Search Results - "Dai, Y. Sophia"
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SDSS-IV MaNGA: How Galaxy Interactions Influence Active Galactic Nuclei
Published in The Astrophysical journal (01-01-2023)“…Abstract We present a comparative study of active galactic nuclei (AGN) between galaxy pairs and isolated galaxies with the final data release of the MaNGA…”
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A Complete 16 μm Selected Galaxy Sample at z ∼ 1. II. Morphological Analysis
Published in The Astrophysical journal (01-07-2024)“…Abstract We present a morphological analysis of the 16 μ m flux-density-limited galaxy sample at 0.8 < z < 1.3 from Huang et al. (2021). At the targeted…”
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Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures
Published in The Astrophysical journal (01-02-2024)“…Abstract Active galactic nucleus (AGN) driven outflows can have a significant impact on the evolution of the host galaxy. In this work, we compare the…”
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Bright z ∼ 9 Galaxies in Parallel: The Bright End of the Rest-frame UV Luminosity Function from HST Parallel Programs
Published in The Astrophysical journal (01-02-2024)“…Abstract The abundance of bright galaxies at z > 8 can provide key constraints on models of galaxy formation and evolution, as the predicted abundance varies…”
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A Close Look at Lyα Emitters with JWST/NIRCam at z ≈ 3.1
Published in The Astrophysical journal (01-05-2024)“…Abstract We study 10 spectroscopically confirmed Ly α emitters (LAEs) at z ≈ 3.1 in the Ultra Deep Survey field, covered by the James Webb Space…”
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SDSS-IV MaNGA: Spatial Evolution of Star Formation Triggered by Galaxy Interactions
Published in The Astrophysical journal (20-08-2019)“…Galaxy interaction is considered a key driver of galaxy evolution and star formation (SF) history. In this paper, we present an empirical picture of the radial…”
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SDSS-IV MaNGA: Galaxy Pair Fraction and Correlated Active Galactic Nuclei
Published in The Astrophysical journal (01-04-2018)“…We have identified 105 galaxy pairs at z ∼ 0.04 with the MaNGA integral-field spectroscopic data. The pairs have projected separations between 1 and 30 kpc,…”
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Lyman Continuum Escape Fraction from Low-mass Starbursts at z = 1.3
Published in The Astrophysical journal (01-11-2020)“…Abstract We present a new constraint on the Lyman continuum (LyC) escape fraction at . We obtain deep, high sensitivity far-UV imaging with the Advanced Camera…”
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A Spatially Resolved Analysis of Star Formation Burstiness by Comparing UV and Hα in Galaxies at z ∼ 1 with UVCANDELS
Published in The Astrophysical journal (01-08-2023)“…Abstract The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides Hubble Space…”
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ALMA MEASUREMENTS OF CIRCUMSTELLAR MATERIAL IN THE GQ LUP SYSTEM
Published in The Astrophysical journal (20-01-2017)“…ABSTRACT We present Atacama Large Millimeter/submillimeter Array observations of the GQ Lup system, a young Sun-like star with a substellar-mass companion in a…”
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Active Galactic Nuclei in a Mid-infrared Selected Galaxy Sample at z > 0.13: [Ne v]λ3426 Line Emission as a Benchmark
Published in The Astrophysical journal (01-03-2024)“…Abstract We present a 24 μ m-selected spectroscopic sample z > 0.13 (median 〈 z 〉 = 0.41) in the Lockman Hole field, consisting of 4035 spectra. Our aim is to…”
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Dust and Cold Gas Properties of Starburst HyLIRG Quasars at z ∼ 2.5
Published in The Astrophysical journal (01-04-2024)“…Abstract Some high- z active galactic nuclei (AGNs) are found to reside in extreme star-forming galaxies, such as hyperluminous infrared galaxies (HyLIRGs),…”
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Rotation of Two Micron All Sky Survey Clumps in Molecular Clouds
Published in The Astrophysical journal (01-08-2020)“…We have analyzed the rotational properties of 12 clumps using 13CO (1-0) and C18O (1-0) maps of the Five College Radio Astronomy Observatory 13.7 m radio…”
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SDSS-IV MaNGA: The Radial Profile of Enhanced Star Formation in Close Galaxy Pairs
Published in The Astrophysical journal (01-03-2021)“…Abstract We compare the radial profiles of the specific star formation rate (sSFR) in a sample of 169 star-forming galaxies in close pairs with those of…”
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Fraction of Clumpy Star-forming Galaxies at 0.5 ≤ z ≤ 3 in UVCANDELS: Dependence on Stellar Mass and Environment
Published in The Astrophysical journal (01-07-2023)“…Abstract High-resolution imaging of galaxies in rest-frame UV has revealed the existence of giant star-forming clumps prevalent in high-redshift galaxies…”
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UV-bright Star-forming Clumps and Their Host Galaxies in UVCANDELS at 0.5 ≤ z ≤ 1
Published in The Astrophysical journal (01-10-2023)“…Abstract Giant star-forming clumps are a prominent feature of star-forming galaxies (SFGs) and contain important clues on galaxy formation and evolution…”
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Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups
Published in The Astrophysical journal (01-04-2023)“…Abstract We explore how the fraction of quenched galaxies changes in groups of galaxies with respect to the distance to the center of the group, redshift, and…”
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The Most Distant H i Galaxies Discovered by the 500 m Dish FAST
Published in Astrophysical journal. Letters (01-05-2024)“…Abstract Neutral hydrogen (H i ) is the primary component of the cool interstellar medium (ISM) and is the reservoir of fuel for star formation. Owing to the…”
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The Velocity Map Asymmetry of Ionized Gas in MaNGA. I. The Catalog and General Properties
Published in The Astrophysical journal. Supplement series (01-09-2022)“…Abstract The SDSS-IV MaNGA survey has measured two-dimensional maps of emission-line velocities for a statistically powerful sample of nearby galaxies. The…”
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Spectroscopically Identified Emission Line Galaxy Pairs in the WISP Survey
Published in The Astrophysical journal (01-12-2021)“…Abstract We identify a sample of spectroscopically measured emission line galaxy (ELG) Pairs up to z = 1.6 from the Wide Field Camera 3 (WFC3) Infrared…”
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