Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP

The statistical distribution and evolution of key properties of active galactic nuclei (AGN), such as their accretion rate, mass, and spin, remains a subject of open debate in astrophysics. The ESA Euclid space mission, launched on July 1 2023, promises a breakthrough in this field. We create detail...

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Detalles Bibliográficos
Autores: Lusso, E., Fotopoulou, S., Selwood, M., Allevato, V., Calderone, G., Mancini, C., Mignoli, M., Scodeggio, M., Bisigello, L., Feltre, A., Ricci, F., La Franca, F., Vergani, D., Gabarra, L., Le Brun, V., Maiorano, E., Palazzi, E., Moresco, M., Zamorani, G., Cresci, G., Jahnke, K., Humphrey, A., Landt, H., Mannucci, F., Marconi, A., Pozzetti, L., Salucci, P., Salvato, M., Shankar, F., Spinoglio, L., Stern, D., Serjeant, Stephen, Aghanim, N., Altieri, B., Amara, A., Andreon, S., Auphan, T., Auricchio, N., Baldi, M., Bardelli, S., Bender, R., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Capobianco, V., Carbone, Carmelita, Carretero, Jorge, Casas, S., Castellano, M., Cavuoti, S., Cimatti, A., Congedo, G., Conselice, C.J., Conversi, L., Copin, Y., Corcione, L., Courbin, Frédéric, Courtois, H.M., Dinis, J., Dubath, F., Duncan, C.A.J., Dupac, X., Dusini, S., Fariñas, María Dolores, Farrens, S., Ferriol, S., Fourmanoit, N., Frailis, M., Franceschi, E., Franzetti, P., Fumana, M., Galeotta, S., Garilli, B., Gillard, W., Gillis, B., Giocoli, Carlo, Grazian, A., Grupp, F., Haugan, S.V.H., Holmes, W., Hook, I., Hormuth, F., Hornstrup, A., Kümmel, M., Keihänen, E., Kermiche, S., Kubik, B., Kunz, M., Kurki-Suonio, H., Ligori, S., Lilje, P.B., Lindholm, V., Lloro, I., Mansutti, O., Marggraf, O., Markovic, K., Martinet, N., Marulli, Federico, Massey, R., Medinaceli, E., Mei, S., Mellier, Y., Merlin, E., Meylan, G., Moscardini, L., Munari, E., Niemi, S.-M., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Percival, Will J., Pettorino, V., Polenta, G., Poncet, M., Popa, L.A., Raison, F., Rebolo López, Rafael, Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rossetti, E., Saglia, R., Sapone, D., Sartoris, B., Schneider, P., Secroun, A., Seidel, G., Serrano, Santiago, Sirignano, C., Sirri, G., Stanco, L., Surace, C., Tallada-Crespí, Pau, Taylor, A.N., Teplitz, H.I., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Tutusaus, Isaac, Valentijn, E.A., Valenziano, L., Vassallo, T., Veropalumbo, A., Vibert, D., Wang, Yun, Weller, J., Zoubian, J., Zucca, E., Biviano, A., Bolzonella, M., Bozzo, E., Burigana, C., Colodro-Conde, C., Di Ferdinando, D., Graciá-Carpio, J., Mainetti, G., Mauri, N., Neissner, C., Sakr, Z., Scottez, V., Tenti, M., Viel, M., Wiesmann, M., Akrami, Yashar, Anselmi, S., Baccigalupi, Carlo, Ballardini, M., Bethermin, M., Borgani, S., Borlaff, A.S., Bruton, S., Cabanac, R., Calabro, A., Cappi, A., Carvalho, C.S., Castignani, G., Castro, T., Cañas-Herrera, G., Chambers, K.C., Cooray, A.R., Coupon, J., Cucciati, O., Davini, S., De Lucia, G., Desprez, G., Di Domizio, S., Dole, H., Díaz-Sánchez, A., Escartin Vigo, J.A., Escoffier, Stephanie, Ferrero, I., Ganga, K., García-Bellido, Juan, Giacomini, F., Gozaliasl, G., Guinet, D., Hall, A., Hildebrandt, H., Jiminez Muñoz, A., Kajava, J.J.E., Kansal, V., Kirkpatrick, C.C., Legrand, L., Loureiro, A., MacIas-Perez, J., Magliocchetti, M., Maoli, R., Martinelli, M., Martins, C.J.A.P., Matthew, S., Maturi, M., Maurin, L., Metcalf, R.B., Migliaccio, M., Monaco, P., Morgante, G., Nadathur, Seshadri, Patrizii, L., Pezzotta, Andrea, Popa, V., Porciani, C., Potter, D., Pöntinen, M., Rocci, P.