Zobrazeno 1 - 10
of 35
pro vyhledávání: '"Michele Ginolfi"'
Publikováno v:
Water, Vol 16, Iss 10, p 1452 (2024)
Analytical solutions for turbulent and laminar water flow conditions are developed considering the drainage process of a simple tank reservoir, using the Darcy–Weisbach and the Poiseuille laws, respectively. Near the critical value of the Reynolds
Externí odkaz:
https://doaj.org/article/cdc0893c83664d559d5ad849d475988c
Autor:
Alessandro Bombini, Fernando García-Avello Bofías, Caterina Bracci, Michele Ginolfi, Chiara Ruberto
Publikováno v:
Machine Learning: Science and Technology, Vol 5, Iss 3, p 035024 (2024)
Extended vision techniques are ubiquitous in physics. However, the data cubes steaming from such analysis often pose a challenge in their interpretation, due to the intrinsic difficulty in discerning the relevant information from the spectra composin
Externí odkaz:
https://doaj.org/article/5298c855b8894350bd871091fe1f92ac
Autor:
Chiara Feruglio, Umberto Maio, Roberta Tripodi, Jan Martin Winters, Luca Zappacosta, Manuela Bischetti, Francesca Civano, Stefano Carniani, Valentina D’Odorico, Fabrizio Fiore, Simona Gallerani, Michele Ginolfi, Roberto Maiolino, Enrico Piconcelli, Rosa Valiante, Maria Vittoria Zanchettin
Publikováno v:
The Astrophysical Journal Letters, Vol 954, Iss 1, p L10 (2023)
We report the detection of CO(6–5) and CO(7–6) and their underlying continua from the host galaxy of quasar J100758.264+211529.207 (Pōniuā‘ena) at z = 7.5149, obtained with the NOrthern Extended Millimeter Array. Pōniuā‘ena belongs to the
Externí odkaz:
https://doaj.org/article/871a280c9b3f40f69bf6200060194ee0
Autor:
Roberta Tripodi, Chiara Feruglio, Francisca Kemper, Francesca Civano, Tiago Costa, Martin Elvis, Manuela Bischetti, Stefano Carniani, Fabio Di Mascia, Valentina D’Odorico, Fabrizio Fiore, Simona Gallerani, Michele Ginolfi, Roberto Maiolino, Enrico Piconcelli, Rosa Valiante, Luca Zappacosta
Publikováno v:
The Astrophysical Journal Letters, Vol 946, Iss 2, p L45 (2023)
We present ALMA Band 9 continuum observation of the ultraluminous quasi-stellar object (QSO) SDSS J0100+2802 providing a ∼10 σ detection at ∼670 GHz. SDSS J0100+2802 is the brightest QSO with the most massive supermassive black hole (SMBH) known
Externí odkaz:
https://doaj.org/article/8ca9edeff90141ee930962e8da6ff6df
Autor:
Andreas L. Faisst, Lin Yan, Matthieu Béthermin, Paolo Cassata, Miroslava Dessauges-Zavadsky, Yoshinobu Fudamoto, Michele Ginolfi, Carlotta Gruppioni, Gareth Jones, Yana Khusanova, Olivier LeFèvre, Francesca Pozzi, Michael Romano, John Silverman, Brittany Vanderhoof
Publikováno v:
Universe, Vol 8, Iss 6, p 314 (2022)
A multiwavelength study of galaxies is important to understand their formation and evolution. Only in the recent past, thanks to the Atacama Large (Sub) Millimeter Array (ALMA), were we able to study the far-infrared (IR) properties of galaxies at hi
Externí odkaz:
https://doaj.org/article/cab2d9272add4167836752a2f1dbb050
Autor:
Meghana Killi, Darach Watson, Seiji Fujimoto, Hollis Akins, Kirsten Knudsen, Johan Richard, Yuichi Harikane, Dimitra Rigopoulou, Francesca Rizzo, Michele Ginolfi, Gergö Popping, Vasily Kokorev
Publikováno v:
Killi, M, Watson, D, Fujimoto, S, Akins, H, Knudsen, K, Richard, J, Harikane, Y, Rigopoulou, D, Rizzo, F, Ginolfi, M, Popping, G & Kokorev, V 2023, ' A solar metallicity galaxy at z > 7? Possible detection of the [N II] 122 mu m and [O III] 52 mu m lines ', Monthly Notices of the Royal Astronomical Society, vol. 521, no. 2, pp. 2526-2534 . https://doi.org/10.1093/mnras/stad687
We present the first detection of the [N II] 122 $\mu$m and [O III] 52 $\mu$m lines for a reionisation-epoch galaxy. Based on these lines and previous [C II] 158 $\mu$m and [O III] 88 $\mu$m measurements, using two different radiative transfer models
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8dcecd69935dbc5deb97bcca0dc3e871
https://curis.ku.dk/ws/files/345315204/stad687.pdf
https://curis.ku.dk/ws/files/345315204/stad687.pdf
Autor:
Ivanna Langan, Johannes Zabl, Nicolas F Bouché, Michele Ginolfi, Gergö Popping, Ilane Schroetter, Martin Wendt, Joop Schaye, Leindert Boogaard, Jonathan Freundlich, Johan Richard, Jorryt Matthee, Wilfried Mercier, Thierry Contini, Yucheng Guo, Maxime Cherrey
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2023, 521, pp.546-557. ⟨10.1093/mnras/stad357⟩
Monthly Notices of the Royal Astronomical Society, 2023, 521, pp.546-557. ⟨10.1093/mnras/stad357⟩
