Zobrazeno 1 - 10
of 380
pro vyhledávání: '"Andrade-Santos, F"'
Autor:
Aymerich, G., Douspis, M., Pratt, G. W., Salvati, L., Soubrié, E., Andrade-Santos, F., Forman, W., Jones, C., Aghanim, N., Kraft, R., van Weeren, R. J.
We provide a new scaling relation between $Y_{\text{SZ}}$, the integrated Sunyaev-Zeldovich signal and $M_{500}^{Y_{\text{X}}}$, the cluster mass derived from X-ray observations, using a sample of clusters from the Planck Early Sunyaev-Zeldovich (ESZ
Externí odkaz:
http://arxiv.org/abs/2402.04006
Autor:
Olivares, V., Su, Y., Forman, W., Gaspari, M., Andrade-Santos, F., Salome, P., Nulsen, P., Edge, A., Combes, F., Jones, C.
We study active galactic nucleus (AGN) feedback in nearby (z<0.35) galaxy clusters from the Planck Sunyaev-Zeldovich (SZ) sample using Chandra observations. This nearly unbiased mass-selected sample includes both relaxed and disturbed clusters and ma
Externí odkaz:
http://arxiv.org/abs/2306.09829
Autor:
Vanzella, E., Claeyssens, A., Welch, B., Adamo, A., Coe, D., Diego, J. M., Mahler, G., Khullar, G., Kokorev, V., Oguri, M., Ravindranath, S., Furtak, L. J., Hsiao, T. Yu-Yang, Abdurro'uf, Mandelker, N., Brammer, G., Bradley, L. D., Bradac, M., Conselice, C. J., Dayal, P., Nonino, M., Andrade-Santos, F., Windhorst, R. A., Pirzkal, N., Sharon, K., de Mink, S. E., Fujimoto, S., Zitrin, A., Eldridge, J. J., Norman, C.
Star cluster formation in the early universe and their contribution to reionization remains to date largely unconstrained. Here we present JWST/NIRCam imaging of the most highly magnified galaxy known at z ~ 6, the Sunrise arc. We identify six young
Externí odkaz:
http://arxiv.org/abs/2211.09839
Autor:
Olivares, V., Su, Y., Nulsen, P., Kraft, R., Somboonpanyakul, T., Andrade-Santos, F., Jones, C., Forman, W.
We present a systematic study of X-ray cavities using archival Chandra observations of nearby galaxy clusters selected by their Sunyaev-Zel'dovich (SZ) signature in the Planck survey, which provides a nearly unbiased mass-selected sample to explore t
Externí odkaz:
http://arxiv.org/abs/2208.04888
Autor:
Osinga, E., van Weeren, R. J., Andrade-Santos, F., Rudnick, L., Bonafede, A., Clarke, T., Duncan, K., Giacintucci, S., Mroczkowski, Tony, Röttgering, H. J. A.
Publikováno v:
A&A 665, A71 (2022)
It has been well established that galaxy clusters have magnetic fields. The exact properties and origin of these magnetic fields are still uncertain even though these fields play a key role in many astrophysical processes. Various attempts have been
Externí odkaz:
http://arxiv.org/abs/2207.09717
Autor:
Rajpurohit, K., Vazza, F., van Weeren, R. J., Hoeft, M., Brienza, M., Bonnassieux, E., Riseley, C. J., Brunetti, G., Bonafede, A., Brüggen, M., Formann, W. R., Rajpurohit, A. S., Röttgering, H. J. A., Drabent, A., Domínguez-Fernández, P., Wittor, D., Andrade-Santos, F.
Publikováno v:
A&A 654, A41 (2021)
We present the first deep low frequency radio observations of the massive and highly disturbed galaxy cluster Abell 2744 using the upgraded Giant Metrewave Radio Telescope (uGMRT). The cluster is experiencing a very complex multiple merger and hosts
Externí odkaz:
http://arxiv.org/abs/2104.05690
Autor:
van Weeren, R. J., Shimwell, T. W., Botteon, A., Brunetti, G., Brüggen, M., Boxelaar, J. M., Cassano, R., Di Gennaro, G., Andrade-Santos, F., Bonnassieux, E., Bonafede, A., Cuciti, V., Dallacasa, D., de Gasperin, F., Gastaldello, F., Hardcastle, M. J., Hoeft, M., Kraft, R . P., Mandal, S., Rossetti, M., Röttgering, H. J. A., Tasse, C., Wilber, A. G.
Publikováno v:
A&A 651, A115 (2021)
Diffuse cluster radio sources, in the form of radio halos and relics, reveal the presence of cosmic rays and magnetic fields in the intracluster medium (ICM). These cosmic rays are thought to be (re-)accelerated through ICM turbulence and shock waves
Externí odkaz:
http://arxiv.org/abs/2011.02387
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:
Hoeft, M., Dumba, C., Drabent, A., Rajpurohit, K., Rossetti, M., Nuza, S. E., van Weeren, R. J., Meusinger, H., Botteon, A., Brunetti, G., Shimwell, T. W., Cassano, R., Brüggen, M., Röttgering, H. J. A., Gastaldello, F., Lovisari, L., Yepes, G., Andrade-Santos, F., Eckert, D.
Publikováno v:
A&A 654, A68 (2021)
Diffuse radio emission has been found in many galaxy clusters, predominantly in massive systems which are in the state of merging. The radio emission can usually be classified as relic or halo emission, which are believed to be related to merger shoc
Externí odkaz:
http://arxiv.org/abs/2010.10331
Autor:
Lovisari, L., Ettori, S., Sereno, M., Schellenberger, G., Forman, W. R., Andrade-Santos, F., Jones, C.
Publikováno v:
A&A 644, A78 (2020)
Total mass is arguably the most fundamental property for cosmological studies with galaxy clusters. We investigate the present differences in the mass estimates obtained through independent X-ray, weak-lensing, and dynamical studies. We quantify the
Externí odkaz:
http://arxiv.org/abs/2010.03582