Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees

Signor, T.; Rodighiero, G.; Bisigello, L.; Bolzonella, M.; Caputi, K.I.; Daddi, E.; De Lucia, G.; Enia, A.; Gabarra, L.; Gruppioni, C.; Humphrey, A.; La Franca, F.; Mancini, C.; Pozzetti, L.; Serjeant, S.; Spinoglio, L.; Van Mierlo, S.E.; Andreon, S.; Auricchio, N.; Baldi, M.; Bardelli, S.; Battaglia, P.; Bender, R.; Bodendorf, C.; Bonino, D.; Branchini, E.; Brescia, M.; Brinchmann, J.; Camera, S.; Capobianco, V.; Carbone, C.; Carretero, J.; Casas, S.; Castellano, M.; Cavuoti, S.; Cimatti, A.; Cledassou, R.; Congedo, G.; Conselice, C.J.; Conversi, L.; Copin, Y.; Corcione, L.; Courbin, Frédéric; Courtois, H.M.; Da Silva, A.; Degaudenzi, H.; Di Giorgio, A.M.; Dinis, J.; Dubath, F.; Dupac, X.; Dusini, S.; Ealet, A.; Farina, M.; Farrens, S.; Ferriol, S.; Fotopoulou, S.; Franceschi, E.; Galeotta, S.; Garilli, B.; Gillard, W.; Gillis, B.; Giocoli, C.; Grazian, A.; Grupp, F.; Guzzo, L.; Haugan, S.V.H.; Hook, I.; Hormuth, F.; Hornstrup, A.; Jahnke, K.; Kümmel, M.; Kermiche, S.; Kiessling, A.; Kilbinger, M.; Kitching, T.; Kurki-Suonio, H.; Ligori, S.; Lilje, P.B.; Lindholm, V.; Lloro, I.; Maino, D.; Maiorano, E.; Mansutti, O.; Marggraf, O.; Martinet, N.; Marulli, F.; Massey, R.; Medinaceli, E.; Melchior, M.; Mellier, Y.; Meneghetti, M.; Merlin, E.; Moresco, M.; Moscardini, L.; Munari, E.; Nichol, R.C.; Niemi, S.-M.; Padilla, C.; Paltani, S.; Pasian, F.; Pedersen, K.; Pettorino, V.; Pires, S.; Polenta, G.; Poncet, M.; Popa, L.A.; Raison, F.; Renzi, A.; Rhodes, J.; Riccio, G.; Romelli, E.; Roncarelli, M.; Rossetti, E.; Saglia, R.; Sapone, D.; Sartoris, B.; Schneider, P.; Schrabback, T.; Secroun, A.; Seidel, G.; Serrano, S.; Sirignano, C.; Sirri, G.; Stanco, L.; Surace, C.; Tallada-Crespí, P.; Teplitz, H.I.; Tereno, I.; Toledo-Moreo, R.; Torradeflot, F.; Tutusaus, I.; Valentijn, E.A.; Vassallo, T.; Veropalumbo, A.; Wang, Yan; Weller, J.; Williams, O.R.; Zoubian, J.; Zucca, E.; Burigana, C.; Scottez, V.

Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees

Context. ALMA observations show that dusty, distant, massive (M∗ & 1011 M) galaxies usually have a remarkable star-formation activity, contributing of the order of 25% of the cosmic star-formation rate density at z ≈ 3–5, and up to 30% at z ∼ 7. Nonetheless, they are elusive in classical optical...

