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Table 5

The temporal variations of the Fe I excited levels in vFe I Exc, heliocentric velocity (km s−1), bFe I Exc value (km s−1) and Log N column density (in Log cm−2, identified by the energy level in cm−1) evaluated by fitting simultaneously all excited levels absorption lines, epoch by epoch.

Periods 2003–2004 2004–2007 2007–2008 2008–2009 2009–2010 2010–2011 2013–2014 2014–2015 2015–2016 2016–2017
Nb. Obs. 215 42 198 417 54 207 453 60 190 1080
vFe I Exc 20.39 ± 0.03 20.37 ± 0.09 20.39 ± 0.08 20.45 ± 0.03 20.47 ± 0.14 20.33 ± 0.07 20.34 ± 0.08 20.85 ± 0.17 20.19 ± 0.15 20.18 ± 0.06
bFe I Exc 0.80 ± 0.10 0.78 ± 0.33 1.20 ± 0.20 0.98 ± 0.09 1.00 ± 0.53 1.22 ± 0.17 0.89 ± 0.29 1.47 ± 0.51 1.14 ± 0.54 1.00 (fixedb)
log NFeI 416a 11.61 ± 0.02 11.55 ± 0.05 11.64 ± 0.03 11.60 ± 0.02 11.54 ± 0.07 11.65 ± 0.03 11.39 ± 0.04 11.54 ± 0.08 11.31 ± 0.08 11.45 ± 0.03
log NFeI 704 11.25 ± 0.03 10.84 11.38 ± 0.05 11.40 ± 0.03 11.15 11.30 ± 0.08 11.09 ± 0.08 11.11 ± 0.15 10.84 11.16 ± 0.06
log NFeI 888 11.01 ± 0.06 11.18 ± 0.08 10.69 10.88 ± 0.07 <10.96 11.03 ± 0.10 10.81 10.86 10.73 10.74
log NFeI 978 10.51 <10.47 <10.10 10.45 10.73 <10.65 10.50 <10.65 <10.06 <9.91
log NFeI 6928a 10.92 ± 0.01 10.87 ± 0.04 10.88 ± 0.04 10.93 ± 0.02 10.90 ± 0.07 11.03 ± 0.03 10.60 ± 0.05 10.75 ± 0.08 10.67 ± 0.07 10.75 ± 0.03
log NFeI 7377 10.47 ± 0.03 10.49 ± 0.08 10.45 ± 0.09 10.54 ± 0.03 10.51 10.45 ± 0.09 10.06 9.92 10.22 ± 0.20 10.34 ± 0.06
log NFeI 7728 <9.67 <10.74 10.83 10.27 10.88 <10.41 <9.80 <10.23 <10.40 <9.93
log NFeI 7986 <9.90 <9.98 <10.14 9.87 <10.07 10.31 10.15 <9.67 <10.02 <9.10
log NFeI 8155 <8.90 <10.15 9.95 10.18 <10.36 <10.08 <9.35 <9.33 10.17 <9.63
log NFeI 11976 9.68 9.56 9.59 9.61 9.55 9.82 ± 0.08 9.43 9.67 ± 0.13 <9.11 9.49 ± 0.12
log NFeI 12561 9.24 <8.39 9.15 9.35 <9.48 9.43 9.00 <9.18 9.14 9.12
log NFeI 12969 9.12 9.27 9.35 9.28 <9.44 9.24 <8.47 9.28 <9.11 9.23
11.93 ± 0.01 11.84 ± 0.04 11.96 ± 0.03 11.97 ± 0.02 11.87 ± 0.06 11.97 ± 0.03 11.73 ± 0.03 11.80 ± 0.06 11.61 ± 0.07 11.75 ± 0.03

Notes. The sum of the column density in all excited levels is given in the last line. (a) Individualizes the rows with the cleanest column density determination. Those are plotted as solid lines in Fig. 3. (b) The b-value was fixed at the median value from past measurements, because Owens.f was unable to converge on a realistic value.

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