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* * * * * 260P/McNaught * * * * *
Year Mn Day MM Mag Ref Scope Pwr coma DC tail p.a. Obs Site 2012 9 15.932 S 12.6 AQ 30.5T 95 0.9 4/ DIJ Burlage 2012 9 15.931 S 12.7 AQ 30.5T 95 1.2 4 BOU Burlage, Germany 2012 9 15.77 S 12.4 TA 40.0L 75 2.4 6/ YOS Kita-karuizawa, Gunma (Bright, strongly condensed and easy to see.) 2012 9 13.97 S 11.4 TK 20.3T 100 2.0 4 GON Alto del Castro, León 2012 9 9.919 S 12.6 TA 30.5T 117 1.1 3 BOU Burlage, Germany 2012 9 9.917 S 12.4 AQ 30.5T 117 0.8 4 DIJ Burlage 2012 9 6.91 S 11.0 TK 20.3T 100 2.5 3 GON Llamas de Rueda, León 2012 8 26.74 S 13.0 AC 30.0L 240 0.8 3 WOL Moera, Lower Hutt 2012 8 23.74 S 13.0 AC 30.0L 240 0.6 4 WOL Moera, Lower Hutt 2012 8 22.02 S 11.8 TK 20.3T 77 1.3 3/ GON Alto del Castro, León (Brighter than expected.} 2012 8 19.74 S 12.8 AC 30.0L 240 1.0 6 WOL Moera, Lower Hutt 2012 8 19.70 S 13.0 TA 40.0L 75 1.6 6 YOS Kita-karuizawa, Gunma (Surprisingly bright, and easy to see. It looks like a 12-mag comet. 7 years passed since my last observation at the discovery in 2005. I remember it was a tiny faint comet at that time. So I was surprised the comet looks very bright now.) 2012 7 28.29 S 11.6 AU 22.0L 160 2.5 2 GOI Araçatuba 2012 7 23.10 S 12.8 TA 20.3T 133 1.3 3 GON Alto del Castro, León (Brighter than expected. Nearby field stars checked in DSS. Comparison stars taken from TASS photometry. Motion observed over a 45-min period. Mountain location, very clear sky.)
2005 10 24.65 S[13.8 TA 40.0L 257 !0.7 YOS Gunma, Japan (Not visible. Very close to the half moon. The field was covered with many faint stars, so it was hard to confirm a diffuse faint comet.) 2005 9 3.965 aS 13.7 HN 31.0J 155 0.6 5 DIJ Lauwersoog 2005 9 3.956 aS 13.7 HN 31.0J 155 0.5 5/ BOU Lauwersoog (Small, condensed object. Motion obvious over a 30m period.) 2005 8 5.72 S 13.9 HS 40.0L 257 0.5 4 YOS Gunma, Japan (A faint and small object was visible. Probably the comet was visible visually. I want other visual observers to confirm it with large telescopes. Michael Jäger reported P/2005 K3 is brighter than C/2005 K1 by 0.5 mag.)