-F., Sánchez, Ariel G., Schneider, A., Sefusatti, E., Raya-Sereno, M. D., Shulevski, A., Simon, P., Spurio Mancini, A., Stadel, J., Stanford, S.A., Steinwagner, J., Testera, G., Teyssier, R., Toft, Sune, Tosi, S., Troja, A., Tucci, Marco, Valieri, C., Valiviita, J., Zinchenko, I.A.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/382573
Acceso en línea:http://hdl.handle.net/10261/382573
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85193450196&doi=10.1051%2f0004-6361%2f202348326&partnerID=40&md5=4e7c7354404761fe13f8a20e7a05e276
Access Level:acceso abierto
Palabra clave:Galaxies: active
Quasars: general
Quasars: supermassive black holes
id ES_e6bf4df369603ee83e2bc174e2a2d817
oai_identifier_str oai:digital.csic.es:10261/382573
network_acronym_str ES
network_name_str España
repository_id_str
dc.title.none.fl_str_mv Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
spellingShingle Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
Lusso, E.
Galaxies: active
Quasars: general
Quasars: supermassive black holes
title_short Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title_full Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title_fullStr Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title_full_unstemmed Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
title_sort Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP
dc.creator.none.fl_str_mv Lusso, E.
Fotopoulou, S.
Selwood, M.
Allevato, V.
Calderone, G.
Mancini, C.
Mignoli, M.
Scodeggio, M.
Bisigello, L.
Feltre, A.
Ricci, F.
La Franca, F.
Vergani, D.
Gabarra, L.
Le Brun, V.
Maiorano, E.
Palazzi, E.
Moresco, M.
Zamorani, G.
Cresci, G.
Jahnke, K.
Humphrey, A.
Landt, H.
Mannucci, F.
Marconi, A.
Pozzetti, L.
Salucci, P.
Salvato, M.
Shankar, F.
Spinoglio, L.
Stern, D.
Serjeant, Stephen
Aghanim, N.
Altieri, B.
Amara, A.
Andreon, S.
Auphan, T.
Auricchio, N.
Baldi, M.
Bardelli, S.
Bender, R.
Bonino, D.
Branchini, E.
Brescia, M.
Brinchmann, J.
Camera, S.
Capobianco, V.
Carbone, Carmelita
Carretero, Jorge
Casas, S.
Castellano, M.
Cavuoti, S.
Cimatti, A.
Congedo, G.
Conselice, C.J.
Conversi, L.
Copin, Y.
Corcione, L.
Courbin, Frédéric
Courtois, H.M.
Dinis, J.
Dubath, F.
Duncan, C.A.J.
Dupac, X.
Dusini, S.
Fariñas, María Dolores
Farrens, S.
Ferriol, S.
Fourmanoit, N.
Frailis, M.
Franceschi, E.
Franzetti, P.
Fumana, M.
Galeotta, S.
Garilli, B.
Gillard, W.
Gillis, B.
Giocoli, Carlo
Grazian, A.
Grupp, F.
Haugan, S.V.H.
Holmes, W.
Hook, I.
Hormuth, F.
Hornstrup, A.
Kümmel, M.
Keihänen, E.
Kermiche, S.
Kubik, B.
Kunz, M.
Kurki-Suonio, H.
Ligori, S.
Lilje, P.B.
Lindholm, V.
Lloro, I.
Mansutti, O.
Marggraf, O.
Markovic, K.
Martinet, N.
Marulli, Federico
Massey, R.
Medinaceli, E.
Mei, S.
Mellier, Y.
Merlin, E.
Meylan, G.
Moscardini, L.
Munari, E.
Niemi, S.-M.
Padilla, C.
Paltani, S.
Pasian, F.
Pedersen, K.
Percival, Will J.
Pettorino, V.
Polenta, G.
Poncet, M.
Popa, L.A.
Raison, F.
Rebolo López, Rafael
Renzi, A.
