# Source code for brainbox.metrics.single_units

```
"""
Computes metrics for assessing quality of single units.
Run the following to set-up the workspace to run the docstring examples:
>>> import brainbox as bb
>>> import alf.io as aio
>>> import numpy as np
>>> import matplotlib.pyplot as plt
>>> import ibllib.ephys.spikes as e_spks
# (*Note, if there is no 'alf' directory, make 'alf' directory from 'ks2' output directory):
>>> e_spks.ks2_to_alf(path_to_ks_out, path_to_alf_out)
# Load the alf spikes bunch and clusters bunch, and get a units bunch.
>>> spks_b = aio.load_object(path_to_alf_out, 'spikes')
>>> clstrs_b = aio.load_object(path_to_alf_out, 'clusters')
>>> units_b = bb.processing.get_units_bunch(spks_b) # may take a few mins to compute
"""
import time
import logging
import numpy as np
import scipy.ndimage.filters as filters
import scipy.stats as stats
import pandas as pd
from ibllib.io import spikeglx
from phylib.stats import correlograms
from iblutil.util import Bunch
from iblutil.numerical import ismember, between_sorted
from brainbox import singlecell
from brainbox.io.spikeglx import extract_waveforms
from brainbox.processing import bincount2D
from brainbox.metrics import electrode_drift
_logger = logging.getLogger('ibllib')
# Parameters to be used in `quick_unit_metrics`
METRICS_PARAMS = {
'acceptable_contamination': 0.1,
'bin_size': 0.25,
'med_amp_thresh_uv': 50,
'min_isi': 0.0001,
'min_num_bins_for_missed_spks_est': 50,
'nc_bins': 100,
'nc_n_low_bins': 2,
'nc_quartile_length': 0.2,
'nc_thresh': 20,
'presence_window': 10,
'refractory_period': 0.0015,
'RPslide_thresh': 0.1,
'spks_per_bin_for_missed_spks_est': 10,
'std_smoothing_kernel_for_missed_spks_est': 4,
}
[docs]def unit_stability(units_b, units=None, feat_names=['amps'], dist='norm', test='ks'):
"""
Computes the probability that the empirical spike feature distribution(s), for specified
feature(s), for all units, comes from a specific theoretical distribution, based on a specified
statistical test. Also computes the coefficients of variation of the spike feature(s) for all
units.
Parameters
----------
units_b : bunch
A units bunch containing fields with spike information (e.g. cluster IDs, times, features,
etc.) for all units.
units : array-like (optional)
A subset of all units for which to create the bar plot. (If `None`, all units are used)
feat_names : list of strings (optional)
A list of names of spike features that can be found in `spks` to specify which features to
use for calculating unit stability.
dist : string (optional)
The type of hypothetical null distribution for which the empirical spike feature
distributions are presumed to belong to.
test : string (optional)
The statistical test used to compute the probability that the empirical spike feature
distributions come from `dist`.
Returns
-------
p_vals_b : bunch
A bunch with `feat_names` as keys, containing a ndarray with p-values (the probabilities
that the empirical spike feature distribution for each unit comes from `dist` based on
`test`) for each unit for all `feat_names`.
cv_b : bunch
A bunch with `feat_names` as keys, containing a ndarray with the coefficients of variation
of each unit's empirical spike feature distribution for all features.
See Also
--------
plot.feat_vars
Examples
--------
1) Compute 1) the p-values obtained from running a one-sample ks test on the spike amplitudes
for each unit, and 2) the variances of the empirical spike amplitudes distribution for each
unit. Create a histogram of the variances of the spike amplitudes for each unit, color-coded by
depth of channel of max amplitudes. Get cluster IDs of those units which have variances greater
than 50.
>>> p_vals_b, variances_b = bb.metrics.unit_stability(units_b)
# Plot histograms of variances color-coded by depth of channel of max amplitudes
>>> fig = bb.plot.feat_vars(units_b, feat_name='amps')
# Get all unit IDs which have amps variance > 50
>>> var_vals = np.array(tuple(variances_b['amps'].values()))
>>> bad_units = np.where(var_vals > 50)
"""
# Get units.
if not (units is None): # we're using a subset of all units
unit_list = list(units_b[feat_names[0]].keys())
# for each `feat` and unit in `unit_list`, remove unit from `units_b` if not in `units`
for feat in feat_names:
[units_b[feat].pop(unit) for unit in unit_list if not (int(unit) in units)]
unit_list = list(units_b[feat_names[0]].keys()) # get new `unit_list` after removing units
# Initialize `p_vals` and `variances`.
p_vals_b = Bunch()
cv_b = Bunch()
# Set the test as a lambda function (in future, more tests can be added to this dict)
tests = \
{
'ks': lambda x, y: stats.kstest(x, y)
}
test_fun = tests[test]
