File name : Imai_2013.LOR Reduction date : 2014年3月27日 Ephemeris : DE430, DE422 Limb basis : Kaguya {0.2deg resolution} O-C basis : limb correction applied Telescopes: Aperture Longitude Latitude Alt # cm o ' " o ' " m A 25 +138 50 26.4 +37 26 43.6 31 ref Tel Observer Star No. y m d h m s PhGrMrCeDb O-C 001 A E. Imai S 138052 2013 4 22 11 39 33.91 DD G 1 0.07 002 A E. Imai X 108189 2013 6 12 11 9 4.32 DD G 1 -0.05 003 A E. Imai X 108190 2013 6 12 11 10 6.85 DD G 1 -0.04 004 A E. Imai S 97663 2013 6 12 11 11 51.86 DD G 1 -0.09 005 A E. Imai R 1925 2013 8 12 9 49 8.29 DD G 1 -0.08 006 A E. Imai R 1925 2013 8 12 10 16 15.26 RD G 1 -0.03 007 A E. Imai X 40731 2013 8 15 10 29 31.68 DD G 1 0.19 008 A E. Imai S 184257 2013 8 15 10 42 29.71 DD G 1 0.12 009 A E. Imai S 159818 2013 8 15 10 50 35.54 DD G 1 0.29 010 A E. Imai R 2338 2013 8 15 11 31 12.34 DD G 1 0.09 011 A E. Imai R 2343 2013 8 15 12 52 19.56 DD G 1 0.07 012 A E. Imai S 159858 2013 8 15 13 6 42.99 DD G 1 0.08 013 A E. Imai S 159860 2013 8 15 13 7 44.96 DD G 1 0.23 014 A E. Imai S 159864 2013 8 15 13 22 54.27 DD G 1 -0.02 015 A E. Imai S 145539 2013 10 14 10 7 9.99 DD G 1 0.02 016 A E. Imai S 145548 2013 10 14 10 56 2.95 DD G 1 0.09 017 A E. Imai S 145564 2013 10 14 11 6 37.97 DD G 1 0.68 018 A E. Imai S 145572 2013 10 14 11 40 23.34 DD G 1 0.03 019 A E. Imai S 145567 2013 10 14 11 50 40.77 DD G 1 -0.04 020 A E. Imai R 3172 2013 10 14 12 18 58.19 DD G 1 0.06 Explanation of columns 'PhGrMrCeDb' Ph - Phase of the event. 1st character D = disappear, R = reappear, B = blink, F = flash, M = Miss 2nd character D = dark limb, B = bright limb, U = in umbra of lunar eclipse Gr - G if the event is during a graze Mr - Method of timing and recording. Main types are: G = video with time insertion, V = video with other time linking S = visual using a stopwatch, T = visual using a tape recorder, E = eye/ear Ce - Certainty. 1 = certain, 2 = may be spurious, 3 = most likely spurious Db - Double star indication - West, East, North, South, Brighter, Fainter ref 番号 Tel 望遠鏡, Observer 観測者 Star No. 星名 y 年 m 月 d 日 h 時 m 分 s 秒 Ph 現象(最初のDは潜入,Rは出現,次のDは暗縁,Bは明縁) Gr グレージング Mr 観測方法(Sは眼視によるストップウォッチ計測) Ce 現象の確実性(1:確実,2:やや疑わしい,3:疑わしい) Db 二重星の場合の星の位置