Rhodes, J.
Riccio, G.
Romelli, E.
Roncarelli, M.
Rossetti, E.
Saglia, R.
Sapone, D.
Sartoris, B.
Schneider, P.
Secroun, A.
Seidel, G.
Serrano, Santiago
Sirignano, C.
Sirri, G.
Stanco, L.
Surace, C.
Tallada-Crespí, Pau
Taylor, A.N.
Teplitz, H.I.
Tereno, I.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, Isaac
Valentijn, E.A.
Valenziano, L.
Vassallo, T.
Veropalumbo, A.
Vibert, D.
Wang, Yun
Weller, J.
Zoubian, J.
Zucca, E.
Biviano, A.
Bolzonella, M.
Bozzo, E.
Burigana, C.
Colodro-Conde, C.
Di Ferdinando, D.
Graciá-Carpio, J.
Mainetti, G.
Mauri, N.
Neissner, C.
Sakr, Z.
Scottez, V.
Tenti, M.
Viel, M.
Wiesmann, M.
Akrami, Yashar
Anselmi, S.
Baccigalupi, Carlo
Ballardini, M.
Bethermin, M.
Borgani, S.
Borlaff, A.S.
Bruton, S.
Cabanac, R.
Calabro, A.
Cappi, A.
Carvalho, C.S.
Castignani, G.
Castro, T.
Cañas-Herrera, G.
Chambers, K.C.
Cooray, A.R.
Coupon, J.
Cucciati, O.
Davini, S.
De Lucia, G.
Desprez, G.
Di Domizio, S.
Dole, H.
Díaz-Sánchez, A.
Escartin Vigo, J.A.
Escoffier, Stephanie
Ferrero, I.
Ganga, K.
García-Bellido, Juan
Giacomini, F.
Gozaliasl, G.
Guinet, D.
Hall, A.
Hildebrandt, H.
Jiminez Muñoz, A.
Kajava, J.J.E.
Kansal, V.
Kirkpatrick, C.C.
Legrand, L.
Loureiro, A.
MacIas-Perez, J.
Magliocchetti, M.
Maoli, R.
Martinelli, M.
Martins, C.J.A.P.
Matthew, S.
Maturi, M.
Maurin, L.
Metcalf, R.B.
Migliaccio, M.
Monaco, P.
Morgante, G.
Nadathur, Seshadri
Patrizii, L.
Pezzotta, Andrea
Popa, V.
Porciani, C.
Potter, D.
Pöntinen, M.
Rocci, P.-F.
Sánchez, Ariel G.
Schneider, A.
Sefusatti, E.
Raya-Sereno, M. D.
Shulevski, A.
Simon, P.
Spurio Mancini, A.
Stadel, J.
Stanford, S.A.
Steinwagner, J.
Testera, G.
Teyssier, R.
Toft, Sune
Tosi, S.
Troja, A.
Tucci, Marco
Valieri, C.
Valiviita, J.
Zinchenko, I.A.
author Lusso, E.
author_facet Lusso, E.
Fotopoulou, S.
Selwood, M.
Allevato, V.
Calderone, G.
Mancini, C.
Mignoli, M.
Scodeggio, M.
Bisigello, L.
Feltre, A.
Ricci, F.
La Franca, F.
Vergani, D.
Gabarra, L.
Le Brun, V.
Maiorano, E.
Palazzi, E.
Moresco, M.
Zamorani, G.
Cresci, G.
Jahnke, K.
Humphrey, A.
Landt, H.
Mannucci, F.
Marconi, A.
Pozzetti, L.
Salucci, P.
Salvato, M.
Shankar, F.
Spinoglio, L.
Stern, D.
Serjeant, Stephen
Aghanim, N.
Altieri, B.
Amara, A.
Andreon, S.
Auphan, T.
Auricchio, N.
Baldi, M.
Bardelli, S.
Bender, R.
Bonino, D.
Branchini, E.
Brescia, M.
Brinchmann, J.
Camera, S.
Capobianco, V.
Carbone, Carmelita
Carretero, Jorge
Casas, S.
Castellano, M.
Cavuoti, S.
Cimatti, A.
Congedo, G.
Conselice, C.J.
Conversi, L.
Copin, Y.
Corcione, L.
