Kervella, Pierre; Arenou, Frédéric; և այլք: (2019). «Stellar and substellar companions of nearby stars from Gaia DR2». Astronomy & Astrophysics. 623: A72. arXiv:1811.08902. Bibcode:2019A&A...623A..72K. doi:10.1051/0004-6361/201834371. ISSN0004-6361. S2CID119491061. «We also detect the signature of a possible planet of a few Jovian masses orbiting τ Ceti…The observed signal could be explained for example, by a Jupiter analog orbiting at 5au.»
Korolik, Maria; Roettenbacher, Rachael M.; և այլք: (2023 թ․ հուլիս). «Refining the Stellar Parameters of τ Ceti: a Pole-on Solar Analog». The Astronomical Journal. arXiv:2307.10394.
Tuomi, M; Jones, H R A; Jenkins, J S; Tinney, C G; Butler, R P; Vogt, S S; Barnes, J R; Wittenmyer, R A; o'Toole, S; Horner, J; Bailey, J; Carter, B D; Wright, D J; Salter, G S; Pinfield, D (2013). «Signals embedded in the radial velocity noise». Astronomy & Astrophysics. 551: A79. arXiv:1212.4277. Bibcode:2012yCat..35510079T. doi:10.1051/0004-6361/201220509. S2CID2390534.
Kervella, Pierre; Arenou, Frédéric; և այլք: (2019). «Stellar and substellar companions of nearby stars from Gaia DR2». Astronomy & Astrophysics. 623: A72. arXiv:1811.08902. Bibcode:2019A&A...623A..72K. doi:10.1051/0004-6361/201834371. ISSN0004-6361. S2CID119491061. «We also detect the signature of a possible planet of a few Jovian masses orbiting τ Ceti…The observed signal could be explained for example, by a Jupiter analog orbiting at 5au.»
Hall, J. C.; Lockwood, G. W.; Gibb, E. L. (1995). «Activity cycles in cool stars. 1: Observation and analysis methods and case studies of four well-observed examples». Astrophysical Journal. 442 (2): 778–793. Bibcode:1995ApJ...442..778H. doi:10.1086/175483.
Walker, Gordon A. H.; Walker Andrew H.; Irwin W. Alan; և այլք: (1995). «A Search for Jupiter-Mass Companions to Nearby Stars». Icarus. 116 (2): 359–375. Bibcode:1995Icar..116..359W. doi:10.1006/icar.1995.1130. However, this does not exclude the possibility of a large planet with a mass greater than Jupiter's and an orbital plane that is nearly perpendicular to the line of sight.
Tuomi, M; Jones, H R A; Jenkins, J S; Tinney, C G; Butler, R P; Vogt, S S; Barnes, J R; Wittenmyer, R A; o'Toole, S; Horner, J; Bailey, J; Carter, B D; Wright, D J; Salter, G S; Pinfield, D (2013). «Signals embedded in the radial velocity noise». Astronomy & Astrophysics. 551: A79. arXiv:1212.4277. Bibcode:2012yCat..35510079T. doi:10.1051/0004-6361/201220509. S2CID2390534.
Henry, Todd J. (2006 թ․ հոկտեմբերի 1). «The One Hundred Nearest Star Systems». Research Consortium on Nearby Stars. Արխիվացված է օրիգինալից 2006 թ․ նոյեմբերի 28-ին. Վերցված է 2006 թ․ դեկտեմբերի 11-ին.
Kervella, Pierre; Arenou, Frédéric; և այլք: (2019). «Stellar and substellar companions of nearby stars from Gaia DR2». Astronomy & Astrophysics. 623: A72. arXiv:1811.08902. Bibcode:2019A&A...623A..72K. doi:10.1051/0004-6361/201834371. ISSN0004-6361. S2CID119491061. «We also detect the signature of a possible planet of a few Jovian masses orbiting τ Ceti…The observed signal could be explained for example, by a Jupiter analog orbiting at 5au.»
Hall, J. C.; Lockwood, G. W.; Gibb, E. L. (1995). «Activity cycles in cool stars. 1: Observation and analysis methods and case studies of four well-observed examples». Astrophysical Journal. 442 (2): 778–793. Bibcode:1995ApJ...442..778H. doi:10.1086/175483.
