<style> /* basic design */ /* copied from https://hackmd.io/mJ6dr_haQWmAchJEq4truw?both */ .reveal h1, .reveal h2, .reveal h3, .reveal h4, .reveal h5, .reveal h6, .reveal section, .reveal table, .reveal li, .reveal blockquote, .reveal th, .reveal td, .reveal p { font-family: 'Meiryo UI', 'Source Sans Pro', Helvetica, sans-serif, 'Helvetica Neue', 'Helvetica', 'Arial', 'Hiragino Sans', 'ヒラギノ角ゴシック', YuGothic, 'Yu Gothic'; text-align: left; line-height: 1.6; letter-spacing: normal; text-shadow: none; word-wrap: break-word; color: #444; } .reveal h1, .reveal h2, .reveal h3, .reveal h4, .reveal h5, .reveal h6 {font-weight: bold;} .reveal h1, .reveal h2, .reveal h3 {color: #2980b9;} .reveal th {background: #DDD;} .reveal section img {background:none; border:none; box-shadow:none; max-width: 95%; max-height: 95%;} .reveal blockquote {width: 90%; padding: 0.5vw 3.0vw;} .reveal table {margin: 1.0vw auto;} .reveal code {line-height: 1.2;} .reveal p, .reveal li {padding: 0vw; margin: 0vw;} .reveal .box {margin: -0.5vw 1.5vw 2.0vw -1.5vw; padding: 0.5vw 1.5vw 0.5vw 1.5vw; background: #EEE; border-radius: 1.5vw;} /* table design */ .reveal table {background: #f5f5f5;} .reveal th {background: #444; color: #fff;} .reveal td {position: relative; transition: all 300ms;} .reveal tbody:hover td { color: transparent; text-shadow: 0 0 3px #aaa;} .reveal tbody:hover tr:hover td {color: #444; text-shadow: 0 1px 0 #fff;} /* blockquote design */ .reveal blockquote { width: 90%; padding: 0.5vw 0 0.5vw 6.0vw; font-style: italic; background: #f5f5f5; } .reveal blockquote:before{ position: absolute; top: 0.1vw; left: 1vw; content: "\f10d"; font-family: FontAwesome; color: #2980b9; font-size: 3.0vw; } /* font size */ .reveal h1 {font-size: 5.0vw;} .reveal h2 {font-size: 4.0vw;} .reveal h3 {font-size: 2.8vw;} .reveal h4 {font-size: 2.6vw;} .reveal h5 {font-size: 2.4vw;} .reveal h6 {font-size: 2.2vw;} .reveal section, .reveal table, .reveal li, .reveal blockquote, .reveal th, .reveal td, .reveal p {font-size: 2.2vw;} .reveal code {font-size: 1.6vw;} /* new color */ .red {color: #EE6557;} .blue {color: #16A6B6;} /* split slide */ #right {left: -18.33%; text-align: left; float: left; width: 50%; z-index: -10;} #left {left: 31.25%; text-align: left; float: left; width: 50%; z-index: -10;} </style> # X線天文学の歴史と概要 <!-- Put the link to this slide here so people can follow --> slide: https://hackmd.io/@tenoto/S1Xgs1HNw author: 榎戸輝揚 (理化学研究所)  twitter: [teru_enoto](https://twitter.com/teru_enoto) :satellite::star: course: [高エネルギー宇宙物理学概論のメインページ](https://hackmd.io/@tenoto/HkNgkbHGv) --- ## 有効面積 (Effective Area) - X線光子を集めることのできる能力を示す - 幾何学的面積と検出効率の積 --- ## 空間分解能 (Angular resolution) - 電波天文学では回折限界に到達しており、ミラーを大きくすることが有利になる。 - X線天文学では回折限界に到達しておらず、鏡の表面精度や集光性能で空間分解能が決まる。 --- ## バックグラウンド --- ## 宇宙X線背景放射 (Cosmic X-ray Background, CXB) - $6\times 10^{-15}$ ergs/s/cm2/arcmin2 (2-10 keV) --- ## 分割 <div id="left"> <br> <iframe src="https://papers.nips.cc/paper/5346-sequence-to-sequence-learning-with-neural-networks.pdf" width="100%" frameBorder="0"></iframe> </div> <div id="right"> <br> - a - hogehoge - aaa - ... </div> --- ## test - test --- ## X線天文衛星の歴史 ```mermaid gantt dateFormat YYYY-MM-DD axisFormat %Y title History of X-ray satellites section US/NASA Uhuru: done, 1970-12-12, 1973-03-31 Einstein: done, 1978-11-13, 1981-04-17 RXTE: done, 1995-12-30, 2012-01-05 Chandra: active, 1999-07-23, 2020-12-31 Swift: active, 2004-12-20, 2020-12-31 NuSTAR: active, 2012-06-13, 2020-12-31 NICER: active, 2017-06-03, 2020-12-31 section Japan/JAXA Hakucho: done, 1979-02-21, 1985-04-15 Tenma: done, 1983-02-20, 1988-12-17 Ginga: done, 1987-02-05, 1991-11-01 ASCA: done, 1993-02-20, 2001-03-02 Suzaku: done, 2005-07-10, 2015-06-01 MAXI: active, 2009-08-13, 2020-12-31 Hitomi: done, 2016-02-17, 2016-04-28 section Europe/ESA Arial 5: done, 1974-10-15, 1980-03-14 EXOSAT: done, 1983-05-26, 1986-05-05 ROSAT: done, 1990-04-01, 1999-02-12 BeppoSAX: done, 1996-04-30, 2002-04-30 XMM-Newton: active, 1999-12-10, 2020-12-31 INTEGRAL: active, 2002-10-17, 2020-12-31 eROSITA: active, 2019-07-13, 2020-12-31 section Russia ART-XC: active, 2019-07-13, 2020-12-31 Kvant-1: done, 1987-03-31, 2001-03-23 Granat: done, 1989-12-01, 1999-05-25 section India/ISRO Astrosat: active, 2015-09-28, 2020-12-31 section China/CAS HMXT: active, 2017-06-15, 2020-12-31 ``` <br> - 主要機関のX線衛星や装置の運用期間(打ち上げ日と運用終了日)。灰色の箱は運用を終了したミッションで、青色の箱は運用中のミッションである。 --- ## Chandra X線望遠鏡 <div id="left"> ![](https://upload.wikimedia.org/wikipedia/commons/thumb/1/1a/Chandra-spacecraft_labeled-en.jpg/1920px-Chandra-spacecraft_labeled-en.jpg) (from [3. Chandra Beauty Shot](https://chandra.harvard.edu/resources/illustrations/craftIllustrations.html#craft3)) </div> <div id="right"> - 高い空間分解能を誇る宇宙X線望遠鏡 - hogehoge - aaa - ... </div> --- --- ## 分割 - このようにスライドを分割することは可能ですが,分割方法を事前にcssで定義する必要があります. <div id="left"> <br> ### left <iframe src="https://papers.nips.cc/paper/5346-sequence-to-sequence-learning-with-neural-networks.pdf" height="600px" width="100%" frameBorder="0"></iframe> </div> <div id="right"> <br> ### right - a - hogehoge - aaa - ... </div>
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