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| K2-38b , the SIMBAD biblio (42 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:35:42 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2016ApJ...820...39J | 16 | D | 2 | 107 | 126 | 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...827...78S | 393 | A | D | X C | 10 | 49 | 94 | Eleven multiplanet systems from K2 campaigns 1 and 2 and the masses of two hot super-earths. | SINUKOFF E., HOWARD A.W., PETIGURA E.A., et al. |
|
2016ApJS..226....7C |
16 | D | 1 | 400 | 165 | 197 candidates and 104 validated planets in K2's first five fields. | CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al. | ||
|
2017AJ....154....5H |
16 | D | 1 | 231 | 145 | Kepler planet masses and eccentricities from TTV analysis. | HADDEN S. and LITHWICK Y. | ||
| 2018AJ....155...84W | 16 | D | 2 | 80 | 18 | The K2-HERMES survey. I. Planet-candidate properties from K2 Campaigns 1-3. | WITTENMYER R.A., SHARMA S., STELLO D., et al. | ||
| 2019MNRAS.482.1017B | 179 | C F | 2 | 3 | 52 | PYANETI: a fast and powerful software suite for multiplanet radial velocity and transit fitting. | BARRAGAN O., GANDOLFI D. and ANTONICIELLO G. | ||
|
2019AJ....157..174O |
16 | D | 1 | 176 | 61 | Discovery of a third transiting planet in the Kepler-47 circumbinary system. | OROSZ J.A., WELSH W.F., HAGHIGHIPOUR N., et al. | ||
|
2019ApJS..244...11K |
16 | D | 1 | 2119 | 48 | Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. | KRUSE E., AGOL E., LUGER R., et al. | ||
|
2020AJ....159...41T |
16 | D | 1 | 564 | ~ | Estimating planetary mass with deep learning. | TASKER E.J., LANEUVILLE M. and GUTTENBERG N. | ||
|
2020A&A...635A..73B |
16 | D | 1 | 73 | 22 | A multiplicity study of transiting exoplanet host stars. I. High-contrast imaging with VLT/SPHERE. | BOHN A.J., SOUTHWORTH J., GINSKI C., et al. | ||
| 2020ApJ...896L..22M | 66 | X | 1 | 3 | 77 | Irradiated ocean planets bridge super-earth and sub-Neptune populations. | MOUSIS O., DELEUIL M., AGUICHINE A., et al. | ||
|
2020MNRAS.496..851W |
16 | D | 2 | 245 | ~ | K2-HERMES II. Planet-candidate properties from K2 Campaigns 1-13. | WITTENMYER R.A., CLARK J.T., SHARMA S., et al. | ||
|
2020A&A...641A..92T |
1813 | A | D | X C | 44 | 8 | 17 | Characterization of the K2-38 planetary system. Unraveling one of the densest planets known to date. | TOLEDO-PADRON B., LOVIS C., SUAREZ MASCARENO A., et al. |
| 2020MNRAS.499..932P | 263 | D | X F | 6 | 40 | 35 | Chemical fingerprints of formation in rocky super-Earths' data. | PLOTNYKOV M. and VALENCIA D. | |
| 2021MNRAS.503.2825H | 17 | D | 1 | 79 | ~ | Implications of an improved water equation of state for water-rich planets. | HUANG C., RICE D.R., GRANDE Z.M., et al. | ||
| 2021A&A...651A..23G | 42 | X | 1 | 10 | ~ | Influence of equilibrium tides on transit-timing variations of close-in super-Earths. I. Application to single-planet systems and the case of K2-265 b. | GOMES G.O., BOLMONT E. and BLANCO-CUARESMA S. | ||
| 2021A&A...652A.110L | 17 | D | 1 | 82 | 7 | Why do more massive stars host larger planets? | LOZOVSKY M., HELLED R., PASCUCCI I., et al. | ||
|
2021ApJ...921...24S |
17 | D | 1 | 328 | 1 | The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. | SCHLAUFMAN K.C. and HALPERN N.D. | ||
| 2021Sci...374..330A | 43 | X | 1 | 47 | 73 | A compositional link between rocky exoplanets and their host stars. | ADIBEKYAN V., DORN C., SOUSA S.G., et al. | ||
| 2022A&A...662A..19J | 213 | X C F | 3 | 12 | 9 | Nucleation and growth of iron pebbles explains the formation of iron-rich planets akin to Mercury. | JOHANSEN A. and DORN C. | ||
|
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. | ||
|
2022A&A...665A.154B |
