Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys

Scharré, L.; Hirschmann, M.; De Lucia, G.; Charlot, S.; Fontanot, F.; Spinelli, M.; Xie, L.; Feltre, A.; Allevato, V.; Plat, A.; Bremer, M.N.; Munari, E.; Niemi, S.-M.; Padilla, C.; Paltani, S.; Pasian, F.; Pedersen, K.; Pettorino, V.; Polenta, G.; Poncet, M.; Popa, L.A.; Fotopoulou, S.; Raison, F.; Renzi, A.; Rhodes, J.; Riccio, G.; Romelli, E.; Roncarelli, M.; Rossetti, E.; Saglia, R.; Sapone, D.; Sartoris, B.; Gabarra, L.; Schirmer, M.; Schneider, P.; Secroun, A.; Seidel, G.; Serrano, S.; Sirignano, C.; Sirri, G.; Stanco, L.; Surace, C.; Tallada-Crespí, P.; Granett, B.R.; Taylor, A.N.; Teplitz, H.I.; Tereno, I.; Toledo-Moreo, R.; Torradeflot, F.; Tutusaus, I.; Valenziano, L.; Vassallo, T.; Veropalumbo, A.; Wang, Y.; Moresco, M.; Weller, J.; Zoubian, J.; Zucca, E.; Biviano, A.; Bolzonella, M.; Bozzo, E.; Burigana, C.; Colodro-Conde, C.; Di Ferdinando, D.; Farinelli, R.; Scarlata, C.; Graciá-Carpio, J.; Mainetti, G.; Martinelli, M.; Mauri, N.; Neissner, C.; Nucita, A.A.; Sakr, Z.; Scottez, V.; Tenti, M.; Viel, M.; Pozzetti, L.; Wiesmann, M.; Akrami, Y.; Anselmi, S.; Baccigalupi, C.; Ballardini, M.; Bethermin, M.; Blanchard, A.; Borgani, S.; Borlaff, A.S.; Bruton, S.; Spinoglio, L.; Cabanac, R.; Calabro, A.; Cañas-Herrera, G.; Cappi, A.; Carvalho, C.S.; Castignani, G.; Castro, T.; Chambers, K.C.; Contarini, S.; Contini, T.; Talia, M.; Cooray, A.R.; Coupon, J.; Cucciati, O.; Desprez, G.; Di Domizio, S.; Dole, H.; Díaz-Sánchez, A.; Escartin Vigo, J.A.; Escoffier, S.; Ferrero, I.; Zamorani, G.; Ganga, K.; García-Bellido, J.; Gaztanaga, E.; George, K.; Giacomini, F.; Gozaliasl, G.; Gregorio, A.; Hall, A.; Hildebrandt, H.; Kajava, J.J.E.; Altieri, B.; Kansal, V.; Kirkpatrick, C.C.; Legrand, L.; Loureiro, Ana; Macias-Perez, J.; Magliocchetti, M.; Mancini, C.; Mannucci, F.; Maoli, R.; Martins, C.J.A.P.; Amara, A.; Matthew, S.; Maurin, L.; Metcalf, R.B.; Migliaccio, M.; Monaco, P.; Morgante, G.; Walton, N.A.; Pöntinen, M.; Popa, V.; Porciani, C.; Andreon, S.; Potter, D.; Risso, I.; Rocci, P.-F.; Sahlén, M.; Sánchez, A.G.; Schneider, A.; Schultheis, M.; Sereno, M.; Simon, P.; Steinwagner, J.; Auricchio, N.; Testera, G.; Tewes, M.; Teyssier, R.; Toft, Søren; Tosi, S.; Troja, A.; Tucci, M.; Valiviita, J.; Vergani, D.; Verza, G.; Baldi, M.; Zinchenko, I.A.; Bardelli, S.; Bonino, D.; Branchini, E.; Brescia, M.; Brinchmann, J.; Camera, S.; Capobianco, V.; Carbone, C.; Carretero, J.; Casas, S.; Castander, F.J.; Castellano, M.; Cavuoti, S.; Cimatti, A.; Congedo, G.; Conselice, C.J.; Conversi, L.; Copin, Y.; Corcione, L.; Courbin, Frédéric; Courtois, H.M.; Da Silva, A.; Degaudenzi, H.; Dinis, J.; Douspis, M.; Dubath, F.; Dupac, X.; Dusini, S.; Farina, M.; Farrens, S.; Ferriol, S.; Frailis, M.; Franceschi, E.; Galeotta, S.; Garilli, B.; Gillis, B.; Giocoli, C.; Grazian, A.; Grupp, F.; Guzzo, L.; Haugan, S.V.H.; Holmes, W.; Hook, I.; Hormuth, F.; Hornstrup, A.; Jahnke, K.; Keihänen, E.; Kermiche, S.; Kiessling, A.; Kitching, T.; Kubik, B.; Kümmel, M.; Kunz, M.; Kurki-Suonio, H.; Ligori, S.; Lilje, P.B.; Lindholm, V.; Lloro, I.; Maino, D.; Maiorano, E.; Mansutti, O.; Marggraf, O.; Markovic, K.; Martinet, N.; Marulli, F.; Massey, R.; Maurogordato, S.; McCracken, H.J.; Medinaceli, E.; Mei, S.; Mellier, Y.; Meneghetti, M.; Merlin, E.; Meylan, G.; Moscardini, L.

Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys

In anticipation of the upcoming Euclid Wide and Deep Surveys, we present optical emission-line predictions at intermediate redshifts from 0.4 to 2.5. Our approach combines a mock light cone from the Gaea semi-analytic model with advanced photoionisation models to construct emissionline catalogues. T...

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Detalles Bibliográficos
Autores:	Scharré, L., Hirschmann, M., De Lucia, G., Charlot, S., Fontanot, F., Spinelli, M., Xie, L., Feltre, A., Allevato, V., Plat, A., Bremer, M.N., Munari, E., Niemi, S.-M., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Pettorino, V., Polenta, G., Poncet, M., Popa, L.A., Fotopoulou, S., Raison, F., Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rossetti, E., Saglia, R., Sapone, D., Sartoris, B., Gabarra, L., Schirmer, M., Schneider, P., Secroun, A., Seidel, G., Serrano, S., Sirignano, C., Sirri, G., Stanco, L., Surace, C., Tallada-Crespí, P., Granett, B.R., Taylor, A.N., Teplitz, H.I., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valenziano, L., Vassallo, T., Veropalumbo, A., Wang, Y., Moresco, M., Weller, J., Zoubian, J., Zucca, E., Biviano, A., Bolzonella, M., Bozzo, E., Burigana, C., Colodro-Conde, C., Di Ferdinando, D., Farinelli, R., Scarlata, C., Graciá-Carpio, J., Mainetti, G., Martinelli, M., Mauri, N., Neissner, C., Nucita, A.A., Sakr, Z., Scottez, V., Tenti, M., Viel, M., Pozzetti, L., Wiesmann, M., Akrami, Y., Anselmi, S., Baccigalupi, C., Ballardini, M., Bethermin, M., Blanchard, A., Borgani, S., Borlaff, A.S., Bruton, S., Spinoglio, L., Cabanac, R., Calabro, A., Cañas-Herrera, G., Cappi, A., Carvalho, C.S., Castignani, G., Castro, T., Chambers, K.C., Contarini, S., Contini, T., Talia, M., Cooray, A.R., Coupon, J., Cucciati, O., Desprez, G., Di Domizio, S., Dole, H., Díaz-Sánchez, A., Escartin Vigo, J.A., Escoffier, S., Ferrero, I., Zamorani, G., Ganga, K., García-Bellido, J., Gaztanaga, E., George, K., Giacomini, F., Gozaliasl, G., Gregorio, A., Hall, A., Hildebrandt, H., Kajava, J.J.E., Altieri, B., Kansal, V., Kirkpatrick, C.C., Legrand, L., Loureiro, Ana, Macias-Perez, J., Magliocchetti, M., Mancini, C., Mannucci, F., Maoli, R., Martins, C.J.A.P., Amara, A., Matthew, S., Maurin, L., Metcalf, R.B., Migliaccio, M., Monaco, P., Morgante, G., Walton, N.A., Pöntinen, M., Popa, V., Porciani, C., Andreon, S., Potter, D., Risso, I., Rocci, P.-F., Sahlén, M., Sánchez, A.G., Schneider, A., Schultheis, M., Sereno, M., Simon, P., Steinwagner, J., Auricchio, N., Testera, G., Tewes, M., Teyssier, R., Toft, Søren, Tosi, S., Troja, A., Tucci, M., Valiviita, J., Vergani, D., Verza, G., Baldi, M., Zinchenko, I.A., Bardelli, S., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Capobianco, V., Carbone, C., Carretero, J., Casas, S., Castander, F.J., Castellano, M., Cavuoti, S., Cimatti, A., Congedo, G., Conselice, C.J., Conversi, L., Copin, Y., Corcione, L., Courbin, Frédéric, Courtois, H.M., Da Silva, A., Degaudenzi, H., Dinis, J., Douspis, M., Dubath, F., Dupac, X., Dusini, S., Farina, M., Farrens, S., Ferriol, S., Frailis, M., Franceschi, E., Galeotta, S., Garilli, B., Gillis, B., Giocoli, C., Grazian, A., Grupp, F., Guzzo, L., Haugan, S.V.H., Holmes, W., Hook, I., Hormuth, F., Hornstrup, A., Jahnke, K., Keihänen, E., Kermiche, S., Kiessling, A., Kitching, T., Kubik, B., Kümmel, M., Kunz, M., Kurki-Suonio, H., Ligori, S., Lilje, P.B., Lindholm, V., Lloro, I., Maino, D., Maiorano, E., Mansutti, O., Marggraf, O., Markovic, K., Martinet, N., Marulli, F., Massey, R., Maurogordato, S., McCracken, H.J., Medinaceli, E., Mei, S., Mellier, Y., Meneghetti, M., Merlin, E., Meylan, G., Moscardini, L.
