Zobrazeno 1 - 10
of 2 227
pro vyhledávání: '"Tosi, M. P."'
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:
Bellazzini, M., Annibali, F., Correnti, M., Gatto, M., Marinelli, M., Pascale, R., Sacchi, E., Tosi, M., Cignoni, M., Cannon, J. M., Schisgal, L., Bortolini, G., Aloisi, A., Beccari, G., Nipoti, C.
New, deep HST photometry allowed us to identify and study eight compact and bright (M_V< -5.8) star clusters in the outskirts of the star-forming isolated dwarf galaxy NGC5238 (M_*= 10^8 M_sun). Five of these clusters are new discoveries, and six app
Externí odkaz:
http://arxiv.org/abs/2409.16436
We present preliminary findings from the photometric survey "Yes, Magellanic Clouds Again" (YMCA, PI: V. Ripepi), covering 110 square degrees in the outer regions of the Magellanic Clouds (MCs), a pair of interacting galaxies and the most massive dwa
Externí odkaz:
http://arxiv.org/abs/2407.19991
Autor:
Pascale, R., Annibali, F., Tosi, M., Nipoti, C., Marinacci, F., Bellazzini, M., Cannon, J. M., Schisgal, L., Calura, E. Sacchi F.
From deep imaging data obtained with the Large Binocular Telescope as part of the Smallest Scale of Hierarchy Survey (SSH), we have discovered low-surface brightness tidal features around NGC 5238 and UGC 8760, two nearby and relatively isolated dwar
Externí odkaz:
http://arxiv.org/abs/2405.12284
Autor:
Bortolini, G., Cignoni, M., Sacchi, E., Tosi, M., Annibali, F., Pascale, R., Bellazzini, M., Calzetti, D., Adamo, A., Dale, Daniel. A., Fumagalli, M., Gallagher, John. S., Grasha, K., Johnson, Kelsey E., Linden, Sean. T., Messa, M., Östlin, G., Sabbi, E., Wofford, A.
We study the resolved stellar populations and derive the star formation history of NGC 5474, a peculiar star-forming dwarf galaxy at a distance of $\sim 7$ Mpc, using Hubble Space Telescope Advanced Camera for Surveys data from the Legacy Extragalact
Externí odkaz:
http://arxiv.org/abs/2311.08160
Autor:
Bornheim, A., Lustermann, W., Stachon, K., Gutiérrez, G. Reales, Benaglia, A., De Guio, F., Ghezzi, A., Lucchini, M. T., Malberti, M., Palluotto, S., de Fatis, T. Tabarelli, Benettoni, M., Carlin, R., Tosi, M., Rossin, R., Meridiani, P., Paramatti, R., Santanastasio, F., Silva, J. C., Varela, J., Heering, A., Karneyeu, A., Musienko, Y., Wayne, M., Anderson, T., Cox, B., Lara, C. E. Perez, Ledovskoy, A., White, S., Schmidt, I.
Publikováno v:
JINST 18 P08020 (2023)
The barrel section of the novel MIP Timing Detector (MTD) will be constructed as part of the upgrade of the CMS experiment to provide a time resolution for single charged tracks in the range of $30-60$ ps using LYSO:Ce crystal arrays read out with Si
Externí odkaz:
http://arxiv.org/abs/2306.00818
Autor:
Hunt, L. K., Belfiore, F., Lelli, F., Draine, B. T., Marasco, A., Garcia-Burillo, S., Venturi, G., Combes, F., Weiß, A., Henkel, C., Menten, K. M., Annibali, F., Casasola, V., Cignoni, M., McLeod, A., Tosi, M., Beltran, M., Concas, A., Cresci, G., Ginolfi, M., Kumari, N., Mannucci, F.
Publikováno v:
A&A 675, A64 (2023)
The factor relating CO emission to molecular hydrogen column density, XCO, is still subject to uncertainty, in particular at low metallicity. Here, to quantify XCO at two different spatial resolutions, we exploit a dust-based method together with ALM
Externí odkaz:
http://arxiv.org/abs/2305.03443
Autor:
Tosi M. Mwakyandile, Grace A. Shayo, Philip G. Sasi, Ferdinand M. Mugusi, Godfrey Barabona, Takamasa Ueno, Eligius F. Lyamuya
Publikováno v:
BMC Infectious Diseases, Vol 24, Iss 1, Pp 1-10 (2024)
Abstract Background The pathogenesis of hypertension (HTN) in people living with HIV/AIDS (PLHIV) is complex and remains not fully understood. Chronic immune activation (IA) is postulated to be one of the culprits. This notion is derived from studies
Externí odkaz:
https://doaj.org/article/6184462c215e4f8dbfd3c0a9b93f9402
Autor:
Cook, D. O., Lee, J. C., Adamo, A., Calzetti, D., Chandar, R., Whitmore, B. C., Aloisi, A., Cignoni, M., Dale, D. A., Elmegreen, B. G., Fumagalli, M., Grasha, K., Johnson, K. E., Kennicutt, R. C., Kim, H., Linden, S. T., Messa, M., Östlin, G., Ryon, J. E., Sacchi, E., Thilker, D. A., Tosi, M., Wofford, A.
