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...

Full description

Bibliographic Details
Authors: 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, S., 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, C., Carretero, J., 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., Farina, M., Farrens, S., Ferriol, S., Fourmanoit, N., Frailis, M., Franceschi, E., Franzetti, P., Fumana, M., Galeotta, S., Garilli, B., Gillard, W., Gillis, B., Giocoli, C., 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, F., 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, W.J., Pettorino, V., Polenta, G., Poncet, M., Popa, L.A., Raison, F., Rebolo, R., 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, S., Sirignano, C., Sirri, G., Stanco, L., Surace, C., Tallada-Crespí, P., Taylor, A.N., Teplitz, H.I., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E.A., Valenziano, L., Vassallo, T., Veropalumbo, A., Vibert, D., Wang, Yan, 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, Y., Anselmi, S., Baccigalupi, C., 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, S., Ferrero, I., Ganga, K., García-Bellido, J., 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, S., Patrizii, L., Pezzotta, A., Popa, V., Porciani, C., Potter, D., Pöntinen, M., Rocci, P.-F., Sánchez, A.G., Schneider, A., Sefusatti, E., Sereno, M., Shulevski, A., Simon, P., Spurio Mancini, A., Stadel, J., Stanford, S.A., Steinwagner, J., Testera, G., Teyssier, R., Toft, S., Tosi, S., Troja, A., Tucci, M., Valieri, C., Valiviita, J., Zinchenko, I.A.
Format: article
Status:Published version
Publication Date:2024
Country:España
Institution:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
Repository:Recercat. Dipósit de la Recerca de Catalunya
OAI Identifier:oai:recercat.cat:2445/221022
Online Access:https://hdl.handle.net/2445/221022
Access Level:Open access
Keyword:Galàxies actives
Forats negres (Astronomia)
Quàsars
Active galaxies
Black holes (Astronomy)
Quasars
id ES_5bea136e7e4232ad0fb6fc5c9efcc155
oai_identifier_str oai:recercat.cat:2445/221022
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.
Galàxies actives
Forats negres (Astronomia)
Quàsars
Active galaxies
Black holes (Astronomy)
Quasars
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, S.
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, C.
Carretero, J.
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.
Farina, M.
Farrens, S.
Ferriol, S.
Fourmanoit, N.
Frailis, M.
Franceschi, E.
Franzetti, P.
Fumana, M.
Galeotta, S.
Garilli, B.
Gillard, W.
Gillis, B.
Giocoli, C.
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, F.
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, W.J.
Pettorino, V.
Polenta, G.
Poncet, M.
Popa, L.A.
Raison, F.
Rebolo, R.
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, S.
Sirignano, C.
Sirri, G.
Stanco, L.
Surace, C.
Tallada-Crespí, P.
Taylor, A.N.
Teplitz, H.I.
Tereno, I.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, I.
Valentijn, E.A.
Valenziano, L.
Vassallo, T.
Veropalumbo, A.
Vibert, D.
Wang, Yan
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, Y.
Anselmi, S.
Baccigalupi, C.
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, S.
Ferrero, I.
Ganga, K.
García-Bellido, J.
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, S.
Patrizii, L.
Pezzotta, A.
Popa, V.
Porciani, C.
Potter, D.
Pöntinen, M.
Rocci, P.-F.
Sánchez, A.G.
Schneider, A.
Sefusatti, E.
Sereno, M.
Shulevski, A.
Simon, P.
Spurio Mancini, A.
Stadel, J.
Stanford, S.A.
Steinwagner, J.
Testera, G.
Teyssier, R.
Toft, S.
Tosi, S.
Troja, A.
Tucci, M.
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, S.
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, C.
Carretero, J.
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.
Farina, M.
Farrens, S.
Ferriol, S.
Fourmanoit, N.
Frailis, M.
Franceschi, E.
Franzetti, P.
Fumana, M.
Galeotta, S.
Garilli, B.
Gillard, W.
Gillis, B.
Giocoli, C.
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, F.
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, W.J.
Pettorino, V.
Polenta, G.
Poncet, M.
Popa, L.A.
Raison, F.
Rebolo, R.
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, S.
Sirignano, C.
Sirri, G.
Stanco, L.
Surace, C.
Tallada-Crespí, P.
Taylor, A.N.
Teplitz, H.I.
Tereno, I.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, I.
Valentijn, E.A.
Valenziano, L.
Vassallo, T.
Veropalumbo, A.
Vibert, D.
Wang, Yan
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, Y.
Anselmi, S.
Baccigalupi, C.
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, S.
Ferrero, I.
Ganga, K.
García-Bellido, J.
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, S.
Patrizii, L.
Pezzotta, A.
Popa, V.
Porciani, C.
Potter, D.
Pöntinen, M.
Rocci, P.-F.
Sánchez, A.G.
Schneider, A.
Sefusatti, E.
Sereno, M.
Shulevski, A.
Simon, P.
