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

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Table 1.

Dataset overview.

Galaxy	ESO Archive ID [Program ID]	Exp. time [s]	Seeing	N_PNe^a	N_PNe, 0.5^b
NGC 1052	ADP.2019-10-05T19-19-48.724 (0103.B-0837)	1685	0 $\overset{″}{.}$ ${{\overset{\prime\prime}{.}}}$ 61	86	26
NGC 1351	ADP.2017-12-12T15-38-27.863 (296.B-5054)	3379	0 $\overset{″}{.}$ ${{\overset{\prime\prime}{.}}}$ 69	86	16
NGC 1380	ADP.2017-01-30T14-39-33.249 (296.B-5054)	3369	0 $\overset{″}{.}$ ${{\overset{\prime\prime}{.}}}$ 63	112	23
NGC 1399	ADP.2017-03-27T13-16-27.827 (094.B-0298; 094.B-0903)	954	0 $\overset{″}{.}$ ${{\overset{\prime\prime}{.}}}$ 81	232	37
NGC 1404	ADP.2017-12-13T01:47:07.213 (296.B-5054)	3287	0 $\overset{″}{.}$ ${{\overset{\prime\prime}{.}}}$ 70	107	21

Notes.

NGC 1380 from Paper I. The other galaxies from Paper II.

Number of PNe at the top 0.5 magnitude of the PNLF.

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