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pro vyhledávání: '"Palmese, A."'
Autor:
Cheng, Ting-Yun, Sánchez, H. Domínguez, Vega-Ferrero, J., Conselice, C. J., Siudek, M., Aragón-Salamanca, A., Bernardi, M., Cooke, R., Ferreira, L., Huertas-Company, M., Krywult, J., Palmese, A., Pieres, A., Malagón, A. A. Plazas, Rosell, A. Carnero, Gruen, D., Thomas, D., Bacon, D., Brooks, D., James, D. J., Hollowood, D. L., Friedel, D., Suchyta, E., Sanchez, E., Menanteau, F., Paz-Chinchón, F., Gutierrez, G., Tarle, G., Sevilla-Noarbe, I., Ferrero, I., Annis, J., Frieman, J., García-Bellido, J., Mena-Fernández, J., Honscheid, K., Kuehn, K., da Costa, L. N., Gatti, M., Raveri, M., Pereira, M. E. S., Rodriguez-Monroy, M., Smith, M., Kind, M. Carrasco, Aguena, M., Swanson, M. E. C., Weaverdyck, N., Doel, P., Miquel, R., Ogando, R. L. C., Gruendl, R. A., Allam, S., Hinton, S. R., Dodelson, S., Bocquet, S., Desai, S., Everett, S., Scarpine, V.
We compare the two largest galaxy morphology catalogues, which separate early and late type galaxies at intermediate redshift. The two catalogues were built by applying supervised deep learning (convolutional neural networks, CNNs) to the Dark Energy
Externí odkaz:
http://arxiv.org/abs/2209.06897