Zobrazeno 1 - 10
of 25
pro vyhledávání: '"L. Ceraj"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Vibor Jelić, Saleem Zaroubi, Cameron Van Eck, Rutger Jaspers, Andrea Bracco, Marijke Haverkorn, Luka Turić, Ana Erceg, L. Ceraj
Publikováno v:
Astronomy & Astrophysics
Astronomy and astrophysics, 654:A5. EDP Sciences
Astronomy & Astrophysics, 654, pp. 1-13
Astronomy & Astrophysics, 654, 1-13
Astronomy and astrophysics, 654:A5. EDP Sciences
Astronomy & Astrophysics, 654, pp. 1-13
Astronomy & Astrophysics, 654, 1-13
Faraday tomography of a field centred on the extragalactic point source 3C 196 with the LOw Frequency ARray (LOFAR) revealed an intertwined structure of diffuse polarised emission with straight depolarisation canals and tracers of the magnetized and
Autor:
I. Delvecchio, E. Daddi, M. T. Sargent, J. Aird, J. R. Mullaney, B. Magnelli, D. Elbaz, L. Bisigello, L. Ceraj, S. Jin, B. S. Kalita, D. Liu, M. Novak, I. Prandoni, J. F. Radcliffe, C. Spingola, G. Zamorani, V. Allevato, G. Rodighiero, V. Smolčić
Publikováno v:
Delvecchio, I, Daddi, E, Sargent, M T, Aird, J, Mullaney, J R, Magnelli, B, Elbaz, D, Bisigello, L, Ceraj, L, Jin, S, Kalita, B S, Liu, D, Novak, M, Prandoni, I, Radcliffe, J F, Spingola, C, Zamorani, G, Allevato, V, Rodighiero, G & Smolčić, V 2022, ' A super-linear 'radio-AGN main sequence' links mean radio-AGN power and galaxy stellar mass since z ~ 3 ', Astronomy and Astrophysics, vol. 668, A81 . https://doi.org/10.1051/0004-6361/202244639
Delvecchio, I, Daddi, E, Sargent, M T, Aird, J, Mullaney, J R, Magnelli, B, Elbaz, D, Bisigello, L, Ceraj, L, Jin, S, Kalita, B S, Liu, D, Novak, M, Prandoni, I, Radcliffe, J F, Spingola, C, Zamorani, G, Allevato, V, Rodighiero, G & Smolcic, V 2022, ' A super-linear ‘radio-AGN main sequence’ links mean radio-AGN power and galaxy stellar mass since z ∼ 3 ', Astronomy and Astrophysics, vol. 668, A81, pp. 1-27 . https://doi.org/10.1051/0004-6361/202244639
Delvecchio, I, Daddi, E, Sargent, M T, Aird, J, Mullaney, J R, Magnelli, B, Elbaz, D, Bisigello, L, Ceraj, L, Jin, S, Kalita, B S, Liu, D, Novak, M, Prandoni, I, Radcliffe, J F, Spingola, C, Zamorani, G, Allevato, V, Rodighiero, G & Smolcic, V 2022, ' A super-linear ‘radio-AGN main sequence’ links mean radio-AGN power and galaxy stellar mass since z ∼ 3 ', Astronomy and Astrophysics, vol. 668, A81, pp. 1-27 . https://doi.org/10.1051/0004-6361/202244639
Mapping the average AGN luminosity across galaxy populations and over time encapsulates important clues on the interplay between supermassive black hole (SMBH) and galaxy growth. This paper presents the demography, mean power and cosmic evolution of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c5742a11d77b97a3f70c85e72ab91c11
Autor:
Sarah K. Leslie, J. Delhaize, Stefano Marchesi, Vernesa Smolčić, A. Butler, Jeyhan S. Kartaltepe, Manolis Plionis, Konstantinos Kolokythas, Eleni Vardoulaki, L. Ceraj, Marguerite Pierre, K. Tisanić, Mladen Novak, Cathy Horellou, Ivan Delvecchio, G. Zamorani
Publikováno v:
Astronomy and Astrophysics
Volume 642
Volume 642
We studied a sample of 274 radio and X-ray selected quasars (XQSOs) detected in the COSMOS and XXL-S radio surveys at 3 GHz and 2.1 GHz, respectively. This sample was identified by adopting a conservative threshold in X-ray luminosity, Lx [2-10\ keV]
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b72f4d901c8155299079414ff46b5f89
https://repozitorij.pmf.unizg.hr/islandora/object/pmf:9070
