Zobrazeno 1 - 10
of 10 690
pro vyhledávání: '"A Caputi"'
Autor:
Stefania Curti, Stefano Mattioli, Dario Consonni, Sara Piro, Lucia Miligi, L Mangone, Maria Teresa Landi, Neil E Caporaso, Carolina Mensi, L Giovannetti, Elisabetta Chellini, Elisa Romeo, Alessandro Marinaccio, Antonella Stura, A Martini, Giovanni Brandi, Carlo Genova, M Gangemi, M Davoli, L Richiardi, P Michelozzi, G Serio, Luigi Vimercati, A Caputi, Enrica Migliore, AC Pesatori, L De Maria, Veronica Casotto, B Dallari, M Bonzini, U Fedeli, Alessandra Binazzi, Corrado Negro, Antonio Romanelli, Francesco Carrozza, Domenica Cavone, Federico Tallarigo, Massimo Melis, C Brentisci, M Gilardetti, C Storchi, O Sala, V Cacciarini, L Ancona, Sg Lio, G Frasca, Mc Giurdanella, C Martorana, P Rollo, E Spata, G Dardanoni, S Scondotto, S Stecchi, D Mirabelli, P De Michieli, Simona Stella, Carmela Gioscia, Silvia Eccher, Stefano Murano, Vera Comiati, Flavia D'Agostin, Lucia Benfatto, Iolanda Grappasonni, Gabriella Madeo, Ilaria Cozzi, Staniscia Tommaso, Michele Labianca, Giuseppe Cascone, D Di Marzio, S Rugarli, C Pascucci, A Balestri, MC Delfino, F Pentimone, MR Angius
Publikováno v:
BMJ Open, Vol 13, Iss 8 (2023)
Objectives Workers in the construction industry have been exposed to asbestos in various occupations. In Italy, a National Mesothelioma Registry has been implemented more than 20 years ago. Using cases selected from this registry and exploiting exist
Externí odkaz:
https://doaj.org/article/361ab209f3c44ff98ed1f05d4aff995e
Autor:
Navarro-Carrera, R., Rinaldi, P., Caputi, K. I., Iani, E., Kokorev, V., Kerutt, J., Cooper, R.
We analyze a sample of 4500 photometrically-selected Ha emitter galaxies at redshifts z~2 and z~4-6 selected from James Webb Space Telescope (JWST) Near-Infrared Camera (NIRCam) medium-band images in the Great Observatories Origins Deep Survey South
Externí odkaz:
http://arxiv.org/abs/2410.23249
We characterise the digraphs for which the multipaths, that is disjoint unions of directed paths, yield a matroid. For such graphs, called MP-digraphs, we prove that the Tutte polynomial of the multipath matroid is related to counting certain digraph
Externí odkaz:
http://arxiv.org/abs/2409.14528
Autor:
Long, Arianna S., Casey, Caitlin M., McKinney, Jed, Zavala, Jorge A., Akins, Hollis B., Cooper, Olivia R., Lambrides, Matthieu Bethermin Erini L., Franco, Maximilien, Caputi, Karina, Champagne, Jaclyn B., Man, Allison W. S., Treister, Ezequiel, Manning, Sinclaire M., Sanders, David B., Talia, Margherita, Aravena, Manuel, Clements, D. L., da Cunha, Elisabete, Faisst, Andreas L., Gentile, Fabrizio, Hodge, Jacqueline, Brammer, Gabriel, Brusa, Marcella, Finkelstein, Steven L., Fujimoto, Seiji, Hayward, Christopher C., Ilbert, Olivier, Jolly, Jean-Baptiste, Kartaltepe, Jeyhan S., Knudsen, Kirsten, Koekemoer, Anton M., Liu, Daizhong, Magdis, Georgios, McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E., Scoville, Nick, Sheth, Kartik, Smolcic, Vernesa, Spilker, Justin, Taniguchi, Yoshiaki, Toft, Sune, Urry, C. Megan, Yun, Min
One of the greatest challenges in galaxy evolution over the last decade has been constraining the prevalence of heavily dust-obscured galaxies in the early Universe. At $z>3$, these galaxies are increasingly rare, and difficult to identify as they ar
