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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Louis Gabarra

Postdoctoral Research Assistant

Sub department

  • Astrophysics
louis.gabarra@physics.ox.ac.uk
Denys Wilkinson Building, room 562
  • About
  • Publications

Euclid. I. Overview of the Euclid mission

Astronomy & Astrophysics EDP Sciences (2024)

Authors:

Y Mellier, Abdurroúf, JA Acevedo Barroso, A Achucarro, J Adamek, R Adam, GE Addison, N Aghanim, M Aguena, V Ajani, Y Akrami, A Al-Bahlawan, A Alavi, IS Albuquerque, G Alestas, G Alguero, A Allaoui, SW Allen, V Allevato, AV Alonso-Tetilla, B Altieri, A Alvarez-Candal, S Alvi, A Amara, L Amendola, J Amiaux, IT Andika, S Andreon, A Andrews, G Angora, RE Angulo, F Annibali, A Anselmi, S Anselmi, S Arcari, M Archidiacono, G Aricò, M Arnaud, S Arnouts, M Asgari, J Asorey, L Atayde, H Atek, F Atrio-Barandela, M Aubert, E Aubourg, T Auphan, N Auricchio, B Aussel, H Aussel, P Avelino, A Avgoustidis, S Avila, S Awan, R Azzollini, C Baccigalupi, E Bachelet, D Bacon, M Baes, MB Bagley, B Bahr-Kalus, A Balaguera-Antolinez, E Balbinot, M Balcells, M Baldi, I Baldry, A Balestra, M Ballardini, O Ballester, M Balogh, E Banados, R Barbier, S Bardelli, M Baron, T Barreiro, R Barrena, J-C Barriere, BJ Barros, A Barthelemy, N Bartolo, A Basset, P Battaglia, AJ Battisti, CM Baugh, L Baumont, L Bazzanini, J-P Beaulieu, V Beckmann, AN Belikov, J Bel, F Bellagamba, M Bella, E Bellini, K Benabed, R Bender, G Benevento, CL Bennett, K Benson, P Bergamini, JR Bermejo-Climent, F Bernardeau, D Bertacca, M Berthe, J Berthier, M Bethermin, F Beutler, C Bevillon, S Bhargava, R Bhatawdekar, D Bianchi, L Bisigello, A Biviano, RP Blake, A Blanchard, J Blazek, L Blot, A Bosco, C Bodendorf, T Boenke, H B\"ohringer, P Boldrini, M Bolzonella, A Bonchi, M Bonici, D Bonino, L Bonino, C Bonvin, W Bon, JT Booth, S Borgani, AS Borlaff, E Borsato, A Bosco, B Bose, MT Botticella, A Boucaud, F Bouche, JS Boucher, D Boutigny, T Bouvard, R Bouwens, H Bouy, RA Bowler, V Bozza, E Bozzo, E Branchini, G Brando, S Brau-Nogue, P Brekke, MN Bremer, M Brescia, M-A Breton, J Brinchmann, T Brinckmann, C Brockley-Blatt, M Brodwin, L Brouard, ML Brown, S Bruton, J Bucko, H Buddelmeijer, G Buenadicha, F Buitrago, P Burger, C Burigana, V Busillo, D Busonero, R Cabanac, L Cabayol-Garcia, MS Cagliari, A Caillat, L Caillat, M Calabrese, A Calabro, G Calderone, F Calura, B Camacho Quevedo, S Camera, L Campos, n, GP Candini, M Cantiello, V Capobianco, E Cappellaro, N Cappelluti, A Cappi, KI Caputi, C Cara, C Carbone, VF Cardone, E Carella, RG Carlberg, M Carle, L Carminati, F Caro, JM Carrasco, J Carretero, P Carrilho, J Carron Duque, B Carry, A Carvalho, CS Carvalho, R Casas, S Casas, P Casenove, CM Casey, P Cassata, FJ Castander, D Castelao, M Castellano, L Castiblanco, G Castignani, T Castro, C Cavet, S Cavuoti, P-Y Chabaud, KC Chambers, Y Charles, S Charlot, N Chartab, R Chary, F Chaumeil, H Cho, G Chon, E Ciancetta, P Ciliegi, A Cimatti, M Cimino, LM-R Cioni, R Claydon, C Cleland, B Cl'ement, DL Clements, N Clerc, S Clesse, S Codis, F Cogato, J Colbert, RE Cole, P Coles, TE Collett, RS Collins, C Colodro-Conde, C Colombo, F Combes, V Conforti, G Congedo, S Conseil, CJ Conselice, S Contarini, T Contini, L Conversi, AR Cooray, Y Copin, P-S Corasaniti, P Corcho-Caballero, L Corcione, O Cordes, O Corpace, M Correnti, M Costanzi, A Costille, F Courbin, L Courcoult