We study the young star cluster populations in 23 dwarf and irregular galaxies observed by the HST Legacy ExtraGalactic Ultraviolet Survey (LEGUS), and examine relationships between the ensemble properties of the cluster populations and those of thei
Externí odkaz:
http://arxiv.org/abs/2212.07519
Autor:
Gilmore, G., Randich, S., Worley, C. C., Hourihane, A., Gonneau, A., Sacco, G. G., Lewis, J. R., Magrini, L., Francois, P., Jeffries, R. D., Koposov, S. E., Bragaglia, A., Alfaro, E. J., Prieto, C. Allende, Blomme, R., Korn, A. J., Lanzafame, A. C., Pancino, E., Recio-Blanco, A., Smiljanic, R., Van Eck, S., Zwitter, T., Bensby, T., Flaccomio, E., Irwin, M. J., Franciosini, E., Morbidelli, L., Damiani, F., Bonito, R., Friel, E. D., Vink, J. S., Prisinzano, L., Abbas, U., Hatzidimitriou, D., Held, E. V., Jordi, C., Paunzen, E., Spagna, A., Jackson, R. J., Apellaniz, J. Maiz, Asplund, M., Bonifacio, P., Feltzing, S., Binney, J., Drew, J., Ferguson, A. M. N., Micela, G., Negueruela, I., Prusti, T., Rix, H. -W., Vallenari, A., Bergemann, M., Casey, A. R., de Laverny, P., Frasca, A., Hill, V., Lind, K., Sbordone, L., Sousa, S. G., Adibekyan, V., Caffau, E., Daflon, S., Feuillet, D. K., Gebran, M., Hernandez, J. I. Gonzalez, Guiglion, G., Herrero, A., Lobel, A., Merle, T., Mikolaitis, S., Montes, D., Morel, T., Ruchti, G., Soubiran, C., Tabernero, H. M., Tautvaisiene, G., Traven, G., Valentini, M., Van der Swaelmen, M., Villanova, S., Vazquez, C. Viscasillas, Bayo, A., Biazzo, K., Carraro, G., Edvardsson, B., Heiter, U., Jofre, P., Marconi, G., Martayan, C., Masseron, T., Monaco, L., Walton, N. A., Zaggia, S., Borsen-Koch, V. Aguirre, Alves, J., Balaguer-Nunez, L., Barklem, P. S., Barrado, D., Bellazzini, M., Berlanas, S. R., Binks, A. S., Bressan, A., Capuzzo-Dolcetta, R., Casagrande, L., Casamiquela, L., Collins, R. S., D'Orazi, V., Dantas, M. L. L., Debattista, V. P., Delgado-Mena, E., Di Marcantonio, P., Drazdauskas, A., Evans, N. W., Famaey, B., Franchini, M., Fremat, Y., Fu, X., Geisler, D., Gerhard, O., Solares, E. A. Gonzalez, Grebel, E. K., Albarran, M. L. Gutierrez, Jimenez-Esteban, F., Jonsson, H., Khachaturyants, T., Kordopatis, G., Kos, J., Lagarde, N., Ludwig, H. -G., Mahy, L., Mapelli, M., Marfil, E., Martell, S. L., Messina, S., Miglio, A., Minchev, I., Moitinho, A., Montalban, J., Monteiro, M. J. P. F. G., Morossi, C., Mowlavi, N., Mucciarelli, A., Murphy, D. N. A., Nardetto, N., Ortolani, S., Paletou, F., Palous, J., Pickering, J. C., Quirrenbach, A., Fiorentin, P. Re, Read, J. I., Romano, D., Ryde, N., Sanna, N., Santos, W., Seabroke, G. M., Spina, L., Steinmetz, M., Stonkute, E., Sutorius, E., Thevenin, F., Tosi, M., Tsantaki, M., Wright, N., Wyse, R. F. G., Zoccali, M., Zorec, J., Zucker, D. B.
Publikováno v:
A&A 666, A120 (2022)
The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100,000 stars, including large representative samples of the stellar populations in the Galaxy, and a well-defin
Externí odkaz:
http://arxiv.org/abs/2208.05432