Search Results - "Wagenveld, J. D"

Mapping H i 21-cm in the Klemola 31 group at z = 0.029: emission and absorption towards PKS 2020−370 by Maina, E K, Mohapatra, Abhisek, Józsa, G I G, Gupta, N, Combes, F, Deka, P, Wagenveld, J D, Srianand, R, Balashev, S A, Chen, Hsiao-Wen, Krogager, J-K, Momjian, E, Noterdaeme, P, Petitjean, P

“…ABSTRACT We present MeerKAT Absorption Line Survey (MALS) observations of the H i gas in the Klemola 31 galaxy group (z = 0.029), located along the line of…”
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The cosmic radio dipole: Bayesian estimators on new and old radio surveys by Wagenveld, J. D, Klöckner, H-R, Schwarz, D. J

“…A&A 675, A72 (2023) The cosmic radio dipole is an anisotropy in the number counts of radio sources, analogous to the dipole seen in the cosmic microwave…”
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Revealing new high redshift quasar populations through Gaussian mixture model selection by Wagenveld, J. D, Saxena, A, Duncan, K. J, Röttgering, H. J. A, Zhang, M

“…A&A 660, A22 (2022) We present a novel method to identify candidate high redshift quasars (HzQs; ($z\gtrsim5.5$), which are unique probes of supermassive black…”
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Plausible association of distant late M dwarfs with low-frequency radio emission by Gloudemans, A. J, Callingham, J. R, Duncan, K. J, Saxena, A, Harikane, Y, Hill, G. J, Zeimann, G. R, Rottgering, H. J. A, Hardcastle, M. J, Pineda, J. S, Shimwell, T. W, Smith, D. J. B, Wagenveld, J. D

“…A&A 678, A161 (2023) We present the serendipitous discovery of 8 distant ($>$ 50 pc) late M dwarfs with plausible associated radio emission at 144 MHz. The M…”
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The MeerKAT Absorption Line Survey: Homogeneous continuum catalogues towards a measurement of the cosmic radio dipole by Wagenveld, J. D, Klöckner, H. -R, Gupta, N, Deka, P. P, Jagannathan, P, Sekhar, S, Balashev, S. A, Boettcher, E, Combes, F, Emig, K. L, Hilton, M, Józsa, G. I. G, Kamphuis, P, Klutse, D. Y, Knowles, K, Krogager, J. -K, Mohapatra, A, Momjian, E, Moodley, K, Muller, S, Petitjean, P, Salas, P, Sikhosana, S, Srianand, R

“…A&A 673, A113 (2023) The number counts of homogeneous samples of radio sources are a tried and true method of probing the large scale structure of the…”
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Mapping HI 21-cm in the Klemola 31 group at z = 0.029: emission and absorption towards PKS2020-370 by Maina, E. K, Mohapatra, Abhisek, Jozsa, G. I. G, Gupta, N, Combes, F, Deka, P, Wagenveld, J. D, Srianand, R, Balashev, S. A, Chen, Hsiao-Wen, Krogager, J. -K, Momjian, E, Noterdaeme, P, Petitjean, P

“…We present MeerKAT Absorption Line Survey (MALS) observations of the HI gas in the Klemola31 galaxy group ($z=0.029$), located along the line of sight to the…”
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The LOFAR Two Metre Sky Survey: Deep Fields Data Release 1 -- III. Host-galaxy identifications and value added catalogues by 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, R\öttgering, H. J. A, Smith, D. J. B, Wo\łowska, A, Bondi, M, Brienza, M, Brown, M. J. I, Br\üggen, M, Chambers, K, Garrett, M. A, G\ürkan, G, Huber, M, Kunert-Bajraszewska, M, Magnier, E, Mingo, B, Mostert, R, Nikiel-Wroczy\\ński, B, OŚullivan, S. P, Paladino, R, Ploeckinger, T, Prandoni, I, Rosenthal, M. J, Schwarz, D. J, Shulevski, A, Wagenveld, J. D, Wang, L

“…A&A 648, A3 (2021) We present the source associations, cross-identifications, and multi-wavelength properties of the faint radio source population detected in…”
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The MeerKAT Absorption Line Survey Data Release 2: Wideband continuum catalogues and a measurement of the cosmic radio dipole by Wagenveld, J. D, Klöckner, H-R, Gupta, N, Sekhar, S, Jagannathan, P, Deka, P. P, Jose, J, Balashev, S. A, Borgaonkar, D, Chatterjee, A, Combes, F, Emig, K. L, Gaunekar, A. N, Hilton, M, Józsa, G. I. G, Klutse, D. Y, Knowles, K, Krogager, J. -K, Momjian, E, Muller, S, Sikhosana, S. P

“…We present the second data release of the MeerKAT Absorption Line Survey (MALS), consisting of wideband continuum catalogues of 391 pointings observed at…”
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Discovery of 24 radio-bright quasars at $4.9 \leq z \leq6.6$ using low-frequency radio observations by Gloudemans, A. J, Duncan, K. J, Saxena, A, Harikane, Y, Hill, G. J, Zeimann, G. R, Rottgering, H. J. A, Yang, D, Best, P. N, Banados, E, Drabent, A, Hardcastle, M. J, Hennawi, J. F, Lansbury, G, Magliocchetti, M, Miley, G. K, Nanni, R, Shimwell, T. W, Smith, D. J. B, Venemans, B. P, Wagenveld, J. D

“…High redshift quasars ($z>5$) that also shine brightly at radio wavelengths are unique signposts of supermassive black hole activity in the early universe…”
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