Reduce STIS NUV low dispersion "slit-less" spectra

will-henney commented 12 years ago

From the Bally observations.

will-henney commented 12 years ago

When Tsamis was here, I finished doing the line identifications and continuum subtractions.

1750 : N III] very weak, LV2 only
1909 : C III doublet
2145 : weak, LV2 and LV4 only
- possibly N III (2143,2144)
- possibly C III (2143,2145)
2326 : C II]
2470 : [O II]
2764 : He I - extremely weak - possibly does not exist
2800 : Mg II (2 795.528, 2 797.930, 2 797.998, 2 802.705)
- LV2, LV6, and possibly 158-326
2830 : He I 2 829.91 + [Fe IV] 2 830.19
- weak, LV2 and LV4 only
2946 : He I (2 945.967 vacuum)
- weak LV2 and LV4 only, possibly also from bowshocks

will-henney commented 11 years ago

Progress on reducing this data:

Testing out the new image attachment feature in Issues.

Those are continuum-subtracted line images of all the believable lines for LV2, LV4, LV6.

will-henney / proplyd-cloudy