| fluence | -- |
| conv | -- |
| tau | -- |
| uBurstLength | -- |
| uSingAlpha | -- |
| num | 0 |
| uPeakLum | -- |
| r1090 | -- |
| r2590 | -- |
| persLum | -- |
| burstLength | -- |
| uConv | -- |
| tDel | -- |
| uTau | -- |
| peakLum | -- |
| uR1090 | -- |
| uR2590 | -- |
| uSingDecay | -- |
| uFluence | -- |
| flag | 1 |
| alpha | -- |
| singAlpha | -- |
| lAcc | 1.5 |
| h | 75.45 |
| uTDel | -- |
| uPersLum | -- |
| model | a314 |
| z | 0.2 |
| singDecay | -- |
| uAlpha | -- |
⚠ (:html:)
<script type="text/javascript"
src="uploads/dygraph-combined.js"></script>
<div id="graphdiv4"
style="width:800px; height:320px;"></div>
<script type="text/javascript">
g4 = new Dygraph(
document.getElementById("graphdiv4"),
"uploads/Kepler/kepler_a314_mean.csv",
{
errorBars: true,
radius: { axis: {} },
ylabel: "Luminosity (1e37 erg/s)",
y2label: "Radius (km)",
xlabel: "Time (s)",
}
);
</script>
(:htmlend:)
The mean luminosity (green line, left-hand y-axis), is plotted
with the lighter green band giving the 1-sigma error calculated from the
variation in the lightcurves included in the average. The radius is shown
in blue (right-hand y-axis)
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