Targets and basic properties for the stars considered. The asteroseismic parameters νmax and Δν are taken from Huber et al. (2013). The Teff and [Fe/H] parameters are taken from the companion paper (Silva Aguirre et al. 2015).
KOI . | KIC . | ID . | νmax . | Δν . | Teff . | [Fe/H] . | Notes . |
---|---|---|---|---|---|---|---|
. | . | . | (μHz) . | (μHz) . | (K) . | (dex) . | . |
268 | 3425851 | 2038 ± 60 | 92.6 ± 1.5 | 6343 ± 85 | −0.04 ± 0.10 | ||
69 | 3544595 | Kepler-93 | 3366 ± 81 | 145.77 ± 0.45 | 5669 ± 75 | −0.18 ± 0.10 | Ballard et al. (2014) |
975 | 3632418 | Kepler-21 | 1153 ± 32 | 60.86 ± 0.55 | 6305 ± 50 | −0.03 ± 0.10 | Howell et al. (2012) |
280 | 4141376 | 2928 ± 97 | 128.8 ± 1.3 | 6134 ± 91 | −0.24 ± 0.10 | ||
281 | 4143755 | 1458 ± 57 | 77.2 ± 1.3 | 5622 ± 106 | −0.4 ± 0.11 | ||
244 | 4349452 | Kepler-25 | 2106 ± 50 | 98.27 ± 0.57 | 6270 ± 79 | −0.04 ± 0.10 | Steffen et al. (2012) |
108 | 4914423 | Kepler-103 | 1663 ± 56 | 81.5 ± 1.6 | 5845 ± 88 | 0.07 ± 0.11 | Marcy et al. (2014) |
123 | 5094751 | Kepler-109 | 1745 ± 117 | 91.1 ± 2.3 | 5952 ± 75 | −0.08 ± 0.10 | Marcy et al. (2014) |
85 | 5866724 | Kepler-65 | 1880 ± 60 | 89.56 ± 0.48 | 6169 ± 50 | 0.09 ± 0.08 | Chaplin et al. (2013) |
285 | 6196457 | Kepler-92 | 1299 ± 53 | 66.6 ± 1.1 | 5871 ± 94 | 0.17 ± 0.11 | Xie (2014) |
3158 | 6278762 | Kepler-444 | 4538 ± 144 | 179.64 ± 0.76 | 5046 ± 74 | −0.37 ± 0.09 | Campante et al. (2015) |
41 | 6521045 | Kepler-100 | 1502 ± 31 | 77.0 ± 1.1 | 5825 ± 75 | 0.02 ± 0.10 | Marcy et al. (2014) |
75 | 7199397 | 644 ± 8b | 38.9 ± 0.8b | 5824 ± 50a | −0.22 ± 0.08a | ||
269 | 7670943 | 1895 ± 73 | 88.6 ± 1.3 | 6463 ± 110 | 0.09 ± 0.11 | ||
274 | 8077137 | Kepler-128 | 1324 ± 39 | 68.8 ± 0.64 | 6105 ± 100 | −0.11 ± 0.07 | Xie (2014) |
260 | 8292840 | Kepler-126 | 1983 ± 37 | 92.85 ± 0.35 | 6205 ± 100 | −0.26 ± 0.07 | Rowe et al. (2014) |
122 | 8349582 | Kepler-95 | 1677 ± 90 | 83.6 ± 1.4 | 5699 ± 74 | 0.3 ± 0.10 | Marcy et al. (2014) |
245 | 8478994 | Kepler-37 | 4660 ± 50 | 178.7 ± 1.4 | 5417 ± 75 | −0.32 ± 0.07 | Barclay et al. (2013) |
370 | 8494142 | Kepler-145 | 1133 ± 81 | 61.8 ± 0.76 | 6144 ± 106 | 0.13 ± 0.10 | Xie (2014) |
5 | 8554498 | 1153 ± 76 | 61.98 ± 0.96 | 5945 ± 60 | 0.17 ± 0.05 | ||
319 | 8684730 | 938 ± 72b | 52.2 ± 0.7b | 5924 ± 50a | 0.17 ± 0.08a | ||
42 | 8866102 | Kepler-410 | 2014 ± 32 | 94.5 ± 0.60 | 6325 ± 75 | 0.01 ± 0.10 | Van Eylen et al. (2014) |
