Fig. 1.
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Set of passbands describing the photometry of mock red quasars. The panels show the transmission efficiencies for the broad-band optical DECam griz filters, the Euclid VIS (optical) and NISP (NIR) filters, and the NIR to MIR VISTA JHKs filters. The vertical dashed lines are placed at the weighted central wavelength of each filter.
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