Comet 260P/McNaught


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
260        2019 06 09.34  C 16.9 AQ 30.0C 6B760   0.4       0.8m241 ICQ XX MAS01I     C 0.42mG4x KA3 KPR 5 U9* 0.0       0.9s 0.9 Martin Masek; Comet Alt.:49.8 Calculated mags:16.9,16.9,16.9,16.9,17.0,16.9
260 2013 03 02.83 C 14.1 TK 54.0L 2a 20 0.6 4 ICQ XX KUT Walter Kutschera
260 2013 02 07.84 C 16.9 UD 40.0Y 8a300 0.48 0.8m229 ICQ XX PRYabI C 0.53mSTL KA1 A48 0 P3 1.8s 1.8 Taras Prystavski
260 2013 01 15.90 C 15.6 MC 40.0Y 8a300 0.73 2.7m221 ICQ XX PRYabI C 0.82mSTL KA1 A48 5 P3 0.1 1.8s 1.8 Taras Prystavski
260 2012 12 06.81 S 14.0: - 25.2L 6 160 2 ICQ XX HAR11 Christian Harder
260 2012 12 04.08 S[11.3 AC 15.0T10 37 ICQ XX AGUaa Salvador Aguirre, campestre Real del Molinito, Hermosillo,. Sonora
260 2012 11 24.77 S 12.7 TA 40.0L 4 144 1.6 4 ICQ XX YOS04 Seiichi Yoshida
260 2012 11 18.42 S 13.0 AC 30.0L 6 240 0.6 3 ICQ TA WOL01 Graham W. Wolf
260 2012 11 14.81 S 13.4: - 25.2L 6 125 0.6 3 ICQ XX HAR11 Christian Harder; unsichere Messung
260 2012 11 14.42 S 12.0 AC 30.0L 6 240 1.5 3 ICQ TA WOL01 Graham W. Wolf
260 2012 11 13.85 M 13.3 HS 35.0L 5 239 0.9 4/ ICQ XX CER01 Jakub Cerny
260 2012 11 13.77 S 12.9 HS 32.0L 5 120 1 4 ICQ XX PIL01 Uwe Pilz; 21.0 Filter wirkt mäßig
260 2012 11 12.79 B 12.0 TK 40.5L 5 140 1 3 ICQ XX KARaa Johan Kärnfelt, Gothenburg, Sweden
260 2012 11 12.58 aC 14.3 HV 35.0C14a240 0.5 5 ICQ XX TSU02 1a 3S 0.99mSTL KA1 SI5 8.2 1.1s 1.1 Mitsunori Tsumura
260 2012 11 11.83 S 11.8 TI 40.6L 4 150 1.2 3 0.03 140 ICQ XX HAR11 Christian Harder
260 2012 11 10.84 S 11.4 TI 23.5T10 94 2 3 ICQ XX LAB02 Carlos Labordena
260 2012 11 10.42 S 11.6 AC 30.0L 6 240 1.8 3 ICQ TA WOL01 Graham W. Wolf
260 2012 11 09.42 S 11.4 AC 30.0L 6 240 2.6 3 ICQ TA WOL01 Graham W. Wolf
260 2012 11 08.42 S 11.0 AC 30.0L 6 240 3.2 3 ICQ TA WOL01 Graham W. Wolf
260 2012 11 06.91 S 10.7 TK 20.3T10 100 3 3 ICQ XX GON05 Juan Jose Gonzalez Suarez
260 2012 11 06.03 S 14.1 AC 44.5L 4 167 0.6 3 ICQ XX MOR03 Warren Morrison, Cavan, Ontario
260 2012 11 05.42 S 10.5 AC 30.0L 6 240 4.5 3 ICQ TA WOL01 Graham W. Wolf
260 2012 11 04.84 S 10.5 TK 20.3T10 100 4 3 ICQ XX GON05 Juan Jose Gonzalez Suarez
260 2012 10 23.70 xC 12.1 TJ 7.1A 3a100 1.1 4 2.0m223 ICQ XX HAR10I S 1.1 mCKD CAC SI5 9.3 5.0s 5.0 Ken Harikae
260 2012 10 21.84 S[11.0 AC 15.0T10 37 ICQ XX AGUaa Salvador Aguirre, Campestre Real del Molinito, Hermosillo, Sonora, Mexico
