Zobrazeno 1 - 10
of 18
pro vyhledávání: '"L K Morabito"'
Autor:
C L Hale, I H Whittam, M J Jarvis, P N Best, N L Thomas, I Heywood, M Prescott, N Adams, J Afonso, Fangxia An, R A A Bowler, J D Collier, R H W Cook, R Davé, B S Frank, M Glowacki, P W Hatfield, S Kolwa, C C Lovell, N Maddox, L Marchetti, L K Morabito, E Murphy, I Prandoni, Z Randriamanakoto, A R Taylor
Publikováno v:
Hale, C L, Whittam, I H, Jarvis, M J, Best, P N, Thomas, N L, Heywood, I, Prescott, M, Adams, N, Afonso, J, An, F, Bowler, R A A, Collier, J D, Cook, R H W, Davé, R, Frank, B S, Glowacki, M, Hatfield, P W, Kolwa, S, Lovell, C C, Maddox, N, Marchetti, L, Morabito, L K, Murphy, E, Prandoni, I, Randriamanakoto, Z & Taylor, A R 2023, ' MIGHTEE: deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei ', Monthly Notices of the Royal Astronomical Society, vol. 520, no. 2, pp. 2668-2691 . https://doi.org/10.1093/mnras/stac3320
Monthly Notices of the Royal Astronomical Society, 2023, Vol.520(2), pp.2668-2691 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 2023, Vol.520(2), pp.2668-2691 [Peer Reviewed Journal]
We present deep 1.4 GHz source counts from $\sim$5 deg$^2$ of the continuum Early Science data release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration (MIGHTEE) survey down to $S_{1.4\textrm{GHz}}\sim$15 $\mu$Jy. Using observa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b5eda3937d1c57c64cfe05ef106ef68a
https://www.pure.ed.ac.uk/ws/files/320364385/2211.05741v1.pdf
https://www.pure.ed.ac.uk/ws/files/320364385/2211.05741v1.pdf
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2022, Vol.513(1), pp.1254-1274 [Peer Reviewed Journal]
We have recently found fundamental differences in the radio properties of red quasars when compared to typical blue quasars. In this paper we use X-shooter data, providing spectral coverage from $\sim 3000-25000$ Ang, of a sample of 40 red and blue l
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2023, Vol.520(3), pp.4427-4442 [Peer Reviewed Journal]
Models of radio galaxy physics have been primarily based on high frequency ($\geqslant$1 GHz) observations of their jets, hotspots, and lobes. Without highly resolved low frequency observations, which provide information on older plasma, our understa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e09cc096c14fc5ab4beab0b168bd4c0
Autor:
P N Best, R Kondapally, W L Williams, R K Cochrane, K J Duncan, C L Hale, P Haskell, K Małek, I McCheyne, D J B Smith, L Wang, A Botteon, M Bonato, M Bondi, G Calistro Rivera, F Gao, G Gürkan, M J Hardcastle, M J Jarvis, B Mingo, H Miraghaei, L K Morabito, D Nisbet, I Prandoni, H J A Röttgering, J Sabater, T Shimwell, C Tasse, R van Weeren
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2023 [Peer Reviewed Journal]
Source classifications, stellar masses and star formation rates are presented for 80,000 radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey (LoTSS) Deep Fields, which represents the widest deep radio survey ever
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::075a5154caad53cbabfcacd80cf3d47c
Autor:
I H Whittam, M J Jarvis, C L Hale, M Prescott, L K Morabito, I Heywood, N J Adams, J Afonso, Fangxia An, Y Ao, R A A Bowler, J D Collier, R P Deane, J Delhaize, B Frank, M Glowacki, P W Hatfield, N Maddox, L Marchetti, A M Matthews, I Prandoni, S Randriamampandry, Z Randriamanakoto, D J B Smith, A R Taylor, N L Thomas, M Vaccari
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2022, Vol.516(1), pp.245-263 [Peer Reviewed Journal]
We study the nature of the faint radio source population detected in the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Early Science data in the COSMOS field, focusing on the properties of the radio-loud active galactic nuclei
