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==References== {{reflist|colwidth=25em|refs= <ref name=Rains2020>{{Cite journal |last1=Rains |first1=Adam D. |last2=Ireland |first2=Michael J. |last3=White |first3=Timothy R. |last4=Casagrande |first4=Luca |last5=Karovicova |first5=I. |date=2020-04-01 |title=Precision angular diameters for 16 southern stars with VLTI/PIONIER |arxiv=2004.02343 |journal=Monthly Notices of the Royal Astronomical Society |volume=493 |issue=2 |pages=2377–2394 |doi=10.1093/mnras/staa282 |doi-access=free |bibcode=2020MNRAS.493.2377R |issn=0035-8711}}</ref> <ref name=aaa474_2_653>{{citation | first1=Floor | last1=van Leeuwen |date=November 2007 | title=Validation of the new Hipparcos reduction | volume=474 | issue=2 | pages=653–664 | bibcode=2007A&A...474..653V | arxiv=0708.1752v1 | doi=10.1051/0004-6361:20078357 | journal=Astronomy and Astrophysics | s2cid=18759600 | postscript=. }} ''Note:'' see VizieR catalogue [http://vizier.u-strasbg.fr/viz-bin/Cat?I/311 I/311].</ref> <ref name=SIMBAD>{{citation | url=http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V*+eps+Eri | title=V* eps Eri – variable of BY Dra type | work=[[SIMBAD]] | publisher=[[Centre de Données astronomiques de Strasbourg]] | access-date=November 5, 2010 | postscript=. }}</ref> <ref name=aj132_1_161>{{citation | display-authors=1 | last1=Gray | first1=R. 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C. | last3=Fischer |first3=Debra A. |last4=Monnier |first4=John D. | last5=Henry |first5=Gregory W. |last6=Harmon |first6=Robert O. | last7=Korhonen |first7=Heidi |last8=Brewer |first8=John M. | last9=Llama |first9=Joe |last10=Petersburg |first10=Ryan R. | last11=Zhao |first11=Lily L. |last12=Kraus |first12=Stefan | last13=Le Bouquin |first13=Jean-Baptiste |last14=Anugu |first14=Narsireddy | last15=Davies |first15=Claire L. |last16=Gardner |first16=Tyler | last17=Lanthermann |first17=Cyprien |last18=Schaefer |first18=Gail | last19=Setterholm |first19=Benjamin |last20=Clark |first20=Catherine A. | last21=Jorstad |first21=Svetlana G. |last22=Kuehn |first22=Kyler | last23=Levine |first23=Stephen | title=EXPRES. III. Revealing the Stellar Activity Radial Velocity Signature of ϵ Eridani with Photometry and Interferometry | journal=The Astronomical Journal |date=January 2022 |volume=163 |issue=1 |page=19 |doi=10.3847/1538-3881/ac3235 |s2cid=239049996 |arxiv=2110.10643 |bibcode=2022AJ....163...19R | doi-access=free }}</ref> <ref name=apj460_993>{{citation | display-authors=1 | last1=Saumon | first1=D. | last2=Hubbard | first2=W. B. | last3=Burrows | first3=A. | last4=Guillot6 | first4=T. | last5=Lunine | first5=J. I. | last6=Chabrier | first6=G. | title=A theory of extrasolar giant planets | journal=The Astrophysical Journal | volume=460 | pages=993–1018 |date=April 1996 | doi=10.1086/177027 | bibcode=1996ApJ...460..993S | arxiv=astro-ph/9510046| s2cid=18116542 | postscript=. }} See Table A1, p. 21.</ref> <ref name=aaa411_3_559>{{citation | display-authors=1 | last1=Kovtyukh | first1=V. V. | last2=Soubiran | first2=C. | last3=Belik | first3=S. I. | last4=Gorlova | first4=N. I. | title=High precision effective temperatures for 181 F-K dwarfs from line-depth ratios | journal=Astronomy and Astrophysics | volume=411 | issue=3 | pages=559–564 |date=December 2003 | doi=10.1051/0004-6361:20031378 | arxiv=astro-ph/0308429 | bibcode=2003A&A...411..559K | s2cid=18478960 | postscript=. }}</ref> <ref name=aaa415>{{citation | last1=Santos | first1=N. C. | last2=Israelian | first2=G. | last3=Mayor | first3=M. | title=Spectroscopic <nowiki>[Fe/H]</nowiki> for 98 extra-solar planet-host stars: Exploring the probability of planet formation | journal=Astronomy and Astrophysics |date=March 2004 | volume=415 | issue=3 | pages=1153–1166 | doi=10.1051/0004-6361:20034469 | arxiv=astro-ph/0311541 | bibcode=2004A&A...415.1153S | s2cid=11800380 | postscript=. }}—the percentage of iron is given by <math>\begin{smallmatrix}10^{-0.13} = 0.74\end{smallmatrix}</math>, or 74%</ref> <ref name=an328_10>{{citation | last1=Fröhlich | first1=H.-E. | title=The differential rotation of Epsilon Eri from MOST data | journal=[[Astronomische Nachrichten]] | volume=328 | issue=10 | pages=1037–1039 |date=December 2007 | doi=10.1002/asna.200710876 | bibcode=2007AN....328.1037F | arxiv=0711.0806 | s2cid=11263751 | postscript=. }}</ref> <ref name=aaa426>{{citation | display-authors=1 | last1=Di Folco | first1=E. | last2=Thévenin | first2=F. | last3=Kervella | first3=P. | last4=Domiciano de Souza | first4=A. | last5=Coudé du Foresto | first5=V. | last6=Ségransan | first6=D. | last7=Morel | first7=P. | title=VLTI near-IR interferometric observations of Vega-like stars. 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P.|last2=Lemarchand|first2=G. A.|last3=Mauas|first3=P. J. D. |title=Ultraviolet radiation constraints around the circumstellar habitable zones|journal=Icarus|volume=183|issue=2|year=2006|pages=491–503|issn=0019-1035|arxiv=astro-ph/0512291|doi=10.1016/j.icarus.2006.03.007|bibcode=2006Icar..183..491B|s2cid=2241081|quote=<span style="font-family:LatinModern;">In near the 41% stars of the sample: HD19994, 70 Vir, 14 Her, 55 Cnc, 47 UMa, ε Eri and HD3651, there is no coincidence at all between the UV region and the HZ...the traditional HZ would not be habitable following the UV criteria exposed in this work.</span>}}</ref> <ref name="SuDe Buizer2017">{{citation | postscript=. |last1=Su|first1=Kate Y. 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Fritz |date=March 2022 |title=Revisiting HST/FGS Astrometry of epsilon Eridani |journal=[[Research Notes of the AAS]] |volume=6 |issue=3 |page=45 |doi=10.3847/2515-5172/ac5b6b |bibcode=2022RNAAS...6...45B |doi-access=free }}</ref> <ref name="Feng2023">{{cite journal |last1=Feng |first1=Fabo |last2=Butler |first2=R. Paul |display-authors=etal |date=July 2023 |title=Revised orbits of the two nearest Jupiters |journal=[[Monthly Notices of the Royal Astronomical Society]] |volume= 525|issue=1 |pages= 607–619|doi= 10.1093/mnras/stad2297|doi-access=free |arxiv=2307.13622|bibcode=2023MNRAS.525..607F }}</ref> }}
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