NAME LP 759-72b , the SIMBAD biblio

NAME LP 759-72b , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:58:56

Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
2016ApJS..226....7C viz 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.
2019MNRAS.485.3999M viz 16       D               1 474 ~ Planetary magnetism as a parameter in exoplanet habitability. McINTYRE S.R.N., LINEWEAVER C.H. and IRELAND M.J.
2019MNRAS.488..633V 16       D               1 148 ~ Can we detect aurora in exoplanets orbiting M dwarfs? VIDOTTO A.A., FEENEY N. and GROH J.H.
2020AJ....159..211C viz 16       D               1 351 93 Evolution of the radius valley around low-mass stars from Kepler and K2. CLOUTIER R. and MENOU K.
2021AJ....162..259Z viz 17       D               1 1094 12 Scaling K2. IV. A uniform planet sample for Campaigns 1-8 and 10-18. ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al.
2022A&A...662A..15M viz 17       D               1 733 3 Tidally driven tectonic activity as a parameter in exoplanet habitability. McINTYRE S.R.N.
2023MNRAS.519.6210M viz 17       D               1 688 1 A rocky exoplanet classification method and its application to calculating surface pressure and surface temperature. McINTYRE S.R.N., KING P.L. and MILLS F.P.
2024ApJ...961...22S 18       D               1 42 ~ Potential Melting of Extrasolar Planets by Tidal Dissipation. SELIGMAN D.Z., FEINSTEIN A.D., LAI D., et al.
2025ApJ...982..111C 19       D               1 130 ~ Observational Signatures of a Previous Dynamical Instability in Multi-planet M-dwarf Systems. CHILDS A.C., HUA A.P.S., MARTIN R.G., et al.
2025ApJ...993..233W viz 19       D               1 391 ~ An Analysis of the Radius Gap in a Sample of Kepler, K2, and TESS Exoplanets Orbiting M-dwarf Stars. WANDERLEY F., CUNHA K., SMITH V.V., et al.

goto View the references in ADS