Zobrazeno 1 - 10
of 17 168
pro vyhledávání: '"Romano , M."'
Autor:
Sawant, P., Nanni, A., Romano, M., Donevski, D., Bruzual, G., Ysard, N., Lemaux, B. C., Inami, H., Calura, F., Pozzi, F., Małek, K., Junais, Boquien, M., Faisst, A. L., Hamed, M., Ginolfi, M., Zamorani, G., Lorenzon, G., Molina, J., Bardelli, S., Ibar, E., Vergani, D., Di Cesare, C., Béthermin, M., Burgarella, D., Cassata, P., Dessauges-Zavadsky, M., D'Onghia, E., Dubois, Y., Magdis, G. E., Mendez-Hernandez, H.
Recent observations reveal a rapid dust build-up in high-redshift galaxies (z > 4), challenging current models of galaxy formation. While our understanding of dust production and destruction in the interstellar medium (ISM) is advancing, probing bary
Externí odkaz:
http://arxiv.org/abs/2412.02505
Autor:
Veraldi, E., Vallini, L., Pozzi, F., Esposito, F., Bethermin, M., Boquien, M., Faisst, A., Ginolfi, M., Gobat, R., Gruppioni, C., Hathi, N., Ibar, E., Molina, J., Rizzo, F., Romano, M., Zamorani, G.
In this work, we devise a model for estimating UV and optical line emission (i.e., CIII] $1909$A, H$\beta$, [OIII] $5007$A, H$\alpha$, [NII] $6583$A) tracing HII regions in the interstellar medium (ISM) of galaxies at $z\sim4-6$ from the ALMA Large P
Externí odkaz:
http://arxiv.org/abs/2411.08124
Autor:
Solimano, M., González-López, J., Aravena, M., Pampliega, B. Alcalde, Assef, R. J., Béthermin, M., Boquien, M., Bovino, S., Casey, C. M., Cassata, P., da Cunha, E., Davies, R. L., De Looze, I., Ding, X., Díaz-Santos, T., Faisst, A. L., Ferrara, A., Fisher, D. B., Förster-Schreiber, N. M., Fujimoto, S., Ginolfi, M., Gruppioni, C., Guaita, L., Hathi, N., Herrera-Camus, R., Ibar, E., Inami, H., Jones, G. C., Koekemoer, A. M., Lee, L., Li, J., Liu, D., Liu, Z., Molina, J., Ogle, P., Posses, A. C., Pozzi, F., Relaño, M., Riechers, D. A., Romano, M., Spilker, J., Sulzenauer, N., Telikova, K., Vallini, L., Vasan, K. G. C., Veilleux, S., Vergani, D., Villanueva, V., Wang, W., Yan, L., Zamorani, G.
Galaxy protoclusters are sites of rapid growth, with a high density of massive galaxies driving elevated rates of star formation and accretion onto supermassive black holes. Here, we present new JWST/NIRSpec IFU observations of the J1000+0234 group a
Externí odkaz:
http://arxiv.org/abs/2407.13020
Autor:
Lorenzon, G., Donevski, D., Lisiecki, K., Lovell, C., Romano, M., Narayanan, D., Davé, R., Man, A., Whitaker, K. E., Nanni, A., Long, A., Lee, M. M., Junais, Małek, K., Rodighiero, G., Li, Q.
Recent discoveries of copious amounts of dust in quiescent galaxies (QGs) at high redshifts ($z\gtrsim 1-2$) challenge the conventional view that these objects have poor interstellar medium (ISM) in proportion to their stellar mass. We use the SIMBA
Externí odkaz:
http://arxiv.org/abs/2404.10568
Autor:
Pearson, W. J., Santos, D. J. D., Goto, T., Huang, T. -C., Kim, S. J., Matsuhara, H., Pollo, A., Ho, S. C. -C., Hwang, H. S., Małek, K., Nakagawa, T., Romano, M., Serjeant, S., Suelves, L., Shim, H., White, G. J.
