Figure 1.
![The distribution of INSPIRE galaxies in $\log$H$\alpha$ – $\log$[O ii] EWs, and colour-coded by DoR. Objects on the left side of the black dashed lines are classified as ‘High [O ii]/H$\alpha$’. The only ‘Low [O ii]/H$\alpha$’ galaxy from the INSPIRE sample is J1142+0122, which shows clear sign of AGN activity in its spectrum. Squares denote objects with a match in GALEX.](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/mnras/539/2/10.1093_mnras_staf514/1/staf514fig1.jpeg?Expires=1749376292&Signature=NAdWDlpHpE0t7DnVF84lnxvbr0hLgTE7j3EuumMc2nudmYtL2P3xFVPqGtUz7NMoKxC3xfBvMq8YpNjX7YhRJ7cWFh~M6YfZQBFKJQnU3WrA4TgpybJJAWHhxezPyd8mzDVwIP9QnJuSI73SAiKNgm4nDKpylOhx2BR0VsBmaHY4ez1lAbxnwCkeLK9w7BfAhTIzQ~SuiX-itM31ZzSBRCzAzIupy69yoqRzt1TpvGg58V8HoicAWjCgEzieiVP127dLjx91flbabBLn1vSLth4PDx2I9ZK2pFT-4zr3Bfj1Zo3iAfBiOnzJvREm7tqoroEKfcouIpcQgKffLYDyhA__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
The distribution of INSPIRE galaxies in |$\log$|H|$\alpha$| – |$\log$|[O ii] EWs, and colour-coded by DoR. Objects on the left side of the black dashed lines are classified as ‘High [O ii]/H|$\alpha$|’. The only ‘Low [O ii]/H|$\alpha$|’ galaxy from the INSPIRE sample is J1142+0122, which shows clear sign of AGN activity in its spectrum. Squares denote objects with a match in GALEX.
