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astropyLicense: MIT

teb: Temperatures for Eclipsing Binary stars

teb is a Python package that calculates fundamental effective temperatures for solar-type stars in eclipsing binary systems using photometry, Gaia parallax and radii. The full method is described in Miller, Maxted & Smalley (2020).

Installation

Clone the repository:

$ git clone https://github.com/nmiller95/teb.git

Then use pip to install the requirements.txt file

$ python3 -m pip install -r requirements.txt

teb was developed in Python 3.7.

Usage

Set up the data file for your star

 python3 teb.py --make-file [star_name]

where [star_name] is a name resolvable by SIMBAD or the coordinates of the star in the form "Jhhhmmmss.s+ddmmss.s". The output file config/[star_name].yaml can be re-named to a more convenient name for the star once it is created.

See ..

 python3 teb.py --help

.. for help with this step.

Add / adjust observed data for your star in the resulting file config/[star_name].yaml

Set the star name and other parameters for the analysis in config/config.yaml

Then run your analysis using

 python3 teb.py

Use the python scripts in the folder "scripts" for plotting your results, and to generate output LaTeX tables.

See the usage instructions in calspec.py if you need to use new filters not already included in cache/fps. The file calspec/calspec_lovar.csv can be used with the multi-cone VO service in topcat to collect photometric data for this sample CALSPEC stars excluding those with known variability > 0.5%. (topcat - https://www.star.bristol.ac.uk/mbt/topcat/)

To add filters used for flux ratio measurements only, use calspec.py with the option "-n".

For further details, see the built-in help for calspec:

 python3 calspec.py --help

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

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, 'i'); if (__m === '*' || __re.test(location.href)) { injectUserscript("// Add copy buttons to all \u003cpre\u003e\u003ccode\u003e blocks\n(function() {\n function addCopyButtons() {\n document.querySelectorAll('pre code').forEach(function(codeBlock) {\n if (codeBlock.parentElement.hasAttribute('data-copy-added')) return;\n codeBlock.parentElement.setAttribute('data-copy-added', 'true');\n \n var btn = document.createElement('button');\n btn.textContent = 'Copy';\n btn.style.cssText = 'position:absolute;top:4px;right:4px;padding:2px 8px;font-size:11px;background:#4ecdc4;border:none;border-radius:4px;color:#1a1a2e;cursor:pointer;opacity:0.7;transition:opacity 0.2s;';\n btn.onmouseover = function() { this.style.opacity = '1'; };\n btn.onmouseout = function() { this.style.opacity = '0.7'; };\n btn.onclick = function() {\n navigator.clipboard.writeText(codeBlock.textContent).then(function() {\n btn.textContent = 'Copied!';\n setTimeout(function() { btn.textContent = 'Copy'; }, 1500);\n });\n };\n codeBlock.parentElement.style.position = 'relative';\n codeBlock.parentElement.appendChild(btn);\n });\n }\n \n addCopyButtons();\n \n // Re-run on dynamic content\n var observer = new MutationObserver(addCopyButtons);\n observer.observe(document.body, { childList: true, subtree: true });\n})();", "Add Copy Buttons to Code Blocks"); } } 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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astropyLicense: MIT

teb: Temperatures for Eclipsing Binary stars

teb is a Python package that calculates fundamental effective temperatures for solar-type stars in eclipsing binary systems using photometry, Gaia parallax and radii. The full method is described in Miller, Maxted & Smalley (2020).

Installation

Clone the repository:

$ git clone https://github.com/nmiller95/teb.git

Then use pip to install the requirements.txt file

$ python3 -m pip install -r requirements.txt

teb was developed in Python 3.7.

Usage

Set up the data file for your star

 python3 teb.py --make-file [star_name]

where [star_name] is a name resolvable by SIMBAD or the coordinates of the star in the form "Jhhhmmmss.s+ddmmss.s". The output file config/[star_name].yaml can be re-named to a more convenient name for the star once it is created.

See ..

 python3 teb.py --help

.. for help with this step.

Add / adjust observed data for your star in the resulting file config/[star_name].yaml

Set the star name and other parameters for the analysis in config/config.yaml

Then run your analysis using

 python3 teb.py

Use the python scripts in the folder "scripts" for plotting your results, and to generate output LaTeX tables.

See the usage instructions in calspec.py if you need to use new filters not already included in cache/fps. The file calspec/calspec_lovar.csv can be used with the multi-cone VO service in topcat to collect photometric data for this sample CALSPEC stars excluding those with known variability > 0.5%. (topcat - https://www.star.bristol.ac.uk/mbt/topcat/)

To add filters used for flux ratio measurements only, use calspec.py with the option "-n".

For further details, see the built-in help for calspec:

 python3 calspec.py --help

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

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Temperatures of Eclipsing Binary stars (TEB)

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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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astropyLicense: MIT

teb: Temperatures for Eclipsing Binary stars

teb is a Python package that calculates fundamental effective temperatures for solar-type stars in eclipsing binary systems using photometry, Gaia parallax and radii. The full method is described in Miller, Maxted & Smalley (2020).

