A super-massive Neptune-sized planet
Author:
Naponiello LucaORCID, Mancini LuigiORCID, Sozzetti AlessandroORCID, Bonomo Aldo S.ORCID, Morbidelli Alessandro, Dou Jingyao, Zeng LiORCID, Leinhardt Zoe M.ORCID, Biazzo KatiaORCID, Cubillos Patricio E., Pinamonti MatteoORCID, Locci DanieleORCID, Maggio AntonioORCID, Damasso Mario, Lanza Antonino F.ORCID, Lissauer Jack J.ORCID, Collins Karen A., Carter Philip J.ORCID, Jensen Eric L. N.ORCID, Bignamini AndreaORCID, Boschin WalterORCID, Bouma Luke G.ORCID, Ciardi David R., Cosentino Rosario, Crossfield Ian, Desidera Silvano, Dumusque XavierORCID, Fiorenzano Aldo F. M.ORCID, Fukui AkihikoORCID, Giacobbe PaoloORCID, Gnilka Crystal L., Ghedina AdrianoORCID, Guilluy GloriaORCID, Harutyunyan Avet, Howell Steve B., Jenkins Jon M.ORCID, Lund Michael B.ORCID, Kielkopf John F.ORCID, Lester Katie V., Malavolta LucaORCID, Mann Andrew W.ORCID, Matson Rachel A.ORCID, Matthews Elisabeth C.ORCID, Nardiello DomenicoORCID, Narita NorioORCID, Pace EmanueleORCID, Pagano IsabellaORCID, Palle EnricORCID, Pedani Marco, Seager SaraORCID, Schlieder Joshua E., Schwarz Richard P., Shporer AviORCID, Twicken Joseph D.ORCID, Winn Joshua N.ORCID, Ziegler Carl, Zingales TizianoORCID
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Reference124 articles.
1. Cubillos, P. et al. An overabundance of low-density Neptune-like planets. Mon. Not. R. Astron. Soc. 466, 1868–1879 (2017). 2. Leleu, A. et al. Removing biases on the density of sub-Neptunes characterised via transit timing variations. Update on the mass-radius relationship of 34 Kepler planets. Astron. Astrophys. 669, A117 (2023). 3. Díaz, M. R. et al. The Magellan/PFS Exoplanet Search: a 55-d period dense Neptune transiting the bright (V = 8.6) star HD 95338. Mon. Not. R. Astron. Soc. 496, 4330–4341 (2020). 4. Armstrong, D. J. et al. A remnant planetary core in the hot-Neptune desert. Nature 583, 39–42 (2020). 5. Persson, C. M. et al. TOI-2196 b: rare planet in the hot Neptune desert transiting a G-type star. Astron. Astrophys. 666, 39–42 (2022).
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