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:2445/221015
Acceso en línea:	https://hdl.handle.net/2445/221015
Access Level:	acceso abierto
Palabra clave:	Evolució de les galàxies Galàxies actives Galàxies Galaxies evolution Active galaxies Galaxies

id	ES_444622e78f2358bb820d7fcbf4cced49
oai_identifier_str	oai:diposit.ub.edu:2445/221015
network_acronym_str	ES
network_name_str	España
repository_id_str
dc.title.none.fl_str_mv	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
title	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
spellingShingle	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys Scharré, L. Evolució de les galàxies Galàxies actives Galàxies Galaxies evolution Active galaxies Galaxies
title_short	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
title_full	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
title_fullStr	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
title_full_unstemmed	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
title_sort	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys
dc.creator.none.fl_str_mv	Scharré, L. Hirschmann, M. De Lucia, G. Charlot, S. Fontanot, F. Spinelli, M. Xie, L. Feltre, A. Allevato, V. Plat, A. Bremer, M.N. Munari, E. Niemi, S.-M. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Pettorino, V. Polenta, G. Poncet, M. Popa, L.A. Fotopoulou, S. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Gabarra, L. Schirmer, M. Schneider, P. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Stanco, L. Surace, C. Tallada-Crespí, P. Granett, B.R. Taylor, A.N. Teplitz, H.I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valenziano, L. Vassallo, T. Veropalumbo, A. Wang, Y. Moresco, M. Weller, J. Zoubian, J. Zucca, E. Biviano, A. Bolzonella, M. Bozzo, E. Burigana, C. Colodro-Conde, C. Di Ferdinando, D. Farinelli, R. Scarlata, C. Graciá-Carpio, J. Mainetti, G. Martinelli, M. Mauri, N. Neissner, C. Nucita, A.A. Sakr, Z. Scottez, V. Tenti, M. Viel, M. Pozzetti, L. Wiesmann, M. Akrami, Y. Anselmi, S. Baccigalupi, C. Ballardini, M. Bethermin, M. Blanchard, A. Borgani, S. Borlaff, A.S. Bruton, S. Spinoglio, L. Cabanac, R. Calabro, A. Cañas-Herrera, G. Cappi, A. Carvalho, C.S. Castignani, G. Castro, T. Chambers, K.C. Contarini, S. Contini, T. Talia, M. Cooray, A.R. Coupon, J. Cucciati, O. Desprez, G. Di Domizio, S. Dole, H. Díaz-Sánchez, A. Escartin Vigo, J.A. Escoffier, S. Ferrero, I. Zamorani, G. Ganga, K. García-Bellido, J. Gaztanaga, E. George, K. Giacomini, F. Gozaliasl, G. Gregorio, A. Hall, A. Hildebrandt, H. Kajava, J.J.E. Altieri, B. Kansal, V. Kirkpatrick, C.C. Legrand, L. Loureiro, Ana Macias-Perez, J. Magliocchetti, M. Mancini, C. Mannucci, F. Maoli, R. Martins, C.J.A.P. Amara, A. Matthew, S. Maurin, L. Metcalf, R.B. Migliaccio, M. Monaco, P. Morgante, G. Walton, N.A. Pöntinen, M. Popa, V. Porciani, C. Andreon, S. Potter, D. Risso, I. Rocci, P.-F. Sahlén, M. Sánchez, A.G. Schneider, A. Schultheis, M. Sereno, M. Simon, P. Steinwagner, J. Auricchio, N. Testera, G. Tewes, M. Teyssier, R. Toft, Søren Tosi, S. Troja, A. Tucci, M. Valiviita, J. Vergani, D. Verza, G. Baldi, M. Zinchenko, I.A. Bardelli, S. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castander, F.J. Castellano, M. Cavuoti, S. Cimatti, A. Congedo, G. Conselice, C.J. Conversi, L. Copin, Y. Corcione, L. Courbin, Frédéric Courtois, H.M. Da Silva, A. Degaudenzi, H. Dinis, J. Douspis, M. Dubath, F. