Dr. John Barentine FRAS<p>"We detected broadband emissions from <a href="https://astrodon.social/tags/Starlink" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Starlink</span></a> <a href="https://astrodon.social/tags/satellites" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>satellites</span></a>, predominantly between 54-66 MHz, with flux densities exceeding 500 Jy. These signals are highly polarized and unlikely to originate from ground-based RFI or reflected astronomical sources. Instead, they are likely intrinsic to the satellites, with distinct differences in emission properties observed between satellite generations."</p><p><a href="https://arxiv.org/abs/2504.10032" rel="nofollow noopener" translate="no" target="_blank"><span class="invisible">https://</span><span class="">arxiv.org/abs/2504.10032</span><span class="invisible"></span></a></p><p><a href="https://astrodon.social/tags/Astronomy" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Astronomy</span></a> <a href="https://astrodon.social/tags/RadioAstronomy" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>RadioAstronomy</span></a> <a href="https://astrodon.social/tags/RFI" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>RFI</span></a> <a href="https://astrodon.social/tags/Space" class="mention hashtag" rel="nofollow noopener" target="_blank">#<span>Space</span></a></p>