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Euclid: the Rb-M* Relation As a Function of Redshift I. the 5 X 109 M⊙ Black Hole in NGC 1272

R. Saglia, K. Mehrgan,S. de Nicola, J. Thomas,M. Kluge,R. Bender, D. Delley,P. Erwin,M. Fabricius,B. Neureiter,S. Andreon,C. Baccigalupi,M. Baldi,S. Bardelli,D. Bonino,E. Branchini,M. Brescia,J. Brinchmann,A. Caillat,S. Camera,V. Capobianco,C. Carbone, J. Carretero,S. Casas,M. Castellano,G. Castignani,S. Cavuoti,A. Cimatti,C. Colodro-Conde,G. Congedo,C. J. Conselice,L. Conversi,Y. Copin,F. Courbin,H. M. Courtois,H. Degaudenzi,G. De Lucia,J. Dinis,X. Dupac,S. Dusini,M. Farina,S. Farrens,F. Faustini,S. Ferriol,N. Fourmanoit,M. Frailis,E. Franceschi,M. Fumana,S. Galeotta,K. George,B. Gillis,C. Giocoli,A. Grazian,F. Grupp,L. Guzzo,S. V. H. Haugan,J. Hoar,W. Holmes,F. Hormuth,A. Hornstrup,K. Jahnke,M. Jhabvala,E. Keihaenen,S. Kermiche,A. Kiessling,M. Kilbinger,B. Kubik,M. Kuemmel,M. Kunz,H. Kurki-Suonio,D. Le Mignant,S. Ligori,P. B. Lilje,V. Lindholm,I. Lloro,G. Mainetti,E. Maiorano,O. Mansutti,O. Marggraf,K. Markovic, M. Martinelli,N. Martinet,F. Marulli,R. Massey,E. Medinaceli,M. Melchior,Y. Mellier,M. Meneghetti,E. Merlin,G. Meylan,M. Moresco,L. Moscardini,E. Munari,R. Nakajima,C. Neissner,R. C. Nichol,S. -M. Niemi,J. W. Nightingale,C. Padilla,S. Paltani,F. Pasian,K. Pedersen,W. J. Percival,V. Pettorino,S. Pires,G. Polenta,M. Poncet,L. A. Popa,L. Pozzetti,F. Raison,R. Rebolo,A. Renzi,J. Rhodes,G. Riccio,E. Romelli,M. Roncarelli,E. Rossetti,Z. Sakr,A. G. Sanchez,D. Sapone,B. Sartoris,M. Schirmer,P. Schneider,T. Schrabback,A. Secroun,M. Seiffert,S. Serrano,C. Sirignano,G. Sirri,J. Skottfelt,L. Stanco,J. Steinwagner,P. Tallada-Crespi,D. Tavagnacco,A. N. Taylor,I. Tereno,R. Toledo-Moreo,F. Torradeflot,I. Tutusaus,L. Valenziano,T. Vassallo,G. Verdoes Kleijn,Y. Wang, J. Weller,G. Zamorani,E. Zucca,C. Burigana,V. Scottez, L. Ferrarese,E. Lusso, D. Scott

ASTRONOMY & ASTROPHYSICS（2024）

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关键词
galaxies: elliptical and lenticular, cD,galaxies: individual: NGC 1272,galaxies: kinematics and dynamics,galaxies: nuclei,galaxies: photometry
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