Photometric analysis of an astronomical imaging system

Spectral type:
Apparent magnitude:	visual bolometric	Extra-atmospheric irradiance =
Apparent size:	arcmin arcsec	Object is

Altitude of source:	degree	Air mass =
Seeing:	arcsec

Model:
Width:	pixel mm	Field =	arcmin
Pitch:	μm	Plate factor =	arcsec/pixel
Quantum efficiency:	%	Sampling =	pixel/FWHM
Max efficiency wavelength:	nm
Full well capacity:	ke-	Integration time to 2/3 full well =
Quantization depth:	bit
Gain:	dB	Integration time to ADU =