260 2012 10 21.09 S[11.0 AC 15.0T10 37 ICQ XX AGUaa Salvador Aguirre
260 2012 10 20.92 S 12.3 HN 20.3L 6 71 1 4 ICQ XX PAR03 Mieczyslaw Leszek Paradowski, Dabrowa; Comparison stars taken from APASS (AQ)
260 2012 10 20.81 S 12.4 TI 40.6L 4 150 0.5 4 ICQ XX HAR11 Christian Harder; M bei 192x kurzer Schweifansatz
260 2012 10 20.71 xC 12.3 TJ 7.1A 3a130 0.7 5 3.2m228 ICQ XX HAR10I S 0.7 mCKD CAC SI5 10.0 5.0s 5.0 Ken Harikae
260 2012 10 19.90 S 12.8 HS 54.0L 5 180 1.1 3 ICQ XX KUT Walter Kutschera; 5.8 komet wirkt etwas schwächer koma erscheind nicht mehr elongiert
260 2012 10 19.90 M 13.0 HS 30.0L 6 128 0.6 5 ICQ XX MAS01 Martin Masek
260 2012 10 19.81 S 12.5 - 40.6L 4 150 0.6 4 ICQ XX HAR11 Christian Harder
260 2012 10 19.72 xC 12.2 TJ 7.1A 3a100 1.1 4 ICQ XX HAR10I S 1.1 mCKD CAC SI5 9.4 5.0s 5.0 Ken Harikae
260 2012 10 18.84 S 12.8 - 40.6L 4 150 0.5 5 0.01 200 ICQ XX HAR11 Christian Harder; bei 192x Schweifansatz & stellarer Kern sichtbar
260 2012 10 18.51 S 12.4 TA 25.4L 4 102 1 4 ICQ XX YOS02 Katsumi Yoshimoto
260 2012 10 16.90 S 11.4 TI 23.5T10 94 3 3 ICQ XX LAB02 Carlos Labordena
260 2012 10 16.70 xC 12.5 TJ 7.1A 3a100 1 5 4.0m225 ICQ XX HAR10I S 1 mCKD CAC SI5 9.8 5.0s 5.0 Ken Harikae
260 2012 10 15.71 xC 12.1 TJ 7.1A 3a119 1.1 5 4.3m225 ICQ XX HAR10I S 1.1 mCKD CAC SI5 9.8 5.0s 5.0 Ken Harikae
260 2012 10 14.72 aH 12.1 LA 16.0L 6a300 0.8 1.8m220 ICQ XX YOS0240a 30C 1.2 mST9 K26 SI5 11.4 4.1s 4.1 Katsumi Yoshimoto
260 2012 10 14.71 aV 12.6 LA 16.0L 6a300 0.8 1.9m220 ICQ XX YOS0240a 30C 1.2 mST9 K26 SI5 12.1 4.1s 4.1 Katsumi Yoshimoto
260 2012 10 14.70 aC 13.0 LA 16.0L 6a300 1.2 6.0m220 ICQ XX YOS0240a 15C 1.2 mST9 K26 SI5 12.1 4.1s 4.1 Katsumi Yoshimoto
260 2012 10 13.94 S 11.3 TI 23.5T10 94 3 3 ICQ XX LAB02 Carlos Labordena
260 2012 10 13.92 S 12.1 HS 44.0L 5 100 0.7 4 ICQ XX HAS02 Werner Hasubick
260 2012 10 13.54 S 11.8 AC 18.0L 5 180 0.6 4 ICQ TA WOL01 Graham W. Wolf
260 2012 10 13.30 S 13.7 AC 44.5L 4 167 0.5 4 ICQ XX MOR03 Warren Morrison, Cavan, Ontario
260 2012 10 12.97 S 12.2 HS 54.0L 5 120 1.1 2 0.03 ICQ XX KUT Walter Kutschera; 6.2 komet zeigt sich als rund mit ansatz
260 2012 10 12.83 S 12.6 TT 20.3L 6 63 1.5 5 ICQ XX GUZ Piotr Guzik
260 2012 10 12.00 S 12.5 TT 20.3L 6 63 1.5 5 ICQ XX GUZ Piotr Guzik
260 2012 10 11.90 S 11.5 TK 20.0T10 80 1.8 2/ ICQ XX KAS01 Volker Kasten; 6.3 Komet als mattes Glimmen am Westrand von NGC 752 zu sehen.
