TY - GEN
T1 - Analyzing and Processing of Astronomical Images using Deep Learning Techniques
AU - Vy, Sandeep
AU - Sen, Snigdha
AU - Santosh, K.
N1 - Publisher Copyright:
© 2021 IEEE.
PY - 2021
Y1 - 2021
N2 - Deep Learning techniques are widely used in various use cases like image detection, pattern recognition, computer vision, and prediction, etc. These days, Convolutional neural networks(CNN) which is an efficient algorithm of Deep Learning are also extensively used in astronomical image processing. In this work, we implemented different architectural models like AlexNet, VGG16, ResNe50, InceptionV3,Xception to classify and predict the Redshift(z) values of unlabeled galaxy images taken from the EFIGI catalog and galaxy-zoo image dataset from the Kaggle website. In addition to these pre-built architectural models, we have introduced a novel, customized CNN classifier and Redshift(z) predictor models to study the behavior of CNN layers and to achieve reasonable accuracy by fine-tuning hyperparameters. Our customized CNN Classifier model achieved a considerably good accuracy of 92.3% with 87.3% validation loss in galaxy classification. Whereas in Redshift(z) prediction, our novel CNN Redshift(z) predictor model achieved a very low loss of 0.000158 when compared to other pre-built architectures.
AB - Deep Learning techniques are widely used in various use cases like image detection, pattern recognition, computer vision, and prediction, etc. These days, Convolutional neural networks(CNN) which is an efficient algorithm of Deep Learning are also extensively used in astronomical image processing. In this work, we implemented different architectural models like AlexNet, VGG16, ResNe50, InceptionV3,Xception to classify and predict the Redshift(z) values of unlabeled galaxy images taken from the EFIGI catalog and galaxy-zoo image dataset from the Kaggle website. In addition to these pre-built architectural models, we have introduced a novel, customized CNN classifier and Redshift(z) predictor models to study the behavior of CNN layers and to achieve reasonable accuracy by fine-tuning hyperparameters. Our customized CNN Classifier model achieved a considerably good accuracy of 92.3% with 87.3% validation loss in galaxy classification. Whereas in Redshift(z) prediction, our novel CNN Redshift(z) predictor model achieved a very low loss of 0.000158 when compared to other pre-built architectures.
UR - https://www.scopus.com/pages/publications/85123359906
UR - https://www.scopus.com/inward/citedby.url?scp=85123359906&partnerID=8YFLogxK
U2 - 10.1109/CONECCT52877.2021.9622583
DO - 10.1109/CONECCT52877.2021.9622583
M3 - Conference contribution
AN - SCOPUS:85123359906
T3 - Proceedings of CONECCT 2021: 7th IEEE International Conference on Electronics, Computing and Communication Technologies
BT - Proceedings of CONECCT 2021
PB - Institute of Electrical and Electronics Engineers Inc.
T2 - 7th IEEE International Conference on Electronics, Computing and Communication Technologies, CONECCT 2021
Y2 - 9 July 2021 through 11 July 2021
ER -