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    <loc>https://gamma-research.space/research-program</loc>
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    <lastmod>2025-08-05</lastmod>
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    <loc>https://gamma-research.space/research-program/spark-bpp9w</loc>
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    <priority>0.5</priority>
    <lastmod>2025-07-08</lastmod>
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      <image:title>Research - Host Galaxies of Massive Black Hole Mergers - The host galaxies of merging massive black holes can be difficult to identify. This image shows an ongoing merger between two simulated galaxies, which will lead to the formation of a massive black hole binary. This image was produced using a cosmological simulation of galaxy formation, through stellar population synthesis and dust radiative transfer. We are using these synthetic telescope images to study the unique morphological properties of the host galaxies of massive black hole mergers.</image:title>
      <image:caption>Image credit: Jaeden Bardati</image:caption>
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  </url>
  <url>
    <loc>https://gamma-research.space/research-program/project-four-rxdg5-k6act</loc>
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    <priority>0.5</priority>
    <lastmod>2025-05-24</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/5fdc70dff65a9a5fd491b52a/70660e3d-7c56-4e24-bf56-f80171a98e4a/bestfits_compare_all_SPARK_lightcurves.png</image:loc>
      <image:title>Research - Kilonova Spectral r-Process Abundance Retrieval - The observed optical/infrared spectrum of GW17017 at 1.4, 2.4, 3.4, and 4.4 days post-merger (black). The blackbody continuum has broad absorption features due to the opacity of freshly-synthesized r-process elements in the kilonova ejecta. We fit the observed spectra to synthetic spectra from radiative transfer simulations of kilonova ejecta, to infer the abundance pattern of r-process elements produced in this merger (Vieira et al., 2023).</image:title>
      <image:caption>Image credit: Nicholas Vieira</image:caption>
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  <url>
    <loc>https://gamma-research.space/research-program/project-four-rxdg5-chjbh</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2024-08-19</lastmod>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/5fdc70dff65a9a5fd491b52a/1625816483289-UFXTB51NEJQ45PNUME1C/GW170817_Chandra_Hubble_v4.png</image:loc>
      <image:title>Research - Electromagnetic Follow-up of Gravitational Wave Events - The optical kilonova counterpart of the first binary neutron star merger GW170817 as observed by the Hubble Space Telescope (background), and the X-ray afterglow of the accompanying short Gamma-ray burst as observed by the Chandra X-ray Observatory (insets).</image:title>
      <image:caption>The X-ray afterglow surprisingly brightened over several months after the merger, unlike any other short Gamma-ray burst afterglow ever observed (Ruan et al., 2018). Image credit: Daryl Haggard</image:caption>
    </image:image>
    <image:image>
      <image:loc>https://images.squarespace-cdn.com/content/v1/5fdc70dff65a9a5fd491b52a/1626979846217-U24VWUL3H389C9J48LTL/GW190814_giz_coverage_separate.jpg</image:loc>
      <image:title>Research - Electromagnetic Follow-up of Gravitational Wave Events - Make it stand out</image:title>
      <image:caption>Sky coverage of the LIGO/Virgo gravitational wave localization of the first possible neutron star - black hole merger GW190814 by our CFHT observations (Vieira et al., 2020). Our systematic tiling approach using a wide-field optical imager on a 3m-class telescope is well-suited for the more-distant mergers expected to be detected by LIGO/Virgo in Observing Run 4.</image:caption>
    </image:image>
  </url>
  <url>
    <loc>https://gamma-research.space/research-program/clquasars</loc>
    <changefreq>monthly</changefreq>
    <priority>0.5</priority>
    <lastmod>2025-08-05</lastmod>
  </url>
  <url>
    <loc>https://gamma-research.space/new-page</loc>
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    <priority>0.75</priority>
    <lastmod>2020-12-19</lastmod>
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    <loc>https://gamma-research.space/home</loc>
    <changefreq>daily</changefreq>
    <priority>1.0</priority>
    <lastmod>2025-04-30</lastmod>
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    <loc>https://gamma-research.space/the-team</loc>
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    <lastmod>2025-11-02</lastmod>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:title>The Team</image:title>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/5fdc70dff65a9a5fd491b52a/b27b38fb-3ea5-4f3f-85b3-ba82836fa1d5/sara.png</image:loc>
      <image:title>The Team</image:title>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/5fdc70dff65a9a5fd491b52a/9ea6fea2-d385-4641-bcf1-7a49bff68cf7/david.png</image:loc>
      <image:title>The Team</image:title>
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  <url>
    <loc>https://gamma-research.space/contact</loc>
    <changefreq>daily</changefreq>
    <priority>0.75</priority>
    <lastmod>2022-08-04</lastmod>
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      <image:title>Contact - Contact us!</image:title>
      <image:caption>jruan@ubishops.ca (514) 463-5414 Mailing Address: 2600 Rue College Sherbrooke, Québec J1M 1Z7 Canada Campus Office: Johnson 104C</image:caption>
    </image:image>
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  <url>
    <loc>https://gamma-research.space/about-me</loc>
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    <lastmod>2026-03-26</lastmod>
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