Externí odkaz:
http://arxiv.org/abs/2408.14546
Autor:
Navarro-Carrera, Rafael, Caputi, Karina I., Iani, Edoardo, Rinaldi, Pierluigi, Kokorev, Vasily, Kerutt, Josephine
Making use of JWST NIRSpec and NIRCam data, we conduct a detailed analysis of the spectroscopic and photometric properties of GN-z8-LAE, a strong Lya emitter at z=8.279. Our goal is to investigate the interstellar medium (ISM) physical conditions tha
Externí odkaz:
http://arxiv.org/abs/2407.14201
Autor:
Costantin, L., Gillman, S., Boogaard, L. A., Pérez-González, P. G., Iani, E., Rinaldi, P., Melinder, J., Gómez, A. Crespo, Colina, L., Greve, T. R., Östlin, G., Wright, G., Alonso-Herrero, A., Álvarez-Márquez, J., Annunziatella, M., Bik., A., Caputi, K. I., Dicken, D., Eckart, A., Hjorth, J., Ilbert, O., Jermann, I., Labiano, A., Langeroodi, D., Peißker, F., Pye, J. P., Tikkanen, T. V., van der Werf, P. P., Walter, F., Ward, M., Güdel, M., Henning, T. K.
Thanks to decades of observations using HST, the structure of galaxies at redshift $z>2$ has been widely studied in the rest-frame ultraviolet regime, which traces recent star formation from young stellar populations. But, we still have little inform
Externí odkaz:
http://arxiv.org/abs/2407.00153
We establish an isomorphism between the 0-degree \"uberhomology and the double homology of finite simplicial complexes, using a Mayer-Vietoris spectral sequence argument. We clarify the correspondence between these theories by providing examples and
Externí odkaz:
http://arxiv.org/abs/2406.18778
Autor:
Iani, Edoardo, Rinaldi, Pierluigi, Caputi, Karina I., Annunziatella, Marianna, Langeroodi, Danial, Melinder, Jens, Pérez-González, Pablo G., Álvarez-Márquez, Javier, Boogaard, Leindert A., Bosman, Sarah E. I., Costantin, Luca, Moutard, Thibaud, Colina, Luis, Östlin, Göran, Greve, Thomas R., Wright, Gillian, Alonso-Herrero, Almudena, Bik, Arjan, Gillman, Steven, Gómez, Alejandro Crespo, Hjorth, Jens, Labiano, Alvaro, Pye, John P., Tikkanen, Tuomo V., van der Werf, Paul P.
We present Virgil, a MIRI extremely red object (MERO) detected with the F1000W filter as part of the MIRI Deep Imaging Survey (MIDIS) observations of the Hubble Ultra Deep Field (HUDF). Virgil is a Lyman-$\alpha$ emitter (LAE) at $z_{spec} = 6.6312\p
Externí odkaz:
http://arxiv.org/abs/2406.18207
This paper extends the possibility to examine the underlying curvature of data through the lens of topology by using the Betti curves, tools of Persistent Homology, as key topological descriptors, building on the clique topology approach. It was prev
Externí odkaz:
http://arxiv.org/abs/2406.15505
Autor:
Rinaldi, P., Navarro-Carrera, R., Caputi, K. I., Iani, E., Ostlin, G., Colina, L., Alberts, S., Alvarez-Marquez, J., Annunziatella, M., Boogaard, L., Costantin, L., Hjorth, J., Langeroodi, D., Melinder, J., Moutard, T., Walter, F.
We investigate the correlation between stellar mass (M*) and star formation rate (SFR) across the stellar mass range log10(M*/Msun)~6-11. We consider almost 50,000 star-forming galaxies at z~3-7, leveraging data from COSMOS/SMUVS, JADES/GOODS-SOUTH,
Externí odkaz:
http://arxiv.org/abs/2406.13554