Zobrazeno 1 - 10
of 661
pro vyhledávání: '"Halliday, C."'
Autor:
Saglia, R. P., Sánchez-Blázquez, P., Bender, R., Simard, L., Desai, V., Aragón-Salamanca, A., Milvang-Jensen, B., Halliday, C., Jablonka, P., Noll, S., Poggianti, B., Clowe, D. I., De Lucia, G., Pelló, R., Rudnick, G., Valentinuzzi, T., White, S. D. M., Zaritsky, D.
We discovered a mistake in Eqs. (7) and (10) of Saglia et al. (2010, A&A, 524, A6), which propagates to Tables 8 and 9 and Fig. 25. We revise the tables, the figure and the affected statements in the paper. As a result, the reduction in the luminosit
Externí odkaz:
http://hdl.handle.net/10150/622690
http://arizona.openrepository.com/arizona/handle/10150/622690
http://arizona.openrepository.com/arizona/handle/10150/622690
Autor:
Guennou, L., Biviano, A., Adami, C., Limousin, M., Neto, G. B. Lima, Mamon, G. A., Ulmer, M. P., Gavazzi, R., Cypriano, E. S., Durret, F., Clowe, D., LeBrun, V., Allam, S., Basa, S., Benoist, C., Cappi, A., Halliday, C., Ilbert, O., Johnston, D., Jullo, E., Just, D., Kubo, J. M., Marquez, I., Marshall, P., Martinet, N., Maurogordato, S., Mazure, A., Murphy, K. J., Plana, H., Rostagni, F., Russeil, D., Schirmer, M., Schrabback, T., Slezak, E., Tucker, D., Zaritsky, D., Ziegler, B.
Constraints on the mass distribution in high-redshift clusters of galaxies are not currently very strong. We aim to constrain the mass profile, M(r), and dynamical status of the $z \sim 0.8$ LCDCS 0504 cluster of galaxies characterized by prominent g
Externí odkaz:
http://arxiv.org/abs/1403.3614
Autor:
Guennou, L., Adami, C., Durret, F., Neto, G. B. Lima, Ulmer, M. P., Clowe, D., LeBrun, V., Martinet, N., Allam, S., Annis, J., Basa, S., Benoist, C., Biviano, A., Cappi, A., Cypriano, E. S., Gavazzi, R., Halliday, C., Ilbert, O., Jullo, E., Just, D., Limousin, M., Márquez, I., Mazure, A., Murphy, K. J., Plana, H., Rostagni, F., Russeil, D., Schirmer, M., Slezak, E., Tucker, D., Zaritsky, D., Ziegler, B.
We analyse the structures of all the clusters in the DAFT/FADA survey for which XMM-Newton and/or a sufficient number of galaxy redshifts in the cluster range is available, with the aim of detecting substructures and evidence for merging events. Thes
Externí odkaz:
http://arxiv.org/abs/1311.6922
Autor:
Cimatti, A., Brusa, M., Talia, M., Mignoli, M., Rodighiero, G., Kurk, J., Cassata, P., Halliday, C., Renzini, A., Daddi, E.
The relationships between galaxies of intermediate stellar mass and moderate luminosity active galactic nuclei (AGNs) at 1
Externí odkaz:
http://arxiv.org/abs/1311.4401
We investigate the morphological properties of 494 galaxies selected from the GMASS survey at z>1, primarily in their optical rest frame, using HST images, from the CANDELS survey. We propose that the Hubble sequence of galaxy morphologies takes shap
Externí odkaz:
http://arxiv.org/abs/1307.1366
Autor:
Talia, M., Mignoli, M., Cimatti, A., Kurk, J., Berta, S., Bolzonella, M., Cassata, P., Daddi, E., Dickinson, M., Franceschini, A., Halliday, C., Pozzetti, L., Renzini, A., Rodighiero, G., Rosati, P., Zamorani, G.
We use rest-frame UV spectroscopy to investigate the properties related to large-scale gas outflows, and to the dust extinction and star-formation rates of a sample of z ~ 2 star-forming galaxies from the Galaxy Mass Assembly ultradeep Spectroscopic
Externí odkaz:
http://arxiv.org/abs/1111.4402
Autor:
Guennou, L., Adami, C., Da Rocha, C., Durret, F., Ulmer, M. P., Allam, S., Basa, S., Benoist, C., Biviano, A., Clowe, D., Gavazzi, R., Halliday, C., Ilbert, O., Johnston, D., Just, D., Kron, R., Kubo, J. M., LeBrun, V., Marshall, P., Mazure, A., Murphy, K. J., Pereira, D. N. E., Rabaca, C. R., Rostagni, F., Rudnick, G., Russeil, D., Schrabback, T., Slezak, E., Tucker, D., Zaritsky, D.
