Christiansen, J. L.J. L.Christiansen0000-0002-9900-4751Vanderburg, A.A.Vanderburg0000-0002-6492-2085Burt, J.J.Burt0000-0003-1784-1431Fulton, B. J.B. J.Fulton0000-0002-1742-7735Batygin, K.K.Batygin0000-0002-7504-365XBenneke, B.B.BennekeBrewer, J. M.J. M.BrewerCharbonneau, D.D.CharbonneauCiardi, D. R.D. R.CiardiCameron, A. C.A. C.CameronCoughlin, J. L.J. L.CoughlinCrossfield, I. J. M.I. J. M.CrossfieldDressing, C.C.DressingGreene, T. P.T. P.GreeneHoward, A. W.A. W.HowardLatham, D. W.D. W.LathamMOLINARI, Emilio CarloEmilio CarloMOLINARIMortier, A.A.MortierMullally, F.F.MullallyPepe, F.F.PepeRice, K.K.RiceSinukoff, E.E.SinukoffSOZZETTI, AlessandroAlessandroSOZZETTIThompson, S. E.S. E.ThompsonUdry, S.S.UdryVogt, S. S.S. S.VogtBarman, T. S.T. S.BarmanBatalha, N. E.N. E.BatalhaBouchy, F.F.BouchyBuchhave, L. A.L. A.BuchhaveButler, R. P.R. P.ButlerCosentino, R.R.CosentinoDupuy, T. J.T. J.DupuyEhrenreich, D.D.EhrenreichFiorenzano, A.A.FiorenzanoHansen, B. M. S.B. M. S.HansenHenning, T.T.HenningHirsch, L.L.HirschHolden, B. P.B. P.HoldenIsaacson, H. T.H. T.IsaacsonJohnson, J. A.J. A.JohnsonKnutson, H. A.H. A.KnutsonKosiarek, M.M.KosiarekLopez-Morales, M.M.Lopez-MoralesLovis, C.C.LovisMalavolta, L.L.MalavoltaMayor, M.M.MayorMICELA, GiuseppinaGiuseppinaMICELAMotalebi, F.F.MotalebiPetigura, E.E.PetiguraPhillips, D. F.D. F.PhillipsPiotto, G.G.PiottoRogers, L. A.L. A.RogersSasselov, D.D.SasselovSchlieder, J. E.J. E.SchliederSegransan, D.D.SegransanWatson, C. A.C. A.WatsonWeiss, L. M.L. M.Weiss2022-03-012022-03-012018http://hdl.handle.net/20.500.12386/31511The final data set includes observations obtained with Keck/HIRES, Automated Planet Finder (APF)/Levy, and HARPS-N. Our observational setup for both Keck/HIRES and the APF/Levy was essentially identical to those described in Fulton et al. (2016, J/ApJ/830/46) and Burt et al. (2014ApJ...789..114B). We collected a total of 60 RV measurements using Keck/HIRES (Vogt et al. 1994SPIE.2198..362V), and 116 measurements using the Levy Spectrograph on the APF (Radovan et al. 2014SPIE.9145E..2BR; Vogt et al. 2014PASP..126..359V) at Lick Observatory between 2016 July 7 and 2016 December 2. We also observed HD 3167 with the HARPS-N spectrograph (Cosentino et al. 2012SPIE.8446E..1VC) located at the 3.58 m Telescopio Nazionale Galileo on the island of La Palma, Spain. HARPS-N is a stabilized spectrograph designed for precise RV measurements. We observed HD 3167 76 times between 2016 July 7 (independently beginning the same night as the HIRES/APF campaign) and 2016 December 7, obtaining high-resolution optical spectra with a spectral resolving power of R=115000. <P />(1 data file).enDatabase10.26093/cds/vizier.51540122https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/154/1222018yCat..51540122CFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_2 Planetary systems sciences