activity
19942025
most citedReviving Fossil Radio Plasma in Clusters of Galaxies by Adiabatic Compression in Environmental Shock Waves

273 citations · 2.2k across the 98 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.HE2013★ 3 cited

Constraints on supermassive black hole spins from observations of active galaxy jets

E. Kun, P. J. Wiita, L. Á. Gergely +3

We discuss the origin of the low-energy cutoff, or LEC, seen in the radio spectra of many extragalactic jets and relate this to the spin of the supermassive black holes that presum…

astro-ph.HE2013★ 3 cited

Supermassive black hole mergers as dual sources for electromagnetic flares in the jet emission and gravitational waves

M. Tápai, L. Á. Gergely, Z. Keresztes +3

We present a new type of observation relating the gravitational wave emission of supermassive black hole mergers to their electromagnetic counterparts. This dual emission involves…

astro-ph.HE2013★ 44 cited

Improved characterisation of intra-night optical variability of prominent AGN classes

Arti Goyal, Gopal-Krishna, Paul J. Wiita +2

The incidence of intra-night optical variability (INOV) is known to to differ significantly among different classes of powerful active galactic nuclei (AGN). A number of statistica…

astro-ph.CO2013★ 4 cited

Incidence of Strong MgII Absorbers Towards Different Types of Quasars

Ravi Joshi, Hum Chand, Gopal-Krishna

We report the first comparative study of strong MgII absorbers seen towards radio-loud quasars of core-dominated (CDQs) and lobe-dominated (LDQs) types and normal QSOs. The MgII as…

astro-ph.CO2013★ 18 cited

On the photometric error calibration for the `differential light curves' of point-like Active Galactic Nuclei

Arti Goyal, Mukul Mhaskey, Gopal-Krishna +3

It is important to quantify the underestimation of rms photometric errors returned by the commonly used algorithm in the software, in the context of dif…

astro-ph.EP2013★ 83 cited

Hint of 150 MHz radio emission from the Neptune-mass extrasolar transiting planet HAT-P-11b

A. Lecavelier des Etangs, S. K. Sirothia, Gopal-Krishna +1

Since the radio-frequency emission from planets is expected to be strongly influenced by their interaction with the magnetic field and corona of the host star, the physics of this…