# Compute the statistical tests and variances. For each feature, iteratively get each unit's
# p-values and variances, and add them as keys to the respective bunches `p_vals_feat` and
# `variances_feat`. After iterating through all units, add these bunches as keys to their
# respective parent bunches, `p_vals` and `variances`.
for feat in feat_names:
p_vals_feat = Bunch((unit, 0) for unit in unit_list)
cv_feat = Bunch((unit, 0) for unit in unit_list)
for unit in unit_list:
# If we're missing units/features, create a NaN placeholder and skip them:
if len(units_b['times'][str(unit)]) == 0:
p_val = np.nan
cv = np.nan
else:
# compute p_val and var for current feature
_, p_val = test_fun(units_b[feat][unit], dist)
cv = np.var(units_b[feat][unit]) / np.mean(units_b[feat][unit])
# Append current unit's values to list of units' values for current feature:
p_vals_feat[str(unit)] = p_val
cv_feat[str(unit)] = cv
p_vals_b[feat] = p_vals_feat
cv_b[feat] = cv_feat
return p_vals_b, cv_b
[docs]def missed_spikes_est(feat, spks_per_bin=20, sigma=5, min_num_bins=50):
"""
Computes the approximate fraction of spikes missing from a spike feature distribution for a
given unit, assuming the distribution is symmetric.
Inspired by metric described in Hill et al. (2011) J Neurosci 31: 8699-8705.
Parameters
----------
feat : ndarray
The spikes' feature values (e.g. amplitudes)
spks_per_bin : int (optional)
The number of spikes per bin from which to compute the spike feature histogram.
sigma : int (optional)
The standard deviation for the gaussian kernel used to compute the pdf from the spike
feature histogram.
min_num_bins : int (optional)
The minimum number of bins used to compute the spike feature histogram.
Returns
-------
fraction_missing : float
The fraction of missing spikes (0-0.5). *Note: If more than 50% of spikes are missing, an
accurate estimate isn't possible.
pdf : ndarray
The computed pdf of the spike feature histogram.
cutoff_idx : int
The index for `pdf` at which point `pdf` is no longer symmetrical around the peak. (This
is returned for plotting purposes).
See Also
--------
plot.feat_cutoff
Examples
--------
1) Determine the fraction of spikes missing from unit 1 based on the recorded unit's spike
amplitudes, assuming the distribution of the unit's spike amplitudes is symmetric.
# Get unit 1 amplitudes from a unit bunch, and compute fraction spikes missing.
>>> feat = units_b['amps']['1']
>>> fraction_missing = bb.plot.feat_cutoff(feat)
"""
# Ensure minimum number of spikes requirement is met, return Nan otherwise
if feat.size <= (spks_per_bin * min_num_bins):
return np.nan, None, None
# compute the spike feature histogram and pdf:
num_bins = int(feat.size / spks_per_bin)
hist, bins = np.histogram(feat, num_bins, density=True)
pdf = filters.gaussian_filter1d(hist, sigma)
# Find where the distribution stops being symmetric around the peak:
peak_idx = np.argmax(pdf)
max_idx_sym_around_peak = np.argmin(np.abs(pdf[peak_idx:] - pdf[0]))
cutoff_idx = peak_idx + max_idx_sym_around_peak
# compute fraction missing from the tail of the pdf (the area where pdf stops being
# symmetric around peak).
fraction_missing = np.sum(pdf[cutoff_idx:]) / np.sum(pdf)
fraction_missing = 0.5 if (fraction_missing > 0.5) else fraction_missing
return fraction_missing, pdf, cutoff_idx
[docs]def wf_similarity(wf1, wf2):
"""
Computes a unit normalized spatiotemporal similarity score between two sets of waveforms.
This score is based on how waveform shape correlates for each pair of spikes between the
two sets of waveforms across space and time. The shapes of the arrays of the two sets of
waveforms must be equal.
Parameters
----------
wf1 : ndarray
An array of shape (#spikes, #samples, #channels).
wf2 : ndarray
An array of shape (#spikes, #samples, #channels).
Returns
-------
s: float
The unit normalized spatiotemporal similarity score.
See Also
--------
io.extract_waveforms
plot.single_unit_wf_comp
Examples
--------
1) Compute the similarity between the first and last 100 waveforms for unit1, across the 20
channels around the channel of max amplitude.
# Get the channels around the max amp channel for the unit, two sets of timestamps for the
# unit, and the two corresponding sets of waveforms for those two sets of timestamps.
# Then compute `s`.
>>> max_ch = clstrs_b['channels'][1]
>>> if max_ch < 10: # take only channels greater than `max_ch`.
>>> ch = np.arange(max_ch, max_ch + 20)
>>> elif (max_ch + 10) > 385: # take only channels less than `max_ch`.
>>> ch = np.arange(max_ch - 20, max_ch)
>>> else: # take `n_c_ch` around `max_ch`.
