|
|
|
While the behavoir of most simple models, i.e. how the spectral
energy distribution (SED) changes when you vary a model parameter,
is intuitively obvious, the same cannot be said about some of the
complicated models.
In order to visualize the behavior of some of models,
what I have done here is basically take the default parameter values when
the model is loaded by XSPEC/ISIS, pick a
parameter and vary it, keeping all other parameters constant. The simple
Gaussian lime emission model zgauss is included just to show the
effect of redshift on spectra.
|
agnjet:
|
(1) M_bh/M_Sun,
(2) Eddrat/L_Edd,
(3) Jetrat/L_Edd,
(4) pspec,
(5) z_sh/rg,
(6) r0/rg,
(7) outfac,
(8) hratio,
(9) visco [not varied],
(10) incl (deg),
(11) u_sh/c,
(12) Tin/Kelvin,
(13) eltemp/Kelvin,
(14) plfrac,
(15) bbsw,
(16) mxsw,
(17) D/kpc,
(18) dopsw,
(19) comsw,
(20) fsc,
(21) zfrac,
(22) zmax (log[cm]),
(23) equip,
(24) tbb2,
(25) bbf2,
(26) gamfac
|
|
eqpair:
|
(1) l_h/l_s,
(2) l_bb,
(3) kT_bb,
(4) l_nt/l_h,
(5) tau_p,
(6) radius,
(7) g_min,
(8) g_max,
(9) G_inj,
(10) pairinj,
(11) cosIncl,
(12) Refl,
(13) Fe_abund,
(14) Ab>He,
(15) T_disk,
(16) xi,
(17) Beta,
(18) Rin,
(19) Rout,
(20) redshift,
(21) norm
|
|
bmc:
|
(1) kT/keV,
(2) alpha,
(3) log(A),
(4) norm
|
|
compTT:
|
(1) redshift,
(2) T0/keV seed photon temp.,
(3) kT plasma temp.,
(4) tau_p plasma optical depth,
(5) approx,
(6) norm
|
|
kerrbb:
|
(1) eta,
(2) a,
(3) inclination,
(4) Mbh,
(5) Mdd,
(6) Dkpc,
(7) hd,
(8) self-irradiation flag,
(9) limb-darkening flag.
|
|
zgauss:
|
(1) LineE/keV,
(2) Sigma/keV,
(3) redshift,
(4) norm
|
|
zedge:
|
(1) edgeE/keV,
(2) MaxTau,
(3) Redshift
|
|
smedge:
|
(1) edgeE/keV,
(2) MaxTau,
(3) Smearing width
|
|
nrich:
|
(1) column,
(2) rlogxi,
(3) nabund,
(4) Redshift,
(5) norm
|
|
![(22) zmax (log[cm])](./models/agnjet/mov_par_22.gif){kind=link}
