53 citations · 107 across the 10 of their papers we have counts for
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MIGHTEE-HI: Environmental effects of cosmic filaments on extragalactic HI detections in the COSMOS and XMM-LSS fields
Seoyoung Lyla Jung, Madalina N. Tudorache, Matt J. Jarvis +8
Cosmic filaments have been recognised as influencing galaxy evolution, but their connection to galactic cold gas reservoirs is elusive, particularly at low redshifts. We investigat…
MIGHTEE-HI: HI catalogue of 293 sources for the COSMOS field and comparative study of 3-dimensional source finding methods
Michalina Maksymowicz-Maciata, Natasha Maddox, Catherine Hale +12
We present a catalogue of HI sources extracted from the MIGHTEE survey data cubes covering the COSMOS field. The catalogue contains 293 sources in the redshift range of 0.004 < z <…
On the relationship between the cosmic web and the alignment of galaxies and AGN jets
Seoyoung Lyla Jung, I. H. Whittam, M. J. Jarvis +3
The impact of active galactic nuclei (AGN) on the evolution of galaxies explains the steep decrease in the number density of the most massive galaxies in the Universe. However, the…
Magnetised HI superbubbles in the Small Magellanic Cloud revealed by the POSSUM pilot survey
Seoyoung Lyla Jung, A. Seta, J. M. Price +13
Neutral hydrogen (HI) bubbles and shells are common in the interstellar medium (ISM). Studying their properties provides insight into the characteristics of the local ISM as well a…
Extragalactic Magnetism with SOFIA (SALSA Legacy Program). VII. A Tomographic View of Far-infrared and Radio Polarimetric Observations through MHD Simulations of Galaxies
Sergio Martin-Alvarez, Enrique Lopez-Rodriguez, Tara Dacunha +17
The structure of magnetic fields in galaxies remains poorly constrained, despite the importance of magnetism in the evolution of galaxies. Radio synchrotron and far-infrared (FIR)…
Sampling the Faraday rotation sky of TNG50: Imprint of the magnetised circumgalactic medium around Milky Way-like galaxies
Seoyoung Lyla Jung, N. M. McClure-Griffiths, Ruediger Pakmor +4
Faraday rotation measure (RM) is arguably the most practical observational tracer of magnetic fields in the diffuse circumgalactic medium (CGM). We sample synthetic Faraday rotatio…
Magnetic field draping around clumpy high-velocity clouds in galactic halo
Seoyoung Lyla Jung, Asger Grønnow, Naomi McClure-Griffiths
Throughout the passage within the Galactic halo, high-velocity clouds (HVCs) sweep up ambient magnetic fields and form stretched and draped configurations of magnetic fields around…
Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
Seoyoung Lyla Jung, Douglas Rennehan, Vida Saeedzadeh +6
Contrary to many stereotypes about massive galaxies, observed brightest group galaxies (BGGs) are diverse in their star formation rates, kinematic properties, and morphologies. Stu…
Distant probes of RM structure -- Where is the Faraday Rotation towards the Magellanic Leading Arm?
Seoyoung Lyla Jung, Naomi M. McClure-Griffiths, Alex S. Hill
Faraday Rotation Measures (RM) should be interpreted with caution because there could be multiple magneto-ionized medium components that contribute to the net Faraday rotation alon…
On the origin of gas-poor galaxies in galaxy clusters using cosmological hydrodynamic simulations
Seoyoung L. Jung, Hoseung Choi, O. Ivy Wong +3
The environmental effect is commonly used to explain the excess of gas-poor galaxies in galaxy clusters. Meanwhile, the presence of gas-poor galaxies at cluster outskirts, where ga…