...
Energy | Flux | Flux_Err | ||
<ac:structured-macro ac:name="unmigrated-wiki-markup" ac:schema-version="1" ac:macro-id="4d25f003204b5310-b90100ff-4c9c4da7-80909cd2-3f1bf5b2b2c23c33404c5c53"><ac:plain-text-body><![CDATA[ | [MeV] | [ph/cm^2/s/MeV] | [ph/cm^2/s/MeV] | ]]></ac:plain-text-body></ac:structured-macro> |
133.4 | 3.5e-10 | 1.6e-10 | ||
237.1 | 4.8e-10 | 4.4e-11 | ||
421.7 | 1.3e-10 | 1.3e-11 | ||
749.9 | 1.2e-11 | 3.5e-12 | ||
1333.5 | <2.9e-12 |
| ||
2371.4 | 6.0e-13 | 2.5e-13 | ||
4217.0 | 1.4e-13 | 6.7e-14 | ||
7498.9 | <6.6e-14 |
| ||
13335.2 | 1.5e-14 | 8.4e-15 | ||
23713.7 | 3.4e-15 | 3.2e-15 | ||
42169.6 | <4.3e-15 |
| ||
74989.4 | <1.5e-15 |
|
...
Energy | Flux | Flux_error | ||
<ac:structured-macro ac:name="unmigrated-wiki-markup" ac:schema-version="1" ac:macro-id="72e2a6e7d9c29d54-c5933e42-43f3411e-b38dad23-70e3b4c1c4a74cd1eb19bc19"><ac:plain-text-body><![CDATA[ | [MeV] | [ph/cm^2/s/MeV] | [ph/cm^2/s/MeV] | ]]></ac:plain-text-body></ac:structured-macro> |
133.4 | <8.8e-12 |
| ||
237.1 | <4.3e-12 |
| ||
421.7 | <5.2e-12 |
| ||
749.9 | <5.6e-12 |
| ||
1333.5 | 1.8e-12 | 4.4e-13 | ||
2371.4 | 1.3e-12 | 1.6e-13 | ||
4217.0 | 4.4e-13 | 5.7e-14 | ||
7498.9 | 9.2e-14 | 1.8e-14 | ||
13335.2 | 3.1e-14 | 7.5e-15 | ||
23713.7 | 7.1e-15 | 3.7e-15 | ||
42169.6 | 2.5e-15 | 1.8e-15 | ||
74989.4 | 2.0e-16 | 3.3e-16 |
...
Energy | Flux | Flux_error | ||
<ac:structured-macro ac:name="unmigrated-wiki-markup" ac:schema-version="1" ac:macro-id="2292e1de6f4b5441-79ae6856-406e46a9-a1eb99c4-85d2ef030ef7ab6bcc8a3d89"><ac:plain-text-body><![CDATA[ | [MeV] | [ph/cm^2/s/MeV] | [ph/cm^2/s/MeV] | ]]></ac:plain-text-body></ac:structured-macro> |
133.4 | <3.1e-11 |
| ||
237.1 | 4.5e-10 | 4.1e-11 | ||
421.7 | 2.1e-10 | 1.2e-11 | ||
749.9 | 5.2e-11 | 3.4e-12 | ||
1333.5 | 1.6e-11 | 9.9e-13 | ||
2371.4 | 3.9e-12 | 2.9e-13 | ||
4217.0 | 1.2e-12 | 1.0e-13 | ||
7498.9 | 3.4e-13 | 3.7e-14 | ||
13335.2 | 4.9e-14 | 1.1e-14 | ||
23713.7 | 1.1e-14 | 4.2e-15 | ||
42169.6 | 4.4e-15 | 2.4e-15 | ||
74989.4 | <1.3e-15 |
|
...
In all of the previous SEDs the Bayesian method was used for the gtlike fitting algorithm. The next gtlike plot for W49B is done using the frequentist fitting algorithm for gtlike: 
Energy | Flux | Flux_error | ||
<ac:structured-macro ac:name="unmigrated-wiki-markup" ac:schema-version="1" ac:macro-id="af9ad16eec6c9b00-9c91d798-4ff44449-bbb5a5c0-1d290ccce57f55138aa965c7"><ac:plain-text-body><![CDATA[ | [MeV] | [ph/cm^2/s/MeV] | [ph/cm^2/s/MeV] | ]]></ac:plain-text-body></ac:structured-macro> |
133.4 | <1.4e-11 |
| ||
237.1 | 4.5e-10 | 4.1e-11 | ||
421.7 | 2.1e-10 | 1.2e-11 | ||
749.9 | 5.2e-11 | 3.4e-12 | ||
1333.5 | 1.6e-11 | 9.9e-13 | ||
2371.4 | 3.9e-12 | 2.9e-13 | ||
4217.0 | 1.2e-12 | 1.0e-13 | ||
7498.9 | 3.4e-13 | 3.7e-14 | ||
13335.2 | 4.9e-14 | 1.1e-14 | ||
23713.7 | 1.1e-14 | 4.2e-15 | ||
42169.6 | 4.4e-15 | 2.4e-15 | ||
74989.4 | <8.1e-16 |
|
...
10 August 2011
The discrepancy in upper limit calculations for flux between the Bayesian and Frequentist fitting algorithms appears to be described at this page .