Figure 3:
Total and prompt fluxes, together with spectral differences
Δ
=
(
𝜑
𝑝
,
𝑔
−
𝜑
𝑔
)
/
𝜑
𝑔
. (
𝜑
𝑝
,
𝑔
from case (f) and
𝜑
𝑔
from case (d) in Table
2
, spectral differences on right axis).