974 | 9414417 | 1115 ± 32 | 60.05 ± 0.27 | 6253 ± 75 | −0.13 ± 0.10 | ||
288 | 9592705 | 1008 ± 21 | 53.54 ± 0.32 | 6174 ± 92 | 0.22 ± 0.10 | ||
1925 | 9955598 | Kepler-409 | 3546 ± 119 | 153.18 ± 0.14 | 5460 ± 75 | 0.08 ± 0.10 | Marcy et al. (2014) |
263 | 10514430 | False-positive | 1303 ± 30 | 70.0 ± 1.0 | 5784 ± 98 | −0.11 ± 0.11 | |
275 | 10586004 | Kepler-129 | 1395 ± 40 | 69.2 ± 1.4 | 5770 ± 83 | 0.29 ± 0.10 | Rowe et al. (2014) |
2 | 10666592 | HAT-P7 | 1115 ± 110 | 59.22 ± 0.59 | 6350 ± 80 | 0.26 ± 0.08 | Pál et al. (2008) |
1612 | 10963065 | Kepler-408 | 2193 ± 48 | 103.2 ± 0.63 | 6104 ± 74 | −0.2 ± 0.10 | Marcy et al. (2014) |
276 | 11133306 | 2381 ± 95 | 107.9 ± 1.9 | 5982 ± 82 | −0.02 ± 0.10 | ||
246 | 11295426 | Kepler-68 | 2154 ± 13 | 101.57 ± 0.10 | 5793 ± 74 | 0.12 ± 0.07 | Gilliland et al. (2013) |
277 | 11401755 | Kepler-36 | 1250 ± 44 | 67.9 ± 1.2 | 5960 ± 80 | −0.24 ± 0.06 | Carter et al. (2012) |
262 | 11807274 | Kepler-50 | 1496 ± 56 | 75.71 ± 0.31 | 6225 ± 75 | −0.0 ± 0.08 | Steffen et al. (2013) |
7 | 11853905 | Kepler-4 | 1436 ± 42 | 74.4 ± 1.1 | 5781 ± 76 | 0.09 ± 0.10 | Borucki et al. (2010) |
72 | 11904151 | Kepler-10 | 2730 ± 280 | 118.2 ± 0.20 | 5647 ± 74 | −0.15 ± 0.10 | Batalha et al. (2011) |
KOI . | KIC . | ID . | νmax . | Δν . | Teff . | [Fe/H] . | Notes . |
---|---|---|---|---|---|---|---|
. | . | . | (μHz) . | (μHz) . | (K) . | (dex) . | . |
268 | 3425851 | 2038 ± 60 | 92.6 ± 1.5 | 6343 ± 85 | −0.04 ± 0.10 | ||
69 | 3544595 | Kepler-93 | 3366 ± 81 | 145.77 ± 0.45 | 5669 ± 75 | −0.18 ± 0.10 | Ballard et al. (2014) |
975 | 3632418 | Kepler-21 | 1153 ± 32 | 60.86 ± 0.55 | 6305 ± 50 | −0.03 ± 0.10 | Howell et al. (2012) |
280 | 4141376 | 2928 ± 97 | 128.8 ± 1.3 | 6134 ± 91 | −0.24 ± 0.10 | ||
281 | 4143755 | 1458 ± 57 | 77.2 ± 1.3 | 5622 ± 106 | −0.4 ± 0.11 | ||
244 | 4349452 | Kepler-25 | 2106 ± 50 | 98.27 ± 0.57 | 6270 ± 79 | −0.04 ± 0.10 | Steffen et al. (2012) |
108 | 4914423 | Kepler-103 | 1663 ± 56 | 81.5 ± 1.6 | 5845 ± 88 | 0.07 ± 0.11 | Marcy et al. (2014) |
123 | 5094751 | Kepler-109 | 1745 ± 117 | 91.1 ± 2.3 | 5952 ± 75 | −0.08 ± 0.10 | Marcy et al. (2014) |
85 | 5866724 | Kepler-65 | 1880 ± 60 | 89.56 ± 0.48 | 6169 ± 50 | 0.09 ± 0.08 | Chaplin et al. (2013) |
285 | 6196457 | Kepler-92 | 1299 ± 53 | 66.6 ± 1.1 | 5871 ± 94 | 0.17 ± 0.11 | Xie (2014) |
