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Table B.1

Spectral characteristics of primitive asteroid families.

Family NSDSS NECAS Albedo (%) SVIS (gi) (μm−1) NUV abs. (μm−1) SNIR1 (YJ) (μm−1) SNIR2 (JKs) (μm−1) Qhyd (%)
IMB
Polana–Eulalia 368 8 6.5 ± 2.8 0.160.08+0.12$\[-0.16_{-0.08}^{+0.12}\]$ 0.10.4+0.3$\[-0.1_{-0.4}^{+0.3}\]$ 0.060.22+0.31$\[0.06_{-0.22}^{+0.31}\]$ (37) 0.140.05+0.06$\[0.14_{-0.05}^{+0.06}\]$ (44) 7(1)
Erigone (h) 127 0 5.4 ± 1.2 0.010.12+0.08$\[0.01_{-0.12}^{+0.08}\]$ 0.80.5+0.5$\[0.8_{-0.5}^{+0.5}\]$ 0.140.09+0.32$\[0.14_{-0.09}^{+0.32}\]$ (14) 0.060.07+0.05$\[0.06_{-0.07}^{+0.05}\]$ (14) 58(2)
Clarissa 6 1 5.6 ± 1.5 0.280.04+0.20$\[-0.28_{-0.04}^{+0.20}\]$ 0.30.7+0.2$\[0.3_{-0.7}^{+0.2}\]$ 9(3)
Sulamitis (h) 16 0 5.4 ± 1.4 0.170.14+0.06$\[0.17_{-0.14}^{+0.06}\]$ 0.70.6+0.5$\[0.7_{-0.6}^{+0.5}\]$ 60(3)
Klio (h) 40 0 6.7 ± 1.8 0.100.15+0.09$\[0.10_{-0.15}^{+0.09}\]$ 0.70.3+0.6$\[0.7_{-0.3}^{+0.6}\]$ 23(4)
Chaldaea 21 1 6.6 ± 1.7 0.020.12+0.09$\[0.02_{-0.12}^{+0.09}\]$ 1.10.5+0.4$\[1.1_{-0.5}^{+0.4}\]$ 0.300.07+0.30$\[0.30_{-0.07}^{+0.30}\]$ (5) 0.130.06+0.15$\[0.13_{-0.06}^{+0.15}\]$ (6) 79(4)

