Observatory code A95
Latest Articles
1: Confimation pictures of the supernova SN 2010V.
Markku Nissinen and Veli-pekka Hentunen photographed the supernova SN 2010V confirmation pictures 7.2.2010 by using the GRAS4 remote telescope (New Mexico). The confirmation was re..
2: Hentunen and Nissinen photographed the supernova SN 2010U
Hentunen and Nissinen photographed the supernova SN 2010U 6.2.2010 with GRAS1 remote telescope (see CBET 2161). The supernova is located in the galaxy NGC 4214. The supernova was discovered by Koichi ..
3: SN 2010O and SN 2010P in Arp299 (NGC 3690)
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 this photograph there are two supernovae in th..
4: NGC 4857 and possible supernova
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5: The confirmation pictures of the supernovae SN 2009nr and SN 2010B
Supernova SN 2009nr confirmation picture was takne with the GRAS09-telescope (CBET 2111).
The confirmation picture of the SN 2010B (CBET2115) was taken in Taurus Hill Observatory.
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6: Publications list has been updated.
The publication list of the Taurus Hill Observatory has been updated. Now there are all publications of the year 2009...
7: Taurus Hill Observatory Board and Staff Members for the Year 2010
Veli-Pekka Hentunen will be the Chairman of Board in the year 2010 and Tuomo Salmi takes the responsibility of the leading the research group of the Taurus Hill Observatory and Warkauden Kassiopeia. O..
8: Supernova SN 2009iy discovered at Taurus Hill Observatory
Veli-Pekka Hentunen and Markku Nissinen started the new observing season by discovering the supernova SN 2009iy. This discovery was made 15th of August from the galaxy UGC 8520. At the time of the dis..
9: Taurus Hill Observatory in European Planetary Science Congress 2009, Potsdam, Germany, 13.-18.9.
Taurus Hill Observatory has prepared a poster about the exoplanet research that is made in THO since 2006. The poster display time, time when the poster will be available for public, is from Wednesday..
10: Superova SN 2009bw is very dim
Superova SN 2009bw is very dim, about 17.5CR magnitudes. This photograph was taken by Markku Nissinen and Veli-Pekka Hentunen 19.8.2009. You can compare the brightness change in the second pictur..
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