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20092023
most citedDiscovery of 21 New Changing-look AGNs in Northern Sky

220 citations · 904 across the 41 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.GA2022★ 4 cited

Evidence of under-developed torus and broad-line region of weak emission line quasars based on their spectral energy distribution

Ritish Kumar, Hum Chand, Ravi Joshi

To unravel the dominant cause of the weak emission line in a subset of optically selected radio-quiet 'weak emission line quasars' (WLQs), we have investigated the possibility of a…

astro-ph.GA2022★ 6 cited

The X-shaped radio galaxy J0725+5835 is associated with an AGN pair

Xiaolong Yang, Jialu Ji, Ravi Joshi +6

X-shaped radio galaxies (XRGs) are those that exhibit two pairs of unaligned radio lobes (main radio lobes and "wings"), one of the promising models for the peculiar morphology is…

astro-ph.GA2022

Probable low-frequency quasi-periodic oscillations in blazars from the ZTF survey

Anuvab Banerjee, Vibhore Negi, Ravi Joshi +6

We investigate the possible presence of quasi-periodic oscillation (QPO) signals in 2103 blazars from the Zwicky Transient Facility (ZTF) time-domain survey. We detect a low-freque…

astro-ph.GA2022★ 22 cited

Finding Quasars behind the Galactic Plane. II. Spectroscopic Identifications of 204 Quasars at

Yuming Fu, Xue-Bing Wu, Linhua Jiang +21

Quasars behind the Galactic plane (GPQs) are important astrometric references and valuable probes of Galactic gas, yet the search for GPQs is difficult due to severe extinction and…

astro-ph.GA2022

The Twin Radio galaxy TRG J104454+354055

Gopal-Krishna, Ravi Joshi, Dusmanta Patra +4

We report observations of a bright dumb-bell system of galaxies () with the upgraded Giant Metrewave Radio Telescope (GMRT), which show that each member of this gravit…

astro-ph.GA2022★ 15 cited

Host Galaxies of Ultra Strong Mg II absorbers at z 0.5

Labanya Kumar Guha, Raghunathan Srianand, Rajeshwari Dutta +3

From a sample of 109 candidate Ultra-Strong Mg II (USMgII; having rest equivalent width of Mg II absorption, Angstrom) systems at z=0.4-0.6, we confirm 27 and identi…