THE X-RAY PROPERTIES OF TYPICAL HIGH-REDSHIFT RADIO-LOUD QUASARS 由 Saez, C., Brandt, W. N., Shemmer, O., Chomiuk, L., Lopez, Laura A., Miller, B. P., Vignali, C., Marshall, Herman

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Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-z Universe 由 Gruppioni, C, Berta, S, Spinoglio, L, Pereira-Santaella, M, Pozzi, F, Andreani, P, Bonato, M, De Zotti, G, Malkan, M, Negrello, M, Vallini, L, Vignali, C

Type 2 AGN host galaxies in the Chandra-COSMOS legacy survey: No evidence of AGN-driven quenching 由 Suh, H, Civano, F, Hasinger, G, Lusso, E, Lanzuisi, G, Marchesi, S, Trakhtenbrot, B, Allevato, V, Cappelluti, N, Capak, P, Elvis, M, Griffiths, R, Laigle, C, Lira, P, Riguccini, L, Rosario, D, Salvato, M, Schawinski, K, Vignali, C

Obscured AGN at z~1 from the zCOSMOS-Bright Survey I. Selection and Optical Properties of a [Ne v]-selected sample 由 Mignoli, M, Vignali, C, Gilli, R, Comastri, A, Zamorani, G, Bolzonella, M, Bongiorno, A, Lamareille, F, Nair, P, Pozzetti, L, Lilly, S, Carollo, C, Contini, T, Kneib, J, Fevre, O, Mainieri, V, Renzini, A, Scodeggio, M, Bardelli, S, Caputi, K, Cucciati, O, Torre, S, Ravel, L, Franzetti, P, Garilli, B

GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connection 由 Rovilos, E, Comastri, A, Gilli, R, Georgantopoulos, I, Ranalli, P, Vignali, C, Lusso, E, Cappelluti, N, Zamorani, G, Elbaz, D, Dickinson, M, Hwang, H, Charmandaris, V, Ivison, R, Merloni, A, Daddi, E, Carrera, F, Brandt, W, Mullaney, JR, Scott, D, Alexander, D, Del Moro, A, Morrison, G, Murphy, E, Altieri, B

The XMM-SERVS survey: new XMM–Newton point-source catalogue for the XMM-LSS field 由 Chen, C-TJ, Brandt, WN, Luo, B, Ranalli, P, Yang, G, Alexander, DM, Bauer, FE, Kelson, DD, Lacy, M, Nyland, K, Tozzi, P, Vito, F, Cirasuolo, M, Gilli, R, Jarvis, MJ, Lehmer, BD, Paolillo, M, Schneider, DP, Shemmer, O, Smail, I, Sun, M, Tanaka, M, Vaccari, M, Vignali, C, Xue, YQ, Banerji, M, Chow, KE, Häußler, B, Norris, RP, Silverman, JD, Trump, JR

The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme 由 Pierre, M, Pacaud, F, Adami, C, Alis, S, Altieri, B, Baran, B, Benoist, C, Birkinshaw, M, Bongiorno, A, Bremer, M, Brusa, M, Butler, A, Ciliegi, P, Chiappetti, L, Clerc, N, Corasaniti, P, Coupon, J, Breuck, C, Democles, J, Desai, S, Delhaize, J, Devriendt, J, Dubois, Y, Eckert, D, Elyiv, A, Ettori, S, Evrard, A, Faccioli, L, Farahi, A, Ferrari, C, Finet, F, Fotopoulou, S, Fourmanoit, N, Gandhi, P, Gastaldello, F, Gastaud, R, Georgantopoulos, I, Giles, P, Guennou, L, Guglielmo, V, Horellou, C, Husband, K, Huynh, M, Iovino, A, Kilbinger, M, Koulouridis, E, Lavoie, S, Brun, A, Fevre, J, Lidman, C, Lieu, M, Lin, C, Mantz, A, Maughan, B, Maurogordato, S, McCarthy, I, McGee, S, Melin, J, Melnyk, O, Menanteau, F, Novak, M, Paltani, S, Plionis, M, Poggianti, B, Pomarede, D, Pompei, E, Ponman, T, Ramos-Ceja, M, Ranalli, P, Rapetti, D, Raychaudury, S, Reiprich, T, Rottgering, H, Rozo, E, Rykoff, E, Sadibekova, T, Santos, J, Sauvageot, J, Schimd, C, Sereno, M, Smith, G, Smolčić, V, Snowden, S, Spergel, D, Stanford, S, Surdej, J, Valageas, P, Valotti, A, Valtchanov, I, Vignali, C, Willis, J, Ziparo, F