Publisher Correction: A super-Earth and two sub-Neptunes transiting the nearby and quiet M dwarf TOI-270 (Nature Astronomy, (2019), 3, 12, (1099-1108), 10.1038/s41550-019-0845-5)

  • Maximilian N. Günther
  • , Francisco J. Pozuelos
  • , Jason A. Dittmann
  • , Diana Dragomir
  • , Stephen R. Kane
  • , Tansu Daylan
  • , Adina D. Feinstein
  • , Chelsea X. Huang
  • , Timothy D. Morton
  • , Andrea Bonfanti
  • , L. G. Bouma
  • , Jennifer Burt
  • , Karen A. Collins
  • , Jack J. Lissauer
  • , Elisabeth Matthews
  • , Benjamin T. Montet
  • , Andrew Vanderburg
  • , Songhu Wang
  • , Jennifer G. Winters
  • , George R. Ricker
  • Roland K. Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, James D. Armstrong, Khalid Barkaoui, Natalie Batalha, Jacob L. Bean, Douglas A. Caldwell, David R. Ciardi, Kevin I. Collins, Ian Crossfield, Michael Fausnaugh, Gabor Furesz, Tianjun Gan, Michaël Gillon, Natalia Guerrero, Keith Horne, Steve B. Howell, Michael Ireland, Giovanni Isopi, Emmanuël Jehin, John F. Kielkopf, Sebastien Lepine, Franco Mallia, Rachel A. Matson, Gordon Myers, Enric Palle, Samuel N. Quinn, Howard M. Relles, Bárbara Rojas-Ayala, Joshua Schlieder, Ramotholo Sefako, Avi Shporer, Juan C. Suárez, Thiam Guan Tan, Eric B. Ting, Joseph D. Twicken, Ian A. Waite

Producción científica: Contribución a una revistaComentario/Debate

1 Cita (Scopus)

Resumen

In the version of this Letter originally published, a technical issue led to data points shifting in Fig. 1a; the correct version is shown below. In addition, in the second paragraph, M and R—the mass and radius of the Sun, respectively—were incorrectly defined as the mass and radius of the Earth. The Letter has now been corrected accordingly.

Idioma originalInglés
Páginas (desde-hasta)1157-1158
Número de páginas2
PublicaciónNature Astronomy
Volumen3
N.º12
DOI
EstadoPublicada - 1 dic. 2019
Publicado de forma externa

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Profundice en los temas de investigación de 'Publisher Correction: A super-Earth and two sub-Neptunes transiting the nearby and quiet M dwarf TOI-270 (Nature Astronomy, (2019), 3, 12, (1099-1108), 10.1038/s41550-019-0845-5)'. En conjunto forman una huella única.

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