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Cited article:

No Transits of Proxima Centauri Planets in High-Cadence TESS Data

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A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU

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Proxima Centauri b is not a transiting exoplanet

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Monthly Notices of the Royal Astronomical Society 487 (1) 268 (2019)
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Flaring Activity of Proxima Centauri from TESS Observations: Quasiperiodic Oscillations during Flare Decay and Inferences on the Habitability of Proxima b

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Stellar and substellar companions of nearby stars from Gaia DR2

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Upper limits for mass and radius of objects around Proxima Cen from SPHERE/VLT

D. Mesa, A. Zurlo, J. Milli, R. Gratton, S. Desidera, M. Langlois, A. Vigan, M. Bonavita, J. Antichi, H. Avenhaus, A. Baruffolo, B. Biller, A. Boccaletti, P. Bruno, E. Cascone, G. Chauvin, R. U. Claudi, V. De Caprio, D. Fantinel, G. Farisato, J. Girard, E. Giro, J. Hagelberg, S. Incorvaia, M. Janson, et al.
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Optical, UV, and X-ray evidence for a 7-yr stellar cycle in Proxima Centauri

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No Conclusive Evidence for Transits of Proxima b in MOST Photometry

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Searching for faint comoving companions to the α Centauri system in the VVV survey infrared images

J. C. Beamín, D. Minniti, J. B. Pullen, et al.
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A terrestrial planet candidate in a temperate orbit around Proxima Centauri

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ON THE METHOD TO INFER AN ATMOSPHERE ON A TIDALLY LOCKED SUPER EARTH EXOPLANET AND UPPER LIMITS TO GJ 876d

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