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20132020
most citedRadio--Far infrared correlation in "blue cloud" galaxies with 0<z<1.2

42 citations · 82 across the 4 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA202016 cited

uGMRT detection of associated HI 21 cm absorption at

J. N. H. S. Aditya, Regina Jorgenson, Vishal Joshi +3

We report a uGMRT detection of HI 21-cm absorption associated with the radio source 8C 0604+728, at . The source is at the highest redshift at which associated HI 21-c…

astro-ph.GA2018

Kpc-scale radio-jets in narrow-line Seyfert 1 galaxies

Veeresh Singh, Hum Chand, C. H. Ishwara-Chandra +1

Narrow-Line Seyfert 1 galaxies (NLS1s) are generally believed to be radio-quiet Active Galactic Nuclei (AGN) with relatively less-massive (1010~M) Super-Ma…

astro-ph.GA2018

Investigating kpc-scale radio emission properties of narrow-line Seyfert 1 galaxies

Veeresh Singh, Hum Chand

In recent years, several Radio-Loud Narrow-Line Seyfert 1 galaxies (RL-NLS1) possessing relativistic jets have come into attention with their detections in Very Large Baseline Arra…

astro-ph.GA20178 cited

On the nature of infrared-faint radio sources in the SXDF and VLA-VVDS fields

Veeresh Singh, Yogesh Wadadekar, C. H. Ishwara-Chandra +4

Infrared-Faint Radio Sources (IFRSs) are an unusual class of objects that are relatively bright at radio wavelengths but have faint or undetected infrared counterparts even in deep…

astro-ph.GA2016

A GMRT Study of Seyfert Galaxies NGC4235 & NGC4594: Evidence of Episodic Activity ?

P. Kharb, S. Srivastava, V. Singh +3

Low frequency observations at 325 and 610 MHz have been carried out for two "radio-loud" Seyfert galaxies, NGC4235 and NGC4594 (Sombrero galaxy), using the Giant Meterwave Radio Te…

astro-ph.GA201542 cited

Radio--Far infrared correlation in "blue cloud" galaxies with 0<z<1.2

Aritra Basu, Yogesh Wadadekar, Alexandre Beelen +4

We study the radio--far infrared (FIR) correlation in "blue cloud" galaxies chosen from the PRism MUltiobject Survey (PRIMUS) up to redshift () of 1.2 in the XMM-LSS field. We u…