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Euclid Quick Data Release (Q1). The Strong Lensing Discovery Engine E -- Ensemble classification of strong gravitational lenses: lessons for Data Release 1

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arxiv 2503.15328 v1 pith:PSGRMSKS submitted 2025-03-19 astro-ph.GA astro-ph.CO

Euclid Quick Data Release (Q1). The Strong Lensing Discovery Engine E -- Ensemble classification of strong gravitational lenses: lessons for Data Release 1

Euclid Collaboration: P. Holloway , A. Verma , M. Walmsley , P. J. Marshall , A. More , T. E. Collett , N. E. P. Lines , L. Leuzzi
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A. Manj\'on-Garc\'ia S. H. Vincken J. Wilde R. Pearce-Casey I. T. Andika J. A. Acevedo Barroso T. Li A. Melo R. B. Metcalf K. Rojas B. Cl\'ement H. Degaudenzi F. Courbin G. Despali R. Gavazzi S. Schuldt B. C. Nagam D. Sluse C. Tortora H. Dom\'inguez S\'anchez K. Finner A. Galan C. Giocoli L. Guzzo N. B. Hogg K. Jahnke S. Kruk G. Mahler M. Millon P. Nugent J. Pearson L. R. Ecker A. Sainz de Murieta C. Scarlata S. Serjeant A. Sonnenfeld C. Spiniello T. T. Thai L. Ulivi L. Weisenbach M. Zumalacarregui N. Aghanim B. Altieri A. Amara S. Andreon N. Auricchio H. Aussel C. Baccigalupi M. Baldi A. Balestra S. Bardelli P. Battaglia R. Bender A. Biviano A. Bonchi E. Branchini M. Brescia J. Brinchmann S. Camera G. Ca\~nas-Herrera V. Capobianco C. Carbone V. F. Cardone J. Carretero M. Castellano G. Castignani S. Cavuoti K. C. Chambers A. Cimatti C. Colodro-Conde G. Congedo C. J. Conselice L. Conversi Y. Copin H. M. Courtois M. Cropper A. Da Silva G. De Lucia A. M. Di Giorgio C. Dolding H. Dole F. Dubath C. A. J. Duncan X. Dupac S. Dusini A. Ealet S. Escoffier M. Farina R. Farinelli F. Faustini S. Ferriol F. Finelli S. Fotopoulou M. Frailis E. Franceschi M. Fumana S. Galeotta K. George B. Gillis P. G\'omez-Alvarez J. Gracia-Carpio B. R. Granett A. Grazian F. Grupp S. V. H. Haugan J. Hoar W. Holmes F. Hormuth A. Hornstrup P. Hudelot M. Jhabvala B. Joachimi E. Keih\"anen S. Kermiche A. Kiessling B. Kubik M. K\"ummel M. Kunz H. Kurki-Suonio Q. Le Boulc'h A. M. C. Le Brun D. Le Mignant S. Ligori P. B. Lilje V. Lindholm I. Lloro G. Mainetti D. Maino E. Maiorano O. Mansutti S. Marcin O. Marggraf M. Martinelli N. Martinet F. Marulli R. Massey S. Maurogordato E. Medinaceli S. Mei M. Melchior Y. Mellier M. Meneghetti E. Merlin G. Meylan A. Mora M. Moresco L. Moscardini R. Nakajima C. Neissner R. C. Nichol S.-M. Niemi J. W. Nightingale C. Padilla S. Paltani F. Pasian K. Pedersen W. J. Percival V. Pettorino S. Pires G. Polenta M. Poncet L. A. Popa L. Pozzetti F. Raison R. Rebolo A. Renzi J. Rhodes G. Riccio E. Romelli M. Roncarelli R. Saglia Z. Sakr D. Sapone B. Sartoris J. A. Schewtschenko P. Schneider A. Secroun G. Seidel S. Serrano P. Simon C. Sirignano G. Sirri L. Stanco J. Steinwagner P. Tallada-Cresp\'i A. N. Taylor I. Tereno S. Toft R. Toledo-Moreo F. Torradeflot I. Tutusaus E. A. Valentijn L. Valenziano J. Valiviita T. Vassallo G. Verdoes Kleijn A. Veropalumbo Y. Wang J. Weller A. Zacchei G. Zamorani F. M. Zerbi E. Zucca V. Allevato M. Ballardini M. Bolzonella E. Bozzo C. Burigana R. Cabanac A. Cappi D. Di Ferdinando J. A. Escartin Vigo L. Gabarra M. Huertas-Company J. Mart\'in-Fleitas S. Matthew N. Mauri A. A. Nucita A. Pezzotta M. P\"ontinen C. Porciani I. Risso V. Scottez M. Sereno M. Tenti M. Viel M. Wiesmann Y. Akrami S. Anselmi M. Archidiacono F. Atrio-Barandela C. Benoist K. Benson P. Bergamini D. Bertacca M. Bethermin A. Blanchard L. Blot S. Borgani M. L. Brown S. Bruton A. Calabro F. Caro C. S. Carvalho T. Castro F. Cogato A. R. Cooray O. Cucciati S. Davini F. De Paolis G. Desprez A. D\'iaz-S\'anchez J. J. Diaz S. Di Domizio J. M. Diego P.