>>> ch = np.arange(max_ch - 10, max_ch + 10)
>>> ts1 = units_b['times']['1'][:100]
>>> ts2 = units_b['times']['1'][-100:]
>>> wf1 = bb.io.extract_waveforms(path_to_ephys_file, ts1, ch)
>>> wf2 = bb.io.extract_waveforms(path_to_ephys_file, ts2, ch)
>>> s = bb.metrics.wf_similarity(wf1, wf2)
TODO check `s` calculation:
take median of waveforms
xcorr all waveforms with median, and divide by autocorr of all waveforms
profile
for two sets of units: xcorr(cl1, cl2) / (sqrt autocorr(cl1) * autocorr(cl2))
"""
# Remove warning for dividing by 0 when calculating `s` (this is resolved by using
# `np.nan_to_num`)
import warnings
warnings.filterwarnings('ignore', r'invalid value encountered in true_divide')
assert wf1.shape == wf2.shape, ('The shapes of the sets of waveforms are inconsistent ({})'
'({})'.format(wf1.shape, wf2.shape))
# Get number of spikes, samples, and channels of waveforms.
n_spks = wf1.shape[0]
n_samples = wf1.shape[1]
n_ch = wf1.shape[2]
# Create a matrix that will hold the similarity values of each spike in `wf1` to `wf2`.
# Iterate over both sets of spikes, computing `s` for each pair.
similarity_matrix = np.zeros((n_spks, n_spks))
for spk1 in range(n_spks):
for spk2 in range(n_spks):
s_spk = \
np.sum(np.nan_to_num(
wf1[spk1, :, :] * wf2[spk2, :, :] /
np.sqrt(wf1[spk1, :, :] ** 2 * wf2[spk2, :, :] ** 2))) / (n_samples * n_ch)
similarity_matrix[spk1, spk2] = s_spk
# Return mean of similarity matrix
s = np.mean(similarity_matrix)
return s
[docs]def firing_rate_coeff_var(ts, hist_win=0.01, fr_win=0.5, n_bins=10):
'''
Computes the coefficient of variation of the firing rate: the ratio of the standard
deviation to the mean.
Parameters
----------
ts : ndarray
The spike timestamps from which to compute the firing rate.
hist_win : float (optional)
The time window (in s) to use for computing spike counts.
fr_win : float (optional)
The time window (in s) to use as a moving slider to compute the instantaneous firing rate.
n_bins : int (optional)
The number of bins in which to compute a coefficient of variation of the firing rate.
Returns
-------
cv : float
The mean coefficient of variation of the firing rate of the `n_bins` number of coefficients
computed.
cvs : ndarray
The coefficients of variation of the firing for each bin of `n_bins`.
fr : ndarray
The instantaneous firing rate over time (in hz).
See Also
--------
singlecell.firing_rate
plot.firing_rate
Examples
--------
1) Compute the coefficient of variation of the firing rate for unit 1 from the time of its
first to last spike, and compute the coefficient of variation of the firing rate for unit 2
from the first to second minute.
>>> ts_1 = units_b['times']['1']
>>> ts_2 = units_b['times']['2']
>>> ts_2 = np.intersect1d(np.where(ts_2 > 60)[0], np.where(ts_2 < 120)[0])
>>> cv, cvs, fr = bb.metrics.firing_rate_coeff_var(ts_1)
>>> cv_2, cvs_2, fr_2 = bb.metrics.firing_rate_coeff_var(ts_2)
'''
# Compute overall instantaneous firing rate and firing rate for each bin.
fr = singlecell.firing_rate(ts, hist_win=hist_win, fr_win=fr_win)
bin_sz = int(fr.size / n_bins)
fr_binned = np.array([fr[(b * bin_sz):(b * bin_sz + bin_sz)] for b in range(n_bins)])
# Compute coefficient of variations of firing rate for each bin, and the mean c.v.
cvs = np.std(fr_binned, axis=1) / np.mean(fr_binned, axis=1)
# NaNs from zero spikes are turned into 0's
# cvs[np.isnan(cvs)] = 0 nan's can happen if neuron doesn't spike in a bin
cv = np.mean(cvs)
return cv, cvs, fr
[docs]def firing_rate_fano_factor(ts, hist_win=0.01, fr_win=0.5, n_bins=10):
'''
Computes the fano factor of the firing rate: the ratio of the variance to the mean.
(Almost identical to coeff. of variation)
Parameters
----------
ts : ndarray
The spike timestamps from which to compute the firing rate.
hist_win : float
The time window (in s) to use for computing spike counts.
fr_win : float
The time window (in s) to use as a moving slider to compute the instantaneous firing rate.
n_bins : int (optional)
The number of bins in which to compute a fano factor of the firing rate.
Returns
-------
ff : float
The mean fano factor of the firing rate of the `n_bins` number of factors
computed.
ffs : ndarray
The fano factors of the firing for each bin of `n_bins`.
fr : ndarray
The instantaneous firing rate over time (in hz).
