|  | 
 
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    |  |  |  |  
    |  | Prof. Kirschbaum presented methods to measure
    the brightness of the night sky |  
    |  | Lux meter |  
    |  | Solar cell |  
    |  | CCD camera |  | 
 
  | 
  
   
    |  |  |  
    |  | Why not a normal digital photo camera? |  
    |  | These cameras are widespread, cheap and easy to
    handle |  
    |  | Can these camera’s be used for reliable
    measurements of the night sky brightness? |  
    |  |  |  | 
 
  | 
  
   
    |  |  |  
    |  | Costs about 150 euro |  
    |  | 3 megapixel |  
    |  | Manual setting |  
    |  | Maximum exposure time of 8 seconds |  
    |  | Raw exposures |  
    |  | F2.8 aperture |  
    |  |  |  | 
 
  |  | 
 
  | 
  
   
    |  |  |  
    |  | Minimal magnitude of stars of about 7 |  
    |  | Magnitude 1 stars saturated |  
    |  | Pixel counts of sky about 20 |  | 
 
  | 
  
   
    |  |  |  
    |  | Possible to make images and measurements of sky
    in different locations |  
    |  |  |  
    |  | Problem 1: always use the same camera and
    results are not comparable |  
    |  | Problem 2: Colour sensitivity of camera and eye
    are different |  | 
 
  | 
  
   
    |  |  |  |  
    |  | To make the measurements objective and
    comparable |  
    |  | Use the brightness of the stars to scale the
    method |  
    |  | Use a specific filter to make responses of the
    camera in visual, specific wavelengths |  
    |  |  |  | 
 
  | 
  
   
    |  |  |  |  
    |  | Falchi and Cinzano, CCD measurements of night
    sky brightness: |  
    |  | Make images of various parts of the sky with
    known stars with different altitudes |  
    |  | Determine the Extinction coefficient k |  
    |  | Determine the Photometric scale factor C |  
    |  | Determine the sky brightness at the location |  | 
 
  | 
  
   
    |  |  |  |  
    |  | Bought |  
    |  | Johnson V filter (100 euro) |  
    |  | A lot of memory (tiff files are 6 Mb) |  
    |  |  |  
    |  |  |  
    |  |  |  | 
 
  | 
  
   
    |  |  |  
    |  | No moon |  
    |  | 8 seconds |  
    |  | Tele (about 10 cm lens) |  
    |  | Aperture F2.8 |  
    |  | Focus 5 meter to obtain not saturated stars |  
    |  | Dark and flat frames |  
    |  |  |  | 
 
  |  | 
 
  |  | 
 
  | 
  
   
    |  |  |  
    |  | Extinction coefficient k= between  0,2 and 0,6 per airmass |  
    |  | Photometric scale factor C= 11,1 ±0,2 magnitude |  | 
 
  | 
  
   
    |  |  |  |  
    |  |  |  
    |  | The photometric scale factor  C gives the correction factor to make
    the camera a real  measuring device |  
    |  | The formula to make a pixel count P into a
    magnitude: |  
    |  | M=C-2,5*log(P/1168) |  
    |  | (1 pixel= 1168 square second) |  | 
 
  |  | 
 
  | 
  
   
    |  |  |  
    |  | Results not reliable with dark(er) skies |  | 
 
  | 
  
   
    |  |  |  |  
    |  | Try to find collaborators |  
    |  | Present results in Paris |  
    |  | Write an article about the results in Dutch |  
    |  | Try to get a camera with longer exposure time |  
    |  | Take this winter measurements in different towns
    in Holland |  
    |  | Take measurements in one sport uring a night |  
    |  | ?? |  
    |  |  |  |