Pupillometry stimuli were generated using a custom-built Maxwellian-view optical system with three light-emitting diode primary lights (5 mm; ‘blue' λmax 464 nm, full width at half maximum (FWHM); 26 nm, ‘cyan' λmax 512 nm, FWHM 32 nm; and ‘green' λmax 560 nm, FWHM 12 nm; measured with a StellarNet EPC200C spectroradiometer, Tampa, FL, USA). The light from the primaries was spatially homogenized with 5° light shaping diffusers (Physical Optics Corp., Torrance, CA, USA) then focused through achromat doublet lenses (Edmund Optics, Barrington, NJ, USA). Each primary light was aligned along the optical axis using 50:50 beam splitters and field size was controlled by an aperture to create a 36° field. A 100-mm Fresnel lens (Edmund Optics, Singapore) projected stimuli into the plane of the right pupil in Maxwellian-view. Adapting field and stimulus irradiances were controlled by custom coded software (Xcode 3.3.3.5, Apple, Inc., Cupertino, CA, USA) and calibrated neutral density filters (Ealing, Natick, MA, USA). A chin rest and temple bars maintained participant alignment. The participant's left eye was recorded under infrared illumination (λmax 851 nm) in monochrome at 60 Hz (640 × 480 pixels; Point Grey FMVU-03MTM-CS; Richmond, BC, Canada; Computar TEC55 55 mm telecentric lens; Computar, Cary, NC, USA); recordings were synchronized to begin at paradigm onset and pupil diameters were analyzed offline using a custom developed program coded in Xcode.