Courbin, Frédéric
Courtois, H.M.
Dinis, J.
Dubath, F.
Duncan, C.A.J.
Dupac, X.
Dusini, S.
Fariñas, María Dolores
Farrens, S.
Ferriol, S.
Fourmanoit, N.
Frailis, M.
Franceschi, E.
Franzetti, P.
Fumana, M.
Galeotta, S.
Garilli, B.
Gillard, W.
Gillis, B.
Giocoli, Carlo
Grazian, A.
Grupp, F.
Haugan, S.V.H.
Holmes, W.
Hook, I.
Hormuth, F.
Hornstrup, A.
Kümmel, M.
Keihänen, E.
Kermiche, S.
Kubik, B.
Kunz, M.
Kurki-Suonio, H.
Ligori, S.
Lilje, P.B.
Lindholm, V.
Lloro, I.
Mansutti, O.
Marggraf, O.
Markovic, K.
Martinet, N.
Marulli, Federico
Massey, R.
Medinaceli, E.
Mei, S.
Mellier, Y.
Merlin, E.
Meylan, G.
Moscardini, L.
Munari, E.
Niemi, S.-M.
Padilla, C.
Paltani, S.
Pasian, F.
Pedersen, K.
Percival, Will J.
Pettorino, V.
Polenta, G.
Poncet, M.
Popa, L.A.
Raison, F.
Rebolo López, Rafael
Renzi, A.
Rhodes, J.
Riccio, G.
Romelli, E.
Roncarelli, M.
Rossetti, E.
Saglia, R.
Sapone, D.
Sartoris, B.
Schneider, P.
Secroun, A.
Seidel, G.
Serrano, Santiago
Sirignano, C.
Sirri, G.
Stanco, L.
Surace, C.
Tallada-Crespí, Pau
Taylor, A.N.
Teplitz, H.I.
Tereno, I.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, Isaac
Valentijn, E.A.
Valenziano, L.
Vassallo, T.
Veropalumbo, A.
Vibert, D.
Wang, Yun
Weller, J.
Zoubian, J.
Zucca, E.
Biviano, A.
Bolzonella, M.
Bozzo, E.
Burigana, C.
Colodro-Conde, C.
Di Ferdinando, D.
Graciá-Carpio, J.
Mainetti, G.
Mauri, N.
Neissner, C.
Sakr, Z.
Scottez, V.
Tenti, M.
Viel, M.
Wiesmann, M.
Akrami, Yashar
Anselmi, S.
Baccigalupi, Carlo
Ballardini, M.
Bethermin, M.
Borgani, S.
Borlaff, A.S.
Bruton, S.
Cabanac, R.
Calabro, A.
Cappi, A.
Carvalho, C.S.
Castignani, G.
Castro, T.
Cañas-Herrera, G.
Chambers, K.C.
Cooray, A.R.
Coupon, J.
Cucciati, O.
Davini, S.
De Lucia, G.
Desprez, G.
Di Domizio, S.
Dole, H.
Díaz-Sánchez, A.
Escartin Vigo, J.A.
Escoffier, Stephanie
Ferrero, I.
Ganga, K.
García-Bellido, Juan
Giacomini, F.
Gozaliasl, G.
Guinet, D.
Hall, A.
Hildebrandt, H.
Jiminez Muñoz, A.
Kajava, J.J.E.
Kansal, V.
Kirkpatrick, C.C.
Legrand, L.
Loureiro, A.
MacIas-Perez, J.
Magliocchetti, M.
Maoli, R.
Martinelli, M.
Martins, C.J.A.P.
Matthew, S.
Maturi, M.
Maurin, L.
Metcalf, R.B.
Migliaccio, M.
Monaco, P.
Morgante, G.
Nadathur, Seshadri
Patrizii, L.
Pezzotta, Andrea
Popa, V.
Porciani, C.
Potter, D.
Pöntinen, M.
Rocci, P.-F.
Sánchez, Ariel G.
Schneider, A.
Sefusatti, E.
Raya-Sereno, M. D.
Shulevski, A.
Simon, P.
Spurio Mancini, A.
Stadel, J.
Stanford, S.A.
Steinwagner, J.
Testera, G.
Teyssier, R.
Toft, Sune
Tosi, S.
Troja, A.
Tucci, Marco
Valieri, C.