260 2012 10 11.80 S 11.6 TI 40.6L 4 150 0.5 4 ICQ XX HAR11 Christian Harder; 6.0
260 2012 10 11.48 S 11.4 AC 18.0L 5 180 1.8 2 ICQ TA WOL01 Graham W. Wolf
260 2012 10 10.85 S 12.3: - 40.6L 4 150 0.6 4 0.01 200 ICQ XX HAR11 Christian Harder; breiter kurzer Schweif bei 192x
260 2012 10 10.52 S 11.6 AC 18.0L 5 180 1.2 2 ICQ TA WOL01 Graham W. Wolf
260 2012 10 09.90 M 13.3 HS 35.0L 5 107 1.2 6/ ICQ XX CER01 Jakub Cerny
260 2012 10 09.84 S 12.3 TI 25.2L 6 88 1.2 3 0.03 160 ICQ XX HAR11 Christian Harder
260 2012 10 09.84 B 11.2 TI 23.5T10 67 3 3 ICQ XX LAB02 Carlos Labordena
260 2012 10 09.79 S 12.2 HS 32.0L 5 48 0.7 2 ICQ XX PIL01 Uwe Pilz; 20.7
260 2012 10 09.51 S 11.4 AC 18.0L 5 180 1.5 2 ICQ TA WOL01 Graham W. Wolf
260 2012 10 09.29 dk 11.9 LA 30.5T 7A020 0.94 ICQ XX CER01MAa 30C 0.94mG2x K6M GAI 5 U9* 0.2 1.0s 1.0 Jakub Cerny
260 2012 10 09.10 S[11.7 AC 15.0T10 37 ICQ XX AGUaa Salvador Aguirre, Campestre Real del Molinito, Hermosillo, Sonora, Mexico
260 2012 10 08.84 S 11.8 TI 25.2L 6 88 1.3 2 ICQ XX HAR11 Christian Harder; 6.3 Swanfilter wirkt nicht
260 2012 10 08.52 S 11.6 AC 18.0L 5 180 1 2 ICQ TA WOL01 Graham W. Wolf
260 2012 10 07.59 S 11.5 AC 18.0L 5 180 1.8 4 ICQ TA WOL01 Graham W. Wolf
260 2012 10 06.54 S 11.0 AC 18.0L 5 180 2.6 4 ICQ TA WOL01 Graham W. Wolf
260 2012 10 05.86 S 10.6 TK 20.3T10 77 5 3/ ICQ XX GON05 Juan Jose Gonzalez Suarez
260 2012 10 05.51 S 10.8 AC 18.0L 5 180 4.5 3 ICQ TA WOL01 Graham W. Wolf
260 2012 10 03.52 S 11.0 AC 18.0L 5 180 1.8 4 ICQ TA WOL01 Graham W. Wolf
260 2012 09 27.38 S 13.1 AC 44.5L 4 167 0.9 3 ICQ XX MOR03 Warren Morrison, Cavan, Ontario
260 2012 09 24.82 S 12.3 TA 25.4L 4 102 1.2 4 ICQ XX YOS02 Katsumi Yoshimoto
260 2012 09 24.69 xS 12.5 TA 25.0L 5 39 1.5 2 ICQ XX WYA Christopher Wyatt
260 2012 09 23.03 S 11.4 HN 20.3L 6 71 2.5 6 ICQ XX PAR03 Mieczyslaw Leszek Paradowski, Dabrowa; Comparison stars taken from APASS (AQ).
