EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 692 (December 2024) A&A, 692 (2024) A263 Full HTML
Open Access

Table B.1

Revised stellar parameters for all the targets of the BEAST survey. The multiplicity flag mf indicates whether the star is known to be a multiple system (1: Gratton et al. 2023, 2: this work, 3: Chini et al. 2012) or not (0).

HIP ID OTHER ID RAa hms DECa dms G mag K mag Dist. pc Age Myr SpT MS pT M⊙ Miso M⊙ mf
HIP50847 * 191 Car 10 22 58.1465 -66 54 05.385 4.93 5.31 128.9 ± 1.6 27 ± 4 B8V 3.4−0.6+0.5$\[3.4_{-0.6}^{+0.5}\]$ 4.9 ± 0.5 1
HIP52742 HD 93563 10 46 57.4734 -56 45 25.89 5.12 5.22 178.5 ± 3.6 150 ± 50 B5V 4.7−0.4+0.4$\[4.7_{-0.4}^{+0.4}\]$ 4.1−0.4+0.6$\[4.1_{-0.4}^{+0.6}\]$ 1
HIP54767 HD 97583 11 12 45.2069 -64 10 11.171 5.2 5.42 97.7 ± 0.6 100−40+50$\[100_{-40}^{+50}\]$ B8V 3.4−0.6+0.5$\[3.4_{-0.6}^{+0.5}\]$ 3.3 ± 0.3 1
HIP58452 HD 104080 11 59 10.6803 -45 49 55.998 6.34 6.53 134.0 ± 0.9 20 ± 5 B8.5V 3.1−0.4+0.6$\[3.1_{-0.4}^{+0.6}\]$ 3.0 ± 0.3 0
HIP58901 HD 104900 12 04 45.2597 -59 15 11.703 6.29 6.28 117.0 ± 1.4 13 ± 3 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.9 ± 0.3 1
HIP59173 V* V863 Cen 12 08 05.2222 -50 39 40.575 4.4 4.87 108.9 ± 2.3 15 ± 3 B5V 4.7−0.4+0.4$\[4.7_{-0.4}^{+0.4}\]$ 5.4 ± 0.5 1
HIP59747 * del Cru 12 15 08.7184 -58 44 56.126 2.77 3.53 139.5 ± 13.9 16 ± 3 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 11.0 ± 1.0 1
HIP60009 * zet Cru 12 18 26.242 -64 00 11.107 4.04 4.53 108.2 ± 2.3 12+4 B2.5V 6.0−0.6+1.3$\[6.0_{-0.6}^{+1.3}\]$ 6.5 ± 0.6 1
HIP60379 HD 107696 12 22 49.4317 -57 40 34.068 5.36 5.64 104.1 ± 0.8 13 ± 3 B7V 3.9−0.5+0.4$\[3.9_{-0.5}^{+0.4}\]$ 3.8 ± 0.4 0
HIP60710 * G Cen 12 26 31.76 -51 27 02.288 4.8 5.23 136.1 ± 3.4 18−3+2$\[18_{-3}^{+2}\]$ B3V 5.4−0.3+0.6$\[5.4_{-0.3}^{+0.6}\]$ 5.6 ± 0.6 1
HIP60823 * sig Cen 12 28 02.3821 -50 13 50.296 3.89 4.48 126.2 ± 3.7 17 ± 3 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 7.2 ± 0.7 1
HIP60855 * u Cen 12 28 22.4671 -39 02 28.19 5.43 5.54 150.4 ± 3.7 16 ± 3 B8.5V 3.1−0.4+0.6$\[3.1_{-0.4}^{+0.6}\]$ 5.0 ± 0.5 1
HIP61257 HD 109195 12 33 12.1871 -52 04 58.236 6.55 6.61 125.8 ± 0.6 17 ± 3 B9.5V 2.7−0.6+0.4$\[2.7_{-0.6}^{+0.4}\]$ 2.7 ± 0.3 1
HIP61585 * alf Mus 12 37 11.0178 -69 08 08.033 2.7 3.25 116.0 ± 11.2 15 ± 3 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 9.8−1.0+1.1$\[9.8_{-1.0}^{+1.1}\]$ 1
HIP62058 HD 110506 12 43 09.1786 -56 10 34.418 5.98 6.17 123.5 ± 0.6 15 ± 3 B7.5V 3.6−0.6+0.5$\[3.6_{-0.6}^{+0.5}\]$ 3.4 ± 0.3 0
