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Two Sub-Neptunes Around the M Dwarf TOI-1470

E. Gonzalez-Alvarez,M. R. Zapatero Osorio,J. A. Caballero,V. J. S. Bejar,C. Cifuentes,A. Fukui,E. Herrero,K. Kawauchi,J. H. Livingston,M. J. Lopez-Gonzalez,G. Morello,F. Murgas,N. Narita,E. Palle,V. M. Passegger,E. Rodriguez,C. Rodriguez-Lopez,J. Sanz-Forcada,A. Schweitzer,H. M. Tabernero,A. Quirrenbach,P. J. Amado,D. Charbonneau,D. R. Ciardi,S. Cikota,K. A. Collins,D. M. Conti,M. Fausnaugh,A. P. Hatzes,C. Hedges,Th. Henning,J. M. Jenkins,D. W. Latham,B. Massey,D. Moldovan,D. Montes,A. Panahi,A. Reiners,I. Ribas,G. R. Ricker,S. Seager,A. Shporer,G. Srdoc,P. Tenenbaum,R. Vanderspek,J. N. Winn,I. Fukuda,M. Ikoma,K. Isogai,Y. Kawai, M. Mori,M. Tamura,N. Watanabe

ASTRONOMY & ASTROPHYSICS（2023）

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关键词
techniques,photometric,radial velocities,stars,individual,TOI-1470,late-type,planetary systems
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