Open Access

Table 1

List of spike features in the spectrum of Obs. 3814 with a significance > 2σ and associated lines, which are defined as having a distance of < 0.05 Å to the features.

Spike (Å) σ Ion Line(s) Wl. (Å) Ref.
4.37 2.0

5.30 2.0 S X L-shell 5.275 5, b
5.32 2.3

6.18 2.5 Si XIV Ly α 6.182 6, b

6.65 3.8 Si XIII i [em.] 6.685 3, b
Si XIII He α 6.648 3, b
Al XII He β 6.64 a

6.78 2.8 Fe XXIV 2p → 7d 6.809 1
Fe XXIV 2s → 6p 6.787 1
Si XI L-shell 6.784 5, b
Si I Kβ 6.753 2
Fe XXIV 2p → 7d 6.751 1
Si XIII f [em.] 6.740 3, a
Mg XII Ly γ 6.738 4

6.83 2.3 Si X L-shell 6.856 5, b
6.85 4.5 Fe XXIV 2p → 7d 6.809 1
Fe XXIV 2s → 6p 6.787 1

6.90 2.5 Fe XXIV 2p → 6s 6.982 1
6.92 5.7 Fe XXIV 2p → 6d 6.970 1
6.93 4.4 Si IX L-shell 6.928 5, b

6.98 2.1 Fe XXIV 2p → 6d 7.033 1
Si VIII L-shell 6.996 5, b
Fe XXIV 2p → 6s 6.982 1
Fe XXIV 2p → 6d 6.970 1

8.05 2.2 Fe XXIV 2p → 5d 8.059 1
Na XI Ly γ 8.021 4, a

9.28 2.2 Mg XI f [em.] 9.314 3, a
Ne X Ly ζ 9.29 a
Ne X Ly η 9.25 a
Ne IX i [em.] 9.23 a

9.37 3.3 Ne X Ly ϵ 9.36 a

9.48 2.1 Fe XXVI 2s → 3p 9.536 1
9.50 3.4 Fe XXVI 2p → 3d 9.532 1
Mg I Kβ 9.521 2
Ne X Ly δ 9.481 4, a

10.01 2.1 Fe XVII 2s22p6 → 2s2p65p 10.102 1
Fe XXV 2s → 3p 10.037 1
Na XI Ly α 10.025 6, a

10.63 2.2 Fe XIX 2p4 → 2p34d 10.664 1
Fe XXIV 2s → 3p 10.663 1
Fe XVII 2p6 → 2p56d 10.658 1
Ne IX He ϵ 10.643 8, a
Fe XXIV 2s → 3p 10.619 1

11.57 2.8 Na I Kβ 11.575 2
Ne IX He β 11.546 7, a
Fe XVIII 2p5 → 2p44d 11.539 1
Fe XVIII 2p5 → 2p44d 11.524 1

12.47 2.1 Fe XX 2p4 → 2p33d 12.475 1
Fe XXI 2p2 → 2p3d 12.445 1

12.57 2.2 Fe XX 2s2 2p3 → 2s 2p3 3p 12.576 1
Fe XXI 2p3 → 2p23d 12.602 1
Fe XX 2p4 → 2p33d 12.592 1
Fe XX 2s22p3 → 2s2p33p 12.570 1
Fe XX 2s22p3 → 2s2p33p 12.569 1
Fe XX 2s22p3 → 2s2p33p 12.558 1

12.70 2.3 Fe XXII 2p2 → 2p3s 12.710 1
Fe XVII 2p6 → 2p54s 12.702 1

12.85 3.2 Fe XX 2p3 → 2p23d 12.867 1
Fe XX 2p3 → 2p23d 12.809 1
Fe XVIII 2s22p5 → 2s2p53p 12.801 1

Notes. The listed lines are compiled the selection described in Sect. 3.4 and previous analyses of the data: (a) Hanke et al. (2009) and (b) Hirsch et al. (2019). Primary references are numbered and given below. (a) obtain line energies from (1, 8). (5) measure blended line complexes (‘L-shell’ for short in the table). Lines listed multiple times with different wavelengths differ in the fine structure. Emission lines are marked with [em.]. Iron lines are exclusively from AtomDB.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.