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Model a166

This page presents lightcurves for Model a166 produced using the KEPLER simulation code, and analysed following Lampe, Heger & Galloway (2015).

The curve presented here is as measured in the neutron star's Newtonian rest frame. To compare this to an observation it is necessary to apply redshift corrections. Instructions for doing this are provided in the companion paper and a summary is provided here

An averaged representation of this burst train is available click here


Lightcurve

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)


Parameters

The following table presents the initial conditions for the model and if a burst occurred, the average burst parameters.

NameValueUnitDescription
modela166--Model ID
num8--Number of simulated bursts
z2.0%Metallicity mass fraction
h70.48%Hydrogen mass fraction
lAcc1.26--Accretion luminosity (1)
burstLength307.4 ± 111.0sBurst duration
peakLum5.04 ± 0.2810+30WPeak lumonisity
persLum16.15 ± 2.2810+28WPersistent luminsoity
fluence3.39 ± 0.8710+32WFluence
tau66.7 ± 15.4sEquivalent burst duration (tau)
tDel0.18 ± 0.02hRecurrence time
conv6.83 ± 1.1%Convexity
r10906.072 ± 0.209s10% rise time
r25904.948 ± 0.129s25% rise time
singAlpha0.63 ± 0.41--Power law decay index
singDecay22.79 ± 10.23sExponential decay timescale
alpha55.9 ± 19.5--Fluence ratio (alpha)
flag4--Analysis quality flag (2)

(1) The accretion rate is in terms of the Eddington accretion rate $(1.75 \times 10^{-8} \, \mathrm{M}_\odot \, \mathrm{yr}^{-1})$

(2) Guide To Analyis Flags

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Page last modified on December 21, 2015, at 06:57 PM