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20142026
most citedWinds as the origin of radio emission in radio-quiet extremely red quasars

70 citations · 1k across the 46 of their papers we have counts for

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24 papers · 1 filter

astro-ph.GA2026

Varstrometry for Off-nucleus and Dual Subkiloparsec AGN (VODKA): Three Quadruply Lensed Quasars at Cosmic Noon in HST and JWST

Mingrui Liu, Yu-Ching Chen, Nadia L. Zakamska +7

We present results from imaging observations of three quadruply lensed quasars by Hubble Space Telescope (HST) and James Webb Space Telescope (JWST) at redshifts , 2.975…

astro-ph.GA2025

VODKA: Complex molecular gas dynamics in a kpc-separation z=2.17 dual quasar with ALMA

Yuzo Ishikawa, Nadia L. Zakamska, Yu-Ching Chen +6

In galaxy mergers, dual quasars - two actively accreting supermassive black holes (SMBHs) - provide a unique opportunity to study the interplay between galaxy dynamics and quasar a…

astro-ph.GA2024

Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): A Mix of Singles, Lenses, and True Duals at Cosmic Noon

Arran C. Gross, Yu-Ching Chen, Masamune Oguri +8

Dual Active Galactic Nuclei (dual AGNs), a phase in some galaxy mergers during which both central supermassive black holes (SMBHs) are active, are expected to be a key observable s…

astro-ph.GA2024

Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): Long-slit optical spectroscopic follow-up with Gemini/GMOS and HST/STIS

Yu-Ching Chen, Arran C. Gross, Xin Liu +4

High spatial and spectral resolution observations are essential for identifying sub-arcsecond dual and lensed quasars and confirming their redshifts. We present Gemini/GMOS and HST…

astro-ph.GA2024

VODKA-JWST: A 3.8 kpc dual quasar at cosmic noon in a powerful starburst galaxy with JWST/MIRI IFU

Yu-Ching Chen, Yuzo Ishikawa, Nadia L. Zakamska +12

Dual quasars, two active supermassive black holes at galactic scales, represent crucial objects for studying the impact of galaxy mergers and quasar activity on the star formation…

astro-ph.GA2024★ 2 cited

VODKA-JWST: Synchronized growth of two SMBHs in a massive gas disk? A 3.8 kpc separation dual quasar at cosmic noon with NIRSpec IFU

Yuzo Ishikawa, Nadia L. Zakamska, Yue Shen +10

The search for dual supermassive black holes (SMBHs) is of immense interest in modern astrophysics. Galaxy mergers may fuel and produce SMBH pairs. Actively accreting SMBH pairs ar…

astro-ph.GA2023★ 1 cited

Varstrometry for Off-nucleus and Dual Sub-kpc AGN (VODKA): Very Long Baseline Array Searches for Dual or Off-nucleus Quasars and Small-scale Jets

Yu-Ching Chen, Xin Liu, Joseph Lazio +5

Dual and off-nucleus active supermassive black holes are expected to be common in the hierarchical structure formation paradigm, but their identification at parsec scales remains a…

astro-ph.GA2023

Discovery and Characterization of Galactic-scale Dual Supermassive Black Holes Across Cosmic Time

Yue Shen, J. Andrew Casey-Clyde, Yu-Ching Chen +10

The hierarchical structure formation paradigm predicts the formation of pairs of supermassive black holes in merging galaxies. When both (or one) members of the SMBH pair are unobs…

astro-ph.GA2023

Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): Investigating the Nature of J0823+2418 at : a Likely Lensed Quasar

Arran C. Gross, Yu-Ching Chen, Adi Foord +8

Dual quasars at small physical separations are an important precursor phase of galaxy mergers, ultimately leading to the coalescence of the two supermassive black holes. Starting f…

astro-ph.GA2023

Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA). SDSS J1608+2716: A Sub-arcsec Quadruply Lensed Quasar at z=2.575

Junyao Li, Xin Liu, Yue Shen +5

We report Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) deep IR (F160W) imaging of SDSS J1608+2716. This system, located at a redshift of z=2.575, was recently reported a…

astro-ph.GA2023★ 14 cited

Wide binary stars formed in the turbulent interstellar medium

Siyao Xu, Hsiang-Chih Hwang, Chris Hamilton +1

The ubiquitous interstellar turbulence regulates star formation and the scaling relations between the initial velocity differences and the initial separations of stars. We propose…

astro-ph.GA2022★ 27 cited

Statistics of Galactic-Scale Quasar Pairs at Cosmic Noon

Yue Shen, Hsiang-Chih Hwang, Masamune Oguri +8

The statistics of galactic-scale quasar pairs can elucidate our understanding of the dynamical evolution of supermassive black hole (SMBH) pairs, the duty cycles of quasar activity…

astro-ph.GA2021★ 11 cited

Wide binaries from the H3 survey: the thick disk and halo have similar wide binary fractions