Spurio Mancini, A.
Stadel, J.
Stanford, S.A.
Steinwagner, J.
Testera, G.
Teyssier, R.
Toft, S.
Tosi, S.
Troja, A.
Tucci, M.
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, S.
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, C.
Carretero, J.
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.
Farina, M.
Farrens, S.
Ferriol, S.
Fourmanoit, N.
Frailis, M.
Franceschi, E.
Franzetti, P.
Fumana, M.
Galeotta, S.
Garilli, B.
Gillard, W.
Gillis, B.
Giocoli, C.
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, F.
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, W.J.
Pettorino, V.
Polenta, G.
Poncet, M.
Popa, L.A.
Raison, F.
Rebolo, R.
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, S.
Sirignano, C.
Sirri, G.
Stanco, L.
Surace, C.
Tallada-Crespí, P.
Taylor, A.N.
Teplitz, H.I.
Tereno, I.
Toledo-Moreo, R.
Torradeflot, F.
Tutusaus, I.
Valentijn, E.A.
Valenziano, L.
Vassallo, T.
Veropalumbo, A.
Vibert, D.
Wang, Yan
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, Y.
Anselmi, S.
Baccigalupi, C.
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, S.
Ferrero, I.
Ganga, K.
García-Bellido, J.
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, S.
Patrizii, L.
Pezzotta, A.
Popa, V.
Porciani, C.
Potter, D.
Pöntinen, M.
Rocci, P.-F.
Sánchez, A.G.
Schneider, A.
Sefusatti, E.
Sereno, M.
Shulevski, A.
Simon, P.
Spurio Mancini, A.
Stadel, J.
Stanford, S.A.
Steinwagner, J.
Testera, G.
Teyssier, R.
Toft, S.
Tosi, S.
Troja, A.
Tucci, M.
Valieri, C.
Valiviita, J.
Zinchenko, I.A.
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
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Galàxies actives
Forats negres (Astronomia)
Quàsars
Active galaxies
Black holes (Astronomy)
Quasars
topic Galàxies actives
Forats negres (Astronomia)
Quàsars
Active galaxies
Black holes (Astronomy)
Quasars
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. 
publishDate 2024
dc.date.none.fl_str_mv 2024
2025
2025
2025
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/2445/221022
url https://hdl.handle.net/2445/221022
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/10.1051/0004-6361/202348326
Astronomy & Astrophysics, 2024, vol. 685, num.A108
https://doi.org/10.1051/0004-6361/202348326
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 30 p.
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:Recercat. Dipósit de la Recerca de Catalunya
instname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
instname_str Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
reponame_str Recercat. Dipósit de la Recerca de Catalunya
collection Recercat. Dipósit de la Recerca de Catalunya
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869408849569513472
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, S.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, C.Carretero, J.Casas, 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.Farina, M.Farrens, S.Ferriol, S.Fourmanoit, N.Frailis, M.Franceschi, E.Franzetti, P.Fumana, M.Galeotta, S.Garilli, B.Gillard, W.Gillis, B.Giocoli, C.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, F.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, W.J.Pettorino, V.Polenta, G.Poncet, M.Popa, L.A.Raison, F.Rebolo, R.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, S.Sirignano, C.Sirri, G.Stanco, L.Surace, C.Tallada-Crespí, P.Taylor, A.N.Teplitz, H.I.Tereno, I.Toledo-Moreo, R.Torradeflot, F.Tutusaus, I.Valentijn, E.A.Valenziano, L.Vassallo, T.Veropalumbo, A.Vibert, D.Wang, YanWeller, 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, Y.Anselmi, S.Baccigalupi, C.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, S.Ferrero, I.Ganga, K.García-Bellido, J.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, S.Patrizii, L.Pezzotta, A.Popa, V.Porciani, C.Potter, D.Pöntinen, M.Rocci, P.-F.Sánchez, A.G.Schneider, A.Sefusatti, E.Sereno, M.Shulevski, A.Simon, P.Spurio Mancini, A.Stadel, J.Stanford, S.A.Steinwagner, J.Testera, G.Teyssier, R.Toft, S.Tosi, S.Troja, A.Tucci, M.Valieri, C.Valiviita, J.Zinchenko, I.A.Galàxies activesForats negres (Astronomia)QuàsarsActive galaxiesBlack holes (Astronomy)QuasarsThe 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. EDP Sciences2025202520242025info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersion30 p.application/pdfhttps://hdl.handle.net/2445/221022Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB))reponame:Recercat. Dipósit de la Recerca de Catalunyainstname:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)InglésReproducció del document publicat a: https://doi.org/10.1051/0004-6361/202348326Astronomy & Astrophysics, 2024, vol. 685, num.A108https://doi.org/10.1051/0004-6361/202348326(c) The European Southern Observatory (ESO), 2024info:eu-repo/semantics/openAccessoai:recercat.cat:2445/2210222026-05-29T05:05:01Z
score 15.81155