Zobrazeno 1 - 10
of 3 808
pro vyhledávání: '"Romero G"'
Autor:
Cáceres G. Germán, Romero G. Luis, Bonilla G. Sergio, Guerrero C. Fatima, Fernandez M. Manuel, Capilla G. Jaime, Tejero C. Jesús
Publikováno v:
Viruses, Vol 16, Iss 7, p 1164 (2024)
Sheep pox and goat pox are infectious viral diseases that affect ovine and caprine animals and are caused by two viruses of the family Poxviridae, genus Capripoxvirus. Sheep pox has been traditionally endemic in Africa, the Middle East, and several S
Externí odkaz:
https://doaj.org/article/4762edffcc6a4da08e1a5318606ad58e
The intense star formation in starburst galaxies results in the formation of intense winds that sweep matter up to several kpc out of the galactic plane. These winds can be detected in many bands of the electromagnetic spectrum. In this opportunity,
Externí odkaz:
http://arxiv.org/abs/2407.21679
Autor:
García-Azorín, P., Cárdenas-López, F. A., Huber, G. B. P., Romero, G., Werninghaus, M., Motzoi, F., Filipp, S., Sanz, M.
Multi-mode superconducting circuits offer a promising platform for engineering robust systems for quantum computation. Previous studies have shown that single-mode devices cannot simultaneously exhibit resilience against multiple decoherence sources
Externí odkaz:
http://arxiv.org/abs/2407.18895
The extragalactic microquasar S26 has the most powerful jets observed in accreting binaries, with a kinetic luminosity of $L_{\rm jet}\sim10^{40}\,{\rm erg\,s^{-1}}$. According to the jet-disk symbiosis model, this implies that the accretion power to
Externí odkaz:
http://arxiv.org/abs/2405.05221
Starburst galaxies are undergoing intense episodes of star formation. In these galaxies, gas is ejected into the surrounding environment through winds created by the effect of hot stars and supernova explosions. When interacting with the intergalacti
Externí odkaz:
http://arxiv.org/abs/2403.05709
Autor:
Abaroa, L., Romero, G. E.
We have recently proposed that supercritical colliding wind binaries (SCWBs) are suitable scenarios for particle acceleration and nonthermal radiation. In these X-ray binary systems (XRBs), the wind from the companion star collides with the wind ejec
Externí odkaz:
http://arxiv.org/abs/2311.15050
Autor:
Mennella, A., Ade, P., Almela, A., Amico, G., Arnaldi, L. H., Aumont, J., Banfi, S., Battistelli, E. S., Bélier, B., Bergé, L., Bernard, J. -Ph., de Bernardis, P., Bersanelli, M., Bonaparte, J., Bonilla, J. D., Bunn, E., Buzi, D., Cacciotti, F., Camilieri, D., Cavaliere, F., Chanial, P., Chapron, C., Colombo, L., Columbro, F., Coppolecchia, A., Costanza, M. B., D'Alessandro, G., De Gasperis, G., De Leo, M., De Petris, M., Del Castillo, N., Dheilly, S., Etchegoyen, A., Ferazzoli, S., Ferreyro, L. P., Franceschet, C., Lerena, M. M. Gamboa, Ganga, K., García, B., Redondo, M. E. García, Gayer, D., Geria, J. M., Gervasi, M., Giard, M., Gilles, V., Berisso, M. Gómez, Gonzalez, M., Gradziel, M., Grandsire, L., Hamilton, J. -Ch., Hampel, M. R., Isopi, G., Kaplan, J., Lamagna, L., Lazarte, F., Loucatos, S., Maffei, B., Mancilla, A., Mandelli, S., Manzan, E., Marchitelli, E., Marnieros, S., Marty, W., Masi, S., May, A., Maya, J., McCulloch, M., Mele, L., Melo, D., Mirón-Granese, N., Montier, L., Mousset, L., Müller, N., Nati, F., O'Sullivan, C., Paiella, A., Pajot, F., Paradiso, S., Pascale, E., Passerini, A., Pelosi, A., Perciballi, M., Pezzotta, F., Piacentini, F., Piat, M., Piccirillo, L., Pisano, G., Platino, M., Polenta, G., Prêle, D., Rambaud, D., Ramos, G., Rasztocky, E., Régnier, M., Reyes, C., Rodríguez, F., Rodríguez, C. A., Romero, G. E., Salum, J. M., Schillaci, A., Scóccola, C., Stankowiak, G., Tartari, A., Thermeau, J. -P., Timbie, P., Tomasi, M., Torchinsky, S., Tucker, G., Tucker, C., Vacher, L., Voisin, F., Wright, M., Zannoni, M., Zullo, A.
The Q&U Bolometric Interferometer for Cosmology (QUBIC) is the first bolometric interferometer designed to measure the primordial B-mode polarization of the Cosmic Microwave Background (CMB). Bolometric interferometry is a novel technique that combin
Externí odkaz:
http://arxiv.org/abs/2311.02779
Autor:
Manzan, E., Regnier, M., Hamilton, J-Ch., Mennella, A., Errard, J., Zapelli, L., Torchinsky, S. A., Paradiso, S., Battistelli, E., Bersanelli, M., De Bernardis, P., De Petris, M., D'Alessandro, G., Gervasi, M., Masi, S., Piat, M., Rasztocky, E., Romero, G. E, Scoccola, C. G., Zannoni, M., Collaboration, the QUBIC
In the quest for the faint primordial B-mode polarization of the Cosmic Microwave Background, three are the key requirements for any present or future experiment: an utmost sensitivity, excellent control over instrumental systematic effects and over
Externí odkaz:
http://arxiv.org/abs/2311.01814
Autor:
Romero, G. E., Gancio, G., Benaglia, P., González, J. M., Rasztocky, E., Command, H., Valdez, G., Tarcetti, E., Hauscarriaga, F., Alarcón, P., Aquino, F., Alí, M., Cabral, L. F., Capuccio, D., Contreras, M., Díaz, E., Duarte, N., García, L. M., Perilli, D., Otonello, P., Spagnolo, S.
We present a proposal for the construction and development of a new instrument for radio astronomical observations based on interferometric techniques, that will provide high angular resolution in the 21 cm band, with the intention of improving and e
Externí odkaz:
http://arxiv.org/abs/2309.16891
Autor:
Regnier, M., Manzan, E., Hamilton, J. -Ch, Mennella, A., Errard, J., Zapelli, L., Torchinsky, S. A., Paradiso, S., Battistelli, E., De Bernardis, P., Colombo, L., De Petris, M., D'Alessandro, G., Garcia, B., Gervasi, M., Masi, S., Mousset, L., Granese, N. Miron, O'Sullivan, C., Piat, M., Rasztocky, E., Romero, G. E., Scoccola, C. G., Zannoni, M.
Publikováno v:
A&A 686, A271 (2024)
Astrophysical polarized foregrounds represent the most critical challenge in Cosmic Microwave Background (CMB) B-mode experiments. Multi-frequency observations can be used to constrain astrophysical foregrounds to isolate the CMB contribution. Howeve
Externí odkaz:
http://arxiv.org/abs/2309.02957