papers

Publications (410)

astro-ph.GA2023

Imaging Molecular Outflow in Massive Star-forming Regions with HNCO Lines

Jinjin Xie, Juan Li, Junzhi Wang +8

Protostellar outflows are considered a signpost of star formation. These outflows can cause shocks in the molecular gas and are typically traced by the line wings of certain molecu…

astro-ph.GA2021

The first evidence for three-dimensional spin-velocity alignment in pulsars

Jumei Yao, Weiwei Zhu, Richard N. Manchester +11

More than 50 years after the discovery of pulsars and confirmation of their association with supernova explosions, the origin of the initial spin and velocity of pulsars remains la…

astro-ph2004

Observations of Water Vapor Outflow from NML Cygnus

Viktor Zubko, Di Li, Tanya Lim +2

We report new observations of the far infrared and submillimeter water vapor emission of NML Cygnus based on data gathered with the Infrared Space Observatory and the Submillimeter…

cs.CV2026

Are VLMs Lost Between Sky and Space? LinkSBench for UAV-Satellite Dynamic Cross-View Spatial Intelligence

Dian Liu, Jie Feng, Di Li +4

Synergistic spatial intelligence between UAVs and satellites is indispensable for emergency response and security operations, as it uniquely integrates macro-scale global coverage…

astro-ph.HE2025

Multi-year Polarimetric Monitoring of Four CHIME-Discovered Repeating Fast Radio Bursts with FAST

Yi Feng, Yong-Kun Zhang, Jintao Xie +50

In this study, we report multi-year polarization measurements of four repeating FRBs initially discovered by CHIME: FRBs~20190117A, 20190208A, 20190303A, and 20190417A. We observed…

astro-ph.HE2022

Deep simultaneous limits on optical emission from FRB 20190520B by 24.4 fps observations with Tomo-e Gozen

Yuu Niino, Mamoru Doi, Shigeyuki Sako +16

We conduct 24.4~fps optical observations of repeating Fast Radio Burst (FRB) 20190520B using Tomo-e Gozen, a high-speed CMOS camera mounted on the Kiso 105-cm Schmidt telescope, si…

astro-ph.GA2021

An Early Transition to Magnetic Supercriticality in Star Formation

Tao-Chung Ching, Di Li, Carl Heiles +5

Magnetic fields play an important role in the evolution of interstellar medium and star formation. As the only direct probe of interstellar field strength, credible Zeeman measurem…

astro-ph.GA2019

Tracing the Formation of Molecular Clouds in a Low-Metallicity Galaxy: A HI Narrow Self-Absorption Survey of the Large Magellanic Cloud

Boyang Liu, Di Li, Lister Staveley-Smith +3

Cold atomic hydrogen clouds are the precursors of molecular clouds. Due to self-absorption, the opacity of cold atomic hydrogen may be high, and this gas may constitute an importan…

astro-ph.GA2021

Independent Core Rotation in Massive Filaments in Orion

Xuefang Xu, Di Li, Y. Sophia Dai +2

We present high-angular-resolution ALMA (Atacama Large Millimeter Array) images of NH (1--0) that has been combined with those from the Nobeyama telescope toward OMC-2…

astro-ph.GA2022

The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2

Jihye Hwang, Jongsoo Kim, Kate Pattle +157

We present and analyze observations of polarized dust emission at 850 m towards the central 1 pc 1 pc hub-filament structure of Monoceros R2 (Mon R2). The data are obt…

astro-ph.GA2021

ATOMS:ALMA Three-millimeter Observations of Massive Star-forming regions -- III :Catalogues of candidate hot molecular cores and Hyper/Ultra compact HII regions

Hong-Li Liu, Tie Liu, Neal J. Evans +50

We have identified 453 compact dense cores in 3 mm continuum emission maps in the ATOMS (ALMA Three-millimeter Observations of Massive Star-forming regions) survey, and compiled th…

astro-ph.GA2020

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- I. Survey description and a first look at G9.62+0.19

Tie Liu, Neal J. Evans, Kee-Tae Kim +41

The "ATOMS," standing for {\it ALMA Three-millimeter Observations of Massive Star-forming regions}, survey has observed 146 active star forming regions with ALMA Band 3, aiming to…

astro-ph.HE2025

Do Multi-Structural One-Off FRBs Trace Similar Cosmology History with Repeaters?