Mifsud, HM Courtois, M-C Cousinou, G Covone, T Cowell, C Cragg, G Cresci, S Cristiani, M Crocce, M Cropper, P E Crouzet, B Csizi, J-G Cuby, E Cucchetti, O Cucciati, J-C Cuillandre, PAC Cunha, V Cuozzo, E Daddi, M D'Addona, C Dafonte, N Dagoneau, E Dalessandro, GB Dalton, G D'Amico, H Dannerbauer, P Danto, I Das, A Da Silva, R da Silva, W d'Assignies Doumerg, G Daste, JE Davies, S Davini, P Dayal, T de Boer, R Decarli, B De Caro, H Degaudenzi, G Degni, JTA de Jong, LF de la Bella, S de la Torre, F Delhaise, D Delley, G Delucchi, G De Lucia, J Denniston, F De Paolis, M De Petris, A Derosa, S Desai, V Desjacques, G Despali, G Desprez, J De Vicente-Albendea, Y Deville, JDF Dias, A Díaz-Sánchez, J Diaz, S Di Domizio, JM Diego, D Di Ferdinando, AM Di Giorgio, P Dimauro, J Dinis, K Dolag, C Dolding, H Dole, H Domínguez Sánchez, O Doré, F Dournac, M Douspis, H Dreihahn, B Droge, B Dryer, F Dubath, P-A Duc, F Ducret, C Duffy, F Dufresne, CAJ Duncan, X Dupac, V Duret, R Durrer, F Durret, S Dusini, A Ealet, A Eggemeier, PRM Eisenhardt, D Elbaz, MY Elkhashab, A Ellien, J Endicott, A Enia, T Erben, JA Escartin Vigo, S Escoffier, I Escudero Sanz, J Essert, S Ettori, M Ezziati, G Fabbian, M Fabricius, Y Fang, A Farina, M Farina, R Farinelli, S Farrens, F Faustini, A Feltre, AMN Ferguson, P Ferrando, AG Ferrari, A Ferré-Mateu, PG Ferreira, I Ferreras, I Ferrero, S Ferriol, P Ferruit, D Filleul, F Finelli, SL Finkelstein, A Finoguenov, B Fiorini, F Flentge, P Focardi, J Fonseca, A Fontana, F Fontanot, F Fornari, P Fosalba, M Fossati, S Fotopoulou, D Fouchez, N Fourmanoit, M Frailis, D Fraix-Burnet, E Franceschi, A Franco, P Franzetti, J Freihoefer, CS Frenk, G Frittoli, P-A Frugier, N Frusciante, A Fumagalli, M Fumagalli, M Fumana, Y Fu, L Gabarra, S Galeotta, L Galluccio, K Ganga, H Gao, J Garc'ia-Bellido, K Garcia, JP Gardner, B Garilli, L-M Gaspar-Venancio, T Gasparetto, V Gautard, R Gavazzi, E Gaztanaga, L Genolet, R Genova Santos, F Gentile, K George, M Gerbino, Z Ghaffari, F Giacomini, F Gianotti, GPS Gibb, W Gillard, B Gillis, M Ginolfi, C Giocoli, M Girardi, SK Giri, LWK Goh, P G'omez-Alvarez, V Gonzalez-Perez, AH Gonzalez, EJ Gonzalez, JC Gonzalez, S Gouyou Beauchamps, G Gozaliasl, J Gracia-Carpio, S Grandis, BR Granett, M Granvik, A Grazian, A Gregorio, C Grenet, C Grillo, F Grupp, C Gruppioni, A Gruppuso, C Guerbuez, S Guerrini, M Guidi, P Guillard, CM Gutierrez, P Guttridge, L Guzzo, S Gwyn, J Haapala, J Haase, CR Haddow, M Hailey, A Hall, D Hall, N Hamaus, BS Haridasu, J Harnois-D'eraps, C Harper, WG Hartley, G Hasinger, F Hassani, NA Hatch, SVH Haugan, B Haussler, A Heavens, L Heisenberg, A Helmi, G Helou, S Hemmati, K Henares, O Herent, C Hern'andez-Monteagudo, T Heuberger, PC Hewett, S Heydenreich, H Hildebrandt, M Hirschmann, J Hjorth, J Hoar, H Hoekstra, AD Holland, MS Holliman, W Holmes, I Hook, B Horeau, F Hormuth, A Hornstrup, S Hosseini, D Hu, P Hudelot, MJ Hudson, M Huertas-Company, EM Huff, ACN Hughes, A Humphrey, LK Hunt, D Huynh, R Ibata, K Ichikawa, S Iglesias-Groth, O Ilbert, S Ili'c, L Ingoglia, E Iodice, H Israel, UE Israelsson, L Izzo, P Jablonka, N Jackson, J Jacobson, M Jafariyazani, K Jahnke, B Jain, H Jansen, MJ Jarvis, J Jasche, M Jauzac, N Jeffrey, M Jhabvala, Y Jimenez-Teja, A Jimenez Munoz, B Joachimi, PH Johansson, S Joudaki, E Jullo, JE Kajava, Y Kang, A Kannawadi, V Kansal, D Karagiannis, M Karcher, A Kashlinsky, MV Kazandjian, F Keck, E Keihanen, E