Zobrazeno 1 - 10
of 14 062
pro vyhledávání: '"Genova, A."'
Autor:
Macías-Pérez, J. F., Fernández-Torreiro, M., Catalano, A., Fasano, A., Aguiar, M., Beelen, A., Benoit, A., Bideaud, A., Bounmy, J., Bourrion, O., Calvo, M., Castro-Almazán, J. A., de Bernardis, P., de Petris, M., de Taoro, A. P., Garde, G., Génova-Santos, R. T., Gomez, A., Gómez-Renasco, M. F., Goupy, J., Hoarau, C., Hoyland, R., Lagache, G., Marpaud, J., Marton, M., Masi, S., Monfardini, A., Peel, M. W., Pisano, G., Ponthieu, N., Rebolo, R., Roni, S., Roudier, S., Rubiño-Martín, J. A., Tourres, D., Tucker, C., Viera-Curvelo, T., Vescovi, C.
Kinetic inductance detectors (KIDs) have been proven as reliable systems for astrophysical observations, especially in the millimetre range. Their compact size enables to optimally fill the focal plane, thus boosting sensitivity. The KISS (KIDs Inter
Externí odkaz:
http://arxiv.org/abs/2409.20272
Autor:
Chae, Sooyong, Huang, Tongyu, Rodrıguez-Nunez, Omar, Lucas, Théotim, Vanel, Jean-Charles, Vizet, Jérémy, Pierangelo, Angelo, Piavchenko, Gennadii, Genova, Tsanislava, Ajmal, Ajmal, Ramella-Roman, Jessica C., Doronin, Alexander, Ma, Hui, Novikova, Tatiana
The translation of imaging Mueller polarimetry to clinical practice is often hindered by large footprint and relatively slow acquisition speed of the existing instruments. Using polarization-sensitive camera as a detector may reduce instrument dimens
Externí odkaz:
http://arxiv.org/abs/2409.13073
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:
Proceedings of the 25th Int. Society for Music Information Retrieval Conference, San Francisco, United States, 2024
Deep generative models are now able to synthesize high-quality audio signals, shifting the critical aspect in their development from audio quality to control capabilities. Although text-to-music generation is getting largely adopted by the general pu
Externí odkaz:
http://arxiv.org/abs/2408.00196
Autor:
Milaković, Dinko, Webb, John K., Molaro, Paolo, Lee, Chung-Chi, Jethwa, Prashin, Cupani, Guido, Murphy, Michael T., Welsh, Louise, D'Odorico, Valentina, Cristiani, Stefano, Santos, Ricardo Génova, Martins, Carlos J. A. P., Nunes, Nelson J., Schmidt, Tobias M., Pepe, Francesco A., Osorio, Maria Rosa Zapatero, Alibert, Yann, Hernández, J. I. González, Di Marcantonio, Paolo, Palle, Enric, Santos, Nuno C., Rebolo, Rafael
Chemical evolution models predict a gradual build-up of $^{13}$C in the universe, based on empirical nuclear reaction rates and assumptions on the properties of stellar populations. However, old metal-poor stars within the Galaxy contain more $^{13}$
Externí odkaz:
http://arxiv.org/abs/2407.17953
Autor:
Remazeilles, M., Douspis, M., Rubiño-Martín, J. A., Banday, A. J., Chluba, J., de Bernardis, P., De Petris, M., Hernández-Monteagudo, C., Luzzi, G., Macias-Perez, J., Masi, S., Namikawa, T., Salvati, L., Tanimura, H., Aizawa, K., Anand, A., Aumont, J., Baccigalupi, C., Ballardini, M., Barreiro, R. B., Bartolo, N., Basak, S., Bersanelli, M., Blinov, D., Bortolami, M., Brinckmann, T., Calabrese, E., Campeti, P., Carinos, E., Carones, A., Casas, F. J., Cheung, K., Clermont, L., Columbro, F., Coppolecchia, A., Cuttaia, F., de Haan, T., de la Hoz, E., Della Torre, S., Diego-Palazuelos, P., D'Alessandro, G., Eriksen, H. K., Fuskeland, U., Galloni, G., Galloway, M., Gervasi, M., Génova-Santos, R. T., Ghigna, T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., González, R. González, Gruppuso, A., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Herranz, D., Kohri, K., Komatsu, E., Lamagna, L., Lattanzi, M., Leloup, C., Levrier, F., Lonappan, A. I., López-Caniego, M., Maffei, B., Martínez-González, E., Matarrese, S., Matsumura, T., Micheli, S., Migliaccio, M., Monelli, M., Montier, L., Morgante, G., Nagano, Y., Nagata, R., Novelli, A., Omae, R., Pagano, L., Paoletti, D., Pavlidou, V., Piacentini, F., Pinchera, M., Polenta, G., Porcelli, L., Ritacco, A., Ruiz-Granda, M., Sakurai, Y., Scott, D., Shiraishi, M., Stever, S. L., Sullivan, R. M., Takase, Y., Tassis, K., Terenzi, L., Tomasi, M., Tristram, M., Vacher, L., van Tent, B., Vielva, P., Wehus, I. K., Westbrook, B., Weymann-Despres, G., Wollack, E. J., Zannoni, M., Zhou, Y.