Yu-Hao Zhu, Chen-Hui Niu, Xiang-Han Cui +7

Fast Radio Bursts (FRBs) are millisecond-duration transient events that are typically observed at radio wavelengths and cosmological distances but their origin remains unclear. Fur…

astro-ph.GA2016

Evolution of OH and CO-dark Molecular Gas Fraction Across a Molecular Cloud Boundary In Taurus

Duo Xu, Di Li, Nannan Yue +1

We present observations of 12CO J=1-0, 13CO J=1-0, HI, and all four ground-state transitions of the hydroxyl (OH) radical toward a sharp boundary region of the Taurus molecular clo…

astro-ph.HE2023

Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534

Chen-Chen Miao, Victoria Blackmon, Wei-Wei Zhu +41

We report the radio observations of the eclipsing black widow pulsar J1720-0534, a 3.26 ms pulsar in orbit with a low mass companion of mass 0.029 to 0.034 M. We obtain t…

astro-ph.GA2024

Turbulent Diffuse Molecular Media with Non-ideal Magnetohydrodynamics and Consistent Thermochemistry: Numerical Simulations and Dynamic Characteristics

Nannan Yue, Lile Wang, Thomas Bisbas +2

Turbulent diffuse molecular clouds can exhibit complicated morphologies caused by the interactions among radiation, chemistry, fluids, and fields. We performed full 3D simulations…

astro-ph.GA2020

OH Evolution in Molecular Clouds

Ningyu Tang, Di Li, Nannan Yue +7

We have conducted OH 18 cm survey toward 141 molecular clouds in various environments, including 33 optical dark clouds, 98 Planck Galactic cold clumps (PGCCs) and 10 Spitzer dark…

astro-ph.GA2018

A new method to quantify differentiate collapse models of star formation

Nannan Yue, Di Li, Zhiyuan Ren

Continuum emissions from dust grains are used as a general probe to constrain the initial physical conditions of molecular dense cores where new stars may born. To get as much info…

astro-ph.IM2011

The Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project

Rendong Nan, Di Li, Chengjin Jin +6

Five-hundred-meter Aperture Spherical radio Telescope (FAST) is a Chinese mega-science project to build the largest single dish radio telescope in the world. Its innovative enginee…

astro-ph.GA2021

Carbon-chain molecule survey toward four low-mass molecular outflow sources

C. Zhang, Y. Wu, X. -C. Liu +4

We performed a carbon-chain molecule (CCM) survey toward four low-mass outflow sources, IRAS 04181+2655 (I04181), HH211, L1524, and L1598, using the 13.7 m telescope at the Purple…

astro-ph.HE2020

The FAST discovery of an Eclipsing Binary Millisecond Pulsar in the Globular Cluster M92 (NGC 6341)

Zhichen Pan, Scott M. Ransom, Duncan R. Lorimer +13

We report the discovery of an eclipsing binary millisecond pulsar in the globular cluster M92 (NGC6341) with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). PSR J…

astro-ph.GA2025

Tiny-Scale Properties within the Interstellar Medium towards PSR J16444559: I. Observational Evidence of Turbulence-induced Tiny Scale Atomic Structures

Mengting Liu, Di Li, J. R. Dawson +21

We investigated HI absorption toward a single pulsar, PSR J16444559, and its variability over timescales from days to years, using Murriyang, CSIRO's Parkes Radio Telescope. Our…

astro-ph.GA2022

Complex Organic Molecules Formation in Cold Cores on Stochastically Heated Grains

Long-Fei Chen, Qiang Chang, Yao Wang +1

We investigate the roles of stochastic grain heating in the formation of complex organic molecules (COMs) in cold cores, where COMs have been detected. Two different types of grain…

astro-ph.IM2012

The Five-hundred-meter Aperture Spherical Radio Telescope Project and its Early Science Opportunities

