Zobrazeno 1 - 10
of 156
pro vyhledávání: '"Vernstrom, T."'
Autor:
Riseley, C. J., Bonafede, A., Bruno, L., Botteon, A., Rossetti, M., Biava, N., Bonnassieux, E., Loi, F., Vernstrom, T., Balboni, M.
Publikováno v:
A&A 686, A44 (2024)
Clusters of galaxies are turbulent environments, whether merging systems with a turbulent intracluster medium (ICM) or relaxed systems sloshing within the potential well. In many such clusters, diffuse radio sources associated with the ICM are found:
Externí odkaz:
http://arxiv.org/abs/2403.00414
Autor:
Duchesne, S. W., Botteon, A., Koribalski, B. S., Loi, F., Rajpurohit, K., Riseley, C. J., Rudnick, L., Vernstrom, T., Andernach, H., Hopkins, A. M., Kapinska, A. D., Norris, R. P., Zafar, T.
Clusters of galaxies have been found to host Mpc-scale diffuse, non-thermal radio emission in the form of central radio halos and peripheral relics. Turbulence and shock-related processes in the intra-cluster medium are generally considered responsib
Externí odkaz:
http://arxiv.org/abs/2402.06192
Autor:
Hoang, D. N., Brüggen, M., Shimwell, T. W., Botteon, A., O'Sullivan, S. P., Pasini, T., Zhang, X., Bonafede, A., Liu, A., Liu, T., Brunetti, G., Bulbul, E., Di Gennaro, G., Röttgering, H. J. A., Vernstrom, T., van Weeren, R. J.
Cosmological simulations predict the presence of warm hot thermal gas in the cosmic filaments that connect galaxy clusters. This gas is thought to constitute an important part of the missing baryons in the Universe. In addition to the thermal gas, co
Externí odkaz:
http://arxiv.org/abs/2306.03904
Autor:
Dunlop, J. S., McLure, R. J., Biggs, A. D., Geach, J. E., Michałowski, M. J., Ivison, R. J., Rujopakarn, W., van Kampen, E., Kirkpatrick, A., Pope, A., Scott, D., Swinbank, A. M., Targett, T. A., Aretxaga, I., Austermann, J. E., Best, P. N., Bruce, V. A., Chapin, E. L., Charlot, S., Cirasuolo, M., Coppin, K., Ellis, R. S., Finkelstein, S. L., Hayward, C. C., Hughes, D. H., Ibar, E., Jagannathan, P., Khochfar, S., Koprowski, M. P., Narayanan, D., Nyland, K., Papovich, C., Peacock, J. A., Rieke, G. H., Robertson, B., Vernstrom, T., Werf, P. P. van der, Wilson, G. W., Yun, M.
We present the results of the first, deep Atacama Large Millimeter Array ( ALMA) imaging covering the full similar or equal to 4.5 arcmin(2) of the Hubble Ultra Deep Field ( HUDF) imaged with Wide Field Camera 3/IR on HST. Using a 45-pointing mosaic,
Externí odkaz:
http://hdl.handle.net/10150/623849
http://arizona.openrepository.com/arizona/handle/10150/623849
http://arizona.openrepository.com/arizona/handle/10150/623849
Autor:
Tompkins, Scott A., Driver, Simon P., Robotham, Aaron S. G., Windhorst, Rogier A., Lagos, Claudia del P., Vernstrom, T., Hopkins, Andrew M.
We present a revised measurement of the extra-galactic background light (EBL) at radio frequencies based on a near complete compendium of radio source counts. We present the radio-EBL at 150 MHz, 325 MHz, 610 MHz, 1.4 GHz, 3 GHz, 5 GHz, and 8.4 GHz.