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Autores:	Signor, T., Rodighiero, G., Bisigello, L., Bolzonella, M., Caputi, K.I., Daddi, E., De Lucia, G., Enia, A., Gabarra, L., Gruppioni, C., Humphrey, A., La Franca, F., Mancini, C., Pozzetti, L., Serjeant, S., Spinoglio, L., Van Mierlo, S.E., Andreon, S., Auricchio, N., Baldi, M., Bardelli, S., Battaglia, P., Bender, R., Bodendorf, C., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Capobianco, V., Carbone, C., Carretero, J., Casas, S., Castellano, M., Cavuoti, S., Cimatti, A., Cledassou, R., Congedo, G., Conselice, C.J., Conversi, L., Copin, Y., Corcione, L., Courbin, Frédéric, Courtois, H.M., Da Silva, A., Degaudenzi, H., Di Giorgio, A.M., Dinis, J., Dubath, F., Dupac, X., Dusini, S., Ealet, A., Farina, M., Farrens, S., Ferriol, S., Fotopoulou, S., Franceschi, E., Galeotta, S., Garilli, B., Gillard, W., Gillis, B., Giocoli, C., Grazian, A., Grupp, F., Guzzo, L., Haugan, S.V.H., Hook, I., Hormuth, F., Hornstrup, A., Jahnke, K., Kümmel, M., Kermiche, S., Kiessling, A., Kilbinger, M., Kitching, T., Kurki-Suonio, H., Ligori, S., Lilje, P.B., Lindholm, V., Lloro, I., Maino, D., Maiorano, E., Mansutti, O., Marggraf, O., Martinet, N., Marulli, F., Massey, R., Medinaceli, E., Melchior, M., Mellier, Y., Meneghetti, M., Merlin, E., Moresco, M., Moscardini, L., Munari, E., Nichol, R.C., Niemi, S.-M., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Pettorino, V., Pires, S., Polenta, G., Poncet, M., Popa, L.A., Raison, F., Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rossetti, E., Saglia, R., Sapone, D., Sartoris, B., Schneider, P., Schrabback, T., Secroun, A., Seidel, G., Serrano, S., Sirignano, C., Sirri, G., Stanco, L., Surace, C., Tallada-Crespí, P., Teplitz, H.I., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E.A., Vassallo, T., Veropalumbo, A., Wang, Yan, Weller, J., Williams, O.R., Zoubian, J., Zucca, E., Burigana, C., Scottez, V.
Tipo de recurso:	artículo
Estado:	Versión publicada
Fecha de publicación:	2024
País:	España
Institución:	Universidad de Barcelona
Repositorio:	Dipòsit Digital de la UB
OAI Identifier:	oai:diposit.ub.edu:2445/221025
Acceso en línea:	https://hdl.handle.net/2445/221025
Access Level:	acceso abierto
Palabra clave:	Galàxies actives Galàxies Evolució de les galàxies Active galaxies Galaxies Galaxies evolution

id	ES_c29fc4dac67b74cf29885c4afbb9ce7d
oai_identifier_str	oai:diposit.ub.edu:2445/221025
network_acronym_str	ES
network_name_str	España
repository_id_str
dc.title.none.fl_str_mv	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees
title	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees
spellingShingle	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees Signor, T. Galàxies actives Galàxies Evolució de les galàxies Active galaxies Galaxies Galaxies evolution
title_short	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees
title_full	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees
title_fullStr	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees
title_full_unstemmed	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees
title_sort	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees
dc.creator.none.fl_str_mv	Signor, T. Rodighiero, G. Bisigello, L. Bolzonella, M. Caputi, K.I. Daddi, E. De Lucia, G. Enia, A. Gabarra, L. Gruppioni, C. Humphrey, A. La Franca, F. Mancini, C. Pozzetti, L. Serjeant, S. Spinoglio, L. Van Mierlo, S.E. Andreon, S. Auricchio, N. Baldi, M. Bardelli, S. Battaglia, P. Bender, R. Bodendorf, C. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Cavuoti, S. Cimatti, A. Cledassou, R. Congedo, G. Conselice, C.J. Conversi, L. Copin, Y. Corcione, L. Courbin, Frédéric Courtois, H.M. Da Silva, A. Degaudenzi, H. Di Giorgio, A.M. Dinis, J. Dubath, F. Dupac, X. Dusini, S. Ealet, A. Farina, M. Farrens, S. Ferriol, S. Fotopoulou, S. Franceschi, E. Galeotta, S. Garilli, B. Gillard, W. Gillis, B. Giocoli, C. Grazian, A. Grupp, F. Guzzo, L. Haugan, S.V.H. Hook, I. Hormuth, F. Hornstrup, A. Jahnke, K. Kümmel, M. Kermiche, S. Kiessling, A. Kilbinger, M. Kitching, T. Kurki-Suonio, H. Ligori, S. Lilje, P.B. Lindholm, V. Lloro, I. Maino, D. Maiorano, E. Mansutti, O. Marggraf, O. Martinet, N. Marulli, F. Massey, R. Medinaceli, E. Melchior, M. Mellier, Y. Meneghetti, M. Merlin, E. Moresco, M. Moscardini, L. Munari, E. Nichol, R.C. Niemi, S.-M. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L.A. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Stanco, L. Surace, C. Tallada-Crespí, P. Teplitz, H.I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E.A. Vassallo, T. Veropalumbo, A. Wang, Yan Weller, J. Williams, O.R. Zoubian, J. Zucca, E. Burigana, C. Scottez, V.
