Open will-henney opened 12 years ago
First step completed. Second step - identify the lines.
Second step completed. Example is
Third step is to wavelength-calibrate the spectra...
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.