SPIP is a new instrument for the 2m Télescope Bernard Lyot (TBL) at Pic du Midi, located in the French Pyrénées. Observing in the 0.95-2.5 μm range (YJHK bands), SPIP at TBL will team with SPIRou at the 3.6m CFHT (Maunakea, Hawaii), aiming together at detecting and characterizing planetary worlds around nearby red dwarfs, and at documenting magnetized star / planet formation. This paper describes the instrument sub-systems integration and validation tests performed in Toulouse (France) with a particular focus on the H4RG detector, failure analysis and mitigation.
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