Installation

Clone the repository:

$ git clone https://github.com/nmiller95/teb.git

Then use pip to install the requirements.txt file

$ python3 -m pip install -r requirements.txt

teb was developed in Python 3.7.

Usage

Set up the data file for your star

 python3 teb.py --make-file [star_name]

where [star_name] is a name resolvable by SIMBAD or the coordinates of the star in the form "Jhhhmmmss.s+ddmmss.s". The output file config/[star_name].yaml can be re-named to a more convenient name for the star once it is created.

See ..

 python3 teb.py --help

.. for help with this step.

Add / adjust observed data for your star in the resulting file config/[star_name].yaml

Set the star name and other parameters for the analysis in config/config.yaml

Then run your analysis using

 python3 teb.py

Use the python scripts in the folder "scripts" for plotting your results, and to generate output LaTeX tables.

See the usage instructions in calspec.py if you need to use new filters not already included in cache/fps. The file calspec/calspec_lovar.csv can be used with the multi-cone VO service in topcat to collect photometric data for this sample CALSPEC stars excluding those with known variability > 0.5%. (topcat - https://www.star.bristol.ac.uk/mbt/topcat/)

To add filters used for flux ratio measurements only, use calspec.py with the option "-n".

For further details, see the built-in help for calspec:

 python3 calspec.py --help

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

About

Temperatures of Eclipsing Binary stars (TEB)

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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 \u003e 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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astropyLicense: MIT

teb: Temperatures for Eclipsing Binary stars

teb is a Python package that calculates fundamental effective temperatures for solar-type stars in eclipsing binary systems using photometry, Gaia parallax and radii. The full method is described in Miller, Maxted & Smalley (2020).

Installation

Clone the repository:

$ git clone https://github.com/nmiller95/teb.git

Then use pip to install the requirements.txt file

$ python3 -m pip install -r requirements.txt

teb was developed in Python 3.7.

Usage

Set up the data file for your star

 python3 teb.py --make-file [star_name]

where [star_name] is a name resolvable by SIMBAD or the coordinates of the star in the form "Jhhhmmmss.s+ddmmss.s". The output file config/[star_name].yaml can be re-named to a more convenient name for the star once it is created.

See ..

 python3 teb.py --help

.. for help with this step.

Add / adjust observed data for your star in the resulting file config/[star_name].yaml

Set the star name and other parameters for the analysis in config/config.yaml

Then run your analysis using

 python3 teb.py

Use the python scripts in the folder "scripts" for plotting your results, and to generate output LaTeX tables.

See the usage instructions in calspec.py if you need to use new filters not already included in cache/fps. The file calspec/calspec_lovar.csv can be used with the multi-cone VO service in topcat to collect photometric data for this sample CALSPEC stars excluding those with known variability > 0.5%. (topcat - https://www.star.bristol.ac.uk/mbt/topcat/)

To add filters used for flux ratio measurements only, use calspec.py with the option "-n".

For further details, see the built-in help for calspec:

 python3 calspec.py --help

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

About

Temperatures of Eclipsing Binary stars (TEB)

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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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astropyLicense: MIT

teb: Temperatures for Eclipsing Binary stars

teb is a Python package that calculates fundamental effective temperatures for solar-type stars in eclipsing binary systems using photometry, Gaia parallax and radii. The full method is described in Miller, Maxted & Smalley (2020).

Installation

Clone the repository:

$ git clone https://github.com/nmiller95/teb.git

Then use pip to install the requirements.txt file

$ python3 -m pip install -r requirements.txt

teb was developed in Python 3.7.

Usage

Set up the data file for your star

 python3 teb.py --make-file [star_name]

where [star_name] is a name resolvable by SIMBAD or the coordinates of the star in the form "Jhhhmmmss.s+ddmmss.s". The output file config/[star_name].yaml can be re-named to a more convenient name for the star once it is created.

See ..

 python3 teb.py --help

.. for help with this step.

Add / adjust observed data for your star in the resulting file config/[star_name].yaml

Set the star name and other parameters for the analysis in config/config.yaml

Then run your analysis using

 python3 teb.py

Use the python scripts in the folder "scripts" for plotting your results, and to generate output LaTeX tables.

See the usage instructions in calspec.py if you need to use new filters not already included in cache/fps. The file calspec/calspec_lovar.csv can be used with the multi-cone VO service in topcat to collect photometric data for this sample CALSPEC stars excluding those with known variability > 0.5%. (topcat - https://www.star.bristol.ac.uk/mbt/topcat/)

To add filters used for flux ratio measurements only, use calspec.py with the option "-n".

For further details, see the built-in help for calspec:

 python3 calspec.py --help

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

About

Temperatures of Eclipsing Binary stars (TEB)

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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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astropyLicense: MIT

teb: Temperatures for Eclipsing Binary stars

teb is a Python package that calculates fundamental effective temperatures for solar-type stars in eclipsing binary systems using photometry, Gaia parallax and radii. The full method is described in Miller, Maxted & Smalley (2020).

