activity
20022023
most citedCompact radio emission indicates a structured jet was produced by a binary neutron star merger

395 citations · 1.2k across the 50 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.IM2019★ 6 cited

The CASA software for radio astronomy: status update from ADASS 2019

B. Emonts, R. Raba, G. Moellenbrock +28

CASA, the Common Astronomy Software Applications package, is the primary data processing software for the Atacama Large Millimeter/submillimeter Array (ALMA) and NSF's Karl G. Jans…

astro-ph.GA2019★ 31 cited

ALMA observations of PKS 1549-79: a case of feeding and feedback in a young radio quasar

Tom Oosterloo, Raffaella Morganti, Clive Tadhunter +4

We present CO(1-0) and CO(3-2) ALMA observations of the molecular gas in PKS 1549-79, as well as mm and VLBI 2.3-GHz continuum observations of its radio jet. PKS 1549-79 is one of…

astro-ph.GA2019★ 12 cited

The presence of interstellar scintillation in the 15 GHz interday variability of 1158 OVRO-monitored blazars

J. Y. Koay, D. L. Jauncey, T. Hovatta +8

We have conducted the first systematic search for interday variability in a large sample of extragalactic radio sources at 15 GHz. From the sample of 1158 radio-selected blazars mo…

astro-ph.GA2019★ 39 cited

Detection statistics of the RadioAstron AGN survey

Y. Y. Kovalev, N. S. Kardashev, K. V. Sokolovsky +57

The largest Key Science Program of the RadioAstron space VLBI mission is a survey of active galactic nuclei (AGN). The main goal of the survey is to measure and study the brightnes…

astro-ph.GA2019★ 12 cited

Spica and the annual cycle of PKS B1322-110 scintillations

Hayley Bignall, Cormac Reynolds, Jamie Stevens +9

PKS B1322-110 is a radio quasar that is located only 8.5' in angular separation from the bright B star Spica. It exhibits intra-day variability in its flux density at GHz frequenci…

astro-ph.HE2019★ 3 cited

Nuclear spallation in active galaxies

L. C. Gallo, J. S. Randhawa, S. G. H. Waddell +3

A number of works point to the presence of narrow emission features at unusual energies in the X-ray spectra of active galactic nuclei (AGN) or to potentially low iron abundances a…