Zobrazeno 1 - 10
of 10 298
pro vyhledávání: '"Pugliese, G."'
Autor:
Pugliese, G., Saccardi, A., Elia, V. D, Vergani, S. D., Heintz, K. E., Savaglio, S., Kaper, L., Postigo, A. de Ugarte, Hartmann, D. H., De Cia, A., Vejlgaard, S., Fynbo, J. P. U., Christensen, L., Campana, S., van Rest, D., Selsing, J., Wiersema, K., Malesani, D. B., Covino, S., Burgarella, D., De Pasquale, M., Jakobsson, P., Japelj, J., Kann, D. A., Kouveliotou, C., Rossi, A., Tanvir, N. R., Thoene, C. C., Xu, D.
Publikováno v:
A&A 690, A35 (2024)
Gamma-ray bursts are the most energetic known explosions. Despite fading rapidly, they allow to measure redshift and important properties of their host-galaxies. We report the photometric and spectroscopic study of GRB 160203A and its host-galaxy. Fi
Externí odkaz:
http://arxiv.org/abs/2406.18754
Autor:
Thöne, C. C., Postigo, A. de Ugarte, Izzo, L., Michalowski, M. J., Levan, A. J., Leung, J. K., Fernández, J. F. Agüí, Géron, T., Friesen, R., Christensen, L., Covino, S., D'Elia, V., Hartmann, D. H., Jakobsson, P., De Pasquale, M., Pugliese, G., Rossi, A., Schady, P., Wiersema, K., Zafar, T.
Long GRB hosts at z<1 are usually low-mass, low metallicity star-forming galaxies. Here we present the until now most detailed, spatially resolved study of the host of GRB 171205A, a grand-design barred spiral galaxy at z=0.036. Our analysis includes
Externí odkaz:
http://arxiv.org/abs/2406.16725
Autor:
Fausey, H. M., Vejlgaard, S., van der Horst, A. J., Heintz, K. E., Izzo, L., Malesani, D. B., Wiersema, K., Fynbo, J. P. U., Tanvir, N. R., Vergani, S. D., Saccardi, A., Rossi, A., Campana, S., Covino, S., D'Elia, V., De Pasquale, M., Hartmann, D., Jakobsson, P., Kouveliotou, C., Levan, A., Martin-Carrillo, A., Melandri, A., Palmerio, J., Pugliese, G., Salvaterra, R.
The Epoch of Reionization (EoR) is a key period of cosmological history in which the intergalactic medium (IGM) underwent a major phase change from being neutral to almost completely ionized. Gamma-ray bursts (GRBs) are luminous and unique probes of
Externí odkaz:
http://arxiv.org/abs/2403.13126
Autor:
Fernández, J. F. Agüí, Postigo, A. de Ugarte, Thöne, C. C., Kobayashi, S., Rossi, A., Toma, K., Jelínek, M., Kann, D. A., Covino, S., Wiersema, K., Hartmann, D., Jakobsson, P., Martin-Carrillo, A., Melandri, A., De Pasquale, M., Pugliese, G., Savaglio, S., Starling, R. L. C., Štrobl, J., Della Valle, M., de Wet, S., Zafar, T.
Long gamma ray bursts (GRBs) are produced by the collapse of some very massive stars, which emit ultra-relativistic jets. When the jets collide with the interstellar medium they decelerate and generate the so-called afterglow emission, which has been
Externí odkaz:
http://arxiv.org/abs/2403.02312
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:
Rastinejad, J. C., Fong, W., Levan, A. J., Tanvir, N. R., Kilpatrick, C. D., Fruchter, A. S., Anand, S., Bhirombhakdi, K., Covino, S., Fynbo, J. P. U., Halevi, G., Hartmann, D. H., Heintz, K. E., Izzo, L., Jakobsson, P., Lamb, G. P., Malesani, D. B., Melandri, A., Metzger, B. D., Milvang-Jensen, B., Pian, E., Pugliese, G., Rossi, A., Siegel, D. M., Singh, P., Stratta, G.
The existence of a secondary (in addition to compact object mergers) source of heavy element ($r$-process) nucleosynthesis, the core-collapse of rapidly-rotating and highly-magnetized massive stars, has been suggested by both simulations and indirect
Externí odkaz:
http://arxiv.org/abs/2312.04630
Autor:
Abbrescia, M., Aielli, G., Aly, R., Arena, M. C., Barroso, M., Benussi, L., Bianco, S., Bordon, F., Boscherini, D., 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., 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., Quaglia, L., Ramos, D., Rigoletti, G., Rocchi, A., Romano, M., Samalan, A., Salvini, P., Santonico, R., Saviano, G., Simone, S., Terlizzi, L., Tytgat, M., Vercellin, E., Verzeroli, M., Zaganidis, N.
Results obtained by the RPC ECOgas@GIF++ Collaboration, using Resistive Plate Chambers operated with new, eco-friendly gas mixtures, based on Tetrafluoropropene and carbon dioxide, are shown and discussed in this paper. Tests aimed to assess the perf
Externí odkaz:
http://arxiv.org/abs/2311.08259
Autor:
Schady, P., Yates, R. M., Christensen, L., De Cia, A., Rossi, A., D'Elia, V., Heintz, K. E., Jakobsson, P., Laskar, T., Levan, A., Salvaterra, R., Starling, R. L. C., Tanvir, N. R, Thöne, C. C., Vergani, S., Wiersema, K., Arabsalmani, M ., Chen, H. -W., De Pasquale, M., Fruchter, A., Fynbo, J. P. U., García-Benito, R., Gompertz, B., Hartmann, D., Kouveliotou, C., Milvang-Jensen, B., Palazzi, E., Perley, D., Piranomonte, S., Pugliese, G., Savaglio, S., Sbarufatti, B., Schulze, S., Tagliaferri, G., Postigo, A. de Ugarte, Watson, D., Wiseman, P.
Much of what is known of the chemical composition of the universe is based on emission line spectra from star forming galaxies. Emission-based inferences are, nevertheless, model-dependent and they are dominated by light from luminous star forming re
Externí odkaz:
http://arxiv.org/abs/2310.15967
Autor:
Ferro, M., Brivio, R., D'Avanzo, P., Rossi, A., Izzo, L., Campana, S., Christensen, L., Dinatolo, M., Hussein, S., Levan, A. J., Melandri, A., Bernardini, M. G., Covino, S., D'Elia, V., Della Valle, M., De Pasquale, M., Gompertz, B. P., Hartmann, D., Heintz, K. E., Jakobsson, P., Kouveliotou, C., Malesani, D. B., Martin-Carrillo, A., Nava, L., Guelbenzu, A. Nicuesa, Pugliese, G., Salvaggio, C., Salvaterra, R., Savaglio, S., Sbarrato, T., Tanvir, N. R., Wijers, R. A. M. J., Zafar, T.
Publikováno v:
A&A 678, A142 (2023)
Context: GRB 211106A and GRB 211227A are recent gamma-ray bursts (GRBs) with initial X-ray positions suggesting associations with nearby galaxies (z < 0.7). Their prompt emission characteristics indicate GRB 211106A is a short-duration GRB and GRB 21
Externí odkaz:
http://arxiv.org/abs/2309.03000