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Table 7: Functions accepted by spf for the parameter SPF_MODEL

Function Description
PLAW(i,j) Simple power-law photon spectrum
BKNP(i,j,k,l) Broken power-law
HENC(i,j) High-energy cut-off (exponential)
BREM(i,j) Thermal bremsstrahlung spectrum
COMP(i,j) Comptonisation factor for bremsstrahlung
BBOD(i,j) Black-body spectrum
RSMT(i,j,k) Raymond-Smith emission spectrum
MEWE(i,j,k) Mewe & Gronenschild emission spectrum
ABSO(i) Photoelectric absorption by interstellar medium using
Morrison & McCammon cross-sections
ABSI(i) As ABSO, but redshifted
IRCO(i) Cold iron absorption (7.11 keV edge)
IRHE(i) He-like iron absorption (8.85 keV edge)
IRHY(i) H-like iron absorption (9.29 keV edge)
KEDG(i,j) K absorption edge
GTRA(i) Scattering by interstellar grains
GSCA(i) Complementary to GTRA
LINE(i,j) Narrow Gaussian line (intrinsic width < 0.1 keV).
BLIN(i,j,k) Broad Gaussian line
CFRA(i) Partial covering fraction absorption
UFRA(i) Complementary to CFRA
POLY(i,j,k,l) Polytropic gas distribution model
COMA(i,j,k) Hughes Coma/Polytropic model for on-axis Ginga
pointing
GABS(i,j) Absorption due to Gaussian distribution of absorbers
LABS(i) Absorption due to power-law distribution of absorbers
PABS(i,j) Absorption due to Poissonian distribution of clouds
PLEM(i,j,k) Power-law distribution of emission measures
TABn(i,j,n) Table model with n (equal to 0, 1 or 2) parameters

The variables i, j, etc. are described in the spf documentation.


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