43 | X | 1 | 32 | 6 | HD 23472: a multi-planetary system with three super-Earths and two potential super-Mercuries,. | BARROS S.C.C., DEMANGEON O.D.S., ALIBERT Y., et al. | ||
| 2022MNRAS.517.3132R | 187 | D | X F | 4 | 11 | 3 | Forming iron-rich planets with giant impacts. | REINHARDT C., MEIER T., STADEL J.G., et al. | |
| 2022ApJ...940..144S | 43 | X | 1 | 5 | ~ | Rocky Histories: The Effect of High Excitations on the Formation of Rocky Planets. | SCORA J., VALENCIA D., MORBIDELLI A., et al. | ||
| 2023AJ....165...47E | 44 | X | 1 | 35 | 1 | TOI-1075 b: A Dense, Massive, Ultra-short-period Hot Super-Earth Straddling the Radius Gap. | ESSACK Z., SHPORER A., BURT J.A., et al. | ||
|
2023A&A...675A..52C |
44 | X | 1 | 25 | ~ | An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244). | CASTRO-GONZALEZ A., DEMANGEON O.D.S., LILLO-BOX J., et al. | ||
| 2023ApJ...955L...3G | 44 | X | 1 | 18 | ~ | Company for the Ultra-high Density, Ultra-short Period Sub-Earth GJ 367 b: Discovery of Two Additional Low-mass Planets at 11.5 and 34 Days. | GOFFO E., GANDOLFI D., EGGER J.A., et al. | ||
|
2023A&A...677A..33B |
17 | D | 1 | 120 | ~ | Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities No excess of cold Jupiters in small planet systems. | BONOMO A.S., DUMUSQUE X., MASSA A., et al. | ||
| 2024MNRAS.529.2577D | 224 | X C F | 3 | 6 | ~ | Formation of super-Mercuries via giant impacts. | DOU J., CARTER P.J. and LEINHARDT Z.M. | ||
| 2024MNRAS.530.1436V | 45 | X | 1 | 28 | ~ | Discoveries and timing of pulsars in M62. | VLEESCHOWER L., CORONGIU A., STAPPERS B.W., et al. | ||
|
2024A&A...685A.143M |
18 | D | 1 | 535 | ~ | Planets similar in size are often dissimilar in interior. | MAMONOVA E., SHAN Y., HATALOVA P., et al. | ||
| 2024AJ....168..281B | 152 | D | X | 4 | 40 | ~ | Revisiting the Relationship Between Rocky Exoplanet and Stellar Compositions: Reduced Evidence for a Super-Mercury Population. | BRINKMAN C.L., POLANSKI A.S., HUBER D., et al. | |
| 2024A&A...692A..67A | 18 | D | 2 | 68 | ~ | Linking the primordial composition of planet building disks to the present-day composition of rocky exoplanets. | ADIBEKYAN V., DEAL M., DORN C., et al. | ||
| 2025A&A...696A.174C | 93 | X | 2 | 17 | ~ | Can metal-rich worlds form by giant impacts? | CAMBIONI S., WEISS B.P., ASPHAUG E., et al. | ||
| 2025MNRAS.539..405W | 19 | D | 3 | 46 | ~ | A link between rocky planet composition and stellar age. | WEEKS A., VAN EYLEN V., HUBER D., et al. | ||
| 2025ApJS..278...52H | 65 | D | X | 2 | 136 | ~ | Planet Masses, Radii, and Orbits from NASA's K2 Mission. | HOWARD A.W., SINUKOFF E., BLUNT S., et al. | |
| 2025AJ....170..282B | 19 | D | 1 | 45 | ~ | A Link between Rocky Planet Density and Host Star Chemistry. | BEHMARD A., BRINKMAN C.L., HATTORI S., et al. | ||
| 2025ApJ...993..235R | 60 | ~ | Terrestrial Exoplanet Internal Structure Constraints Enabled by Comprehensive Host Star Characterization Reveal That Terrestrial Planets in Mean Motion Resonances Are Water Rich. | ROSS A., REGGIANI H., SCHLAUFMAN K.C., et al. | |||||
| 2025ApJS..281...61L | 19 | D | 1 | 643 | ~ | Stellar Characterization, Magnesium Abundances, and Chromospheric Activity Analysis of Stars with Confirmed Exoplanets from the K2 Mission. | LOAIZA-TACURI V., SOUTO D., QUISPE-HUAYNASI F., et al. | ||
| 2025A&A...704A.108C | 19 | D | 1 | 111 | ~ | Refractory element abundances in rocky planets and their host stars: Revisiting the compositional link. | CHEN X. and NI D. | ||
| 2026ApJ...997..253P | 120 | D | X | 3 | 41 | ~ | Evidence of 1:1 Slope between Rocky Super-Earths and Their Host Stars. | PLOTNYKOV M., VALENCIA D., ROSS A., et al. | |
| 2026ApJ...998...46T | 50 | X | 1 | 4 | ~ | Origins of Mercury's Big Heart of Iron: Exploring Pathways to Form High Core Mass Fraction Planets via N-body Simulations. | TAJER H., WANG J., CHILDS A.C., et al. |