Hsiang-Chih Hwang, Yuan-Sen Ting, Charlie Conroy +8

Due to the different environments in the Milky Way's disk and halo, comparing wide binaries in the disk and halo is key to understanding wide binary formation and evolution. By usi…

astro-ph.GA2021★ 55 cited

A hidden population of high-redshift double quasars unveiled by astrometry

Yue Shen, Yu-Ching Chen, Hsiang-Chih Hwang +6

Galaxy mergers occur frequently in the early universe and bring multiple supermassive black holes (SMBHs) into the nucleus, where they may eventually coalesce. Identifying post-mer…

astro-ph.GA2020★ 23 cited

Evidence for the Accretion of Gas in Star-Forming Galaxies: High N/O Abundances in Regions of Anomalously-Low Metallicity

Yuanze Luo, Timothy Heckman, Hsiang-Chih Hwang +11

While all models for the evolution of galaxies require the accretion of gas to sustain their growth via on-going star formation, it has proven difficult to directly detect this inf…

astro-ph.GA2019★ 66 cited

Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): How Well-centered Are Low-z AGN?

Yue Shen, Hsiang-Chih Hwang, Nadia Zakamska +1

Off-nucleus active galactic nuclei (AGN) can be signposts of inspiraling supermassive black holes (SMBHs) on galactic scales, or accreting SMBHs recoiling after the coalescence of…

astro-ph.GA2019★ 67 cited

Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): Methodology and Initial Results with Gaia DR2

Hsiang-Chih Hwang, Yue Shen, Nadia Zakamska +1

Gaia's milli-arcsec (mas) astrometric precision allows systematic identification of optically-selected sub-kpc dual active galactic nuclei (AGN), off-nucleus AGN, and small-scale l…

astro-ph.GA2019★ 34 cited

A Pseudodisk Threaded with a Toroidal and Pinched Poloidal Magnetic Field Morphology in the HH 211 Protostellar System

Chin-Fei Lee, Woojin Kwon, Kai-Syun Jhan +6

The HH 211 protostellar system is currently the youngest Class 0 system found with a rotating disk. We have mapped it at ~ 50 au (0.16") resolution, studying its magnetic field mor…

astro-ph.GA2019★ 47 cited

Characterizing the local relation between star formation rate and gas-phase metallicity in MaNGA spiral galaxies

Laura Sánchez-Menguiano, Jorge Sánchez Almeida, Casiana Muñoz-Tuñón +4

The role of gas accretion in galaxy evolution is still a matter of debate. The presence of inflows of metal-poor gas that trigger star formation bursts of low metallicity has been…

astro-ph.GA2018★ 54 cited

Anomalously low metallicity regions in MaNGA star-forming galaxies: Accretion Caught in Action?

Hsiang-Chih Hwang, Jorge K. Barrera-Ballesteros, Timothy M. Heckman +14

We use data from 1222 late-type star-forming galaxies in the SDSS IV MaNGA survey to identify regions in which the gas-phase metallicity is anomalously-low compared to expectations…

astro-ph.GA2018★ 45 cited

SDSS-IV MaNGA: Spatially resolved star-formation histories and the connection to galaxy physical properties

K. Rowlands, T. Heckman, V. Wild +11

A key task of observational extragalactic astronomy is to determine where -- within galaxies of diverse masses and morphologies -- stellar mass growth occurs, how it depends on gal…

astro-ph.GA2018★ 70 cited

Winds as the origin of radio emission in radio-quiet extremely red quasars

Hsiang-Chih Hwang, Nadia L. Zakamska, Rachael M. Alexandroff +4

Most active galactic nuclei (AGNs) are radio-quiet, and the origin of their radio emission is not well-understood. One hypothesis is that this radio emission is a by-product of qua…

astro-ph.GA2016★ 35 cited

Angular momentum loss in the envelope-disk transition region of HH 111 protostellar system: evidence for magnetic braking?

Chin-Fei Lee, Hsiang-Chih Hwang, Zhi-Yun Li

HH 111 is a Class I protostellar system at a distance of ~ 400 pc, with the central source VLA 1 associated with a rotating disk deeply embedded in a flattened envelope. Here we pr…

astro-ph.GA2014★ 20 cited

Magnetic field structure in the Flattened Envelope and Jet in the young protostellar system HH 211

Chin-Fei Lee, Ramprasad Rao, Tao-Chung Ching +4

HH 211 is a young Class 0 protostellar system, with a flattened envelope, a possible rotating disk, and a collimated jet. We have mapped it with the Submillimeter Array in 341.6 GH…