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author | Aaron LI <aly@aaronly.me> | 2019-01-10 00:12:10 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2019-01-10 00:12:10 +0800 |
commit | b11592e71aa948170c5ac0be2ff70fbc3b2aeaf8 (patch) | |
tree | 8752cf05970100911f234394db4349b37be92c07 /fg21sim/extragalactic/clusters | |
parent | 9a5478446d5e28b64783efe9c8282f2eb27be1a5 (diff) | |
download | fg21sim-b11592e71aa948170c5ac0be2ff70fbc3b2aeaf8.tar.bz2 |
clusters/halo: Remove is_geniune()
The similar functionality will be implemented in another wrapper class.
Diffstat (limited to 'fg21sim/extragalactic/clusters')
-rw-r--r-- | fg21sim/extragalactic/clusters/halo.py | 32 |
1 files changed, 0 insertions, 32 deletions
diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py index 19a1575..8216b2d 100644 --- a/fg21sim/extragalactic/clusters/halo.py +++ b/fg21sim/extragalactic/clusters/halo.py @@ -473,38 +473,6 @@ class RadioHalo: return n_e - def is_genuine(self, n_e): - """ - Check whether the radio halo is genuine/observable by comparing the - radio flux density to the fiducial value, which is calculated from - the fiducial electron spectrum derived with turbulent acceleration - turned off. - - Parameters - ---------- - n_e : float 1D `~numpy.ndarray` - The finally derived electron spectrum. - Unit: [cm^-3] - - Returns - ------- - genuine : bool - Whether the radio halo is genuine? - factor : float - Acceleration factor of the flux. - """ - haloem = HaloEmission(gamma=self.gamma, n_e=n_e, - B=self.B_obs, radius=self.radius, - redshift=self.z_obs) - flux = haloem.calc_flux(self.fiducial_freq) - - ne_fiducial = self.calc_electron_spectrum(fiducial=True) - haloem.n_e = ne_fiducial - flux_fiducial = haloem.calc_flux(self.fiducial_freq) - - factor = flux / flux_fiducial - return (flux >= self.fiducial_factor, factor) - def fp_injection(self, gamma, t=None): """ Electron injection (rate) term for the Fokker-Planck equation. |