activity
20182024
most citedBH Mass, Jet and Accretion Disk Connection: An Analysis of Radio-loud and Radio-quiet Quasars

5 citations · 12 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2024★ 1 cited

Spectral Energy Distribution Modeling of Broad Emission Line Quasars: From X-ray to Radio Wavelengths

Avinanda Chakraborty, Maitreya Kundu, Suchetana Chatterjee +4

We study the differences in physical properties of quasar-host galaxies using an optically selected sample of radio loud (RL) and radio quiet (RQ) quasars (in the redshift range 0.…

astro-ph.CO2023★ 2 cited

Cosmological Simulations of Galaxy Groups and Clusters-III: Constraining Quasar Feedback Models with the Atacama Large Millimeter Array

Avinanda Chakraborty, Suchetana Chatterjee, Mark Lacy +3

The thermal Sunyaev-Zeldovich (SZ) effect serves as a direct potential probe of the energetic outflows from quasars that are responsible for heating the intergalactic medium. In th…

astro-ph.GA2021★ 3 cited

Properties of Very Broad Line MgII Radio-Loud and Radio-Quiet Quasars

Avinanda Chakraborty, Anirban Bhattacharjee, Suchetana Chatterjee

We perform an analysis of the properties of radio-loud (RL) and radio-quiet (RQ) quasars with MgII broad emission line (i-band magnitude and z ), selected fro…

astro-ph.GA2020★ 5 cited

BH Mass, Jet and Accretion Disk Connection: An Analysis of Radio-loud and Radio-quiet Quasars

Avinanda Chakraborty, Anirban Bhattacharjee

Surveys have shown radio-loud (RL) quasars constitute - of the total quasar population. However, it is unknown if the radio-loud fraction (RL quasars/Total quasars) r…

astro-ph.GA2020

Spectroscopic properties of radio-loud and radio-quiet quasars

Avinanda Chakraborty, Anirban Bhattacharjee

Surveys have shown radio-loud (RL) quasars constitute 10%-15% of the total quasar population and rest are radio-quiet (RQ). However, it is unknown if this radio-loud fraction (RLF)…

astro-ph.GA2018★ 1 cited

Science with an ngVLA: The Sunyaev-Zeldovich Effect from Quasar and Starburst Winds

Mark Lacy, Suchetana Chatterjee, Avinanda Chakraborty +6

The Sunyaev-Zeldovich Effect (SZE) can be used to detect the hot bubbles in the intergalactic medium blown by energetic winds from AGN and starbursts. By directly constraining the…