Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Duncan, K. J."'
Autor:
Gloudemans, A. J., Duncan, K. J., R��ttgering, H. J. A., Shimwell, T. W., Venemans, B. P., Best, P. N., Br��ggen, M., Rivera, G. Calistro, Drabent, A., Hardcastle, M. J., Miley, G. K., Schwarz, D. J., Saxena, A., Smith, D. J. B., Williams, W. L.
Optically luminous quasars at $z > 5$ are important probes of super-massive black hole (SMBH) formation. With new and future radio facilities, the discovery of the brightest low-frequency radio sources in this epoch would be an important new probe of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4a0c19efe8f31da8081f325996cdd03f
Autor:
Kondapally, R., Best, P. N., Hardcastle, M. J., Nisbet, D., Bonato, M., Sabater, J., Duncan, K. J., McCheyne, I., Cochrane, R. K., Bowler, R. A. A., Williams, W. L., Shimwell, T. W., Tasse, C., Croston, J. H., Goyal, A., Jamrozy, M., Jarvis, M. J., Mahatma, V. H., Röttgering, H. J. A., Smith, D. J. B., Wołowska, A., Bondi, M., Brienza, M., Brown, M. J. I., Brüggen, M., Chambers, K., Garrett, M. A., Gürkan, G., Huber, M., Kunert-Bajraszewska, M., Magnier, E., Mingo, B., Mostert, R., Nikiel-Wroczyński, B., O’Sullivan, S. P., Paladino, R., Ploeckinger, T., Prandoni, I., Rosenthal, M. J., Schwarz, D. J., Shulevski, A., Wagenveld, J. D., Wang, L.
We present the source associations, cross-identifications, and multi-wavelength properties of the faint radio source population detected in the deep tier of the LOFAR Two Metre Sky Survey (LoTSS): the LoTSS Deep Fields. The first LoTSS Deep Fields da
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::288ebf60a79c0c566ce95d76253b1608
http://oro.open.ac.uk/76117/1/aa38813-20.pdf
http://oro.open.ac.uk/76117/1/aa38813-20.pdf
Autor:
Hardcastle, M. J., Williams, W. L., Best, P. N., Croston, J. H., Duncan, K. J., Rottgering, H. J. A., Sabater, J., Shimwell, T. W., Tasse, C., Callingham, J. R., Cochrane, R. K., Gasperin, F. de, Gurkan, G., Jarvis, M. J., Mahatma, V., Miley, G. K., Mingo, B., Mooney, S., Morabito, L. K., O'Sullivan, S. P., Prandoni, I., Shulevski, A., Smith, D. J. B.
Publikováno v:
Hardcastle, M J, Williams, W L, Best, P N, Croston, J H, Duncan, K J, Rottgering, H J A, Sabater, J, Shimwell, T W, Tasse, C, Callingham, J R, Cochrane, R K, Gasperin, F D, Gurkan, G, Jarvis, M J, Mahatma, V, Miley, G K, Mingo, B, Mooney, S, Morabito, L K, O'Sullivan, S P, Prandoni, I, Shulevski, A & Smith, D J B 2019, ' Radio-loud AGN in the first LoTSS data release : The lifetimes and environmental impact of jet-driven sources ', Astronomy & Astrophysics . < https://www.aanda.org/component/solr/?task=results#!q=Radio-loud%20AGN%20in%20the%20first%20LoTSS%20data%20release%20The%20lifetimes%20and%20environmental%20impact%20of%20jet-driven%20sources&sort=relevance&rows=10 >
We constructed a sample of 23,344 radio-loud active galactic nuclei (RLAGN) from the catalogue derived from the LOFAR Two-Metre Sky Survey (LoTSS) survey of the HETDEX Spring field. Although separating AGN from star-forming galaxies remains challengi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3094::ee1b683f1a9f6f82a499b02ddffad122
https://www.pure.ed.ac.uk/ws/files/77278555/1811.07943.pdf
https://www.pure.ed.ac.uk/ws/files/77278555/1811.07943.pdf
Autor:
Williams, W. L., Rivera, G. Calistro, Best, P. N., Hardcastle, M. J., R��ttgering, H. J. A., Duncan, K. J., de Gasperin, F., Jarvis, M. J., Miley, G. K., Mahony, E. K., Morabito, L. K., Nisbet, D. M., Prandoni, I., Smith, D. J. B., Tasse, C., White, G. J.