See Also
--------
singlecell.firing_rate
plot.firing_rate
Examples
--------
1) Compute the fano factor of the firing rate for unit 1 from the time of its
first to last spike, and compute the fano factor of the firing rate for unit 2
from the first to second minute.
>>> ts_1 = units_b['times']['1']
>>> ts_2 = units_b['times']['2']
>>> ts_2 = np.intersect1d(np.where(ts_2 > 60)[0], np.where(ts_2 < 120)[0])
>>> ff, ffs, fr = bb.metrics.firing_rate_fano_factor(ts_1)
>>> ff_2, ffs_2, fr_2 = bb.metrics.firing_rate_fano_factor(ts_2)
'''
# Compute overall instantaneous firing rate and firing rate for each bin.
fr = singlecell.firing_rate(ts, hist_win=hist_win, fr_win=fr_win)
# this procedure can cut off data at the end, up to n_bins last timesteps
bin_sz = int(fr.size / n_bins)
fr_binned = np.array([fr[(b * bin_sz):(b * bin_sz + bin_sz)] for b in range(n_bins)])
# Compute fano factor of firing rate for each bin, and the mean fano factor
ffs = np.var(fr_binned, axis=1) / np.mean(fr_binned, axis=1)
# ffs[np.isnan(ffs)] = 0 nan's can happen if neuron doesn't spike in a bin
ff = np.mean(ffs)
return ff, ffs, fr
[docs]def average_drift(feat, times):
"""
Computes the cumulative drift (normalized by the total number of spikes) of a spike feature
array.
Parameters
----------
feat : ndarray
The spike feature values from which to compute the maximum drift.
Usually amplitudes
Returns
-------
cd : float
The cumulative drift of the unit.
See Also
--------
max_drift
Examples
--------
1) Get the cumulative depth drift for unit 1.
>>> unit_idxs = np.where(spks_b['clusters'] == 1)[0]
>>> depths = spks_b['depths'][unit_idxs]
>>> amps = spks_b['amps'][unit_idxs]
>>> depth_cd = bb.metrics.cum_drift(depths)
>>> amp_cd = bb.metrics.cum_drift(amps)
"""
cd = np.sum(np.abs(np.diff(feat) / np.diff(times))) / len(feat)
return cd
[docs]def pres_ratio(ts, hist_win=10):
"""
Computes the presence ratio of spike counts: the number of bins where there is at least one
spike, over the total number of bins, given a specified bin width.
Parameters
----------
ts : ndarray
The spike timestamps from which to compute the presence ratio.
hist_win : float (optional)
The time window (in s) to use for computing the presence ratio.
Returns
-------
pr : float
The presence ratio.
spks_bins : ndarray
The number of spks in each bin.
See Also
--------
plot.pres_ratio
Examples
--------
1) Compute the presence ratio for unit 1, given a window of 10 s.
>>> ts = units_b['times']['1']
>>> pr, pr_bins = bb.metrics.pres_ratio(ts)
"""
bins = np.arange(0, ts[-1] + hist_win, hist_win)
spks_bins, _ = np.histogram(ts, bins)
pr = len(np.where(spks_bins)[0]) / len(spks_bins)
return pr, spks_bins
[docs]def ptp_over_noise(ephys_file, ts, ch, t=2.0, sr=30000, n_ch_probe=385, car=True):
"""
For specified channels, for specified timestamps, computes the mean (peak-to-peak amplitudes /
the MADs of the background noise).
Parameters
----------
ephys_file : string
The file path to the binary ephys data.
ts : ndarray_like
The timestamps (in s) of the spikes.
ch : ndarray_like
The channels on which to extract the waveforms.
t : numeric (optional)
The time (in ms) of the waveforms to extract to compute the ptp.
sr : int (optional)
The sampling rate (in hz) that the ephys data was acquired at.
n_ch_probe : int (optional)
The number of channels of the recording.
car: bool (optional)
A flag to perform common-average-referencing before extracting waveforms.
Returns
-------
ptp_sigma : ndarray
An array containing the mean ptp_over_noise values for the specified `ts` and `ch`.
Examples
--------
1) Compute ptp_over_noise for all spikes on 20 channels around the channel of max amplitude
for unit 1.
>>> ts = units_b['times']['1']
>>> max_ch = max_ch = clstrs_b['channels'][1]
>>> if max_ch < 10: # take only channels greater than `max_ch`.
>>> ch = np.arange(max_ch, max_ch + 20)
>>> elif (max_ch + 10) > 385: # take only channels less than `max_ch`.
>>> ch = np.arange(max_ch - 20, max_ch)
>>> else: # take `n_c_ch` around `max_ch`.
