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Table 2

Taxonomic classification using the standard error method.

Ast. num. Tax. type Dist. Reliab. Obs. night
1914 Hartbeespoortdam V-type 0.020 29.2% 2019-04-22
R-type 0.046
2704 Julian Loewe V-type 0.020 24.3% 2018-04-03
R-type 0.058
2798 Vergilius R-type 0.050 29.2% 2018-04-22
V-type 0.057
2823 Van der Laan V-type 0.076 97.5% 2019-06-09
Sv-type 0.161
3302 Schliemann Sv-type 0.074 29.2% 2019-06-09
Sr-type 0.079
3331 Kvitasberg V-type 0.035 29.2% 2019-04-22
R-type 0.060
4434 Nikulin V-type 0.075 95.1% 2018-04-03
R-type 0.120
5037 Habing V-type 0.057 29.2% 16-09-2016
R-type 0.075
5235 Jean-Loup V-type 0.036 100% 16-09-2016
Sv-type 0.157
5525 (1991 TS4) R-type 0.041 26.8% 16-09-2016
V-type 0.056
5560 Amytis V-type 0.076 100% 2018-09-16
R-type 0.185
5754 (1992 FR2) V-type 0.04 100% 2018-04-22
Sv-type 0.135
6819 McGarvey V-type 0.030 26.8% 2018-09-16
R-type 0.084
7558 Yurlov R-type 0.048 24.3% 2018-04-03
V-type 0.067
8645 (1988 TN) V-type 0.068 92.6% 2018-09-16
Sv-type 0.189
9652 (1996 AF2) R-type 0.046 29.2% 2020-01-08
Sr-type 0.047
17057 (1999 GS4) R-type 0.099 29.2% 2018-09-16
V-type 0.109

Notes. Columns are asteroid number, taxonomic type distance from the template, and reliability of the classification. For each spectrum we list the two best matches. When possible we supplemented the spectra with the NIR counterpart from the literature.

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