Valiviita, J.
Zinchenko, I.A.
author_role author
author2 Fotopoulou, S.
Selwood, M.
Allevato, V.
Calderone, G.
Mancini, C.
Mignoli, M.
Scodeggio, M.
Bisigello, L.
Feltre, A.
Ricci, F.
La Franca, F.
Vergani, D.
Gabarra, L.
Le Brun, V.
Maiorano, E.
Palazzi, E.
Moresco, M.
Zamorani, G.
Cresci, G.
Jahnke, K.
Humphrey, A.
Landt, H.
Mannucci, F.
Marconi, A.
Pozzetti, L.
Salucci, P.
Salvato, M.
Shankar, F.
Spinoglio, L.
Stern, D.
Serjeant, Stephen
Aghanim, N.
Altieri, B.
Amara, A.
Andreon, S.
Auphan, T.
Auricchio, N.
Baldi, M.
Bardelli, S.
Bender, R.
Bonino, D.
Branchini, E.
Brescia, M.
Brinchmann, J.
Camera, S.
Capobianco, V.
Carbone, Carmelita
Carretero, Jorge
Casas, S.
Castellano, M.
Cavuoti, S.
Cimatti, A.
Congedo, G.
Conselice, C.J.
Conversi, L.
Copin, Y.
Corcione, L.
Courbin, Frédéric
Courtois, H.M.
Dinis, J.
Dubath, F.
Duncan, C.A.J.
Dupac, X.
Dusini, S.
Fariñas, María Dolores
Farrens, S.
Ferriol, S.
Fourmanoit, N.
Frailis, M.
Franceschi, E.
Franzetti, P.
Fumana, M.
Galeotta, S.
Garilli, B.
Gillard, W.
Gillis, B.
Giocoli, Carlo
Grazian, A.
Grupp, F.
Haugan, S.V.H.
Holmes, W.
Hook, I.
Hormuth, F.
Hornstrup, A.
Kümmel, M.
Keihänen, E.
Kermiche, S.
Kubik, B.
Kunz, M.
Kurki-Suonio, H.
Ligori, S.
Lilje, P.B.
Lindholm, V.
Lloro, I.
Mansutti, O.
Marggraf, O.
Markovic, K.
Martinet, N.
Marulli, Federico
Massey, R.
Medinaceli, E.
Mei, S.
Mellier, Y.
Merlin, E.
Meylan, G.
Moscardini, L.
Munari, E.
Niemi, S.-M.
Padilla, C.
Paltani, S.
Pasian, F.
Pedersen, K.
Percival, Will J.
Pettorino, V.
Polenta, G.
Poncet, M.
Popa, L.A.
Raison, F.
Rebolo López, Rafael
Renzi, A.
Rhodes, J.
Riccio, G.
Romelli, E.
Roncarelli, M.
Rossetti, E.
Saglia, R.
Sapone, D.
Sartoris, B.
Schneider, P.
Secroun, A.
Seidel, G.
Serrano, Santiago
Sirignano, C.
Sirri, G.
Stanco, L.
Surace, C.
Tallada-Crespí, Pau
Taylor, A.N.
Teplitz, H.I.
Tereno, I.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, Isaac
Valentijn, E.A.
Valenziano, L.
Vassallo, T.
Veropalumbo, A.
Vibert, D.
Wang, Yun
Weller, J.
Zoubian, J.
Zucca, E.
Biviano, A.
Bolzonella, M.
Bozzo, E.
Burigana, C.
Colodro-Conde, C.
Di Ferdinando, D.
Graciá-Carpio, J.
Mainetti, G.
Mauri, N.
Neissner, C.
Sakr, Z.
Scottez, V.
Tenti, M.
Viel, M.
Wiesmann, M.
Akrami, Yashar
Anselmi, S.
Baccigalupi, Carlo
Ballardini, M.
Bethermin, M.
Borgani, S.
Borlaff, A.S.
Bruton, S.
Cabanac, R.
Calabro, A.
Cappi, A.
Carvalho, C.S.
Castignani, G.
Castro, T.
Cañas-Herrera, G.
Chambers, K.C.
Cooray, A.R.
Coupon, J.
Cucciati, O.
Davini, S.
De Lucia, G.
Desprez, G.
Di Domizio, S.
