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PHYSICS 366: Statistical Methods in Astrophysics

Course notes and resources for Stanford University graduate lecture course PHYSICS 366.

Course Description

This course is intended to provide an introduction to modern statistical methodology, and its applications to problems in astrophysics and cosmology, and is aimed at graduate students intending to do research in this area. We strongly encourage most first and second year students working in KIPAC to take the course. Our goal is to provide a background that will be directly relevant to the kind of problems that typical KIPAC students will encounter in their research.

Course Objectives

Our goal is that students taking this course will:

  • develop familiarity in working with various types of astronomical data.
  • understand the role of modeling in data analysis.
  • develop facility with various types of inference from data.
  • be able to critically evaluate and apply commonly used statistical methodologies.
  • be able to apply advanced statistical reasoning to problems they are likely to encounter in their research.

Information

For anyone

For Stanford students

Content

The course content can be browsed on GitHub, or you can clone the repository and run the notebooks locally. The easiest way to navigate the materials is through the links in the Schedule document.

Contact

All materials Copyright 2015, 2017, 2019 Adam Mantz and Phil Marshall, and distributed for copying and extension under the GPLv2 License, unless otherwise noted. If you have any feedback for us, please write us an issue. If you would like to help us improve this course, please do fork this repo and submit a pull request.

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Course notes and resources for Stanford University gradutate lecture course PHYS366: Special Topics in Astrophysics: Statistical Methods

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Add copy buttons to all
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}
} catch(__e) { console.warn('[Userscript:Add Copy Buttons to Code Blocks]', __e); }
})();
(function(){
try {
var __m = "github.com";
var __re = new RegExp('^' + "github\\.com" + '
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PHYSICS 366: Statistical Methods in Astrophysics

Course notes and resources for Stanford University graduate lecture course PHYSICS 366.

Course Description

This course is intended to provide an introduction to modern statistical methodology, and its applications to problems in astrophysics and cosmology, and is aimed at graduate students intending to do research in this area. We strongly encourage most first and second year students working in KIPAC to take the course. Our goal is to provide a background that will be directly relevant to the kind of problems that typical KIPAC students will encounter in their research.

Course Objectives

Our goal is that students taking this course will:

  • develop familiarity in working with various types of astronomical data.
  • understand the role of modeling in data analysis.
  • develop facility with various types of inference from data.
  • be able to critically evaluate and apply commonly used statistical methodologies.
  • be able to apply advanced statistical reasoning to problems they are likely to encounter in their research.

Information

For anyone

For Stanford students

Content

The course content can be browsed on GitHub, or you can clone the repository and run the notebooks locally. The easiest way to navigate the materials is through the links in the Schedule document.

Contact

All materials Copyright 2015, 2017, 2019 Adam Mantz and Phil Marshall, and distributed for copying and extension under the GPLv2 License, unless otherwise noted. If you have any feedback for us, please write us an issue. If you would like to help us improve this course, please do fork this repo and submit a pull request.

About

Course notes and resources for Stanford University gradutate lecture course PHYS366: Special Topics in Astrophysics: Statistical Methods

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Force GitHub README to respect dark mode\n(function() {\n var style = document.createElement('style');\n style.textContent = '\n .markdown-body {\n color-scheme: dark light;\n }\n .markdown-body pre { background: #161b22 !important; }\n .markdown-body code { background: rgba(110, 118, 129, 0.4) !important; }\n .markdown-body table th, .markdown-body table td { border-color: #30363d !important; }\n .markdown-body img { background: #0d1117; }\n .markdown-body blockquote { border-left-color: #8b949e; }\n .markdown-body hr { border-color: #30363d; }\n ';\n document.head.appendChild(style);\n})();", "GitHub Dark Mode README Fix"); } } catch(__e) { console.warn('[Userscript:GitHub Dark Mode README Fix]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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PHYSICS 366: Statistical Methods in Astrophysics

Course notes and resources for Stanford University graduate lecture course PHYSICS 366.

Course Description

This course is intended to provide an introduction to modern statistical methodology, and its applications to problems in astrophysics and cosmology, and is aimed at graduate students intending to do research in this area. We strongly encourage most first and second year students working in KIPAC to take the course. Our goal is to provide a background that will be directly relevant to the kind of problems that typical KIPAC students will encounter in their research.

