<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>DESI | Salman Webpage</title><link>https://salmanhiro.github.io/tags/desi/</link><atom:link href="https://salmanhiro.github.io/tags/desi/index.xml" rel="self" type="application/rss+xml"/><description>DESI</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Wed, 24 Jun 2026 00:00:00 +0000</lastBuildDate><image><url>https://salmanhiro.github.io/media/icon_hu5823104125410023470.png</url><title>DESI</title><link>https://salmanhiro.github.io/tags/desi/</link></image><item><title>Tidal Stream Search in DESI Legacy Survey with Particle Spray</title><link>https://salmanhiro.github.io/project/mockstream/</link><pubDate>Wed, 24 Jun 2026 00:00:00 +0000</pubDate><guid>https://salmanhiro.github.io/project/mockstream/</guid><description>&lt;p>Stellar tidal streams — ribbons of stars stripped from globular clusters and dwarf galaxies by the Milky Way&amp;rsquo;s tidal field — encode the history of the Galaxy&amp;rsquo;s accretion events and the shape of its gravitational potential. This research uses the &lt;strong>particle-spray (Mock Stream) algorithm&lt;/strong> to generate fast, N-body-free synthetic stream tracks and searches for their counterparts across the DESI Legacy Survey (DESI LS) footprint.&lt;/p>
&lt;p>By forward-modeling stream morphology across a grid of progenitor orbits and matching mock tracks to stellar density maps built from DESI LS photometry, the pipeline recovers multiple tidal stream candidates over a wide area of sky.&lt;/p>
&lt;p>A key result is the orbital connection between the &lt;strong>LMS-1 stream&lt;/strong> and associated globular clusters, shedding light on the origin and accretion history of this substructure. The analysis suggests that several globular clusters share a common progenitor with LMS-1, pointing to an accreted dwarf galaxy origin.&lt;/p>
&lt;h2 id="approach">Approach&lt;/h2>
&lt;ul>
&lt;li>Generate mock stream tracks with the particle-spray method over a grid of progenitor orbital parameters and Galactic potential models.&lt;/li>
&lt;li>Build stellar density maps from DESI LS photometry using color–magnitude diagram filtering to isolate old, metal-poor populations consistent with tidal debris.&lt;/li>
&lt;li>Match mock tracks to the data and score candidates to identify statistically significant stream detections.&lt;/li>
&lt;li>Trace recovered streams back to known substructures, including LMS-1 and its associated globular cluster system.&lt;/li>
&lt;/ul></description></item></channel></rss>