NGTS-5 , the SIMBAD biblio

NGTS-5 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST04:15:13

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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
2019A&A...625A.142E 528           X C       12 8 5 NGTS-5b: a highly inflated planet offering insights into the sub-Jovian desert. EIGMULLER P., CHAUSHEV A., GILLEN E., et al.
2020ApJ...890...23L viz 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.
2021ApJ...909..115C viz 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.
2022AJ....164..234V 17       D               1 33 22 The Upper Edge of the Neptune Desert Is Stable Against Photoevaporation. VISSAPRAGADA S., KNUTSON H.A., GREKLEK-MCKEON M., et al.
2023A&A...673A..37F 17       D               2 57 ~ Possible origin of the non-detection of metastable He I in the upper atmosphere of the hot Jupiter WASP-80b. FOSSATI L., PILLITTERI I., SHAIKHISLAMOV I.F., et al.
2024MNRAS.532.4752D 45           X         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.
2024A&A...691A..53S viz 18       D               1 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2024AJ....168..252A viz 18       D               1 155 ~ Measuring Sub-Kelvin Variations in Stellar Temperature with High-resolution Spectroscopy. ARTIGAU E., CADIEUX C., COOK N.J., et al.
2025A&A...698A.112L 47           X         1 84 ~ sunset: A database of synthetic atmospheric-escape transmission spectra for nearly every transiting planet. LINSSEN D., OKLOPCIC A. and MacLEOD M.
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.
2026A&A...707A.315W viz 400           X C       7 10 ~ Evidence for stellar contamination and water absorption in NGTS-5b's transmission spectra with GTC/OSIRIS. WANG W.-H., CHEN G., JIANG C., et al.

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