{"id":7106,"date":"2018-02-21T00:00:00","date_gmt":"2018-02-20T23:00:00","guid":{"rendered":"https:\/\/www.ieec.cat\/iccub-seminar-radiative-transfer-modeling-of-lyman-alpha-emitters-as-a-probe-of-reionization-not-translated-2\/"},"modified":"2023-01-17T15:09:04","modified_gmt":"2023-01-17T14:09:04","slug":"iccub-seminar-radiative-transfer-modeling-of-lyman-alpha-emitters-as-a-probe-of-reionization-not-translated","status":"publish","type":"post","link":"https:\/\/www.ieec.cat\/es\/iccub-seminar-radiative-transfer-modeling-of-lyman-alpha-emitters-as-a-probe-of-reionization-not-translated\/","title":{"rendered":"ICCUB SEMINAR \u2013 Radiative Transfer Modeling of Lyman-Alpha Emitters as a Probe of Reionization [NOT TRANSLATED]"},"content":{"rendered":"<p>[et_pb_section fb_built=\u00bb1&#8243; fullwidth=\u00bbon\u00bb _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb background_image=\u00bb\/wp-content\/uploads\/2022\/04\/slider-corpo2.jpg\u00bb height=\u00bb114px\u00bb global_colors_info=\u00bb{}\u00bb][\/et_pb_section][et_pb_section fb_built=\u00bb1&#8243; 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_module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_column type=\u00bb4_4&#8243; _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb][et_pb_image src=\u00bbhttps:\/\/www.ieec.cat\/wp-content\/uploads\/2022\/12\/1544521783_c3c72fa45349db2e44554ba8f9e7d365_logoiccub.jpg\u00bb alt=\u00bbICCUB SEMINAR \u2013 Radiative Transfer Modeling of Lyman-Alpha Emitters as a Probe of Reionization\u00bb title_text=\u00bbICCUB SEMINAR \u2013 Radiative Transfer Modeling of Lyman-Alpha Emitters as a Probe of Reionization\u00bb _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb width=\u00bb600px\u00bb module_alignment=\u00bbcenter\u00bb global_colors_info=\u00bb{}\u00bb][\/et_pb_image][et_pb_text _builder_version=\u00bb4.14.8&#8243; _module_preset=\u00bbdefault\u00bb global_colors_info=\u00bb{}\u00bb]Reionization is the last major phase transition in the Universe during which the Intergalactic medium (IGM) changed from a fully neutral to highly ionized state. As Lyman-alpha emission from star-forming galaxies is sensitive to the neutral gas environment, Lyman-alpha emitters (LAEs) are among the few observational probes to the reionization process.<\/p>\n<p>I will present results from radiative transfer calculations aimed at modeling the Lyman-alpha properties of LAEs during reionization.<\/p>\n<p>I will first show how the expected variation in the ionizing UV background level during reionization can account for the observed evolution in the fraction of Lyman-alpha emitters among dropout galaxies at z~6-7. I will also describe our work on the statistical properties of LAEs at high-z from radiative transfer modeling of galaxies in high-resolution cosmological reionization simulations. As the simulation outputs are chosen to match the targeted redshifts of upcoming narrowband LAE surveys, our study provides an important tool to help interpreting future observations.<\/p>\n<p><strong>Contact email:<\/strong> jmiralda(a)fqa.ub.edu [NOT TRANSLATED][\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Reionization is the last major phase transition in the Universe during which the Intergalactic medium (IGM) changed from a fully neutral to highly ionized state. As Lyman-alpha emission from star-forming galaxies is sensitive to the neutral gas environment, Lyman-alpha emitters (LAEs) are among the few observational probes to the reionization process. I will present results [&hellip;]<\/p>\n","protected":false},"author":0,"featured_media":7101,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":"2880","footnotes":""},"categories":[95,73],"tags":[],"class_list":["post-7106","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-charla","category-eventos"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>ICCUB SEMINAR \u2013 Radiative Transfer Modeling of Lyman-Alpha Emitters as a Probe of Reionization [NOT TRANSLATED] - IEEC<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/www.ieec.cat\/es\/iccub-seminar-radiative-transfer-modeling-of-lyman-alpha-emitters-as-a-probe-of-reionization-not-translated\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"ICCUB SEMINAR \u2013 Radiative Transfer Modeling of Lyman-Alpha Emitters as a Probe of Reionization [NOT TRANSLATED] - IEEC\" \/>\n<meta property=\"og:description\" content=\"Reionization is the last major phase transition in the Universe during which the Intergalactic medium (IGM) changed from a fully neutral to highly ionized state. 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