Externí odkaz:
http://arxiv.org/abs/2301.03699
Measuring the magnetic field in cosmic filaments reveals how the Universe is magnetised and the process that magnetised it. Using the Rotation Measures (RM) at 144-MHz from the LoTSS DR2 data, we analyse the rms of the RM extragalactic component as a
Externí odkaz:
http://arxiv.org/abs/2210.06220
Autor:
Riseley, C. J., Bonnassieux, E., Vernstrom, T., Galvin, T. J., Chokshi, A., Botteon, A., Rajpurohit, K., Duchesne, S. W., Bonafede, A., Rudnick, L., Hoeft, M., Quici, B., Eckert, D., Brienza, M., Tasse, C., Carretti, E., Collier, J. D., Diego, J. M., Di Mascolo, L., Hopkins, A. M., Johnston-Hollitt, M., Keel, R. R., Koribalski, B. S., Reiprich, T. H.
Abell 3266 is a massive and complex merging galaxy cluster that exhibits significant substructure. We present new, highly sensitive radio continuum observations of Abell 3266 performed with the Australian Square Kilometre Array Pathfinder (0.8$-$1.1
Externí odkaz:
http://arxiv.org/abs/2208.00395
Autor:
Carretti, E., Vacca, V., O'Sullivan, S. P., Heald, G. H., Horellou, C., Rottgering, H. J. A., Scaife, A. M. M., Shimwell, T. W., Shulevski, A., Stuardi, C., Vernstrom, T.
We used the Rotation Measure (RM) catalogue derived from the LOFAR Two-metre Sky Survey Data Release 2 (LoTSS DR2) at 144-MHz to measure the evolution with redshift of the extragalactic RM (RRM: Residual RM) and the polarization fraction ($p$) of sou
Externí odkaz:
http://arxiv.org/abs/2202.04607
Autor:
Filipović, Miroslav D., Payne, J. L., Alsaberi, R. Z. E., Norris, R. P., Macgregor, P. J., Rudnick, L., Koribalski, B. S., Leahy, D., Ducci, L., Kothes, R., Andernach, H., Barnes, L., Bojičić, I. S., Bozzetto, L. M., Brose, R., Collier, J. D., Crawford, E. J., Crocker, R. M., Dai, S., Galvin, T. J., Haberl, F., Heber, U., Hill, T., Hopkins, A. M., Hurley-Walker, N., Ingallinera, A., Jarrett, T., Kavanagh, P. J., Lenc, E., Luken, K. J., Mackey, D., Manojlović, P., Maggi, P., Maitra, C., Pennock, C. M., Points, S., Riggi, S., Rowell, G., Safi-Harb, S., Sano, H., Sasaki, M., Shabala, S., Stevens, J., van Loon, J. Th., Tothill, N. F. H., Umana, G., Urošević, D., Velović, V., Vernstrom, T., West, J. L., Wan, Z.
We report the discovery of J0624-6948, a low-surface brightness radio ring, lying between the Galactic Plane and the Large Magellanic Cloud (LMC). It was first detected at 888 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP), and wit
Externí odkaz:
http://arxiv.org/abs/2201.10026
Autor:
Venturi, T., Giacintucci, S., Merluzzi, P., Bardelli, S., Busarello, G., Dallacasa, D., Sikhosana, S. P., Marvil, J., Smirnov, O., Bourdin, H., Mazzotta, P., Rossetti, M., Rudnick, L., Bernardi, G., Bruggen, M., Carretti, E., Cassano, R., Di Gennaro, G., Gastaldello, F., Kale, R., Knowles, K., Koribalski, B. S., Heywood, I., Hopkins, A. M., Norris, R. P., Reiprich, T. H., Tasse, C., Vernstrom, T., Zucca, E., Bester, L. H., Diego, J. M., Kanapathippillai, J.
Publikováno v:
A&A 660, A81 (2022)
The Shapley Supercluster ($\langle z \rangle\approx0.048$) contains several tens of gravitationally bound clusters and groups, making it it is an ideal subject for radio studies of cluster mergers. We used new high sensitivity radio observations to i
Externí odkaz:
http://arxiv.org/abs/2201.04887