>>> ch = np.arange(max_ch - 10, max_ch + 10)
>>> p = bb.metrics.ptp_over_noise(ephys_file, ts, ch)
"""
# Ensure `ch` is ndarray
ch = np.asarray(ch)
ch = ch.reshape((ch.size, 1)) if ch.size == 1 else ch
# Get waveforms.
wf = extract_waveforms(ephys_file, ts, ch, t=t, sr=sr, n_ch_probe=n_ch_probe, car=car)
# Initialize `mean_ptp` based on `ch`, and compute mean ptp of all spikes for each ch.
mean_ptp = np.zeros((ch.size,))
for cur_ch in range(ch.size, ):
mean_ptp[cur_ch] = np.mean(np.max(wf[:, :, cur_ch], axis=1) -
np.min(wf[:, :, cur_ch], axis=1))
# Compute MAD for `ch` in chunks.
with spikeglx.Reader(ephys_file) as s_reader:
file_m = s_reader.data # the memmapped array
n_chunk_samples = 5e6 # number of samples per chunk
n_chunks = np.ceil(file_m.shape[0] / n_chunk_samples).astype('int')
# Get samples that make up each chunk. e.g. `chunk_sample[1] - chunk_sample[0]` are the
# samples that make up the first chunk.
chunk_sample = np.arange(0, file_m.shape[0], n_chunk_samples, dtype=int)
chunk_sample = np.append(chunk_sample, file_m.shape[0])
# Give time estimate for computing MAD.
t0 = time.perf_counter()
stats.median_absolute_deviation(file_m[chunk_sample[0]:chunk_sample[1], ch], axis=0)
dt = time.perf_counter() - t0
print('Performing MAD computation. Estimated time is {:.2f} mins.'
' ({})'.format(dt * n_chunks / 60, time.ctime()))
# Compute MAD for each chunk, then take the median MAD of all chunks.
mad_chunks = np.zeros((n_chunks, ch.size), dtype=np.int16)
for chunk in range(n_chunks):
mad_chunks[chunk, :] = stats.median_absolute_deviation(
file_m[chunk_sample[chunk]:chunk_sample[chunk + 1], ch], axis=0, scale=1)
print('Done. ({})'.format(time.ctime()))
# Return `mean_ptp` over `mad`
mad = np.median(mad_chunks, axis=0)
ptp_sigma = mean_ptp / mad
return ptp_sigma
[docs]def contamination_alt(ts, rp=0.002):
"""
An estimate of the contamination of the unit (i.e. a pseudo false positive measure) based on
the number of spikes, number of isi violations, and time between the first and last spike.
(see Hill et al. (2011) J Neurosci 31: 8699-8705).
Parameters
----------
ts : ndarray_like
The timestamps (in s) of the spikes.
rp : float (optional)
The refractory period (in s).
Returns
-------
ce : float
An estimate of the fraction of contamination.
See Also
--------
contamination_alt
Examples
--------
1) Compute contamination estimate for unit 1.
>>> ts = units_b['times']['1']
>>> ce = bb.metrics.contamination(ts)
"""
# Get number of spikes, number of isi violations, and time from first to final spike.
n_spks = ts.size
n_isi_viol = np.size(np.where(np.diff(ts) < rp)[0])
t = ts[-1] - ts[0]
# `ce` is min of roots of solved quadratic equation.
c = (t * n_isi_viol) / (2 * rp * n_spks ** 2) # 3rd term in quadratic
ce = np.min(np.abs(np.roots([-1, 1, c]))) # solve quadratic
return ce
[docs]def contamination(ts, min_time, max_time, rp=0.002, min_isi=0.0001):
"""
An estimate of the contamination of the unit (i.e. a pseudo false positive measure) based on
the number of spikes, number of isi violations, and time between the first and last spike.
(see Hill et al. (2011) J Neurosci 31: 8699-8705).
Modified by Dan Denman from cortex-lab/sortingQuality GitHub by Nick Steinmetz.
Parameters
----------
ts : ndarray_like
The timestamps (in s) of the spikes.
min_time : float
The minimum time (in s) that a potential spike occurred.
max_time : float
The maximum time (in s) that a potential spike occurred.
rp : float (optional)
The refractory period (in s).
min_isi : float (optional)
The minimum interspike-interval (in s) for counting duplicate spikes.
Returns
-------
ce : float
An estimate of the contamination.
A perfect unit has a ce = 0
A unit with some contamination has a ce < 0.5
A unit with lots of contamination has a ce > 1.0
num_violations : int
The total number of isi violations.
See Also
--------
contamination
Examples
--------
1) Compute contamination estimate for unit 1, with a minimum isi for counting duplicate
spikes of 0.1 ms.
