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-search_query=cat:astro-ph.*+AND+lastUpdatedDate:[202407262000+TO+202408012000]&start=0&max_results=5000
-<h1>New astro-ph.* submissions cross listed on cs.LG, cs.AI, stat.*, physics.data-an staritng 202407262000 and ending 202408012000</h1>Feed last updated: 2024-08-01T00:00:00-04:00<a href="http://arxiv.org/pdf/2407.19481v1"><h2>What can we learn about Reionization astrophysical parameters using
+search_query=cat:astro-ph.*+AND+lastUpdatedDate:[202407272000+TO+202408022000]&start=0&max_results=5000
+<h1>New astro-ph.* submissions cross listed on cs.AI, stat.*, cs.LG, physics.data-an staritng 202407272000 and ending 202408022000</h1>Feed last updated: 2024-08-02T00:00:00-04:00<a href="http://arxiv.org/pdf/2407.19481v1"><h2>What can we learn about Reionization astrophysical parameters using
   Gaussian Process Regression?</h2></a>Authors:  Purba Mukherjee, Antara Dey, Supratik Pal</br>Comments: No comment found</br>Primary Category: astro-ph.CO</br>All Categories: astro-ph.CO, astro-ph.IM, cs.LG</br><p>Reionization is one of the least understood processes in the evolution
 history of the Universe, mostly because of the numerous astrophysical processes
 occurring simultaneously about which we do not have a very clear idea so far.