Kerins, S Kermiche, A Khalil, A Kiessling, K Kiiveri, M Kilbinger, J Kim, R King, C Kirkpatrick, T Kitching, M Kluge, M Knabenhans, JH Knapen, A Knebe, J-P Kneib, R Kohley, LVE Koopmans, H Koskinen, E Koulouridis, R Kou, A Kov'acs, I Kova, c, i, c, A Kowalczyk, K Koyama, K Kraljic, O Krause, S Kruk, B Kubik, U Kuchner, K Kuijken, M Kummel, M Kunz, H Kurki-Suonio, F Lacasa, CG Lacey, F La Franca, N Lagarde, O Lahav, C Laigle, A La Marca, O La Marle, B Lamine, MC Lam, A Lan, c, on, H Landt, M Langer, A Lapi, C Larcheveque, S Larsen, M Lattanzi, F Laudisio, D Laugier, R Laureijs, V Laurent, G Lavaux, A Lawrenson, A Lazanu, T Lazeyras, Q Le Boulc'h, AMC Le Brun, V Le Brun, F Leclercq, S Lee, J Le Graet, L Legrand, KN Leirvik, M Le Jeune, M Lembo, D Le Mignant, MD Lepinzan, F Lepori, A Le Reun, G Leroy, GF Lesci, J Lesgourgues, L Leuzzi, ME Levi, TI Liaudat, G Libet, P Liebing, S Ligori, PB Lilje, C-C Lin, D Linde, E Linder, V Lindholm, L Linke, S-S Li, SJ Liu, I Lloro, FSN Lobo, N Lodieu, M Lombardi, L Lombriser, P Lonare, G Longo, M L'opez-Caniego, X Lopez Lopez, J Lorenzo Alvarez, A Loureiro, J Loveday, E Lusso, J Macias-Perez, T Maciaszek, G Maggio, M Magliocchetti, F Magnard, EA Magnier, A Magro, G Mahler, G Mainetti, D Maino, E Maiorano, E Maiorano, N Malavasi, GA Mamon, C Mancini, R Mandelbaum, M Manera, A Manjón-García, F Mannucci, O Mansutti, M Manteiga Outeiro, R Maoli, C Maraston, S Marcin, P Marcos-Arenal, B Margalef-Bentabol, O Marggraf, D Marinucci, M Marinucci, K Markovic, FR Marleau, J Marpaud, J Martignac, i, n-Fleitas, P Martin-Moruno, EL Martin, M Martinelli, N Martinet, H Martin, CJAP Martins, F Marulli, D Massari, R Massey, DC Masters, S Matarrese, Y Matsuoka, S Matthew, BJ Maughan, N Mauri, L Maurin, S Maurogordato, K McCarthy, AW McConnachie, HJ McCracken, I McDonald, JD McEwen, CJR McPartland, E Medinaceli, V Mehta, S Mei, M Melchior, J-B Melin, B M'enard, J Mendes, J Mendez-Abreu, M Meneghetti, A Mercurio, E Merlin, RB Metcalf, G Meylan, M Migliaccio, M Mignoli, L Miller, M Miluzio, B Milvang-Jensen, JP Mimoso, R Miquel, H Miyatake, B Mobasher, J Mohr, P Monaco, o, A Montoro, A Mora, A Moradinezhad Dizgah, M Moresco, C Moretti, G Morgante, N Morisset, TJ Moriya, PW Morris, DJ Mortlock, L Moscardini, DF Mota, S Mottet, LA Moustakas, T Moutard, u, ller, E Munari, G Murphree, C Murray, N Murray, P Musi, S Nadathur, BC Nagam, T Nagao, K Naidoo, R Nakajima, C Nally, P Natoli, A Navarro-Alsina, D Navarro Girones, C Neissner, A Nersesian, S Nesseris, HN Nguyen-Kim, L Nicastro, RC Nichol, M Nielbock, S-M Niemi, S Nieto, K Nilsson, J Noller, P Norberg, A Nouri-Zonoz, P Ntelis, A Nucita, P Nugent, NJ Nunes, T Nutma, I Ocampo, J Odier, PA Oesch, M Oguri, D Magalhaes Oliveira, M Onoue, T Oosterbroek, F Oppizzi, C Ordenovic, K Osato, F Pacaud, F Pace, C Padilla, K Paech, L Pagano, MJ Page, E Palazzi, S Paltani, S Pamuk, S Pandolfi, D Paoletti, M Paolillo, P Papaderos, K Pardede, G Parimbelli, A Parmar, C Partmann, F Pasian, F Passalacqua, K Paterson, L Patrizii, C Pattison, A Paulino-Afonso, R Paviot, JA Peacock, FR Pearce, K Pedersen, A Peel, RF Peletier, M Pellejero Ibanez, R Pello, MT Penny, WJ Percival, A Perez-Garrido, L Perotto, V Pettorino, A Pezzotta, S Pezzuto, A Philippon, M Pierre, O Piersanti, M Pietroni, L Piga, L Pilo, S Pires, A Pisani, A Pizzella, L Pizzuti, C Plana, G Polenta, JE Pollack, M Poncet, M P\"ontinen, P Pool, LA Popa, V Popa, J Popp, C