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Frailis, M. Franceschi, E. Galeotta, S. Garilli, B. Gillis, B. Giocoli, C. Grazian, A. Grupp, F. Guzzo, L. Haugan, S.V.H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Jahnke, K. Keihänen, E. Kermiche, S. Kiessling, A. Kitching, T. Kubik, B. Kümmel, M. Kunz, M. Kurki-Suonio, H. Ligori, S. Lilje, P.B. Lindholm, V. Lloro, I. Maino, D. Maiorano, E. Mansutti, O. Marggraf, O. Markovic, K. Martinet, N. Marulli, F. Massey, R. Maurogordato, S. McCracken, H.J. Medinaceli, E. Mei, S. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Moscardini, L.
author	Scharré, L.
author_facet	Scharré, L. Hirschmann, M. De Lucia, G. Charlot, S. Fontanot, F. Spinelli, M. Xie, L. Feltre, A. Allevato, V. Plat, A. Bremer, M.N. Munari, E. Niemi, S.-M. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Pettorino, V. Polenta, G. Poncet, M. Popa, L.A. Fotopoulou, S. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Gabarra, L. Schirmer, M. Schneider, P. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Stanco, L. Surace, C. Tallada-Crespí, P. Granett, B.R. Taylor, A.N. Teplitz, H.I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valenziano, L. Vassallo, T. Veropalumbo, A. Wang, Y. Moresco, M. Weller, J. Zoubian, J. Zucca, E. Biviano, A. Bolzonella, M. Bozzo, E. Burigana, C. Colodro-Conde, C. Di Ferdinando, D. Farinelli, R. Scarlata, C. Graciá-Carpio, J. Mainetti, G. Martinelli, M. Mauri, N. Neissner, C. Nucita, A.A. Sakr, Z. Scottez, V. Tenti, M. Viel, M. Pozzetti, L. Wiesmann, M. Akrami, Y. Anselmi, S. Baccigalupi, C. Ballardini, M. Bethermin, M. Blanchard, A. Borgani, S. Borlaff, A.S. Bruton, S. Spinoglio, L. Cabanac, R. Calabro, A. Cañas-Herrera, G. Cappi, A. Carvalho, C.S. Castignani, G. Castro, T. Chambers, K.C. Contarini, S. Contini, T. Talia, M. Cooray, A.R. Coupon, J. Cucciati, O. Desprez, G. Di Domizio, S. Dole, H. Díaz-Sánchez, A. Escartin Vigo, J.A. Escoffier, S. Ferrero, I. Zamorani, G. Ganga, K. García-Bellido, J. Gaztanaga, E. George, K. Giacomini, F. Gozaliasl, G. Gregorio, A. Hall, A. Hildebrandt, H. Kajava, J.J.E. Altieri, B. Kansal, V. Kirkpatrick, C.C. Legrand, L. Loureiro, Ana Macias-Perez, J. Magliocchetti, M. Mancini, C. Mannucci, F. Maoli, R. Martins, C.J.A.P. Amara, A. Matthew, S. Maurin, L. Metcalf, R.B. Migliaccio, M. Monaco, P. Morgante, G. Walton, N.A. Pöntinen, M. Popa, V. Porciani, C. Andreon, S. Potter, D. Risso, I. Rocci, P.-F. Sahlén, M. Sánchez, A.G. Schneider, A. Schultheis, M. Sereno, M. Simon, P. Steinwagner, J. Auricchio, N. Testera, G. Tewes, M. Teyssier, R. Toft, Søren Tosi, S. Troja, A. Tucci, M. Valiviita, J. Vergani, D. Verza, G. Baldi, M. Zinchenko, I.A. Bardelli, S. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castander, F.J. Castellano, M. Cavuoti, S. Cimatti, A. Congedo, G. Conselice, C.J. Conversi, L. Copin, Y. Corcione, L. Courbin, Frédéric Courtois, H.M. Da Silva, A. Degaudenzi, H. Dinis, J. Douspis, M. Dubath, F. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Frailis, M. Franceschi, E. Galeotta, S. Garilli, B. Gillis, B. Giocoli, C. Grazian, A. Grupp, F. Guzzo, L. Haugan, S.V.H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Jahnke, K. Keihänen, E. Kermiche, S. Kiessling, A. Kitching, T. Kubik, B. Kümmel, M. Kunz, M. Kurki-Suonio, H. Ligori, S. Lilje, P.B. Lindholm, V. Lloro, I. Maino, D. Maiorano, E. Mansutti, O. Marggraf, O. Markovic, K. Martinet, N. Marulli, F. Massey, R. Maurogordato, S. McCracken, H.J. Medinaceli, E. Mei, S. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Moscardini, L.