Di Li, Rendong Nan, Zhichen Pan

The National Astronomical Observatories, Chinese Academy of Science (NAOC), has started building the largest antenna in the world. Known as FAST, the Five-hundred-meter Aperture Sp…

astro-ph.GA2024

FAST survey of H I and OH absorption towards extragalactic radio sources

Yogesh Chandola, D. J. Saikia, Yin-Zhe Ma +5

Neutral atomic hydrogen and molecular gas in the host galaxies of radio active galactic nuclei (AGN) can be traced using H I 21-cm and OH-1667 MHz absorption lines to understand th…

astro-ph.GA2020

Observations of magnetic fields surrounding LkH 101 taken by the BISTRO survey with JCMT-POL-2

Nguyen Bich Ngoc, Pham Ngoc Diep, Harriet Parsons +146

We report the first high spatial resolution measurement of magnetic fields surrounding LkH 101, a part of the Auriga-California molecular cloud. The observations were taken wit…

astro-ph.GA2020

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP) II. Survey overview: a first look at 1.3 mm continuum maps and molecular outflows

Somnath Dutta, Chin-Fei Lee, Tie Liu +32

Planck Galactic Cold Clumps (PGCCs) are contemplated to be the ideal targets to probe the early phases of star formation. We have conducted a survey of 72 young dense cores inside…

astro-ph.SR2021

HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure

Dennis Lee, Marc Berthoud, Che-Yu Chen +14

We present a study of the relative orientation between the magnetic field and elongated cloud structures for the Oph A and Oph E regions in L1688 in the Ophiuchus molecul…

astro-ph.SR2019

First detection of vibrationally excited Glycolaldehyde in the solar-type protostar IRAS 16293-2422

Yan Zhou, Sheng-Li Qin, Alvaro Sanchez-Monge +7

This paper was withdrawed from the ApJ after the comments from the referee, please be carefully.

astro-ph.IM2024

Polarization Calibration of the FAST L-band 19-beam Receiver: I. On-axis Mueller Matrix Parameters

Tao-Chung Ching, Carl Heiles, Di Li +6

We present the polarization calibration of the 19-beam receiver at 1420 MHz within the full illumination of the Five-hundred-meter Aperture Spherical Telescope from October 2018 to…

astro-ph.HE2022

FAST observations of an extremely active episode of FRB 20201124A: II. Energy Distribution

Yong-Kun Zhang, Pei Wang, Yi Feng +17

We report the properties of more than 800 bursts detected from the repeating fast radio burst (FRB) source FRB 20201124A with the Five-hundred-meter Aperture Spherical radio Telesc…

astro-ph.IM2025

TransientVerse: A Comprehensive Real-Time Alert and Multi-Wavelength Analysis System for Transient Astronomical Events

Jian-Hua Fang, Di Li, Pei Wang +18

Transient astrophysical events are characterized by short timescales, high energy, and multi-wavelength radiation, often accompanied by violent energy releases. These phenomena are…

cond-mat.supr-con2015

Superconductivity in efficient thermoelectric CuSbAlSe

Xiao-Miao Zhao, Yong-Hui Zhou, Qiao-Wei Huang +8

Both superconductivity and thermoelectricity offer promising prospects for daily energy efficiency applications. The advancements of thermoelectric materials have led to the huge i…

astro-ph.GA2025

Constraints on the fractional changes of the fundamental constants at a look-back time of 2.5 Myrs

Renzhi Su, Tao An, Stephen J. Curran +3

The quantum nature of gravity remains one of the greatest mysteries of modern physics, with many unified theories predicting variations in fundamental constants across space and ti…

astro-ph.HE2022

Interstellar scintillation and polarization of PSR B0656+14 in the Monogem Ring

Jumei Yao, William A. Coles, Richard N. Manchester +8

High sensitivity interstellar scintillation and polarization observations of PSR~B0656+14 made at three epochs over a year using the Five-hundred-meter Aperture Spherical radio Tel…

astro-ph.GA2019

The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region

Simon Coudé, Pierre Bastien, Martin Houde +118

We present the POL-2 850 m linear polarization map of the Barnard 1 clump in the Perseus molecular cloud complex from the B-fields In STar-forming Region Observations (BISTRO)…

