Four hot DOGs in the microwave

S Frey, Z Paragi, KÉ Gabányi… - Monthly Notices of the …, 2016 - academic.oup.com
Hot dust-obscured galaxies (hot DOGs) are a rare class of hyperluminous infrared galaxies
identified with the Wide-field Infrared Survey Explorer (WISE) satellite. The majority of them …

Structural and spectral properties of Galactic plane variable radio sources

J Yang, Y Chen, LI Gurvits, Z Paragi… - Monthly Notices of …, 2022 - academic.oup.com
In the time domain, the radio sky in particular along the Galactic plane direction may vary
significantly because of various energetic activities associated with stars, stellar, and …

Magnetospheric origin of a fast radio burst constrained using scintillation

K Nimmo, Z Pleunis, P Beniamini, P Kumar… - arXiv preprint arXiv …, 2024 - arxiv.org
Fast radio bursts (FRBs) are micro-to-millisecond duration radio transients that originate
mostly from extragalactic distances. The emission mechanism responsible for these high …

The radio structure of the peculiar narrow-line Seyfert 1 galaxy candidate J1100+ 4421

KÉ Gabányi, S Frey, Z Paragi, E Järvelä… - Monthly Notices of …, 2018 - academic.oup.com
Narrow-line Seyfert 1 galaxies (NLS1) are an intriguing subclass of active galactic nuclei.
Their observed properties indicate low central black hole mass and high accretion rate. The …

A Radio Study of Persistent Radio Sources in Nearby Dwarf Galaxies: Implications for Fast Radio Bursts

Y Dong, T Eftekhari, W Fong, S Bhandari… - arXiv preprint arXiv …, 2024 - arxiv.org
We present 1-12 GHz Karl G. Jansky Very Large Array observations of 9 off-nuclear
persistent radio sources (PRSs) in nearby (z< 0.055) dwarf galaxies, along with high …

European VLBI Network Observations of the Proposed Dual AGN SDSS J101022. 95+ 141300.9

PM Veres, KÉ Gabányi, S Frey, Z Paragi… - The Astrophysical …, 2021 - iopscience.iop.org
During galaxy merger events, the supermassive black holes in the center of the galaxies
may form a pair of active galactic nuclei (AGN) with kiloparsec-scale or even parsec-scale …

A radio structure resolved at the deca-parsec scale in the radio-quiet quasar PDS 456 with an extremely powerful X-ray outflow

J Yang, T An, F Zheng, WA Baan… - Monthly Notices of …, 2019 - academic.oup.com
Active galactic nuclei (AGNs) accreting at rates close to the Eddington limit can host
radiatively driven mildly relativistic outflows. Some of these X-ray absorbing but powerful …

A VLBI Software Correlator for Fast Radio Transients

C Leung, S Andrew, KW Masui, C Brar… - arXiv preprint arXiv …, 2024 - arxiv.org
One major goal in fast radio burst science is to detect fast radio bursts (FRBs) over a wide
field of view without sacrificing the angular resolution required to pinpoint them to their host …

VLBI astrometry on the white dwarf pulsar AR Scorpii

P Jiang, L Cui, J Yang, B Zhang, S Xu… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT AR Scorpii (AR Sco), the only-known radio-pulsing white dwarf binary, shows
unusual pulsating emission at the radio, infrared, optical, and ultraviolet bands. To …

A long-lived compact jet in the black hole X-ray binary candidate AT2019wey

HM Cao, G Migliori, M Giroletti, S Frey, J Yang… - Astronomy & …, 2022 - aanda.org
AT2019wey is a transient discovered by the Asteroid Terrestrial-impact Last Alert System
survey in December of 2019. Follow-up optical, radio, and X-ray observations led to …