author_role	author
author2	Hirschmann, M. De Lucia, G. Charlot, S. Fontanot, F. Spinelli, M. Xie, L. Feltre, A. Allevato, V. Plat, A. Bremer, M.N. Munari, E. Niemi, S.-M. Padilla, C. Paltani, S. Pasian, F. Pedersen, K. Pettorino, V. Polenta, G. Poncet, M. Popa, L.A. Fotopoulou, S. Raison, F. Renzi, A. Rhodes, J. Riccio, G. Romelli, E. Roncarelli, M. Rossetti, E. Saglia, R. Sapone, D. Sartoris, B. Gabarra, L. Schirmer, M. Schneider, P. Secroun, A. Seidel, G. Serrano, S. Sirignano, C. Sirri, G. Stanco, L. Surace, C. Tallada-Crespí, P. Granett, B.R. Taylor, A.N. Teplitz, H.I. Tereno, I. Toledo-Moreo, R. Torradeflot, F. Tutusaus, I. Valenziano, L. Vassallo, T. Veropalumbo, A. Wang, Y. Moresco, M. Weller, J. Zoubian, J. Zucca, E. Biviano, A. Bolzonella, M. Bozzo, E. Burigana, C. Colodro-Conde, C. Di Ferdinando, D. Farinelli, R. Scarlata, C. Graciá-Carpio, J. Mainetti, G. Martinelli, M. Mauri, N. Neissner, C. Nucita, A.A. Sakr, Z. Scottez, V. Tenti, M. Viel, M. Pozzetti, L. Wiesmann, M. Akrami, Y. Anselmi, S. Baccigalupi, C. Ballardini, M. Bethermin, M. Blanchard, A. Borgani, S. Borlaff, A.S. Bruton, S. Spinoglio, L. Cabanac, R. Calabro, A. Cañas-Herrera, G. Cappi, A. Carvalho, C.S. Castignani, G. Castro, T. Chambers, K.C. Contarini, S. Contini, T. Talia, M. Cooray, A.R. Coupon, J. Cucciati, O. Desprez, G. Di Domizio, S. Dole, H. Díaz-Sánchez, A. Escartin Vigo, J.A. Escoffier, S. Ferrero, I. Zamorani, G. Ganga, K. García-Bellido, J. Gaztanaga, E. George, K. Giacomini, F. Gozaliasl, G. Gregorio, A. Hall, A. Hildebrandt, H. Kajava, J.J.E. Altieri, B. Kansal, V. Kirkpatrick, C.C. Legrand, L. Loureiro, Ana Macias-Perez, J. Magliocchetti, M. Mancini, C. Mannucci, F. Maoli, R. Martins, C.J.A.P. Amara, A. Matthew, S. Maurin, L. Metcalf, R.B. Migliaccio, M. Monaco, P. Morgante, G. Walton, N.A. Pöntinen, M. Popa, V. Porciani, C. Andreon, S. Potter, D. Risso, I. Rocci, P.-F. Sahlén, M. Sánchez, A.G. Schneider, A. Schultheis, M. Sereno, M. Simon, P. Steinwagner, J. Auricchio, N. Testera, G. Tewes, M. Teyssier, R. Toft, Søren Tosi, S. Troja, A. Tucci, M. Valiviita, J. Vergani, D. Verza, G. Baldi, M. Zinchenko, I.A. Bardelli, S. Bonino, D. Branchini, E. Brescia, M. Brinchmann, J. Camera, S. Capobianco, V. Carbone, C. Carretero, J. Casas, S. Castander, F.J. Castellano, M. Cavuoti, S. Cimatti, A. Congedo, G. Conselice, C.J. Conversi, L. Copin, Y. Corcione, L. Courbin, Frédéric Courtois, H.M. Da Silva, A. Degaudenzi, H. Dinis, J. Douspis, M. Dubath, F. Dupac, X. Dusini, S. Farina, M. Farrens, S. Ferriol, S. Frailis, M. Franceschi, E. Galeotta, S. Garilli, B. Gillis, B. Giocoli, C. Grazian, A. Grupp, F. Guzzo, L. Haugan, S.V.H. Holmes, W. Hook, I. Hormuth, F. Hornstrup, A. Jahnke, K. Keihänen, E. Kermiche, S. Kiessling, A. Kitching, T. Kubik, B. Kümmel, M. Kunz, M. Kurki-Suonio, H. Ligori, S. Lilje, P.B. Lindholm, V. Lloro, I. Maino, D. Maiorano, E. Mansutti, O. Marggraf, O. Markovic, K. Martinet, N. Marulli, F. Massey, R. Maurogordato, S. McCracken, H.J. Medinaceli, E. Mei, S. Mellier, Y. Meneghetti, M. Merlin, E. Meylan, G. Moscardini, L.
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 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	Evolució de les galàxies Galàxies actives Galàxies Galaxies evolution Active galaxies Galaxies
