The 256×1 linear array of multiple quantum wells infrared photodetector (QWIP) is designed and fabricated for the peak response wavelength at λ P = 14.6 μm. The response spectral width is bigger than 2.2 μm. The two-dimensional (2D) diffractive coupling grating has been formed on the top QWIP photosensitive pixel for coupling the infrared radiation to the infrared detective layers. The performance of the device at V B = 3 V and T = 45 K has the responsibility 4.28×10 −2 (A/W), the blackbody detectivity D b * = 5.14×10 9 (cm·Hz 1/2 /W), and the peak detectivity D λ * = 4.24× 10 10 (cm⋅Hz 1/2 /W). The sensor pixels are connected with CMOS read out circuit (ROC) hybridization by indium bumps. When integral time is 100 μs, the linear array has the effective pixel of QWIP FPA N ef of 99.2%, the average responsibility R (V/W) of 3.48×10 6 (V/W), the average peak detectivity D λ * of 8.29×10 9 (cm·Hz 1/2 /W), and the non-uniformity U R of 5.83%. This device is ready for the thermal image application. quantum well, focal plane arrays, very long wavelength, infrared detector, diffraction gratingThe IR imaging systems that operate in the very long wavelength IR (VWIR) region are required in the space detection applications due to their correlation with the CO 2 absorption band. The square quantum wells are designed in such a way that the energy separation between the first excited state and ground state matches the energy of the infrared photons to be detected, which can cover the response wavelength from 3 to 18 µm for quantum well infrared photoconductor (QWIP). Both HgCdTe photodiodes and QWIPs have demonstrated the capability in the LWIR range. The performance figures of merit of state-of-the-art for QWIP and HgCdTe FPAs are similar because the main limitations come from the readout circuits. However, the HgCdTe process yield is low for