Course Objectives

Our goal is that students taking this course will:

  • develop familiarity in working with various types of astronomical data.
  • understand the role of modeling in data analysis.
  • develop facility with various types of inference from data.
  • be able to critically evaluate and apply commonly used statistical methodologies.
  • be able to apply advanced statistical reasoning to problems they are likely to encounter in their research.

Information

For anyone

For Stanford students

Content

The course content can be browsed on GitHub, or you can clone the repository and run the notebooks locally. The easiest way to navigate the materials is through the links in the Schedule document.

Contact

All materials Copyright 2015, 2017, 2019 Adam Mantz and Phil Marshall, and distributed for copying and extension under the GPLv2 License, unless otherwise noted. If you have any feedback for us, please write us an issue. If you would like to help us improve this course, please do fork this repo and submit a pull request.

About

Course notes and resources for Stanford University gradutate lecture course PHYS366: Special Topics in Astrophysics: Statistical Methods

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Highlight search terms from Google/DuckDuckGo/Bing referrer\n(function() {\n var ref = document.referrer;\n var terms = [];\n \n if (ref.includes('google.com') || ref.includes('duckduckgo.com') || ref.includes('bing.com')) {\n var url = new URL(ref);\n var q = url.searchParams.get('q') || url.searchParams.get('p');\n if (q) {\n terms = q.split(/\\s+/).filter(function(t) { return t.length > 2; });\n }\n }\n \n if (terms.length === 0) return;\n \n var style = document.createElement('style');\n style.textContent = '.userscript-highlight { background: #fbbf24; color: #1a1a2e; padding: 1px 3px; border-radius: 2px; }';\n document.head.appendChild(style);\n \n function highlight(node) {\n if (node.nodeType === 3) { // text node\n var text = node.textContent;\n var found = false;\n terms.forEach(function(term) {\n var regex = new RegExp('(' + term.replace(/[.*+?^${}()|[\\]\\\\]/g, '\\\\') + ')', 'gi');\n if (regex.test(text)) {\n found = true;\n var frag = document.createDocumentFragment();\n var parts = text.split(regex);\n parts.forEach(function(part, i) {\n if (i % 2 === 0) {\n frag.appendChild(document.createTextNode(part));\n } else {\n var span = document.createElement('span');\n span.className = 'userscript-highlight';\n span.textContent = part;\n frag.appendChild(span);\n }\n });\n node.parentNode.replaceChild(frag, node);\n }\n });\n } else if (node.nodeType === 1 && node.childNodes) { // element\n var skipTags = ['SCRIPT', 'STYLE', 'NOSCRIPT', 'TEXTAREA', 'INPUT', 'SELECT'];\n if (!skipTags.includes(node.tagName)) {\n Array.from(node.childNodes).forEach(highlight);\n }\n }\n }\n \n highlight(document.body);\n \n // Re-highlight on dynamic content\n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1 || node.nodeType === 3) highlight(node);\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Highlight Search Terms"); } } catch(__e) { console.warn('[Userscript:Highlight Search Terms]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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PHYSICS 366: Statistical Methods in Astrophysics

Course notes and resources for Stanford University graduate lecture course PHYSICS 366.

Course Description

This course is intended to provide an introduction to modern statistical methodology, and its applications to problems in astrophysics and cosmology, and is aimed at graduate students intending to do research in this area. We strongly encourage most first and second year students working in KIPAC to take the course. Our goal is to provide a background that will be directly relevant to the kind of problems that typical KIPAC students will encounter in their research.

Course Objectives

Our goal is that students taking this course will:

  • develop familiarity in working with various types of astronomical data.
  • understand the role of modeling in data analysis.
  • develop facility with various types of inference from data.
  • be able to critically evaluate and apply commonly used statistical methodologies.
  • be able to apply advanced statistical reasoning to problems they are likely to encounter in their research.

Information

For anyone

For Stanford students

Content

The course content can be browsed on GitHub, or you can clone the repository and run the notebooks locally. The easiest way to navigate the materials is through the links in the Schedule document.

