Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Meriem Behiri"'
Autor:
Meriem Behiri, Marika Giulietti, Vincenzo Galluzzi, Andrea Lapi, Elisabetta Liuzzo, Marcella Massardi
Publikováno v:
Galaxies, Vol 12, Iss 2, p 14 (2024)
In this paper, we investigate the benefits of teaming up data from the radio to the far-infrared (FIR) regime for the characterization of dusty star-forming galaxies (DSFGs). These galaxies are thought to be the star-forming progenitors of local mass
Externí odkaz:
https://doaj.org/article/9b57b8181cb54f9f949eaec530ba105e
Publikováno v:
Galaxies, Vol 12, Iss 2, p 9 (2024)
Gravitational lensing, a compelling physical phenomenon, offers a unique avenue to investigate the morphology and physical properties of distant and faint celestial objects. This paper seeks to provide a comprehensive overview of the current state of
Externí odkaz:
https://doaj.org/article/cf3238ccbefb43a385ab5c7048d1779d
Autor:
Fabrizio Gentile, Margherita Talia, Meriem Behiri, Giovanni Zamorani, Luigi Barchiesi, Cristian Vignali, Francesca Pozzi, Matthieu Bethermin, Andrea Enia, Andreas L. Faisst, Marika Giulietti, Carlotta Gruppioni, Andrea Lapi, Marcella Massardi, Vernesa Smolčić, Mattia Vaccari, Andrea Cimatti
Publikováno v:
The Astrophysical Journal, Vol 962, Iss 1, p 26 (2024)
In the last decades, an increasing scientific interest has been growing in the elusive population of dark (i.e., lacking an optical/near-IR, hereafter NIR, counterpart) dusty star-forming galaxies (DSFGs). Although extremely promising for their likel
Externí odkaz:
https://doaj.org/article/45ea0afc8b224f4a81b66733930ca393
Autor:
Meriem Behiri, Margherita Talia, Andrea Cimatti, Andrea Lapi, Marcella Massardi, Andrea Enia, Cristian Vignali, Matthieu Bethermin, Andreas Faisst, Fabrizio Gentile, Marika Giulietti, Carlotta Gruppioni, Francesca Pozzi, Vernesa Smolçić, Gianni Zamorani
Publikováno v:
The Astrophysical Journal, Vol 957, Iss 2, p 63 (2023)
About 12 billion years ago, the Universe was first experiencing light again after the dark ages, and galaxies filled the environment with stars, metals, and dust. How efficient was this process? How fast did these primordial galaxies form stars and d
Externí odkaz:
https://doaj.org/article/88009a63ca4347569d8640b826b05c46
Autor:
Francesca Perrotta, Marika Giulietti, Marcella Massardi, Giovanni Gandolfi, Tommaso Ronconi, Maria Vittoria Zanchettin, Quirino D’ Amato, Meriem Behiri, Martina Torsello, Francesco Gabrielli, Lumen Boco, Vincenzo Galluzzi, Andrea Lapi
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 1, p 90 (2023)
We report Atacama Large Millimeter/submillimeter Array (ALMA) high-resolution (≲0.3″) observations of water emission lines p -H _2 O(2 _02 − 1 _11 ), o -H _2 O(3 _21 − 3 _12 ), p -H _2 O(4 _22 − 4 _13 ), in the strongly lensed galaxy HATLAS
Externí odkaz:
https://doaj.org/article/ddd79f7f90454eb9b49eabbf64cf6772
Autor:
Marika Giulietti, Andrea Lapi, Marcella Massardi, Meriem Behiri, Martina Torsello, Quirino D’Amato, Tommaso Ronconi, Francesca Perrotta, Alessandro Bressan
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 2, p 151 (2023)
We present high-resolution (≲0.″1) Atacama Large Millimeter/submillimeter Array observations of the strongly lensed galaxy HATLASJ113526.2-01460 at redshift z ∼ 3.1, discovered in the GAMA 12th field of the Herschel-ATLAS survey. This
Externí odkaz:
https://doaj.org/article/8c9cabc485ad4b9b97a69d3122b75ba7
Autor:
Marika Giulietti, Andrea Lapi, Marcella Massardi, Meriem Behiri, Martina Torsello, Quirino D’Amato, Tommaso Ronconi, Francesca Perrotta, Alessandro Bressan
We present high-resolution ($\lesssim0.1$arcsec) ALMA observations of the strongly-lensed galaxy HATLASJ113526.2-01460 at redshift $z\sim3.1$ discovered in the Gama 12$^{\rm th}$ field of the Herschel-ATLAS survey. The gravitationally lensed system i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b68420e976aad8ebac651e55c5740f5
Autor:
Andrea Enia, Margherita Talia, Francesca Pozzi, Andrea Cimatti, Ivan Delvecchio, Gianni Zamorani, Quirino D’Amato, Laura Bisigello, Carlotta Gruppioni, Giulia Rodighiero, Francesco Calura, Daniele Dallacasa, Marika Giulietti, Luigi Barchiesi, Meriem Behiri, Michael Romano
The Star Formation Rate Density (SFRD) history of the Universe is well constrained up to redshift $z \sim 2$. At earlier cosmic epochs, the picture has been largely inferred from UV-selected galaxies (e.g. Lyman-break galaxies, LBGs). However, LBGs'
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f094bf8f34654d450a251e6a6f1ab24e