Zobrazeno 1 - 10
of 441
pro vyhledávání: '"Galluzzi, V."'
Autor:
Perrotta, F., Giulietti, M., Massardi, M., Gandolfi, G., Ronconi, T., Zanchettin, M. V., D'Amato, Q., Behiri., M., Torsello, M., Gabrielli, F., Boco, L., Galluzzi, V., Lapi, A.
We report ALMA high-resolution observations of water emission lines $p-{\rm{H_2O}} (2_{02}-1_{11}$), $o-{\rm{H_2O}} (3_{21}-3_{12})$, $p-{\rm{H_2O}} (4_{22}-4_{13})$, in the strongly lensed galaxy HATLASJ113526.2-01460 at redshift z $\sim$ 3.1. From
Externí odkaz:
http://arxiv.org/abs/2304.08563
Autor:
Massardi, M., Bonato, M., Lopez-Caniego, M., Galluzzi, V., De Zotti, G., Bonavera, L., Gonzalez-Nuevo, J., Lapi, A., Liuzzo, E.
The \textit{Herschel} Astrophysical Terahertz Large Area Survey (H-ATLAS), that has covered about 642 sq. deg. in 5 bands from 100 to 500 $\mu\rm m$, allows a blind flux-limited selection of blazars at sub-mm wavelengths. However, blazars constitute
Externí odkaz:
http://arxiv.org/abs/2205.07497
Publikováno v:
Planetary and Space Science, Volume 212, March 2022, 105397
The link between the surface temperature of Mercury and the exosphere sodium content has been investigated. Observations show that, along the orbit of Mercury, two maxima of total Na content are present: one at aphelion and one at perihelion. Previou
Externí odkaz:
http://arxiv.org/abs/2202.11467
Autor:
Massardi, M., Stoehr, F., Bendo, G. J., Bonato, M., Brand, J., Galluzzi, V., Guglielmetti, F., Liuzzo, E., Marchili, N., Richards, A. M. S., Rygl, K. L. J., Bedosti, F., Giannetti, A., Stagni, M., Knapic, C., Sponza, M., Fuller, G. A., Muxlow, T. W. B.
The Additional Representative Images for Legacy (ARI-L) project is a European Development project for ALMA Upgrade approved by the Joint ALMA Observatory (JAO) and the European Southern Observatory (ESO), started in June 2019. It aims to increase the
Externí odkaz:
http://arxiv.org/abs/2107.11071
Autor:
Pompeo, N., Alimenti, A, Torokhtii, K, Bartolomé, E, Palau, A, Puig, T, Augieri, A, Galluzzi, V, Mancini, A, Celentano, G, Obradors, X, Silva, E
Anisotropy is an intrinsic factor that dictates the magnetic properties of YBCO, thus with great impact for many applications. Artificial pinning centres are often introduced in an attempt to mitigate its effect, resulting in less anisotropic electri
Externí odkaz:
http://arxiv.org/abs/2001.10299
Autor:
Bonato, M., Liuzzo, E., Giannetti, A., Massardi, M., De Zotti, G., Burkutean, S., Galluzzi, V., Negrello, M., Baronchelli, I., Brand, J., Zwaan, M. A., Rygl, K. L. J., Marchili, N., Klitsch, A., Oteo, I.
We present a catalogue of ALMA flux density measurements of 754 calibrators observed between August 2012 and September 2017, for a total of 16,263 observations in different bands and epochs. The flux densities were measured reprocessing the ALMA imag
Externí odkaz:
http://arxiv.org/abs/1805.00024
Autor:
Puglisi, G., Galluzzi, V., Bonavera, L., Gonzalez-Nuevo, J., Lapi, A., Massardi, M., Perrotta, F., Baccigalupi, C., Celotti, A., Danese, L.
We combine the latest datasets obtained with different surveys to study the frequency dependence of polarized emission coming from Extragalactic Radio Sources (ERS). We consider data over a very wide frequency range starting from $1.4$ GHz up to $217
Externí odkaz:
http://arxiv.org/abs/1712.09639
Publikováno v:
A&A 618, A29 (2018)
Recent detailed simulations have shown that an insufficiently accurate characterization of the contamination of unresolved polarized extragalactic sources can seriously bias measurements of the primordial cosmic microwave background (CMB) power spect
Externí odkaz:
http://arxiv.org/abs/1712.08412
Autor:
Galluzzi, V., Massardi, M.
Publikováno v:
International Journal of Modern Physics D, Volume 25, Issue 11 (2016)
The polarization properties of extragalactic radio sources at frequencies higher than 20 GHz are still poorly constrained. However, their characterization would provide invaluable information about the physics of the emission processes and is crucial
Externí odkaz:
http://arxiv.org/abs/1611.08159
Autor:
Galluzzi, V., Massardi, M., Bonaldi, A., Casasola, V., Gregorini, L., Trombetti, T., Burigana, C., De Zotti, G., Ricci, R., Stevens, J., Ekers, R. D., Bonavera, L., Alighieri, S. di Serego, Liuzzo, E., Lopez-Caniego, M., Mignano, A., Paladino, R., Toffolatti, L., Tucci, M.
We present high sensitivity polarimetric observations in 6 bands covering the 5.5-38 GHz range of a complete sample of 53 compact extragalactic radio sources brighter than 200 mJy at 20 GHz. The observations, carried out with the Australia Telescope
Externí odkaz:
http://arxiv.org/abs/1611.07746