Taurus Hill Observatory research team measured the spectrum of the supernova SN 2014J. For measurement the THO research team used SBIG STT-8300M -camera, StarAnalyser100 spectrum lattice and Rspec-program. The image shows clearly the typical Ia-type of supernova spectrum, including the Si-II absorbtion line with wavelength of 6100 Angstrom. This is caused by fusion of the […]
It has been a while since THO research team photographed supernovae. Here is a picture about the supernova SN 2014J, located in M82, taken by Veli-Pekka Hentunen in Taurus Hill Observatory. According to Veli-Pekka’s picture, the brightness of the supernova was about 10,92 magnitudes (CR, comparison star NOMAD1 1596-0106875).