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Walker, Gordon A. H.; Walker Andrew H.; Irwin W. Alan; և այլք: (1995). «A Search for Jupiter-Mass Companions to Nearby Stars». Icarus. 116 (2): 359–375. Bibcode:1995Icar..116..359W. doi:10.1006/icar.1995.1130. However, this does not exclude the possibility of a large planet with a mass greater than Jupiter's and an orbital plane that is nearly perpendicular to the line of sight.
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Tuomi, M; Jones, H R A; Jenkins, J S; Tinney, C G; Butler, R P; Vogt, S S; Barnes, J R; Wittenmyer, R A; o'Toole, S; Horner, J; Bailey, J; Carter, B D; Wright, D J; Salter, G S; Pinfield, D (2013). «Signals embedded in the radial velocity noise». Astronomy & Astrophysics. 551: A79. arXiv:1212.4277. Bibcode:2012yCat..35510079T. doi:10.1051/0004-6361/201220509. S2CID2390534.
陳輝樺, ed. (2006 թ․ հուլիսի 10). 天文教育資訊網 [Activities of Exhibition and Education in Astronomy (AEEA)] (չինարեն). Արխիվացված է օրիգինալից 2011 թ․ հուլիսի 16-ին. Վերցված է 2024 թ․ հունվարի 24-ին.
Kervella, Pierre; Arenou, Frédéric; և այլք: (2019). «Stellar and substellar companions of nearby stars from Gaia DR2». Astronomy & Astrophysics. 623: A72. arXiv:1811.08902. Bibcode:2019A&A...623A..72K. doi:10.1051/0004-6361/201834371. ISSN0004-6361. S2CID119491061. «We also detect the signature of a possible planet of a few Jovian masses orbiting τ Ceti…The observed signal could be explained for example, by a Jupiter analog orbiting at 5au.»
Tuomi, M; Jones, H R A; Jenkins, J S; Tinney, C G; Butler, R P; Vogt, S S; Barnes, J R; Wittenmyer, R A; o'Toole, S; Horner, J; Bailey, J; Carter, B D; Wright, D J; Salter, G S; Pinfield, D (2013). «Signals embedded in the radial velocity noise». Astronomy & Astrophysics. 551: A79. arXiv:1212.4277. Bibcode:2012yCat..35510079T. doi:10.1051/0004-6361/201220509. S2CID2390534.
Torres, Abel Mendez (2012 թ․ դեկտեմբերի 28). «Two Nearby Habitable Worlds?». Planetary Habitability Laboratory. University of Puerto Rico. Արխիվացված է օրիգինալից 2021 թ․ մարտի 8-ին. Վերցված է 2013 թ․ մարտի 22-ին.
Torres, Abel Mendez (2012 թ․ դեկտեմբերի 28). «Two Nearby Habitable Worlds?». Planetary Habitability Laboratory. University of Puerto Rico. Արխիվացված է օրիգինալից 2021 թ․ մարտի 8-ին. Վերցված է 2013 թ․ մարտի 22-ին.
陳輝樺, ed. (2006 թ․ հուլիսի 10). 天文教育資訊網 [Activities of Exhibition and Education in Astronomy (AEEA)] (չինարեն). Արխիվացված է օրիգինալից 2011 թ․ հուլիսի 16-ին. Վերցված է 2024 թ․ հունվարի 24-ին.
Henry, Todd J. (2006 թ․ հոկտեմբերի 1). «The One Hundred Nearest Star Systems». Research Consortium on Nearby Stars. Արխիվացված է օրիգինալից 2006 թ․ նոյեմբերի 28-ին. Վերցված է 2006 թ․ դեկտեմբերի 11-ին.
Kervella, Pierre; Arenou, Frédéric; և այլք: (2019). «Stellar and substellar companions of nearby stars from Gaia DR2». Astronomy & Astrophysics. 623: A72. arXiv:1811.08902. Bibcode:2019A&A...623A..72K. doi:10.1051/0004-6361/201834371. ISSN0004-6361. S2CID119491061. «We also detect the signature of a possible planet of a few Jovian masses orbiting τ Ceti…The observed signal could be explained for example, by a Jupiter analog orbiting at 5au.»