{% extends 'core/lcars_app.html' %} {% load static %} {% block header_title %} AutoWISP Reductions Progress {% endblock header_title %} {% block extra_head %} {% endblock extra_head %} {% block app_title %} Processing Progress {% endblock app_title %} {% block left_menu %} {% if running %} {% if await_start >= 0 %}
Waiting to start {{ await_start }}
{% else %}
Processing
{% endif %} {% else %} {% endif %}
Add New Images
{% endblock left_menu %} {% block main %}
{% csrf_token %} {# Expose refresh config to JS via data attributes #} {% if refresh_seconds %}
{% endif %} {% for channel in channels %} {% endfor %} {% for step, imtype, by_channel, runs, step_errors in progress %} {% for success, failure, pending, by_status in by_channel %} {% with final=success|add:failure %} {% with total=final|add:pending %} {% endwith %} {% endwith %} {% endfor %} {% endfor %}
Step {% if not running %}
Select all
{% endif %}
Image Type{{ channel }}
{% if step.0 == 'calibrate' %} Calibrates raw frames using bias, dark, and flat corrections. This normalizes pixel values so later steps work on clean data. {% elif step.0 == 'find' and step.1 == 'stars' %} Detects point sources using your threshold and extraction settings. This produces initial star coordinates used by later steps. {% elif step.0 == 'solve' and step.1 == 'astrometry' %} Solves the WCS so sky coordinates map to pixel coordinates. This enables catalog matching and accurate positions. {% elif step.0 == 'fit' and step.1 == 'star' and step.2 == 'shape' %} Fits PSF/PRF shapes to measure flux more precisely. These fits provide the basis for high-quality photometry. {% elif step.0 == 'measure' and step.1 == 'aperture' and step.2 == 'photometry' %} Measures flux in fixed apertures for each source. This provides robust brightness estimates for later modeling. {% elif step.0 == 'fit' and step.1 == 'source' and step.2 == 'extracted' and step.4 == 'map' %} Fits a smooth PSF map across the image using many stars. This reduces noise in PSF parameters and improves consistency. {% elif step.0 == 'fit' and step.1 == 'magnitudes' %} Fits relative magnitudes by comparing each frame to a reference. This removes frame-to-frame systematics and normalizes fluxes. {% elif step.0 == 'create' and step.1 == 'lightcurves' %} Reorganizes measurements into per-star lightcurves. This collects each star’s time series into a single file. {% elif step.0 == 'epd' or step.1 == 'epd' %} Removes trends correlated with external parameters. This reduces instrumental systematics in each lightcurve. {% elif step.0 == 'tfa' or step.1 == 'tfa' %} Filters trends shared across many stars in the field. This improves precision while preserving real variability. {% else %} Runs this pipeline step and updates its outputs. Use hover for quick context while monitoring progress. {% endif %}
{{ step|join:" " }}
{% if step_errors %} {{ step_errors }} recorded error{{ step_errors|pluralize }} — review
{{ imtype }} ⚠
{% elif step.0 == 'fit' and step.1 == 'magnitudes' or step.0 == 'find' and step.1 == 'stars' %} {% if step.0 == 'fit' and step.1 == 'magnitudes' %} select reference image {% else %} tune source extraction {% endif %}
{{ imtype }}
{% else %} {{ imtype }} {% endif %}
{% for status, count in by_status %} {% endfor %}
{% if step.0 == 'calibrate' %} Review cilabration diagnostics {% url 'diagnostics:display_image_diagnostics' diagnostic_name='quantiles' as diagnostic_url %} {% elif step.0 == 'find' and step.1 == 'stars' %} Review star finding diagnostics {% url 'diagnostics:display_image_diagnostics' diagnostic_name='num_extracted_src' as diagnostic_url %} {% elif step.0 == 'solve' and step.1 == 'astrometry' %} Review astrometry diagnostics {% url 'diagnostics:display_image_diagnostics' diagnostic_name='pointing_offset' as diagnostic_url %} {% elif step.0 == 'fit' and step.1 == 'star' and step.2 == 'shape' %} Review star shepe fit diagnostics {% url 'diagnostics:display_image_diagnostics' diagnostic_name='bg_center' as diagnostic_url %} {% elif step.0 == 'measure' and step.1 == 'aperture' and step.2 == 'photometry' %} Review aperture photometry diagnostics {% url 'diagnostics:display_image_diagnostics' diagnostic_name='bg_center' as diagnostic_url %} {% elif step.0 == 'fit' and step.1 == 'source' and step.2 == 'extracted' and step.4 == 'map' %} Review source extraction PSF diagnostics {% url 'diagnostics:display_image_diagnostics' diagnostic_name='s_center' as diagnostic_url %} {% elif step.0 == 'fit' and step.1 == 'magnitudes' or step.0 == 'epd' or step.0 == 'tfa' or step.1 == 'epd' or step.1 == 'tfa' %} Review magnitude fitting performance {% url 'diagnostics:display_detrending_diagnostics' as diagnostic_url %} {% endif %} {% if diagnostic_url %} {% endif %}
{{success}}/{{total}} {% if failure > 0 %} | {{failure}}/{{total}} {% endif %}
{% if diagnostic_url %} {% endif %}
Status {{ status }}
{{count}}/{{pending}}
{% endblock main %} {% block scripts %} {# Moved all JS to static/processing/js/progress.js #} {% endblock %}