J/A+A/616/A97          SDSS QSO DR7 and DR9                   (D'Isanto+, 2018)

Return of the features. Efficient feature selection and interpretation for photometric redshifts. D'Isanto A., Cavuoti S., Gieseke F., Polsterer K.L. <Astron. Astrophys. 616, A97 (2018)> =2018A&A...616A..97D 2018A&A...616A..97D (SIMBAD/NED BibCode)
ADC_Keywords: QSOs ; Surveys Keywords: methods: data analysis - methods: statistical - galaxies: distances and redshifts - quasars: general Abstract: The explosion of data in recent years has generated an increasing need for new analysis techniques in order to extract knowledge from massive data-sets. Machine learning has proved particularly useful to perform this task. Fully automatized methods (e.g. deep neural networks) have recently gathered great popularity, even though those methods often lack physical interpretability. In contrast, feature based approaches can provide both well-performing models and understandable causalities with respect to the correlations found between features and physical processes. Efficient feature selection is an essential tool to boost the performance of machine learning models. In this work, we propose a forward selection method in order to compute, evaluate, and characterize better performing features for regression and classification problems. Given the importance of photometric redshift estimation, we adopt it as our case study. We synthetically created 4520 features by combining magnitudes, errors, radii, and ellipticities of quasars, taken from the Sloan Digital Sky Survey (SDSS). We apply a forward selection process, a recursive method in which a huge number of feature sets is tested through a k-Nearest-Neighbours algorithm, leading to a tree of feature sets. The branches of the feature tree are then used to perform experiments with the random forest, in order to validate the best set with an alternative model. We demonstrate that the sets of features determined with our approach improve the performances of the regression models significantly when compared to the performance of the classic features from the literature. The found features are unexpected and surprising, being very different from the classic features. Therefore, a method to interpret some of the found features in a physical context is presented. The feature selection methodology described here is very general and can be used to improve the performance of machine learning models for any regression or classification task. Description: The SDSS object IDs and coordinates of the extracted quasars for the three catalogues used for the experiments. The catalogue dr7a.dat contains quasars from SDSS DR7 using photometric flags in the query. The catalogue dr7b.dat is retrieved using the same query but without photometric flags. The catalogue dr7_9.dat contains quasars from DR7 and DR9, with a wider redshift distribution. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file dr7a.dat 61 83982 SDSS object IDs and coordinates of the quasars for experiment DR7a dr7b.dat 45 97041 SDSS object IDs and coordinates of the quasars for experiment DR7b dr7_9.dat 47 152137 SDSS object IDs and coordinates of the quasars for experiment DR7+9 -------------------------------------------------------------------------------- See also: II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009) V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012) VII/260 : The SDSS-DR7 quasar catalog, DR7Q (Schneider+, 2010) VII/269 : The SDSS-DR9 quasar catalog, DR9Q (Paris+, 2012) http://www.sdss.org/dr7 : SDSS DR7 home page http://www.sdss3.org/dr9 : SDSS DR9 home page Byte-by-byte Description of file: dr7a.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 A18 --- objID SDSS DR7 objID 20- 40 F21.17 deg RAdeg Right ascension (J2000.0) 42- 61 F20.16 deg DEdeg Declination (J2000.0) -------------------------------------------------------------------------------- Byte-by-byte Description of file: dr7b.dat dr7_9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 A18 --- objID SDSS DR7 objID 20- 32 F13.9 deg RAdeg Right ascension (J2000.0) 34- 47 F14.10 deg DEdeg Declination (J2000.0) -------------------------------------------------------------------------------- Acknowledgements: Antonio D'Isanto, antonio.disanto(at)h-its.org
(End) Antonio D'Isanto [HITS, Germany], Patricia Vannier [CDS] 11-May-2018
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line