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Table 2.
Results of the observations presented in this work for STARLINK-1130 (Darksat) and STARLINK-1113.
Passband | Detector | Obs. trail length | Time on detector | Obs. | Est. trail length | Est. | |
---|---|---|---|---|---|---|---|
(arcsec) | (s) | (mag) | (arcsec) | (mag) | |||
STARLINK-1130 | |||||||
Sloan r′ | 1 | 1938 ± 44 | 1.56 ± 0.08 | 9.29 ± 0.01 | 12386 ± 111 | 6.50 ± 0.02 | |
Sloan i′ | 1 | 202 ± 14 | 0.14 ± 0.01 | 8.50 ± 0.02 | 1491 ± 39 | 6.33 ± 0.03 | |
J-band | 4 | 742 ± 27 | 0.70 ± 0.05 | 9.73 ± 0.01 | 31919 ± 178 | 5.64 ± 0.02 | |
J-band | 8 | 241 ± 16 | 0.23 ± 0.01 | 10.99 ± 0.02 | 31919 ± 178 | 5.68 ± 0.02 | |
J-band | 11 | 741 ± 27 | 0.70 ± 0.05 | 9.72 ± 0.01 | 31919 ± 178 | 5.65 ± 0.01 | |
J-band | 15 | 299 ± 17 | 0.28 ± 0.03 | 10.70 ± 0.02 | 31919 ± 178 | 5.63 ± 0.02 | |
5.65 ± 0.01 | |||||||
Ks-band | 11 | 735 ± 27 | 0.56 ± 0.04 | 8.77 ± 0.01 | 13051 ± 114 | 5.65 ± 0.03 | |
Ks-band | 13 | 332 ± 18 | 0.25 ± 0.02 | 9.65 ± 0.02 | 13051 ± 114 | 5.66 ± 0.03 | |
Ks-band | 14 | 410 ± 20 | 0.31 ± 0.02 | 9.36 ± 0.01 | 13051 ± 114 | 5.60 ± 0.02 | |
5.63 ± 0.02 | |||||||
STARLINK-1113 | |||||||
Sloan r′ | 1 | 1035 ± 32 | 0.35 ± 0.02 | 7.37 ± 0.03 | 5993 ± 77 | 5.46 ± 0.05 | |
Sloan i′ | 1 | 634 ± 25 | 0.47 ± 0.03 | 6.32 ± 0.03 | 1438 ± 38 | 5.43 ± 0.04 | |
J-band | 3 | 692 ± 26 | 0.73 ± 0.05 | 9.31 ± 0.01 | 28865 ± 170 | 5.11 ± 0.01 | |
J-band | 7 | 698 ± 26 | 0.73 ± 0.05 | 9.26 ± 0.01 | 28865 ± 170 | 5.08 ± 0.01 | |
J-band | 11 | 698 ± 26 | 0.73 ± 0.05 | 9.27 ± 0.01 | 28865 ± 170 | 5.09 ± 0.01 | |
J-band | 15 | 698 ± 26 | 0.73 ± 0.05 | 9.31 ± 0.01 | 28865 ± 170 | 5.15 ± 0.02 | |
5.10 ± 0.01 | |||||||
Ks-band | 8 | 254 ± 16 | 0.12 ± 0.01 | 9.42 ± 0.02 | 21127 ± 145 | 4.62 ± 0.04 | |
Ks-band | 11 | 775 ± 28 | 0.37 ± 0.02 | 8.23 ± 0.01 | 21127 ± 145 | 4.63 ± 0.03 | |
Ks-band | 13 | 400 ± 20 | 0.19 ± 0.01 | 8.99 ± 0.02 | 21127 ± 145 | 4.68 ± 0.03 | |
Ks-band | 14 | 524 ± 23 | 0.25 ± 0.02 | 8.67 ± 0.01 | 21127 ± 145 | 4.66 ± 0.03 | |
4.65 ± 0.02 |
Notes. The results are the weighted means of the individual results from each comparison star per detector. The weighted mean of the estimated magnitude after combining the different detector results is given in bold.
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