
38 | X | 1 | 14 | 9 | HAT-P-42b and HAT-P-43b. Two inflated transiting hot jupiters from the HATNet survey. | BOISSE I., HARTMAN J.D., BAKOS G.A., et al. | ||
| 2014ApJ...786..102V | 15 | D | 1 | 110 | 47 | Tidal dissipation and obliquity evolution in hot Jupiter systems. | VALSECCHI F. and RASIO F.A. | ||
| 2014ApJ...790L..31D | 78 | C | 1 | 14 | 55 | On the tidal origin of hot Jupiter stellar obliquity trends. | DAWSON R.I. | ||
| 2014MNRAS.442.1844B | 15 | D | 2 | 81 | 26 | Discrepancies between isochrone fitting and gyrochronology for exoplanet host stars? | BROWN D.J.A. | ||
|
2015A&A...575A..18B |
16 | D | 1 | 319 | 28 | Revising the ages of planet-hosting stars. | BONFANTI A., ORTOLANI S., PIOTTO G., et al. | ||
|
2016A&A...585A...5B |
16 | D | 2 | 339 | 83 | Age consistency between exoplanet hosts and field stars. | BONFANTI A., ORTOLANI S. and NASCIMBENI V. | ||
| 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. | ||
|
2016A&A...589A..58E |
94 | D | X | 3 | 85 | 36 | High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). I. Lucky imaging observations of 101 systems in the southern hemisphere. | EVANS D.F., SOUTHWORTH J., MAXTED P.F.L., et al. | |
|
2016AJ....152..181H |
16 | D | 1 | 9279 | 22 | SETI observations of exoplanets with the Allen Telescope Array. | HARP G.R., RICHARDS J., TARTER J.C., et al. | ||
| 2017MNRAS.464..810B | 40 | X | 1 | 28 | 52 | Rossiter-McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems. | BROWN D.J.A., TRIAUD A.H.M.J., DOYLE A.P., et al. | ||
|
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. | ||
|
2017A&A...603A..30S |
16 | D | 2 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
|
2018AJ....155..177D |
80 | S | 1 | 124 | 2 | Stellar obliquity and magnetic activity of planet-hosting stars and eclipsing binaries based on transit chord correlation. | DAI F., WINN J.N., BERTA-THOMPSON Z., et al. | ||
| 2018A&A...617A...4S | 80 | X | 2 | 50 | 13 | The Gaia-ESO Survey: properties of newly discovered Li-rich giants. | SMILJANIC R., FRANCIOSINI E., BRAGAGLIA A., et al. | ||
|
2018ApJS..239...14J |
16 | D | 1 | 1561 | 6 | Revised exoplanet radii and habitability using Gaia data release 2. | JOHNS D., MARTI C., HUFF M., et al. | ||
|
2018A&A...620A..58S |
16 | D | 1 | 164 | 10 | SWEET-Cat updated. New homogenous spectroscopic parameters. | SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al. | ||
|
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. | ||
|
2020AJ....159..194V |
16 | D | 1 | 288 | ~ | A statistical search for star-planet interaction in the ultraviolet using GALEX. | VISWANATH G., NARANG M., MANOJ P., 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. | ||
|
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. | ||
|
2021AJ....162...75L |
17 | D | 1 | 517 | 28 | Speckle observations of TESS exoplanet host stars. II. Stellar companions at 1-1000 au and implications for small planet detection. | LESTER K.V., MATSON R.A., HOWELL S.B., et al. | ||
|
2021AJ....162..263H |
17 | D | 1 | 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. | ||
|
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. | ||
|
2022AJ....163..228P |
17 | D | 1 | 354 | 20 | Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. | PATEL J.A. and ESPINOZA N. | ||
|
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. | ||
|
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. | ||
|
2022AJ....164..104R |
60 | D | X | 2 | 105 | 10 | A Tendency Toward Alignment in Single-star Warm-Jupiter Systems. | RICE M., WANG S., WANG X.-Y., et al. | |
|
2022PASP..134h2001A |
43 | X | 1 | 366 | 39 | Stellar Obliquities in Exoplanetary Systems. | ALBRECHT S.H., DAWSON R.I. and WINN J.N. | ||
| 2024ApJS..274...20P | 18 | D | 1 | 223 | ~ | Statistics and Habitability of F-type Star-Planet Systems. | PATEL S.D., CUNTZ M. and WEINBERG N.N. | ||
| 2024ApJ...973L..21W | 45 | X | 1 | 46 | ~ | Single-star Warm-Jupiter Systems Tend to Be Aligned, Even around Hot Stellar Hosts: No Teff-λ Dependency. | WANG X.-Y., RICE M., WANG S., 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. | ||
|
2025A&A...697A.102T |
19 | D | 1 | 176 | ~ | Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel mission candidate sample. | TSANTAKI M., MAGRINI L., DANIELSKI C., et al. | ||
| 2025AJ....170...70E | 47 | X | 1 | 38 | ~ | The Spin-Orbit Alignment of Eight Warm Gas Giant Systems. | ESPINOZA-RETAMAL J.I., JORDAN A., BRAHM R., et al. | ||
| 2025PASP..137g4401G | 47 | X | 1 | 13 | ~ | A Hot Jupiter with a Retrograde Orbit Around A Sun-like Star and a Toy Model of Hot Jupiters in Wide Binary Star Systems. | GIACALONE S., HOWARD A.W., RUBENZAHL R.A., et al. | ||
| 2026ApJ...996L...7W | 50 | X | 1 | 48 | ~ | Unified Kraft Break at ∼6500 K: A Newly Identified Single-star Obliquity Transition Matches the Classical Rotation Break. | WANG X.-Y., WANG S. and ONG J.M.J. | ||
| 2026AJ....171..157S | 20 | D | 2 | 480 | ~ | Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr. | SCHMIDT S.P. and SCHLAUFMAN K.C. |