Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Capalbo V."'
Publikováno v:
EPJ Web of Conferences, Vol 293, p 00009 (2024)
The study of the morphology of 2D projected maps of galaxy clusters is a suitable approach to infer, from real data, the dynamical state of those systems. We recently developed a new method to recover the morphological features in galaxy cluster maps
Externí odkaz:
https://doaj.org/article/97f2972c19344dcfbb5a1f70d9c8ef54
Autor:
Battistelli E.S., Barbavara E., de Bernardis P., Cacciotti F., Capalbo V., Carbone A., Carretti E., Ciccalotti D., Columbro F., Coppolecchia A., Cruciani A., D’Alessandro G., De Petris M., Govoni F., Isopi G., Lamagna L., Levati E., Marongiu P., Mascia A., Masi S., Molinari E., Murgia M., Navarrini A., Novelli A., Occhiuzzi A., Orlati A., Pappalardo E., Paiella A., Pettinari G., Piacentini F., Pisanu T., Poppi S., Porceddu I., Ritacco A., Schirru M.R., Vargiu G.P.
Publikováno v:
EPJ Web of Conferences, Vol 293, p 00005 (2024)
Galaxy clusters and surrounding medium, can be studied using X-ray bremsstrahlung emission and Sunyaev Zel’dovich (SZ) effect. Both astrophysical probes, sample the same environment with different parameters dependance. The SZ effect is relatively
Externí odkaz:
https://doaj.org/article/7fe8507019694635a78819a83f9b27cc
Autor:
Isopi, G., Capalbo, V., Hincks, A. D., Di Mascolo, L., Barbavara, E., Battistelli, E. S., Bond, J. R., Cui, W., Coulton, W. R., De Petris, M., Devlin, M., Dolag, K., Dunkley, J., Fabjan, D., Ferragamo, A., Gill, A. S., Guan, Y., Halpern, M., Hilton, M., Hughes, J. P., Lokken, M., van Marrewijk, J., Moodley, K., Mroczkowski, T., Orlowski-Scherer, J., Rasia, E., Santoni, S., Sifón, C., Wollack, E. J., Yepes, G.
According to CMB measurements, baryonic matter constitutes about $5\%$ of the mass-energy density of the universe. A significant population of these baryons, for a long time referred to as `missing', resides in a low density, warm-hot intergalactic m
Externí odkaz:
http://arxiv.org/abs/2410.14404
Autor:
D’Alessandro G., Barbavara E., Battistelli E.S., de Bernardis P., Cacciotti F., Capalbo V., Carretti E., Columbro F., Coppolecchia A., Cruciani A., De Petris A., Govoni F., Isopi G., Lamagna L., Marongiu P., Masi S., Mele L., Molinari M., Murgia M., Navarrini A., Orlati A., Paiella A., Pettinari G., Piacentini F., Pisanu T., Poppi S., Presta G., Radiconi F.
Publikováno v:
EPJ Web of Conferences, Vol 257, p 00047 (2022)
Externí odkaz:
https://doaj.org/article/381f1662585448379882b7e8baa4c399
Autor:
D’Alessandro G., Barbarava E., Battistelli E.S., de Bernardis P., Cacciotti F., Capalbo V., Carretti E., Columbro F., Coppolecchia A., Cruciani A., De Petris M., Govoni F., Isopi G., Lamagna L., Marongiu P., Masi S., Mele L., Molinari M., Murgia M., Navarrini A., Orlati A., Paiella A., Pettinari G., Piacentini F., Pisanu T., Poppi S., Presta G., Radiconi F.