3158 | 6278762 | Kepler-444 | 4538 ± 144 | 179.64 ± 0.76 | 5046 ± 74 | −0.37 ± 0.09 | Campante et al. (2015) |
41 | 6521045 | Kepler-100 | 1502 ± 31 | 77.0 ± 1.1 | 5825 ± 75 | 0.02 ± 0.10 | Marcy et al. (2014) |
75 | 7199397 | 644 ± 8b | 38.9 ± 0.8b | 5824 ± 50a | −0.22 ± 0.08a | ||
269 | 7670943 | 1895 ± 73 | 88.6 ± 1.3 | 6463 ± 110 | 0.09 ± 0.11 | ||
274 | 8077137 | Kepler-128 | 1324 ± 39 | 68.8 ± 0.64 | 6105 ± 100 | −0.11 ± 0.07 | Xie (2014) |
260 | 8292840 | Kepler-126 | 1983 ± 37 | 92.85 ± 0.35 | 6205 ± 100 | −0.26 ± 0.07 | Rowe et al. (2014) |
122 | 8349582 | Kepler-95 | 1677 ± 90 | 83.6 ± 1.4 | 5699 ± 74 | 0.3 ± 0.10 | Marcy et al. (2014) |
245 | 8478994 | Kepler-37 | 4660 ± 50 | 178.7 ± 1.4 | 5417 ± 75 | −0.32 ± 0.07 | Barclay et al. (2013) |
370 | 8494142 | Kepler-145 | 1133 ± 81 | 61.8 ± 0.76 | 6144 ± 106 | 0.13 ± 0.10 | Xie (2014) |
5 | 8554498 | 1153 ± 76 | 61.98 ± 0.96 | 5945 ± 60 | 0.17 ± 0.05 | ||
319 | 8684730 | 938 ± 72b | 52.2 ± 0.7b | 5924 ± 50a | 0.17 ± 0.08a | ||
42 | 8866102 | Kepler-410 | 2014 ± 32 | 94.5 ± 0.60 | 6325 ± 75 | 0.01 ± 0.10 | Van Eylen et al. (2014) |
974 | 9414417 | 1115 ± 32 | 60.05 ± 0.27 | 6253 ± 75 | −0.13 ± 0.10 | ||
288 | 9592705 | 1008 ± 21 | 53.54 ± 0.32 | 6174 ± 92 | 0.22 ± 0.10 | ||
1925 | 9955598 | Kepler-409 | 3546 ± 119 | 153.18 ± 0.14 | 5460 ± 75 | 0.08 ± 0.10 | Marcy et al. (2014) |
263 | 10514430 | False-positive | 1303 ± 30 | 70.0 ± 1.0 | 5784 ± 98 | −0.11 ± 0.11 | |
275 | 10586004 | Kepler-129 | 1395 ± 40 | 69.2 ± 1.4 | 5770 ± 83 | 0.29 ± 0.10 | Rowe et al. (2014) |
2 | 10666592 | HAT-P7 | 1115 ± 110 | 59.22 ± 0.59 | 6350 ± 80 | 0.26 ± 0.08 | Pál et al. (2008) |
1612 | 10963065 | Kepler-408 | 2193 ± 48 | 103.2 ± 0.63 | 6104 ± 74 | −0.2 ± 0.10 | Marcy et al. (2014) |
276 | 11133306 | 2381 ± 95 | 107.9 ± 1.9 | 5982 ± 82 | −0.02 ± 0.10 | ||
246 | 11295426 | Kepler-68 | 2154 ± 13 | 101.57 ± 0.10 | 5793 ± 74 | 0.12 ± 0.07 | Gilliland et al. (2013) |
277 | 11401755 | Kepler-36 | 1250 ± 44 | 67.9 ± 1.2 | 5960 ± 80 | −0.24 ± 0.06 | Carter et al. (2012) |
262 | 11807274 | Kepler-50 | 1496 ± 56 | 75.71 ± 0.31 | 6225 ± 75 | −0.0 ± 0.08 | Steffen et al. (2013) |
7 | 11853905 | Kepler-4 | 1436 ± 42 | 74.4 ± 1.1 | 5781 ± 76 | 0.09 ± 0.10 | Borucki et al. (2010) |
72 | 11904151 | Kepler-10 | 2730 ± 280 | 118.2 ± 0.20 | 5647 ± 74 | −0.15 ± 0.10 | Batalha et al. (2011) |
Notes.aBuchhave et al. (2012). bThis work.