topic	Evolució de les galàxies Galàxies actives Galàxies Galaxies evolution Active galaxies Galaxies
description	In anticipation of the upcoming Euclid Wide and Deep Surveys, we present optical emission-line predictions at intermediate redshifts from 0.4 to 2.5. Our approach combines a mock light cone from the Gaea semi-analytic model with advanced photoionisation models to construct emissionline catalogues. This has allowed us to self-consistently model nebular emission from H ii regions around young stars, and, for the first time with asemi-analytic model, narrow-line regions of active galactic nuclei (AGNs) and evolved stellar populations. Gaea, with a box size of 500 h −1 Mpc, marks the largest volume to which this set of models has been applied. We validated our methodology against observational and theoretical data at low redshift. Our analysis focusses on seven optical emission lines: Hα, Hβ, [S ii]λλ6717, 6731, [N ii]λ6584, [O i]λ6300, [O iii]λ5007, and [O ii]λλ3727, 3729. In assessing Euclid’s selection bias, we find that it predominantly observes line-emitting galaxies, which are massive (stellar mass &109 M), star-forming (specific star formation rate >10−10 yr−1 ), and metal-rich (oxygen-to-hydrogen abundance log10(O/H) + 12 > 8). We provide Euclid-observable percentages of emission-line populations in our underlying Gaea sample with a mass resolution limit of 109 M and an H-band magnitude cut of 25. We compared results with and without an estimate of interstellar dust attenuation, which we modelled using a Calzetti law with a mass-dependent scaling. According to this estimate, the presence of dust may decrease observable percentages by a further 20–30% with respect to the overall population, which presents challenges for detecting intrinsically fainter lines. We predict Euclid to observe around 30–70% of Hα-, [N ii]-, [S ii]-, and [O iii]-emitting galaxies at redshifts below one. At higher redshifts, these percentages decrease below 10%. Hβ, [O ii], and [O i] emission are expected to appear relatively faint, thus limiting observability to 5% at the lower end of their detectable redshift range, and below 1% at the higher end. This is the case both for these lines individually and in combination with other lines. For galaxies with line emission above the flux threshold in the Euclid Deep Survey, we find that BPT diagrams can effectively distinguish between different galaxy types up to around redshift 1.8, attributed to the bias towards metal-rich systems. Moreover, we show that the relationships of Hα and [Oiii]+Hβ to the star formation rate, as well as the [O iii]–AGN luminosity relation, exhibit minimal, if any, changes with increasing redshift when compared to local calibrations. Based on the line ratios [N ii]/Hα, [N ii]/[O ii], and [N ii]/[S ii], we further propose novel redshift-invariant tracers for the black hole accretion rate-to-star formation rate ratio. Lastly, we find that commonly used metallicity estimators display gradual shifts in normalisations with increasing redshift, while maintaining the overall shape of local calibrations. This is in tentative agreement with recent JWST data.