This paper presents a study of the redshift evolution of radio-loud active galactic nuclei (AGN) as a function of the properties of their galaxy hosts in the Bo��tes field. To achieve this we match low-frequency radio sources from deep $150$-MHz
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b92ce7d6a2ec84eb9effc27ea6ebb677
Autor:
Daniel Smith, Best, P. N., Duncan, K. J., Hatch, N. A., Jarvis, M. J., Röttgering, H. J. A., Simpson, C. J., Stott, J. P., Cochrane, R. K., Coppin, K. E., Dannerbauer, H., Davis, T. A., Geach, J. E., Hale, C. L., Hardcastle, M. J., Hatfield, P. W., Houghton, R. C. W., Maddox, N., Mcgee, S. L., Morabito, L., Nisbet, D., Pandey-Pommier, M., Prandoni, I., Saxena, A., Shimwell, T. W., Tarr, M., Bemmel, I., Verma, A., White, G. J., Williams, W. L.
Publikováno v:
Journées de la SF2A
Lancaster EPrints
CORE
arXiv.org e-Print Archive
NASA Astrophysics Data System
Lancaster University-Pure
Lancaster EPrints
CORE
arXiv.org e-Print Archive
NASA Astrophysics Data System
Lancaster University-Pure
In these proceedings we highlight the primary scientific goals and design of the WEAVE-LOFAR survey, which will use the new WEAVE spectrograph on the 4.2m William Herschel Telescope to provide the primary source of spectroscopic information for the L
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::72435dc8637d78a1e508ed4984cec117
http://arxiv.org/abs/1611.02706
http://arxiv.org/abs/1611.02706
Autor:
K. C. Chambers, T. Ploeckinger, M. E. Huber, Rachel Cochrane, L. Wang, M. J. Rosenthal, Isabella Prandoni, A. Wo łowska, R. Kondapally, Rosita Paladino, B. Nikiel-Wroczy ński, Philip Best, H. J. A. R öttgering, Timothy W. Shimwell, Martin J. Hardcastle, E. A. Magnier, A. Shulevski, Kenneth Duncan, J. Sabater, V. H. Mahatma, Dominik J. Schwarz, J. H. Croston, Daniel J. Smith, Magdalena Kunert-Bajraszewska, I. McCheyne, D. Nisbet, R. I. J. Mostert, J. D. Wagenveld, Michael J. I. Brown, Matt J. Jarvis, Beatriz Mingo, Wendy L. Williams, S. P. OŚullivan, G. G ürkan, M. Brienza, Arti Goyal, Rebecca A. A. Bowler, M. A. Garrett, M. Br üggen, M. Bondi, M. Bonato, C. Tasse, Marek Jamrozy
Publikováno v:
Astronomy and Astrophysics, 648, 1-31
Astron.Astrophys.
Astron.Astrophys., 2021, 648, pp.A3. ⟨10.1051/0004-6361/202038813⟩
Astronomy and astrophysics, 648:A3. EDP Sciences
Astron.Astrophys.
Astron.Astrophys., 2021, 648, pp.A3. ⟨10.1051/0004-6361/202038813⟩
Astronomy and astrophysics, 648:A3. EDP Sciences
We present the source associations, cross-identifications, and multi-wavelength properties of the faint radio source population detected in the deep tier of the LOFAR Two Metre Sky Survey (LoTSS): the LoTSS Deep Fields. The first LoTSS Deep Fields da