Contact

All materials Copyright 2015, 2017, 2019 Adam Mantz and Phil Marshall, and distributed for copying and extension under the GPLv2 License, unless otherwise noted. If you have any feedback for us, please write us an issue. If you would like to help us improve this course, please do fork this repo and submit a pull request.

About

Course notes and resources for Stanford University gradutate lecture course PHYS366: Special Topics in Astrophysics: Statistical Methods

Resources

Stars

2 stars

Watchers

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Strip utm_, fbclid, gclid, etc. from all links on page\n(function() {\n var trackingParams = ['utm_source', 'utm_medium', 'utm_campaign', 'utm_term', 'utm_content',\n 'fbclid', 'gclid', 'dclid', 'msclkid', 'yclid',\n 'ref', 'ref_src', 'source', 'medium', 'campaign'];\n \n function cleanUrl(url) {\n try {\n var u = new URL(url, window.location.origin);\n var changed = false;\n trackingParams.forEach(function(p) {\n if (u.searchParams.has(p)) {\n u.searchParams.delete(p);\n changed = true;\n }\n });\n return changed ? u.toString() : url;\n } catch (e) {\n return url;\n }\n }\n \n function cleanLinks() {\n document.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n \n cleanLinks();\n \n var observer = new MutationObserver(function(mutations) {\n mutations.forEach(function(m) {\n m.addedNodes.forEach(function(node) {\n if (node.nodeType === 1) {\n if (node.tagName === 'A') cleanLinks();\n node.querySelectorAll('a[href]').forEach(function(a) {\n var clean = cleanUrl(a.href);\n if (clean !== a.href) a.href = clean;\n });\n }\n });\n });\n });\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Remove Tracking Parameters from Links"); } } catch(__e) { console.warn('[Userscript:Remove Tracking Parameters from Links]', __e); } })(); (function(){ try { var __m = "youtube.com"; var __re = new RegExp('^' + "youtube\\.com" + '
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PHYSICS 366: Statistical Methods in Astrophysics

Course notes and resources for Stanford University graduate lecture course PHYSICS 366.

Course Description

This course is intended to provide an introduction to modern statistical methodology, and its applications to problems in astrophysics and cosmology, and is aimed at graduate students intending to do research in this area. We strongly encourage most first and second year students working in KIPAC to take the course. Our goal is to provide a background that will be directly relevant to the kind of problems that typical KIPAC students will encounter in their research.

Course Objectives

Our goal is that students taking this course will:

  • develop familiarity in working with various types of astronomical data.
  • understand the role of modeling in data analysis.
  • develop facility with various types of inference from data.
  • be able to critically evaluate and apply commonly used statistical methodologies.
  • be able to apply advanced statistical reasoning to problems they are likely to encounter in their research.

Information

For anyone

For Stanford students

Content

The course content can be browsed on GitHub, or you can clone the repository and run the notebooks locally. The easiest way to navigate the materials is through the links in the Schedule document.

Contact

All materials Copyright 2015, 2017, 2019 Adam Mantz and Phil Marshall, and distributed for copying and extension under the GPLv2 License, unless otherwise noted. If you have any feedback for us, please write us an issue. If you would like to help us improve this course, please do fork this repo and submit a pull request.

About

Course notes and resources for Stanford University gradutate lecture course PHYS366: Special Topics in Astrophysics: Statistical Methods

Resources

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Auto-enable theater mode on YouTube\n(function() {\n function tryTheater() {\n var btn = document.querySelector('button[aria-label=\"Theater mode\"], ytd-player #player button[title=\"Theater mode\"]');\n if (btn && !btn.classList.contains('activated')) {\n btn.click();\n }\n }\n \n // Try immediately\n tryTheater();\n \n // Try after navigation (SPA)\n var lastUrl = location.href;\n setInterval(function() {\n if (location.href !== lastUrl) {\n lastUrl = location.href;\n setTimeout(tryTheater, 500);\n }\n }, 1000);\n \n // Also try on player load\n var observer = new MutationObserver(tryTheater);\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "YouTube Theater Mode Default"); } } catch(__e) { console.warn('[Userscript:YouTube Theater Mode Default]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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PHYSICS 366: Statistical Methods in Astrophysics

Course notes and resources for Stanford University graduate lecture course PHYSICS 366.

