The unabsorbed flux and luminosity of SN 2005gj, assuming various emission models with different parameters, and a distance of 266 Mpc. ‘Temp’ = Temperature of the plasma. Column refers to the intrinsic column, in addition to the Galactic column of 6.87 × 1020 towards the source. 3σ results are quoted.
Model . | Temp . | Column . | Flux . | Luminosity . |
---|---|---|---|---|
. | (keV) . | (cm−2) . | (erg s−1 cm−2) . | (erg s−1) . |
Power-law, Γ = 2 | – | – | 1.3 × 10−15 | 1.1 × 1040 |
(Using srcflux) | – | – | 1.13 × 10−15 | 9.5 × 1039 |
Plasma/APEC | 1.93 | – | 9.78 × 10−16 | 8.2 × 1039 |
Plasma/APEC | 4.85 | – | 1.42 × 10−15 | 1.2 × 1040 |
Plasma/APEC | 9.67 | – | 1.63 × 10−15 | 1.4 × 1040 |
Plasma/APEC | 1.53 | 1 × 1021 | 1 × 10−15 | 8.4 × 1039 |
Plasma/APEC | 1.53 | 5 × 1021 | 1.58 × 10−15 | 1.3 × 1040 |
Plasma/APEC | 1.53 | 1 × 1022 | 2.44 × 10−15 | 2.1 × 1040 |
Plasma/APEC | 1.53 | 2 × 1022 | 4.49 × 10−15 | 3.8 × 1040 |
Plasma/APEC | 3.06 | 1 × 1021 | 1.34 × 10−15 | 1.1 × 1040 |
Plasma/APEC | 3.06 | 5 × 1021 | 1.91 × 10−15 | 1.6 × 1040 |
Plasma/APEC | 3.06 | 1 × 1022 | 2.6 × 10−15 | 2.2 × 1040 |
Plasma/APEC | 3.06 | 2 × 1022 | 3.92 × 10−15 | 3.3 × 1040 |
Plasma/APEC | 4.85 | 1 × 1021 | 1.58 × 10−15 | 1.3 × 1040 |
Plasma/APEC | 4.85 | 5 × 1021 | 2.17 × 10−15 | 1.8 × 1040 |
Plasma/APEC | 4.85 | 1 × 1022 | 2.83 × 10−15 | 2.4 × 1040 |
Plasma/APEC | 4.85 | 2 × 1022 | 4.03 × 10−15 | 3.4 × 1040 |
Model . | Temp . | Column . | Flux . | Luminosity . |
---|---|---|---|---|
. | (keV) . | (cm−2) . | (erg s−1 cm−2) . | (erg s−1) . |
Power-law, Γ = 2 | – | – | 1.3 × 10−15 | 1.1 × 1040 |
(Using srcflux) | – | – | 1.13 × 10−15 | 9.5 × 1039 |
Plasma/APEC | 1.93 | – | 9.78 × 10−16 | 8.2 × 1039 |
Plasma/APEC | 4.85 | – | 1.42 × 10−15 | 1.2 × 1040 |
Plasma/APEC | 9.67 | – | 1.63 × 10−15 | 1.4 × 1040 |
Plasma/APEC | 1.53 | 1 × 1021 | 1 × 10−15 | 8.4 × 1039 |
Plasma/APEC | 1.53 | 5 × 1021 | 1.58 × 10−15 | 1.3 × 1040 |
Plasma/APEC | 1.53 | 1 × 1022 | 2.44 × 10−15 | 2.1 × 1040 |
Plasma/APEC | 1.53 | 2 × 1022 | 4.49 × 10−15 | 3.8 × 1040 |
Plasma/APEC | 3.06 | 1 × 1021 | 1.34 × 10−15 | 1.1 × 1040 |
Plasma/APEC | 3.06 | 5 × 1021 | 1.91 × 10−15 | 1.6 × 1040 |
Plasma/APEC | 3.06 | 1 × 1022 | 2.6 × 10−15 | 2.2 × 1040 |
Plasma/APEC | 3.06 | 2 × 1022 | 3.92 × 10−15 | 3.3 × 1040 |
Plasma/APEC | 4.85 | 1 × 1021 | 1.58 × 10−15 | 1.3 × 1040 |
Plasma/APEC | 4.85 | 5 × 1021 | 2.17 × 10−15 | 1.8 × 1040 |
Plasma/APEC | 4.85 | 1 × 1022 | 2.83 × 10−15 | 2.4 × 1040 |
Plasma/APEC | 4.85 | 2 × 1022 | 4.03 × 10−15 | 3.4 × 1040 |
The unabsorbed flux and luminosity of SN 2005gj, assuming various emission models with different parameters, and a distance of 266 Mpc. ‘Temp’ = Temperature of the plasma. Column refers to the intrinsic column, in addition to the Galactic column of 6.87 × 1020 towards the source. 3σ results are quoted.
