| INTEGRAL General Reference Catalog: Models |
|
Every source in the INTEGRAL Reference Catalog has a Spectral Energy Distribution (SED) model with parameters such as column density, photon index, and normalization. These models are used to determine instrumental counting rates. We use values from the literature when available. For example, sources from the ASCA catalog came with a model, parameters and a normalization. In other cases, we assign default models and parameters depending on the source type, and then offer a normalization. These values can be adjusted to reflect INTEGRAL observations that have been made public. The table below lists the default models and parameters for sources in the INTEGRAL Reference Catalog. Details of the models are given after the table. Click here to return to the Catalog page. |
| Source Type | SED Model |
NH ·1022 [cm−2] |
Γ1 |
Γ2 |
Ecut [keV] |
Efold [keV] |
Ebreak [keV] |
| X-ray Binaries | |||||||
| LMXB | wabs∗cutoff | 1.0 | 1.7 | − | 5 | − | − |
| LMXB with hardtail | wabs∗(cutoff + powerlaw) | 1.0 | 1.7 | 2.5 | 10 | − | − |
| HMXB | wabs∗highecut∗powerlaw | 1.0 | 1.0 | − | 10 | 15 | − |
| AGN | |||||||
| Seyfert I | wabs∗cutoff | 1.0 | 1.7 | − | 100 | − | − |
| Seyfert II | wabs∗cutoff | 10.0 | 1.7 | − | 100 | − | − |
| Blazar | wabs∗cutoff | 1.0 | 1.7 | − | 100 | − | − |
| Quasar | wabs∗cutoff | 1.0 | 1.7 | − | 100 | − | − |
| Radio Pulsars | |||||||
| Radio Pulsar | wabs∗powerlaw | 1.0 | 2.0 | − | − | − | − |
| Unidentified | |||||||
| X-band detection | wabs∗cutoff | 1.0 | 1.7 | − | 10 | − | − |
| COMPTEL detection | wabs∗bknpower | 100.0 | −1.5 | 2.1 | − | − | 1000 |
| EGRET detection | wabs∗bknpower | 100.0 | −1.5 | 2.1 | − | − | 10000 |
|
The equations governing the models used in the catalog are:
Eo : reference energy [keV] (1 keV in XSPEC) Ecut : exponential cutoff energy [keV] Efold : exponential folding energy [keV] Ebreak : break energy [keV] Γ1 : photon index for E < Ebreak Γ2 : photon index for E > Ebreak NH : column density of hydrogen [1022atoms·cm−2] S(E) : monochromatic flux at energy E [ph·cm−2·s−1] A = S(Eo) : normalization at 1 keV (Fobs / Fcomp) [ph·cm−2·s−1·keV−1] m(E) : multiplicative flux coefficient of S(E) at energy E σ(E) : photoelectric cross section (excluding Thompson scattering) In the HTML format, the model parameters column can be read as follows:
|