What is it about?
The need for accurate photometric redshifts estimation is a topic that has fundamental importance in Astronomy, due to the necessity of efficiently obtaining redshift information without the need of spectroscopic analysis. We propose a method for determining accurate multimodal photo-z probability density functions (PDFs) using Mixture Density Networks (MDN) and Deep Convolutional Networks (DCN). A comparison with a Random Forest (RF) is performed.
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Why is it important?
New approach for photometric redshift estimation, through the direct use of images via deep learning, in a full probabilistic way.
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This page is a summary of: Uncertain Photometric Redshifts with Deep Learning Methods, Proceedings of the International Astronomical Union, October 2016, Cambridge University Press,
DOI: 10.1017/s1743921316013090.
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