activity
19952022
most citedRadio-loud Narrow-Line Type 1 Quasars

337 citations · 1.2k across the 38 of their papers we have counts for

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29 papers · 1 filter

astro-ph.GA2022

On Odd Radio Circles as Supernova Remnants

Sumit K. Sarbadhicary, Todd A. Thompson, Laura A. Lopez +1

The origin of arcmin-sized Odd Radio Circles (ORCs) found in modern all-sky radio surveys remain uncertain, with explanations ranging from starburst/AGN-driven shocks to supernova…

astro-ph.GA202144 cited

The hot circumgalactic medium of the Milky Way: evidence for super-virial, virial, and sub-virial temperature, non-solar chemical composition, and non-thermal line broadening

Sanskriti Das, Smita Mathur, Anjali Gupta +1

For the first time, we present the simultaneous detection and characterization of three distinct phases at K in absorption, using deep observations tow…

astro-ph.GA2021

X-ray sources in the 1.75 Ms Ultra Narrow Deep Field observed by XMM-Newton

M. Elías-Chávez, A. L. Longinotti, Y. Krongold +5

In this work we present the results of the survey carried out on one of the deepest X-ray fields observed by the XMM-Newton satellite. The 1.75 Ms Ultra Narrow Deep Field (XMM175UN…

astro-ph.GA202124 cited

Detection of a Multi-Phase Ultra-Fast Wind in the Narrow-Line Seyfert 1 Galaxy Mrk 1044

Y. Krongold, A. L. Longinotti, M. Santos-Lleo +6

We present a detailed analysis of XMM-Newton X-ray spectra of the Narrow-Line Seyfert 1 galaxy Mrk 1044. We find robust evidence for a multi-phase, ultra-fast outflow, traced by fo…

astro-ph.GA2020

Observations of the gamma-ray emitting narrow-line Seyfert 1, SBS 0846+513, and its host galaxy

Timothy S. Hamilton, Marco Berton, Sonia Antón +9

The gamma-ray emitting galaxy SBS 0846+513 has been classified as a Narrow-Line Seyfert 1 from its spectroscopy, and on that basis it was thought likely to have a small central bla…

astro-ph.GA2020

The host galaxy of OJ 287 revealed by optical and near-infrared imaging

K. Nilsson, J. Kotilainen, M. Valtonen +11

The BL Lacertae object OJ 287 (z = 0.306) has unique double-peaked optical outbursts every ~12 years, and it presents one of the best cases for a small-separation binary supermassi…