Wide Field Imaging. I. Applications of Neural Networks to object detection and star/galaxy classification
arXiv:astro-ph/0006115 · doi:10.1046/j.1365-8711.2000.03700.x
Abstract
[Abriged] Astronomical Wide Field Imaging performed with new large format CCD detectors poses data reduction problems of unprecedented scale which are difficult to deal with traditional interactive tools. We present here NExt (Neural Extractor): a new Neural Network (NN) based package capable to detect objects and to perform both deblending and star/galaxy classification in an automatic way. Traditionally, in astronomical images, objects are first discriminated from the noisy background by searching for sets of connected pixels having brightnesses above a given threshold and then they are classified as stars or as galaxies through diagnostic diagrams having variables choosen accordingly to the astronomer's taste and experience. In the extraction step, assuming that images are well sampled, NExt requires only the simplest a priori definition of "what an object is" (id est, it keeps all structures composed by more than one pixels) and performs the detection via an unsupervised NN approaching detection as a clustering problem which has been thoroughly studied in the artificial intelligence literature. In order to obtain an objective and reliable classification, instead of using an arbitrarily defined set of features, we use a NN to select the most significant features among the large number of measured ones, and then we use their selected features to perform the classification task. In order to optimise the performances of the system we implemented and tested several different models of NN. The comparison of the NExt performances with those of the best detection and classification package known to the authors (SExtractor) shows that NExt is at least as effective as the best traditional packages.
MNRAS, in press. Paper with higher resolution images is available at http://www.na.astro.it/~andreon/listapub.html
References in corpus (1)
Cited by in corpus (37)
- ANNz: estimating photometric redshifts using artificial neural networks
- Data Mining and Machine Learning in Astronomy
- Estimating photometric redshifts with artificial neural networks
- Galaxy Types in the Sloan Digital Sky Survey Using Supervised Artificial Neural Networks
- SKYNET: an efficient and robust neural network training tool for machine learning in astronomy
- The DAWES review 10: The impact of deep learning for the analysis of galaxy surveys
- Deblending and Classifying Astronomical Sources with Mask R-CNN Deep Learning
- Astronomia ex machina: a history, primer, and outlook on neural networks in astronomy
- An Artificial Neural Network Approach For Ranking Quenching Parameters In Central Galaxies
- Neural Networks and Photometric Redshifts
- Automated Galaxy Morphology: A Fourier Approach
- Lightcurve Classification in Massive Variability Surveys
- Comparison of source detection procedures for XMM-Newton images
- Deblending galaxy superpositions with branched generative adversarial networks
- Automated Clustering Algorithms for Classification of Astronomical Objects
- A review of unsupervised learning in astronomy
- A difference boosting neural network for automated star-galaxy classification
- Decoding spectral energy distributions of dust-obscured starburst-AGN
- The infra-red luminosities of ~332,000 SDSS galaxies predicted from artificial neural networks and the Herschel Stripe 82 survey
- Detection, Instance Segmentation, and Classification for Astronomical Surveys with Deep Learning (DeepDISC): Detectron2 Implementation and Demonstration with Hyper Suprime-Cam Data
- A nanoflare model for active region radiance: application of artificial neural networks
- A Bayesian approach to star-galaxy classification
- Large-scale density and velocity field reconstructions with neural networks
- Machine learning applied to proton radiography
- Mathematical Morphology: Star/Galaxy Differentiation & Galaxy Morphology Classification
- Applying Machine Learning to Catalogue Matching in Astrophysics
- Classifying galaxy spectra at 0.5<z<1 with self-organizing maps
- Crowded Cluster Cores: Algorithms for Deblending in Dark Energy Survey Images
- ASPECT: A spectra clustering tool for exploration of large spectral surveys
- Scientific Data Mining in Astronomy
- Artificial neural network based calibrations for the prediction of galactic [NII] 6584 and H line luminosities
- A machine learning approach for identifying the counterparts of submillimetre galaxies and applications to the GOODS-North field
- Artificial Neural Networks for cosmic gamma-ray propagation in the Universe
- A comparative study of source-finding techniques in HI emission line cubes using SoFiA, MTObjects, and supervised deep learning
- The Transient Optical Sky Survey Data Pipeline
- Neural networks as a tool for parameter estimation in astrophysical data
- Application of Neural Networks to the study of stellar model solutions