π Measuring Sky Background for Sensor Calibration
Accurately measuring the sky background level with your astroimaging setup allows you to calibrate your sky brightness sensor.
π Requirements:
- π· Monochromatic camera with luminance filter
- π» Software: ASTAP (or similar)
βοΈ Procedure:
- π Download and install ASTAP and the star database (H17 recommended) from https://www.hnsky.org/astap.htm
- πΈ Capture a 15β60 second exposure with your camera and Luminance (L) filter
- πΌοΈ Open the image file in ASTAP
- π§© Click Solve to perform plate solving
- π§ Navigate to Tools β SQM Measurement
- βοΈ Enter the pedestal value β the mean value from the corresponding dark frame
- π The SQM (Sky Quality Meter) value is displayed directly
β Your sky brightness sensor is now calibrated.
Happy measuring!












