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Table A.1
LGGS sources within d < 4″ of the silicate emission candidates identified as members of IC 10.
| ID | d (″) | LGGS | V | V − R | R − I |
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| #3 | 2.33 | J002001.84+591933.9 | 23.463 | 0.684 | ... |
| 2.89 | J002001.22+591934.6 | 22.928 | 0.647 | 1.032 | |
| 3.40 | J002001.82+591930.5 | 22.891 | 0.691 | 0.653 | |
| 3.83 | J002001.96+591935.4 | 23.475 | 1.025 | 0.904 | |
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| #4 | 0.18 | J002002.61+591748.2 | 21.629 | 2.008 | 2.192 |
| 2.22 | J002002.55+591750.3 | 23.484 | 1.020 | 1.241 | |
| 3.29 | J002002.94+591746.2 | 21.804 | 0.492 | 0.480 | |
| 3.79 | J002003.05+591749.5 | 22.522 | 0.440 | ... | |
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| #6 | 0.31 | J002003.23+591801.6 | 21.274 | 1.848 | 2.035 |
| 2.27 | J002003.48+591800.2 | 23.084 | 0.537 | ... | |
| 2.59 | J002003.31+591803.8 | 23.142 | 0.938 | 1.183 | |
| 3.77 | J002002.94+591804.4 | 21.656 | 0.745 | 0.848 | |
| 3.91 | J002003.25+591805.2 | 23.494 | 0.703 | ... | |
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| #7 | 0.25 | J002004.54+591852.3 | 22.559 | 2.207 | 2.428 |
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| #8 | 0.21 | J002005.11+591804.1 | 21.096 | 1.666 | 1.717 |
| 0.98 | J002005.19+591804.6 | 21.529 | 0.238 | 1.206 | |
| 2.52 | J002005.00+591806.3 | 22.979 | 0.720 | 0.601 | |
| 3.60 | J002005.45+591801.5 | 19.672 | 0.875 | 0.997 | |
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| #12 | 0.30 | J002012.73+591712.3 | 22.020 | 1.722 | 1.978 |
| 2.23 | J002012.75+591709.9 | 22.271 | 1.535 | 1.453 | |
| 2.51 | J002013.00+591713.1 | 23.496 | 0.845 | 1.139 | |
| 3.02 | J002012.59+591715.0 | 22.626 | 0.689 | 1.024 | |
| 3.64 | J002012.90+591715.4 | 23.185 | 0.928 | 1.220 | |
| 3.82 | J002013.19+591711.4 | 21.644 | 0.909 | 0.976 | |
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| #13 | 0.25 | J002022.28+591743.3 | 21.682 | 1.870 | 2.095 |
| 1.54 | J002022.45+591743.0 | 22.817 | 0.632 | ... | |
| 2.49 | J002022.46+591741.3 | 21.704 | 0.358 | 0.290 | |
| 2.93 | J002021.97+591741.2 | 20.790 | 0.492 | 0.141 | |
| 3.30 | J002022.23+591746.5 | 22.346 | 2.662 | 1.090 | |
| 3.33 | J002022.13+591746.4 | 20.599 | 1.013 | 0.972 | |
| 3.39 | J002022.68+591742.4 | 21.850 | 0.478 | 0.779 | |
| 3.59 | J002021.87+591741.1 | 19.094 | 0.452 | 0.447 | |
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| #14 | 0.18 | J002022.01+591724.5 | 20.096 | 1.581 | 1.626 |
| 0.84 | J002022.05+591725.1 | 22.266 | 3.631 | 1.774 | |
| 1.63 | J002022.10+591725.8 | 21.842 | 1.368 | 0.601 | |
| 1.76 | J002022.11+591725.9 | 22.051 | 1.566 | 0.616 | |
| 1.89 | J002021.78+591725.4 | 22.936 | 0.132 | ... | |
| 2.25 | J002022.22+591723.0 | 23.046 | 1.235 | 1.264 | |
| 2.35 | J002022.05+591722.1 | 21.650 | 0.932 | 1.078 | |
| 2.45 | J002021.85+591722.2 | 22.018 | 0.846 | 1.099 | |
| 2.82 | J002021.82+591726.9 | 23.105 | 1.172 | 1.418 | |
| 3.75 | J002021.68+591721.5 | 20.448 | 0.514 | 0.444 | |
| 3.94 | J002022.44+591726.3 | 22.516 | 0.469 | 0.702 | |
| 3.96 | J002021.60+591721.8 | 20.446 | 0.512 | 0.444 | |
Notes. The LGGS ID in bold indicates the best match in terms of distance and infrared brightness.
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