author	Signor, T.
author_facet	Signor, T. Rodighiero, G. Bisigello, L. Bolzonella, M. Caputi, K.I. Daddi, E. De Lucia, G. Enia, A. Gabarra, L. Gruppioni, C. Humphrey, A. La Franca, F. Mancini, C. Pozzetti, L. Serjeant, S. Spinoglio, L. Van Mierlo, S.E. Andreon, S. Auricchio, N. Baldi, M. Bardelli, S. Battaglia, P. Bender, R. Bodendorf, C. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Cavuoti, S. Cimatti, A. Cledassou, R. Congedo, G. Conselice, C.J. Conversi, L. Copin, Y. Corcione, L. Courbin, Frédéric Courtois, H.M. Da Silva, A. Degaudenzi, H. Di Giorgio, A.M. Dinis, J. Dubath, F. Dupac, X. Dusini, S. Ealet, A. Farina, M. Farrens, S. Ferriol, S. Fotopoulou, S. Franceschi, E. Galeotta, S. Garilli, B. Gillard, W. Gillis, B. Giocoli, C. Grazian, A. Grupp, F. Guzzo, L. Haugan, S.V.H. Hook, I. Hormuth, F. Hornstrup, A. Jahnke, K. Kümmel, M. Kermiche, S. Kiessling, A. Kilbinger, M. Kitching, T. Kurki-Suonio, H. Ligori, S. Lilje, P.B. Lindholm, V. Lloro, I. Maino, D. Maiorano, E. Mansutti, O. Marggraf, O. Martinet, N. Marulli, F. Massey, R. Medinaceli, E. Melchior, M. Mellier, Y. Meneghetti, M. Merlin, E. Moresco, M. Moscardini, L. Munari, E. Nichol, R.C. Niemi, S.-M. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L.A. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Stanco, L. Surace, C. Tallada-Crespí, P. Teplitz, H.I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E.A. Vassallo, T. Veropalumbo, A. Wang, Yan Weller, J. Williams, O.R. Zoubian, J. Zucca, E. Burigana, C. Scottez, V.
author_role	author
author2	Rodighiero, G. Bisigello, L. Bolzonella, M. Caputi, K.I. Daddi, E. De Lucia, G. Enia, A. Gabarra, L. Gruppioni, C. Humphrey, A. La Franca, F. Mancini, C. Pozzetti, L. Serjeant, S. Spinoglio, L. Van Mierlo, S.E. Andreon, S. Auricchio, N. Baldi, M. Bardelli, S. Battaglia, P. Bender, R. Bodendorf, C. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castellano, M. Cavuoti, S. Cimatti, A. Cledassou, R. Congedo, G. Conselice, C.J. Conversi, L. Copin, Y. Corcione, L. Courbin, Frédéric Courtois, H.M. Da Silva, A. Degaudenzi, H. Di Giorgio, A.M. Dinis, J. Dubath, F. Dupac, X. Dusini, S. Ealet, A. Farina, M. Farrens, S. Ferriol, S. Fotopoulou, S. Franceschi, E. Galeotta, S. Garilli, B. Gillard, W. Gillis, B. Giocoli, C. Grazian, A. Grupp, F. Guzzo, L. Haugan, S.V.H. Hook, I. Hormuth, F. Hornstrup, A. Jahnke, K. Kümmel, M. Kermiche, S. Kiessling, A. Kilbinger, M. Kitching, T. Kurki-Suonio, H. Ligori, S. Lilje, P.B. Lindholm, V. Lloro, I. Maino, D. Maiorano, E. Mansutti, O. Marggraf, O. Martinet, N. Marulli, F. Massey, R. Medinaceli, E. Melchior, M. Mellier, Y. Meneghetti, M. Merlin, E. Moresco, M. Moscardini, L. Munari, E. Nichol, R.C. Niemi, S.-M. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Pettorino, V. Pires, S. Polenta, G. Poncet, M. Popa, L.A. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Schneider, P. Schrabback, T. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Stanco, L. Surace, C. Tallada-Crespí, P. Teplitz, H.I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valentijn, E.A. Vassallo, T. Veropalumbo, A. Wang, Yan Weller, J. Williams, O.R. Zoubian, J. Zucca, E. Burigana, C. Scottez, V.