Publikováno v:
A&A 686, A94 (2024)
Aims. In this work, we intend to examine how environment influences the merger fraction, from the low density field environment to higher density groups and clusters. We also aim to study how the properties of a group or cluster, as well as the posit
Externí odkaz:
http://arxiv.org/abs/2403.11615
Autor:
Quaglia, L., Abbrescia, M., Aielli, G., Aly, R., Arena, M. C., Barroso, M., Benussi, L., Bianco, S., Boscherini, D., Bordon, F., Bruni, A., Buontempo, S., Busato, M., Camarri, P., Cardarelli, R., Congedo, L., Damiao, D. De Jesus, De Serio, M., Di Ciaccio, A., Di Stante, L., Dupieux, P., Eysermans, J., Ferretti, A., Galati, G., Gagliardi, M., Guida, R., Iaselli, G., Joly, B., Juks, S. A., Lee, K. S., Liberti, B., Ramirez, D. Lucero, Mandelli, B., Manen, S. P., Massa, L., Pastore, A., Pastori, E., Piccolo, D., Pizzimento, L., Polini, A., Proto, G., Pugliese, G., Ramos, D., Rigoletti, G., Rocchi, A., Romano, M., Samalan, A., Salvini, P., Santonico, R., Saviano, G., Sessa, M., Simone, S., Terlizzi, L., Tytgat, M., Vercellin, E., Verzeroli, M., Zaganidis, N.
ALICE (A Large Ion Collider Experiment) studies the Quark-Gluon Plasma (QGP): a deconfined state of matter obtained in ultra-relativistic heavy-ion collisions. One of the probes for QGP study are quarkonia and open heavy flavour, of which ALICE explo
Externí odkaz:
http://arxiv.org/abs/2402.19408
Autor:
collaboration, The RPC ECOGas@GIF, Quaglia, L., Abbrescia, M., Aielli, G., Aly, R., Arena, M. C., Barroso, M., Benussi, L., Bianco, S., Boscherini, D., Bordon, F., Bruni, A., Buontempo, S., Busato, M., Camarri, P., Cardarelli, R., Congedo, L., Damiao, D. De Jesus, De Serio, M., Di Ciaccio, A., Di Stante, L., Dupieux, P., Eysermans, J., Ferretti, A., Galati, G., Gagliardi, M., Garetti, S., Guida, R., Iaselli, G., Joly, B., Juks, S. A., Lee, K. S., Liberti, B., Ramirez, D. Lucero, Mandelli, B., Manen, S. P., Massa, L., Pastore, A., Pastori, E., Piccolo, D., Pizzimento, L., Polini, A., Proto, G., Pugliese, G., Ramos, D., Rigoletti, G., Rocchi, A., Romano, M., Samalan, A., Salvini, P., Santonico, R., Saviano, G., Sessa, M., Simone, S., Terlizzi, L., Tytgat, M., Vercellin, E., Verzeroli, M., Zaganidis, N.
Resistive Plate Chambers (RPCs) are gaseous detectors widely used in high energy physics experiments, operating with a gas mixture primarily containing Tetrafluoroethane (C$_{2}$H$_{2}$F$_{4}$), commonly known as R-134a, which has a global warming po
Externí odkaz:
http://arxiv.org/abs/2402.19395
Autor:
Romano, M., Donevski, D., Junais, Nanni, A., Ginolfi, M., Jones, G. C., Shivaei, I., Lorenzon, G., Hamed, M., Salak, D., Sawant, P.
Publikováno v:
A&A 683, L9 (2024)
The evolution of dwarf galaxies is dramatically affected by gaseous and dusty outflows, which can easily deprive their interstellar medium of the material needed for the formation of new stars, simultaneously enriching their surrounding circumgalacti
Externí odkaz:
http://arxiv.org/abs/2402.17662
Autor:
Małek, K., Junais, Pollo, A., Boquien, M., Buat, V., Salim, S., Brough, S., Demarco, R., Graham, A. W., Hamed, M., Mullaney, J. R., Romano, M., Sifón, C., Aravena, M., Benavides, J. A., Busà, I., Donevski, D., Dorey, O., Hernandez-Toledo, H. M., Nanni, A., Pearson, W. J., Pistis, F., Ragusa, R., Riccio, G., Román, J.
Large future sky surveys, such as the LSST, will provide optical photometry for billions of objects. This paper aims to construct a proxy for the far ultraviolet attenuation (AFUVp) from the optical data alone, enabling the rapid estimation of the st
Externí odkaz:
http://arxiv.org/abs/2401.12831
Publikováno v:
A&A 690, A255 (2024)
Galaxies evolve through a dynamic exchange of material with their immediate surrounding environment, the so-called circumgalactic medium (CGM). Understanding the physics of gas flows and the nature of the CGM is thus fundamental to studying galaxy ev
Externí odkaz:
http://arxiv.org/abs/2401.03020