Table 3.

Observational data for C/1723 T1 made by the court astronomers of the Joseon dynasty.*

(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)
RecordObs.Obs.TJDH.A.RAL.A.L.A.ErrorDecP.A.P.A.Error
datesdatestimeshαEAobsAcaleAδEΔobsΔcal|$e_\Delta$|
(lunar)(Greg.)geng/hh:mm(d)(°)(°)(du)(du)(du)(°)(du)(du)(du)
09.25October 202/21:573.0440.78308.9177.65−14.46105105.99A
October 212/21:544.0442.54307.3876.11−11.68105103.17B
October 222/21:565.049.49306.2274.922.08−9.68105100.944.06C
09.26October 221/19:344.949.49306.3245.03−9.68101101.14|$\bigcirc{1}$|
October 231/19:335.9411.16305.3944.09−0.09−7.8910199.321.68|$\bigcirc{2}$|
09.27October 241/19:326.9412.64304.6533.33−0.33−6.429897.830.17
09.28October 251/19:317.9413.98304.0422.72−0.72−5.209696.59−0.59
09.30October 271/19:299.9416.36303.1311.79−0.79−3.289594.650.35
10.01October 281/19:2810.9417.44302.7811.44−0.44−2.529493.870.13
10.02October 291/19:2611.9318.22302.4911.14−0.14−1.859393.19−0.19
10.03October 301/19:2612.9319.45302.2410.890.11−1.2592.592.59−0.09
10.04October 311/19:2513.9320.40302.0310.680.32−0.739292.05−0.05
10.05November 011/19:2414.9321.32301.8510.490.51−0.2591.591.55−0.05
Statistics for full dataeA〉 = +0.05|$\langle {e_\Delta }\rangle =+0.5$|
|$\langle {S_{e_{\rm A}}}\rangle \simeq 0.8$||$\langle {S_{e_\Delta }}\rangle \simeq 1.4$|
Statistics for records except for the records of 09.25 and 09.26eA〉 ≃ −0.2|$\langle {e_\Delta }\rangle =-0.04$|
|$\langle {S_{e_{\rm A}}}\rangle \simeq 0.5$||$\langle {S_{e_\Delta }}\rangle \simeq 0.3$|
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)
RecordObs.Obs.TJDH.A.RAL.A.L.A.ErrorDecP.A.P.A.Error
datesdatestimeshαEAobsAcaleAδEΔobsΔcal|$e_\Delta$|
(lunar)(Greg.)geng/hh:mm(d)(°)(°)(du)(du)(du)(°)(du)(du)(du)
09.25October 202/21:573.0440.78308.9177.65−14.46105105.99A
October 212/21:544.0442.54307.3876.11−11.68105103.17B
October 222/21:565.049.49306.2274.922.08−9.68105100.944.06C
09.26October 221/19:344.949.49306.3245.03−9.68101101.14|$\bigcirc{1}$|
October 231/19:335.9411.16305.3944.09−0.09−7.8910199.321.68|$\bigcirc{2}$|
09.27October 241/19:326.9412.64304.6533.33−0.33−6.429897.830.17
09.28October 251/19:317.9413.98304.0422.72−0.72−5.209696.59−0.59
09.30October 271/19:299.9416.36303.1311.79−0.79−3.289594.650.35
10.01October 281/19:2810.9417.44302.7811.44−0.44−2.529493.870.13
10.02October 291/19:2611.9318.22302.4911.14−0.14−1.859393.19−0.19
10.03October 301/19:2612.9319.45302.2410.890.11−1.2592.592.59−0.09
10.04October 311/19:2513.9320.40302.0310.680.32−0.739292.05−0.05
10.05November 011/19:2414.9321.32301.8510.490.51−0.2591.591.55−0.05
Statistics for full dataeA〉 = +0.05|$\langle {e_\Delta }\rangle =+0.5$|
|$\langle {S_{e_{\rm A}}}\rangle \simeq 0.8$||$\langle {S_{e_\Delta }}\rangle \simeq 1.4$|
Statistics for records except for the records of 09.25 and 09.26eA〉 ≃ −0.2|$\langle {e_\Delta }\rangle =-0.04$|
|$\langle {S_{e_{\rm A}}}\rangle \simeq 0.5$||$\langle {S_{e_\Delta }}\rangle \simeq 0.3$|
*

The dates in the lunar calendar are given in the first column. For example, 09.21 means the 21st day of the 9th month (of the 3rd reign year of King Gyeongjong, or 1723). The second column represents the dates of observations in the Gregorian calendar. The third column represents the observing times, where the first numbers are the times in watches or geng, and the final numbers are the mid-watch times. The fourth column represents the dates and times, TJD, in Julian days of J1723.0 counted after JD =2350662. The fifth column is the hour angle of the comet at the observing time. The sixth, seventh, and eighth columns represent the right ascensions, the observed lodge angles, and the ephemeris lodge angles of the comet, respectively. The lodge angles are referenced to the lunar lodge of Niu or Quanniu (β Cap), whose right ascension was |$\alpha _0={301.36\circ }$| during this period. The ninth column represents the errors in the lodge angles |$e_{\rm A}=A_{\rm obs}-A_{\rm cal}$|⁠. The 10th, 11th, and 12th columns represent the ephemeris declinations, the observed polar angles, and the ephemeris polar angles of the comet, respectively. The 13th column represents the errors in the polar angles |$e_\Delta=\Delta_{\rm obs}-\Delta_{\rm cal}$|⁠. We do not show the observational data that do not have measurements.

Table 3.