We assess the capabilities of the LiteBIRD mission to map the hot gas distribution in the Universe through the thermal Sunyaev-Zeldovich (SZ) effect. Our analysis relies on comprehensive simulations incorporating various sources of Galactic and extra
Externí odkaz:
http://arxiv.org/abs/2407.17555
Autor:
Tsujii, Miku, Baselmans, Jochem J. A., Choi, Jihoon, Coppens, Antonio H. M., Fasano, Alessandro, Génova-Santos, Ricardo Tanausú, Hattori, Makoto, Hazumi, Masashi, Honda, Shunsuke, Ikemitsu, Takuji, Ishida, Hidesato, Ishitsuka, Hikaru, Jeong, Hoyong, Jo, Yonggil, Karatsu, Kenichi, Kataoka, Keisuke, Kiuchi, Kenji, Komine, Junta, Koyano, Ryo, Kutsuma, Hiroki, Lee, Kyungmin, Mima, Satoru, Nagai, Makoto, Nagasaki, Taketo, Naruse, Masato, Oguri, Shugo, Otani, Chiko, Peel, Michael W., Rebolo, Rafael, Rubiño-Martín, José Alberto, Sekimoto, Yutaro, Sueno, Yoshinori, Suzuki, Junya, Taino, Tohru, Tajima, Osamu, Tanaka, Tomonaga, Thoen, David J., Tomita, Nozomu, Tsuji, Yuta, Uchida, Tomohisa, Won, Eunil, Yoshida, Mitsuhiro
GroundBIRD is a ground-based cosmic microwave background (CMB) experiment for observing the polarization pattern imprinted on large angular scales ($\ell > 6$ ) from the Teide Observatory in Tenerife, Spain. Our primary scientific objective is a prec
Externí odkaz:
http://arxiv.org/abs/2407.17019
Surface cracks in infrastructure can lead to significant deterioration and costly maintenance if not efficiently repaired. Manual repair methods are labor-intensive, time-consuming, and imprecise and thus difficult to scale to large areas. Breakthrou
Externí odkaz:
http://arxiv.org/abs/2407.16874
Autor:
Mennella, Aniello, Arnold, Kam, Azzoni, Susanna, Baccigalupi, Carlo, Banday, A. J., Barreiro, Rita Belén, Barron, Darcy, Bersanelli, Marco, Casas, Francisco J., Casey, Sean, de la Hoz, Elena, Franceschet, Cristian, Jones, Michael E., Genóva-Santos, Ricardo T., Hoyland, R., Lee, Adrian T., Martinez-Gonzalez, Enrique, Montonati, Filippo, Rubiño-Martín, José-Alberto, Taylor, Angela, Vielva, Patricio
Publikováno v:
Proc. SPIE conference on Astronomical Telescopes + Instrumentation, Yokohama, 16-22 June 2024
In this paper we present the European Low Frequency Survey (ELFS), a project that will enable foregrounds-free measurements of the primordial $B$-mode polarization and a detection of the tensor-to-scalar ratio, $r$, to a level $\sigma(r) = 0.001$ by
Externí odkaz:
http://arxiv.org/abs/2406.10309
Autor:
Hobson, M. J., Bouchy, F., Lavie, B., Lovis, C., Adibekyan, V., Prieto, C. Allende, Alibert, Y., Barros, S. C. C., Castro-González, A., Cristiani, S., D'Odorico, V., Damasso, M., Di Marcantonio, P., Dumusque, X., Ehrenreich, D., Figueira, P., Santos, R. Génova, Hernández, J. I. González, Lillo-Box, J., Curto, G. Lo, Martins, C. J. A. P., Mehner, A., Micela, G., Molaro, P., Nunes, N. J., Palle, E., Pepe, F., Rebolo, R., Rodrigues, J., Santos, N., Sousa, S. G., Sozzetti, A., Mascareño, A. Suárez, Tabernero, H. M., Udry, S., Osorio, M. -R. Zapatero, Armstrong, D. J., Ciardi, D. R., Collins, K. A., Collins, K. I., Everett, M., Gandolfi, D., Howell, S. B., Jenkins, J. M., Kielkopf, J., Livingston, J. H., Lund, M. B., Mireles, I., Ricker, G. R., Schwarz, R. P., Seager, S., Tan, T. -G., Ting, E. B., Winn, J. N.
Publikováno v:
A&A 688, A216 (2024)
Since 2018, the ESPRESSO spectrograph at the VLT has been hunting for planets in the Southern skies via the RV method. One of its goals is to follow up candidate planets from transit surveys such as the TESS mission, particularly small planets. We an
Externí odkaz:
http://arxiv.org/abs/2406.06278