Zobrazeno 1 - 10
of 15 674
pro vyhledávání: '"Piro, A."'
Autor:
Arora, M. M., Balogh, L., Beaufort, C., Brossard, A., Chapellier, M., Clarke, J., Corcoran, E. C., Coquillat, J. -M., Dastgheibi-Fard, A., Deng, Y., Durnford, D., Garrah, C., Gerbier, G., Giomataris, I., Giroux, G., Gorel, P., Gros, M., Gros, P., Guillaudin, O., Hoppe, E. W., Katsioulas, I., Kelly, F., Knights, P., Lautridou, P., Makowski, A., Manthos, I., Martin, R. D., Matthews, J., McCallum, H. M., Meadows, H., Millins, L., Muraz, J. -F., Neep, T., Nikolopoulos, K., Panchal, N., Piro, M. -C., Rowe, N., Santos, D., Savvidis, G., Savvidis, I., Spathara, D., Fernandez, F. Vazquez de Sola, Ward, R.
Spherical proportional counters (SPCs) are gaseous particle detectors sensitive to single ionization electrons in their target media, with large detector volumes and low background rates. The $\mbox{NEWS-G}$ collaboration employs this technology to s
Externí odkaz:
http://arxiv.org/abs/2410.16350
Autor:
Anderson, J. P., Contreras, C., Stritzinger, M. D., Hamuy, M., Phillips, M. M., Suntzeff, N. B., Morrell, N., Gonzalez-Gaitan, S., Gutierrez, C. P., Burns, C. R., Hsiao, E. Y., Anais, J., Ashall, C., Baltay, C., Baron, E., Bersten, M., Busta, L., Castellon, S., de Jaeger, T., DePoy, D., Filippenko, A. V., Folatelli, G., Forster, F., Galbany, L., Gall, C., Goobar, A., Gonzalez, C., Hadjiyska, E., Hoeflich, P., Krisciunas, K., Krzeminski, W., Li, W., Madore, B., Marshall, J., Martinez, L., Nugent, P., Pessi, P. J., Piro, A. L., Rheault, J-P., Ryder, S., Seron, J., Shappee, B. J., Taddia, F., Torres, S., Thomas-Osip, J., Uddin, S.
Type II supernovae (SNeII) mark the endpoint in the lives of hydrogen-rich massive stars. Their large explosion energies and luminosities allow us to measure distances, metallicities, and star formation rates into the distant Universe. To fully explo
Externí odkaz:
http://arxiv.org/abs/2410.06738
Failed supernovae (SNe), which are likely the main channel for forming stellar-mass black holes, are predicted to accompany mass ejections much weaker than typical core-collapse SNe. We conduct a grid of one-dimensional radiation hydrodynamical simul
Externí odkaz:
http://arxiv.org/abs/2410.07055
Autor:
Alfonso-Pita, E., Behnke, E., Bressler, M., Broerman, B., Clark, K., Coppejans, R., Corbett, J., Crisler, M., Dahl, C. E., Dering, K., Croix, A. de St., Durnford, D., Giampa, P., Hall, J., Harris, O., Hawley-Herrera, H., Lamb, N., Laurin, M., Levine, I., Lippincott, W. H., Neilson, R., Piro, M. -C., Pyda, D., Sheng, Z., Sweeney, G., Vázquez-Jáuregui, E., Westerdale, S., Whitis, T. J., Wright, A., Zhang, J., Zhang, R., Zuñiga-Reyes, A.
A device filled with pure xenon first demonstrated the ability to operate simultaneously as a bubble chamber and scintillation detector in 2017. Initial results from data taken at thermodynamic thresholds down to ~4 keV showed sensitivity to ~20 keV
Externí odkaz:
http://arxiv.org/abs/2410.07241
The study of motility control by smart agents offers a promising platform for systematically exploring the fundamental physical constraints underlying the functioning of bio-inspired micro-machines operating far from equilibrium. Here, we address the
Externí odkaz:
http://arxiv.org/abs/2409.12595
We investigate how the Large Magellanic Cloud (LMC) impacts the predicted signals in near-future direct detection experiments for non-standard dark matter (DM) interactions, using the Auriga cosmological simulations. We extract the local DM distribut
Externí odkaz:
http://arxiv.org/abs/2409.09119
Autor:
Kremer, Kyle, Ye, Claire S., Heinke, Craig O., Piro, Anthony L., Ransom, Scott M., Rasio, Frederic A.
