MUSE crowded field 3D spectroscopy in NGC 300 - IV. Planetary nebula luminosity function

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Table B.1.

Comparison for extinction values in [O III]λ5007 derived using different aperture correction methods.

ID	A₀	A₁	A₂	A₃	ΔA
E-2	0.542	0.589^a	0.353	0.457	0.189
E-11	0.615	0.663^a	0.445	0.531	0.170
P-2	1.342	1.229	1.093^b	1.252	0.113
H9-1	0.358	0.147	0.257	0.223	0.211
H9-6	0.490	0.279	-0.027^b	0.354	0.211
H10-2	0.694	0.420	0.344	0.506	0.274
H11-1	0.570	0.494	0.412	0.413	0.076
H11-2	1.440	1.364	1.276	1.283	0.076
L9-8	0.633	0.466	0.463	0.410	0.167

Notes. A₀ – no aperture correction; A₁ – reference star method; A₂ – bright PN method; A₃ – empirical relation method. The preferred extinction values are marked in bold.

bad reference star

uniform diffuse Hα background

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