Table 1.
Optical photometry of the local sequences for LSQ13abf in the “natural” system.
| ID | α(2000) | δ(2000) | r | i | B | V |
|---|---|---|---|---|---|---|
| 2 | 177.23423 | 19.13506 | … | … | 14.077(0.012) | … |
| 3 | 177.24424 | 19.11977 | 14.272(0.017) | 14.113(0.027) | 14.957(0.016) | 14.438(0.014) |
| 4 | 177.27493 | 19.22754 | 15.441(0.016) | 15.296(0.017) | 16.080(0.029) | 15.601(0.016) |
| 5 | 177.31714 | 19.16629 | 16.183(0.026) | 16.060(0.025) | 16.851(0.035) | 16.346(0.027) |
| 6 | 177.29127 | 19.10672 | 17.884(0.054) | 17.603(0.083) | 19.110(0.056) | 18.279(0.095) |
| 7 | 177.25087 | 19.20356 | 18.177(0.059) | 17.996(0.098) | 19.107(0.157) | 18.458(0.070) |
| 9 | 177.28277 | 19.19292 | 18.761(0.100) | 18.704(0.103) | 19.313(0.143) | 18.861(0.130) |
| 13 | 177.31741 | 19.11532 | 19.027(0.087) | 18.759(0.156) | 19.640(0.158) | 19.184(0.127) |
| 14 | 177.34702 | 19.11574 | 19.029(0.141) | 18.557(0.168) | … | 19.618(0.158) |
Notes. Values in parenthesis are 1-σ uncertainties and correspond to an rms of the instrumental errors of the photometry obtained over a minimum of three nights. This Swope (+ e2V) natural system photometry can be transformed to the standard system using the color terms presented by Phillips et al. (2019, see their Table 5).
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