HIP62327 HD 110956 12 46 22.7144 -56 29 19.735 4.61 5.06 117.9 ± 3.1b 17 ± 3 B2.5V 6.0−0.6+1.3$\[6.0_{-0.6}^{+1.3}\]$ 5.4 ± 0.5 1
HIP62434 * bet Cru 12 47 43.2687 -59 41 19.579 — 1.99 85.4 ± 7.1b 16 ± 3 B1V 11.0−1.0+4.0$\[11.0_{-1.0}^{+4.0}\]$ 11.0 ± 1.0 1
HIP62786 HD 111774 12 51 56.931 -39 40 49.55 5.97 6.22 140.3 ± 1.1 17 ± 3 B7.5V 3.6−0.6+0.5$\[3.6_{-0.6}^{+0.5}\]$ 3.7 ± 0.4 0
HIP63003 * mu. 01 Cru 12 54 35.6242 -57 10 40.528 4.0 4.58 124.8 ± 3.3 16 ± 3 B2V-V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 7.1 ± 0.7 1
HIP63005 * mu. 02 Cru 12 54 36.8841 -57 10 07.193 5.15 5.31 121.0 ± 1.7 16 ± 3 B5V 4.7−0.4+0.4$\[4.7_{-0.4}^{+0.4}\]$ 4.7 ± 0.5 1
HIP63210 * H Cen 12 57 04.3514 -51 11 55.512 5.14 5.34 128.8 ± 1.7 19 ± 3 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 4.8 ± 0.5 1
HIP63945 * f Cen 13 06 16.7036 -48 27 47.846 4.67 5.05 122.6 ± 2.3 15 ± 3 B4V 5.1−0.4+0.3$\[5.1_{-0.4}^{+0.3}\]$ 5.5 ± 0.5 1
HIP64004 * ksi02 Cen 13 06 54.6394 -49 54 22.487 4.22 4.84 147.1 ± 3.9 20 ± 4 B3V 5.4−0.3+0.6$\[5.4_{-0.3}^{+0.6}\]$ 7.0 ± 0.7 1
HIP65021 HD 115583 13 19 43.4213 -67 21 51.567 7.25 7.22 171.4 ± 0.7 16 ± 3 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.9 ± 0.3 0
HIP65112 V* V964 Cen 13 20 37.8253 -52 44 52.169 5.43 5.8 119.2 ± 1.4 15 ± 3 B5V 4.7−0.4+0.4$\[4.7_{-0.4}^{+0.4}\]$ 4.0 ± 0.4 0
HIP66454 HD 118354 13 37 23.476 -46 25 40.432 5.89 6.14 143.0 ± 2.7 17 ± 3 B8V 3.4−0.6+0.5$\[3.4_{-0.6}^{+0.5}\]$ 4.0 ± 0.4 1
HIP67464 * nu. Cen 13 49 30.2765 -41 41 15.75 3.38 4.24 124.3 ± 5.4 18−5+3$\[18_{-5}^{+3}\]$ B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 8.2 ± 0.8 1
HIP67669 * 3 Cen A 13 51 49.6013 -32 59 38.706 4.51 4.97 105.4 ± 9.9b 17 ± 3 B5V+B9V 4.7−0.4+0.4$\[4.7_{-0.4}^{+0.4}\]$ 4.8 ± 0.5 1
HIP67703 * N Cen 13 52 04.8623 -52 48 41.506 5.25 5.51 93.1 ± 0.8 16 ± 3 B8V 3.4−0.6+0.5$\[3.4_{-0.6}^{+0.5}\]$ 3.4 ± 0.3 1
HIP68245 * phi Cen 13 58 16.2661 -42 06 02.724 3.81 4.49 140.8 ± 5.4 17 ± 3 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 7.9 ± 0.8 0
HIP68282 * ups01 Cen 13 58 40.7486 -44 48 12.908 3.85 4.47 131.1 ± 2.7b 21−2+4$\[21_{-2}^{+4}\]$ B2V-V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 6.6 ± 0.7 1
HIP68862 * chi Cen 14 06 02.768 -41 10 46.678 4.31 4.93 154.1 ± 5.1 25 ± 5 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 6.8 ± 0.7 0
HIP69011 HD 123247 14 07 40.808 -48 42 14.498 6.42 6.43 97.6 ± 0.5 17 ± 3 B9.5V 2.7−0.6+0.4$\[2.7_{-0.6}^{+0.4}\]$ 2.3 ± 0.2 0