Model . | Temp . | Column . | Flux . | Luminosity . |
---|---|---|---|---|
. | (keV) . | (cm−2) . | (erg s−1 cm−2) . | (erg s−1) . |
Power-law, Γ = 2 | – | – | 1.3 × 10−15 | 1.1 × 1040 |
(Using srcflux) | – | – | 1.13 × 10−15 | 9.5 × 1039 |
Plasma/APEC | 1.93 | – | 9.78 × 10−16 | 8.2 × 1039 |
Plasma/APEC | 4.85 | – | 1.42 × 10−15 | 1.2 × 1040 |
Plasma/APEC | 9.67 | – | 1.63 × 10−15 | 1.4 × 1040 |
Plasma/APEC | 1.53 | 1 × 1021 | 1 × 10−15 | 8.4 × 1039 |
Plasma/APEC | 1.53 | 5 × 1021 | 1.58 × 10−15 | 1.3 × 1040 |
Plasma/APEC | 1.53 | 1 × 1022 | 2.44 × 10−15 | 2.1 × 1040 |
Plasma/APEC | 1.53 | 2 × 1022 | 4.49 × 10−15 | 3.8 × 1040 |
Plasma/APEC | 3.06 | 1 × 1021 | 1.34 × 10−15 | 1.1 × 1040 |
Plasma/APEC | 3.06 | 5 × 1021 | 1.91 × 10−15 | 1.6 × 1040 |
Plasma/APEC | 3.06 | 1 × 1022 | 2.6 × 10−15 | 2.2 × 1040 |
Plasma/APEC | 3.06 | 2 × 1022 | 3.92 × 10−15 | 3.3 × 1040 |
Plasma/APEC | 4.85 | 1 × 1021 | 1.58 × 10−15 | 1.3 × 1040 |
Plasma/APEC | 4.85 | 5 × 1021 | 2.17 × 10−15 | 1.8 × 1040 |
Plasma/APEC | 4.85 | 1 × 1022 | 2.83 × 10−15 | 2.4 × 1040 |
Plasma/APEC | 4.85 | 2 × 1022 | 4.03 × 10−15 | 3.4 × 1040 |
Model . | Temp . | Column . | Flux . | Luminosity . |
---|---|---|---|---|
. | (keV) . | (cm−2) . | (erg s−1 cm−2) . | (erg s−1) . |
Power-law, Γ = 2 | – | – | 1.3 × 10−15 | 1.1 × 1040 |
(Using srcflux) | – | – | 1.13 × 10−15 | 9.5 × 1039 |
Plasma/APEC | 1.93 | – | 9.78 × 10−16 | 8.2 × 1039 |
Plasma/APEC | 4.85 | – | 1.42 × 10−15 | 1.2 × 1040 |
Plasma/APEC | 9.67 | – | 1.63 × 10−15 | 1.4 × 1040 |
Plasma/APEC | 1.53 | 1 × 1021 | 1 × 10−15 | 8.4 × 1039 |
Plasma/APEC | 1.53 | 5 × 1021 | 1.58 × 10−15 | 1.3 × 1040 |
Plasma/APEC | 1.53 | 1 × 1022 | 2.44 × 10−15 | 2.1 × 1040 |
Plasma/APEC | 1.53 | 2 × 1022 | 4.49 × 10−15 | 3.8 × 1040 |
Plasma/APEC | 3.06 | 1 × 1021 | 1.34 × 10−15 | 1.1 × 1040 |
Plasma/APEC | 3.06 | 5 × 1021 | 1.91 × 10−15 | 1.6 × 1040 |
Plasma/APEC | 3.06 | 1 × 1022 | 2.6 × 10−15 | 2.2 × 1040 |
Plasma/APEC | 3.06 | 2 × 1022 | 3.92 × 10−15 | 3.3 × 1040 |
Plasma/APEC | 4.85 | 1 × 1021 | 1.58 × 10−15 | 1.3 × 1040 |
Plasma/APEC | 4.85 | 5 × 1021 | 2.17 × 10−15 | 1.8 × 1040 |
Plasma/APEC | 4.85 | 1 × 1022 | 2.83 × 10−15 | 2.4 × 1040 |
Plasma/APEC | 4.85 | 2 × 1022 | 4.03 × 10−15 | 3.4 × 1040 |
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