Dole, H.
Díaz-Sánchez, A.
Escartin Vigo, J.A.
Escoffier, Stephanie
Ferrero, I.
Ganga, K.
García-Bellido, Juan
Giacomini, F.
Gozaliasl, G.
Guinet, D.
Hall, A.
Hildebrandt, H.
Jiminez Muñoz, A.
Kajava, J.J.E.
Kansal, V.
Kirkpatrick, C.C.
Legrand, L.
Loureiro, A.
MacIas-Perez, J.
Magliocchetti, M.
Maoli, R.
Martinelli, M.
Martins, C.J.A.P.
Matthew, S.
Maturi, M.
Maurin, L.
Metcalf, R.B.
Migliaccio, M.
Monaco, P.
Morgante, G.
Nadathur, Seshadri
Patrizii, L.
Pezzotta, Andrea
Popa, V.
Porciani, C.
Potter, D.
Pöntinen, M.
Rocci, P.-F.
Sánchez, Ariel G.
Schneider, A.
Sefusatti, E.
Raya-Sereno, M. D.
Shulevski, A.
Simon, P.
Spurio Mancini, A.
Stadel, J.
Stanford, S.A.
Steinwagner, J.
Testera, G.
Teyssier, R.
Toft, Sune
Tosi, S.
Troja, A.
Tucci, Marco
Valieri, C.
Valiviita, J.
Zinchenko, I.A.
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dc.contributor.none.fl_str_mv Agencia Estatal de Investigación (España)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Galaxies: active
Quasars: general
Quasars: supermassive black holes
topic Galaxies: active
Quasars: general
Quasars: supermassive black holes
description The statistical distribution and evolution of key properties of active galactic nuclei (AGN), such as their accretion rate, mass, and spin, remains a subject of open debate in astrophysics. The ESA Euclid space mission, launched on July 1 2023, promises a breakthrough in this field. We create detailed mock catalogues of AGN spectra from the rest-frame near-infrared down to the ultraviolet -including emission lines -to simulate what Euclid will observe for both obscured (type 2) and unobscured (type 1) AGN. We concentrate on the red grisms of the NISP instrument, which will be used for the wide-field survey, opening a new window for spectroscopic AGN studies in the near-infrared. We quantify the efficiency in the redshift determination as well as in retrieving the emission line flux of the Hα+[N II] complex, as Euclid is mainly focused on this emission line, given that it is expected to be the brightest one in the probed redshift range. Spectroscopic redshifts are measured for 83% of the simulated AGN in the interval where the Hα is visible (i.e. 0.89 < z < 1.83 at a line flux of > 2 × 10-16 erg s-1 cm-2, encompassing the peak of AGN activity at z ≃ 1 - 1.5) within the spectral coverage of the red grism. Outside this redshift range, the measurement efficiency decreases significantly. Overall, a spectroscopic redshift iscorrectly determined for about 90% of type 2 AGN down to an emission line flux of roughly 3 × 10-16 erg s-1 cm-2, and for type 1 AGN down to 8.5 × 10-16 erg s-1 cm-2. Recovered values for black hole mass show a small offset with respect to the input values by about 10%, but the agreement is good overall. With such a high spectroscopic coverage at z < 2, we will be able to measure AGN demography, scaling relations, and clustering from the epoch of the peak of AGN activity down to the present-day Universe for hundreds of thousands of AGN with homogeneous spectroscopic information. © 2024 EDP Sciences. All rights reserved.
