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Table 2

Physical and spectral properties of the Pallas family asteroids.

Asteroid H (mag) S′ (µm−1) σS D (km) σD pV σPv Taxonomy Gaia S′ (µm−1) Gaia σS
2 4.12 −0.114 0.004 513 3 0.126 0.025 B −0.074 0.016
3579 13.86 −0.116 0.004 7.296 0.114 0.120 0.005 B +0.536 0.145
4969 12.92 −0.170 0.005 6.712 1.472 0.171 0.057 B +0.021 0.089
5222 11.60 −0.095 0.003 20.252 4.787 0.085 0.099 B −0.099 0.016
5234 12.28 −0.051 0.006 14.125 0.183 0.154 0.023 B −0.122 0.057
5690 13.21 −0.102 0.004 5.791 1.075 0.208 0.069 B −0.334 0.048
25853 13.57 −0.114 0.004 7.443 0.189 0.167 0.023 B −0.124 0.110
33750 12.91 −0.025 0.003 11.737 0.178 0.128 0.076 B +0.117 0.039
46037 14.01 −0.043 0.003 6.918 0.142 0.134 0.016 B −0.044 0.086
57050 13.83 −0.092 0.008 6.891 0.248 0.102 0.006 B −0.085 0.071
58296 14.26 −0.046 0.006 7.295 0.141 0.076 0.005 B +0.335 0.082
66714 14.31 −0.132 0.006 6.139 0.032 0.076 0.017 B
66803 13.00 −0.007 0.013 7.533 0.143 0.212 0.051 B +0.129 0.051
66846 14.08 −0.008 0.003 B/Xn +0.089 0.066
68299 13.93 −0.035 0.004 7.127 0.139 0.105 0.017 B +0.154 0.103
69371 13.77 −0.118 0.006 7.363 0.193 0.108 0.020 B −0.231 0.046
87306 13.44 −0.061 0.007 B −0.153 0.059
90368 13.82 −0.014 0.003 7.605 0.22 0.133 0.017 B/Xn +0.018 0.128
101283 14.23 −0.050 0.007 6.137 0.122 0.129 0.026 B
109640 14.00 +0.059 0.004 7.157 0.087 0.150 0.016 Ch −0.120 0.145
136038 15.01 −0.189 0.007 5.776 1.141 0.053 0.02 B −0.104 0.055
153652 13.77 −0.049 0.004 7.987 2.357 0.075 0.043 B −0.079 0.043

Notes. H is the absolute magnitude, S′ is the spectral slope, D is the diameter, pV is the visible albedo whereas σS, σD and σpv are the uncertainties in spectral slope, diameter, and visible albedo, respectively. The data is obtained from the AKARI IRC asteroid flux catalog by Alí-Lagoa et al. (2018), and from the recent 2019 NEOWISE diameters and albedos archive, taken by the WISE Camera instrument of Wide-Field Infrared Survey Explorer (Wright et al. 2010).

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