![]() It's functions (like typed command history, scrollback, multiple window support, etc.) and solidly implemted emulations make it the preferred tool for people who have to access Unix shell accounts from a Windows platform. | convention.ZOC is a well known telnet/SSH/SSH2 client and terminal emulator. ![]() | (inclination, pi/2) in the reference frame. | Now, if inclination is given, the waveform is evaluated at The y-axis completes the right-handed triad. | an azimuthal angle phi_ref from the ve x-axis, in the orbital plane at | that the separation vector from the lighter BH to the heavier BH is at The orbital phase at the reference epoch is phi_ref. | The ve z-axis is along the orbital angular momentum at the reference | The reference frame (or inertial frame) is defined as follows: | The time-dependent inertial frame chiB with shape (L, 3) | The time-dependent inertial frame chiA with shape (L, 3) | The orbital phase in the coprecessing frame with length L. | The quaternion representing the coprecessing frame with | return_dynamics in precessing_opts is False (Default). | dynamics: A dict containing the frame dynamics and spin evolution. | code units: r*h/M extrapolated to future null-infinity. | If M and dist_mpc are given, the physical waveform | Else, h is a dictionary of available modes with (l, m) | Default: None, in which case all available modes are included. | mode_list : A list of (ell, m) modes tuples to be included. | Default: None, in which case all available modes wll be | indicies for each ell will be included automatically. | ellMax: Maximum ell index for modes to include. | M (cycles/M) if units = 'dimensionless', should be in | waveform, depending on whether the surrogate is a | Array of time/frequency samples at which to evaluate the | should be in seconds (Hertz) if units = 'mks'. | dt (df) Should be in M (cycles/M) if units = 'dimensionless', | used, which can be nonuniformly sampled. If None, the internal domain of the surrogate is | depending on whether the surrogate is a time/frequency domain | dt, df : Time/Frequency step size, specify at most one of dt/df, | such that the orbital frequency in the coprecessing frame | For time domain models, f_ref is used to determine a t_ref, | f_low is 0, this corresponds to the initial index. | Default: If f_ref is not given, we set f_ref = f_low. | Should be in cycles/M if units = 'dimensionless', should be | See below for definition of the reference frame. | reference frame is defined and the spins are specified. | f_ref: Frequency used to set the reference epoch at which the ![]() | very expensive evaluation for hybridized surrogates. | WARNING: Using f_low=0 with a small dt (like 0.1M) can lead to | Default: None, must be specified by user. | Should be in cycles/M if units = 'dimensionless', should be in | practice, this is estimated to be twice the initial orbital | f_low : Instantaneous initial frequency of the (2, 2) mode. | dist_mpc : Distance to binary system (MegaParsecs). | M, dist_mpc: Either specify both M and dist_mpc or neither. | momentum is constant and this is the same as the inertial | For nonprecessing models, the direction of orbital angular | the direction of the instantaneous orbital angular momentum. | arXiv:1110.2965, where the z-axis of this frame always tracks | The coprecessing frame is the minimal rotation frame of | chiB0: Dimensionless spin vector of the lighter black hole, given in | the coprecessing frame at reference epoch. | chiA0: Dimensionless spin vector of the heavier black hole, given in | _call_(self, q, chiA0, chiB0, M=None, dist_mpc=None, f_low=None, f_ref=None, dt=None, df=None, times=None, freqs=None, mode_list=None, ellMax=None, inclination=None, phi_ref=0, precessing_opts=None, tidal_opts=None, par_dict=None, units='dimensionless', skip_param_checks=False, taper_end_duration=None) | Methods inherited from SurrogateEvaluator: | In the _call_ method, x must have format x =. | See the _call_ method on how to evaluate waveforms. | in the above range and has been tested against existing NR waveforms in that | q \in and chi1z/chi2z \in, but produces reasonable waveforms | The surrogate has been trained in the range | BH, respectively, in the direction of orbital angular momentum. | where q is the mass ratio and chi1z/chi2z are the spins of the heavier/lighter | This model includes the following spin-weighted spherical harmonic modes: | have been hybridized using post-Newtonian (PN) and effective one body (EOB) This model was built using numerical relativity (NR) waveforms that | Evaluates gravitational waveforms generated by aligned-spin binary black hole | A class for the NRHybSur3dq8 surrogate model presented in Varma et al. Help on NRHybSur3dq8 in module gwsurrogate.surrogate object:
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