astro-ph.GA2022

B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main

Woojin Kwon, Kate Pattle, Sarah Sadavoy +149

We present 850 m polarimetric observations toward the Serpens Main molecular cloud obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope (JCMT) as part of t…

astro-ph.GA2017

Widespread Presence of Glycolaldehyde and Ethylene Glycol Around Sagittarius B2

Juan Li, Zhiqiang Shen, Junzhi Wang +10

We report the detection of widespread CHOHCHO and HOCHCHOH emission in Galactic center giant molecular cloud Sagittarius B2 using the Shanghai Tianma 65m Radio Telescop…

astro-ph.GA2025

Imprints of Stellar Feedback on Magnetic Fields in the Iris Nebula NGC 7023

Ekta Sharma, Kate Pattle, Di Li +5

We present 850 m polarized continuum observations carried out with the POL-2 polarimeter mounted on the James Clerk Maxwell Telescope (JCMT) towards NGC 7023 located in the Cep…

astro-ph.SR2020

Rotation of Two Micron All Sky Survey Clumps in Molecular Clouds

Xuefang Xu, Di Li, Y. Sophia Dai +2

We have analyzed the rotational properties of 12 clumps using CO (1--0) and CO (1--0) maps of the Five College Radio Astronomy Observatory 13.7 m radio telescope. The…

cs.CV2026

A3R: Agentic Affordance Reasoning via Cross-Dimensional Evidence in 3D Gaussian Scenes

Di Li, Jie Feng, Guanbin Li +4

Affordance reasoning in 3D Gaussian scenes aims to identify the region that supports the action specified by a given text instruction in complex environments. Existing methods typi…

astro-ph.GA2017

The TOP-SCOPE survey of Planck Galactic Cold Clumps: Survey overview and results of an exemplar source, PGCC G26.53+0.17

Tie Liu, Kee-Tae Kim, Mika Juvela +11

The low dust temperatures (<14 K) of Planck Galactic Cold Clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. TOP-SCOPE i…

astro-ph.GA2016

Discovery of an extremely wide-angle bipolar outflow in AFGL 5142

Tie Liu, Qizhou Zhang, Kee-Tae Kim +12

Most bipolar outflows are associated with individual young stellar objects and have small opening angles. Here we report the discovery of an extremely wide-angle (180$\arcdeg…

cs.CV2025

EgoSplat: Open-Vocabulary Egocentric Scene Understanding with Language Embedded 3D Gaussian Splatting

Di Li, Jie Feng, Jiahao Chen +4

Egocentric scenes exhibit frequent occlusions, varied viewpoints, and dynamic interactions compared to typical scene understanding tasks. Occlusions and varied viewpoints can lead…

astro-ph.GA2024

A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey

Jintai Wu, Keping Qiu, Frederick Poidevin +152

As part of the BISTRO survey, we present JCMT 850 m polarimetric observations towards the Orion Integral-Shaped Filament (ISF) that covers three portions known as OMC-1, OMC-2,…

astro-ph.CO2025

CRAFTS for HI cosmology: I. data processing pipeline and validation tests

Wenxiu Yang, Laura Wolz, Yichao Li +20

We present the calibration procedures and validation of source measurement with the data of the Commensal Radio Astronomy FAST Survey (CRAFTS) for \HI intensity mapping by the Five…

astro-ph.IM2020

Machine Learning for Nanohertz Gravitational Wave Detection and Parameter Estimation with Pulsar Timing Array

MengNi Chen, Yuanhong Zhong, Yi Feng +2

Studies have shown that the use of pulsar timing arrays (PTAs) is among the approaches with the highest potential to detect very low-frequency gravitational waves in the near futur…

astro-ph.SR2014

Characterization of Molecular Outflows in The Substellar Domain

Ngoc Phan-Bao, Chin-Fei Lee, Paul T. P. Ho +2

We report here our latest search for molecular outflows from young brown dwarfs and very low-mass stars in nearby star-forming regions. We have observed three sources in Taurus wit…

astro-ph.HE2023

Sub-second periodic radio oscillations in a microquasar

Pengfu Tian, Ping Zhang, Wei Wang +18

Powerful relativistic jets are one of the ubiquitous features of accreting black holes in all scales. GRS 1915+105 is a well-known fast-spinning black-hole X-ray binary with a rela…

astro-ph.GA2026

SwinYNet: A Transformer-based Multi-Task Model for Accurate and Efficient FRB Search