https://repozitorij.pmf.unizg.hr/islandora/object/pmf:9070
Autor:
Konstantinos Kolokythas, M. N. Bremer, K. Tisanić, Mark Birkinshaw, Cathy Horellou, Bruno Šlaus, H. J. A. Röttgering, Paolo Ciliegi, L. Ceraj, Mladen Novak, M. Huynh, Sotiria Fotopoulou, L. Chiappetti, Marguerite Pierre, Somak Raychaudhury, Hubertus Intema, Vernesa Smolčić, N. Jurlin
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A46. ⟨10.1051/0004-6361/201937258⟩
Astronomy and astrophysics, 638:A46. EDP Sciences
Astronomy and Astrophysics
Volume 638
Astronomy and Astrophysics-A&A, 2020, 638, pp.A46. ⟨10.1051/0004-6361/201937258⟩
Astronomy & Astrophysics, 638, A46
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A46. ⟨10.1051/0004-6361/201937258⟩
Astronomy and astrophysics, 638:A46. EDP Sciences
Astronomy and Astrophysics
Volume 638
Astronomy and Astrophysics-A&A, 2020, 638, pp.A46. ⟨10.1051/0004-6361/201937258⟩
Astronomy & Astrophysics, 638, A46
We study the space density evolution of active galactic nuclei (AGN) using the 610 MHz radio survey of the XXL-North field, performed with the Giant Metrewave Radio Telescope. The survey covers an area of 30.4 deg2, with a beamsize of 6.5 arcsec. The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b228e5bc7676e310a7490f807fc01607
https://hal-cea.archives-ouvertes.fr/cea-02863069/file/aa37258-19.pdf
https://hal-cea.archives-ouvertes.fr/cea-02863069/file/aa37258-19.pdf
Autor:
Emilio Romano-Diaz, K. Tisanić, Kevin Harrington, Alexis Finoguenov, G. Zamorani, Ivan Delvecchio, T. Badescu, Benjamin Magnelli, M. Bondi, Alexander Karim, Ghassem Gozaliasl, Frank Bertoldi, L. Ceraj, E. F. Jiménez Andrade, Eva Schinnerer, Vernesa Smolčić, Mark Sargent, Sarah K. Leslie, Eleni Vardoulaki
Publikováno v:
Astronomy & Astrophysics. 648:A102
($ABRIDGED$) We probe the physical properties and large-scale environment of radio AGN in the faintest FR population to-date, and link them to their radio structure. We use the VLA-COSMOS Large Project at 3 GHz, with resolution and sensitivity of 0".
Autor:
K. Tisanić, L. Ceraj, M. Imbrišak, M. Bondi, Vernesa Smolčić, G. Zamorani, J. Delhaize, Eleni Vardoulaki
Publikováno v:
Astronomy and Astrophysics
Volume 643
Volume 643
As the SKA is expected to be operational in the next decade, investigations of the radio sky in the range of 100 MHz to 10 GHz have become important for simulations of the SKA observations. In determining physical properties of galaxies from radio da
Autor:
J. Delhaize, Vernesa Smolčić, Eleni Vardoulaki, Eva Schinnerer, Mladen Novak, L. Ceraj, N. Herrera Ruiz, G. Zamorani, Ivan Delvecchio
Publikováno v:
Astronomy and Astrophysics
Volume 620
Volume 620
We study a sample of 1,604 moderate-to-high radiative luminosity active galactic nuclei (HLAGN) selected at 3 GHz within the VLA-COSMOS 3 GHz Large Project. These were classified by combining multiple AGN diagnostics: X-ray data, mid-infrared data an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::016e7f49097d97f3b6f5f4b1c9acc7fb
https://repozitorij.pmf.unizg.hr/islandora/object/pmf:8151
https://repozitorij.pmf.unizg.hr/islandora/object/pmf:8151
We study the moderate-to-high radiative luminosity active galactic nuclei (HLAGN) within the VLA-COSMOS 3 GHz Large Project. The survey covers 2.6 square degrees centered on the COSMOS field with a 1$\sigma$ sensitivity of 2.3 $\mathrm{\mu Jy}$/beam
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::873cdfd2a512b690ae6c090cab9119c3
http://arxiv.org/abs/1712.09838
http://arxiv.org/abs/1712.09838