The discovery name of this star is LP 816-60,[12] which indicates that its discovery was published between 1963 and 1981 in University of Minnesota, Minneapolis.[13] LP 816-60 is known at least from 1979, when it was included to Luyten's catalogue NLTT.[10]
No massive planets were detected around LP 816-60 as in 2013.[3] The star has a magnetic starspot cycle of 10.6±1.7 years,[9] and weak magnetic fields in chromosphere averaging 4.4 G.[14]
^ abcdPerryman; et al. (1997). "HIP 103039". The Hipparcos and Tycho Catalogues. Retrieved 2014-11-29.
^Cite error: The named reference Koen2010 was invoked but never defined (see the help page).
^ abcMontet, Benjamin T.; Crepp, Justin R.; Johnson, John Asher; Howard, Andrew W.; Marcy, Geoffrey W. (2013), "The Trends High-Contrast Imaging Survey. Iv. The Occurrence Rate of Giant Planets Around M Dwarfs", The Astrophysical Journal, 781: 28, arXiv:1307.5849, doi:10.1088/0004-637X/781/1/28, S2CID26620552
^Henry, Todd J.; Jao, Wei-Chun; Winters, Jennifer G.; Dieterich, Sergio B.; Finch, Charlie T.; Ianna, Philip A.; Riedel, Adric R.; Silverstein, Michele L.; Subasavage, John P.; Vrijmoet, Eliot Halley (2018), "The Solar Neighborhood XLIV: RECONS Discoveries within 10 parsecs", The Astronomical Journal, 155 (6): 265, arXiv:1804.07377, Bibcode:2018AJ....155..265H, doi:10.3847/1538-3881/aac262, S2CID53983430
^Moutou, C.; Hébrard, E. M.; Morin, J.; Malo, L.; Fouqué, P.; Torres-Rivas, A.; Martioli, E.; Delfosse, X.; Artigau, E.; Doyon, R. (2017), "SPIRou input catalogue: Activity, rotation and magnetic field of cool dwarfs", Monthly Notices of the Royal Astronomical Society, 472 (4): 4563–4586, arXiv:1709.01650, Bibcode:2017MNRAS.472.4563M, doi:10.1093/mnras/stx2306