A characterization of ASAS-SN core-collapse supernova environments with VLT+MUSE - I. Sample selection, analysis of local environments, and correlations with light curve properties (Corrigendum)

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Volume 705 (January 2026)

A&A, 705 (2026) C1

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202346512]

Table 1.

General properties of the SNe and their host galaxies.

Name	Type^a	RA^b	Dec	Host Galaxy Name	z_host	A_v, MW ^c	M_B, host ^d
SN2018eog	II	20 28 11.970	−03 08 13.47	2MASS J20281135−0308096	0.01886	–	–
SN2018ant	II	08 36 31.450	−11 49 40.73	MCG-2-22-22	0.019784	0.192	–20.67
ASASSN-18oa	IIn	01 30 27.120	−26 47 05.98	ESO476-G16	0.019744	0.055	–20.48
SN2018bl	II	08 24 11.590	−77 47 16.55	ESO18-G9	0.017773	0.357	–20.70
SN2018evy	II	18 22 38.170	−15 41 47.66	NGC6627	0.017647	0.611	–20.59
SN2018cho	IIP	00 13 26.515	−17 29 19.57	IC4	0.016558	0.173	–20.72
SN2018ie	Ic	10 54 01.060	−16 01 21.40	NGC3456	0.013954	0.211	–20.76
...

Notes. The entire table is available online.

All the supernova types, coordinates, and host galaxy names were taken from Holoien et al. (2017a,b,c, 2019) and Neumann et al. (2023);

RA and Dec are given in the J2000 epoch;

the Galactic extinction, A_v, MW, was taken from the NASA-IPAC Extragalactic Database (NED);

the host galaxy absolute magnitudes in the B band, M_B, were taken from HyperLeda.

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