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<p><a href="page.php?w=free-free_emission">free-free emission</a> and other emission mechanisms.  In <a href="page.php?w=infrared_astronomy">infrared astronomy</a>, SEDs can be used to classify <a href="page.php?w=young_stellar_object">young stellar object</a>s.</p>

<p><big>Detector for spectral energy distribution</big></p>
<p>The count rates observed from a given astronomical radiation source have no simple relationship to the flux from that source, such as might be incident at the top of the <a href="page.php?w=Earth%27s_atmosphere">Earth's atmosphere</a>.</p><p>
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