>>> ts = units_b['times']['1']
>>> ce = bb.metrics.contamination_alt(ts, min_isi=0.0001)
"""
duplicate_spikes = np.where(np.diff(ts) <= min_isi)[0]
ts = np.delete(ts, duplicate_spikes + 1)
isis = np.diff(ts)
num_spikes = ts.size
num_violations = np.sum(isis < rp)
violation_time = 2 * num_spikes * (rp - min_isi)
total_rate = ts.size / (max_time - min_time)
violation_rate = num_violations / violation_time
ce = violation_rate / total_rate
return ce, num_violations
def _max_acceptable_cont(FR, RP, rec_duration, acceptableCont, thresh):
"""
Function to compute the maximum acceptable refractory period contamination
called during slidingRP_viol
"""
time_for_viol = RP * 2 * FR * rec_duration
expected_count_for_acceptable_limit = acceptableCont * time_for_viol
max_acceptable = stats.poisson.ppf(thresh, expected_count_for_acceptable_limit)
if max_acceptable == 0 and stats.poisson.pmf(0, expected_count_for_acceptable_limit) > 0:
max_acceptable = -1
return max_acceptable
[docs]def slidingRP_viol(ts, bin_size=0.25, thresh=0.1, acceptThresh=0.1):
"""
A binary metric which determines whether there is an acceptable level of
refractory period violations by using a sliding refractory period:
This takes into account the firing rate of the neuron and computes a
maximum acceptable level of contamination at different possible values of
the refractory period. If the unit has less than the maximum contamination
at any of the possible values of the refractory period, the unit passes.
A neuron will always fail this metric for very low firing rates, and thus
this metric takes into account both firing rate and refractory period
violations.
Parameters
----------
ts : ndarray_like
The timestamps (in s) of the spikes.
bin_size : float
The size of binning for the autocorrelogram.
thresh : float
Spike rate used to generate poisson distribution (to compute maximum
acceptable contamination, see _max_acceptable_cont)
acceptThresh : float
The fraction of contamination we are willing to accept (default value
set to 0.1, or 10% contamination)
Returns
-------
didpass : int
0 if unit didn't pass
1 if unit did pass
See Also
--------
contamination
Examples
--------
1) Compute whether a unit has too much refractory period contamination at
any possible value of a refractory period, for a 0.25 ms bin, with a
threshold of 10% acceptable contamination
>>> ts = units_b['times']['1']
>>> didpass = bb.metrics.slidingRP_viol(ts, bin_size=0.25, thresh=0.1,
acceptThresh=0.1)
"""
b = np.arange(0, 10.25, bin_size) / 1000 + 1e-6 # bins in seconds
bTestIdx = [5, 6, 7, 8, 10, 12, 14, 16, 18, 20, 24, 28, 32, 36, 40]
bTest = [b[i] for i in bTestIdx]
if len(ts) > 0 and ts[-1] > ts[0]: # only do this for units with samples
recDur = (ts[-1] - ts[0])
# compute acg
c0 = correlograms(ts, np.zeros(len(ts), dtype='int8'), cluster_ids=[0],
bin_size=bin_size / 1000, sample_rate=20000,
window_size=2,
symmetrize=False)
# cumulative sum of acg, i.e. number of total spikes occuring from 0
# to end of that bin
cumsumc0 = np.cumsum(c0[0, 0, :])
# cumulative sum at each of the testing bins
res = cumsumc0[bTestIdx]
total_spike_count = len(ts)
# divide each bin's count by the total spike count and the bin size
bin_count_normalized = c0[0, 0] / total_spike_count / bin_size * 1000
num_bins_2s = len(c0[0, 0]) # number of total bins that equal 2 secs
num_bins_1s = int(num_bins_2s / 2) # number of bins that equal 1 sec
# compute fr based on the mean of bin_count_normalized from 1 to 2 s
# instead of as before (len(ts)/recDur) for a better estimate
fr = np.sum(bin_count_normalized[num_bins_1s:num_bins_2s]) / num_bins_1s
mfunc = np.vectorize(_max_acceptable_cont)
# compute the maximum allowed number of spikes per testing bin
m = mfunc(fr, bTest, recDur, fr * acceptThresh, thresh)
# did the unit pass (resulting number of spikes less than maximum
# allowed spikes) at any of the testing bins?
didpass = int(np.any(np.less_equal(res, m)))
else:
didpass = 0
return didpass
[docs]def noise_cutoff(amps, quartile_length=.2, n_bins=100, n_low_bins=2):
"""
A metric to determine whether a unit's amplitude distribution is cut off
(at floor), without assuming a Gaussian distribution.
This metric takes the amplitude distribution, computes the mean and std
of an upper quartile of the distribution, and determines how many standard
deviations away from that mean a lower quartile lies.
Parameters
----------
amps : ndarray_like
The amplitudes (in uV) of the spikes.
quartile_length : float
The size of the upper quartile of the amplitude distribution.
n_bins : int
The number of bins used to compute a histogram of the amplitude
distribution.
n_low_bins : int
The number of bins used in the lower part of the distribution (where
cutoff is determined).
Returns
-------
cutoff : float
Number of standard deviations that the lower mean is outside of the
mean of the upper quartile.