Alongside the population of several hundred radio millisecond pulsars currently known in Milky Way globular clusters, a subset of six slowly spinning pulsars (spin periods $0.3-4$\,s) are also observed. With inferred magnetic fields $\gtrsim 10^{11}\
Externí odkaz:
http://arxiv.org/abs/2409.07527
Autor:
Rinella, Gianluca Aglieri, Aglietta, Luca, Antonelli, Matias, Barile, Francesco, Benotto, Franco, Beolè, Stefania Maria, Botta, Elena, Bruno, Giuseppe Eugenio, Carnesecchi, Francesca, Colella, Domenico, Colelli, Angelo, Contin, Giacomo, De Robertis, Giuseppe, Dumitrache, Florina, Elia, Domenico, Ferrero, Chiara, Fransen, Martin, Kluge, Alex, Kumar, Shyam, Lemoine, Corentin, Licciulli, Francesco, Lim, Bong-Hwi, Loddo, Flavio, Mager, Magnus, Marras, Davide, Martinengo, Paolo, Pastore, Cosimo, Patra, Rajendra Nath, Perciballi, Stefania, Piro, Francesco, Prino, Francesco, Ramello, Luciano, Ramos, Arianna Grisel Torres, Reidt, Felix, Russo, Roberto, Sarritzu, Valerio, Savino, Umberto, Schledewitz, David, Selina, Mariia, Senyukov, Serhiy, Sitta, Mario, Snoeys, Walter, Sonneveld, Jory, Suljic, Miljenko, Triloki, Triloki, Turcato, Andrea
In the context of the CERN EP R&D on monolithic sensors and the ALICE ITS3 upgrade, the Tower Partners Semiconductor Co (TPSCo) 65 nm process has been qualified for use in high energy physics, and adopted for the ALICE ITS3 upgrade. An Analog Pixel T
Externí odkaz:
http://arxiv.org/abs/2407.18528
Autor:
D'Andrea, Matteo, Macculi, Claudio, Lotti, Simone, Piro, Luigi, Argan, Andrea, Minervini, Gabriele, Torrioli, Guido, Chiarello, Fabio, Barusso, Lorenzo Ferrari, Gatti, Flavio, Rigano, Manuela
Publikováno v:
Proceedings Volume 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray; 130930X (2024)
The X-IFU is one of the two instruments of ATHENA, the next ESA large X-ray observatory. It is a cryogenic spectrometer based on an array of TES microcalorimeters. To reduce the particle background, the TES array works in combination with a Cryogenic
Externí odkaz:
http://arxiv.org/abs/2407.14083
Autor:
Arora, M. M., Balogh, L., Beaufort, C., Brossard, A., Chapellier, M., Clarke, J., Corcoran, E. C., Coquillat, J. -M., Dastgheibi-Fard, A., Deng, Y., Durnford, D., Garrah, C., Gerbier, G., Giomataris, I., Giroux, G., Gorel, P., Gros, M., Gros, P., Guillaudin, O., Hoppe, E. W., Katsioulas, I., Kelly, F., Knights, P., Lautridou, P., Makowski, A., Manthos, I., Martin, R. D., Matthews, J., McCallum, H. M., Meadows, H., Millins, L., Muraz, J. -F., Neep, T., Nikolopoulos, K., Panchal, N., Piro, M. -C., Rowe, N., Santos, D., Savvidis, G., Savvidis, I., Spathara, D., Fernandez, F. Vazquez de Sola, Ward, R.
The NEWS-G direct detection experiment uses spherical proportional counters to search for light dark matter candidates. New results from a 10 day physics run with a $135\,\mathrm{cm}$ in diameter spherical proportional counter at the Laboratoire Sout
Externí odkaz:
http://arxiv.org/abs/2407.12769