Table 2: Predicted broad Ly$\alpha $, Ly$\beta $, Ly$\gamma $, H$\beta $, P$\alpha $, and broad/narrow two-photon luminosities (erg s-1).
Object Ly$\alpha $ Ly$\beta $ Ly$\gamma $ H$\beta $ P$\alpha $ Broad 2$\gamma $ Narrow 2$\gamma $
0505-67.9 $(4.90 \pm 4.61)_{36}$ $(1.09 \pm 0.34)_{36}$ - - - $(6.14 \pm 1.38)_{35}$ $(2.51 \pm 0.12)_{35}$
0509-67.5 $(2.68 \pm 2.05)_{35}$ $(1.29 \pm 0.14)_{35}$ $(2.04 \pm 0.08)_{34}$ $(5.97 \pm 0.36)_{33}$ $(1.07 \pm 0.06)_{33}$ $(6.16 \pm 0.02)_{35}$ -
0519-69.0 $(1.46 \pm 1.29)_{36}$ $(2.93 \pm 1.45)_{35}$ - - - $(5.00 \pm 1.37)_{35}$ $(2.86 \pm 1.83)_{35}$
SN 1006 $(8.42 \pm 2.57)_{32}$ $(2.54 \pm 0.15)_{32}$ - - - $(5.91 \pm 2.04)_{32}$ $(2.97 \pm 2.03)_{32}$
Kepler $(2.95 \pm 1.24)_{33}$ $(5.30 \pm 2.18)_{32}$ - - - $(1.01 \pm 0.15)_{33}$ $(5.82 \pm 3.70)_{32}$
RCW 86 $(2.30 \pm 0.94)_{32}$ $(3.48 \pm 1.47)_{31}$ - - - $(1.76 \pm 0.48)_{31}$ $(4.11 \pm 0.06)_{30}$
SNR 1987A $(2.96 \pm 0.05)_{35}$ $(7.64 \pm 0.59)_{34}$ $(1.99 \pm 0.44)_{34}$ $(5.96 \pm 1.40)_{33}$ $(1.06 \pm 0.25)_{33}$ $(6.43 \pm 0.52)_{35}$ $(5.75 \pm 0.70)_{35}$
Tycho $(1.03 \pm 0.04)_{32}$ $(2.32 \pm 0.44)_{31}$ - - - $(6.83 \pm 4.52)_{31}$ $(5.38 \pm 4.78)_{31}$

Note: Ab is shorthand notation for $A \times 10^b$.


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