In the last decade a new generation of telescopes and sensors has allowed the production of a very large amount of data and astronomy has become a data-rich science. New automatic methods largely based on machine learning are needed to cope with such data tsunami. We present some results in the fields of photometric redshifts and galaxy classification, obtained using the MLPQNA algorithm available in the DAMEWARE (Data Mining and Web Application Resource) for the SDSS galaxies (DR9 and DR10). We present PhotoRApToR (Photometric Research Application To Redshift): a Java based desktop application capable to solve regression and classification problems and specialized for photo-z estimation.

Data-Rich Astronomy: Mining Sky Surveys with PhotoRApToR / Cavuoti, Stefano; Brescia, Massimo; Longo, Giuseppe. - 306:(2015), pp. 307-309. (Intervento presentato al convegno Statistical Challenges in 21st Century Cosmology tenutosi a Lisbona nel Maggio 2014) [10.1017/S1743921314013416].

Data-Rich Astronomy: Mining Sky Surveys with PhotoRApToR

Massimo Brescia;Giuseppe Longo
2015

Abstract

In the last decade a new generation of telescopes and sensors has allowed the production of a very large amount of data and astronomy has become a data-rich science. New automatic methods largely based on machine learning are needed to cope with such data tsunami. We present some results in the fields of photometric redshifts and galaxy classification, obtained using the MLPQNA algorithm available in the DAMEWARE (Data Mining and Web Application Resource) for the SDSS galaxies (DR9 and DR10). We present PhotoRApToR (Photometric Research Application To Redshift): a Java based desktop application capable to solve regression and classification problems and specialized for photo-z estimation.
2015
Data-Rich Astronomy: Mining Sky Surveys with PhotoRApToR / Cavuoti, Stefano; Brescia, Massimo; Longo, Giuseppe. - 306:(2015), pp. 307-309. (Intervento presentato al convegno Statistical Challenges in 21st Century Cosmology tenutosi a Lisbona nel Maggio 2014) [10.1017/S1743921314013416].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/900719
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