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Table B.1.

Properties of the targets observed with the ARCES spectrometer.

KIC Visit mKep dGaia RGaia Rast Mast Teff, Gaia Teff, apg log gapg [Fe/H]apg Hosc νmax Δν ΔΠ1 Sph Prot σRV vsin90 Evol Comment Literature
pc R R M K K dex dex ppm2μHz−1 μHz μHz s % days km s−1 km s−1
3.5 m APO without oscillations

2441154 1 10.33 577(8) 8.91(64) 4536(159) 0.00 1.32 32.0 0.00 SB from APOGEE
2852961 4 10.15 762(15) 10.05(46) 4645(93) 1.10 35.5 10.41 SB1, flares, DR16 (2 vis) Flares Bal15, Pug2016, Kat18
3459199 4 10.05 990(30) 12.46(64) 5340(107) 5008 2.64 −0.09 0.00 11.6 11.83 12.0 SB1, EB signal EB contamination Sch12
4278024 3 11.48 959(24) 8.39(63) 4711(165) 0.00 2.87 37.0 17.68 SB1, DR16 (4 vis)
5112741 1 12.45 2711(151) 15(1) 4659(93) 0.00 0.63 8.8 0.00 93.2 SB2
5166899 4 10.91 876(19) 8.54(63) 4762(167) 4741 2.95 −0.05 1.57 23.8 28.50 SB2, faint star within 2 pix, faint Li line
5182131 2 12.41 1495(50) 7.14(56) 4975(174) 0.00 2.36 76.0 12.85 SB1
5437763 2 11.79 1438(50) 10.26(81) 4696(164) 4523 3.04 −0.15 0.56 14.0 16.72 SB1.
5630212 2 10.21 560(10) 9.74(70) 3999(140) 0.00 3.89 31.1 15.17 3.0 SB1, faint Li line
5821762 3 12.30 2734(204) 13(1) 5209(182) 5205 2.68 0.05 0.47 9.2 10.08 Unclear, BF 120 km s−1
6372268 5 11.45 645(11) 6.57(48) 4014(140) 0.00 7.81 5.2 39.12 52.4 SB2, Kep EB, BF 120 km s−1, X-ray How16
6522973 2 11.80 1877(80) 15(1) 4556(159) 4385 2.68 −0.04 0.59 30.3 2.02 SB1
6707805 1 12.45 1621(71) 6.79(41) 5259(105) 0.00 1.76 22.0 0.00 SB2, faint Li line
7552750 2 12.29 1252(62) 5.47(48) 5236(183) 0.00 0.16 101.0 5.20 SB1
7869590 7 10.88 629(10) 7.18(52) 4647(163) 4370 3.22 0.26 3.53 40.5 13.84 9.5 SB1, no clear Hα line Long term var Tan12
7899428 1 11.34 598(10) 4.53(33) 4915(172) 0.00 3.71 11.5 0.00 SB3, Li line
8517303 2 11.43 851(18) 8.06(38) 4554(91) 4547 3.08 −0.10 5.51 53.5 6.41 SB1
8749284 3 12.19 1002(25) 7.97(38) 4424(88) 1.52 3.5 8.34 Unclear, BF 100 km s−1, Hα em.
8822505 3 11.80 1369(48) 10.30(81) 4729(166) 4422 2.91 −0.09 3.01 40.0 7.90 SB1
9770992 4 10.53 1249(98) 14(2) 4921(172) 0.00 1.78 17.8 35.93 SB2
10297952 2 11.49 1215(34) 9.29(71) 3787(133) 4484 3.33 −0.51 3.01 17.6 10.16 SB1, DR16 (2 vis)
10908111 2 12.12 1585(65) 8.83(72) 4908(172) 4473 2.55 −0.13 1.54 13.6 29.04 3.1 SB1/2
10991377 3 12.12 1950(112) 12(1) 4872(171) 4587 2.63 −0.07 1.36 15.7 7.00 5.0 Unclear, BF 75 km s−1, Li rich
11146520 2 12.42 1518(51) 7.78(61) 4832(169) 4608 2.87 −0.29 1.64 34.0 9.39 SB1
11551404 4 0.00 325(2) 2.67(19) 4968(174) 4703 3.62 −0.16 0.00 14.26 SB2, weak Hα abs., faint Li line Flares, wide binary candidate Dav16, Dea16, GR18
11554998 4 11.78 1082(26) 8.16(61) 4727(165) 4301 3.03 −0.13 5.80 30.4 22.04 SB1
11907579 3 12.06 2105(101) 12(1) 4998(175) 4679 2.84 0.08 0.53 14.9 0.27 RV stable, BF 60 km s−1, Li line
12118682 2 11.89 1674(66) 10.77(87) 4918(172) 4515 2.81 −0.26 2.03 45.0 18.24 SB1
12157366 2 12.47 1765(87) 11.21(97) 4483(157) 0.00 1.67 18.1 2.77 3.9 SB1
12406908 1 12.35 789(13) 4.47(32) 4585(160) 0.00 5.30 13.4 0.00 SB2, Hα em., Ca II H K, triplet

