TbAbs

# Parameters
func_name = "TbAbs"
wide_energy_range = False
x_scale = "log"
y_scale = "log"
linear_range = False

Description

func.display()

• description: Photometric absorption (Tbabs implementation), f(E) = exp(- NH * sigma(E)) contributed by Dominique Eckert
• formula: $n.a.$
• parameters:
  • NH:
    • value: 1.0
    • desc: absorbing column density in units of 1e22 particles per cm^2
    • min_value: 0.0001
    • max_value: 10000.0
    • unit:
    • is_normalization: True
    • delta: 0.1
    • free: True
  • redshift:
    • value: 0.0
    • desc: the redshift of the source
    • min_value: 0.0
    • max_value: 15.0
    • unit:
    • is_normalization: False
    • delta: 0.1
    • free: False
  • abundance_table:
    • value: WILM
    • desc: the abundance table for the model
    • allowed values: ['WILM', 'AG89', 'ASPL']
    • defer: False
    • function: _init_xsect

Shape

The shape of the function.

If this is not a photon model but a prior or linear function then ignore the units as these docs are auto-generated

fig, ax = plt.subplots()


ax.plot(energy_grid, func(energy_grid), color=blue)

ax.set_xlabel("energy (keV)")
ax.set_ylabel("photon flux")
ax.set_xscale(x_scale)
ax.set_yscale(y_scale)

F\(_{\nu}\)

The F\(_{\nu}\) shape of the photon model if this is not a photon model, please ignore this auto-generated plot

fig, ax = plt.subplots()

ax.plot(energy_grid, energy_grid * func(energy_grid), red)


ax.set_xlabel("energy (keV)")
ax.set_ylabel(r"energy flux (F$_{\nu}$)")
ax.set_xscale(x_scale)
ax.set_yscale(y_scale)

\(\nu\)F\(_{\nu}\)

The \(\nu\)F\(_{\nu}\) shape of the photon model if this is not a photon model, please ignore this auto-generated plot

fig, ax = plt.subplots()

ax.plot(energy_grid, energy_grid**2 * func(energy_grid), color=green)


ax.set_xlabel("energy (keV)")
ax.set_ylabel(r"$\nu$F$_{\nu}$")
ax.set_xscale(x_scale)
ax.set_yscale(y_scale)