NAME LP 791-18b , the SIMBAD biblio

NAME LP 791-18b , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:55:35


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Title First 3 Authors
2019ApJ...883L..16C 465       D     X         12 16 40 A super-earth and sub-Neptune transiting the late-type M dwarf LP 791-18. CROSSFIELD I.J.M., WAALKES W., NEWTON E.R., et al.
2020AJ....160....3C viz 17       D               1 35 58 A pair of TESS planets spanning the radius valley around the nearby mid-M dwarf LTT 3780. CLOUTIER R., EASTMAN J.D., RODRIGUEZ J.E., et al.
2020AJ....160..116G 43           X         1 34 78 The first habitable-zone Earth-sized planet from TESS. I. Validation of the TOI-700 system. GILBERT E.A., BARCLAY T., SCHLIEDER J.E., et al.
2020AJ....160..172N 82               F     1 32 ~ π Earth: a 3.14 day Earth-sized planet from K2's kitchen served warm by the SPECULOOS team. NIRAULA P., DE WIT J., RACKHAM B.V., et al.
2021AJ....161..174M viz 17       D               2 31 ~ Phase-curve pollution of exoplanet transmission spectra. MORELLO G., ZINGALES T., MARTIN-LAGARDE M., et al.
2021A&A...650A..78B 42           X         1 32 25 An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685. BLUHM P., PALLE E., MOLAVERDIKHANI K., et al.
2021ApJS..254...39G viz 17       D               1 2206 165 The TESS Objects of Interest Catalog from the TESS Prime Mission. GUERRERO N.M., SEAGER S., HUANG C.X., et al.
2021AJ....162...54H 17       D               1 24 21 TOI-2076 and TOI-1807: two young, comoving planetary systems within 50 pc identified by TESS that are ideal candidates for further follow up. HEDGES C., HUGHES A., ZHOU G., et al.
2022AJ....163....3C 43           X         1 14 3 A hot Mars-sized exoplanet transiting an M dwarf. CANAS C.I., MAHADEVAN S., COCHRAN W.D., et al.
2022MNRAS.509.4817G 102       D         F     2 25 17 PROSE: a PYTHON framework for modular astronomical images processing. GARCIA L.J., TIMMERMANS M., POZUELOS F.J., et al.
2022A&A...661A.101R viz 17       D               1 66 1 Internal structures and magnetic moments of rocky planets. Application to the first exoplanets discovered by TESS. RODRIGUEZ-MOZOS J.M. and MOYA A.
2022AJ....164...15E viz 17       D               1 514 13 The Ariel Target List: The Impact of TESS and the Potential for Characterizing Multiple Planets within a System. EDWARDS B. and TINETTI G.
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.
2023MNRAS.522..648C 757   K   D S   X C       16 12 ~ Surface pressure impact on nitrogen-dominated USP super-Earth atmospheres. CHOUQAR J., LUSTIG-YAEGER J., BENKHALDOUN Z., et al.
2023Natur.617..701P 174           X         4 5 1 A temperate Earth-sized planet with tidal heating transiting an M6 star. PETERSON M.S., BENNEKE B., COLLINS K., et al.
2023AJ....166...35B 44           X         1 39 ~ The MUSCLES Extension for Atmospheric Transmission Spectroscopy: UV and X-Ray Host-star Observations for JWST ERS & GTO Targets. BEHR P.R., FRANCE K., BROWN A., et al.
2024A&A...687A.264B 90               F     1 58 ~ Three short-period Earth-sized planets around M dwarfs discovered by TESS: TOI-5720 b, TOI-6008 b, and TOI-6086 b. BARKAOUI K., SCHWARZ R.P., NARITA N., et al.
2024MNRAS.532.4752D 18       D               1 130 ~ The SHERLOCK pipeline: new exoplanet candidates in the WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 systems. DEVORA-PAJARES M., POZUELOS F.J., THUILLIER A., et al.
2025ApJ...986L...3P 19       D               1 56 ~ The Receding Cosmic Shoreline of Mid-to-late M Dwarfs: Measurements of Active Lifetimes Worsen Challenges for Atmosphere Retention by Rocky Exoplanets. PASS E.K., CHARBONNEAU D. and VANDERBURG A.
2025ApJ...992..198J 19       D               1 94 ~ The Cosmic Shoreline Revisited: A Metric for Atmospheric Retention Informed by Hydrodynamic Escape. JI X., CHATTERJEE R.D., COY B.P., et al.

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