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<urlset xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.sitemaps.org/schemas/sitemap/0.9" xmlns:image="http://www.google.com/schemas/sitemap-image/1.1" xsi:schemaLocation="http://www.sitemaps.org/schemas/sitemap/0.9 http://www.sitemaps.org/schemas/sitemap/0.9/sitemap.xsd"><url><loc>https://astrovayner.com/about/</loc><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/10/arp148_header.jpg</image:loc><image:title>arp148_header</image:title></image:image><lastmod>2025-08-15T05:28:32+00:00</lastmod><changefreq>weekly</changefreq><priority>0.6</priority></url><url><loc>https://astrovayner.com/research/molecular-interstellar-medium-of-distant-quasar-host-galaxies/</loc><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/12/spec_broad.png</image:loc><image:title>spec_broad</image:title></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/12/alma_spec_compact-e1513761731601.png</image:loc><image:title>ALMA_spec_compact</image:title></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/12/alma_panel_no_axis-e1513759141113.png</image:loc><image:title>ALMA_panel_no_axis</image:title><image:caption>Molecular gas distribution in the host galaxy of 3C 298. Contours are of faintest Ha emission detected with Keck OSIRIS</image:caption></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/12/alma_header.png</image:loc><image:title>ALMA_header</image:title></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/12/alma-observatory.jpg</image:loc><image:title>ALMA Observatory</image:title></image:image><lastmod>2018-10-06T01:24:11+00:00</lastmod><changefreq>weekly</changefreq><priority>0.6</priority></url><url><loc>https://astrovayner.com/research/</loc><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/12/3c298_multi_color_for_astro-e1513763624870.png</image:loc><image:title>3c298_multi_color_for_astro</image:title></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/11/m87.jpg</image:loc><image:title>m87</image:title></image:image><lastmod>2018-10-06T01:22:18+00:00</lastmod><changefreq>weekly</changefreq><priority>0.6</priority></url><url><loc>https://astrovayner.com/research/quasar-host-galaxies/</loc><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/11/n2ha_bpt-e1511172521742.png</image:loc><image:title>n2ha_BPT</image:title><image:caption>Figure 3: Resolved BPT photoionization diagnostic diagram for the host galaxy of 3C 298. Distinct photoionization regions are color coded to the dominant source of ionization.</image:caption></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/11/osiris_panel1-e1511170356477.png</image:loc><image:title>OSIRIS_panel</image:title><image:caption>Figure 2: velocity dispersion map of ionized gas in the host galaxy of 3C 298 as traced by the nebular emission line [OIII] 500.7 nm. Synchrotron emission from the extended jet is shown with black contours observed with the VLA.</image:caption></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/11/osiris_panel-e1511166683532.png</image:loc><image:title>OSIRIS_panel</image:title><image:caption>Figure 1: Three color composite image of ionized gas in the host galaxy of the quasar 3C 298.</image:caption></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/11/keck.jpg</image:loc><image:title>keck</image:title></image:image><image:image><image:loc>https://astrovayner.com/wp-content/uploads/2017/11/keck_1920x715_courtesy-of-andrew-hara.jpg</image:loc><image:title>keck_1920x715_courtesy-of-andrew-hara</image:title></image:image><lastmod>2018-10-06T01:20:57+00:00</lastmod><changefreq>weekly</changefreq><priority>0.6</priority></url><url><loc>https://astrovayner.com/cv/</loc><lastmod>2017-10-15T09:37:10+00:00</lastmod><changefreq>weekly</changefreq><priority>0.6</priority></url><url><loc>https://astrovayner.com/contact/</loc><lastmod>2017-10-14T21:59:18+00:00</lastmod><changefreq>weekly</changefreq><priority>0.6</priority></url><url><loc>https://astrovayner.com</loc><changefreq>daily</changefreq><priority>1.0</priority><lastmod>2025-08-15T05:28:32+00:00</lastmod></url></urlset>