HIP69618 V* V795 Cen 14 14 57.1383 -57 05 10.049 5.01 4.77 131.5 ± 2.3 2 ± 1 B4V 5.1−0.4+0.3$\[5.1_{-0.4}^{+0.3}\]$ 6.3−3.0+0.6$\[6.3_{-3.0}^{+0.6}\]$ 0
HIP70300 * a Cen 14 23 02.2387 -39 30 42.544 4.36 4.92 120.1 ± 2.6 17−5+3$\[17_{-5}^{+3}\]$ B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 5.9 ± 0.6 2
HIP70626 HD 126475 14 26 49.8732 -39 52 26.344 6.34 6.59 141.0 ± 1.1 15 ± 3 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 3.3 ± 0.3 0
HIP71352 * eta Cen 14 35 30.4241 -42 09 28.17 2.25 2.96 93.7 ± 1.8b 15 ± 3 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 9.7 ± 1.0 3
HIP71353 HD 127971 14 35 31.479 -41 31 02.792 5.86 6.03 108.3 ± 2.6 15 ± 3 B7V 3.9−0.5+0.4$\[3.9_{-0.5}^{+0.4}\]$ 3.2 ± 0.3 1
HIP71453 HD 128207 14 36 44.1322 -40 12 41.696 5.72 6.01 136.4 ± 1.5 16 ± 3 B8V 3.4−0.6+0.5$\[3.4_{-0.6}^{+0.5}\]$ 4.0 ± 0.4 0
HIP71536 * rho Lup 14 37 53.2261 -49 25 32.981 4.0 4.51 107.0 ± 2.3 14 ± 4 B3/4V 5.2−0.3+0.8$\[5.2_{-0.3}^{+0.8}\]$ 6.2 ± 0.6 1
HIP71860 * alf Lup 14 41 55.7557 -47 23 17.515 2.32 2.67 142.5 ± 3.4b 19 ± 3 B1.5V 10.0−3.0+1.0$\[10.0_{-3.0}^{+1.0}\]$ 11.0 ± 1.0 1
HIP71865 * b Cen 14 41 57.5905 -37 47 36.58 3.99 4.49 99.7 ± 3.1 15 ± 2 B2.5V 6.0−0.6+1.3$\[6.0_{-0.6}^{+1.3}\]$ 5.9 ± 0.6 1
HIP73266 HD 132094 14 58 24.2646 -37 21 44.902 7.26 7.28 170.9 ± 1.2 15 ± 3 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.7 ± 0.3 1
HIP73624 HD 132955 15 02 59.2764 -32 38 35.849 5.42 5.73 146.7 ± 2.8 17 ± 3 B3V 5.4−0.3+0.6$\[5.4_{-0.3}^{+0.6}\]$ 5.0 ± 0.5 1
HIP74100 HD 133937 15 08 39.198 -42 52 04.522 5.81 6.1 144.2 ± 1.6 19 ± 3 B5/7V 4.3−0.4+0.4$\[4.3_{-0.4}^{+0.4}\]$ 4.1 ± 0.4 1
HIP74449 * e Lup 15 12 49.5875 -44 30 01.49 4.79 5.28 138.2 ± 3.9 18 ± 3 B3V 5.4−0.3+0.6$\[5.4_{-0.3}^{+0.6}\]$ 5.7 ± 0.6 1
HIP74657 HD 135174 15 15 19.6424 -44 08 58.18 6.73 6.95 154.9 ± 1.2 18 ± 3 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 3.0 ± 0.3 0
HIP74752 HD 135454 15 16 37.1496 -42 22 12.565 6.75 6.83 130.9 ± 0.7 14 ± 3 B9.5V 2.7−0.6+0.4$\[2.7_{-0.6}^{+0.4}\]$ 2.6 ± 0.3 1
HIP74950 V* GG Lup 15 18 56.3746 -40 47 17.596 5.57 6.21 150.1 ± 2.0 18 ± 3 B7V 3.9−0.5+0.4$\[3.9_{-0.5}^{+0.4}\]$ 4.4 ± 0.4 1
HIP75141 * del Lup 15 21 22.3138 -40 38 51.109 3.21 3.96 148.6 ± 10.6 16 ± 4 B1.5V 10.0−3.0+1.0$\[10.0_{-3.0}^{+1.0}\]$ 9.8−1.0+1.1$\[9.8_{-1.0}^{+1.1}\]$ 1
HIP75304 * phi02 Lup 15 23 09.3506 -36 51 30.557 4.51 4.94 159.2 ± 5.1b 15 ± 3 B4V 5.1−0.4+0.3$\[5.1_{-0.4}^{+0.3}\]$ 7.1 ± 0.7 1