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c2f8457e8ed66d71c20bab8b01022b7
http://dro.dur.ac.uk/36900/1/36900.pdf
http://dro.dur.ac.uk/36900/1/36900.pdf
Autor:
F. Sweijen, Y. Lyu, L. Wang, F. Gao, H. J. A. Röttgering, R. J. van Weeren, L. K. Morabito, P. N. Best, K. Małek, W. Williams, I. Prandoni, M. Bonato, M. Bondi
Publikováno v:
Astronomy & Astrophysics, 2023, Vol.671, pp.A85 [Peer Reviewed Journal]
Context. Hyper-luminous infrared galaxies (HLIRGs) are among the most extreme systems in the Universe. With infrared (IR) luminosities of LIR > 1013 L⊙ they can have IR-derived star formation rates (SFRs) exceeding 103 M⊙ yr−1. Theoretical mode
Autor:
C. Groeneveld, R. J. van Weeren, G. K. Miley, L. K. Morabito, F. de Gasperin, J. R. Callingham, F. Sweijen, M. Brüggen, A. Botteon, A. Offringa, G. Brunetti, J. Moldon, M. Bondi, A. Kappes, H. J. A. Röttgering
Publikováno v:
Astronomy & Astrophysics, 658. EDP Sciences
Astronomy and astrophysics, 658:A9. EDP Sciences
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & astrophysics, 2022, Vol.658, pp.A9 [Peer Reviewed Journal]
Astronomy and astrophysics, 658:A9. EDP Sciences
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & astrophysics, 2022, Vol.658, pp.A9 [Peer Reviewed Journal]
Relatively little information is available about the Universe at ultra-low radio frequencies (ULF; i.e., below 50 MHz), although the ULF spectral window contains a wealth of unique diagnostics for studying galactic and extragalactic phenomena. Subarc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::484fbbeab22753109e64c825ef99ff8f
https://hdl.handle.net/1887/3281000
https://hdl.handle.net/1887/3281000
Autor:
F. Sweijen, R. J. van Weeren, H. J. A. Röttgering, L. K. Morabito, N. Jackson, A. R. Offringa, S. van der Tol, B. Veenboer, J. B. R. Oonk, P. N. Best, M. Bondi, T. W. Shimwell, C. Tasse, A. P. Thomson
Publikováno v:
Sweijen, F, van Weeren, R J, Rottgering, H J A, Morabito, L K, Jackson, N, Offringa, A R, van der Tol, S, Veenboer, B, Oonk, J B R, Best, P, Bondi, M, Shimwell, T W, Tasse, C & Thomson, A P 2022, ' Deep sub-arcsecond wide-field imaging of the Lockman Hole field at 144 MHz ', Nature Astronomy, vol. 6, no. 3, pp. 350-356 . https://doi.org/10.1038/s41550-021-01573-z
Nature astronomy, 2022, Vol.6(3), pp.350-356 [Peer Reviewed Journal]
Nature Astronomy, 6, 350-356
Nature astronomy, 2022, Vol.6(3), pp.350-356 [Peer Reviewed Journal]
Nature Astronomy, 6, 350-356
High quality low-frequency radio surveys have the promise of advancing our understanding of many important topics in astrophysics, including the life cycle of active galactic nuclei (AGN), particle acceleration processes in jets, the history of star
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::074ae4ac2e657ba0b8d3a6f7006497e5
Autor:
R. Timmerman, R. J. van Weeren, J. R. Callingham, W. D. Cotton, R. Perley, L. K. Morabito, N. A. B. Gizani, A. H. Bridle, C. P. O’Dea, S. A. Baum, G. R. Tremblay, P. Kharb, N. E. Kassim, H. J. A. Röttgering, A. Botteon, F. Sweijen, C. Tasse, M. Brüggen, J. Moldon, T. Shimwell, G. Brunetti
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & astrophysics, 2022, Vol.658, pp.A5 [Peer Reviewed Journal]
Astronomy & Astrophysics, 658:A5
instname
Astronomy & astrophysics, 2022, Vol.658, pp.A5 [Peer Reviewed Journal]
Astronomy & Astrophysics, 658:A5
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8c17e2a28b0d24ab7ce46f014d69e09b
https://hdl.handle.net/1887/3515630
https://hdl.handle.net/1887/3515630
Autor:
A. Kappes, P. R. Burd, M. Kadler, G. Ghisellini, E. Bonnassieux, M. Perucho, M. Brüggen, C. C. Cheung, B. Ciardi, E. Gallo, F. Haardt, L. K. Morabito, T. Sbarrato, A. Drabent, J. Harwood, N. Jackson, J. Moldon
Publikováno v:
Astronomy & Astrophysics. 663:A44
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid