Discovering Strong Gravitational Lenses in the Dark Energy Survey with Interactive Machine Learning and Crowd-sourced Inspection with Space Warps

Fuente: arXiv
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Auteurs principaux: Gonzalez, J., Holloway, P., Collett, T., Verma, A., Bechtol, K., Marshall, P., More, A., Barroso, J. Acevedo, Cartwright, G., Martinez, M., Li, T., Rojas, K., Schuldt, S., Birrer, S., Diehl, H. T., Morgan, R., Drlica-Wagner, A., O'Donnell, J. H., Zaborowski, E., Nord, B., Baeten, E. M., Johnson, L. C., Macmillan, C., Roodman, A., Pieres, A., Walker, A. R., Malagón, A. A. Plazas, Rosell, A. Carnero, Santiago, B., Flaugher, B., Gruen, D., Brooks, D., Burke, D. L., James, D. J., Cid, D. Sanchez, Hollowood, D. L., Tucker, D. L., Buckley-Geer, E., Gaztanaga, E., Suchyta, E., Sanchez, E., Gutierrez, G., Giannini, G., Tarle, G., Sevilla-Noarbe, I., Marshall, J. L., Carretero, J., Frieman, J., De Vicente, J., García-Bellido, J., Mena-Fernández, J., Myles, J., Honscheid, K., Kuehn, K., Lima, M., Pereira, M. E. S., Smith, M., Aguena, M., Weaverdyck, N., Lahav, O., Doel, P., Miquel, R., Gruendl, R. A., Cawthon, R., Hinton, S. R., Allam, S. S., Desai, S., Samuroff, S., Everett, S., Lee, S., Davis, T. M., Abbott, T. M. C., Vikram, V.
Format: Preprint
Publié: 2025
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author Gonzalez, J.
Holloway, P.
Collett, T.
Verma, A.
Bechtol, K.
Marshall, P.
More, A.
Barroso, J. Acevedo
Cartwright, G.
Martinez, M.
Li, T.
Rojas, K.
Schuldt, S.
Birrer, S.
Diehl, H. T.
Morgan, R.
Drlica-Wagner, A.
O'Donnell, J. H.
Zaborowski, E.
Nord, B.
Baeten, E. M.
Johnson, L. C.
Macmillan, C.
Roodman, A.
Pieres, A.
Walker, A. R.
Malagón, A. A. Plazas
Rosell, A. Carnero
Santiago, B.
Flaugher, B.
Gruen, D.
Brooks, D.
Burke, D. L.
James, D. J.
Cid, D. Sanchez
Hollowood, D. L.
Tucker, D. L.
Buckley-Geer, E.
Gaztanaga, E.
Suchyta, E.
Sanchez, E.
Gutierrez, G.
Giannini, G.
Tarle, G.
Sevilla-Noarbe, I.
Marshall, J. L.
Carretero, J.
Frieman, J.
De Vicente, J.
García-Bellido, J.
Mena-Fernández, J.
Myles, J.
Honscheid, K.
Kuehn, K.
Lima, M.
Pereira, M. E. S.
Smith, M.
Aguena, M.
Weaverdyck, N.
Lahav, O.
Doel, P.
Miquel, R.
Gruendl, R. A.
Cawthon, R.
Hinton, S. R.
Allam, S. S.
Desai, S.
Samuroff, S.
Everett, S.
Lee, S.
Davis, T. M.
Abbott, T. M. C.
Vikram, V.
author_facet Gonzalez, J.
Holloway, P.
Collett, T.
Verma, A.
Bechtol, K.
Marshall, P.
More, A.
Barroso, J. Acevedo
Cartwright, G.
Martinez, M.
Li, T.
Rojas, K.
Schuldt, S.
Birrer, S.
Diehl, H. T.
Morgan, R.
Drlica-Wagner, A.
O'Donnell, J. H.
Zaborowski, E.
Nord, B.
Baeten, E. M.
Johnson, L. C.
Macmillan, C.
Roodman, A.
Pieres, A.
Walker, A. R.
Malagón, A. A. Plazas
Rosell, A. Carnero
Santiago, B.
Flaugher, B.
Gruen, D.
Brooks, D.
Burke, D. L.
James, D. J.
Cid, D. Sanchez
Hollowood, D. L.
Tucker, D. L.
Buckley-Geer, E.
Gaztanaga, E.
Suchyta, E.
Sanchez, E.
Gutierrez, G.
Giannini, G.
Tarle, G.
Sevilla-Noarbe, I.
Marshall, J. L.
Carretero, J.
Frieman, J.
De Vicente, J.
García-Bellido, J.
Mena-Fernández, J.
Myles, J.
Honscheid, K.
Kuehn, K.
Lima, M.
