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<oembed><version>1.0</version><provider_name>weobserve</provider_name><provider_url>https://www.weobserve.eu</provider_url><author_name>nikoletta karitsioti</author_name><author_url>https://www.weobserve.eu/author/karitsioti/</author_url><title>How to help scientists in the Gravitational Wave noise hunt - weobserve</title><type>rich</type><width>600</width><height>338</height><html>&lt;blockquote class="wp-embedded-content"&gt;&lt;a href="https://www.weobserve.eu/event/how-to-help-scientists-in-the-gravitational-wave-noise-hunt/"&gt;How to help scientists in the Gravitational Wave noise hunt&lt;/a&gt;&lt;/blockquote&gt;
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&lt;/script&gt;&lt;iframe sandbox="allow-scripts" security="restricted" src="https://www.weobserve.eu/event/how-to-help-scientists-in-the-gravitational-wave-noise-hunt/embed/" width="600" height="338" title="&#x201C;How to help scientists in the Gravitational Wave noise hunt&#x201D; &#x2014; weobserve" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"&gt;&lt;/iframe&gt;</html><thumbnail_url>https://www.weobserve.eu/wp-content/uploads/2020/09/reinforce_webinar-16-october-scaled.jpg</thumbnail_url><thumbnail_width>2560</thumbnail_width><thumbnail_height>1280</thumbnail_height><description>The sensitivity of Gravitational Waves detectors is limited by several types of noise, called&#xA0;glitches, whose presence affects the quality of the data. The glitches can have various origins, having a stationary nature (e.g. a noise signal with a stable frequency) or being transient on various timescales. In order to optimize and run the interferometers it is fundamental to identify the sources of noise and reduce or eliminate its origin. In this framework, citizen scientists can play a fundamental role by [&hellip;]</description></oembed>