Observational data for C/1723 T1 made by the court astronomers of the Joseon dynasty.*

(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)
RecordObs.Obs.TJDH.A.RAL.A.L.A.ErrorDecP.A.P.A.Error
datesdatestimeshαEAobsAcaleAδEΔobsΔcal|$e_\Delta$|
(lunar)(Greg.)geng/hh:mm(d)(°)(°)(du)(du)(du)(°)(du)(du)(du)
09.25October 202/21:573.0440.78308.9177.65−14.46105105.99A
October 212/21:544.0442.54307.3876.11−11.68105103.17B
October 222/21:565.049.49306.2274.922.08−9.68105100.944.06C
09.26October 221/19:344.949.49306.3245.03−9.68101101.14|$\bigcirc{1}$|
October 231/19:335.9411.16305.3944.09−0.09−7.8910199.321.68|$\bigcirc{2}$|
09.27October 241/19:326.9412.64304.6533.33−0.33−6.429897.830.17
09.28October 251/19:317.9413.98304.0422.72−0.72−5.209696.59−0.59
09.30October 271/19:299.9416.36303.1311.79−0.79−3.289594.650.35
10.01October 281/19:2810.9417.44302.7811.44−0.44−2.529493.870.13
10.02October 291/19:2611.9318.22302.4911.14−0.14−1.859393.19−0.19
10.03October 301/19:2612.9319.45302.2410.890.11−1.2592.592.59−0.09
10.04October 311/19:2513.9320.40302.0310.680.32−0.739292.05−0.05
10.05November 011/19:2414.9321.32301.8510.490.51−0.2591.591.55−0.05
Statistics for full dataeA〉 = +0.05|$\langle {e_\Delta }\rangle =+0.5$|
|$\langle {S_{e_{\rm A}}}\rangle \simeq 0.8$||$\langle {S_{e_\Delta }}\rangle \simeq 1.4$|
Statistics for records except for the records of 09.25 and 09.26eA〉 ≃ −0.2|$\langle {e_\Delta }\rangle =-0.04$|
|$\langle {S_{e_{\rm A}}}\rangle \simeq 0.5$||$\langle {S_{e_\Delta }}\rangle \simeq 0.3$|
(1)(2)(3)(4)(5)(6)(7)(8)(9)(10)(11)(12)(13)
RecordObs.Obs.TJDH.A.RAL.A.L.A.ErrorDecP.A.P.A.Error
datesdatestimeshαEAobsAcaleAδEΔobsΔcal|$e_\Delta$|
(lunar)(Greg.)geng/hh:mm(d)(°)(°)(du)(du)(du)(°)(du)(du)(du)
09.25October 202/21:573.0440.78308.9177.65−14.46105105.99A
October 212/21:544.0442.54307.3876.11−11.68105103.17B
October 222/21:565.049.49306.2274.922.08−9.68105100.944.06C
09.26October 221/19:344.949.49306.3245.03−9.68101101.14|$\bigcirc{1}$|
October 231/19:335.9411.16305.3944.09−0.09−7.8910199.321.68|$\bigcirc{2}$|
09.27October 241/19:326.9412.64304.6533.33−0.33−6.429897.830.17
09.28October 251/19:317.9413.98304.0422.72−0.72−5.209696.59−0.59
09.30October 271/19:299.9416.36303.1311.79−0.79−3.289594.650.35
10.01October 281/19:2810.9417.44302.7811.44−0.44−2.529493.870.13
10.02October 291/19:2611.9318.22302.4911.14−0.14−1.859393.19−0.19
10.03October 301/19:2612.9319.45302.2410.890.11−1.2592.592.59−0.09
10.04October 311/19:2513.9320.40302.0310.680.32−0.739292.05−0.05
10.05November 011/19:2414.9321.32301.8510.490.51−0.2591.591.55−0.05
Statistics for full dataeA〉 = +0.05|$\langle {e_\Delta }\rangle =+0.5$|
|$\langle {S_{e_{\rm A}}}\rangle \simeq 0.8$||$\langle {S_{e_\Delta }}\rangle \simeq 1.4$|
Statistics for records except for the records of 09.25 and 09.26eA〉 ≃ −0.2|$\langle {e_\Delta }\rangle =-0.04$|
|$\langle {S_{e_{\rm A}}}\rangle \simeq 0.5$||$\langle {S_{e_\Delta }}\rangle \simeq 0.3$|
*

The dates in the lunar calendar are given in the first column. For example, 09.21 means the 21st day of the 9th month (of the 3rd reign year of King Gyeongjong, or 1723). The second column represents the dates of observations in the Gregorian calendar. The third column represents the observing times, where the first numbers are the times in watches or geng, and the final numbers are the mid-watch times. The fourth column represents the dates and times, TJD, in Julian days of J1723.0 counted after JD =2350662. The fifth column is the hour angle of the comet at the observing time. The sixth, seventh, and eighth columns represent the right ascensions, the observed lodge angles, and the ephemeris lodge angles of the comet, respectively. The lodge angles are referenced to the lunar lodge of Niu or Quanniu (β Cap), whose right ascension was |$\alpha _0={301.36\circ }$| during this period. The ninth column represents the errors in the lodge angles |$e_{\rm A}=A_{\rm obs}-A_{\rm cal}$|⁠. The 10th, 11th, and 12th columns represent the ephemeris declinations, the observed polar angles, and the ephemeris polar angles of the comet, respectively. The 13th column represents the errors in the polar angles |$e_\Delta=\Delta_{\rm obs}-\Delta_{\rm cal}$|⁠. We do not show the observational data that do not have measurements.

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