MMB
Nemesis 57 3 8.4 ± 2.7 0.050.07+0.10$\[0.05_{-0.07}^{+0.10}\]$ 0.80.6+0.5$\[0.8_{-0.6}^{+0.5}\]$ 0.150.13+0.12$\[0.15_{-0.13}^{+0.12}\]$ (5) 0.060.06+0.09$\[0.06_{-0.06}^{+0.09}\]$ 0(5)
Adeona (h) 251 1 6.3 ± 1.7 0.110.09+0.10$\[-0.11_{-0.09}^{+0.10}\]$ 1.10.5+0.5$\[1.1_{-0.5}^{+0.5}\]$ 0.200.14+0.15$\[0.20_{-0.14}^{+0.15}\]$ (23) 0.040.06+0.12$\[0.04_{-0.06}^{+0.12}\]$ (27) 69(6)
Padua 76 1 7.2 ± 1.4 0.250.08+0.10$\[0.25_{-0.08}^{+0.10}\]$ 1.00.4+0.4$\[1.0_{-0.4}^{+0.4}\]$ 0.060.20+0.19$\[0.06_{-0.20}^{+0.19}\]$ (12) 0.070.06+0.16$\[0.07_{-0.06}^{+0.16}\]$ (18) 0(5,6)
Chloris (h) 43 1 8.1 ± 3.6 0.120.08+0.09$\[0.12_{-0.08}^{+0.09}\]$ 1.20.9+0.7$\[1.2_{-0.9}^{+0.7}\]$ 0.140.05+0.07$\[0.14_{-0.05}^{+0.07}\]$ (4) 0.040.13+0.09$\[0.04_{-0.13}^{+0.09}\]$ (8)
Misa (h) 37 0 6.1 ± 1.7 0.010.17+0.07$\[0.01_{-0.17}^{+0.07}\]$ 1.30.5+0.4$\[1.3_{-0.5}^{+0.4}\]$
Dora (h) 179 0 5.6 ± 1.7 0.120.10+0.11$\[-0.12_{-0.10}^{+0.11}\]$ 0.90.5+0.4$\[0.9_{-0.5}^{+0.4}\]$ 0.170.53+0.19$\[0.17_{-0.53}^{+0.19}\]$ (26) 0.040.05+0.04$\[0.04_{-0.05}^{+0.04}\]$ (19) 83(6)
Astrid (h) 12 0 5.6 ± 1.9 0.060.05+0.05$\[0.06_{-0.05}^{+0.05}\]$ 0.80.3+0.8$\[0.8_{-0.3}^{+0.8}\]$ 20(6)
Konig (h) 13 0 5.0 ± 1.6 0.020.05+0.09$\[-0.02_{-0.05}^{+0.09}\]$ 1.00.3+0.1$\[1.0_{-0.3}^{+0.1}\]$ 0.420.20+0.37$\[0.42_{-0.20}^{+0.37}\]$ (4)
Hoffmeister 82 0 5.0 ± 1.4 0.050.09+0.07$\[-0.05_{-0.09}^{+0.07}\]$ 0.00.5+0.5$\[0.0_{-0.5}^{+0.5}\]$ 0.200.29+0.12$\[0.20_{-0.29}^{+0.12}\]$ (14) 0.280.08+0.15$\[0.28_{-0.08}^{+0.15}\]$ (13) 0(5,6)
Vibilia (h) 15 0 6.4 ± 1.0 0.050.05+0.16$\[-0.05_{-0.05}^{+0.16}\]$ 0.90.2+0.3$\[0.9_{-0.2}^{+0.3}\]$ 0.160.08+0.08$\[0.16_{-0.08}^{+0.08}\]$ (5)
Phaeo 20 1 5.8 ± 1.5 0.360.07+0.17$\[0.36_{-0.07}^{+0.17}\]$ 0.30.5+0.5$\[0.3_{-0.5}^{+0.5}\]$
Mitidika 103 2 7.2 ± 2.0 0.040.08+0.06$\[-0.04_{-0.08}^{+0.06}\]$ 0.00.4+0.4$\[0.0_{-0.4}^{+0.4}\]$ 0.170.13+0.30$\[0.17_{-0.13}^{+0.30}\]$ (12) 0.110.06+0.11$\[0.11_{-0.06}^{+0.11}\]$ (11)
Karma 9 0 5.8 ± 1.0 0.250.02+0.05$\[0.25_{-0.02}^{+0.05}\]$ 0.40.4+0.5$\[0.4_{-0.4}^{+0.5}\]$
Postrema 9 0 5.2 ± 2.3 0.220.15+0.01$\[0.22_{-0.15}^{+0.01}\]$ 0.00.3+0.2$\[0.0_{-0.3}^{+0.2}\]$
Pallas 20 1 13.0 ± 3.3 0.210.15+0.08$\[-0.21_{-0.15}^{+0.08}\]$ 0.70.2+0.3$\[0.7_{-0.2}^{+0.3}\]$ 0(7)
Brucato (h) 44 0 6.5 ± 1.4 0.080.09+0.10$\[-0.08_{-0.09}^{+0.10}\]$ 1.00.6+0.3$\[1.0_{-0.6}^{+0.3}\]$ 0.120.05+0.05$\[0.12_{-0.05}^{+0.05}\]$ (5)

