Commit message (Collapse) | Author | Age | Files | Lines | |
---|---|---|---|---|---|
* | clusters/halo: Add velocity_turb_base() method | Aaron LI | 2019-02-21 | 1 | -0/+5 |
| | | | | | | | | | | This method calculates the velocity dispersion of the base turbulence, i.e., the turbulence existing in a relaxed system without the merger injection. Add new configuration option 'extragalactic/halos/x_turb' to parameterize the energy fraction of the base turbulence w.r.t. the ICM thernal energy. | ||||
* | configs/spec: Adjust some min/max values for simplicity | Aaron LI | 2019-02-21 | 1 | -5/+5 |
| | |||||
* | clusters/halo: Further extend the halo radius calculation | Aaron LI | 2019-02-18 | 1 | -1/+5 |
| | |||||
* | clusters/main: Add 'genuine' property for halos | Aaron LI | 2019-01-30 | 1 | -0/+4 |
| | | | | Configuration option 'genuine_threshold' is added together. | ||||
* | clusters/halo: Add options bolo_freq_{min,max,num} | Aaron LI | 2019-01-29 | 1 | -0/+8 |
| | | | | Update the default bolometric frequency band to: 10 MHz -- 100 GHz. | ||||
* | configs/spec: Tweak gamma_max and gamma_np | Aaron LI | 2019-01-27 | 1 | -3/+3 |
| | |||||
* | clusters/halo: Rewrite is_genuine() to be calc_acc_factor() | Aaron LI | 2019-01-27 | 1 | -7/+0 |
| | | | | | | | Calculate the bolometric emissivity instead of the emissivity at a certain frequency. This should capture the acceleration effect more effectively. In addition, remove the now obsolete config options "fiducial_freq" and "fiducial_factor". | ||||
* | configs/spec: Various minor tweaks | Aaron LI | 2019-01-25 | 1 | -31/+32 |
| | |||||
* | clusters/halo: Account for mass scaling in tau_acceleration() | Aaron LI | 2019-01-25 | 1 | -0/+4 |
| | | | | Add configuration option "mass_index" to specify the scaling index. | ||||
* | clusters/halo: Fold parameter "zeta_ins" into "f_acc" | Aaron LI | 2019-01-25 | 1 | -7/+3 |
| | |||||
* | clusters: Assume equipartition between B field and CR | Aaron LI | 2019-01-25 | 1 | -13/+3 |
| | | | | | | Equipartition between the magnetic fields and cosmic rays is assumed, i.e., eta_b == x_cr. Therefore remove "extragalactic/clusters/eta_b" configuration option. | ||||
* | Minor tweaks | Aaron LI | 2019-01-18 | 1 | -3/+3 |
| | |||||
* | clusters/halo: Apply option 'f_radius' to derive halo radius | Aaron LI | 2018-11-08 | 1 | -4/+3 |
| | | | | The config option 'f_radius' is renamed from the old 'f_lturb'. | ||||
* | clusters/halo: Add and use 'f_rc' and 'beta' options | Aaron LI | 2018-11-08 | 1 | -0/+7 |
| | |||||
* | clusters/halo: Support to check whether halo is genuine | Aaron LI | 2018-11-01 | 1 | -0/+7 |
| | | | | | | | Add the 'is_genuine()' method to check whether the radio halo is genuine by comparing the flux density to the fiducial value. Two new configuration options (fiducial_freq and fiducial_factor) are added to specify the frequency and limit whether the radio halo is regarded as genuine. | ||||
* | clusters/halo: Update calculations of injection and halo radius | Aaron LI | 2018-10-30 | 1 | -5/+4 |
| | |||||
* | Deprecate the pointsource component (2) | Aaron LI | 2018-10-30 | 1 | -49/+0 |
| | |||||
* | configs: Merge config specs into one single file | Aaron LI | 2018-10-30 | 1 | -0/+492 |