Pereira, M. E. S.
Smith, M.
Aguena, M.
Weaverdyck, N.
Lahav, O.
Doel, P.
Miquel, R.
Gruendl, R. A.
Cawthon, R.
Hinton, S. R.
Allam, S. S.
Desai, S.
Samuroff, S.
Everett, S.
Lee, S.
Davis, T. M.
Abbott, T. M. C.
Vikram, V.
contents We conduct a search for strong gravitational lenses in the Dark Energy Survey (DES) Year 6 imaging data. We implement a pre-trained Vision Transformer (ViT) for our machine learning (ML) architecture and adopt Interactive Machine Learning to construct a training sample with multiple classes to address common types of false positives. Our ML model reduces 236 million DES cutout images to 22,564 targets of interest, including around 85% of previously reported galaxy-galaxy lens candidates discovered in DES. These targets were visually inspected by citizen scientists, who ruled out approximately 90% as false positives. Of the remaining 2,618 candidates, 149 were expert-classified as 'definite' lenses and 516 as 'probable' lenses, with 147 of these candidates being newly identified. Additionally, we trained a second ViT to find double-source plane lens systems, finding at least one double-source system. Our main ViT excels at identifying galaxy-galaxy lenses, consistently assigning high scores to candidates with high confidence. The top 800 ViT-scored images include around 100 of our `definite' lens candidates. This selection is an order of magnitude higher in purity than previous convolutional neural network-based lens searches and demonstrates the feasibility of applying our methodology for discovering large samples of lenses in future surveys.
format Preprint
id arxiv_https___arxiv_org_abs_2501_15679
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Discovering Strong Gravitational Lenses in the Dark Energy Survey with Interactive Machine Learning and Crowd-sourced Inspection with Space Warps
Gonzalez, J.
Holloway, P.
Collett, T.
Verma, A.
Bechtol, K.
Marshall, P.
More, A.
Barroso, J. Acevedo
Cartwright, G.
Martinez, M.
Li, T.
Rojas, K.
Schuldt, S.
Birrer, S.
Diehl, H. T.
Morgan, R.
Drlica-Wagner, A.
O'Donnell, J. H.
Zaborowski, E.
Nord, B.
Baeten, E. M.
Johnson, L. C.
Macmillan, C.
Roodman, A.
Pieres, A.
Walker, A. R.
Malagón, A. A. Plazas
Rosell, A. Carnero
Santiago, B.
Flaugher, B.
Gruen, D.
Brooks, D.
Burke, D. L.
James, D. J.
Cid, D. Sanchez
Hollowood, D. L.
Tucker, D. L.
Buckley-Geer, E.
Gaztanaga, E.
Suchyta, E.
Sanchez, E.
Gutierrez, G.
Giannini, G.
Tarle, G.
Sevilla-Noarbe, I.
Marshall, J. L.
Carretero, J.
Frieman, J.
De Vicente, J.
García-Bellido, J.
Mena-Fernández, J.
Myles, J.
Honscheid, K.
Kuehn, K.
Lima, M.
Pereira, M. E. S.
Smith, M.
Aguena, M.
Weaverdyck, N.
Lahav, O.
Doel, P.
Miquel, R.
Gruendl, R. A.
Cawthon, R.
Hinton, S. R.
Allam, S. S.
Desai, S.
Samuroff, S.
Everett, S.
Lee, S.
Davis, T. M.
Abbott, T. M. C.
Vikram, V.
Astrophysics of Galaxies
We conduct a search for strong gravitational lenses in the Dark Energy Survey (DES) Year 6 imaging data. We implement a pre-trained Vision Transformer (ViT) for our machine learning (ML) architecture and adopt Interactive Machine Learning to construct a training sample with multiple classes to address common types of false positives. Our ML model reduces 236 million DES cutout images to 22,564 targets of interest, including around 85% of previously reported galaxy-galaxy lens candidates discovered in DES. These targets were visually inspected by citizen scientists, who ruled out approximately 90% as false positives. Of the remaining 2,618 candidates, 149 were expert-classified as 'definite' lenses and 516 as 'probable' lenses, with 147 of these candidates being newly identified. Additionally, we trained a second ViT to find double-source plane lens systems, finding at least one double-source system. Our main ViT excels at identifying galaxy-galaxy lenses, consistently assigning high scores to candidates with high confidence. The top 800 ViT-scored images include around 100 of our `definite' lens candidates. This selection is an order of magnitude higher in purity than previous convolutional neural network-based lens searches and demonstrates the feasibility of applying our methodology for discovering large samples of lenses in future surveys.
title Discovering Strong Gravitational Lenses in the Dark Energy Survey with Interactive Machine Learning and Crowd-sourced Inspection with Space Warps
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2501.15679