<p>A. Relative change in AP (red, diamonds) and SP (blue, stars) as τ<i><sub>s</sub></i> (i) or τ<i><sub>θ</sub></i> (ii) is varied. For comparison, the linear change in both AP and SP when τ<i><sub>θ</sub></i> and τ<i><sub>s</sub></i> are varied together by the same factor is shown (iii, τ<i><sub>s</sub></i> & τ<i><sub>θ</sub></i>). B. Variations of the duty cycle with τ<i><sub>s</sub></i> (i), τ<i><sub>θ</sub></i> (ii) and τ<i><sub>s</sub></i> & τ<i><sub>θ</sub></i> (iii).</p
<p>Normalized amplitudes of the peaks in <i>recA</i> PA are plotted as function of peak time for ind...
International audienceContext. A number of high-precision time series have recently become available...
<p>Magenta triangles: <i>κ</i><sub>s,A</sub>/25, blue inverted triangles: <i>κ</i><sub>s,ACP</sub>/2...
<p>A. Contributions of <i>s</i> to episode termination (C<sup>s</sup><sub>AP</sub>, red, diamonds) a...
<p>(<i>A</i>) The <i>τ</i> values are shown in pseudocolor within the <i>K<sub>r</sub></i>-<i>V<sub>...
<p>Dependence on <i>G</i><sub><i>m</i></sub> of the quantities characterizing the patterns of activi...
<p>Time-activity curves of [<sup>11</sup>C]ITMM with (A) conventional SA and (B) ultra-high SA.</p
<p>(a)τ<sub><i>s</i></sub> increases (not always monotonically) with τ<sub><i>w</i></sub>. For the s...
<p>(A) Raw multiunit activity data following a shift of the light-dark cycle. After smoothing of the...
<p>A. Time courses of activity (<i>a</i>, black), the synaptic recovery variable (<i>s</i>, red), an...
Aims. We study the time variations in the cycles of 20 active stars based on decade-long photometri...
<p>a) Metrics <i>Q</i><sub>0</sub> (in solid line) and <i>Q</i><sub><i>d</i></sub> (dashed) as a fun...
<p>(<i>A</i>) The <i>τ</i>values are shown in pseudocolor within the <i>K<sub>r</sub></i>-<i>V<sub>r...
Context. A number of high-precision time series have recently become available for many stars as a r...
<p>Time periods of oscillation, <i>T</i> (in sec) at two different values of </p><p></p><p></p><p><m...
<p>Normalized amplitudes of the peaks in <i>recA</i> PA are plotted as function of peak time for ind...
International audienceContext. A number of high-precision time series have recently become available...
<p>Magenta triangles: <i>κ</i><sub>s,A</sub>/25, blue inverted triangles: <i>κ</i><sub>s,ACP</sub>/2...
<p>A. Contributions of <i>s</i> to episode termination (C<sup>s</sup><sub>AP</sub>, red, diamonds) a...
<p>(<i>A</i>) The <i>τ</i> values are shown in pseudocolor within the <i>K<sub>r</sub></i>-<i>V<sub>...
<p>Dependence on <i>G</i><sub><i>m</i></sub> of the quantities characterizing the patterns of activi...
<p>Time-activity curves of [<sup>11</sup>C]ITMM with (A) conventional SA and (B) ultra-high SA.</p
<p>(a)τ<sub><i>s</i></sub> increases (not always monotonically) with τ<sub><i>w</i></sub>. For the s...
<p>(A) Raw multiunit activity data following a shift of the light-dark cycle. After smoothing of the...
<p>A. Time courses of activity (<i>a</i>, black), the synaptic recovery variable (<i>s</i>, red), an...
Aims. We study the time variations in the cycles of 20 active stars based on decade-long photometri...
<p>a) Metrics <i>Q</i><sub>0</sub> (in solid line) and <i>Q</i><sub><i>d</i></sub> (dashed) as a fun...
<p>(<i>A</i>) The <i>τ</i>values are shown in pseudocolor within the <i>K<sub>r</sub></i>-<i>V<sub>r...
Context. A number of high-precision time series have recently become available for many stars as a r...
<p>Time periods of oscillation, <i>T</i> (in sec) at two different values of </p><p></p><p></p><p><m...
<p>Normalized amplitudes of the peaks in <i>recA</i> PA are plotted as function of peak time for ind...
International audienceContext. A number of high-precision time series have recently become available...
<p>Magenta triangles: <i>κ</i><sub>s,A</sub>/25, blue inverted triangles: <i>κ</i><sub>s,ACP</sub>/2...