Installation

Clone the repository:

$ git clone https://github.com/nmiller95/teb.git

Then use pip to install the requirements.txt file

$ python3 -m pip install -r requirements.txt

teb was developed in Python 3.7.

Usage

Set up the data file for your star

 python3 teb.py --make-file [star_name]

where [star_name] is a name resolvable by SIMBAD or the coordinates of the star in the form "Jhhhmmmss.s+ddmmss.s". The output file config/[star_name].yaml can be re-named to a more convenient name for the star once it is created.

See ..

 python3 teb.py --help

.. for help with this step.

Add / adjust observed data for your star in the resulting file config/[star_name].yaml

Set the star name and other parameters for the analysis in config/config.yaml

Then run your analysis using

 python3 teb.py

Use the python scripts in the folder "scripts" for plotting your results, and to generate output LaTeX tables.

See the usage instructions in calspec.py if you need to use new filters not already included in cache/fps. The file calspec/calspec_lovar.csv can be used with the multi-cone VO service in topcat to collect photometric data for this sample CALSPEC stars excluding those with known variability > 0.5%. (topcat - https://www.star.bristol.ac.uk/mbt/topcat/)

To add filters used for flux ratio measurements only, use calspec.py with the option "-n".

For further details, see the built-in help for calspec:

 python3 calspec.py --help

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

About

Temperatures of Eclipsing Binary stars (TEB)

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Readme
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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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astropyLicense: MIT

teb: Temperatures for Eclipsing Binary stars

teb is a Python package that calculates fundamental effective temperatures for solar-type stars in eclipsing binary systems using photometry, Gaia parallax and radii. The full method is described in Miller, Maxted & Smalley (2020).

Installation

Clone the repository:

$ git clone https://github.com/nmiller95/teb.git

Then use pip to install the requirements.txt file

$ python3 -m pip install -r requirements.txt

teb was developed in Python 3.7.

Usage

Set up the data file for your star

 python3 teb.py --make-file [star_name]

where [star_name] is a name resolvable by SIMBAD or the coordinates of the star in the form "Jhhhmmmss.s+ddmmss.s". The output file config/[star_name].yaml can be re-named to a more convenient name for the star once it is created.

See ..

 python3 teb.py --help

.. for help with this step.

Add / adjust observed data for your star in the resulting file config/[star_name].yaml

Set the star name and other parameters for the analysis in config/config.yaml

Then run your analysis using

 python3 teb.py

Use the python scripts in the folder "scripts" for plotting your results, and to generate output LaTeX tables.

See the usage instructions in calspec.py if you need to use new filters not already included in cache/fps. The file calspec/calspec_lovar.csv can be used with the multi-cone VO service in topcat to collect photometric data for this sample CALSPEC stars excluding those with known variability > 0.5%. (topcat - https://www.star.bristol.ac.uk/mbt/topcat/)

To add filters used for flux ratio measurements only, use calspec.py with the option "-n".

For further details, see the built-in help for calspec:

 python3 calspec.py --help

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

About

Temperatures of Eclipsing Binary stars (TEB)

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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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astropyLicense: MIT

teb: Temperatures for Eclipsing Binary stars

teb is a Python package that calculates fundamental effective temperatures for solar-type stars in eclipsing binary systems using photometry, Gaia parallax and radii. The full method is described in Miller, Maxted & Smalley (2020).

Installation

Clone the repository:

$ git clone https://github.com/nmiller95/teb.git

Then use pip to install the requirements.txt file

$ python3 -m pip install -r requirements.txt

teb was developed in Python 3.7.

Usage

Set up the data file for your star

 python3 teb.py --make-file [star_name]

where [star_name] is a name resolvable by SIMBAD or the coordinates of the star in the form "Jhhhmmmss.s+ddmmss.s". The output file config/[star_name].yaml can be re-named to a more convenient name for the star once it is created.

See ..

 python3 teb.py --help

.. for help with this step.

Add / adjust observed data for your star in the resulting file config/[star_name].yaml

Set the star name and other parameters for the analysis in config/config.yaml

Then run your analysis using

 python3 teb.py

Use the python scripts in the folder "scripts" for plotting your results, and to generate output LaTeX tables.

See the usage instructions in calspec.py if you need to use new filters not already included in cache/fps. The file calspec/calspec_lovar.csv can be used with the multi-cone VO service in topcat to collect photometric data for this sample CALSPEC stars excluding those with known variability > 0.5%. (topcat - https://www.star.bristol.ac.uk/mbt/topcat/)

To add filters used for flux ratio measurements only, use calspec.py with the option "-n".

For further details, see the built-in help for calspec:

 python3 calspec.py --help

Contributing

Pull requests are welcome. For major changes, please open an issue first to discuss what you would like to change.

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Temperatures of Eclipsing Binary stars (TEB)

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