{"id":12963,"date":"2023-04-01T09:00:46","date_gmt":"2023-04-01T00:00:46","guid":{"rendered":"https:\/\/www.waseda.jp\/inst\/wias\/?p=12963"},"modified":"2024-02-06T17:03:34","modified_gmt":"2024-02-06T08:03:34","slug":"%e7%a7%8b%e5%b1%b1-%e5%be%b9-2-13-2-6","status":"publish","type":"post","link":"https:\/\/www.waseda.jp\/inst\/wias\/other-en\/2023\/04\/01\/12963\/","title":{"rendered":"SHIMAKAWA, Rhythm"},"content":{"rendered":"<h5>Name<\/h5>\n<p>SHIMAKAWA, Rhythm<\/p>\n<h5>Degree<\/h5>\n<p>Doctor of Philosophy<\/p>\n<h5>Status<\/h5>\n<p>Associate Professor<\/p>\n<h5>HP (URL)<\/h5>\n<p><a href=\"https:\/\/sites.google.com\/view\/rhythmshimakawa\/home\">https:\/\/sites.google.com\/view\/rhythmshimakawa\/home<\/a><\/p>\n<h5>Research Topic<\/h5>\n<p>Large-scale structure and galaxy formation in big data astronomy<\/p>\n<p style=\"text-align: justify;\">How did the universe evolve, and how did the Milky Way and its surrounding supercluster form? To answer these questions, we aim to draw the large-scale structure of the distant universe and statistically clarify the formation and evolutionary history of associated galaxies by using big data covering tens of thousands to tens of billions of objects and mathematical statistical analysis.<\/p>\n<h5>Monthly Spotlight<\/h5>\n<p>[Monthly Spotlight] is focusing on a researcher to introduce his\/her research.<br \/>\n<a href=\"https:\/\/www.waseda.jp\/inst\/wias\/news-en\/2023\/08\/31\/14026\/\"><strong>Uncovering the Mystery of the Origin and Formation of Galaxies through a National Survey of Space Using Citizen Science and AI<\/strong><\/a><\/p>\n<h5>Education and Academic Employment<\/h5>\n<p><strong>Education<\/strong><\/p>\n<table class=\"table table-striped table-chronology table-colored-tbhd\" style=\"width: 100%; border-collapse: collapse; height: 69px;\" border=\"0\">\n<tbody>\n<tr style=\"height: 23px;\">\n<td style=\"width: 17.1004%; height: 23px;\">2012<\/td>\n<td style=\"width: 82.8996%; height: 23px;\">B.A. Osaka University<\/td>\n<\/tr>\n<tr style=\"height: 23px;\">\n<td style=\"width: 17.1004%; height: 23px;\">2017<\/td>\n<td style=\"width: 82.8996%; height: 23px;\">Ph.D. The Graduate University for Advanced Studies, SOKENDAI<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p><strong>Academic Employment<\/strong><\/p>\n<table class=\"table table-striped table-chronology table-colored-tbhd\" style=\"width: 100%; border-collapse: collapse; height: 69px;\" border=\"0\">\n<tbody>\n<tr style=\"height: 23px;\">\n<td style=\"width: 17.1004%; height: 23px;\">2013-2015<\/td>\n<td style=\"width: 82.8996%; height: 23px;\">\u00a0RCUH Subaru Research Intern (Subaru Telescope, NAOJ)<\/td>\n<\/tr>\n<tr style=\"height: 23px;\">\n<td style=\"width: 17.1004%; height: 23px;\">2015-2017<\/td>\n<td style=\"width: 82.8996%; height: 23px;\">JSPS Research Fellow DC2 (SOKENDAI)<\/td>\n<\/tr>\n<tr style=\"height: 23px;\">\n<td style=\"width: 17.1004%; height: 23px;\">2017-2018<\/td>\n<td style=\"width: 82.8996%; height: 23px;\">JSPS Overseas Research Fellow (University of California, Santa Cruz)<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 17.1004%;\">2018-2022<\/td>\n<td style=\"width: 82.8996%;\">NAOJ Fellow, Project Assistant Professor (Subaru Telescope, NAOJ)<\/td>\n<\/tr>\n<tr>\n<td style=\"width: 17.1004%;\">2023-Present<\/td>\n<td style=\"width: 82.8996%;\">Associate Professor, Non-tenured (WIAS, Waseda University)<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<h5>Fields of Research Interests<\/h5>\n<p>Astronomy<\/p>\n<h5>Academic Publications<\/h5>\n<ul style=\"list-style-type: square;\">\n<li>R. Shimakawa, et al., \u201cKing Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z = 0.55 using the Subaru Hyper Suprime-Cam\u201d, Monthly Notice of the Royal Astronomical Society Letter, vol.519, issue.1, pp.L45-L50, February 2023<\/li>\n<li>R. Shimakawa, \u201cSearch for extended Lyman-\u03b1 emission around 9k quasars at z = 2-3\u201d, Monthly Notice of the Royal Astronomical Society, vol.514, issue.3, pp.3910-3924, August 