activity
19982024
most citedGiant Radio Sources

153 citations · 2.1k across the 89 of their papers we have counts for

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36 papers · 1 filter

astro-ph.GA2023★ 4 cited

Star formation history of mass-selected galaxies in the ELAIS-N1 Field

E. F. Ocran, M. Vaccari, J. M. Stil +3

We measure the specific star formation rates of \textit{K}-band selected galaxies from the ELAIS-N1 by stacking GMRT data at 610 MHz. We identify a sample of SFGs, spanning $\rm{0.…

astro-ph.GA2023★ 18 cited

Radio spectral properties of star-forming galaxies between 150-5000MHz in the ELAIS-N1 field

Fangxia An, M. Vaccari, P. N. Best +9

By combining high-sensitivity LOFAR 150MHz, uGMRT 400MHz and 1,250MHz, GMRT 610MHz, and VLA 5GHz data in the ELAIS-N1 field, we study the radio spectral properties of radio-detecte…

astro-ph.GA2023★ 20 cited

AGN Feedback Through Multiple Jet Cycles in the Seyfert Galaxy NGC 2639

Vaishnav V. Rao, Preeti Kharb, Rubinur K. +7

The Seyfert galaxy NGC 2639 was known to exhibit three episodes of AGN jet/lobe activity. We present here the upgraded Giant Metrewave Radio Telescope (uGMRT) 735 MHz image of NGC…

astro-ph.GA2022★ 13 cited

Barbell-shaped giant radio galaxy with ~100 kpc kink in the jet

Pratik Dabhade, Timothy W. Shimwell, Joydeep Bagchi +8

We present for the first time a study of peculiar giant radio galaxy (GRG) J223301+131502 using deep multi-frequency radio observations from GMRT (323, 612, and 1300 MHz) and LOFAR…

astro-ph.GA2022★ 3 cited

The structure at the centre of the giant radio galaxy GRS J0844+4627: a compact symmetric object?

A. Marecki, B. Sebastian, C. H. Ishwara-Chandra

We observed the core region of the giant radio galaxy GRS J0844+4627 with e-MERLIN at 1.52 and 5.07 GHz. These observations revealed that the apparent single feature at the centre…

astro-ph.GA2022★ 13 cited

Selecting and Modelling Remnant AGNs with Limited Spectral Coverage

B. Quici, R. J. Turner, N. Seymour +3

Quantifying the energetics and lifetimes of remnant radio-loud active galactic nuclei (AGNs) is much more challenging than for active sources due to the added complexity of accurat…