{"id":2399,"date":"2023-05-29T09:36:44","date_gmt":"2023-05-29T12:36:44","guid":{"rendered":"https:\/\/astro.uc.cl\/?post_type=charlas&#038;p=2399"},"modified":"2023-05-29T09:36:52","modified_gmt":"2023-05-29T12:36:52","slug":"the-winered-starting-observations-with-magellan-6-5m-noriyuki-matsunaga","status":"publish","type":"charlas","link":"https:\/\/astro.uc.cl\/en\/charlas\/the-winered-starting-observations-with-magellan-6-5m-noriyuki-matsunaga\/","title":{"rendered":"The WINERED starting observations with Magellan 6.5m \u2013 Noriyuki Matsunaga"},"content":{"rendered":"\n<p>WINERED is a near-IR spectrograph for a wide wavelength range of 0.9-1.35 micron with resolving powers of 28,000 and 70,000. After successful observations at Araki 1.3-m telescope in Japan and the NTT 3.58-m telescope at La Silla, ESO, we have started its operation with the Magellan 6.5-m telescope (Clay). With the high sensitivity, we can reach J=14.5 for a high S\/N of 100 or J=16.5 for low S\/N of 20. In this talk, I will report the first light made with the Magellan in 2022 June and discuss some of our sciences based on previous data and projects being planned in future runs including the one soon in June.<\/p>\n\n\n\n<p>Related links:<br><a href=\"http:\/\/lihweb.kyoto-su.ac.jp\/WINERED\/\" target=\"_blank\" rel=\"noreferrer noopener\">http:\/\/lihweb.kyoto-su.ac.jp\/WINERED\/<\/a><br><a href=\"http:\/\/merlot.kyoto-su.ac.jp\/WINERED\/Magellan\/Public\/\" target=\"_blank\" rel=\"noreferrer noopener\">http:\/\/merlot.kyoto-su.ac.jp\/WINERED\/Magellan\/Public\/<\/a><br><a href=\"http:\/\/merlot.kyoto-su.ac.jp\/WINERED\/ETC\/etc1.php\" target=\"_blank\" rel=\"noreferrer noopener\">http:\/\/merlot.kyoto-su.ac.jp\/WINERED\/ETC\/etc1.php<\/a><\/p>\n","protected":false},"featured_media":0,"template":"","meta":[],"categorias_charlas":[59],"class_list":["post-2399","charlas","type-charlas","status-publish","hentry","categorias_charlas-seminarios"],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v25.8 - 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