activity
20142024
most citedMultiwavelength characterization of faint Ultra Steep Spectrum radio sources : A search for high-redshift radio galaxies

38 citations · 86 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2024

Large Projects in Astronomy: An Indian Endeavour

Yogesh Wadadekar, Shriharsh Tendulkar, Sanjit Mitra +6

Policy Brief on "Large Projects in Astronomy: An Indian Endeavour", distilled from the corresponding panel that was part of the discussions during S20 Policy Webinar on Astroinform…

astro-ph.IM20241 cited

AstroInformatics: Recommendations for Global Cooperation

Ashish Mahabal, Pranav Sharma, Rana Adhikari +45

Policy Brief on "AstroInformatics, Recommendations for Global Collaboration", distilled from panel discussions during S20 Policy Webinar on Astroinformatics for Sustainable Develop…

astro-ph.GA20221 cited

Detection of radio-AGN in dust-obscured galaxies using deep uGMRT radio continuum observations

Abhijit Kayal, Veeresh Singh, C. H. Ishwara Chandra +2

Radio observations being insensitive to the dust-obscuration, have been exploited to unveil the population of Active Galactic Nuclei (AGN) residing in galaxies with large dust cont…

astro-ph.GA20219 cited

Remnant radio galaxy candidates of small angular sizes

Veeresh Singh, Sushant Dutta, Yogesh Wadadekar +1

Remnant radio galaxies (RRGs), characterized by the cessation of AGN activity, represent a short-lived last phase of radio galaxy's life-cycle. Hitherto, searches for RRGs, mainly…

astro-ph.GA20168 cited

Seyfert 1 Composite Spectrum using SDSS Legacy Survey Data

Nihan Pol, Yogesh Wadadekar

We present a rest-frame composite spectrum for Seyfert 1 galaxies using spectra obtained from the DR12 release of the Sloan Digital Sky Survey (SDSS). The spectrum is constructed b…

astro-ph.GA201429 cited

Kiloparsec-scale radio emission in Seyfert and LINER galaxies

Veeresh Singh, C. H. Ishwara-Chandra, Yogesh Wadadekar +2

Seyfert and LINER galaxies are known to exhibit compact radio emission on 10 to 100 parsec scales, but larger Kiloparsec-Scale Radio structures (KSRs) often remain undetecte…