Y. Sophia Dai
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View article: Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution (PASSAGE): Survey Overview
Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution (PASSAGE): Survey Overview Open
During the second half of Cycle 1 of the James Webb Space Telescope (JWST), we conducted the Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution (PASSAGE) program. PASSAGE received the largest allocation of JWST obser…
View article: Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and Their Protohalos
Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and Their Protohalos Open
We investigated the evolution of the physical properties of the brightest galaxies in clusters and their protohalos from z = 4 to z = 0. Galaxy clusters and groups are identified using a halo-based group finder applied to the COSMOS2020 ga…
View article: Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and their Protohalos
Evolution of the Physical Properties of the Most Massive Galaxies in Clusters and their Protohalos Open
We investigated the evolution of the physical properties of the brightest galaxies in clusters and their protohalos from $z = 4$ to $z = 0$. Galaxy clusters and groups are identified using a halo-based group finder applied to the COSMOS202…
View article: Noema formIng Cluster survEy (NICE): A census of star formation and cold gas properties in massive protoclusters at 1.5<z<4
Noema formIng Cluster survEy (NICE): A census of star formation and cold gas properties in massive protoclusters at 1.5<z<4 Open
Massive protoclusters at z ∼ 1.5-4, the peak of the cosmic star formation history, are key to understanding the formation mechanisms of massive galaxies in today's clusters. However, studies of protoclusters at these high redshifts remain …
View article: JWST/MIRI Reveals the True Number Density of Massive Galaxies in the Early Universe
JWST/MIRI Reveals the True Number Density of Massive Galaxies in the Early Universe Open
Early JWST studies reporting an unexpected abundance of massive galaxies at z ∼ 5–8 challenge galaxy formation models in the ΛCDM framework. Previous stellar mass ( M ⋆ ) estimates suffered from large uncertainties due to the lack of rest-…
View article: Immunoglobulin-derived peptide MEANP1 of human Milk in the protection against experimental necrotizing Enterocolitis via IκB/ NF-κB pathway
Immunoglobulin-derived peptide MEANP1 of human Milk in the protection against experimental necrotizing Enterocolitis via IκB/ NF-κB pathway Open
View article: The JWST/PASSAGE Survey: Testing Reionization Histories with JWST’s First Unbiased Survey for Ly<i>α</i> Emitters at Redshifts 7.5–9.5
The JWST/PASSAGE Survey: Testing Reionization Histories with JWST’s First Unbiased Survey for Ly<i>α</i> Emitters at Redshifts 7.5–9.5 Open
Ly α emission is one of a few observable features of galaxies that can trace the neutral hydrogen content in the Universe during the Epoch of Reionization (EoR). To accomplish this, we need an efficient way to survey for Ly α emitters (LAE…
View article: Creation of a rat model of ovarian endometriosis: a novel and easy approach to simulating chocolate cysts
Creation of a rat model of ovarian endometriosis: a novel and easy approach to simulating chocolate cysts Open
Ovarian endometriosis(OEM) is the most common type of endometriosis, but there is still a lack of simple and easy-to-promote animal models. Therefore, it is necessary to establish a feasible animal model of OEM and analyze its pathogenesis…
View article: The JWST/PASSAGE Survey: Testing Reionization Histories with JWST's First Unbiased Survey for Lyman alpha Emitters at Redshifts 7.5-9.5
The JWST/PASSAGE Survey: Testing Reionization Histories with JWST's First Unbiased Survey for Lyman alpha Emitters at Redshifts 7.5-9.5 Open
Lyman $α$ (Ly$α$) emission is one of few observable features of galaxies that can trace the neutral hydrogen content in the Universe during the Epoch of Reionization (EoR). To accomplish this we need an efficient way to survey for Ly$α$ em…