publishDate 2024
dc.date.none.fl_str_mv 2024
2025
2025
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/382573
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85193450196&doi=10.1051%2f0004-6361%2f202348326&partnerID=40&md5=4e7c7354404761fe13f8a20e7a05e276
url http://hdl.handle.net/10261/382573
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85193450196&doi=10.1051%2f0004-6361%2f202348326&partnerID=40&md5=4e7c7354404761fe13f8a20e7a05e276
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv https://doi.org/10.1051/0004-6361/202348326

dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
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 reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869422793774333952
spelling Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISPLusso, E.Fotopoulou, S.Selwood, M.Allevato, V.Calderone, G.Mancini, C.Mignoli, M.Scodeggio, M.Bisigello, L.Feltre, A.Ricci, F.La Franca, F.Vergani, D.Gabarra, L.Le Brun, V.Maiorano, E.Palazzi, E.Moresco, M.Zamorani, G.Cresci, G.Jahnke, K.Humphrey, A.Landt, H.Mannucci, F.Marconi, A.Pozzetti, L.Salucci, P.Salvato, M.Shankar, F.Spinoglio, L.Stern, D.Serjeant, StephenAghanim, N.Altieri, B.Amara, A.Andreon, S.Auphan, T.Auricchio, N.Baldi, M.Bardelli, S.Bender, R.Bonino, D.Branchini, E.Brescia, M.Brinchmann, J.Camera, S.Capobianco, V.Carbone, CarmelitaCarretero, JorgeCasas, S.Castellano, M.Cavuoti, S.Cimatti, A.Congedo, G.Conselice, C.J.Conversi, L.Copin, Y.Corcione, L.Courbin, FrédéricCourtois, H.M.Dinis, J.Dubath, F.Duncan, C.A.J.Dupac, X.Dusini, S.Fariñas, María DoloresFarrens, S.Ferriol, S.Fourmanoit, N.Frailis, M.Franceschi, E.Franzetti, P.Fumana, M.Galeotta, S.Garilli, B.Gillard, W.Gillis, B.Giocoli, CarloGrazian, A.Grupp, F.Haugan, S.V.H.Holmes, W.Hook, I.Hormuth, F.Hornstrup, A.Kümmel, M.Keihänen, E.Kermiche, S.Kubik, B.Kunz, M.Kurki-Suonio, H.Ligori, S.Lilje, P.B.Lindholm, V.Lloro, I.Mansutti, O.Marggraf, O.Markovic, K.Martinet, N.Marulli, FedericoMassey, R.Medinaceli, E.Mei, S.Mellier, Y.Merlin, E.Meylan, G.Moscardini, L.Munari, E.Niemi, S.-M.Padilla, C.Paltani, S.Pasian, F.Pedersen, K.Percival, Will J.Pettorino, V.Polenta, G.Poncet, M.Popa, L.A.Raison, F.Rebolo López, RafaelRenzi, A.Rhodes, J.Riccio, G.Romelli, E.Roncarelli, M.Rossetti, E.Saglia, R.Sapone, D.Sartoris, B.Schneider, P.Secroun, A.Seidel, G.Serrano, SantiagoSirignano, C.Sirri, G.Stanco, L.Surace, C.Tallada-Crespí, PauTaylor, A.N.Teplitz, H.I.Tereno, I.Toledo-Moreo, R.Torradeflot, F.Tutusaus, IsaacValentijn, E.A.Valenziano, L.Vassallo, T.Veropalumbo, A.Vibert, D.Wang, YunWeller, J.Zoubian, J.Zucca, E.Biviano, A.Bolzonella, M.Bozzo, E.Burigana, C.Colodro-Conde, C.Di Ferdinando, D.Graciá-Carpio, J.Mainetti, G.Mauri, N.Neissner, C.Sakr, Z.Scottez, V.Tenti, M.Viel, M.Wiesmann, M.Akrami, YasharAnselmi, S.Baccigalupi, CarloBallardini, M.Bethermin, M.Borgani, S.Borlaff, A.S.Bruton, S.Cabanac, R.Calabro, A.Cappi, A.Carvalho, C.S.Castignani, G.Castro, T.Cañas-Herrera, G.Chambers, K.C.Cooray, A.R.Coupon, J.Cucciati, O.Davini, S.De Lucia, G.Desprez, G.Di Domizio, S.Dole, H.Díaz-Sánchez, A.Escartin Vigo, J.A.Escoffier, StephanieFerrero, I.Ganga, K.García-Bellido, JuanGiacomini, F.Gozaliasl, G.Guinet, D.Hall, A.Hildebrandt, H.Jiminez Muñoz, A.Kajava, J.J.E.Kansal, V.Kirkpatrick, C.C.Legrand, L.Loureiro, A.MacIas-Perez, J.Magliocchetti, M.Maoli, R.Martinelli, M.Martins, C.J.A.P.Matthew, S.Maturi, M.Maurin, L.Metcalf, R.B.Migliaccio, M.Monaco, P.Morgante, G.Nadathur, SeshadriPatrizii, L.Pezzotta, AndreaPopa, V.Porciani, C.Potter, D.Pöntinen, M.Rocci, P.