HIP75647 HD 137432 15 27 18.1304 -36 46 03.214 5.43 5.84 142.3 ± 2.4 17 ± 3 B5V 4.7−0.4+0.4$\[4.7_{-0.4}^{+0.4}\]$ 4.6 ± 0.5 1
HIP76048 HD 138221 15 31 50.2295 -32 52 52.015 6.45 6.25 163.7 ± 1.0 2 ± 1 B7V 3.9−0.5+0.4$\[3.9_{-0.5}^{+0.4}\]$ 3.3−0.3+1.6$\[3.3_{-0.3}^{+1.6}\]$ 0
HIP76126 * zet Lib 15 32 55.2212 -16 51 10.241 5.48 5.89 230.8 ± 8.4 11 ± 3 B3V 5.4−0.3+0.6$\[5.4_{-0.3}^{+0.6}\]$ 7.2 ± 0.7 1
HIP76591 HD 139233 15 38 32.6385 -39 09 38.52 6.58 6.76 145.7 ± 1.0 17 ± 3 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 3.0 ± 0.3 0
HIP76600 * tau Lib 15 38 39.3694 -29 46 39.895 3.65 4.12 112.5 ± 2.5b 13−3+4$\[13_{-3}^{+4}\]$ B2.5V 6.0−0.6+1.3$\[6.0_{-0.6}^{+1.3}\]$ 7.5 ± 0.7 1
HIP76633 HD 139486 15 39 00.0577 -19 43 57.199 7.63 7.49 164.7 ± 1.0 7−2+3$\[7_{-2}^{+3}\]$ B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.4 ± 0.2 0
HIP77562 HD 141168 15 50 07.0836 -53 12 35.174 5.77 5.95 96.5 ± 0.5 17 ± 3 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.9 ± 0.3 0
HIP77968 HD 142256 15 55 22.8856 -44 31 33.651 6.96 6.99 181.9 ± 1.0 17−2+5$\[17_{-2}^{+5}\]$ B8V 3.4−0.6+0.5$\[3.4_{-0.6}^{+0.5}\]$ 3.4 ± 0.3 0
HIP78104 * rho Sco 15 56 53.0772 -29 12 50.667 3.87 4.46 136.6 ± 5.5 14−3+2$\[14_{-3}^{+2}\]$ B2V-V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 7.9 ± 0.8 1
HIP78168 HD 142883 15 57 40.4636 -20 58 59.082 5.81 5.73 157.4 ± 1.3 10 ± 3 B3V 5.4−0.3+0.6$\[5.4_{-0.3}^{+0.6}\]$ 5.3 ± 0.5 1
HIP78207 * 48 Lib 15 58 11.3682 -14 16 45.681 4.74 4.59 139.8 ± 2.4 0.5−0.3+0.5$\[0.5_{-0.3}^{+0.5}\]$ B5Vp 4.7−0.4+0.4$\[4.7_{-0.4}^{+0.4}\]$ 4.7 ± 0.5 0
HIP78324 HD 143022 15 59 30.8817 -40 51 54.598 8.12 7.49 167.2 ± 1.0 7 ± 2 B9.5V 2.7−0.6+0.4$\[2.7_{-0.6}^{+0.4}\]$ 2.1 ± 0.2 0
HIP78384 * eta Lup 16 00 07.3279 -38 23 48.138 3.41 4.1 135.5 ± 3.3b 14 ± 3 B2.5V 6.0−0.6+1.3$\[6.0_{-0.6}^{+1.3}\]$ 9.1 ± 0.9 1
HIP78655 HD 143699 16 03 24.1895 -38 36 09.141 4.87 5.27 122.5 ± 4.5b 14 ± 3 B5/7V 4.3−0.4+0.4$\[4.3_{-0.4}^{+0.4}\]$ 5.1 ± 0.5 0
HIP78702 HD 143956 16 04 00.2383 -19 46 02.926 7.76 7.24 148.4 ± 0.8 10−5+2$\[10_{-5}^{+2}\]$ B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.4 ± 0.2 1
HIP78918 * tet Lup 16 06 35.5439 -36 48 08.173 4.16 4.7 135.7 ± 4.7 17 ± 3 B2.5V 6.0−0.6+1.3$\[6.0_{-0.6}^{+1.3}\]$ 6.9 ± 0.7 1
HIP78933 * ome Sco 16 06 48.4249 -20 40 09.079 3.92 4.01 140.9 ± 5.4 11 ± 3 B1V 11.0−1.0+4.0$\[11.0_{-1.0}^{+4.0}\]$ 9.8 ± 1.0 0
HIP78968 HD 144586 16 07 14.9283 -17 56 09.731 7.76 7.4 149.1 ± 0.6 9−2+3$\[9_{-2}^{+3}\]$ B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.4 ± 0.2 0
