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Table C.2.

Feige 80: Used intervals (Int) in constrained abundance results from GSSP.

Element Int (Å) Line (Int) (Å)
C 7115.19 (7080-7152)
7111.47 & 7113.18 & 7115.19 & 7116.99 & 7119.67 (7080-7152)
N 8683.40 (8673-8740)
O 7771.94 & 7774.17 & 7775.39 (7770-7848)
8446.25 & 8446.36 & 8446.76 (8673-8740a)
Na 5657-5713 5688.21 (5657-5713)
6154.22 & 6160.75 (6133-6199)
Mg 5117-5210 4702.99 (4698-4724)
5528.40 (5496-5545)
8717.82 (8673-8739)
8736.02 (8673-8739)
Al 8673-8740 (d 8772.87 & 8773.9a)
Si 5904-6267 & 6333-6510 5772.15 (5751-5818)
6155.13 (5904-6267 & 6333-6510)
6347.10 (5904-6267 & 6333-6510)
8728.01 (8673-8740)
S 6748.79 (6694-6812)
6757.16 (6694-6812)
K 7698.97 (7697-7791a)
Ca 5904-6267 & 6333-6510 4581.40 & 4581.47 (4498-4609)
4498-4609 6717.70 (6694-6812)
5200-5355
Ti 4987-5054
5974-6267 & 6333-6510
V 4378-4446
Cr 4563-4608
5200-5354
Mn 5974-6267
4749-4769
4782-4824
Fe 5904-6267 & 6333-6510
4519-4608
5200-5354
Co 4117-4162
Ni 5904-6267 & 6333-6510 6767.77 (6694-6812)
Cu 5782.13 (5751-5818)
Zn 4722.16 (4694-4738)
4810.53 (4782-4830)
Sr 4077.71 (4043-4086)
4215.52 (4197-4252)
Y 4883.68 (4877-4927)
4900.12 (4877-4927)
Zr 4149.20 (44117-4162)
4211.88 (4197-4252)
Ba 4554.03 (4497-4609)
6141.71 (6006-6197)

a: not possible to constraint dilution from interval containing the line due to telluric bands. Dilution fixed using a clean nearby interval

Notes. Tables C.1 and C.2: When abundance is derived from specific line/s, the used procedure is to cut and normalise an interval containing the studied line (Line(Int)), firstly developing an abundance calculation with GSSP, based on that interval. From this preliminary study, the dilution value of the interval is obtained. Eventually, a new abundance calculation is developed on the specific line/s (short interval around) meanwhile the value of dilution, previously obtained, is fixed.

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