Towards precision cosmology with improved PNLF distances using VLT-MUSE - III. Impact of stellar populations in early-type galaxies

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Table B.1.

Distance modulus for each galaxy derived using three methods: PNLF, SBF, and TRGB.

Galaxy	(m − M)_{0, PNLF}	(m − M)_{0, SBF}	(m − M)_{0, TRGB}
NGC 1052	$31 . 26_{- 0.08}^{+ 0.07}$ $31.26^{+0.07}_{-0.08}$	31.44 ± 0.27	–
NGC 1351	$31 . 39_{- 0.08}^{+ 0.04}$ $31.39^{+0.04}_{-0.08}$	31.42 ± 0.07	–
NGC 1380	$31 . 10_{- 0.05}^{+ 0.04}$ $31.10^{+0.04}_{-0.05}$	31.63 ± 0.08	31.40 ± 0.07
NGC 1399	$31 . 23_{- 0.07}^{+ 0.06}$ $31.23^{+0.06}_{-0.07}$	31.60 ± 0.09	31.51 ± 0.07
NGC 1404	$31 . 37_{- 0.08}^{+ 0.05}$ $31.37^{+0.05}_{-0.08}$	31.53 ± 0.07	31.36 ± 0.07

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