Astronomers using a 2.0-m-diameter telescope observe a distant supernova—an exploding star. The telescope's detector records 9.1 × 10−11 J of light energy during the first 10 s. It's known that during this time, the supernova emitted 3.8 × 10−11 J of energy in the blue portion of the spectrum (λ = 470 nm) and 1.2 × 10−11 J in the red portion (λ = 650 nm). Assuming the detector is 100% efficient for both blue and red light, what is the flux of each type of light (in W/m²) at the telescope's location?