The MUSE view of the Sculptor galaxy: Survey overview and the luminosity function of planetary nebulae

Open Access

Table 3.

Summary of the three distance-based samples and results of the fit.

Sample	All	Used	μ (mag)	D (Mpc)
All	571	320	$28 . 07_{- 0.05}^{+ 0.04}$ $28.07^{+0.04}_{-0.05}$	$4 . 10_{- 0.09}^{+ 0.07}$ $4.10^{+0.07}_{-0.09}$
0–4 kpc	158	87	$28 . 46_{- 0.09}^{+ 0.06}$ $28.46^{+0.06}_{-0.09}$	$4 . 91_{- 0.21}^{+ 0.14}$ $4.91^{+0.14}_{-0.21}$
4–8 kpc	251	148	$28 . 00_{- 0.08}^{+ 0.05}$ $28.00^{+0.05}_{-0.08}$	$3 . 97_{- 0.14}^{+ 0.09}$ $3.97^{+0.09}_{-0.14}$
> 8 kpc	162	85	$28 . 02_{- 0.10}^{+ 0.07}$ $28.02^{+0.07}_{-0.10}$	$4 . 02_{- 0.19}^{+ 0.12}$ $4.02^{+0.12}_{-0.19}$

Notes. The columns show the name of the sample, the number of PNe contained in the sample, the number of PNe used in the PNLF fit, the distance modulus, and the distance in Mpc.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.