Fig. 3.
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PNLFs of the inner and outer regions of NGC 1351, binned in 0.2 mag intervals. The solid and open points represent data brighter than and fainter than the completeness limit, respectively. One overluminous PN was excluded from the outer PN sample; that object is also shown as an open circle. The curves show the analytic PNLF, shifted using the most likely apparent distance modulus and normalization.
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