The impact of human expert visual inspection on the discovery of strong gravitational lenses
We investigate the ability of human 'expert' classifiers to identify strong gravitational lens candidates in Dark Energy Survey like imaging. We recruited a total of 55 people that completed more than 25\(\%\) of the project. During the classification task, we present to the participants 1...
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creator | Rojas, Karina Collett, Thomas E Ballard, Daniel Magee, Mark R Birrer, Simon Buckley-Geer, Elizabeth Chan, James H H Clément, Benjamin Diego, José M Gentile, Fabrizio González, Jimena Rémy, Joseph Mastache, Jorge Schuldt, Stefan Tortora, Crescenzo Verdugo, Tomás Verma, Aprajita Daylan, Tansu Millon, Martin Jackson, Neal Dye, Simon Melo, Alejandra Mahler, Guillaume Ogando, Ricardo L C Courbin, Frédéric Fritz, Alexander Herle, Aniruddh Acevedo Barroso, Javier A Cañameras, Raoul Cornen, Claude Dhanasingham, Birendra Glazebrook, Karl Martinez, Michael N Ryczanowski, Dan Savary, Elodie Góis-Silva, Filipe Ureña-López, L Arturo Wiesner, Matthew P Wilde, Joshua Gabriel Valim Calçada Cabanac, Rémi Pan, Yue Sierra, Isaac Despali, Giulia Cavalcante-Gomes, Micaele V Macmillan, Christine Maresca, Jacob Grudskaia, Aleksandra O'Donnell, Jackson H Paic, Eric Niemiec, Anna Lucia F de la Bella Bromley, Jane Williams, Devon M More, Anupreeta Levine, Benjamin C |
description | We investigate the ability of human 'expert' classifiers to identify strong gravitational lens candidates in Dark Energy Survey like imaging. We recruited a total of 55 people that completed more than 25\(\%\) of the project. During the classification task, we present to the participants 1489 images. The sample contains a variety of data including lens simulations, real lenses, non-lens examples, and unlabeled data. We find that experts are extremely good at finding bright, well-resolved Einstein rings, whilst arcs with \(g\)-band signal-to-noise less than \(\sim\)25 or Einstein radii less than \(\sim\)1.2 times the seeing are rarely recovered. Very few non-lenses are scored highly. There is substantial variation in the performance of individual classifiers, but they do not appear to depend on the classifier's experience, confidence or academic position. These variations can be mitigated with a team of 6 or more independent classifiers. Our results give confidence that humans are a reliable pruning step for lens candidates, providing pure and quantifiably complete samples for follow-up studies. |
doi_str_mv | 10.48550/arxiv.2301.03670 |
format | Article |
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We recruited a total of 55 people that completed more than 25\(\%\) of the project. During the classification task, we present to the participants 1489 images. The sample contains a variety of data including lens simulations, real lenses, non-lens examples, and unlabeled data. We find that experts are extremely good at finding bright, well-resolved Einstein rings, whilst arcs with \(g\)-band signal-to-noise less than \(\sim\)25 or Einstein radii less than \(\sim\)1.2 times the seeing are rarely recovered. Very few non-lenses are scored highly. There is substantial variation in the performance of individual classifiers, but they do not appear to depend on the classifier's experience, confidence or academic position. These variations can be mitigated with a team of 6 or more independent classifiers. 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We recruited a total of 55 people that completed more than 25\(\%\) of the project. During the classification task, we present to the participants 1489 images. The sample contains a variety of data including lens simulations, real lenses, non-lens examples, and unlabeled data. We find that experts are extremely good at finding bright, well-resolved Einstein rings, whilst arcs with \(g\)-band signal-to-noise less than \(\sim\)25 or Einstein radii less than \(\sim\)1.2 times the seeing are rarely recovered. Very few non-lenses are scored highly. There is substantial variation in the performance of individual classifiers, but they do not appear to depend on the classifier's experience, confidence or academic position. These variations can be mitigated with a team of 6 or more independent classifiers. 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Jackson, Neal ; Dye, Simon ; Melo, Alejandra ; Mahler, Guillaume ; Ogando, Ricardo L C ; Courbin, Frédéric ; Fritz, Alexander ; Herle, Aniruddh ; Acevedo Barroso, Javier A ; Cañameras, Raoul ; Cornen, Claude ; Dhanasingham, Birendra ; Glazebrook, Karl ; Martinez, Michael N ; Ryczanowski, Dan ; Savary, Elodie ; Góis-Silva, Filipe ; Ureña-López, L Arturo ; Wiesner, Matthew P ; Wilde, Joshua ; Gabriel Valim Calçada ; Cabanac, Rémi ; Pan, Yue ; Sierra, Isaac ; Despali, Giulia ; Cavalcante-Gomes, Micaele V ; Macmillan, Christine ; Maresca, Jacob ; Grudskaia, Aleksandra ; O'Donnell, Jackson H ; Paic, Eric ; Niemiec, Anna ; Lucia F de la Bella ; Bromley, Jane ; Williams, Devon M ; More, Anupreeta ; Levine, Benjamin 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subjects | Classifiers Dark energy Gravitational lenses Human performance Inspection Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Sky surveys (astronomy) |
title | The impact of human expert visual inspection on the discovery of strong gravitational lenses |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-21T17%3A48%3A59IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20impact%20of%20human%20expert%20visual%20inspection%20on%20the%20discovery%20of%20strong%20gravitational%20lenses&rft.jtitle=arXiv.org&rft.au=Rojas,%20Karina&rft.date=2023-04-25&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2301.03670&rft_dat=%3Cproquest_arxiv%3E2763960309%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2763960309&rft_id=info:pmid/&rfr_iscdi=true |