Porciani, L Porth, D Potter, M Poulain, A Pourtsidou, L Pozzetti, I Prandoni, GW Pratt, S Prezelus, E Prieto, A Pugno, S Quai, L Quilley, GD Racca, A Raccanelli, G R'acz, S Radinovi'c, M Radovich, A Ragagnin, U Ragnit, F Raison, N Ramos-Chernenko, C Ranc, Y Rasera, N Raylet, R Rebolo, A Refregier, P Reimberg, TH Reiprich, F Renk, A Renzi, J Retre, Y Revaz, C Reyl'e, L Reynolds, J Rhodes, F Ricci, M Ricci, G Riccio, SO Ricken, S Rissanen, I Risso, H-W Rix, AC Robin, B Rocca-Volmerange, P-F Rocci, M Rodenhuis, G Rodighiero, M Rodriguez Monroy, RP Rollins, M Romanello, J Roman, E Romelli, M Romero-Gomez, M Roncarelli, P Rosati, C Rosset, E Rossetti, W Roster, HJA Rottgering, A Rozas-Fernández, K Ruane, JA Rubino-Martin, A Rudolph, F Ruppin, B Rusholme, S Sacquegna, I S'aez-Casares, S Saga, R Saglia, M Sahl'en, T Saifollahi, Z Sakr, J Salvalaggio, R Salvaterra, L Salvati, M Salvato, J-C Salvignol, AG Sanchez, E Sanchez, DB Sanders, D Sapone, M Saponara, E Sarpa, F Sarron, S Sartori, B Sartoris, B Sassolas, L Sauniere, M Sauvage, M Sawicki, R Scaramella, C Scarlata, L Scharr'e, J Schaye, JA Schewtschenko, J-T Schindler, E Schinnerer, M Schirmer, F Schmidt, F Schmidt, M Schmidt, A Schneider, M Schneider, P Schneider, N Schöneberg, T Schrabback, M Schultheis, S Schulz, N Schuster, J Schwartz, D Sciotti, M Scodeggio, D Scognamiglio, D Scott, V Scottez, A Secroun, E Sefusatti, G Seidel, M Seiffert, E Sellentin, M Selwood, E Semboloni, M Sereno, S Serjeant, S Serrano, G Setnikar, F Shankar, RM Sharples, A Short, A Shulevski, M Shuntov, M Sias, G Sikkema, A Silvestri, P Simon, C Sirignano, G Sirri, J Skottfelt, E Slezak, D Sluse, GP Smith, LC Smith, RE Smith, SJA Smit, F Soldano, BG Solheim, JG Sorce, F Sorrenti, E Soubrie, L Spinoglio, A Spurio Mancini, J Stadel, L Stagnaro, L Stanco, SA Stanford, J-L Starck, P Stassi, J Steinwagner, D Stern, C Stone, P Strada, F Strafella, D Stramaccioni, C Surace, F Sureau, SH Suyu, I Swindells, M Szafraniec, I Szapudi, S Taamoli, M Talia, i, K Tanidis, C Tao, P Tarr'io, D Tavagnacco, AN Taylor, JE Taylor, PL Taylor, EM Teixeira, M Tenti, P Teodoro Idiago, HI Teplitz, I Tereno, N Tessore, V Testa, G Testera, M Tewes, R Teyssier, N Theret, C Thizy, PD Thomas, Y Toba, S Toft, R Toledo-Moreo, E Tolstoy, E Tommasi, O Torbaniuk, F Torradeflot, C Tortora, S Tosi, S Tosti, M Trifoglio, A Troja, T Trombetti, A Tronconi, M Tsedrik, A Tsyganov, M Tucci, I Tutusaus, C Uhlemann, L Ulivi, M Urbano, L Vacher, L Vaillon, P Valageas, I Valdes, EA Valentijn, L Valenziano, C Valieri, J Valiviita, M Van den Broeck, T Vassallo, R Vavrek, J Vega-Ferrero, B Venemans, A Venhola, S Ventura, G Verdoes Kleijn, D Vergani, A Verma, F Vernizzi, A Veropalumbo, G Verza, C Vescovi, D Vibert, M Viel, P Vielzeuf, C Viglione, A Viitanen, F Villaescusa-Navarro, S Vinciguerra, F Visticot, K Voggel, M von Wietersheim-Kramsta, WJ Vriend, S Wachter, M Walmsley, G Walth, DM Walton, NA Walton, M Wander, L Wang, Y Wang, JR Weaver, J Weller, M Wetzstein, DJ Whalen, IH Whittam, A Widmer, M Wiesmann, J Wilde, OR Williams, H-A Winther, A Wittje, JHW Wong, AH Wright, V Yankelevich, HW Yeung, M Yoon, S Youles, LYA Yung, A Zacchei, L Zalesky, G Zamorani, A Zamorano Vitorelli, M Zanoni Marc, M Zennaro, FM Zerbi, IA Zinchenko, J Zoubian, E Zucca, M Zumalacarregui
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MOSAIC at the ELT: a unique instrument for the largest ground-based telescope