260 2012 09 22.90 S 11.8 TI 25.0L 6 125 1.2 3 ICQ XX HAR11 Christian Harder
260 2012 09 22.16 S 11.3 TT 10.8L 4 27 2.5 4 ICQ TA GET Stephen Getliffe
260 2012 09 21.42 C 12.5 MC 61.0C10a 35 ICQ XX DYMaaI C 6.4 sFL9 KA9 A46 5 P5 0.8s 0.8 Roger Dymock, SSON, USA
260 2012 09 20.56 xS 12.3 TA 25.0L 5 83 1.6 3/ ICQ XX WYA Christopher Wyatt
260 2012 09 19.85 S 11.8 TI 40.6L 4 150 1.1 5 ICQ XX HAR11 Christian Harder; Swanfilter wirkte nicht
260 2012 09 18.89 S 11.8 TI 40.6L 4 150 1 5 ICQ XX HAR11 Christian Harder; Swanfilter wirkte nicht
260 2012 09 18.00 M 12.8 AU 35.6L 5 133 1.1 6 ICQ XX NOV01 Artyom Novichonok
260 2012 09 16.20 dk 12.3 LA 30.5T 7A120 1 ICQ XX CER01MAa 30C 1 mG2x K6M GAI 5 U9* 0.2 1.0s 1.0 Jakub Cerny
260 2012 09 15.97 M 11.9 HN 20.3L 6 71 1.5 5 ICQ XX PAR03 Mieczyslaw Leszek Paradowski, Dabrowa; Comparison stars taken from APASS (AQ)
260 2012 09 15.92 M 12.5 AU 35.6L 5 133 1.5 6 ICQ XX NOV01 Artyom Novichonok
260 2012 09 15.80 xC 11.4 TJ 7.1A 3a 59 1 4 ICQ XX HAR10I S 1 mCKD CAC SI5 7.2 5.0s 5.0 Ken Harikae
260 2012 09 15.77 S 12.4 TA 40.0L 4 75 2.4 6/ ICQ XX YOS04 Seiichi Yoshida
260 2012 09 15.70 S 13.0 AC 40.0L 6 240 0.8 6 ICQ TA WOL01 Graham W. Wolf
260 2012 09 15.06 S 11.9 TI 23.5T10 138 2 3 ICQ XX LAB02 Carlos Labordena
260 2012 09 14.99 S 12.6 HS 32.0L 5 96 1 d3 ICQ XX PIL01 Uwe Pilz; 21.6 fächerförmiger Schweifansatz nach Westen, auffallend längliche zentrale Kondensation (NNO-SSW). Reagiert nur schwach auf Filter.
260 2012 09 14.70 S 12.6 AC 30.0L 6 240 1.5 3 ICQ TA WOL01 Graham W. Wolf
260 2012 09 14.68 xS 12.8 TA 25.0L 5 39 1.7 2 ICQ XX WYA Christopher Wyatt
260 2012 09 13.97 S 11.4 TK 20.3T10 100 2 4 ICQ XX GON05 Juan Jose Gonzalez Suarez
260 2012 09 13.91 M 12.4 HS 35.0L 5 107 2.2 7 ICQ XX CER01 Jakub Cerny
260 2012 09 13.21 dk 12.4 LA 30.5T 7A520 1 ICQ XX CER01MAa 30C 1 mG2x K6M GAI 5 U9* 0.2 1.0s 1.0 Jakub Cerny
260 2012 09 12.91 M 12.8 AU 35.6L 5 133 1.2 6 ICQ XX NOV01 Artyom Novichonok
260 2012 09 12.79 xC 12.0 TJ 7.1A 3a 59 1.4 4 ICQ XX HAR10I S 1.4 mCKD CAC SI5 8.5 5.0s 5.0 Ken Harikae
260 2012 09 11.90 M 13.1 AU 35.6L 5 133 0.7 6 ICQ XX NOV01 Artyom Novichonok
260 2012 09 11.20 dk 13.0 LA 30.5T 7a560 0.94 ICQ XX CER01MAa 30C 0.94mG2x K6M GAI 5 U7* 0.2 1.0s 1.0 Jakub Cerny
260 2012 09 11.00 C 13.2 HN 15.0L 5a 30 0.81 ICQ XX PAR03I C 0.81mCKD CAC MIm 5 U9 0.1 12.1 2.0s 2.0 Mieczyslaw Leszek Paradowski, Lublin; Baader Neodymium filter used. Processing&Photometry in IRIS on selected green channel. Calibration star from APASS [AQ]
260 2012 09 09.57 xS 12.7 TA 25.0L 5 83 0.9 2 ICQ XX WYA Christopher Wyatt
260 2012 09 08.85 M 12.4 HS 35.0L 5 64 1.3 6 ICQ XX CER01 Jakub Cerny