Targets and basic properties for the stars considered. The asteroseismic parameters νmax and Δν are taken from Huber et al. (2013). The Teff and [Fe/H] parameters are taken from the companion paper (Silva Aguirre et al. 2015).
KOI . | KIC . | ID . | νmax . | Δν . | Teff . | [Fe/H] . | Notes . |
---|---|---|---|---|---|---|---|
. | . | . | (μHz) . | (μHz) . | (K) . | (dex) . | . |
268 | 3425851 | 2038 ± 60 | 92.6 ± 1.5 | 6343 ± 85 | −0.04 ± 0.10 | ||
69 | 3544595 | Kepler-93 | 3366 ± 81 | 145.77 ± 0.45 | 5669 ± 75 | −0.18 ± 0.10 | Ballard et al. (2014) |
975 | 3632418 | Kepler-21 | 1153 ± 32 | 60.86 ± 0.55 | 6305 ± 50 | −0.03 ± 0.10 | Howell et al. (2012) |
280 | 4141376 | 2928 ± 97 | 128.8 ± 1.3 | 6134 ± 91 | −0.24 ± 0.10 | ||
281 | 4143755 | 1458 ± 57 | 77.2 ± 1.3 | 5622 ± 106 | −0.4 ± 0.11 | ||
244 | 4349452 | Kepler-25 | 2106 ± 50 | 98.27 ± 0.57 | 6270 ± 79 | −0.04 ± 0.10 | Steffen et al. (2012) |
108 | 4914423 | Kepler-103 | 1663 ± 56 | 81.5 ± 1.6 | 5845 ± 88 | 0.07 ± 0.11 | Marcy et al. (2014) |
123 | 5094751 | Kepler-109 | 1745 ± 117 | 91.1 ± 2.3 | 5952 ± 75 | −0.08 ± 0.10 | Marcy et al. (2014) |
85 | 5866724 | Kepler-65 | 1880 ± 60 | 89.56 ± 0.48 | 6169 ± 50 | 0.09 ± 0.08 | Chaplin et al. (2013) |
285 | 6196457 | Kepler-92 | 1299 ± 53 | 66.6 ± 1.1 | 5871 ± 94 | 0.17 ± 0.11 | Xie (2014) |
3158 | 6278762 | Kepler-444 | 4538 ± 144 | 179.64 ± 0.76 | 5046 ± 74 | −0.37 ± 0.09 | Campante et al. (2015) |
41 | 6521045 | Kepler-100 | 1502 ± 31 | 77.0 ± 1.1 | 5825 ± 75 | 0.02 ± 0.10 | Marcy et al. (2014) |
75 | 7199397 | 644 ± 8b | 38.9 ± 0.8b | 5824 ± 50a | −0.22 ± 0.08a | ||
269 | 7670943 | 1895 ± 73 | 88.6 ± 1.3 | 6463 ± 110 | 0.09 ± 0.11 | ||
274 | 8077137 | Kepler-128 | 1324 ± 39 | 68.8 ± 0.64 | 6105 ± 100 | −0.11 ± 0.07 | Xie (2014) |
260 | 8292840 | Kepler-126 | 1983 ± 37 | 92.85 ± 0.35 | 6205 ± 100 | −0.26 ± 0.07 | Rowe et al. (2014) |
122 | 8349582 | Kepler-95 | 1677 ± 90 | 83.6 ± 1.4 | 5699 ± 74 | 0.3 ± 0.10 | Marcy et al. (2014) |
245 | 8478994 | Kepler-37 | 4660 ± 50 | 178.7 ± 1.4 | 5417 ± 75 | −0.32 ± 0.07 | Barclay et al. (2013) |
370 | 8494142 | Kepler-145 | 1133 ± 81 | 61.8 ± 0.76 | 6144 ± 106 | 0.13 ± 0.10 | Xie (2014) |
5 | 8554498 | 1153 ± 76 | 61.98 ± 0.96 | 5945 ± 60 | 0.17 ± 0.05 | ||
319 | 8684730 | 938 ± 72b | 52.2 ± 0.7b | 5924 ± 50a | 0.17 ± 0.08a | ||
42 | 8866102 | Kepler-410 | 2014 ± 32 | 94.5 ± 0.60 | 6325 ± 75 | 0.01 ± 0.10 | Van Eylen et al. (2014) |