Course Description

This course is intended to provide an introduction to modern statistical methodology, and its applications to problems in astrophysics and cosmology, and is aimed at graduate students intending to do research in this area. We strongly encourage most first and second year students working in KIPAC to take the course. Our goal is to provide a background that will be directly relevant to the kind of problems that typical KIPAC students will encounter in their research.

Course Objectives

Our goal is that students taking this course will:

  • develop familiarity in working with various types of astronomical data.
  • understand the role of modeling in data analysis.
  • develop facility with various types of inference from data.
  • be able to critically evaluate and apply commonly used statistical methodologies.
  • be able to apply advanced statistical reasoning to problems they are likely to encounter in their research.

Information

For anyone

For Stanford students

Content

The course content can be browsed on GitHub, or you can clone the repository and run the notebooks locally. The easiest way to navigate the materials is through the links in the Schedule document.

Contact

All materials Copyright 2015, 2017, 2019 Adam Mantz and Phil Marshall, and distributed for copying and extension under the GPLv2 License, unless otherwise noted. If you have any feedback for us, please write us an issue. If you would like to help us improve this course, please do fork this repo and submit a pull request.

About

Course notes and resources for Stanford University gradutate lecture course PHYS366: Special Topics in Astrophysics: Statistical Methods

Resources

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Remove or un-stick sticky/fixed headers that block content\n(function() {\n function unstick() {\n document.querySelectorAll('header, nav, [role=\"banner\"], .header, .navbar, .sticky, .fixed-top, [style*=\"position: fixed\"], [style*=\"position:sticky\"]').forEach(function(el) {\n if (el.style.position === 'fixed' || el.style.position === 'sticky' || \n getComputedStyle(el).position === 'fixed' || getComputedStyle(el).position === 'sticky') {\n el.style.position = 'static';\n el.style.top = 'auto';\n el.style.zIndex = 'auto';\n }\n });\n }\n \n unstick();\n \n var observer = new MutationObserver(unstick);\n observer.observe(document.body, { childList: true, subtree: true, attributes: true, attributeFilter: ['style', 'class'] });\n})();", "Kill Sticky Headers"); } } catch(__e) { console.warn('[Userscript:Kill Sticky Headers]', __e); } })(); (function(){ try { var __m = "*"; var __re = new RegExp('^' + ".*" + '
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PHYSICS 366: Statistical Methods in Astrophysics

Course notes and resources for Stanford University graduate lecture course PHYSICS 366.

Course Description

This course is intended to provide an introduction to modern statistical methodology, and its applications to problems in astrophysics and cosmology, and is aimed at graduate students intending to do research in this area. We strongly encourage most first and second year students working in KIPAC to take the course. Our goal is to provide a background that will be directly relevant to the kind of problems that typical KIPAC students will encounter in their research.

Course Objectives

Our goal is that students taking this course will:

  • develop familiarity in working with various types of astronomical data.
  • understand the role of modeling in data analysis.
  • develop facility with various types of inference from data.
  • be able to critically evaluate and apply commonly used statistical methodologies.
  • be able to apply advanced statistical reasoning to problems they are likely to encounter in their research.

Information

For anyone

For Stanford students

Content

The course content can be browsed on GitHub, or you can clone the repository and run the notebooks locally. The easiest way to navigate the materials is through the links in the Schedule document.

Contact

All materials Copyright 2015, 2017, 2019 Adam Mantz and Phil Marshall, and distributed for copying and extension under the GPLv2 License, unless otherwise noted. If you have any feedback for us, please write us an issue. If you would like to help us improve this course, please do fork this repo and submit a pull request.

