Between 1989-1997 an intensive comet photometry program at Crni Vrh Observatory resulted in contribution of hundreds of CCD observations to the ICQ database and IAU Circulars. This also created a need for an observation database. The first version was created in 2002 and was used by Slovenian comet observers, The database currently contains 35 visually observed comets during the period 2002-2008. The best observed comets, with complete light-curves collected have been C/2002 C1 (Ikeya-Zhang), C/2002 V1 (NEAT), C/2001 Q4 (NEAT) and C/2004 Q2 (Machholz) as well as outburst of comet 17P/Holmes in late 2007.
The new online Comet Observation Database (COBS) is unique service, offering comet observers to submit, display and analyse comet data in a single location. It is maintained by the Crni Vrh Observatory and is opened to comet observers worldwide. Registered observers may now submit the observations using a simple web-based form which will store their observations into an SQL database and display them in ICQ format. Furthermore the users will be able to create light-curve graphs of a selected comets and see all the observations. We encourage comet observers worldwide to submit their observations and contribute to the COBS database.
Observers are reminded that the ultimate address which is collecting and storing comet data is International Comet Quarterly.
Type Comet name Obs date Mag Dia DC Tail Observer
C 2012F6 2013 06 16.95 8.6 5.3 5 PAR03
C 2013G1 2013 06 16.66 17.9 0.2 HILaa
C 29 2013 06 16.61 12.5 0.5 HILaa
C 2012C1 2013 06 15.80 16.8 0.2 HILaa
C 29 2013 06 15.43 12.5 0.4 HILaa
V 29 2013 06 15.08 12.2 0.5 7/ GOI
C 29 2013 06 14.63 12.6 0.4 HILaa
C 29 2013 06 10.64 13.9 0.5 HILaa
C 2012F6 2013 06 10.00 8.2 5.1 5 PAR03
C 2011L4 2013 06 09.99 9.7 5.1 5 PAR03
C 2013E2 2013 06 09.85 13.3 0.3 HILaa
C 246 2013 06 09.80 14.5 0.4 HILaa
C 117 2013 06 09.62 14.5 0.4 HILaa
C 2012K1 2013 06 09.60 14.7 0.4 HILaa
C 2013G7 2013 06 08.63 17.6 0.2 HILaa
Comet Magnitude Trend Observable When visible Lemmon (2012 F6) 7.5 fade 50 N to 40 S best morning PanSTARRS (2011 L4) 9 fade 50 N to 10 N all night LINEAR (2012 L2) 10 steady 30 S to 70 S early evening LINEAR (2011 F1) 11 ? steady 5 S to 90 S morning LONEOS (2006 S3) 11 fade 45 N to 70 S best evening 63P/Wild 11 steady 45 N to 55 S evening 246P/NEAT 12 steady ? 40 N to 90 S best morning Iwamoto (2013 E2) 12.5 fade 35 N to 45 S dawn ISON (2012 S1) 13 bright Poor elongation McNaught (2011 R1) 13 fade 50 N to 40 S best evening LINEAR (2012 A2) 13 fade Poor elongation 29P/Schwassmann-Wachmann 13 ? varies 40 N to 80 S best evening Garradd (2009 P1) 13.5 ? fade 15 N to 65 S evening LINEAR (2010 S1) 13.5 steady 50 N to 25 S best morning PanSTARRS (2012 K1) 13.5 bright 50 N to 40 S all night 2P/Encke 15 ? bright 15 N to 30 S dawn
List of comets maintained by Jonathan Shanklin at http://www.ast.cam.ac.uk/~jds.
Cbet nr. 3548, issued on 2013, June 09, announces the discovery of an apparently asteroidal object (discovery magnitude ~19.6) by R. A. Kowalski on CCD images obtained with the Catalina Sky Survey 0.68-m Schmidt telescopeon June 02. After posting on the Minor Planet Centers NEOCP webpage, this apparently asteroidal object as been found to show cometary features by by astrometric observers elsewhere. The new comet has been designated C/2013 L2 (CATALINA).
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Comet C/2012 S1 (ISON) was discovered on September 21, 2012 by Vitali Nevski and Artyom Novichonok on CCD images obtained with a 0.4-m f/3 Santel reflector of the International Scientific Optical Network (ISON) near Kislovodsk, Russia.
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This NASA Hubble Space Telescope image of Comet C/2012 S1 (ISON) was photographed on April 10, when the comet was slightly closer than Jupiters orbit at a distance of 386 million miles from the Sun (394 million miles from Earth).
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Cbet nr. 3478, issued on 2013, April 19, announces the discovery of a apparently asteroidal object (discovery magnitude ~19.6) by M. Schwartz and P. R. Holvorcem on CCD images obtained with the Tenagra II 0.41-m f/3.75 astrograph located near Nogales, AZ, U.S.A.
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Cbet nr. 3476, issued on 2013, April 16, announces the discovery of a new comet (discovery magnitude ~18) by R. H. McNaught on CCD images obtained with the 0.5-m Uppsala Schmidt telescope at Siding Spring on april 13.6. The new comet has been designated C/2013 G7 (McNAUGHT).
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