{"blog_url":"https://yoshiyuki-kitne.hatenadiary.org/","title":" 2002, ApJ, 565, L71-L74","author_name":"yoshiyuki_kitne","width":"100%","version":"1.0","height":"190","html":"<iframe src=\"https://hatenablog-parts.com/embed?url=https%3A%2F%2Fyoshiyuki-kitne.hatenadiary.org%2Fentry%2F20061123%2Fp1\" title=\" 2002, ApJ, 565, L71-L74 - \u5929\u6587\u5b66\u7684\u7814\u7a76\u30e1\u30e2\" class=\"embed-card embed-blogcard\" scrolling=\"no\" frameborder=\"0\" style=\"display: block; width: 100%; height: 190px; max-width: 500px; margin: 10px 0px;\"></iframe>","blog_title":"\u5929\u6587\u5b66\u7684\u7814\u7a76\u30e1\u30e2","type":"rich","provider_name":"Hatena Blog","description":"Large equivalent width Ly line emission at : young galaxies in a young universe? Malhotra et al. LALA\u30b5\u30fc\u30d9\u30a4\u3067\u306b\u304a\u3088\u305d150\u500b\u306eLAEs\u304c\u898b\u3064\u304b\u3063\u305f\u3002\u6052\u661f\u9032\u5316\u306e\u30e2\u30c7\u30eb\u304b\u3089Ly\u7b49\u4fa1\u5e45\u306e\u6700\u5927\u5024\u306f240A\u3067\u3042\u308b\u3068\u4e88\u6e2c\u3055\u308c\u3066\u3044\u308b\u304c\u3001\u672c\u7814\u7a76\u3067\u6271\u3063\u305f\u30b5\u30f3\u30d7\u30eb\u306e60%\u304c\u3053\u306e\u5024\u3092\u8d85\u3048\u305f\u3002\u89b3\u6e2c\u3055\u308c\u305f\u7b49\u4fa1\u5e45\u306e\u5206\u5e03\u3092\u3001\u3067\u306eLBGs\u306eLF\u3092\u5916\u633f\u3057\u305fstellar population\u30e2\u30c7\u30eb\u3092\u7d44\u307f\u5408\u308f\u305b\u3001\u89b3\u6e2c\u306b\u3088\u308bselection effects\u3068Malmquist bias\u3092\u8003\u616e\u3059\u308b\u3053\u3068\u3067\u518d\u73fe\u3092\u8a66\u307f\u305f\u3002\u30b5\u30f3\u30d7\u30eb\u306b\u3042\u2026","published":"2006-11-23 00:00:00","categories":["\u8ad6\u6587"],"url":"https://yoshiyuki-kitne.hatenadiary.org/entry/20061123/p1","image_url":null,"provider_url":"https://hatena.blog","author_url":"https://blog.hatena.ne.jp/yoshiyuki_kitne/"}