About

Course notes and resources for Stanford University gradutate lecture course PHYS366: Special Topics in Astrophysics: Statistical Methods

Resources

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Universal Dark Mode - works on any site\n(function() {\n var enabled = true;\n \n function applyDarkMode() {\n if (!enabled) return;\n \n // Create style element if it doesn't exist\n var style = document.getElementById('universal-dark-mode-style');\n if (!style) {\n style = document.createElement('style');\n style.id = 'universal-dark-mode-style';\n document.head.appendChild(style);\n }\n \n // Dark mode CSS - inverts colors but preserves images/video\n style.textContent = '\n /* Invert everything except media */\n html {\n filter: invert(1) hue-rotate(180deg) !important;\n background: #1a1a2e !important;\n }\n \n /* Restore images, videos, iframes, canvas */\n img, video, iframe, canvas, svg, picture, [style*=\"background-image\"] {\n filter: invert(1) hue-rotate(180deg) !important;\n }\n \n /* Preserve specific elements that should not be inverted */\n .no-dark-mode, .no-dark-mode *,\n [data-theme=\"light\"], [data-theme=\"light\"],\n .ace_editor, .ace_editor *,\n .CodeMirror, .CodeMirror *,\n .monaco-editor, .monaco-editor *,\n .markdown-body pre, .markdown-body pre *,\n .highlight, .highlight *,\n pre code, pre code * {\n filter: none !important;\n }\n \n /* Fix common UI elements */\n .modal, .popup, .dropdown-menu, .tooltip, .popover {\n filter: invert(1) hue-rotate(180deg) !important;\n background: #2d2d44 !important;\n border-color: #444 !important;\n }\n \n /* Scrollbars */\n ::-webkit-scrollbar { background: #1a1a2e !important; }\n ::-webkit-scrollbar-thumb { background: #444 !important; }\n ::-webkit-scrollbar-thumb:hover { background: #555 !important; }\n \n /* Selection */\n ::selection { background: #4ecdc4 !important; color: #1a1a2e !important; }\n ::-moz-selection { background: #4ecdc4 !important; color: #1a1a2e !important; }\n ';\n }\n \n function removeDarkMode() {\n var style = document.getElementById('universal-dark-mode-style');\n if (style) style.remove();\n }\n \n // Toggle with Alt+Shift+D\n document.addEventListener('keydown', function(e) {\n if (e.altKey && e.shiftKey && e.key === 'D') {\n e.preventDefault();\n enabled = !enabled;\n if (enabled) {\n applyDarkMode();\n console.log('[Universal Dark Mode] Enabled');\n } else {\n removeDarkMode();\n console.log('[Universal Dark Mode] Disabled');\n }\n }\n });\n \n // Apply on load\n applyDarkMode();\n \n // Re-apply on dynamic content\n var observer = new MutationObserver(function(mutations) {\n if (enabled && !document.getElementById('universal-dark-mode-style')) {\n applyDarkMode();\n }\n });\n observer.observe(document.head, { childList: true });\n \n console.log('[Universal Dark Mode] Loaded - Press Alt+Shift+D to toggle');\n})();", "Universal Dark Mode"); } } catch(__e) { console.warn('[Userscript:Universal Dark Mode]', __e); } })(); })();
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PHYSICS 366: Statistical Methods in Astrophysics

Course notes and resources for Stanford University graduate lecture course PHYSICS 366.

Course Description

This course is intended to provide an introduction to modern statistical methodology, and its applications to problems in astrophysics and cosmology, and is aimed at graduate students intending to do research in this area. We strongly encourage most first and second year students working in KIPAC to take the course. Our goal is to provide a background that will be directly relevant to the kind of problems that typical KIPAC students will encounter in their research.

Course Objectives

Our goal is that students taking this course will:

  • develop familiarity in working with various types of astronomical data.
  • understand the role of modeling in data analysis.
  • develop facility with various types of inference from data.
  • be able to critically evaluate and apply commonly used statistical methodologies.
  • be able to apply advanced statistical reasoning to problems they are likely to encounter in their research.

Information

For anyone

For Stanford students

Content

The course content can be browsed on GitHub, or you can clone the repository and run the notebooks locally. The easiest way to navigate the materials is through the links in the Schedule document.

Contact

All materials Copyright 2015, 2017, 2019 Adam Mantz and Phil Marshall, and distributed for copying and extension under the GPLv2 License, unless otherwise noted. If you have any feedback for us, please write us an issue. If you would like to help us improve this course, please do fork this repo and submit a pull request.

About

Course notes and resources for Stanford University gradutate lecture course PHYS366: Special Topics in Astrophysics: Statistical Methods

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