| 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 | 0.94 |
|---|
| h | 76.0 |
|---|
| uTDel | -- |
|---|
| uPersLum | -- |
|---|
| model | a92 |
|---|
| z | 0.0 |
|---|
| 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_a92_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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