-F.Sánchez, Ariel G.Schneider, A.Sefusatti, E.Raya-Sereno, M. D.Shulevski, A.Simon, P.Spurio Mancini, A.Stadel, J.Stanford, S.A.Steinwagner, J.Testera, G.Teyssier, R.Toft, SuneTosi, S.Troja, A.Tucci, MarcoValieri, C.Valiviita, J.Zinchenko, I.A.Galaxies: activeQuasars: generalQuasars: supermassive black holesThe statistical distribution and evolution of key properties of active galactic nuclei (AGN), such as their accretion rate, mass, and spin, remains a subject of open debate in astrophysics. The ESA Euclid space mission, launched on July 1 2023, promises a breakthrough in this field. We create detailed mock catalogues of AGN spectra from the rest-frame near-infrared down to the ultraviolet -including emission lines -to simulate what Euclid will observe for both obscured (type 2) and unobscured (type 1) AGN. We concentrate on the red grisms of the NISP instrument, which will be used for the wide-field survey, opening a new window for spectroscopic AGN studies in the near-infrared. We quantify the efficiency in the redshift determination as well as in retrieving the emission line flux of the Hα+[N II] complex, as Euclid is mainly focused on this emission line, given that it is expected to be the brightest one in the probed redshift range. Spectroscopic redshifts are measured for 83% of the simulated AGN in the interval where the Hα is visible (i.e. 0.89 < z < 1.83 at a line flux of > 2 × 10-16 erg s-1 cm-2, encompassing the peak of AGN activity at z ≃ 1 - 1.5) within the spectral coverage of the red grism. Outside this redshift range, the measurement efficiency decreases significantly. Overall, a spectroscopic redshift iscorrectly determined for about 90% of type 2 AGN down to an emission line flux of roughly 3 × 10-16 erg s-1 cm-2, and for type 1 AGN down to 8.5 × 10-16 erg s-1 cm-2. Recovered values for black hole mass show a small offset with respect to the input values by about 10%, but the agreement is good overall. With such a high spectroscopic coverage at z < 2, we will be able to measure AGN demography, scaling relations, and clustering from the epoch of the peak of AGN activity down to the present-day Universe for hundreds of thousands of AGN with homogeneous spectroscopic information. © 2024 EDP Sciences. All rights reserved.We thank the anonymous reviewer for their thorough reading and for useful comments and suggestions that have improved the clarity of the paper. V. A. acknowledges support from INAF-PRIN 1.05.01.85.08. L. B. acknowledges financial support from grant PRIN2017. A. F. acknowledges the support from project “VLT-MOONS” CRAM 1.05.03.07, INAF Large Grant 2022 “The metal circle: a new sharp view of the baryon cycle up to Cosmic Dawn with the latest generation IFU facilities” and INAF Large Grant 2022 “Dual and binary SMBH in the multi-messenger era”. F. S. acknowledges partial support from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 860744. The Euclid Consortium acknowledges the European Space Agency and a number of agencies and institutes that have supported the development of Euclid, in particular the Academy of Finland, the Agenzia Spaziale Italiana, the Belgian Science Policy, the Canadian Euclid Consortium, the French Centre National d’Études Spatiales, the Deutsches Zentrum für Luft- und Raumfahrt, the Danish Space Research Institute, the Fundação para a Ciência e a Tecnologia, the Ministerio de Ciencia e Innovación, the National Aeronautics and Space Administration, the National Astronomical Observatory of Japan, the Netherlandse Onderzoekschool Voor Astronomie, the Norwegian Space Agency, the Romanian Space Agency, the State Secretariat for Education, Research and Innovation (SERI) at the Swiss Space Office (SSO), and the United Kingdom Space Agency. A complete and detailed list is available on the Euclid web site (http://www.euclid-ec.org)Peer reviewedEDP SciencesAgencia Estatal de Investigación (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202520252024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/382573https://www.scopus.com/inward/record.uri?eid=2-s2.0-85193450196&doi=10.1051%2f0004-6361%2f202348326&partnerID=40&md5=4e7c7354404761fe13f8a20e7a05e276reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttps://doi.org/10.1051/0004-6361/202348326Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3825732026-05-22T06:33:51Z
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