2022<\/li>\n<li>R. Shimakawa, et al. \u201cPassive spiral galaxies deeply captured by Subaru Hyper Suprime-Cam\u201d, Publications of the Astronomical Society of Japan, vol.74, issue.3, pp.612-624, June 2022<\/li>\n<li>R. Shimakawa, et al., \u201cH-alpha emission in the outskirts of galaxies at z=0.4\u201d, Publications of the Astronomical Society of Japan, vol.74, issue.2, pp.318-325, April 2022<\/li>\n<li>R. Shimakawa, et al., \u201cSubaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg2 at z=0.3-0.6\u201d, Publications of the Astronomical Society of Japan, vol.73, issue.6, pp.1575-1588, December 2021<\/li>\n<li>R. Shimakawa, et al., \u201cSubaru Hyper Suprime-Cam excavates colossal over- and underdense structures over 360 deg2 out to z=1\u201d, Monthly Notice of the Royal Astronomical Society, vol.503, issue.3, pp.3896-3912, May 2021<\/li>\n<li>R. Shimakawa, et al., \u201cMAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z=2.2\u201d, Monthly Notice of the Royal Astronomical Society, vol.481, issue.4, pp.5630-5650, December 2018<\/li>\n<li>R. Shimakawa, et al., \u201cMAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z=2.5\u201d, Monthly Notice of the Royal Astronomical Society, vol.473, issue.2, pp.1977-1999, January 2018<\/li>\n<li>Shimakawa, et al., \u201cDirect evidence for Ly\u03b1 depletion in the protocluster core\u201d, Monthly Notice of the Royal Astronomical Society Letter, vol.468, issue.1, pp.L21-L25, June 2017<\/li>\n<li>R. Shimakawa, et al., \u201cSimilarities and uniqueness of Ly\u03b1 emitters among star-forming galaxies at z=2.5\u201d, Monthly Notice of the Royal Astronomical Society, vol.468, issue.1, pp.1123-1141, June 2017<\/li>\n<li>R. Shimakawa, et al., \u201cCorrelation between star formation activity and electron density of ionized gas at z=2.5\u201d, Monthly Notices of the Royal Astronomical Society, vol.451, issue.2, pp.1284-1289, August 2015<\/li>\n<li>R. Shimakawa, et al., \u201cAn early phase of environmental effects on galaxy properties unveiled by near-infrared spectroscopy of protocluster galaxies at z&gt;2\u201d, Monthly Notice of the Royal Astronomical Society, vol.448, issue.1, pp.666-680, March 2015<\/li>\n<li>R. Shimakawa et al., \u201cIdentification of the progenitors of rich clusters and member galaxies in rapid formation at z&gt;2\u201d, Monthly Notice of the Royal Astronomical Society Letter, vol.441, pp.L1-L5, June 2014<\/li>\n<\/ul>\n<h5>Other Interests<\/h5>\n<p>Basketball<\/p>\n<h5>Affiliated Academic Organizations<\/h5>\n<p>The Astronomical Society of Japan<\/p>\n<h5>Awards<\/h5>\n<p><b>2015<\/b> SOKENDAI Future Scientist Award<br \/>\n<strong>2017<\/strong> The SOKENDAI Research Award<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Name SHIMAKAWA, Rhythm Degree Doctor of Philosophy Status Associate Professor HP (URL) https:\/\/sites.google.co [&hellip;]<\/p>\n","protected":false},"author":6,"featured_media":12935,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"footnotes":""},"categories":[97],"tags":[],"class_list":["post-12963","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-other-en"],"acf":[],"_links":{"self":[{"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/posts\/12963","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/users\/6"}],"replies":[{"embeddable":true,"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/comments?post=12963"}],"version-history":[{"count":2,"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/posts\/12963\/revisions"}],"predecessor-version":[{"id":15142,"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/posts\/12963\/revisions\/15142"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/media\/12935"}],"wp:attachment":[{"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/media?parent=12963"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/categories?post=12963"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.waseda.jp\/inst\/wias\/wp-json\/wp\/v2\/tags?post=12963"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}