author2_role	author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author
dc.subject.none.fl_str_mv	Galàxies actives Galàxies Evolució de les galàxies Active galaxies Galaxies Galaxies evolution
topic	Galàxies actives Galàxies Evolució de les galàxies Active galaxies Galaxies Galaxies evolution
description	Context. ALMA observations show that dusty, distant, massive (M∗ & 1011 M) galaxies usually have a remarkable star-formation activity, contributing of the order of 25% of the cosmic star-formation rate density at z ≈ 3–5, and up to 30% at z ∼ 7. Nonetheless, they are elusive in classical optical surveys, and current near-IR surveys are able to detect them only in very small sky areas. Since these objects have low space densities, deep and wide surveys are necessary to obtain statistically relevant results about them. Euclid will potentially be capable of delivering the required information, but, given the lack of spectroscopic features at these distances within its bands, it is still unclear if Euclid will be able to identify and characterise these objects. Aims. The goal of this work is to assess the capability of Euclid, together with ancillary optical and near-IR data, to identify these distant, dusty, and massive galaxies based on broadband photometry. Methods. We used a gradient-boosting algorithm to predict both the redshift and spectral type of objects at high z. To perform such an analysis, we made use of simulated photometric observations that mimic the Euclid Deep Survey, derived using the state-of-the-art Spectro-Photometric Realizations of Infrared-selected Targets at all-z (SPRITZ) software. Results. The gradient-boosting algorithm was found to be accurate in predicting both the redshift and spectral type of objects within the simulated Euclid Deep Survey catalogue at z > 2, while drastically decreasing the runtime with respect to spectral-energy-distribution-fitting methods. In particular, we studied the analogue of HIEROs (i.e. sources selected on the basis of a red H − [4.5] > 2.25), combining Euclid and Spitzer data at the depth of the Deep Fields. These sources include the bulk of obscured and massive galaxies in a broad redshift range, 3 < z < 7. We find that the dusty population at 3 . z . 7 is well identified, with a redshift root mean squared error and catastrophic outlier fraction of only 0.55 and 8.5% (HE ≤ 26), respectively. Our findings suggest that with Euclid we will obtain meaningful insights into the impact of massive and dusty galaxies on the cosmic star-formation rate over time.
publishDate	2024
dc.date.none.fl_str_mv	2024
dc.type.none.fl_str_mv	info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion
format	article
status_str	publishedVersion
dc.identifier.none.fl_str_mv	https://hdl.handle.net/2445/221025
url	https://hdl.handle.net/2445/221025
dc.language.none.fl_str_mv	Inglés
language_invalid_str_mv	Inglés
dc.relation.none.fl_str_mv	Reproducció del document publicat a: https://doi.org/10.1051/0004-6361/202348737 Astronomy & Astrophysics, 2024, vol. 685, num.A127 https://doi.org/10.1051/0004-6361/202348737
dc.rights.none.fl_str_mv	(c) The European Southern Observatory (ESO), 2024 info:eu-repo/semantics/openAccess
rights_invalid_str_mv	(c) The European Southern Observatory (ESO), 2024
eu_rights_str_mv	openAccess
dc.format.none.fl_str_mv	application/pdf
dc.publisher.none.fl_str_mv	EDP Sciences
publisher.none.fl_str_mv	EDP Sciences
dc.source.none.fl_str_mv	Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB)) reponame:Dipòsit Digital de la UB instname:Universidad de Barcelona
instname_str	Universidad de Barcelona
reponame_str	Dipòsit Digital de la UB
collection	Dipòsit Digital de la UB
repository.name.fl_str_mv
repository.mail.fl_str_mv