3.5 m APO with oscillations

3654361 5 11.27 732(15) 4.77(22) 4.24(44) 1.39(43) 5066(101) 5109 3.36 −0.22 257(26) 18.10 82.70 0.25 41.5 0.61 5.2 RGB
5430224 7 11.01 1171(30) 10.81(81) 11.22(45) 2.05(25) 4949(173) 4899 3.19 0.05 111(19) 55(2) 5.09 1.11 55.0 0.70 10.3 RC
5514251 7 8.98 451(5) 10.17(72) 9.83(31) 0.884(87) 4944(173) 0.00 1373(172) 30.73(78) 4.08 260.90 0.44 33.0 0.85 15.1 RC Li rich
5559520 5 10.16 766(15) 10.71(79) 10.73(27) 1.078(86) 4875(171) 0.00 2853(202) 31.63(54) 3.95 239.80 0.25 41.0 0.74 13.2 RC
5633342 5 9.79 497(36) 6.69(68) 4.537(85) 1.58(10) 5136(180) 0.00 4.74(58) 253(2) 17.39 94.90 0.31 109.0 0.76 2.1 RGB DR16 (4 vis)
6221548 7 10.98 1075(42) 8.62(49) 8.42(12) 2.44(11) 5043(101) 5104 2.82 −0.06 57(3) 114(1) 8.55 184.10 0.82 102.0 0.83 4.2 RC
7103951 5 9.38 515(10) 9.40(42) 10.71(16) 1.795(87) 4906(98) 4902 2.95 0.02 637(31) 52.70(57) 5.11 304.10 0.25 75.0 2.60 7.2 RC SB1, DR16 (2 vis) Rapid rot. RG Cos15
7183551 7 8.23 327(3) 9.93(70) 9.99(39) 1.00(12) 4953(173) 0.00 860(121) 34(1) 4.23 0.26 36.3 0.55 13.9 ℓ = 1 dep.
7451465 5 11.33 1204(36) 8.36(64) 8.70(25) 3.04(28) 5204(182) 0.00 8(2) 131(3) 9.08 0.87 47.1 0.35 9.3 RGB? DR16 (4 vis)
7465993 5 10.70 748(19) 7.16(34) 7.078(92) 2.148(91) 5019(100) 5044 2.84 0.12 35(2) 143(1) 10.41 54.50 0.26 81.5 0.73 4.4 RGB ℓ = 1 dep.
7703954 5 9.42 593(8) 9.95(43) 9.94(16) 2.83(15) 5045(101) 5099 2.81 0.07 75(4) 95(1) 7.18 216.00 0.30 72.0 0.71 7.0 RC
7743728 5 10.93 957(32) 6.92(36) 6.25(17) 2.41(20) 5308(106) 5296 3.46 0.04 7(1) 200(5) 13.28 0.50 38.6 0.41 8.2 RGB
8160175 6 10.99 782(13) 7.30(32) 7.382(79) 1.270(46) 4741(95) 4743 2.83 0.03 840(24) 79.85(22) 7.51 73.00 3.86 69.8 0.99 5.3 RGB Likely contamination activity
8326469 5 8.40 334(3) 8.56(61) 8.36(17) 2.44(17) 5203(182) 0.00 63(3) 114(1) 8.64 248.30 0.48 144.0 0.66 2.9 RC faint star within 2 pix Flares Hon16
8515227 7 11.18 1172(57) 10.94(71) 4.286(74) 0.939(48) 4706(94) 4778 3.17 −0.68 11.21(86) 176(2) 14.60 82.20 0.99 28.0 23.66 7.7 RGB SB3, DR16 (2 vis)
8816525 6 8.91 499(7) 10.16(44) 9.90(15) 2.28(11) 5058(101) 5084 2.76 0.05 215(9) 77.29(85) 6.49 274.40 0.23 68.5 1.05 7.3 RC faint Li line
9788756 6 11.38 999(23) 7.75(58) 7.94(39) 1.75(23) 4843(170) 4903 3.05 −0.10 59(5) 94(3) 7.90 218.00 2.75 95.0 0.57 4.2 RC Very low modes
10198347 5 10.29 1020(27) 11.40(86) 10.81(24) 1.42(10) 5191(182) 4924 2.96 −0.16 2282(139) 39.65(50) 4.47 276.60 0.28 45.6 2.84 12.0 RC SB2 Anom. rot. Tay15
10461323 7 10.01 642(9) 8.56(38) 8.95(17) 2.14(13) 4902(98) 4874 2.99 0.12 88(5) 90(1) 7.30 0.53 79.7 0.66 5.7 ℓ = 1 dep.
10793890 6 9.95 675(13) 8.04(59) 8.49(17) 2.49(16) 5310(186) 5113 2.79 0.04 70(3) 111.51(98) 8.51 267.70 0.29 130.0 0.64 3.3 RC
11037219 7 10.22 680(15) 7.97(59) 8.49(17) 2.44(16) 5064(177) 4947 3.10 0.25 80(3) 112.14(98) 8.44 146.50 0.34 140.0 0.75 3.1 RC faint star within 2 pix
11087027 8 10.88 1238(103) 14(2) 13(5) 2(2) 4918(172) 252(94) 33(12) 3.70 0.63 30.5 0.77 21.1 Flares, Li rich, Hα em.
12266731 5 10.21 899(19) 9.72(44) 9.62(16) 2.72(14) 5152(103) 5104 2.84 0.15 92(5) 97(1) 7.40 246.90 0.21 79.0 0.56 6.2 RC Star nearby

