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| KELT-16 , the SIMBAD biblio (32 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST01:51:24 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2017AJ....153...97O | 1884 | D | X C | 47 | 11 | 42 | KELT-16b: a highly irradiated, ultra-short period hot Jupiter nearing tidal disruption. | OBERST T.E., RODRIGUEZ J.E., COLON K.D., et al. | |
|
2017MNRAS.472..675A |
16 | D | 1 | 13582 | 89 | Wide binaries in Tycho-Gaia: search method and the distribution of orbital separations. | ANDREWS J.J., CHANAME J. and AGUEROS M.A. | ||
|
2018ApJS..237...38B |
16 | D | 1 | 1111 | 42 | Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. | BREWER J.M. and FISCHER D.A. | ||
|
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. | ||
|
2019AJ....158..190H |
41 | X | 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. | ||
| 2020MNRAS.491.1243P | 17 | D | 1 | 18 | 19 | Discarding orbital decay in WASP-19b after one decade of transit observations. | PETRUCCI R., JOFRE E., GOMEZ MAQUEO CHEW Y., 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..150P |
42 | A | D | 3 | 33 | 51 | The continuing search for evidence of tidal orbital decay of hot Jupiters. | PATRA K.C., WINN J.N., HOLMAN M.J., et al. | |
| 2020MNRAS.497.3911L | 16 | D | 1 | 18 | ~ | Orbital period modulation in hot Jupiter systems. | LANZA A.F. | ||
|
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. | ||
| 2021MNRAS.506.2247A | 42 | X | 1 | 11 | 6 | The impact of tidal friction evolution on the orbital decay of ultra-short-period planets. | ALVARADO-MONTES J.A., SUCERQUIA M., GARCIA-CARMONA C., et al. | ||
|
2021AJ....162..127W |
543 | A | D | S X C | 12 | 47 | 35 | Visible-light phase curves from the second Year of the TESS primary mission. | WONG I., KITZMANN D., SHPORER A., et al. |
| 2021MNRAS.508.5514G | 42 | X | 1 | 8 | 7 | Is the orbit of the exoplanet WASP-43b really decaying? TESS and MuSCAT2 observations confirm no detection. | GARAI Z., PRIBULLA T., PARVIAINEN H., et al. | ||
|
2022MNRAS.509.1447M |
1005 | K A | X C F | 22 | 48 | 5 |
The ultra-hot-Jupiter KELT-16 b: dynamical evolution and atmospheric properties. |
MANCINI L., SOUTHWORTH J., NAPONIELLO L., et al. | |
|
2022ApJS..258...16P |
17 | D | 1 | 4582 | 43 | TESS Eclipsing Binary stars. I. Short-cadence observations of 4584 eclipsing binaries in sectors 1-26. | PRSA A., KOCHOSKA A., CONROY K.E., et al. | ||
|
2022AJ....163..160B |
17 | D | 2 | 240 | 9 | Stellar Companions to TESS Objects of Interest: A Test of Planet-Companion Alignment. | BEHMARD A., DAI F. and HOWARD A.W. | ||
|
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. | ||
|
2022ApJS..259...62I |
17 | D | 1 | 395 | 24 | TESS Transit Timing of Hundreds of Hot Jupiters. | IVSHINA E.S. and WINN J.N. | ||
|
2022AJ....164...60S |
17 | D | 1 | 854 | 2 | Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? | SWASTIK C., BANYAL R.K., NARANG 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. | ||
|
2022A&A...667A.127M |
213 | A | D | X | 6 | 12 | 3 | Planet-star interactions with precise transit timing III. Entering the regime of dynamical tides,. | MACIEJEWSKI G., FERNANDEZ M., SOTA A., et al. |
| 2022A&A...668A.114R | 102 | D | X | 3 | 17 | 2 | Measuring the orbit shrinkage rate of hot Jupiters due to tides. | ROSARIO N.M., BARROS S.C.C., DEMANGEON O.D.S., et al. | |
|
2023A&A...669A.124H |
157 | A | X | 4 | 10 | 3 |
Examining the orbital decay targets KELT-9 b, KELT-16 b, and WASP-4b, and the transit-timing variations of HD 97658 b,. |
HARRE J.-V., SMITH A.M.S., BARROS S.C.C., 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...685A.131B | 45 | X | 1 | 12 | ~ | Star-spot activity, orbital obliquity, transmission spectrum, physical properties, and transit time variations of the HATS-2 planetary system. | BIAGIOTTI F., MANCINI L., SOUTHWORTH J., et al. | ||
| 2024MNRAS.534..800A | 242 | D | X C | 5 | 16 | ~ | Searching for tidal orbital decay in hot Jupiters. | ALVARADO III E., BOSTOW K.B., PATRA K.C., 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. | ||
|
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. | ||
| 2025ApJ...993...78S | 19 | D | 3 | 63 | ~ | In Search of Decay: An Analysis of Transit Times of Hot Jupiters in Main-sequence and Post-main-sequence Systems. | SODICKSON N. and GRUNBLATT S. | ||
| 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. |