See Also
--------
missed_spikes_est
Examples
--------
1) Compute whether a unit's amplitude distribution is cut off
>>> amps = spks_b['amps'][unit_idxs]
>>> cutoff = bb.metrics.noise_cutoff(amps, quartile_length=.2,
n_bins=100, n_low_bins=2)
"""
if amps.size > 1:
bins_list = np.linspace(0, np.max(amps), n_bins)
n, bins = np.histogram(amps, bins=bins_list)
dx = np.diff(n)
idx_nz = np.nonzero(dx) # indices of nonzeros
idx_peak = np.argmax(n)
length_top_half = idx_nz[0][-1] - idx_peak
high_quartile = 1 - (2 * quartile_length)
high_quartile_start_ind = int(np.ceil(high_quartile * length_top_half + idx_peak))
xx = idx_nz[0][idx_nz[0] > high_quartile_start_ind]
if len(n[xx]) > 0:
mean_high_quartile = np.mean(n[xx])
std_high_quartile = np.std(n[xx])
first_low_quartile = np.mean(n[idx_nz[0][1:n_low_bins]])
if std_high_quartile > 0:
cutoff = (first_low_quartile - mean_high_quartile) / std_high_quartile
else:
cutoff = np.float64(np.nan)
else:
cutoff = np.float64(np.nan)
else:
cutoff = np.float64(np.nan)
return cutoff
[docs]def spike_sorting_metrics(times, clusters, amps, depths, cluster_ids=None, params=METRICS_PARAMS):
"""
Computes:
- cell level metrics (cf quick_unit_metrics)
- label the metrics according to quality thresholds
- estimates drift as a function of time
:param times: vector of spike times
:param clusters:
:param amplitudes:
:param depths:
:param cluster_ids (optional): set of clusters (if None the output datgrame will match
the unique set of clusters represented in spike clusters)
:param params: dict (optional) parameters for qc computation (
see constant at the top of the module for default values and keys)
:return: data_frame of metrics (cluster records, columns are qc attributes)|
:return: dictionary of recording qc (keys 'time_scale' and 'drift_um')
"""
# compute metrics and convert to `DataFrame`
df_units = quick_unit_metrics(
clusters, times, amps, depths, cluster_ids=cluster_ids, params=params)
df_units = pd.DataFrame(df_units)
# compute drift as a function of time and put in a dictionary
drift, ts = electrode_drift.estimate_drift(times, amps, depths)
rec_qc = {'time_scale': ts, 'drift_um': drift}
return df_units, rec_qc
[docs]def quick_unit_metrics(spike_clusters, spike_times, spike_amps, spike_depths,
params=METRICS_PARAMS, cluster_ids=None, tbounds=None):
"""
Computes single unit metrics from only the spike times, amplitudes, and
depths for a set of units.
Metrics computed:
'amp_max',
'amp_min',
'amp_median',
'amp_std_dB',
'contamination',
'contamination_alt',
'drift',
'missed_spikes_est',
'noise_cutoff',
'presence_ratio',
'presence_ratio_std',
'slidingRP_viol',
'spike_count'
Parameters (see the METRICS_PARAMS constant)
----------
spike_clusters : ndarray_like
A vector of the unit ids for a set of spikes.
spike_times : ndarray_like
A vector of the timestamps for a set of spikes.
spike_amps : ndarray_like
A vector of the amplitudes for a set of spikes.
spike_depths : ndarray_like
A vector of the depths for a set of spikes.
clusters_id: (optional) lists of cluster ids. If not all clusters are represented in the
spikes_clusters (ie. cluster has no spike), this will ensure the output size is consistent
with the input arrays.
tbounds: (optional) list or 2 elements array containing a time-selection to perform the
metrics computation on.
params : dict (optional)
Parameters used for computing some of the metrics in the function:
'presence_window': float
The time window (in s) used to look for spikes when computing the presence ratio.
'refractory_period': float
The refractory period used when computing isi violations and the contamination
estimate.
'min_isi': float
The minimum interspike-interval (in s) for counting duplicate spikes when computing
the contamination estimate.
'spks_per_bin_for_missed_spks_est': int
The number of spikes per bin used to compute the spike amplitude pdf for a unit,
when computing the missed spikes estimate.
'std_smoothing_kernel_for_missed_spks_est': float
The standard deviation for the gaussian kernel used to compute the spike amplitude
pdf for a unit, when computing the missed spikes estimate.
'min_num_bins_for_missed_spks_est': int
The minimum number of bins used to compute the spike amplitude pdf for a unit,
when computing the missed spikes estimate.
Returns
-------
r : bunch
A bunch whose keys are the computed spike metrics.
Notes
-----
This function is called by `ephysqc.unit_metrics_ks2` which is called by `spikes.ks2_to_alf`
during alf extraction of an ephys dataset in the ibl ephys extraction pipeline.