Yunchuan Chen, Shulei Ni, Chan Li +11

In this study, we present a transformer-based multi-task model for Fast Radio Burst (FRB) detection, signal segmentation, and parameter estimation directly from time-frequency data…

astro-ph.HE2026

Evidence for a Damped Millisecond Quasi-Periodic Structure in a Fast Radio Burst

Shuo Xiao, Zheng-Huo Jiang, Di Li

Fast radio bursts (FRBs) are millisecond-duration transients of unknown origin, likely associated with compact astrophysical objects. We report evidence for a damped millisecond qu…

cs.NI2014

Mobile Adhoc Offloading

Di Li, Asya Mitseva

This problem is a series of biddings and auctions. Each round of bidding and auction are different from previous ones because of the change of network topology, variance of budget…

astro-ph.HE2025

Simultaneous multi-wavelength observations of the repeating fast radio burst FRB 20190520B with Swift and FAST

Zhen Yan, Wenfei Yu, Kim L. Page +8

Among several dozen known repeating Fast radio bursts (FRBs), those precisely localized offer the best opportunities to explore their multi-wavelength counterparts, which are key t…

astro-ph.IM2018

Studies of Turbulence Dissipation in Taurus Molecular Cloud with Core Velocity Dispersion (CVD)

Lei Qian, Di Li, Yang Gao +2

Turbulence dissipation is an important process affecting the energy balance in molecular clouds, the birth place of stars. Previously, the rate of turbulence dissipation is often e…

astro-ph.HE2024

An extremely active repeating fast radio burst source in a likely non-magneto-ionic environment

Yi Feng, Di Li, Yong-Kun Zhang +24

Fast radio bursts (FRBs) are bright radio bursts originating at cosmological distances. Only three repeating FRBs FRB 20121102A, FRB 20190520B and FRB 20201124A among 60 kno…

astro-ph.HE2026

A 44-minute periodic radio transient in a supernova remnant

Di Li, Mao Yuan, Lin Wu +45

Long-period radio transients (LPTs) are a newly discovered class of radio emitters with periods ranging from minutes to hours. The astrophysical nature remains undetermined, partic…

astro-ph.GA2026

Divergent Evolution of Radial Metallicity Gradients in the Thin and Thick Disks of the Milky Way

Weixiang Sun, Gaohuan Long, Hui Li +6

The paper analyzes radial metallicity gradients in the Milky Way's thin and thick disks using over 200,000 red clump stars, finding a strong negative gradient in the thin disk that…

#milky way#galactic disk#metallicity gradients#thin disk
astro-ph.HE2026

Flux Variations of Fast Radio Bursts and Their Persistent Radio Sources: Evidence for a Shared Progenitor

Xinming Li, Chenhui Niu, Jiaheng Zhang +24

Fast radio bursts (FRBs) are millisecond-duration extragalactic radio transients, some of which are associated with compact persistent radio sources (PRSs), hinting at a physical c…

astro-ph.GA2023

HI Self-absorption toward the Cygnus X North: From Atomic Filament to Molecular Filament

Chong Li, Keping Qiu, Di Li +5

Using the HI self-absorption data from the Five-hundred-meter Aperture Spherical radio Telescope (FAST), we perform a study of the cold atomic gas in the Cygnus-X North region. The…

astro-ph.GA2022

Compact and variable radio emission from an active galaxy with supersoft X-ray emission

Lei Yang, Xinwen Shu, Fabao Zhang +15

RX J1301.9+2747 is a unique active galaxy with supersoft X-ray spectrum that lacks significant emission at energies above 2 keV. In addition, it is one of few galaxies displaying q…

astro-ph.IM2020

Readout for Kinetic-Inductance-Detector-Based Submillimeter Radio Astronomy

Ran Duan, MUSIC Team, Xinxin Zhang +2

A substantial amount of important scientific information is contained within astronomical data at the submillimeter and far-infrared (FIR) wavelengths, including information regard…

cs.CV2024

Multi-Teacher Multi-Objective Meta-Learning for Zero-Shot Hyperspectral Band Selection