The study of intracluster light can help us to understand the mechanisms taking place in galaxy clusters, and to place constraints on the cluster formation history and physical properties. However, owing to the intrinsic faintness of ICL emission, mo
Externí odkaz:
http://arxiv.org/abs/1109.3967
Autor:
Silverman, J. D., Kampczyk, P., Jahnke, K., Andrae, R., Lilly, S., Elvis, M., Civano, F., Mainieri, V., Vignali, C., Zamorani, G., Nair, P., Fevre, O. Le, de Ravel, L., Bardelli, S., Bongiorno, A., Bolzonella, M., Brusa, M., Cappelluti, N., Cappi, A., Caputi, K., Carollo, C. M., Contini, T., Coppa, G., Cucciati, O., de la Torre, S., Franzetti, P., Garilli, B., Halliday, C., Hasinger, G., Iovino, A., Knobel, C., koekemoer, A., Kovac, K., Lamareille, F., Borgne, J. -F. Le, Brun, V. Le, Maier, C., Mignoli, M., Pello, R., Montero, E. Perez, Ricciardelli, E., Peng, Y., Scodeggio, M., Tanaka, M., Tasca, L., Tresse, L., Vergani, D., Zucca, E., Comastri, A., Finoguenov, A., Fu, H., Gilli, R., Hao, H., Ho, L., Salvato, M.
Close encounters between galaxies are expected to be a viable mechanism, as predicted by numerical simulations, by which accretion onto supermassive black holes can be initiated. To test this scenario, we construct a sample of 562 galaxies (M*>2.5x10
Externí odkaz:
http://arxiv.org/abs/1109.1292
Autor:
Salvato, M., Ilbert, O., Hasinger, G., Rau, A., Civano, F., Zamorani, G., Brusa, M., Elvis, M., Vignali, C., Aussel, H., Comastri, A., Fiore, F., Floc'h, E. Le, Mainieri, V., Bardelli, S., Bolzonella, M., Bongiorno, A., Capak, P., Caputi, K., Cappelluti, N., Carollo, C. M., Contini, T., Garilli, B., Iovino, A., Fotopoulou, S., Fruscione, A., Gilli, R., Halliday, C., Kneib, J-P., Kakazu, Y., Kartaltepe, J. S., Koekemoer, A. M., Kovac, K., Ideue, Y., Ikeda, H., Impey, C. D., Fevre, O. Le, Lamareille, F., Lanzuisi, G., Borgne, J-F. Le, Brun, V. Le, Lilly, S. J., Maier, C., Manohar, S., Masters, D., McCracken, H., Messias, H., Mignoli, M., Mobasher, B., Nagao, T., Pello, R., Puccetti, S., Renzini, E. Perez Montero A., Sargent, M., Sanders, D. B., Scodeggio, M., Scoville, N., Shopbell, P., Silvermann, J., Taniguchi, Y., Tasca, L., Tresse, L., Trump, J. R., Zucca, E.
With this paper, we release accurate photometric redshifts for 1692 counterparts to Chandra sources in the central square degree of the COSMOS field. The availability of a large training set of spectroscopic redshifts that extends to faint magnitudes
Externí odkaz:
http://arxiv.org/abs/1108.6061
Autor:
Mainieri, V., Bongiorno, A., Merloni, A., Aller, M., Carollo, M., Iwasawa, K., Koekemoer, A. M., Mignoli, M., Silverman, J. D., Bolzonella, M., Brusa, M., Comastri, A., Gilli, R., Halliday, C., Ilbert, O., Lusso, E., Salvato, M., Vignali, C., Zamorani, G., Contini, T., Kneib, J. -P., Fevre, O. Le, Lilly, S., Renzini, A., Scodeggio, M., Balestra, I., Bardelli, S., Caputi, K., Coppa, G., Cucciati, O., de la Torre, S., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Kovac, K., Lamareille, F., Borgne, J. -F. Le, Brun, V . Le, Maier, C., Nair, P., Pello, R., Peng, Y., Montero, E. Perez, Pozzetti, L., Ricciardelli, E., Tanaka, M., Tasca, L., Tresse, L., Vergani, D., Zucca, E., Aussel, H., Capak, P., Cappelluti, N., Elvis, M., Fiore, F., Hasinger, G., Impey, C., Floc'h, E. Le, Scoville, N., Taniguchi, Y., Trump, J.
We explore the connection between black hole growth at the center of obscured quasars selected from the XMM-COSMOS survey and the physical properties of their host galaxies. We study a bolometric regime ( 8 x 10^45 erg/s) where several theoret
Externí odkaz:
http://arxiv.org/abs/1105.5395