Publikováno v:
EPJ Web of Conferences, Vol 257, p 00012 (2022)
MISTRAL is a millimetric camera working in the W-band (78–103 GHz) which will take data from the Sardinia Radio Telescope, the Italian 64-m radio telescope located 50 km form Cagliari, at 600m above the sea level, in Sardinia. It is being built as
Externí odkaz:
https://doaj.org/article/63bcd9b72981427ba2a850702ae437e2
Autor:
Battistelli, E. S., Barbavara, E., de Bernardis, P., Cacciotti, F., Capalbo, V., Carbone, A., Carretti, E., Ciccalotti, D., Columbro, F., Coppolecchia, A., Cruciani, A., D'Alessandro, G., De Petris, M., Govoni, F., Isopi, G., Lamagna, L., Levati, E., Marongiu, P., Mascia, A., Masi, S., Molinari, E., Murgia, M., Navarrini, A., Novelli, A., Occhiuzzi, A., Orlati, A., Pappalardo, E., Paiella, A., Pettinari, G., Piacentini, F., Pisanu, T., Poppi, S., Porceddu, I., Ritacco, A., Schirru, M. R., Vargiu, G. P.
Galaxy clusters and surrounding medium, can be studied using X-ray bremsstrahlung emission and Sunyaev Zel'dovich (SZ) effect. Both astrophysical probes, sample the same environment with different parameters dependance. The SZ effect is relatively mo
Externí odkaz:
http://arxiv.org/abs/2310.18029
Autor:
Battistelli, E. S., Barbavara, E., de Bernardis, P., Cacciotti, F., Capalbo, V., Carretti, E., Columbro, F., Coppolecchia, A., Cruciani, A., D'Alessandro, G., De Petris, M., Govoni, F., Isopi, G., Lamagna, L., Marongiu, P., Masi, S., Mele, L., Molinari, E., Murgia, M., Navarrini, A., Orlati, A., Paiella, A., Pettinari, G., Piacentini, F., Pisanu, T., Poppi, S., Presta, G., Radiconi, F.
The MIllimeter Sardinia radio Telescope Receiver based on Array of Lumped elements kids, MISTRAL, is a millimetric ($\simeq 90GHz$) multipixel camera being built for the Sardinia Radio Telescope. It is going to be a facility instrument and will sampl
Externí odkaz:
http://arxiv.org/abs/2204.04222
Akademický článek
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Autor:
Zmuidzinas, Jonas, Gao, Jian-Rong, Barbavara, E., Battistelli, E. S., de Bernardis, P., Cacciotti, F., Capalbo, V., Carbone, A., Carretti, E., Ciccalotti, D., Columbro, F., Coppolecchia, A., Cruciani, A., D'Alessandro, G., De Petris, M., Govoni, F., Isopi, G., Lamagna, L., Marongiu, P., Mascia, A., Masi, S., Molinari, E., Murgia, M., Navarrini, A., Novelli, A., Occhiuzzi, A., Orlati, A., Paiella, A., Pettinari, G., Piacentini, F., Pisanu, T., Poppi, S., Porceddu, I., Ritacco, A., Schirru, R., Vargiu, G.
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13102 Issue: 1 p131022T-131022T-12, 12971191p
Autor:
D'Alessandro, G., Barbarava, E., Battistelli, E. S., de Bernardis, P., Cacciotti, F., Capalbo, V., CARRETTI, ETTORE, Columbro, F., Coppolecchia, A., Cruciani, A., De Petris, M., GOVONI, FEDERICA, Isopi, G., Lamagna, L., MARONGIU, Pasqualino, Masi, S., Mele, L., Molinari, M., MURGIA, MATTEO, NAVARRINI, Alessandro, ORLATI, ANDREA, Paiella, A., Pettinari, G., Piacentini, F., PISANU, Tonino, POPPI, Sergio, Presta, G., Radiconi, F.
Publikováno v:
EPJ Web of Conferences, Vol 257, p 00012 (2022)
MISTRAL is a millimetric camera working in the W-band (78–103 GHz) which will take data from the Sardinia Radio Telescope, the Italian 64-m radio telescope located 50 km form Cagliari, at 600m above the sea level, in Sardinia. It is being built as