-A. Duc A. Enia Y. Fang A. G. Ferrari P. G. Ferreira A. Finoguenov A. Fontana A. Franco K. Ganga J. Garc\'ia-Bellido T. Gasparetto V. Gautard E. Gaztanaga F. Giacomini F. Gianotti G. Gozaliasl C. M. Gutierrez A. Hall W. G. Hartley C. Hern\'andez-Monteagudo H. Hildebrandt J. Hjorth J. J. E. Kajava Y. Kang V. Kansal D. Karagiannis K. Kiiveri C. C. Kirkpatrick J. Le Graet L. Legrand M. Lembo F. Lepori G. Leroy G. F. Lesci J. Lesgourgues T. I. Liaudat A. Loureiro J. Macias-Perez G. Maggio M. Magliocchetti E. A. Magnier F. Mannucci R. Maoli C. J. A. P. Martins L. Maurin M. Miluzio P. Monaco A. Montoro C. Moretti G. Morgante K. Naidoo A. Navarro-Alsina S. Nesseris F. Passalacqua K. Paterson L. Patrizii A. Pisani D. Potter S. Quai M. Radovich S. Sacquegna M. Sahl\'en D. B. Sanders E. Sarpa A. Schneider D. Sciotti E. Sellentin L. C. Smith K. Tanidis G. Testera R. Teyssier S. Tosi A. Troja M. Tucci C. Valieri A. Venhola D. Vergani G. Vernardos G. Verza P. Vielzeuf N. A. Walton D. Scott
This is my paper
classification astro-ph.GA astro-ph.CO
keywords dataeuclidlensesreleasegradeensembleimagesstrong
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Euclid Wide Survey (EWS) is expected to identify of order $100\,000$ galaxy-galaxy strong lenses across $14\,000$deg$^2$. The Euclid Quick Data Release (Q1) of $63.1$deg$^2$ Euclid images provides an excellent opportunity to test our lens-finding ability, and to verify the anticipated lens frequency in the EWS. Following the Q1 data release, eight machine learning networks from five teams were applied to approximately one million images. This was followed by a citizen science inspection of a subset of around $100\,000$ images, of which $65\%$ received high network scores, with the remainder randomly selected. The top scoring outputs were inspected by experts to establish confident (grade A), likely (grade B), possible (grade C), and unlikely lenses. In this paper we combine the citizen science and machine learning classifiers into an ensemble, demonstrating that a combined approach can produce a purer and more complete sample than the original individual classifiers. Using the expert-graded subset as ground truth, we find that this ensemble can provide a purity of $52\pm2\%$ (grade A/B lenses) with $50\%$ completeness (for context, due to the rarity of lenses a random classifier would have a purity of $0.05\%$). We discuss future lessons for the first major Euclid data release (DR1), where the big-data challenges will become more significant and will require analysing more than $\sim300$ million galaxies, and thus time investment of both experts and citizens must be carefully managed.

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    A vision transformer classifier trained on simulated and real Euclid data recovers all known strong lenses in test sets and finds 8 Grade A plus 26 Grade B new candidates in the Q1 data.