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Table 2

Bright spots per region and spectral slope values.

Region Ntot Npre Nperih Npost Areatot [m2] Slopepre [%/ (100 nm)] Slopeperih [%/(100nm)] Slopepost [%/(100 nm)]
Aker 1 1 0 0 3 7.2
Anhur 86 5 8 73 9512 3.5±2.2 4.8±0.9 −0.7±0.5
Anubis 5 0 4 1 701 7.5±0.6 8.1
Anuket 30 24 1 5 1573 3.4±0.7 9.2 1.1±1.3
Apis 0 0 0 0 0
Ash 63 30 0 33 466 5.5±0.5 2.7±0.6
Aten 31 3 0 28 741 6.5±1.8 1.2±0.4
Atum 7 2 0 5 166 0.2 1.1±0.5
Babi 32 5 0 27 384 5.5±1.5 0.2±0.5
Bastet 7 3 0 4 30 6.1 ±0.6 −0.8±1.2
Bes 25 4 6 15 8158 3.4±1.4 8.7±1.1 2.1±0.8
Geb 4 4 0 0 86 8.1±1.2
Hapi 12 2 2 8 399 7.0 1.1±1.2
Hathor 4 0 0 4 81 0.3±1.3
Hatmehit 30 1 1 28 466 7.3 8.8 2.3±0.7
Imhotep 80 38 13 29 15714 4.8±0.5 6.4±0.8 1.9±0.8
Khepry 9 6 1 2 202 3.3±1.9 3.9 −1.1±4.1
Khonsu 61 10 5 46 5472 6.4±1.0 7.0±1.1 1.1±0.7
Ma’at 14 2 0 12 207 6.3±0.3 1.5±0.8
Maftet 6 5 0 1 22 7.6±0.6 3.6
Neith 2 2 0 0 48 5.2±0.30
Nut 2 0 0 2 7 5.9±0.2
Serqet 5 0 1 4 214 5.9 5.2±1.6
Seth 54 0 1 53 1197 10.4 0.3±0.4
Sobek 1 0 0 1 60 3.7
Wosret 31 3 1 27 805 5.6±1.4 9.2 −0.5± 0.8

Notes. Ntot is the total number of bright spots per region identified, while Npre, Nperih, and Npost are the BS observed pre-, during-, and post-perihelion, respectively. The average spectral slope values of the bright spots are reported for the three time frames, when at least one BS is observed, with the associated errors when available (i.e., when there are at least two BS per region).

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