Occultation of TYC 2913-02146-1 by 1637 Swings on 2023 Nov 23 Distance from center of occultation path - in km Distances are positive to the right, referenced to the direction of motion along the path Uncertainty in time = +/- 2 secs d Proba- Location Longitude Latitude alt U.T. Sepn Alt Sun km bility o ' o ' m h m s " o o 63 - 0% ** Path limit plus 3-Sigma ** 62 N 0% 380 Ishiki 137 5. 34 45. -37 20 54 20 -0.032 34 -8 51 - 2% ** Path limit plus 2-Sigma ** 40 - 16% ** Path limit plus 1-Sigma ** 39 N 18% 402 Dynic Astronomical Observat 136 15. 35 15. 190 20 54 23 -0.020 35 -9 28 - 50% *** Path limit *** 11 N 91% 352 Konan 136 15. 34 55. 179 20 54 22 -0.006 35 -9 5 N 96% 900 Moriyama 135 55. 35 5. 112 20 54 23 -0.003 35 -9 0 - 98% **** Centre Line **** -2 S 97% 351 Sakamoto 135 55. 35 5. 99 20 54 23 0.001 35 -9 -12 S 89% 377 Kwasan Observatory, Kyoto 135 45. 34 55. 208 20 54 23 0.006 35 -9 -27 S 53% 348 Ayabe 135 15. 35 15. 33 20 54 25 0.014 35 -10 -27 S 51% 378 Murou 136 5. 34 35. 354 20 54 20 0.014 34 -9 -28 - 50% *** Path limit *** -36 S 25% 903 Fukuchiyama and Kannabe 135 15. 35 15. 15 20 54 25 0.019 35 -10 -40 - 16% ** Path limit plus 1-Sigma ** -43 S 11% 365 Uto Observatory 135 55. 34 25. 459 20 54 19 0.022 34 -9 -48 S 5% 340 Toyonaka 135 25. 34 45. 69 20 54 22 0.025 35 -9 -51 - 2% ** Path limit plus 2-Sigma ** -63 - 0% ** Path limit plus 3-Sigma ** Prediction of 2023 Oct 3.0