974 | 9414417 | 1115 ± 32 | 60.05 ± 0.27 | 6253 ± 75 | −0.13 ± 0.10 | ||
288 | 9592705 | 1008 ± 21 | 53.54 ± 0.32 | 6174 ± 92 | 0.22 ± 0.10 | ||
1925 | 9955598 | Kepler-409 | 3546 ± 119 | 153.18 ± 0.14 | 5460 ± 75 | 0.08 ± 0.10 | Marcy et al. (2014) |
263 | 10514430 | False-positive | 1303 ± 30 | 70.0 ± 1.0 | 5784 ± 98 | −0.11 ± 0.11 | |
275 | 10586004 | Kepler-129 | 1395 ± 40 | 69.2 ± 1.4 | 5770 ± 83 | 0.29 ± 0.10 | Rowe et al. (2014) |
2 | 10666592 | HAT-P7 | 1115 ± 110 | 59.22 ± 0.59 | 6350 ± 80 | 0.26 ± 0.08 | Pál et al. (2008) |
1612 | 10963065 | Kepler-408 | 2193 ± 48 | 103.2 ± 0.63 | 6104 ± 74 | −0.2 ± 0.10 | Marcy et al. (2014) |
276 | 11133306 | 2381 ± 95 | 107.9 ± 1.9 | 5982 ± 82 | −0.02 ± 0.10 | ||
246 | 11295426 | Kepler-68 | 2154 ± 13 | 101.57 ± 0.10 | 5793 ± 74 | 0.12 ± 0.07 | Gilliland et al. (2013) |
277 | 11401755 | Kepler-36 | 1250 ± 44 | 67.9 ± 1.2 | 5960 ± 80 | −0.24 ± 0.06 | Carter et al. (2012) |
262 | 11807274 | Kepler-50 | 1496 ± 56 | 75.71 ± 0.31 | 6225 ± 75 | −0.0 ± 0.08 | Steffen et al. (2013) |
7 | 11853905 | Kepler-4 | 1436 ± 42 | 74.4 ± 1.1 | 5781 ± 76 | 0.09 ± 0.10 | Borucki et al. (2010) |
72 | 11904151 | Kepler-10 | 2730 ± 280 | 118.2 ± 0.20 | 5647 ± 74 | −0.15 ± 0.10 | Batalha et al. (2011) |
KOI . | KIC . | ID . | νmax . | Δν . | Teff . | [Fe/H] . | Notes . |
---|---|---|---|---|---|---|---|
. | . | . | (μHz) . | (μHz) . | (K) . | (dex) . | . |
268 | 3425851 | 2038 ± 60 | 92.6 ± 1.5 | 6343 ± 85 | −0.04 ± 0.10 | ||
69 | 3544595 | Kepler-93 | 3366 ± 81 | 145.77 ± 0.45 | 5669 ± 75 | −0.18 ± 0.10 | Ballard et al. (2014) |
975 | 3632418 | Kepler-21 | 1153 ± 32 | 60.86 ± 0.55 | 6305 ± 50 | −0.03 ± 0.10 | Howell et al. (2012) |
280 | 4141376 | 2928 ± 97 | 128.8 ± 1.3 | 6134 ± 91 | −0.24 ± 0.10 | ||
281 | 4143755 | 1458 ± 57 | 77.2 ± 1.3 | 5622 ± 106 | −0.4 ± 0.11 | ||
244 | 4349452 | Kepler-25 | 2106 ± 50 | 98.27 ± 0.57 | 6270 ± 79 | −0.04 ± 0.10 | Steffen et al. (2012) |
108 | 4914423 | Kepler-103 | 1663 ± 56 | 81.5 ± 1.6 | 5845 ± 88 | 0.07 ± 0.11 | Marcy et al. (2014) |
123 | 5094751 | Kepler-109 | 1745 ± 117 | 91.1 ± 2.3 | 5952 ± 75 | −0.08 ± 0.10 | Marcy et al. (2014) |
85 | 5866724 | Kepler-65 | 1880 ± 60 | 89.56 ± 0.48 | 6169 ± 50 | 0.09 ± 0.08 | Chaplin et al. (2013) |
285 | 6196457 | Kepler-92 | 1299 ± 53 | 66.6 ± 1.1 | 5871 ± 94 | 0.17 ± 0.11 | Xie (2014) |
3158 | 6278762 | Kepler-444 | 4538 ± 144 | 179.64 ± 0.76 | 5046 ± 74 | −0.37 ± 0.09 | Campante et al. (2015) |
