Euclid Quick Data Release (Q1). The active galaxies of Euclid

We present three catalogues of candidate active galactic nuclei (AGN) in the Euclid Quick Release (Q1) fields. For each Euclid source, we collected multi-wavelength photometric and spectroscopic information from surveys such as the Galaxy Evolution Explorer (GALEX) the Dark Energy Survey (DES), the Wide-field Infrared Survey Explorer (WISE) Spitzer the Dark Energy Spectroscopic Instrument (DESI), and the Sloan Digital Sky Survey (SDSS), including spectroscopic redshifts from public compilations when available. We investigated the AGN content of the Q1 fields using multiple selection methods. Applying Euclid colours and WISE-AllWISE cuts, we identified 292,222 and 65,131 candidates, respectively. We compiled a high-purity QSO catalogue based on DR3 information, containing 1971 candidates. Using spectroscopic information from DESI, we performed broad-line and narrow-line AGN selections, yielding 4392 AGN candidates across the Q1 fields. We investigated and refined the Euclid Q1 probabilistic random forest QSO population, selecting a refined sample of 180,666 candidates. Additionally, we performed spectral energy distribution (SED) fitting on sources with available z_ spec and utilising the derived AGN fraction, we identified 7766 AGN candidates. To improve the purity of the selection, we defined two new colour criteria (JH_I_E Y and I_E H_gz), finding 313,714 and 267,513 candidates, respectively, across the Q1 fields. We have found a total of 229,779 AGN candidates equivalent to an AGN surface density of 3641 deg^-2 for $18< 24.5$ and a subsample of 30,422 candidates corresponding to an AGN surface density of 482 deg^-2 when limiting the depth to $18< 22$. The AGN surface densities recovered are consistent with predictions based on AGN X-ray luminosity functions.

Authors

Publication Details

Journal
Astronomy and Astrophysics
Published
2025-08-08
DOI
https://doi.org/10.1051/0004-6361/202554619
Citations
1
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
1.19
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Euclid Quick Data Release (Q1). The active galaxies of Euclid

G. Seidel, J. Brinchmann, Laura Bisigello, G. Rodighiero et al.
1 citations
Astronomy and Astrophysics
Astronomy and Astrophysical Research
1.19
article