OMB
Hygiea 381 3 7.8 ± 2.6 0.120.08+0.10$\[-0.12_{-0.08}^{+0.10}\]$ 0.60.5+0.5$\[0.6_{-0.5}^{+0.5}\]$ 0.030.26+0.17$\[0.03_{-0.26}^{+0.17}\]$ (43) 0.150.08+0.09$\[0.15_{-0.08}^{+0.09}\]$ (48) 0–15(6,8)
Themis 536 19 7.7 ± 2.4 0.100.09+0.09$\[-0.10_{-0.09}^{+0.09}\]$ 0.90.4+0.4$\[0.9_{-0.4}^{+0.4}\]$ 0.090.10+0.14$\[0.09_{-0.10}^{+0.14}\]$ (89) 0.150.08+0.10$\[0.15_{-0.08}^{+0.10}\]$ (102) 11–13(6,8)
Sylvia 13 2 6.3 ± 1.7 0.150.10+0.09$\[0.15_{-0.10}^{+0.09}\]$ 0.10.8+0.3$\[0.1_{-0.8}^{+0.3}\]$
Meliboea (h) 53 3 6.3 ± 1.7 0.010.09+0.14$\[0.01_{-0.09}^{+0.14}\]$ 0.80.6+0.3$\[0.8_{-0.6}^{+0.3}\]$ 0.120.10+0.14$\[0.12_{-0.10}^{+0.14}\]$ (9) 0.050.09+0.19$\[-0.05_{-0.09}^{+0.19}\]$ (9) 78(6)
Emma (h) 46 0 4.8 ± 1.6 0.080.09+0.11$\[0.08_{-0.09}^{+0.11}\]$ 0.10.5+0.4$\[-0.1_{-0.5}^{+0.4}\]$ 0.470.16+0.43$\[0.47_{-0.16}^{+0.43}\]$ (6) 0.290.13+0.10$\[0.29_{-0.13}^{+0.10}\]$ (7)
Veritas (h) 85 0 6.8 ± 1.9 0.030.08+0.07$\[0.03_{-0.08}^{+0.07}\]$ 1.60.5+0.5$\[1.6_{-0.5}^{+0.5}\]$ 0.120.10+0.14$\[0.12_{-0.10}^{+0.14}\]$ (7) 0.040.04+0.10$\[0.04_{-0.04}^{+0.10}\]$ (11) 75–77(6,8)
Naema (h) 22 0 6.8 ± 1.9 0.060.09+0.12$\[-0.06_{-0.09}^{+0.12}\]$ 0.90.3+0.3$\[0.9_{-0.3}^{+0.3}\]$ 0.150.20+0.26$\[0.15_{-0.20}^{+0.26}\]$ (4)
Lixiaohua 68 0 4.4 ± 1.0 0.120.09+0.08$\[0.12_{-0.09}^{+0.08}\]$ 0.00.5+0.3$\[0.0_{-0.5}^{+0.3}\]$ 0.130.13+0.52$\[0.13_{-0.13}^{+0.52}\]$ (11) 0.1070.03+0.15$\[0.107_{-0.03}^{+0.15}\]$ (10) 0(8)
Theobalda 39 1 7.4 ± 2.3 0.250.07+0.05$\[-0.25_{-0.07}^{+0.05}\]$ 0.10.4+0.3$\[0.1_{-0.4}^{+0.3}\]$ 0.390.25+0.31$\[-0.39_{-0.25}^{+0.31}\]$ (4) 0.190.10+0.14$\[0.19_{-0.10}^{+0.14}\]$ (4)
Beagle 17 1 7.2 ± 1.6 0.160.11+0.06$\[-0.16_{-0.11}^{+0.06}\]$ 0.90.1+0.2$\[0.9_{-0.1}^{+0.2}\]$
Fringilla 17 0 5.1 ± 1.5 0.310.07+0.07$\[0.31_{-0.07}^{+0.07}\]$ 0.50.3+0.4$\[-0.5_{-0.3}^{+0.4}\]$
Ursula 136 1 6.5 ± 2.2 0.150.11+0.13$\[0.15_{-0.11}^{+0.13}\]$ 0.10.5+0.4$\[0.1_{-0.5}^{+0.4}\]$ 0.210.08+0.22$\[0.21_{-0.08}^{+0.22}\]$ (13) 0.180.09+0.06$\[0.18_{-0.09}^{+0.06}\]$ (20) 0(8)
Inarradas (h) 10 0 7.2 ± 1.5 0.060.09+0.08$\[-0.06_{-0.09}^{+0.08}\]$ 1.40.3+0.1$\[1.4_{-0.3}^{+0.1}\]$
Euphrosyne 150 0 5.8 ± 1.9 0.050.12+0.09$\[0.05_{-0.12}^{+0.09}\]$ 0.00.4+0.5$\[0.0_{-0.4}^{+0.5}\]$ 0.050.36+0.14$\[0.05_{-0.36}^{+0.14}\]$ (10) 0.250.09+0.18$\[0.25_{-0.09}^{+0.18}\]$ (12)
Alauda 176 2 7.2 ± 2.7 0.030.11+0.12$\[-0.03_{-0.11}^{+0.12}\]$ 0.50.5+0.6$\[0.5_{-0.5}^{+0.6}\]$ 0.250.24+0.11$\[0.25_{-0.24}^{+0.11}\]$ (18) 0.180.09+0.21$\[0.18_{-0.09}^{+0.21}\]$ (36)
Luthera 14 0 5.1 ± 1.0 0.500.11+0.12$\[0.50_{-0.11}^{+0.12}\]$ 0.90.3+0.3$\[-0.9_{-0.3}^{+0.3}\]$ 0.270.01+0.07$\[0.27_{-0.01}^{+0.07}\]$ (4)

Notes. Numbers in the brackets of SNIR are numbers of samples from the MOVIS-C catalog by Popescu et al. (2016), Qhyd is the fraction of family members with the 0.7 μm band from previous studies (see the references under the table). The notation of “(h)” indicates presence of the 0.7-μm absorption based on the positive HYD value.

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