Zobrazeno 1 - 10
of 1 036
pro vyhledávání: '"Duffy R"'
Autor:
Iqbal, A., Pratt, G. W., Bobin, J., Arnaud, M., Rasia, E., Rossetti, M., Duffy, R. T., Bartalucci, I., Bourdin, H., De Luca, F., De Petris, M., Donahue, M., Eckert, D., Ettori, S., Ferragamo, A., Gaspari, M., Gastaldello, F., Gavazzi, R., Ghizzardi, S., Lovisari, L., Mazzotta, P., Maughan, B. J., Pointecouteau, E., Sereno, M.
Publikováno v:
A&A 679, A51 (2023)
Temperature profiles of the hot galaxy cluster intracluster medium (ICM) have a complex non-linear structure that traditional parametric modelling may fail to fully approximate. For this study, we made use of neural networks, for the first time, to c
Externí odkaz:
http://arxiv.org/abs/2309.02075
Autor:
Citrome L, Eramo A, Francois C, Duffy R, Legacy SN, Offord SJ, Krasa HB, Johnston SS, Guiraud-Diawara A, Kamat SA, Rohman P
Publikováno v:
Neuropsychiatric Disease and Treatment, Vol 2015, Iss Issue 1, Pp 3095-3104 (2015)
Leslie Citrome,1 Anna Eramo,2 Clement Francois,2 Ruth Duffy,3 Susan N Legacy,3 Steve J Offord,3 Holly B Krasa,3 Stephen S Johnston,4 Alice Guiraud-Diawara,5 Siddhesh A Kamat,3 Patricia Rohman3 1Department of Psychiatry and Behavioral Sciences, New Yo
Externí odkaz:
https://doaj.org/article/f52fce680c02433a94e07a79f62deb18
Autor:
Bartalucci, I., Molendi, S., Rasia, E., Pratt, G. W., Arnaud, M., Rossetti, M., Gastaldello, F., Eckert, D., Balboni, M., Borgani, S., Bourdin, H., Campitiello, M. G., De Grandi, S., De Petris, M., Duffy, R. T., Ettori, S., Ferragamo, A., Gaspari, M., Gavazzi, R., Ghizzardi, S., Iqbal, A., Kay, S. T., Lovisari, L., Mazzotta, P., Maughan, B. J., Pointecouteau, E., Riva, G., Sereno, M.
Publikováno v:
A&A 674, A179 (2023)
We investigate the statistical properties and the origin of the scatter within the spatially resolved surface brightness profiles of the CHEX-MATE sample, formed by 118 galaxy clusters selected via the SZ effect. These objects have been drawn from th
Externí odkaz:
http://arxiv.org/abs/2305.03082
Autor:
Duffy, R. T., Logan, C. H. A., Maughan, B. J., Eckert, D., Clerc, N., Ettori, S., Gastaldello, F., Koulouridis, E., Pierre, M., Ricci, M., Sereno, M., Valtchanov, I., Willis, J. P.
Publikováno v:
2022MNRAS.512.2525D
We use deep follow-up XMM-Newton observations of 6 clusters discovered in the XXL Survey at $z>1$ to gain robust measurements of their X-ray properties and to investigate the extent to which scaling relations at low redshift are valid at $z>1$. This
Externí odkaz:
http://arxiv.org/abs/2204.03945
Autor:
Collaboration, The CHEX-MATE, Arnaud, M., Ettori, S., Pratt, G. W., Rossetti, M., Eckert, D., Gastaldello, F., Gavazzi, R., Kay, S. T., Lovisari, L., Maughan, B. J., Pointecouteau, E., Sereno, M., Bartalucci, I., Bonafede, A., Bourdin, H., Cassano, R., Duffy, R. T., Iqbal, A., Maurogordato, S., Rasia, E., Sayers, J., Andrade-Santos, F., Aussel, H., Barnes, D. J., Barrena, R., Borgani, S., Burkutean, S., Clerc, N., Corasaniti, P. -S., Cuillandre, J. -C., De Grandi, S., De Petris, M., Dolag, K., Donahue, M., Ferragamo, A., Gaspari, M., Ghizzardi, S., Gitti, M., Haines, C. P., Jauzac, M., Johnston-Hollitt, M., Jones, C., Kéruzoré, F., Brun, A. M. C. Le, Mayet, F., Mazzotta, P., Melin, J. -B., Molendi, S., Nonino, M., Okabe, N., Paltani, S., Perotto, L., Pires, S., Radovich, M., Rubino-Martin, J. -A., Salvati, L., Saro, A., Sartoris, B., Schellenberger, G., Streblyanska, A., Tarrio, P., Tozzi, P., Umetsu, K., van der Burg, R. F. J., Vazza, F., Venturi, T., Yepes, G., Zarattini, S.
Publikováno v:
A&A 650, A104 (2021)
The Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE) is a three mega-second Multi-Year Heritage Programme to obtain X-ray observations of a minimally-biased, signal-to-nois
Externí odkaz:
http://arxiv.org/abs/2010.11972
Autor:
de Vries, M. N., Wise, M. W., Huppenkothen, D., Nulsen, P. E. J., Snios, B., Hardcastle, M. J., Birkinshaw, M., Worrall, D. M., Duffy, R. T., McNamara, B. R.
We present a spectral analysis of the lobes and X-ray jets of Cygnus A, using more than 2 Ms of $\textit{Chandra}$ observations. The X-ray jets are misaligned with the radio jets and significantly wider. We detect non-thermal emission components in b
Externí odkaz:
http://arxiv.org/abs/1805.03114
Autor:
Duffy, R. T., Worrall, D. M., Birkinshaw, M., Nulsen, P. E. J., Wise, M. W., de Vries, M. N., Snios, B., Mathews, W. G., Perley, R. A., Hardcastle, M. J., Rafferty, D. A., McNamara, B. R., Edge, A. C., McKean, J. P., Carilli, C. L., Croston, J. H., Godfrey, L. E. H., Laing, R. A.
We use new and archival Chandra observations of Cygnus A, totalling $\sim$1.9 Ms, to investigate the distribution and temperature structure of gas lying within the projected extent of the cocoon shock and exhibiting a rib-like structure. We confirm t
Externí odkaz:
http://arxiv.org/abs/1802.09476
Autor:
Coleman, E., Mirabelli, G., Bolshakov, P., Zhao, P., Caruso, E., Gity, F., Monaghan, S., Cherkaoui, K., Balestra, V., Wallace, R.M., Young, C.D., Duffy, R., Hurley, P.K.
Publikováno v:
In Solid State Electronics December 2021 186
We report measurements from an XMM-Newton observation of the low-excitation radio galaxy 3C 386. The study focusses on an X-ray-emitting gas belt, which lies between and orthogonal to the radio lobes of 3C 386 and has a mean temperature of $0.94\pm0.
Externí odkaz:
http://arxiv.org/abs/1604.05946