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NGTS-EB-8: A Double-lined Eclipsing M+M Binary Discovered by Citizen Scientists

  • Authors: Sean M. O'Brien, Megan E. Schwamb, Christopher A. Watson, Louise D. Nielsen, Edward M. Bryant, Sarah L. Casewell, Matthew R. Burleigh, Lucy Fortson, Samuel Gill, Chris J. Lintott, Katlyn L. Hobbs, Ioannis Apergis, Daniel Bayliss, Jorge Fernández Fernández, Maximilian N. Günther, Faith Hawthorn, James S. Jenkins, Alicia Kendall, James McCormac, Ernst J. W. de Mooij, Toby Rodel, Suman Saha, Laura Trouille, Richard G. West, Peter J. Wheatley, Marius Constantin Agafitei, Deniz Rüzgar Apaydın, Elisabeth Baeten, Bruce Baller, Jeff Carabott, Sallyann Chesson, Sebastián Alejandro Freigeiro, Virgilio Gonano, Matthias Hanke, Pete Hermes, Avery Hildebrand, John S. Langley, See Min Lim, Leo Ryan McCarthy, Graham Mitchell, Ken O'Neill, Charles R. Pearson, Nolan Reket, Jeanne Riethmiller, Juergen Saeftel, Arttu Sainio, Charlie Steiner, Amanda Strickland, Christopher Tanner, Ivan A. Terentev, Ernest Jude P. Tiu, Sergey Y. Tumanov, Marciniak Urszula, Pia Vahlenkamp, Femke de Vroome, Paweł Wantuch, Timothy Woodruff

Sean M. O’Brien et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 14.

Secondary radius vs. host stellar mass for low-mass stars hosting confirmed exoplanets, TOIs, and candidates identified in B23. Colored by disposition as described for Figure 13. The previously assumed position of NGTS-EB-8 when it was described as a planet candidate in S. M. O’Brien et al. (2024) is plotted as an unfilled magenta star, and the position of NGTS-EB-8 as determined by the high k-range model from this work is shown as a filled cyan star.

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