Proceedings Volume 13096, Ground-based and Airborne Instrumentation for Astronomy X Society of Photo-optical Instrumentation Engineers (2024)

Authors:

Roser Pelló, Mathieu Puech, Éric Prieto, Gavin B Dalton, Ian Lewis, Louis Gabarra, Adam Lowe, Ellen Schallig, Jurgen Schmoll, David Terrett, Alec York

Abstract:

MOSAIC is the Multi-Object Spectrograph (MOS) for the 39m Extremely Large Telescope (ELT) of the European Southern Observatory (ESO), with unique capabilities in terms of multiplex, wavelength coverage and spectral resolution. It is a versatile multi-object spectrograph working in both the Visible and NIR domains, designed to cover the largest possible area (∼40 arcmin2) on the focal plane, and optimized to achieve the best possible signal-to-noise ratio on the faintest sources, from stars in our Galaxy to galaxies at the epoch of the reionization. In this paper we describe the main characteristics of the instrument, including its expected performance in the different observing modes. The status of the project will be briefly presented, together with the positioning of the instrument in the landscape of the ELT instrumentation. We also review the main expected scientific contributions of MOSAIC, focusing on the synergies between this instrument and other major ground-based and space facilities.
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Euclidpreparation

Astronomy & Astrophysics EDP Sciences 685 (2024) A108-A108

Authors:

E Lusso, S Fotopoulou, M Selwood, V Allevato, G Calderone, C Mancini, M Mignoli, M Scodeggio, L Bisigello, A Feltre, F Ricci, F La Franca, D Vergani, L Gabarra, V Le Brun, E Maiorano, E Palazzi, M Moresco, G Zamorani, G Cresci, K Jahnke, A Humphrey, H Landt, F Mannucci, A Marconi

