Zobrazeno 1 - 10
of 6 107
pro vyhledávání: '"Watson, R A"'
Autor:
González-González, R., Génova-Santos, R. T., Rubiño-Martín, J. A., Peel, M. W., Guidi, F., López-Caraballo, C. H., Fernández-Torreiro, M., Rebolo, R., Hernández-Monteagudo, C., Adak, D., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Fasano, A., Herranz, D., Hoyland, R. J., Martínez-González, E., Pascual-Cisneros, G., Piccirillo, L., Poidevin, F., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
This work focuses on the study of the AME, an important emission mechanism between 10 and 60 GHz whose polarization properties are not yet fully understood, and is therefore a potential contaminant for future CMB polarization observations. We use new
Externí odkaz:
http://arxiv.org/abs/2409.03418
Publikováno v:
New J. Phys. 26, 063033 (2024)
We undertake a theoretical study of a finite-time quantum Otto engine cycle driven by inter-particle interactions in a weakly interacting one-dimensional Bose gas in the quasicondensate regime. Utilizing a $c$-field approach, we simulate the entire O
Externí odkaz:
http://arxiv.org/abs/2404.16470
Autor:
Watson, R. S., Kheruntsyan, K. V.
Particle-particle correlations, characterized by Glauber's second-order correlation function,play an important role in the understanding of various phenomena in radio and optical astronomy, quantum and atom optics, particle physics, condensed matter
Externí odkaz:
http://arxiv.org/abs/2308.05266
Autor:
Fernández-Torreiro, M., Génova-Santos, R. T., Rubiño-Martín, J. A., López-Caraballo, C. H., Peel, M. W., Arce-Tord, C., Rebolo, R., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Guidi, F., Herranz, D., Hoyland, R., Lasenby, A., Martínez-Gonzalez, E., Piccirillo, L., Poidevin, F., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
The Andromeda Galaxy (M31) is the Local Group galaxy that is most similar to the Milky Way (MW). The similarities between the two galaxies make M31 useful for studying integrated properties common to spiral galaxies. We use the data from the recent Q
Externí odkaz:
http://arxiv.org/abs/2305.08547
Autor:
Fernández-Torreiro, M., Rubiño-Martín, J. A., López-Caraballo, C. H., Génova-Santos, R. T., Peel, M. W., Guidi, F., Harper, S. E., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Herranz, D., Hoyland, R., Lasenby, A., Martínez-Gonzalez, E., Piccirillo, L., Poidevin, F., Rebolo, R., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
Anomalous Microwave Emission (AME) is an important emission component between 10 and 60 GHz that is not yet fully understood. It seems to be ubiquituous in our Galaxy and is observed at a broad range of angular scales. Here we use the new QUIJOTE-MFI
Externí odkaz:
http://arxiv.org/abs/2305.06762
Autor:
Herranz, D., López-Caniego, M., López-Caraballo, C. H., Génova-Santos, R. T., Perrott, Y. C., Rubiño-Martín, J. A., Rebolo, R., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Fernández-Torreiro, M., Guidi, F., Hoyland, R. J., Lasenby, A. N., Martínez-González, E., Peel, M. W., Piccirillo, L., Poidevin, F., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
We present the catalogue of Q-U-I JOint TEnerife (QUIJOTE) Wide Survey radio sources extracted from the maps of the Multi-Frequency Instrument compiled between 2012 and 2018. The catalogue contains 786 sources observed in intensity and polarization,
Externí odkaz:
http://arxiv.org/abs/2301.05118
Autor:
de la Hoz, E., Barreiro, R. B., Vielva, P., Martínez-González, E., Rubiño-Martín, J. A., Casaponsa, B., Guidi, F., Ashdown, M., Génova-Santos, R. T., Artal, E., Casas, F. J., Fernández-Cobos, R., Fernández-Torreiro, M., Herranz, D., Hoyland, R. J., Lasenby, A. N., López-Caniego, M., López-Caraballo, C. H., Peel, M. W., Piccirillo, L., Poidevin, F., Rebolo, R., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Watson, R. A.
We derive linearly polarized astrophysical component maps in the Northern Sky from the QUIJOTE-MFI data at 11 and 13 GHz in combination with the WMAP K and Ka bands (23 and 33 GHz) and all Planck polarized channels (30-353 GHz), using the parametric
Externí odkaz:
http://arxiv.org/abs/2301.05117
Autor:
Poidevin, F., Génova-Santos, R. T., Rubiño-Martín, J. A., López-Caraballo, C. H., Watson, R. A., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Fernández-Torreiro, M., Guidi, F., Herranz, D., Hoyland, R. J., Lasenby, A. N., Martinez-Gonzalez, E., Peel, M. W., Piccirillo, L., Rebolo, R., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P.
The QUIJOTE-MFI Northern Hemisphere Wide-Survey has provided maps of the sky above declinations $-30^\circ$ at 11, 13, 17 and 19$\,$GHz. These data are combined with ancillary data to produce Spectral Energy Distributions in intensity in the frequenc
Externí odkaz:
http://arxiv.org/abs/2301.05116
Autor:
Guidi, F., Génova-Santos, R. T., Rubiño-Martín, J. A., Peel, M. W., Fernández-Torreiro, M., López-Caraballo, C. H., Vignaga, R., de la Hoz, E., Vielva, P., Watson, R. A., Ashdown, M., Dickinson, C., Artal, E., Barreiro, R. B., Casas, F. J., Herranz, D., Hoyland, R. J., Lasenby, A. N., Martinez-Gonzalez, E., Piccirillo, L., Poidevin, F., Rebolo, R., Ruiz-Granados, B., Tramonte, D., Vansyngel, F.
The Haze is an excess of microwave intensity emission surrounding the Galactic centre. It is spatially correlated with the $\gamma$-ray Fermi bubbles, and with the S-PASS radio polarization plumes, suggesting a possible common provenance. The models
Externí odkaz:
http://arxiv.org/abs/2301.05115
Autor:
Tramonte, D., Génova-Santos, R. T., Rubiño-Martín, J. A., Vielva, P., Poidevin, F., López-Caraballo, C. H., Peel, M. W., Ashdown, M., Artal, E., Barreiro, R. B., Casas, F. J., de la Hoz, E., Fernández-Torreiro, M., Guidi, F., Herranz, D., Hoyland, R. J., Lasenby, A. N., Martinez-Gonzalez, E., Piccirillo, L., Rebolo, R., Ruiz-Granados, B., Vansyngel, F., Watson, R. A.
We present new intensity and polarisation maps obtained with the QUIJOTE experiment towards the Galactic regions W49, W51 and IC443, covering the frequency range from 10 to 20 GHz at $\sim$ 1 deg angular resolution, with a sensitivity in the range 35
Externí odkaz:
http://arxiv.org/abs/2301.05114