Each star has its own zip file which contains .csv files with the integrated flux and FWHM values for each emission line, and a data quality code for the line profile. The data quality codes are 0 = well-detected emission line, 1 = non-detection, 2 = line-blending interference, and 3 = low signal to noise ratio in the data. The zip file also contains individual .csv files for each emission line with the raw wavelength, flux, error, and velocity data. Lastly, the files contain two sets of plots for the emission lines – wavelength vs flux plots and velocity vs flux plots. The table below gives the wavelength range and center for each emission line, these are standard for all stars.

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Line Ranges and Centers

Emission Line	Line Center (Å)	Minimum Wavelength (Å)	Maximum Wavelength (Å)
Si III	1206.50	1201.50	1211.50
H I	1215.67	1211.67	1221.67
N V – 1st Doublet	1238.821	1233.821	1240.821
N V – 2nd Doublet	1242.804	1240.824	1246.804
CO 14-3	1315	1309	1321
H2 [0,1] a	1338.57	1336.57	1340.57
H2 [0,2]a	1342.45	1340.45	1344.45
CO 14-4	1355	1350	1360
Si IV – 1st Doublet	1393.755	1383.755	1398.755
Si IV – 2nd Doublet	1402.77	1400.77	1409.77
H2 [0,1]b	1398.95	1396.95	1400.95
H2 [2,12]a	1434.53	1432.53	1436.53
H2 [0,2]b	1463.83	1461.83	1465.83
H2 [1,4]a	1489.57	1487.57	1491.57
H2 [1,7]a	1500.45	1498.45	1502.45
H2 [1,4]b	1504.76	1502.76	1506.76
H2 [1,7]b	1524.65	1522.65	1526.65
C IV – 1st Doublet	1548.202	1542.202	1549.702
C IV – 2nd Doublet	1550.774	1549.714	1555.774
H2 [2,12]b	1555.89	1553.89	1557.89
He II	1640.40	1635.40	1645.40

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Downloadable Zip Files: