Update app.py
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app.py
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st.markdown("<div style='border-radius:5px;background-color:#F3F4F6;padding-top:8px;padding-bottom:8px;padding-left:14px;padding-right:14px;line-height:140%;font-size:120%'>\
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Cavity Detection Tool (CADET) is a machine learning pipeline trained to detect <b>X-ray cavities</b> from <b><em>Chandra</em></b> images of early-type galaxies, groups, and clusters. \
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To use this tool: <b>1)</b> upload your image, <b>2)</b> select the scale of interest, <b>3)</b> make a prediction, and <b>4)</b> decompose it into individual cavities
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Input images should be FITS files in units of counts, centred at the galaxy center, and point sources should be filled with surrounding background \
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(<a href='https://cxc.cfa.harvard.edu/ciao/ahelp/dmfilth.html'>dmfilth</a>). <br><br>\
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If you use this tool for your research, please cite <a href='https://arxiv.org/abs/2304.05457'>Plšek et al. 2023</a>.\
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st.markdown("<div style='border-radius:5px;background-color:#F3F4F6;padding-top:8px;padding-bottom:8px;padding-left:14px;padding-right:14px;line-height:140%;font-size:120%'>\
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Cavity Detection Tool (CADET) is a machine learning pipeline trained to detect <b>X-ray cavities</b> from <b><em>Chandra</em></b> images of early-type galaxies, groups, and clusters. \
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+
To use this tool: <b>1)</b> upload your image, <b>2)</b> select the scale of interest, <b>3)</b> make a prediction, and <b>4)</b> decompose it into individual cavities. \
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Input images should be FITS files in units of counts, centred at the galaxy center, and point sources should be filled with surrounding background \
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(<a href='https://cxc.cfa.harvard.edu/ciao/ahelp/dmfilth.html'>dmfilth</a>). <br><br>\
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If you use this tool for your research, please cite <a href='https://arxiv.org/abs/2304.05457'>Plšek et al. 2023</a>.\
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