Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Koekemoer, A. M."'
Autor:
S. Bardelli, Paolo Cassata, G. C. Jones, Michele Ginolfi, Andreas L. Faisst, L. Morselli, Livia Vallini, Matthieu Béthermin, O. Le Fevre, D. Vergani, Y. Fudamoto, Miroslava Dessauges-Zavadsky, G. Rodighiero, E. Zucca, Edo Ibar, Margherita Talia, John D. Silverman, Dominik Riechers, Brian C. Lemaux, Peter Capak, Daniel Schaerer, Seiji Fujimoto, A. Enia, Médéric Boquien, Lin Yan, Andrea Cimatti, Chiara Mancini, L. Rodríguez-Muñoz, F. Loiacono, G. Zamorani, M. Romano, Nimish P. Hathi, Carlotta Gruppioni, Anton M. Koekemoer
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 496, pp.875-887. ⟨10.1093/mnras/staa1546⟩
Monthly Notices of the Royal Astronomical Society, 496(1), 875-887
Romano, M, Cassata, P, Morselli, L, Lemaux, B C, Bethermin, M, Capak, P, Faisst, A, Le Fevre, O, Schaerer, D, Silverman, J, Yan, L, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Enia, A, Fudamoto, Y, Fujimoto, S, Ginolfi, M, Gruppioni, C, Hathi, N P, Ibar, E, Jones, G C, Koekemoer, A M, Loiacono, F, Mancini, C, Riechers, D A, Rodighiero, G, Rodriguez-Munoz, L, Talia, M, Vallini, L, Vergani, D, Zamorani, G & Zucca, E 2020, ' The ALPINE ALMA [C II] Survey : on the nature of an extremely obscured serendipitous galaxy ', Monthly Notices of the Royal Astronomical Society, vol. 496, no. 1, pp. 875-887 . https://doi.org/10.1093/mnras/staa1546
Monthly Notices of the Royal Astronomical Society, 2020, 496, pp.875-887. ⟨10.1093/mnras/staa1546⟩
Monthly Notices of the Royal Astronomical Society, 496(1), 875-887
Romano, M, Cassata, P, Morselli, L, Lemaux, B C, Bethermin, M, Capak, P, Faisst, A, Le Fevre, O, Schaerer, D, Silverman, J, Yan, L, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Enia, A, Fudamoto, Y, Fujimoto, S, Ginolfi, M, Gruppioni, C, Hathi, N P, Ibar, E, Jones, G C, Koekemoer, A M, Loiacono, F, Mancini, C, Riechers, D A, Rodighiero, G, Rodriguez-Munoz, L, Talia, M, Vallini, L, Vergani, D, Zamorani, G & Zucca, E 2020, ' The ALPINE ALMA [C II] Survey : on the nature of an extremely obscured serendipitous galaxy ', Monthly Notices of the Royal Astronomical Society, vol. 496, no. 1, pp. 875-887 . https://doi.org/10.1093/mnras/staa1546
We report the serendipitous discovery of a bright galaxy (Gal-A) observed as part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). While this galaxy is detected both in line and continuum emission in ALMA Band 7, it is complete
Autor:
Yongquan Xue, W. N. Brandt, Maurizio Paolillo, Donald P. Schneider, Guang Yang, Anton M. Koekemoer, B. Luo, Andrea Comastri, Jun Xian Wang, M. Volonteri, Piero Ranalli, Roberto Gilli, Ohad Shemmer, Cristian Vignali, Teng Liu, Bret D. Lehmer, Fabio Vito
Publikováno v:
NASA Astrophysics Data System
We investigate the population of high-redshift ($3\leq z < 6$) AGN selected in the two deepest X-ray surveys, the 7 Ms \textit{Chandra} Deep Field-South and 2 Ms \textit{Chandra} Deep Field-North. Their outstanding sensitivity and spectral characteri
Autor:
C. Vignali, X. C. Zheng, Guang Yang, Tong Liu, I. E. Papadakis, Roberto Gilli, Andrea Comastri, Anton M. Koekemoer, Paolo Tozzi, Franz E. Bauer, Ohad Shemmer, Maurizio Paolillo, Jun Xian Wang, Fabio Vito, W. N. Brandt, Viola Allevato, Bin Luo, Yongquan Xue
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 471:4398-4411
We study the X-ray variability properties of distant AGNs in the Chandra Deep Field-South region over 17 years, up to $z\sim 4$, and compare them with those predicted by models based on local samples. We use the results of Monte Carlo simulations to
Autor:
C. Mancini, E. Daddi, A. Renzini, F. Salmi, H. J. McCracken, A. Cimatti, M. Onodera, M. Salvato, A. M. Koekemoer, H. Aussel, E. Le Floc'h, C. Willott, P. Capak
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 401:933-940
We investigate the properties of 12 ultra-massive passively evolving early type galaxies (ETGs) at z_phot>1.4 in the COSMOS 2 deg^2 field. These 12 ETGs were selected as pBzKs, have accurate 1.42.5x10^11 M_sun (Chabrier IMF). Contrary to previous cla