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report_template.html
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report_template.html
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<!DOCTYPE html>
<html>
<header lang="en">
<title> Report page ExoTiC-ISM </title>
</header>
<body>
<h1> Report page ExoTIC-ISM </h1>
<h2> {{ data_file }} - {{ run_name }} </h2>
<h3> Input parameters: </h3>
<p>
Number of systematic models: {{ nsys }}<br>
Wavelength mid point = {{ wavelength_mid_point }}<br>
Wavelength half width = {{ wavelength_half_width }}
</p>
<p>
<h5> Planet parameters: </h5>
Rp/R* = {{ rl_in }}<br>
Epoch (MJD) = {{ epoch_in }}<br>
Inclination (deg) = {{ incl_deg_in }}<br>
Eccentricity = {{ ecc_in }}<br>
Omega (deg) = {{ omega_in }}<br>
Period (days) = {{ period_in }}<br>
a/R* = {{ aor_in }}
<h5> Stellar parameters:</h5>
FeH (dex) = {{ metallicity }}<br>
Teff (K) = {{ teff_in }}<br>
log(g) (cgs) = {{ logg_in }}<br>
</p>
<h3> Output parameters: </h3>
<h5> Limb-darkening coefficients: </h5>
<p>
C1 = {{ c1 }}<br>
C2 = {{ c2 }}<br>
C3 = {{ c3 }}<br>
C4 = {{ c4 }}
</p>
<h5> Top five systematic models by their weight </h5>
<p>
Check the chi-squared values and the AIC evidence for reasonable fits. <br>
If the chi-squared values far exceed the DOF then it is likely that the input data contains additional noise, double check the spectral extraction. <br>
Model numbers = {{ top_five_numbers }}<br>
DOF = {{ top_five_dof }}<br>
Chi-squared = {{ top_five_chisq }}<br>
AIC evidence = {{ top_five_aicevidence}}<br>
Weights = {{ top_five_weights }}<br>
SDNR = {{ top_five_sdnr }}<br>
<br>
<h5> Top model Noise Statistics: </h5>
White noise = {{ white_noise }}<br>
Red noise = {{ red_noise }}<br>
Beta = {{ beta }} <br>
If the red-noise is significant it means the data is poorly fit by any of the systematic models. It is recommended that the input lightcurves are checked for additional noise sources.
</p>
<h3> Marginalised parameters: </h3>
<!-- <p>
{{ num_rejected }} models do not satisfy the AIC evidence condition and were removed
from the marginalisation. Their model numbers are (numbering starts at 0):<br>
{{ indices_rejected }}
</p> -->
<p>
If None, parameter was not fit for.<br>
<br>
Rp/R* = {{ rl_marg }} +/- {{ rl_marg_err }}<br>
Epoch (MJD) = {{ epoch_marg }} +/- {{ epoch_marg_err }}<br>
Inclination (rad) = {{ inclin_rad_marg }} +/- {{ inclin_rad_marg_err }}<br>
Inclination (deg) = {{ inclin_deg_marg }} +/- {{ inclin_deg_marg_err }}<br>
System density (Ms+Mp/R^3) = {{ msmpr_marg }} +/- {{ msmpr_marg_err }}<br>
a/R* = {{ aor_marg }} +/- {{ aor_marg_err }}<br>
</p>
<h3> Systematics </h3>
<p>
<img src="{{ systematics_figure }}" alt="systematics" width="900" height="650"><br>
<br>
<i>Top:</i> Evidence-based weight associated with each systematic model when fit with the data.
<i>Middle:</i> Standard deviation of the residuals after correcting for each systematic model.
<i>Bottom:</i> Radius ratio measured from the transit depth when the light curve has been corrected
using each systematic model. <i>If present, grey crosses mark discarded systematic models (poor AIC evidence).</i>
</p>
<h3> Lightcurves </h3>
<p>
<img src="{{ lightcurve_figure }}" alt="lightcurve" width="900" height="650"><br>
<br>
<i>Top:</i> Input lightcurve with no systematic model correction applied.
<i>Middle:</i> Lightcurve corrected by highest weight systematic model plotted with the smooth
planetary transit model centred on the mid-transit time.
<i>Bottom:</i> Residuals and uncertainties associated with the middle panel lightcurve. The upper and
lower standard deviation bounds are shown in dotted lines relative to zero.
</p>
</body>
</html>