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Table 3.

Ratio of the relative intensity of Fe XVII emission lines at 15.014 and 15.261 Å (I(15.01 Å)/I(15.26 Å), also labeled as I3C/I3D).

Source Ratio [I3C/I3D] References
Theory:
Bhatia & Doschek (1992) 4.28
Cornille et al. (1994) 4.57
Mohan et al. (1997) 3.99
Safronova et al. (2001) 3.43
Chen (2007) 3.54
Gu (2009) 3.50
Bernitt et al. (2012) 3.49
Oreshkina et al. (2014) 3.56
Santana et al. (2015) 3.44
Mendoza & Bautista (2017) 2.82
Wu & Gao (2019) 3.567

Laboratory:
LCLS (a) 2.61 ± 0.23 1
PLT (b) 2.48 ± 0.40 2
2.13 ± 0.37 3
EBIT (c) 3.04 ± 0.12 4
1.90 ± 0.11 (d) 5
2.63 ± 0.15 (e) 6
2.77 ± 0.3 7
PolarX-EBIT (f) 3.09 ± 0.08stat. ± 0.06sys. 8
AtomDB (g) 3.22

Astrophysical sources:
Sun 2.02 ± 0.28 9
NGC 4635 2.30 ± 0.18 10
Capella 2.42 ± 0.22 11
2.85 ± 0.14 12
EX Hya 2.46 ± 0.42 13
CAL 87 0.70−0.80 This work

Notes.

(a)

Linac Coherent Light Source (LCLS) (Emma et al. 2010) free-electron X-ray laser.

(b)

Princeton Large Torus (PLT) tokamak.

(c)

Livermore electron beam ion trap (EBIT).

(d)

Injection condition is in the high-pressure case.

(e)

Injection condition is in the low-pressure case.

(f)

PolarX-electron beam ion trap (PolarX-EBIT) (Micke et al. 2018).

(g)

AtomDB database version 3.0.9 (Smith et al. 2001; Foster et al. 2012; Foster & Heuer 2020).

References: (1) Bernitt et al. (2012); (2) Beiersdorfer et al. (2001); (3) Beiersdorfer et al. (2004); (4) Brown et al. (1998); (5) Brown et al. (2001); (6) Brown et al. (2001); (7) Brown et al. (2006); (8) Kühn et al. (2020); (9) Saba et al. (1999); (10) Xu et al. (2002); (11) Behar et al. (2001); (12) Mewe et al. (2001); (13) Mauche et al. (2001).

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