Examples
--------
1) Compute quick metrics from a ks2 output directory:
>>> from ibllib.ephys.ephysqc import phy_model_from_ks2_path
>>> m = phy_model_from_ks2_path(path_to_ks2_out)
>>> cluster_ids = m.spike_clusters
>>> ts = m.spike_times
>>> amps = m.amplitudes
>>> depths = m.depths
>>> r = bb.metrics.quick_unit_metrics(cluster_ids, ts, amps, depths)
"""
metrics_list = [
'cluster_id',
'amp_max',
'amp_min',
'amp_median',
'amp_std_dB',
'contamination',
'contamination_alt',
'drift',
'missed_spikes_est',
'noise_cutoff',
'presence_ratio',
'presence_ratio_std',
'slidingRP_viol',
'spike_count'
]
if tbounds:
ispi = between_sorted(spike_times, tbounds)
spike_times = spike_times[ispi]
spike_clusters = spike_clusters[ispi]
spike_amps = spike_amps[ispi]
spike_depths = spike_depths[ispi]
if cluster_ids is None:
cluster_ids = np.unique(spike_clusters)
nclust = cluster_ids.size
r = Bunch({k: np.full((nclust,), np.nan) for k in metrics_list})
r['cluster_id'] = cluster_ids
# vectorized computation of basic metrics such as presence ratio and firing rate
tmin = spike_times[0]
tmax = spike_times[-1]
presence_ratio = bincount2D(spike_times, spike_clusters,
xbin=params['presence_window'],
ybin=cluster_ids, xlim=[tmin, tmax])[0]
r.presence_ratio = np.sum(presence_ratio > 0, axis=1) / presence_ratio.shape[1]
r.presence_ratio_std = np.std(presence_ratio, axis=1)
r.spike_count = np.sum(presence_ratio, axis=1)
r.firing_rate = r.spike_count / (tmax - tmin)
# computing amplitude statistical indicators by aggregating over cluster id
camp = pd.DataFrame(np.c_[spike_amps, 20 * np.log10(spike_amps), spike_clusters],
columns=['amps', 'log_amps', 'clusters'])
camp = camp.groupby('clusters')
ir, ib = ismember(r.cluster_id, camp.clusters.unique())
r.amp_min[ir] = np.array(camp['amps'].min())
r.amp_max[ir] = np.array(camp['amps'].max())
# this is the geometric median
r.amp_median[ir] = np.array(10 ** (camp['log_amps'].median() / 20))
r.amp_std_dB[ir] = np.array(camp['log_amps'].std())
# loop over each cluster to compute the rest of the metrics
for ic in np.arange(nclust):
# slice the spike_times array
ispikes = spike_clusters == cluster_ids[ic]
if np.all(~ispikes): # if this cluster has no spikes, continue
continue
ts = spike_times[ispikes]
amps = spike_amps[ispikes]
depths = spike_depths[ispikes]
# compute metrics
r.contamination_alt[ic] = contamination_alt(ts, rp=params['refractory_period'])
r.contamination[ic], _ = contamination(
ts, tmin, tmax, rp=params['refractory_period'], min_isi=params['min_isi'])
r.slidingRP_viol[ic] = slidingRP_viol(ts,
bin_size=params['bin_size'],
thresh=params['RPslide_thresh'],
acceptThresh=params['acceptable_contamination'])
r.noise_cutoff[ic] = noise_cutoff(amps,
quartile_length=params['nc_quartile_length'],
n_bins=params['nc_bins'],
n_low_bins=params['nc_n_low_bins'])
r.missed_spikes_est[ic], _, _ = missed_spikes_est(
amps, spks_per_bin=params['spks_per_bin_for_missed_spks_est'],
sigma=params['std_smoothing_kernel_for_missed_spks_est'],
min_num_bins=params['min_num_bins_for_missed_spks_est'])
# wonder if there is a need to low-cut this
r.drift[ic] = np.sum(np.abs(np.diff(depths))) / (tmax - tmin) * 3600
r.label = compute_labels(r)
return r
[docs]def compute_labels(r, params=METRICS_PARAMS, return_details=False):
"""
From a dataframe or a dictionary of unit metrics, compute a lablel
:param r: dictionary or pandas dataframe containing unit qcs
:param return_details: False (returns a full dictionary of metrics)
:return: vector of proportion of qcs passed between 0 and 1, where 1 denotes an all pass
"""
# right now the score is a value between 0 and 1 denoting the proportion of passing qcs
# we could eventually do a bitwise qc
labels = np.c_[
r.slidingRP_viol,
r.noise_cutoff < params['nc_thresh'],
r.amp_median > params['med_amp_thresh_uv'] / 1e6,
]
if not return_details:
return np.mean(labels, axis=1)
column_names = ['slidingRP_viol', 'noise_cutoff', 'amp_median']
qcdict = {}
for c in np.arange(labels.shape[1]):
qcdict[column_names[c]] = labels[:, c]
return np.mean(labels, axis=1), qcdict
```