View article: Comparison of Global H i and Hα Line Profiles in MaNGA Galaxy Pairs with FAST
Comparison of Global H i and Hα Line Profiles in MaNGA Galaxy Pairs with FAST Open
We present case studies comparing the global H i and H α emission line profiles of six galaxy pairs. The six pairs are selected to have different nuclear activities, with two hosting an active galactic nucleus, and in different merging sta…
View article: Starburst Galaxies in Their Last Billion Years: An H<i>δ</i> Absorption Line Selected Sample
Starburst Galaxies in Their Last Billion Years: An H<i>δ</i> Absorption Line Selected Sample Open
In this paper, we focus on the study of starburst galaxies in their final billion years. Our galaxy selection is based solely on the presence of the H δ absorption line, which permits the later evolution of starburst galaxies to be traced,…
View article: Starburst Galaxies in Their Last Billion Years: An H$δ$ Absorption Line Selected Sample
Starburst Galaxies in Their Last Billion Years: An H$δ$ Absorption Line Selected Sample Open
In this paper, we focus on the study of starburst galaxies in their final billion years. Our galaxy selection is based solely on the presence of the H$δ$ absorption line, which permits tracing the later evolution of starburst galaxies, coi…
View article: The Lyman Continuum Escape Fraction of Star-forming Galaxies at 2.4 ≲ <i>z</i> ≲ 3.0 from UVCANDELS
The Lyman Continuum Escape Fraction of Star-forming Galaxies at 2.4 ≲ <i>z</i> ≲ 3.0 from UVCANDELS Open
The UltraViolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) survey is a Hubble Space Telescope (HST) Cycle-26 Treasury Program, allocated in total 164 orbits of primary Wide-Field Camera…
View article: Molecular mechanism of aberrant decidualization in adenomyosis leading to reduced endometrial receptivity
Molecular mechanism of aberrant decidualization in adenomyosis leading to reduced endometrial receptivity Open
Patients with adenomyosis not only experience a decrease in quality of life as a result of dysmenorrhea and severe monthly flow but they are also rendered infertile. Pregnancy rates are still low among women with adenomyosis, even with ass…
View article: Nanozyme‐Based Flexible Wearable Devices for the Detection of Human Biomarkers
Nanozyme‐Based Flexible Wearable Devices for the Detection of Human Biomarkers Open
View article: Shared Attention-based Autoencoder with Hierarchical Fusion-based Graph Convolution Network for sEEG SOZ Identification
Shared Attention-based Autoencoder with Hierarchical Fusion-based Graph Convolution Network for sEEG SOZ Identification Open
Diagnosing seizure onset zone (SOZ) is a challenge in neurosurgery, where stereoelectroencephalography (sEEG) serves as a critical technique. In sEEG SOZ identification, the existing studies focus solely on the intra-patient representation…
View article: Development and Experiment of Adaptive Oolong Tea Harvesting Robot Based on Visual Localization
Development and Experiment of Adaptive Oolong Tea Harvesting Robot Based on Visual Localization Open
Aimed to improve the quality of picked tea leaves and the efficiency of tea harvesting, an adaptive oolong tea harvesting robot with an adjustment module of a cutting tool and a harvesting line localization algorithm is proposed. The robot…
View article: The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data
The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data Open
This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete release of the Mapping Nearby Galaxies at Apache Point Obs…
View article: UVCANDELS: Catalogs of Photometric Redshifts and Galaxy Physical Properties
UVCANDELS: Catalogs of Photometric Redshifts and Galaxy Physical Properties Open
The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep Hubble Space Telescope (HST) F275W and F435W imaging over four CANDELS fields (GOODS-N, GOODS-S, COSMOS,…
View article: UVCANDELS: Catalogs of photometric redshifts and galaxy physical properties
UVCANDELS: Catalogs of photometric redshifts and galaxy physical properties Open