Euclid Quick Data Release (Q1). The active galaxies of Euclid

G. Seidel, J. Brinchmann, Laura Bisigello, G. Rodighiero, Pratika Dayal, A. Ealet, P.-A. Duc, F Passalacqua, J. Graciá‐Carpio, J. Hjorth, Will J. Percival, M. Ballardini, G. Mainetti, E. A. Magnier, R. P. Saglia, S Sacquegna, P. Hudelot, G. Riccio, L. Conversi, F. Gianotti, D. Le Mignant, C. Sirignano, M. Brescia, E. Merlin, I. Hook, M. Kunz, F. Dubath, J. García-Bellido, Hermine Landt, A. Viitanen, Brivael Laloux, J. Carretero, J. Steinwagner, N. Aghanim, D. B. Sanders, F. Marulli, A.G Ferrari, A. Navarro-Alsina, N. Mauri, C. Giocoli, O. Marggraf, M. Mezcua, A. Franco, S. A. Stanford, J. F. Macías–Pérez, F. Courbin, V. Scottez, H. J. A. Röttgering, F. Torradeflot, A. Pisani, M. Schultheis, Alex D. Hall, A. Kiessling, A. Troja, Michael D. Brown, F Caro, A. Grazian, M. Fabricius, M. Jhabvala, A. Feltre, Elena Sellentin, A. Díaz‐Sánchez, J.J Diaz, G. Gozaliasl, Pierluigi Monaco, Harald J. Hoekstra, S. Bardelli, W. Holmes, T. Contini, F Faustini, Francisco Javier Castander, Daniele Bertacca, M. Radovich, M. Martinelli, A. Finoguenov, M. Magliocchetti, Alberto Basset, C.J.A.P. Martins, S. Nadathur, A.R. Cooray, L. Spinoglio, Andrea Bonchi, O. Cucciati, V. Capobianco, L. Moscardini, T. Schrabback, L. Gabarra, M Miluzio, I. A. Zinchenko, Stephen Gwyn, E. Zucca, S. Andreon, S. Maurogordato, F. La Franca, S. V. H. Haugan, J. Skottfelt, D. Vergani, R. Massey, A Enia, S. Paltani, Valérie Gautard, R. Toledo-Moreo, B. Camacho Quevedo, S Bruton, M. Moresco, G Sirri, B. R. Granett, Y Fang, D. Sapone, T. Castro, M. Meneghetti, J.W Nightingale, A. Veropalumbo, L. Patrizii, P. Tallada-Crespí, G. Congedo, L. Valenziano, A. Cappi, T.I Liaudat, D. Scott, K. Ganga, M. Salvato, A. Fontana, Yoshiki Toba, E. Romelli, C. Burigana, A. M. Di Giorgio, S Quai, Christopher J. Conselice, A. Biviano, I. Tutusaus, H. Degaudenzi, O. Mansutti, G. Zamorani, Matteo Viel, M Lembo, Julien Lesgourgues, N. Martinet, I Risso, K. Benson, V. Allevato, J. Väliviita, F Tarsitano, S. Escoffier, C. Padilla Aranda, L Blot, E. Maiorano, B. Gillis, M Sahlén, M. Roncarelli, F. De Paolis, M. Giulietti, R. B. Metcalf, S. Fotopoulou, E. Medinaceli, Sergey Kruk, M. Pöntinen, S. Di Domizio, Francesco Shankar, S. Marcin, F. M. Zerbi, M. Béthermin, K. Jahnkę, A. Secroun, M. Farina, Antonello Calabrò, F. Mannucci, F. Pasian, A. Venhola, V. Kansal, L. Wang, S. Ligori, M. Castellano, F Lepori, F. Grupp, R. Farinelli, F. Giacomini, C. Valieri, A. Zacchei, S. Galeotta, F. Raison, M. Melchior, E. Franceschi, Daniel Masters, J.A Schewtschenko, ENRIQUE GAZTAÑAGA, J Martín-Fleitas, P. Gómez-Álvarez, J.M. Diego, M. Siudek, I Lloro, Q. Le Boulc'h, S. Dusini, Pardis Simon, N. A. Walton, Antonio La Marca, B. Margalef-Bentabol, G Cañas-Herrera, S. Davini, Antonio M. Mora, Alain Blanchard, I.T Andika, R. Cabanac, R. Shirley, S. Camera, Z. Sakr, F. Hormuth, J. J. Mohr, K Tanidis, João Calhau, L. Legrand, E. Bozzo, Romain Teyssier, LAURENCE C. SMITH, G.F Lesci, K. C. Chambers, M. Archidiacono, T Gasparetto, V. Lindholm, R. Rébolo, G. Verdoes Kleijn, P.-F Rocci, M. Sereno, M. Cropper, B. Sartoris, G. Meylan, P Vielzeuf, Koshy George, S. Cavuoti, Krishna Naidoo, N. Auricchio, M. Frailis, Mark Taylor, F. Ricci, Petra Schneider, M. Scialpi, C. Carbone, Shoubaneh Hemmati, B. Altieri, K. Paterson, S. Kermiche, Arthur Loureiro, E. Soubrie, E Sarpa, D. M. Alexander, Sune Toft, A.G. Sánchez, V. Pettorino, D. Sluse, P. B. Lilje, M. Scodeggio, A. Shulevski, Y. Mellier, Giulio Fabbian, S. Serrano, G. Polenta, C.S. Carvalho, B. Rusholme, E. Rossetti, A Pezzotta, Clare Murray, A.M.C Le Brun, Aurel Schneider, D. Potter, E. Branchini, S Nesseris, M. Kümmel, Y. Akrami, G. De Lucia, F. Atrio‐Barandela, Claudio Moretti, H. M. Courtois, F. Cogato, D Sciotti, W. Roster, Yun Wang, A. Da Silva, L. Stančo, L. Maurin, C. M. Gutiérrez, J.E. Kajava, R.A. Shaw, M. Selwood, G. Testera, Ryota Nakajima, X. López López, M. D. Seiffert, F. Finelli, G Leroy, M. Bolzonella, C. Porciani, Y. Fu, D. Maino, K. Kiiveri, M. Tenti, D. Di Ferdinando, I. Tereno, V. Pettorino, A. Renzi, L. A. Popa, P Battaglia, A. Bongiorno, H. Kurki‐Suonio, M. Wiesmann, P. Liebing, C. Hernández-Monteagudo, G. Maggio, C. Baccigalupi, W. G. Hartley, Christophe Benoıst, C. Neissner, S. Pires, M. Poncet, Jason Rhodes, J.A. Escartin Vigo, C. Saulder, B. Kubik, H. Hildebrandt, H. Dole, N. Fourmanoit, A Cimatti, A. N. Taylor, G Verza, M. N. Bremer, C Colodro-Conde, S.-M Niemi, M Guidi, S. Ferriol, C. A. J. Duncan, H. Böhringer, G Morgante, X. Dupac, A. Gregorio, L. Leuzzi, Y Kang
article en
1 citations

Abstract

We present three catalogues of candidate active galactic nuclei (AGN) in the Euclid Quick Release (Q1) fields. For each Euclid source, we collected multi-wavelength photometric and spectroscopic information from surveys such as the Galaxy Evolution Explorer (GALEX) the Dark Energy Survey (DES), the Wide-field Infrared Survey Explorer (WISE) Spitzer the Dark Energy Spectroscopic Instrument (DESI), and the Sloan Digital Sky Survey (SDSS), including spectroscopic redshifts from public compilations when available. We investigated the AGN content of the Q1 fields using multiple selection methods. Applying Euclid colours and WISE-AllWISE cuts, we identified 292,222 and 65,131 candidates, respectively. We compiled a high-purity QSO catalogue based on DR3 information, containing 1971 candidates. Using spectroscopic information from DESI, we performed broad-line and narrow-line AGN selections, yielding 4392 AGN candidates across the Q1 fields. We investigated and refined the Euclid Q1 probabilistic random forest QSO population, selecting a refined sample of 180,666 candidates. Additionally, we performed spectral energy distribution (SED) fitting on sources with available z_ spec and utilising the derived AGN fraction, we identified 7766 AGN candidates. To improve the purity of the selection, we defined two new colour criteria (JH_I_E Y and I_E H_gz), finding 313,714 and 267,513 candidates, respectively, across the Q1 fields. We have found a total of 229,779 AGN candidates equivalent to an AGN surface density of 3641 deg^-2 for $18< 24.5$ and a subsample of 30,422 candidates corresponding to an AGN surface density of 482 deg^-2 when limiting the depth to $18< 22$. The AGN surface densities recovered are consistent with predictions based on AGN X-ray luminosity functions.

Astronomy and Astrophysics
Affordable and clean energy
Openalex Percentile: Top 18%
Astronomy and Astrophysical Research
1.19
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.