Comet C/2015 O1 (PANSTARRS)

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
   2015O1  2017 08 14.83  S 14.4 AQ 35.5L 4 177   0.9  5/           ICQ XX CER01                                                  Jakub Cerny; Comet Alt.:51.97 AS:-1.0,2.0,-3.0,-2.0,2.0 Star mags:13.923,14.543,14.442,14.182,14.758 ,,,,
2015O1 2017 08 14.47 xS 14.1 AQ 25.0L 5 166 0.4 3 ICQ XX WYA Christopher Wyatt
2015O1 2017 08 13.83 S 14.7 AQ 35.5L 4 177 0.7 5/ ICQ XX CER01 Jakub Cerny; Comet Alt.:52.7 AS:-3.0,-1.0,-2.0,2.0 Star mags:14.401,14.475,14.605,14.913 UCAC4,UCAC4,UCAC4,UCAC4
2015O1 2017 08 13.46 S 13.8 AQ 40.6L 4 260 0.7 4 ICQ XX CAM03 Paul Camilleri
2015O1 2017 08 11.45 S 13.7 AQ 40.6L 4 165 0.5 3 ICQ XX CAM03 Paul Camilleri
2015O1 2017 08 10.47 S 13.9 AQ 40.6L 4 165 0.6 3 ICQ XX CAM03 Paul Camilleri
2015O1 2017 08 10.38 xS 14.3 AQ 25.0L 5 83 0.8 3 ICQ XX WYA Christopher Wyatt
2015O1 2017 08 09.97 Z 15.2 U4 35.0T 6a720 0.38 ICQ XX BUCaa a720C26 sST9 K41 CMP 0 U 2.0s 2.0 Denis Buczynski, Tarbatness MPC Code I81; vem Mag derived from Comphot Nick James BAA
2015O1 2017 07 27.53 S 13.7 AQ 40.6L 4 165 0.8 4 ICQ XX CAM03 Paul Camilleri
2015O1 2017 07 26.96 Z 15.2 U4 35.0T 6a360 ICQ XX BUCaa C22.6 sST9 K26 CMP 5 U 2.0s 2.0 Denis Buczynski, I81 tarbatness; Magnitude derived using Nick James BAA comphot for VEM
2015O1 2017 07 24.50 S 14.2 AQ 40.6L 4 266 0.5 5 ICQ XX CAM03 Paul Camilleri
2015O1 2017 07 22.97 C 13.1 MC 50.0L 3a120 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
2015O1 2017 07 20.53 S 13.8 AQ 40.6L 4 165 0.4 5 ICQ XX CAM03 Paul Camilleri
2015O1 2017 07 14.96 I 14.5 AQ 20.3T10 133 0.2 7 ICQ XX GON05 Juan Jose Gonzalez Suarez
2015O1 2017 07 14.05 C 14.0 MC 50.0L 3a120 0.7 1.5m131 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
2015O1 2017 07 03.93 S[13.5 HS 44.0L 5 250 ICQXXX HAS02 Werner Hasubick
2015O1 2017 06 30.62 xM 14.7 AQ 25.0L 5 166 0.2 5/ ICQ XX WYA Christopher Wyatt
2015O1 2017 06 29.07 C 14.1 MC 50.0L 3a120 0.6 1.6m132 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
2015O1 2017 05 28.18 C 14.1 MC 50.0L 3a120 0.5 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
2015O1 2017 05 06.03 C 14.5 MC 50.0L 3a120 0.4 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
2015O1 2017 04 22.15 C 15.0 MC 50.0L 3a120 0.4 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
2015O1 2017 04 02.23 C 15.1 MC 50.0L 3a120 0.3 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
2015O1 2017 03 30.12 B 16.5 U4 20.0L 4a450 0.17S1 ICQ XX NAGaa S dCDS CFC 5 U9 d Akos Nagy Melykuti, Szalánta
2015O1 2017 03 28.09 B 15.5 U4 20.0L 4a450 0.33S6 ICQ XX NAGaa S dCDS CFC 5 U9 d Akos Nagy Melykuti, Szalánta
2015O1 2016 10 31.79 B 16.1 U4 8.0R 7a450 9 ICQ XX NAGaa S dCDS CFC 5 U9 d Akos Nagy Melykuti, Szalánta
2015O1 2016 10 20.07 C 15.8 TK 25.0L 3a300 0.3 ICQ XX RAMaa C sSTM K32 A32 5 U5 0.3 1.6s 1.6 Raymond Ramlow
2015O1 2016 09 29.90 C 14.4 MC 50.0L 3a120 0.3 ICQ XX HILaaI C 0.19mFL9 K32 AFo 5 P5 0.1 1.0s 1.0 Kevin Hills; Multibox data generated using Astrometrica and FoCas, then Kphot used to estimate visual equivalent magnitude as reported above
2015O1 2016 08 31.85 S 16.2 U4 60.3L 4 518 0.1 5 ICQ XX SZA Sandor Szabo, Csapod; SQM: 21.3 mag/arcsec^2, Motion was checked
2015O1 2016 08 02.21 C 15.9 TK 40.6C12a200 0.2 ICQ XX RAMaa S dSTA K6N MIm U5 0.2 1.0s 1.0 Raymond Ramlow, Boulder, Colorado, USA
2015O1 2016 07 14.05 C 15.3 MC 50.0L 3a150 0.2 ICQ XX HILaaI C 0.19mFL9 K32 AFo 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
2015O1 2016 06 07.17 C 16.4 MC 50.0L 3a150 0.4 ICQ XX HILaaI C 0.19mFL9 K32 AFo 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
2015O1 2015 10 31.83 C 18.1 MC 50.0L 3a150 0.2 ICQ XX HILaaI C 0.19mFL9 K32 AFo P5 0.1 1.0s 1.0 Kevin Hills; Multibox data generated using Astrometrica and FoCas, then Kphot used to estimate visual equivalent magnitude as reported above
2015O1 2015 10 14.88 C 18.3 MC 50.0L 3a150 0.2 ICQ XX HILaaI C 0.19mFL9 K32 AFo 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
2015O1 2015 10 04.59 C[17.7 UO 51.0Y 4a 47 ICQ XX PRYabI C 0.22mFL9 KA9 A48 U1 2.2s 2.2 Taras Prystavski
2015O1 2015 09 29.92 C 18.0 MC 50.0L 3a150 0.2 ICQ XX HILaaI C 0.19mFL9 K32 AFo P5 0.1 1.0s 1.0 Kevin Hills; Multibox data generated using Astrometrica and FoCas, then Kphot used to estimate visual equivalent magnitude as reported above
2015O1 2015 09 15.94 C 18.2 MC 50.0L 3a150 0.2 ICQ XX HILaaI C 0.19mFL9 K32 AFo P5 0.1 1.0s 1.0 Kevin Hills; Multibox data generated using Astrometrica and FoCas, then Kphot used to estimate visual equivalent magnitude as reported above
2015O1 2015 09 03.93 C 16.4 MC 50.0L 3a150 0.2 ICQ XX HILaaI C 0.19mFL9 K32 AFo P5 0.1 1.0s 1.0 Kevin Hills; Multibox data generated using Astrometrica and FoCas, then Kphot used to estimate visual equivalent magnitude as reported above.