Comet C/2018 L2 (ATLAS)

IIIYYYYMnL YYYY MM DD.DD eM/mm.m:r AAA.ATF/xxxx /dd.ddnDC /t.ttmANG ICQ XX*OBSxxf InT APERTURcamchip SFW C ## u.uu xx.x PIXELSIZE
   2018L2  2018 12 06.77  S  9.2 TK 20.3T10  77   4.5  3            ICQ XX GON05                                                  Juan Jose Gonzalez Suarez
2018L2 2018 12 05.70 S 11.8 U4 60.0L 172 1.2 5 ICQ XX SZA Sandor Szabo, Agfalva
2018L2 2018 12 04.72 Z 10.5 AQ 10.0R 6a781 5.3 FRIaaI Steffen Fritsche
2018L2 2018 12 01.38 S 11.7 TA 40.0L 4 144 1.3 3 ICQ XX YOS04 Seiichi Yoshida
2018L2 2018 11 30.37 S 11.3 TJ 40.0L 4 144 1.3 4 ICQ XX YOS04 Seiichi Yoshida
2018L2 2018 11 29.70 M 10.4 AQ 32.6L 5 67 2.5 4 ICQ XX GUZ Piotr Guzik
2018L2 2018 11 28.71 Z 10.3 AQ 10.0R 6a540 6.5 FRIaaI Steffen Fritsche
2018L2 2018 11 28.70 Z 10.5 AQ 10.0R 6a330 5.3 FRIaaI Steffen Fritsche
2018L2 2018 11 17.69 S 10.8 AQ 30.5L 5 94 2 2 ICQ XX KAR02 Timo Karhula, Virsbo, Sweden; SQM-L: 19.5 mag/arcsec^2, Strong local light pollution, 69% gibbous moon.
2018L2 2018 11 16.71 Z 10.7 AQ 10.0R 6A042 4.8 FRIaaI Steffen Fritsche
2018L2 2018 11 11.73 S 9.2 TK 10.0R 5 54 2.9 3 ICQXXX HAS02 Werner Hasubick
2018L2 2018 11 06.72 S 9.2 TK 7.0B 6 16 6 PIL01 Uwe Pilz
2018L2 2018 11 06.72 S 9.8 TT 10.0B 20 4 2 ICQ XX LEH Martin Lehký
2018L2 2018 11 03.78 S 9.1 TK 20.3T10 77 6 2/ ICQ XX GON05 Juan Jose Gonzalez Suarez
2018L2 2018 11 03.74 S 10.4 TI 53.1L 129 2.2 2 ICQ XX HAR11 Christian Harder, Jeersdorf, Germany; SQM-L: 19.5 mag/arcsec^2, Swanfilter wirkte
2018L2 2018 10 31.73 M 11.1 AQ 32.6L 5 67 2 4 ICQ XX GUZ Piotr Guzik
2018L2 2018 10 30.74 B 10.5 TK 44.0L 5 100 1 4 ICQXXX HAS02 Werner Hasubick
2018L2 2018 10 27.74 S 10.4 TI 30.3L 5 137 2.5 2 ICQ XX HAR11 Christian Harder, Jeersdorf, Germany; SQM-L: 19.1 mag/arcsec^2, Swanfilter wirkte. Der Komet stand nur 14° hoch.
2018L2 2018 10 12.43 S 10.8 AQ 40.6L 4 76 4 1 ICQ XX CAM03 Paul Camilleri
2018L2 2018 10 11.43 S 10.8 AQ 40.6L 4 76 4 3 ICQ XX CAM03 Paul Camilleri
2018L2 2018 10 05.74 S 12.4 U4 60.0L 4 187 0.8 4 ICQ XX SZA Sandor Szabo, Agfalva
2018L2 2018 10 03.82 S 9.8 TK 20.3T10 100 5 2/ ICQ XX GON05 Juan Jose Gonzalez Suarez
2018L2 2018 09 06.44 M 14.2 AQ 40.6L 4 165 1 3 ICQ XX CAM03 Paul Camilleri
2018L2 2018 09 03.44 M 13.9 AQ 40.6L 4 165 1.2 4 ICQ XX CAM03 Paul Camilleri
2018L2 2018 09 01.44 M 13.8 AQ 40.6L 4 165 1 4 ICQ XX CAM03 Paul Camilleri
2018L2 2018 08 31.44 M 13.8 AQ 40.6L 4 165 1 4 ICQ XX CAM03 Paul Camilleri
2018L2 2018 08 13.48 S 14.0 AQ 40.6L 4 165 1 3 ICQ XX CAM03 Paul Camilleri
2018L2 2018 08 11.44 S 13.9 AQ 40.6L 4 165 1.2 3 ICA XX CAM03 Paul Camilleri
2018L2 2018 08 10.45 S 14.2 AQ 40.6L 4 266 1 3 ICQ XX CAM03 Paul Camilleri
2018L2 2018 08 09.44 S 14.3 AQ 40.6L 4 266 1 3 ICQ XX CAM03 Paul Camilleri
2018L2 2018 07 13.90 C 14.2 MC 50.0L 3a150 0.7 ICQ XX HILaaI C 0.19mFL9 K32 AFo 5 P5 0.0 1.0s 1.0 Kevin Hills
2018L2 2018 07 06.91 C 13.5 MC 50.0L 3a150 0.9 ICQ XX HILaaI C 0.19mFL9 K32 AFo 5 P5 0.0 1.0s 1.0 Kevin Hills; Multibox data generated using Astrometrica and FoCas, then Kphot used to estimate visual equivalent magnitude as reported above