Abstract:

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
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Euclid preparation. XXX. Performance assessment of the NISP Red-Grism through spectroscopic simulations for the Wide and Deep surveys

(2023)

Authors:

Euclid Collaboration, L Gabarra, C Mancini, L Rodriguez Munoz, G Rodighiero, C Sirignano, M Scodeggio, M Talia, S Dusini, W Gillard, BR Granett, E Maiorano, M Moresco, L Paganin, E Palazzi, L Pozzetti, A Renzi, E Rossetti, D Vergani, V Allevato, L Bisigello, G Castignani, B De Caro, M Fumana, K Ganga, B Garilli, M Hirschmann, F La Franca, C Laigle, F Passalacqua, M Schirmer, L Stanco, A Troja, LYA Yung, G Zamorani, J Zoubian, N Aghanim, A Amara, N Auricchio, M Baldi, R Bender, C Bodendorf, D Bonino, E Branchini, M Brescia, J Brinchmann, S Camera, V Capobianco, C Carbone, J Carretero, FJ Castander, M Castellano, S Cavuoti, R Cledassou, G Congedo, CJ Conselice, L Conversi, Y Copin, L Corcione, A Costille, F Courbin, A Da Silva, H Degaudenzi, J Dinis, F Dubath, X Dupac, A Ealet, S Farrens, S Ferriol, M Frailis, E Franceschi, P Franzetti, S Galeotta, B Gillis, C Giocoli, A Grazian, F Grupp, L Guzzo, W Holmes, A Hornstrup, P Hudelot, K Jahnke, M Kümmel, S Kermiche, A Kiessling, M Kilbinger, T Kitching, R Kohley, B Kubik, M Kunz, H Kurki-Suonio, S Ligori, PB Lilje, I Lloro, O Mansutti, O Marggraf, K Markovic, F Marulli, R Massey, S Maurogordato, S Mei, M Meneghetti, G Meylan, L Moscardini, E Munari, RC Nichol, S-M Niemi, J Nightingale, C Padilla, S Paltani, F Pasian, K Pedersen, WJ Percival, V Pettorino, G Polenta, M Poncet, F Raison, J Rhodes, G Riccio, E Romelli, M Roncarelli, R Saglia, D Sapone, P Schneider, A Secroun, G Seidel, S Serrano, G Sirri, C Surace, P Tallada-Crespí, D Tavagnacco, AN Taylor, I Tereno, R Toledo-Moreo, F Torradeflot, M Trifoglio, I Tutusaus, EA Valentijn, L Valenziano, T Vassallo, Y Wang, J Weller, A Zacchei, S Andreon, H Aussel, S Bardelli, M Bolzonella, A Boucaud, E Bozzo, C Colodro-Conde, D Di Ferdinando, M Farina, J Graciá-Carpio, E Keihänen, V Lindholm, D Maino, N Mauri, Y Mellier, C Neissner, V Scottez, M Tenti, E Zucca, Y Akrami, C Baccigalupi, M Ballardini, F Bernardeau, A Biviano, AS Borlaff, E Borsato, C Burigana, R Cabanac, A Cappi, CS Carvalho, S Casas, T Castro, K Chambers, AR Cooray, J Coupon, HM Courtois, S Davini, S de la Torre, G De Lucia, G Desprez, H Dole, JA Escartin, S Escoffier, I Ferrero, F Finelli, S Fotopoulou, J Garcia-Bellido, K George, F Giacomini, G Gozaliasl, H Hildebrandt, I Hook, O Ilbert, A Jimenez Muñoz, JJE Kajava, V Kansal, CC Kirkpatrick, L Legrand, A Loureiro, J Macias-Perez, M Magliocchetti, G Mainetti, R Maoli, S Marcin, M Martinelli, N Martinet, CJAP Martins, S Matthew, L Maurin, RB Metcalf, G Morgante, S Nadathur, AA Nucita, L Patrizii, V Popa, C Porciani, D Potter, M Pöntinen, AG Sánchez, Z Sakr, A Schneider, E Sefusatti, M Sereno, A Shulevski, A Spurio Mancini, J Stadel, J Steinwagner, R Teyssier, J Valiviita, A Veropalumbo, M Viel, IA Zinchenko
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Details from ArXiV

Characterizing the galaxy shape effect on the Euclid slitless spectroscopy using simulations

ArXiv 2301.12803 (2023)
Details from ArXiV

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