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	<title><![CDATA[Projects]]></title>
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	<description><![CDATA[Externally funded and collaborative projects&nbsp;]]></description>
	<copyright><![CDATA[Copyright 2026, Institute of Astrophysics Team - Forth]]></copyright>
	<pubDate>Sun, 05 Apr 2026 20:48:39 +0000</pubDate>
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		<title><![CDATA[TARGET]]></title>
		<description><![CDATA[<img style="margin:5px; float:left;" src="https://salt.ia.forth.gr/media/images/articles/Screenshot2025-03-20at131135_thumb.png" alt="Projects" /> <p>This is the Target Project</p>TARGET: A high-precision timing and frequency standard for FORTH&nbsp;]]></description>
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		<pubDate>Thu, 20 Mar 2025 11:05:00 +0000</pubDate>
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		<title><![CDATA[Argos]]></title>
		<description><![CDATA[<img style="margin:5px; float:left;" src="https://salt.ia.forth.gr/media/images/articles/argos_midjourney3_thumb.webp" alt="Projects" /> <p>This is the Argos Project</p><p>ARGOS is a project to design a "small-D, big-N" interferometer currently in its design phase. The project is supported by a HORIZON-INFRADEV grant by the European Commission.<br></p>]]></description>
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		<pubDate>Sun, 02 Jul 2023 08:49:00 +0000</pubDate>
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		<title><![CDATA[EPTA]]></title>
		<description><![CDATA[<img style="margin:5px; float:left;" src="https://salt.ia.forth.gr/media/images/articles/epta-min_thumb.jpg" alt="Projects" /> <p>The European Pulsar Timing Array</p><p>The European Pulsar Timing Array (EPTA) is a scientific collaboration bringing together teams of astronomers around the largest European radio telescopes, as well as groups specialized in data analysis and modelling of gravitational-wave (GW) signals.</p>]]></description>
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		<pubDate>Fri, 02 Jun 2023 08:50:00 +0000</pubDate>
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		<title><![CDATA[EPICS]]></title>
		<description><![CDATA[<img style="margin:5px; float:left;" src="https://salt.ia.forth.gr/media/images/articles/epics-min_thumb.jpg" alt="Projects" /> <p>European Pulsar Interior Composition Survey</p><p>Neutron stars comprise the densest form of matter in the observable Universe. Their mass distribution contains crucial information about the late evolution of massive stars the supernova explosion mechanism and the equation-of-state ot cold. nuclear matter below the nuclear saturation density. The European Pulsar Interior Composition Survey (EPICS) is a project that combines novel experimental approaches with state-of-the-art theoretical modelling to achieve an appreciable increase in the number of&nbsp;precise neutron star mass measurements.&nbsp;These data will lead to unprecedented insights into the mechanisms driving&nbsp;the formation and evolution o neutron stars, as well as the properties of&nbsp;super-dense matter.</p>]]></description>
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		<pubDate>Tue, 02 Jun 2020 08:51:00 +0000</pubDate>
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