Details

Autor(en) / Beteiligte

• Vega-Ferrero, J
• Domínguez Sánchez, H
• Bernardi, M
• Huertas-Company, M
• Morgan, R
• Margalef, B
• Aguena, M
• Allam, S
• Annis, J
• Avila, S
• Bacon, D
• Bertin, E
• Brooks, D
• Carnero Rosell, A
• Carrasco Kind, M
• Carretero, J
• Choi, A
• Conselice, C
• Costanzi, M
• da Costa, L N
• Pereira, M E S
• De Vicente, J
• Desai, S
• Ferrero, I
• Fosalba, P
• Frieman, J
• García-Bellido, J
• Gruen, D
• Gruendl, R A
• Gschwend, J
• Gutierrez, G
• Hartley, W G
• Hinton, S R
• Hollowood, D L
• Honscheid, K
• Hoyle, B
• Jarvis, M
• Kim, A G
• Kuehn, K
• Kuropatkin, N
• Lima, M
• Maia, M A G
• Menanteau, F
• Miquel, R
• Ogando, R L C
• Palmese, A
• Paz-Chinchón, F
• Plazas, A A
• Romer, A K
• Sanchez, E
• Scarpine, V
• Schubnell, M
• Serrano, S
• Sevilla-Noarbe, I
• Smith, M
• Suchyta, E
• Swanson, M E C
• Tarle, G
• Tarsitano, F
• To, C
• Tucker, D L
• Varga, T N
• Wilkinson, R D

Titel

Pushing automated morphological classifications to their limits with the Dark Energy Survey

Ist Teil von

• Monthly notices of the Royal Astronomical Society, 2021-09, Vol.506 (2), p.1927-1943

Ort / Verlag

United States: Oxford University Press

Erscheinungsjahr

2021

Quelle

Free E-Journal (出版社公開部分のみ）

Beschreibungen/Notizen

• ABSTRACT We present morphological classifications of ∼27 million galaxies from the Dark Energy Survey (DES) Data Release 1 (DR1) using a supervised deep learning algorithm. The classification scheme separates: (a) early-type galaxies (ETGs) from late-type galaxies (LTGs); and (b) face-on galaxies from edge-on. Our convolutional neural networks (CNNs) are trained on a small subset of DES objects with previously known classifications. These typically have mr ≲ 17.7 mag; we model fainter objects to mr < 21.5 mag by simulating what the brighter objects with well-determined classifications would look like if they were at higher redshifts. The CNNs reach 97 per cent accuracy to mr < 21.5 on their training sets, suggesting that they are able to recover features more accurately than the human eye. We then used the trained CNNs to classify the vast majority of the other DES images. The final catalogue comprises five independent CNN predictions for each classification scheme, helping to determine if the CNN predictions are robust or not. We obtain secure classifications for ∼87 per cent and 73 per cent of the catalogue for the ETG versus LTG and edge-on versus face-on models, respectively. Combining the two classifications (a) and (b) helps to increase the purity of the ETG sample and to identify edge-on lenticular galaxies (as ETGs with high ellipticity). Where a comparison is possible, our classifications correlate very well with Sérsic index (n), ellipticity (ϵ), and spectral type, even for the fainter galaxies. This is the largest multiband catalogue of automated galaxy morphologies to date.