The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep HST F275W and F435W imaging over four CANDELS fields (GOODS-N, GOODS-S, COSMOS, and EGS). We combine thi…
View article: Emission-line galaxies at <i>z</i> ∼ 1 from near-IR <i>HST</i> slitless spectroscopy: metallicities, star formation rates, and redshift confirmations from VLT/FORS2 spectroscopy
Emission-line galaxies at <i>z</i> ∼ 1 from near-IR <i>HST</i> slitless spectroscopy: metallicities, star formation rates, and redshift confirmations from VLT/FORS2 spectroscopy Open
We follow up emission line galaxies identified through the near-infrared slitless HST/WFC3 WISP survey with VLT/FORS2 optical spectroscopy. Over 4 WISP fields, we targeted 85 of 138 line emission objects at $0.4\lt z\lt 2$ identified in WF…
View article: The Ultraviolet Luminosity Function at 0.6 < z < 1 from UVCANDELS
The Ultraviolet Luminosity Function at 0.6 < z < 1 from UVCANDELS Open
UVCANDELS is a Hubble Space Telescope Cycle-26 Treasury Program awarded 164 orbits of primary ultraviolet (UV) F275W imaging and coordinated parallel optical F435W imaging in four CANDELS fields—GOODS-N, GOODS-S, EGS, and COSMOS—covering a…
View article: NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5 < <i>z</i> < 4 in the COSMOS field
NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5 < <i>z</i> < 4 in the COSMOS field Open
The NOrthern Extended Millimeter Array (NOEMA) formIng Cluster survEy (NICE) is a NOEMA large programme targeting 69 massive galaxy group candidates at z > 2 over six deep fields with a total area of 46 deg 2 . Here we report the spectrosc…
View article: NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at $1.5 < z < 4$ in the COSMOS field
NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at $1.5 < z < 4$ in the COSMOS field Open
The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at $z>2$ in six deep fields. We report spectroscopic confirmation of eight groups at $1.65\leq z\leq3.61$ in COSMOS. Homogeneously sele…
View article: A Complete 16 μm Selected Galaxy Sample at z ∼ 1. II. Morphological Analysis
A Complete 16 μm Selected Galaxy Sample at z ∼ 1. II. Morphological Analysis Open
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 redshift, the 16 μ m emission corresponds to the polycyclic aromatic hydrocarbon feature from i…
View article: A Complete 16 $μ$m selected Galaxy Sample at $z \sim 1$. II: Morphological Analysis
A Complete 16 $μ$m selected Galaxy Sample at $z \sim 1$. II: Morphological Analysis Open
We present morphological analysis of the 16$μ$m flux-density-limited galaxy sample at 0.8$
View article: A Close Look at Lyα Emitters with JWST/NIRCam at z ≈ 3.1
A Close Look at Lyα Emitters with JWST/NIRCam at z ≈ 3.1 Open
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 Telescope/NIRCam in the Public Release Imaging for Extragalactic Research program. All LAEs are detecte…
View article: The Most Distant H i Galaxies Discovered by the 500 m Dish FAST
The Most Distant H i Galaxies Discovered by the 500 m Dish FAST Open
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 sensitivity of existing radio telescopes, our understanding of the evolution of the ISM in…
View article: WFC3 Infrared Spectroscopic Parallel (WISP) Survey: Photometric and Emission Line Data Release
WFC3 Infrared Spectroscopic Parallel (WISP) Survey: Photometric and Emission Line Data Release Open
We present reduced images and catalogues of photometric and emission line data ($\sim$230,000 and $\sim$8,000 sources, respectively) for the WFC3 Infrared Spectroscopic Parallel (WISP) Survey. These data are made publicly available on the …
View article: WFC3 Infrared Spectroscopic Parallel (WISP) survey: photometric and emission-line data release
WFC3 Infrared Spectroscopic Parallel (WISP) survey: photometric and emission-line data release Open
We present reduced images and catalogues of photometric and emission-line data (∼230 000 and ∼8000 sources, respectively) for the WFC3 (Wide Field Camera 3) Infrared Spectroscopic Parallel (WISP) survey. These data are made publicly availa…