Notes. Columns report KIC identification number, number of epochs of spectroscopic observations, Gaia distance dGaia and radius RGaia, asteroseismic radius Rast, and mass Mast, Gaia effective temperature Teff, Gaia, SDSS/APOGEE (DR16) temperature Teff, apg, surface gravity log gapg and metallicity [Fe/H]apg, height of oscillation envelope Hosc, frequency at maximum amplitude νmax and mean frequency separation Δν of the oscillations, mean l = 1 mixed-mode period spacing ΔΠ1, photometric activity index Sph, rotation period Prot, RV standard deviation σRV, and v sin (i = 90° ). Evolutionary status, comments, and literature information are reported in the last three columns. When errors are available, the least significant digits in brackets after the value indicates the uncertainty. Among the comments, the abbreviation “BF x km s−1” indicates the width of the broadening function (Rucinski 2002), which is used to point out fast rotators. The abbreviation “Li line” or “Li rich” indicate when the Lithium absorption line at 6707.7 Å is clearly detectable or very deep.

References. Bal15 Balona (2015); Cei17 Ceillier et al. (2017); Cos15 Costa et al. (2015); Dav16 Davenport (2016); Dea16 Deacon et al. (2016); GR18 Godoy-Rivera & Chanamé (2018); Hwl16 Howell et al. (2016); Hnd16 Houdek et al. (2016); Kat18 Katsova et al. (2018); Kum18 Bharat Kumar et al. (2018); Pug16 Pugh et al. (2016); Sch12 Schwamb et al. (2012); Tan12 Tang (2012); Tay15 Tayar et al. (2015)

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