260 2012 09 06.91 S 11.0 TK 20.3T10 100 2.5 3 ICQ XX GON05 Juan Jose Gonzalez Suarez
260 2012 08 29.36 S 13.7 AC 44.5L 4 167 0.5 5 ICQ XX MOR03 Warren Morrison, Cavan, Ontario
260 2012 08 26.80 H 12.6 TA 16.0L 6a360 1.2 8.0m241 ICQ XX YOS02I a 15C 1.2 mST9 K26 SI5 11.1 4.1s 4.1 Katsumi Yoshimoto
260 2012 08 26.79 C 13.6 TA 16.0L 6a660 1.2 10.0m241 ICQ XX YOS02I a 5C 1.2 mST9 K26 SI5 11.9 4.1s 4.1 Katsumi Yoshimoto
260 2012 08 26.79 V 13.7 TA 16.0L 6a360 0.8 8.0m241 ICQ XX YOS02I a 15C 1.2 mST9 K26 SI5 11.9 4.1s 4.1 Katsumi Yoshimoto
260 2012 08 26.74 S 13.0 AC 30.0L 6 240 0.8 3 ICQ TA WOL01 Graham W. Wolf
260 2012 08 24.75 xS 13.2 AQ 25.0L 5 83 0.5 3/ ICQ XX WYA Christopher Wyatt
260 2012 08 23.74 S 13.0 AC 30.0L 6 240 0.6 4 ICQ TA WOL01 Graham W. Wolf
260 2012 08 22.05 S 12.6 HN 30.0L 5 100 1.1 5 0.03 240 ICQ XX PAR03 Mieczyslaw Leszek Paradowski, Dabrowa; Comparison stars taken from APASS (AQ). Nearby field stars checked in DSS. 14.28 mag (AQ) star in coma. Coma elongated in PA 240 deg
260 2012 08 22.02 S 11.8 TK 20.3T10 77 1.3 3/ ICQ XX GON05 Juan Jose Gonzalez Suarez
260 2012 08 21.37 S 13.7 AC 44.5L 4 167 0.5 4 ICQ XX MOR03 Warren Morrison, Cavan, Ontario
260 2012 08 20.35 dk 12.3 LA 30.5T 7a960 0.97 ICQ XX CER01MAa 30C 0.97mG2x K6M GAI 5 U9* 0.2 1.0s 1.0 Jakub Cerny
260 2012 08 19.74 S 12.8 AC 30.0L 6 240 1 6 ICQ TA WOL01 Graham W. Wolf
260 2012 08 19.70 S 13.0 TA 40.0L 4 75 1.6 6 ICQ XX YOS04 Seiichi Yoshida
260 2012 08 18.34 dk 12.9 LA 30.5T 7A280 0.97 ICQ XX CER01MAa 30C 0.97mG2x K6M GAI 5 U9* 0.2 1.0s 1.0 Jakub Cerny
260 2012 08 16.34 dk 13.1 LA 30.5T 7A440 0.84 ICQ XX CER01MAa 30C 0.84mG2x K6M GAI 5 U9* 0.2 1.0s 1.0 Jakub Cerny
260 2012 08 07.71 aC 14.5 HV 35.0C14a360 0.3 5 1.0m240 ICQ XX TSU02 1a 3S 1 mSTL KA1 SI6 9.5 1.1s 1.1 Mitsunori Tsumura
260 2012 07 28.29 S 11.6 AU 22.0L 6 160 2.5 2 ICQ XX GOI Marco Goiato
260 2012 07 23.96 C 14.6 UD 40.0Y 8a120 0.4 2.1m238 ICQ XX NOV01I C 0.46mSTL KA1 A46 4 P3 1.8s 1.8 Artyom Novichonok
260 2012 07 23.10 S 12.8 TA 20.3T10 133 1.3 3 ICQ XX GON05 Juan Jose Gonzalez Suarez
260 2012 07 19.04 O[14.7 HS 35.0L 5 117 ! 0.8 ICQ XX CER01 Jakub Cerny
260 2012 07 01.35 dk 15.7 LA 30.5T 7C040 0.45 ICQ XX CER01MAa 30C 0.45mG2x K6M GAI 5 U9* 0.2 1.0s 1.0 Jakub Cerny
260 2012 06 30.32 dk 15.8 LA 30.5T 7A440 0.45 ICQ XX CER01MAa 30C 0.45mG2x K6M GAI 5 U9* 0.2 1.0s 1.0 Jakub Cerny
260 2005 10 24.65 S[13.8 TA 40.0L 4 257 ! 0.7 ICQ XX YOS04 Seiichi Yoshida
260 2005 09 03.96 aS 13.7 HN 31.0J 6 155 0.5 5/ ICQ TA BOU Reinder J. Bouma
260 2005 08 29.99 S 13.7 HS 44.0L 5 156 0.4 4 ICQ XX HAS02 Werner Hasubick
260 2005 08 05.72 S 13.9 HS 40.0L 4 257 0.5 4 ICQ XX YOS04 Seiichi Yoshida