Team One Astronomical observatory
Moments of the ІІІ and 
  ІV contacts in UT
φ=42,667°; λ=26,317°; h=228m
І and ІІ contact are not registered due to dense cloudiness continued to 8,30 UT. After the sky became clear wind in blasts came out with speed of 4-5 m/s and that continued to the end of the observation. The telescope 150/2250 is in a pavilion. The telescope 63/840 was mounted in open and the wind influenced greater on its stability. The air-temperature was about 24°С.
ІІІ contact: 
Nikolai
Kacharov:  11h.03m.38,27s.;
visual with telescope150/2250
and magnification
W=140x
ІV contact:
Nikolai Kacharov:  
  11h.22m.48,41s.; visual with telescope 
  150/2250 and magnification W=140x
  Ivanka Gecova:      
  11h.22m.34,29s.; visual with telescope 
  63/840 and magnification W= 84х
  
 
     
 
     

 
     
 
     
  
 
     
 
      
  
   
      
     
  
 
     
Team Two Astronomical observatory
Astronomical observatory, observation stage – roof of TCC
Φ
= 42,667°
N; λ = 26,317°
E; H = 261 m
Diana Kiryakova – Team leader
Participants: Polina Doneva, Marina Koleva, Ivelina Vankova, Elena Slavcheva, 
  Zlatina Vankova, Vasilena Barbayaneva, Plamena Stefanova, Ivelina Kalcheva and 
  Christo Dimitrov.
  
  Observational devices: 
  Telescope – refractor 100/1000, with SFO – 80 filter and 
  following the Sun. Used for taking pictures with eyepiece multiplication of 
  25-H and 10-H, with camera “Zenith 12XP”; visual observations with 
  eye-lens revolver; visual location of IIIrd and IVth contact 
  with 10-H eye-lens and Hershel’s prism.
  Telescope – refractor 63/840  with 
  following the Sun and solar screen. Used for 16-H eye-lensed solar projection.
  Telescope – refractor 63/840 with SFO-80 
  filter, without following the Sun. Used for public observations with 16-H eye-lens. 
  At first it was enmarked for visual location of the moments of contacts but 
  because of the strong swaying from the wind, contacts were determined by the 
  100/1000 telescope.
  Camera “Canon Power Shot A70”.
Materials about what and how to be observed had been published in the 
  local press, before the Venus’s passage. We had also explained to the local radio stations and cable televisions what the 
  phenomenon was, why it was interesting and what precautions should be taken 
  during observation. Some of the journalists joined during the transit. The phenomenon 
  was also observed by students and other people who came to the observation place.
 
     
  
 
     

 
     
  