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/2445/221015
url	https://hdl.handle.net/2445/221015
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/10.1051/0004-6361/202449500 Astronomy & Astrophysics, 2024, vol. 689, num.A276 https://doi.org/10.1051/0004-6361/202449500
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
_version_	1869407081300230144
spelling	Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide SurveysScharré, L.Hirschmann, M.De Lucia, G.Charlot, S.Fontanot, F.Spinelli, M.Xie, L.Feltre, A.Allevato, V.Plat, A.Bremer, M.N.Munari, E.Niemi, S.-M.Padilla, C.Paltani, S.Pasian, F.Pedersen, K.Pettorino, V.Polenta, G.Poncet, M.Popa, L.A.Fotopoulou, S.Raison, F.Renzi, A.Rhodes, J.Riccio, G.Romelli, E.Roncarelli, M.Rossetti, E.Saglia, R.Sapone, D.Sartoris, B.Gabarra, L.Schirmer, M.Schneider, P.Secroun, A.Seidel, G.Serrano, S.Sirignano, C.Sirri, G.Stanco, L.Surace, C.Tallada-Crespí, P.Granett, B.R.Taylor, A.N.Teplitz, H.I.Tereno, I.Toledo-Moreo, R.Torradeflot, F.Tutusaus, I.Valenziano, L.Vassallo, T.Veropalumbo, A.Wang, Y.Moresco, M.Weller, J.Zoubian, J.Zucca, E.Biviano, A.Bolzonella, M.Bozzo, E.Burigana, C.Colodro-Conde, C.Di Ferdinando, D.Farinelli, R.Scarlata, C.Graciá-Carpio, J.Mainetti, G.Martinelli, M.Mauri, N.Neissner, C.Nucita, A.A.Sakr, Z.Scottez, V.Tenti, M.Viel, M.Pozzetti, L.Wiesmann, M.Akrami, Y.Anselmi, S.Baccigalupi, C.Ballardini, M.Bethermin, M.Blanchard, A.Borgani, S.Borlaff, A.S.Bruton, S.Spinoglio, L.Cabanac, R.Calabro, A.Cañas-Herrera, G.Cappi, A.Carvalho, C.S.Castignani, G.Castro, T.Chambers, K.C.Contarini, S.Contini, T.Talia, M.Cooray, A.R.Coupon, J.Cucciati, O.Desprez, G.Di Domizio, S.Dole, H.Díaz-Sánchez, A.Escartin Vigo, J.A.Escoffier, S.Ferrero, I.Zamorani, G.Ganga, K.García-Bellido, J.Gaztanaga, E.George, K.Giacomini, F.Gozaliasl, G.Gregorio, A.Hall, A.Hildebrandt, H.Kajava, J.J.E.Altieri, B.Kansal, V.Kirkpatrick, C.C.Legrand, L.Loureiro, AnaMacias-Perez, J.Magliocchetti, M.Mancini, C.Mannucci, F.Maoli, R.Martins, C.J.A.P.Amara, A.Matthew, S.Maurin, L.Metcalf, R.B.Migliaccio, M.Monaco, P.Morgante, G.Walton, N.A.Pöntinen, M.Popa, V.Porciani, C.Andreon, S.Potter, D.Risso, I.Rocci, P.-F.Sahlén, M.Sánchez, A.G.Schneider, A.Schultheis, M.Sereno, M.Simon, P.Steinwagner, J.Auricchio, N.Testera, G.Tewes, M.Teyssier, R.Toft, SørenTosi, S.Troja, A.Tucci, M.Valiviita, J.Vergani, D.Verza, G.Baldi, M.Zinchenko, I.A.Bardelli, S.Bonino, D.Branchini, E.Brescia, M.Brinchmann, J.Camera, S.Capobianco, V.Carbone, C.Carretero, J.Casas, S.Castander, F.J.Castellano, M.Cavuoti, S.Cimatti, A.Congedo, G.Conselice, C.J.Conversi, L.Copin, Y.Corcione, L.Courbin, FrédéricCourtois, H.M.Da Silva, A.Degaudenzi, H.Dinis, J.Douspis, M.Dubath, F.Dupac, X.Dusini, S.Farina, M.Farrens, S.Ferriol, S.Frailis, M.Franceschi, E.Galeotta, S.Garilli, B.Gillis, B.Giocoli, C.Grazian, A.Grupp, F.Guzzo, L.Haugan, S.V.H.Holmes, W.Hook, I.Hormuth, F.Hornstrup, A.Jahnke, K.Keihänen, E.Kermiche, S.Kiessling, A.Kitching, T.Kubik, B.Kümmel, M.Kunz, M.Kurki-Suonio, H.Ligori, S.Lilje, P.B.Lindholm, V.Lloro, I.Maino, D.Maiorano, E.Mansutti, O.Marggraf, O.Markovic, K.Martinet, N.Marulli, F.Massey, R.Maurogordato, S.McCracken, H.J.Medinaceli, E.Mei, S.Mellier, Y.Meneghetti, M.Merlin, E.Meylan, G.Moscardini, L.Evolució de les galàxiesGalàxies activesGalàxiesGalaxies evolutionActive galaxiesGalaxiesIn anticipation of the upcoming Euclid Wide and Deep Surveys, we present optical emission-line predictions at intermediate redshifts from 0.4 to 2.5. Our approach combines