...
Energy | Flux | Flux_Err | ||
<ac:structured-macro ac:name="unmigrated-wiki-markup" ac:schema-version="1" ac:macro-id="2d34e570fb24c737-b341db82-44164312-a7ada95a-c87a377dfa8862665b6cc386"><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="23cfcd44b45794e8-3e48aa17-439a4540-b31fa20b-6476d3d005181bda44f6b2c9"><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="7d42aeb33a16ecfc-643c397e-4cc34193-bd899043-21d925611d8c3887d08a3edc"><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="0ef5d8b627cc7e08-efa3a249-463e48cc-821596d4-b0e8ba4be2189dffe0865fa5"><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 .