The host of the Type I SLSN 2017egm - A young, sub-solar metallicity environment in a massive spiral galaxy

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Table 1

Coordinates (J2000.0) of the emission peaks for each H ii region that we identified.

Region	RA	Dec

H ii-1	10^h19^m07.90^s	+ 46^d26^m48.35^s
H ii-2	10^h19^m07.81^s	+ 46^d26^m47.32^s
H ii-3	10^h19^m07.84^s	+ 46^d26^m46.58^s
H ii-4	10^h19^m07.93^s	+ 46^d26^m47.36^s
H ii-5	10^h19^m08.00^s	+ 46^d26^m48.14^s
H ii-6	10^h19^m08.00^s	+ 46^d26^m49.14^s
H ii-7	10^h19^m08.05^s	+ 46^d26^m46.91^s

Notes. The H ii-2 region corresponds to the galaxy centre, while H ii-4 is the SLSN site.

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