a mock light cone from the Gaea semi-analytic model with advanced photoionisation models to construct emissionline catalogues. This has allowed us to self-consistently model nebular emission from H ii regions around young stars, and, for the first time with asemi-analytic model, narrow-line regions of active galactic nuclei (AGNs) and evolved stellar populations. Gaea, with a box size of 500 h −1 Mpc, marks the largest volume to which this set of models has been applied. We validated our methodology against observational and theoretical data at low redshift. Our analysis focusses on seven optical emission lines: Hα, Hβ, [S ii]λλ6717, 6731, [N ii]λ6584, [O i]λ6300, [O iii]λ5007, and [O ii]λλ3727, 3729. In assessing Euclid’s selection bias, we find that it predominantly observes line-emitting galaxies, which are massive (stellar mass &109 M), star-forming (specific star formation rate >10−10 yr−1 ), and metal-rich (oxygen-to-hydrogen abundance log10(O/H) + 12 > 8). We provide Euclid-observable percentages of emission-line populations in our underlying Gaea sample with a mass resolution limit of 109 M and an H-band magnitude cut of 25. We compared results with and without an estimate of interstellar dust attenuation, which we modelled using a Calzetti law with a mass-dependent scaling. According to this estimate, the presence of dust may decrease observable percentages by a further 20–30% with respect to the overall population, which presents challenges for detecting intrinsically fainter lines. We predict Euclid to observe around 30–70% of Hα-, [N ii]-, [S ii]-, and [O iii]-emitting galaxies at redshifts below one. At higher redshifts, these percentages decrease below 10%. Hβ, [O ii], and [O i] emission are expected to appear relatively faint, thus limiting observability to 5% at the lower end of their detectable redshift range, and below 1% at the higher end. This is the case both for these lines individually and in combination with other lines. For galaxies with line emission above the flux threshold in the Euclid Deep Survey, we find that BPT diagrams can effectively distinguish between different galaxy types up to around redshift 1.8, attributed to the bias towards metal-rich systems. Moreover, we show that the relationships of Hα and [Oiii]+Hβ to the star formation rate, as well as the [O iii]–AGN luminosity relation, exhibit minimal, if any, changes with increasing redshift when compared to local calibrations. Based on the line ratios [N ii]/Hα, [N ii]/[O ii], and [N ii]/[S ii], we further propose novel redshift-invariant tracers for the black hole accretion rate-to-star formation rate ratio. Lastly, we find that commonly used metallicity estimators display gradual shifts in normalisations with increasing redshift, while maintaining the overall shape of local calibrations. This is in tentative agreement with recent JWST data.EDP Sciences2024info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttps://hdl.handle.net/2445/221015Articles 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/10.1051/0004-6361/202449500Astronomy & Astrophysics, 2024, vol. 689, num.A276https://doi.org/10.1051/0004-6361/202449500(c) The European Southern Observatory (ESO), 2024info:eu-repo/semantics/openAccessoai:diposit.ub.edu:2445/2210152026-05-27T06:46:51Z
score	15.811543

Euclid preparation: XLV. Optical emission-line predictions of intermediate-z galaxy populations in GAEA for the Euclid Deep and Wide Surveys

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