Fig. 19.
Effective survey area as a function of redshift and M1450. The contours are plotted at 10 deg2, 40 deg2, 70 deg2, 100 deg2, and 130 deg2. The effective survey area includes the efficiency of the color selection for the mock quasars. The upper and lower edges are determined with i > 20.0 and i < 24.0 mag selection criteria. The gap seen in the middle reflects the effect of the masks around HSC objects brighter than i < 22.0 mag. For objects brighter than i < 22.0 mag, the masks are not applied. The completeness of the stellar classification is not included in the calculation.

Effective survey area as a function of redshift and M1450. The contours are plotted at 10 deg2, 40 deg2, 70 deg2, 100 deg2, and 130 deg2. The effective survey area includes the efficiency of the color selection for the mock quasars. The upper and lower edges are determined with i > 20.0 and i < 24.0 mag selection criteria. The gap seen in the middle reflects the effect of the masks around HSC objects brighter than i < 22.0 mag. For objects brighter than i < 22.0 mag, the masks are not applied. The completeness of the stellar classification is not included in the calculation.

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