Zobrazeno 1 - 10
of 4 519
pro vyhledávání: '"P, Barria"'
Autor:
Addesa, F., Anderson, T., Barria, P., Basile, C., Benaglia, A., Bertoni, R., Bethani, A., Bianco, R., Bornheim, A., Boldrini, G., Boletti, A., Bulla, A., Campana, M., Cardwell, B., Carniti, P., Cetorelli, F., De Guio, F., De Leo, K., De Riggi, F., Dervan, J., Fernandez, E., Gaile, A., Gallinaro, M., Ghezzi, A., Gotti, C., Goldouzian, R., Guglielmi, V., Heering, A., Hu, Z., Jose, M., Karneyeu, A., Krishna, A., Kronheim, B., Kuo, C., La Torre, A., Li, A., Lombardi, F., Lucchini, M. T., Malberti, M., Mao, Y., Marzocchi, B., Meridiani, P., Musienko, Y., Neu, C., Organtini, G., Orimoto, T., Palmer, C., Paganoni, M., Palluotto, S., Paramatti, R., Pessina, G., Perelman, R. T., Quaranta, C., Redaelli, N., Redaelli, S., Gutiérrez, G. Reales, Ronchi, S., Santanastasio, F., Schmidt, I., Silva, J. C., Sorrentino, G., Sun, X., de Fatis, T. Tabarelli, Tosi, M., Ujvari, B., Varela, J., Wang, J., Wayne, M., White, S., Zhang, L., Zhang, M.
For the High-Luminosity (HL-LHC) phase, the upgrade of the Compact Muon Solenoid (CMS) experiment at CERN will include a novel MIP Timing Detector (MTD). The central part of MTD, the barrel timing layer (BTL), is designed to provide a measurement of
Externí odkaz:
http://arxiv.org/abs/2410.08738
Autor:
Peña, Cristián, Wang, Christina, Xie, Si, Bornheim, Adolf, Barría, Matías, Martín, Claudio San, Vega, Valentina, Apresyan, Artur, Knehr, Emanuel, Korzh, Boris, Narváez, Lautaro, Patel, Sahil, Shaw, Matthew, Spiropulu, Maria
We present the first detailed study of an 8-channel $2\times2$ mm$^{2}$ WSi superconducting microwire single photon detector (SMSPD) array exposed to 120 GeV proton beam and 8 GeV electron and pion beam at the Fermilab Test Beam Facility. The SMSPD d
Externí odkaz:
http://arxiv.org/abs/2410.00251
Autor:
Van de Steene, Griet, van Hoof, Peter, Kimeswenger, Stefan, Hajduk, Marcin, Tafoya, Daniel, Toala, Jesus, Zijlstra, Albert, Barria, Daniela
Optical spectra of the Very Late Thermal Pulse (VLTP) object V4334 Sgr have shown a rapidly changing spectrum resulting from shocks in the outflow, which created a new bipolar nebula inside the old nebula. We see C II and C III emission lines emergin
Externí odkaz:
http://arxiv.org/abs/2409.13289
Autor:
Hajduk, Marcin, van Hoof, Peter A. M., Zijlstra, Albert A., Van de Steene, Griet, Kimeswenger, Stefan, Barría, Daniela, Tafoya, Daniel, Toalá, Jesús A.
Publikováno v:
A&A 688, L21 (2024)
The very late thermal pulse (VLTP) affects the evolution of $\sim$20\% of 1--8\,$\mathrm M_\odot$ stars, repeating the last phases of the red giant within a few years and leading to the formation of a new, but hydrogen-poor nebula within the old plan
Externí odkaz:
http://arxiv.org/abs/2407.18020
Autor:
Dutta, Irene, Madrid, Christopher, Heller, Ryan, Nanda, Shirsendu, Shekar, Danush, Martín, Claudio San, Barría, Matías, Apresyan, Artur, Ye, Zhenyu, Brooks, William K., Chen, Wei, D'Amen, Gabriele, Giacomini, Gabriele, Tricoli, Alessandro, Hayrapetyan, Aram, Lee, Hakseong, Köseyan, Ohannes Kamer, Los, Sergey, Nakamura, Koji, Kita, Sayuka, Imamura, Tomoka, Peña, Cristían, Xie, Si
We present the results of an extensive evaluation of strip and pixel AC-LGAD sensors tested with a 120 GeV proton beam, focusing on the influence of design parameters on the sensor temporal and spatial resolutions. Results show that reducing the thic
Externí odkaz:
http://arxiv.org/abs/2407.09928
Autor:
