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In the meantime, we could measure the widths of the [O III] and [N II], auroral and nebular, lines to use in the linewidth method for determining temperatures, for which I have opened a new issue: #30
In Henney & O'Dell (1999) we published only 4959, 6568, 6563, 6300, 6312, 5875. But there are many other lines in there too.
First step would be to get the spectra from Bob.
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