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Arp299 (NGC3690) is combine of two merging galaxy. Due this, there are lot of areas where dust is condensed and where supernovae occurs. At the moment of photographing there were two supernovae in the Arp299, SN 2010O and SN 2010P. The SN 2010P was discovered by researchers Seppo Mattila and Erkki Kankare by using the NOT-telescope. SN 2010P is only visible with the infrared wavelength and therefore it isn't "visible" in the pictures below that is taken by the THO research team by using the THO's 14" S-C-telescope.
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1:
Confimation pictures of the supernova SN 2010V.
Markku Nissinen and Veli-pekka Hentunen photographed the supernova SN 2010V confirmation pictures 7.2.2010
2:
Hentunen and Nissinen photographed the supernova SN 2010U
The brightness of the SN 2010U was about 16.6CR magnitudes.
3:
SN 2010O and SN 2010P in Arp299 (NGC 3690)
Supernova SN 2010O was observed by the THO research team.
4:
NGC 4857 and possible supernova
NGC 4857 photographed at THO by Hentunen
5:
The confirmation pictures of the supernovae SN 2009nr and SN 2010B
SN 2009nr and SN 2010B photgraphed.