Fasano, Alessandro, Ade, Peter, Aravena, Manuel, Barria, Emilio, Beelen, Alexandre, Benoit, Alain, Béthermin, Matthieu, Bounmy, Julien, Bourrion, Olivier, Bres, Guillaume, Calvo, Martino, Catalano, Andrea, De Breuck, Carlos, Désert, François-Xavier, Dubois, Cédric, Durán, Carlos, Fenouillet, Thomas, Garcia, Jose, Garde, Gregory, Goupy, Johannes, Hoarau, Christophe, Hu, Wenkai, Lagache, Guilaine, Lambert, Jean-Charles, Levy-Bertrand, Florence, Lundgren, Andreas, Macías-Pérez, Juan-Francisco, Marpaud, Julien, Monfardini, Alessandro, Pisano, Giampaolo, Ponthieu, Nicolas, Prieur, Leo, Roni, Samuel, Roudier, Sebastien, Tourres, Damien, Tucker, Carol, Van Cuyck, Mathilde
Modern astrophysics relies on intricate instrument setups to meet the demands of sensitivity, sky coverage, and multi-channel observations. An example is the CONCERTO project, employing advanced technology like kinetic inductance detectors and a Mart
Externí odkaz:
http://arxiv.org/abs/2406.16334
Autor:
Hu, W., Beelen, A., Lagache, G., Fasano, A., Lundgren, A., Ade, P., Aravena, M., Barria, E., Benoit, A., Bethermin, M., Bounmy, J., Bourrion, O., Bres, G., De Breuck, C., Calvo, M., Catalano, A., Desert, F. -X., Dubois, C., Duran, C. A, Fenouillet, T., Garcia, J., Garde, G., Goupy, J., Hoarau, C., Lambert, J. -C., Lellouch, E., Levy-Bertrand, F., Macias-Perez, J., Marpaud, J., Monfardini, A., Pisano, G., Ponthieu, N., Prieur, L., Quinatoa, D., Roni, S., Roudier, S., Tourres, D., Tucker, C., Van Cuyck, M.
Publikováno v:
A&A 689, A20 (2024)
We present the data-processing algorithms and the performance of CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn epoch) in continuum by analysing the data from the commissioning and scientific observations. The beam pattern is charact
Externí odkaz:
http://arxiv.org/abs/2406.15572
Autor:
Raba, Matthias, Triqueneaux, Sébastien, Butterworth, James, Schmoranzer, David, Barria, Emilio, Debray, Jérôme, Donnier-Valentin, Guillaume, Gandit, Thibaut, Gerardin, Anne, Goupy, Johannes, Tissot, Olivier, Collin, Eddy, Fefferman, Andrew
Publikováno v:
Physical Review APPLIED 22, 024027 (2024)
Many laboratories routinely cool samples to 10 mK, but relatively few can cool condensed matter below 1 mK. Easy access to the microkelvin range would propel fields such as quantum sensors and quantum materials. Such temperatures are achieved with ad
Externí odkaz:
http://arxiv.org/abs/2404.19352
Autor:
Barría, Sebastián
Let $\mathbb{A}$ and $\mathbb{S}$ denote the double arrow of Alexandroff and the Sorgenfrey line, respectively. We show that for any $n\geq 1$, the space of all unions of at most $n$ closed intervals of $\mathbb{A}$ is not homogeneous. We also prove
Externí odkaz:
http://arxiv.org/abs/2404.13741
Autor:
Fasano, Alessandro, Ade, Peter, Aravena, Manuel, Barria, Emilio, Beelen, Alexandre, Benoît, Alain, Béthermin, Matthieu, Bounmy, Julien, Bourrion, Olivier, Bres, Guillaume, Calvo, Martino, Catalano, Andrea, De Breuck, Carlos, Désert, François-Xavier, Durán, Carlos, Fenouillet, Thomas, Garcia, Jose, Garde, Gregory, Goupy, Johannes, Groppi, Christopher, Hoarau, Christophe, Hu, Wenkai, Lagache, Guilaine, Lambert, Jean-Charles, Leggeri, Jean-Paul, Levy-Bertrand, Florence, Lundgren, Andreas, Macías-Pérez, Juan, Mani, Hamdi, Marpaud, Julien, Mauskopf, Philip, Monfardini, Alessandro, Pisano, Giampaolo, Ponthieu, Nicolas, Prieur, Leo, Roni, Samuel, Roudier, Sebastien, Tourres, Damien, Tucker, Carol
Publikováno v:
EPJ Web of Conferences 293, 00018 (2024)
CONCERTO (CarbON CII line in post-rEionization and ReionizaTiOn) is a low-resolution Fourier transform spectrometer dedicated to the study of star-forming galaxies and clusters of galaxies in the transparent millimeter windows from the ground. It is
Externí odkaz:
http://arxiv.org/abs/2311.04704