We study the link between gas flow events and key galaxy scaling relations: the relations between star formation rate (SFR) and stellar mass (the main sequence, MS), gas metallicity and stellar mass (the mass-metallicity relation, MZR) and gas metall
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d9bcdee7fc7c53073021ba51af0b13e
https://insu.hal.science/insu-04038708
https://insu.hal.science/insu-04038708
Autor:
Luca Di Mascolo, Alexandro Saro, Tony Mroczkowski, Stefano Borgani, Eugene Churazov, Elena Rasia, Paolo Tozzi, Helmut Dannerbauer, Kaustuv Basu, Christopher L. Carilli, Michele Ginolfi, George Miley, Mario Nonino, Maurilio Pannella, Laura Pentericci, Francesca Rizzo
Galaxy clusters are the most massive gravitationally bound structures in the Universe, comprising thousands of galaxies and pervaded by a diffuse, hot ``intracluster medium'' (ICM) that dominates the baryonic content of these systems. The formation a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ca9819e550154794d45ba00551854d01
https://hdl.handle.net/11368/3044380
https://hdl.handle.net/11368/3044380
Autor:
Médéric Boquien, Véronique Buat, Denis Burgarella, Sandro Bardelli, Matthieu Béthermin, Andreas Faisst, Michele Ginolfi, Nimish Hathi, Gareth Jones, Anton Koekemoer, Brian Lemaux, Desika Narayanan, Michael Romano, Daniel Schaerer, Daniela Vergani, Giovanni Zamorani, Elena Zucca
Publikováno v:
Boquien, M, Buat, V, Burgarella, D, Bardelli, S, Bethermin, M, Faisst, A, Ginolfi, M, Hathi, N, Jones, G, Koekemoer, A, Lemaux, B, Narayanan, D, Romano, M, Schaerer, D, Vergani, D, Zamorani, G & Zucca, E 2022, ' The ALPINE-ALMA [C II] survey. Dust attenuation curves at z=4.4-5.5 ', Astronomy & Astrophysics, vol. 663, A50 . https://doi.org/10.1051/0004-6361/202142537
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142537⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142537⟩
There is now ample evidence that dust is already present in abundance at high z. However, given the faintness of distant galaxies in the optical and the NIR, datasets are still limited and how the dust affects the emerging radiation of galaxies at ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ca0eed26f31d8ac346f33f10f5fe99cf
Autor:
S. Bardelli, Paolo Cassata, G. C. Jones, Michele Ginolfi, Andreas L. Faisst, L. Morselli, Livia Vallini, Matthieu Béthermin, O. Le Fevre, D. Vergani, Y. Fudamoto, Miroslava Dessauges-Zavadsky, G. Rodighiero, E. Zucca, Edo Ibar, Margherita Talia, John D. Silverman, Dominik Riechers, Brian C. Lemaux, Peter Capak, Daniel Schaerer, Seiji Fujimoto, A. Enia, Médéric Boquien, Lin Yan, Andrea Cimatti, Chiara Mancini, L. Rodríguez-Muñoz, F. Loiacono, G. Zamorani, M. Romano, Nimish P. Hathi, Carlotta Gruppioni, Anton M. Koekemoer
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 496, pp.875-887. ⟨10.1093/mnras/staa1546⟩
Monthly Notices of the Royal Astronomical Society, 496(1), 875-887
Romano, M, Cassata, P, Morselli, L, Lemaux, B C, Bethermin, M, Capak, P, Faisst, A, Le Fevre, O, Schaerer, D, Silverman, J, Yan, L, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Enia, A, Fudamoto, Y, Fujimoto, S, Ginolfi, M, Gruppioni, C, Hathi, N P, Ibar, E, Jones, G C, Koekemoer, A M, Loiacono, F, Mancini, C, Riechers, D A, Rodighiero, G, Rodriguez-Munoz, L, Talia, M, Vallini, L, Vergani, D, Zamorani, G & Zucca, E 2020, ' The ALPINE ALMA [C II] Survey : on the nature of an extremely obscured serendipitous galaxy ', Monthly Notices of the Royal Astronomical Society, vol. 496, no. 1, pp. 875-887 . https://doi.org/10.1093/mnras/staa1546
Monthly Notices of the Royal Astronomical Society, 2020, 496, pp.875-887. ⟨10.1093/mnras/staa1546⟩
Monthly Notices of the Royal Astronomical Society, 496(1), 875-887
Romano, M, Cassata, P, Morselli, L, Lemaux, B C, Bethermin, M, Capak, P, Faisst, A, Le Fevre, O, Schaerer, D, Silverman, J, Yan, L, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Enia, A, Fudamoto, Y, Fujimoto, S, Ginolfi, M, Gruppioni, C, Hathi, N P, Ibar, E, Jones, G C, Koekemoer, A M, Loiacono, F, Mancini, C, Riechers, D A, Rodighiero, G, Rodriguez-Munoz, L, Talia, M, Vallini, L, Vergani, D, Zamorani, G & Zucca, E 2020, ' The ALPINE ALMA [C II] Survey : on the nature of an extremely obscured serendipitous galaxy ', Monthly Notices of the Royal Astronomical Society, vol. 496, no. 1, pp. 875-887 . https://doi.org/10.1093/mnras/staa1546
We report the serendipitous discovery of a bright galaxy (Gal-A) observed as part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). While this galaxy is detected both in line and continuum emission in ALMA Band 7, it is complete