How to Calculate Detected Power by a Radiotelescope?

[RHK]

Homework Statement

The specific power received by a radiotelescope is given by:

P_\nu = A \int {I_\nu (θ,\phi) f (θ,\phi) dθ d\phi}

where:
θ, \phi are the angular coordinates on the celestial sphere around the pointing direction;
I_\nu is the angular distribution of the specific intensity of the source (in units of W/m² Hz std);
A f(θ, \phi) is the effective area of the antenna in the direction (θ, \phi).

The radiotelescope, operating at a frequency of 3 GHz, of area A= 1000 m² and with f(θ, \phi)= 1 for θ₀>θ and f(θ, \phi)= 0 for θ>θ₀, with θ₀=1.9 arcminutes, is pointed in the direction of Mars (distance from the Earth d= 56 x 10⁶ km, diameter D= 6794 km), which has an emission approximated with a black body at T=210 K.
Calculate the detected power by the antenna in a band with Δ\nu=30 GHz around the working frequency.

[The specific intensity of a black body is: \frac{2h}{c^2}\frac{\nu^3}{e^{h\nu/KT}-1}
K=1.381 x 10^-23 J/K
h = 6.6 x 10^-34 J s ]

Homework Equations

The intensiy of a black body

The Attempt at a Solution

I can not go so far.
Just I have calculated the angular diameter of Mars: δ=arctan D/d = 25"=0.417'.

Any suggestion please?
I can not how to carry out the result, but I think that this is a particular educational exercise.
Thanks in advance.

 

[RHK]

Can I have just a start please?