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spelling	Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted treesSignor, T.Rodighiero, G.Bisigello, L.Bolzonella, M.Caputi, K.I.Daddi, E.De Lucia, G.Enia, A.Gabarra, L.Gruppioni, C.Humphrey, A.La Franca, F.Mancini, C.Pozzetti, L.Serjeant, S.Spinoglio, L.Van Mierlo, S.E.Andreon, S.Auricchio, N.Baldi, M.Bardelli, S.Battaglia, P.Bender, R.Bodendorf, C.Bonino, D.Branchini, E.Brescia, M.Brinchmann, J.Camera, S.Capobianco, V.Carbone, C.Carretero, J.Casas, S.Castellano, M.Cavuoti, S.Cimatti, A.Cledassou, R.Congedo, G.Conselice, C.J.Conversi, L.Copin, Y.Corcione, L.Courbin, FrédéricCourtois, H.M.Da Silva, A.Degaudenzi, H.Di Giorgio, A.M.Dinis, J.Dubath, F.Dupac, X.Dusini, S.Ealet, A.Farina, M.Farrens, S.Ferriol, S.Fotopoulou, S.Franceschi, E.Galeotta, S.Garilli, B.Gillard, W.Gillis, B.Giocoli, C.Grazian, A.Grupp, F.Guzzo, L.Haugan, S.V.H.Hook, I.Hormuth, F.Hornstrup, A.Jahnke, K.Kümmel, M.Kermiche, S.Kiessling, A.Kilbinger, M.Kitching, T.Kurki-Suonio, H.Ligori, S.Lilje, P.B.Lindholm, V.Lloro, I.Maino, D.Maiorano, E.Mansutti, O.Marggraf, O.Martinet, N.Marulli, F.Massey, R.Medinaceli, E.Melchior, M.Mellier, Y.Meneghetti, M.Merlin, E.Moresco, M.Moscardini, L.Munari, E.Nichol, R.C.Niemi, S.-M.Padilla, C.Paltani, S.Pasian, F.Pedersen, K.Pettorino, V.Pires, S.Polenta, G.Poncet, M.Popa, L.A.Raison, F.Renzi, A.Rhodes, J.Riccio, G.Romelli, E.Roncarelli, M.Rossetti, E.Saglia, R.Sapone, D.Sartoris, B.Schneider, P.Schrabback, T.Secroun, A.Seidel, G.Serrano, S.Sirignano, C.Sirri, G.Stanco, L.Surace, C.Tallada-Crespí, P.Teplitz, H.I.Tereno, I.Toledo-Moreo, R.Torradeflot, F.Tutusaus, I.Valentijn, E.A.Vassallo, T.Veropalumbo, A.Wang, YanWeller, J.Williams, O.R.Zoubian, J.Zucca, E.Burigana, C.Scottez, V.Galàxies activesGalàxiesEvolució de les galàxiesActive galaxiesGalaxiesGalaxies evolutionContext. ALMA observations show that dusty, distant, massive (M∗ & 1011 M) galaxies usually have a remarkable star-formation activity, contributing of the order of 25% of the cosmic star-formation rate density at z ≈ 3–5, and up to 30% at z ∼ 7. Nonetheless, they are elusive in classical optical surveys, and current near-IR surveys are able to detect them only in very small sky areas. Since these objects have low space densities, deep and wide surveys are necessary to obtain statistically relevant results about them. Euclid will potentially be capable of delivering the required information, but, given the lack of spectroscopic features at these distances within its bands, it is still unclear if Euclid will be able to identify and characterise these objects. Aims. The goal of this work is to assess the capability of Euclid, together with ancillary optical and near-IR data, to identify these distant, dusty, and massive galaxies based on broadband photometry. Methods. We used a gradient-boosting algorithm to predict both the redshift and spectral type of objects at high z. To perform such an analysis, we made use of simulated photometric observations that mimic the Euclid Deep Survey, derived using the state-of-the-art Spectro-Photometric Realizations of Infrared-selected Targets at all-z (SPRITZ) software. Results. The gradient-boosting algorithm was found to be accurate in predicting both the redshift and spectral type of objects within the simulated Euclid Deep Survey catalogue at z > 2, while drastically decreasing the runtime with respect to spectral-energy-distribution-fitting methods. In particular, we studied the analogue of HIEROs (i.e. sources selected on the basis of a red H − [4.5] > 2.25), combining Euclid and Spitzer data at the depth of the Deep Fields. These sources include the bulk of obscured and massive galaxies in a broad redshift range, 3 < z < 7. We find that the dusty population at 3 . z . 7 is well identified, with a redshift root mean squared error and catastrophic outlier fraction of only 0.55 and 8.5% (HE ≤ 26), respectively. Our findings suggest that with Euclid we will obtain meaningful insights into the impact of massive and dusty galaxies on the cosmic star-formation rate over time. EDP Sciences2024info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttps://hdl.handle.net/2445/221025Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB))reponame:Dipòsit Digital de la UBinstname:Universidad de BarcelonaInglésReproducció del document publicat a: https://doi.org/10.1051/0004-6361/202348737Astronomy & Astrophysics, 2024, vol. 685, num.A127https://doi.org/10.1051/0004-6361/202348737(c) The European Southern Observatory (ESO), 2024info:eu-repo/semantics/openAccessoai:diposit.ub.edu:2445/2210252026-05-27T06:46:51Z
score	15,812429

Euclid: Identifying the reddest high-redshift galaxies in the Euclid Deep Fields with gradient-boosted trees

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