HIP79044 HD 144591 16 08 04.3798 -36 13 54.598 6.74 6.91 138.5 ± 0.9 17 ± 3 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.7 ± 0.3 1
HIP79404 * 13 Sco 16 12 18.2046 -27 55 34.953 4.53 4.98 147.4 ± 3.1 11 ± 3 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 7.4 ± 0.7 1
HIP80142 HD 147001 16 21 27.0327 -48 11 19.041 6.5 6.62 176.3 ± 1.2 17 ± 3 B7V 3.9−0.5+0.4$\[3.9_{-0.5}^{+0.4}\]$ 3.9 ± 0.4 1
HIP80208 HD 147152 16 22 27.9955 -49 34 20.468 5.07 5.4 141.8 ± 6.4b 17 ± 3 B3V 5.4−0.3+0.6$\[5.4_{-0.3}^{+0.6}\]$ 5.4 ± 0.5 0
HIP80569 * chi Oph 16 27 01.4355 -18 27 22.499 4.2 3.02 152.9 ± 4.6 7−4+3$\[7_{-4}^{+3}\]$ B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 11.0 ± 1.0 1
HIP80911 * N Sco 16 31 22.9344 -34 42 15.725 4.18 4.69 182.4 ± 6.8 16 ± 4 B2V-V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 8.8 ± 0.9 0
HIP81208 HD 149274 16 35 13.8392 -35 43 28.725 6.63 6.77 146.1 ± 1.0 17−4+3$\[17_{-4}^{+3}\]$ B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 2.6 ± 0.3 1
HIP81266 * tau Sco 16 35 52.9528 -28 12 57.661 2.8 3.57 195.2 ± 42.3 12−4+2$\[12_{-4}^{+2}\]$ B0.2V 17.7−2.7+0.8$\[17.7_{-2.7}^{+0.8}\]$ 12.0−1.0+2.0$\[12.0_{-1.0}^{+2.0}\]$ 1
HIP81316 HD 149425 16 36 28.673 -40 18 10.916 7.07 6.71 184.4 ± 1.0 18 ± 4 B9V 2.8−0.6+0.6$\[2.8_{-0.6}^{+0.6}\]$ 3.9 ± 0.4 1
HIP81472 V* V1003 Sco 16 38 26.2919 -43 23 54.328 5.81 5.93 190.9 ± 1.9 17 ± 3 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 5.7 ± 0.6 1
HIP81474 HD 149914 16 38 28.6527 -18 13 13.713 6.64 5.69 154.4 ± 0.6 2.0−0.2+0.5$\[2.0_{-0.2}^{+0.5}\]$ B9.5V 2.7−0.6+0.4$\[2.7_{-0.6}^{+0.4}\]$ 3.1−0.3+1.6$\[3.1_{-0.3}^{+1.6}\]$ 1
HIP81891 HD 150638 16 43 38.7239 -32 06 21.406 6.45 6.63 153.0 ± 1.0 14 ± 3 B8V 3.4−0.6+0.5$\[3.4_{-0.6}^{+0.5}\]$ 3.4 ± 0.3 0
HIP81914 HD 150591 16 43 54.082 -41 06 48.038 6.12 6.29 174.6 ± 1.6 17 ± 3 B6/7V 4.1−0.5+0.4$\[4.1_{-0.5}^{+0.4}\]$ 4.7 ± 0.5 1
HIP81972 HD 150742 16 44 42.5926 -40 50 22.83 5.61 5.84 173.8 ± 1.9 18 ± 3 B3V 5.4−0.3+0.6$\[5.4_{-0.3}^{+0.6}\]$ 5.6 ± 0.6 1
HIP82514 * mu. 01 Sco 16 51 52.2283 -38 02 50.638 3.07 3.7 169.5 ± 8.6c 20 ± 4 B1V+BV 11.0−1.0+4.0$\[11.0_{-1.0}^{+4.0}\]$ 10.0 ± 1.0 1
HIP82545 * mu. 02 Sco 16 52 20.1453 -38 01 03.125 3.54 4.29 169.5 ± 8.6c 20 ± 4 B2V 7.0−1.0+3.0$\[7.0_{-1.0}^{+3.0}\]$ 9.1 ± 0.3 0

Notes. a: coordinates are given in J2000 IRCS. b: using Hipparcos parallax. c: see Squicciarini et al. (2022).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.