The effect of the object magnitude at a specific observation band

For all the previous input flux distributions the intensity is rescaled according to the object magnitude and the observing band set by the user from the interface.

The following table provides the photometric zero points (Vega system) and links to the broad-band filter curves used in the magnitude calculations.

Band	Filter curve	Photometric zeropoint in ergs/s/cm2/A (flux for zero mag in Vega system)
U	U filter curve	U0 = 4.18023e-09
B	B filter curve	B0 = 6.60085e-09
V	V filter curve	V0 = 3.60994e-09
R	R filter curve	R0 = 2.28665e-09
I	I filter curve	I0 = 1.22603e-09
Z	Z filter curve	Z0 = 7.76068e-10
Y	Y filter curve	Y0 = 5.973e-10
J	J filter curve	J0 = 3.12e-10
H	H filter curve	H0 = 1.14e-10
K	K filter curve	K0 = 3.94e-11
L	L filter curve	L0 = 4.83e-12
M	M filter curve	M0 = 2.04e-12
N	N filter curve	N0 = 1.23e-13
Q	Q filter curve	Q0 = 6.8e-15