41 | 6521045 | Kepler-100 | 1502 ± 31 | 77.0 ± 1.1 | 5825 ± 75 | 0.02 ± 0.10 | Marcy et al. (2014) |
75 | 7199397 | 644 ± 8b | 38.9 ± 0.8b | 5824 ± 50a | −0.22 ± 0.08a | ||
269 | 7670943 | 1895 ± 73 | 88.6 ± 1.3 | 6463 ± 110 | 0.09 ± 0.11 | ||
274 | 8077137 | Kepler-128 | 1324 ± 39 | 68.8 ± 0.64 | 6105 ± 100 | −0.11 ± 0.07 | Xie (2014) |
260 | 8292840 | Kepler-126 | 1983 ± 37 | 92.85 ± 0.35 | 6205 ± 100 | −0.26 ± 0.07 | Rowe et al. (2014) |
122 | 8349582 | Kepler-95 | 1677 ± 90 | 83.6 ± 1.4 | 5699 ± 74 | 0.3 ± 0.10 | Marcy et al. (2014) |
245 | 8478994 | Kepler-37 | 4660 ± 50 | 178.7 ± 1.4 | 5417 ± 75 | −0.32 ± 0.07 | Barclay et al. (2013) |
370 | 8494142 | Kepler-145 | 1133 ± 81 | 61.8 ± 0.76 | 6144 ± 106 | 0.13 ± 0.10 | Xie (2014) |
5 | 8554498 | 1153 ± 76 | 61.98 ± 0.96 | 5945 ± 60 | 0.17 ± 0.05 | ||
319 | 8684730 | 938 ± 72b | 52.2 ± 0.7b | 5924 ± 50a | 0.17 ± 0.08a | ||
42 | 8866102 | Kepler-410 | 2014 ± 32 | 94.5 ± 0.60 | 6325 ± 75 | 0.01 ± 0.10 | Van Eylen et al. (2014) |
974 | 9414417 | 1115 ± 32 | 60.05 ± 0.27 | 6253 ± 75 | −0.13 ± 0.10 | ||
288 | 9592705 | 1008 ± 21 | 53.54 ± 0.32 | 6174 ± 92 | 0.22 ± 0.10 | ||
1925 | 9955598 | Kepler-409 | 3546 ± 119 | 153.18 ± 0.14 | 5460 ± 75 | 0.08 ± 0.10 | Marcy et al. (2014) |
263 | 10514430 | False-positive | 1303 ± 30 | 70.0 ± 1.0 | 5784 ± 98 | −0.11 ± 0.11 | |
275 | 10586004 | Kepler-129 | 1395 ± 40 | 69.2 ± 1.4 | 5770 ± 83 | 0.29 ± 0.10 | Rowe et al. (2014) |
2 | 10666592 | HAT-P7 | 1115 ± 110 | 59.22 ± 0.59 | 6350 ± 80 | 0.26 ± 0.08 | Pál et al. (2008) |
1612 | 10963065 | Kepler-408 | 2193 ± 48 | 103.2 ± 0.63 | 6104 ± 74 | −0.2 ± 0.10 | Marcy et al. (2014) |
276 | 11133306 | 2381 ± 95 | 107.9 ± 1.9 | 5982 ± 82 | −0.02 ± 0.10 | ||
246 | 11295426 | Kepler-68 | 2154 ± 13 | 101.57 ± 0.10 | 5793 ± 74 | 0.12 ± 0.07 | Gilliland et al. (2013) |
277 | 11401755 | Kepler-36 | 1250 ± 44 | 67.9 ± 1.2 | 5960 ± 80 | −0.24 ± 0.06 | Carter et al. (2012) |
262 | 11807274 | Kepler-50 | 1496 ± 56 | 75.71 ± 0.31 | 6225 ± 75 | −0.0 ± 0.08 | Steffen et al. (2013) |
7 | 11853905 | Kepler-4 | 1436 ± 42 | 74.4 ± 1.1 | 5781 ± 76 | 0.09 ± 0.10 | Borucki et al. (2010) |
72 | 11904151 | Kepler-10 | 2730 ± 280 | 118.2 ± 0.20 | 5647 ± 74 | −0.15 ± 0.10 | Batalha et al. (2011) |
Notes.aBuchhave et al. (2012). bThis work.
This PDF is available to Subscribers Only
View Article Abstract & Purchase OptionsFor full access to this pdf, sign in to an existing account, or purchase an annual subscription.