Jie Feng, Xiaojian Zhong, Di Li +3

Band selection plays a crucial role in hyperspectral image classification by removing redundant and noisy bands and retaining discriminative ones. However, most existing deep learn…

astro-ph.SR2014

IC348-SMM2E: a Class 0 proto-brown dwarf candidate forming as a scaled-down version of low-mass stars

Aina Palau, Luis A. Zapata, Luis F. Rodriguez +7

We report on Submillimeter Array observations of the 870 micron continuum and CO(3-2), 13CO(2-1) and C18O(2-1) line emission of a faint object, SMM2E, near the driving source of th…

astro-ph.HE2025

The magnetar model's energy crisis for a prolific repeating fast radio burst source

Jun-Shuo Zhang, Tian-Cong Wang, Pei Wang +61

Fast radio bursts (FRBs) are widely considered to originate from magnetars that power the explosion through releasing magnetic energy. Active repeating FRBs have been seen to produ…

astro-ph.EP2022

Sensitive Multi-beam Targeted SETI Observations towards 33 Exoplanet Systems with FAST

Zhen-Zhao Tao, Hai-Chen Zhao, Tong-Jie Zhang +19

As a major approach to looking for life beyond the Earth, the search for extraterrestrial intelligence (SETI) is committed to detecting technosignatures such as engineered radio si…

astro-ph.GA2022

The Distribution of UV Radiation Field in the Molecular Clouds of Gould Belt

Jifeng Xia, Ningyu Tang, Qijun Zhi +5

The distribution of ultraviolet (UV) radiation field provides critical constraints on the physical environments of molecular clouds. Within 1 kpc of our solar system and fostering…

astro-ph.GA2018

Low-mass Active Galactic Nuclei on the Fundamental Plane of Black Hole Activity

Lei Qian, Xiao-Bo Dong, Fu-Guo Xie +2

It is widely known that in active galactic nuclei (AGNs) and black hole X-ray binaries (BHXBs), there is a tight correlation among their radio luminosity (), X-ray luminosity…

astro-ph.GA2018

First Data Release of the ESO-ARO Public Survey SAMPLING --- SMT "All-sky" Mapping of PLanck Interstellar Nebulae in the Galaxy

Ke Wang, Sarolta Zahorecz, Maria R. Cunningham +17

We make the first data release (DR1) of the ongoing ESO Public Survey SAMPLING (http://dx.doi.org/10.7910/DVN/0L8NHX). DR1 comprises of 124 fields distributed in $70^\circ < l < 21…

astro-ph.HE2016

Intensity Distribution Function and Statistical Properties of Fast Radio Bursts

LongBiao Li, YongFeng Huang, ZhiBin Zhang +2

Fast Radio Bursts (FRBs) are intense radio flashes from the sky that are characterized by millisecond durations and Jansky-level flux densities. We carried out a statistical analys…

astro-ph.SR2014

Massive Quiescent Cores in Orion: V. The Physical Structures on Sub-Jeans Scale and the Chemical Properties in Two Extremely Dense Cores

Zhiyuan Ren, Di Li, Nicholas Chapman

We present a high-resolution observational study towards two massive dust-and-gas cores, ORI8nw\_2 and ORI2\_6 in Orion Molecular Cloud using the Combined Array for Research…

astro-ph.HE2020

A Fast Radio Burst discovered in FAST drift scan survey

Weiwei Zhu, Di Li, Rui Luo +67

We report the discovery of a highly dispersed fast radio burst, FRB~181123, from an analysis of 1500~hr of drift-scan survey data taken using the Five-hundred-meter Aperture…

astro-ph.IM2022

J-comb: An image fusion algorithm to combine observations covering different spatial frequency ranges

Sihan Jiao, Yuxin Lin, Xiangyu Shui +3

Ground-based, high-resolution bolometric (sub)millimeter continuum mapping observations on spatially extended target sources are often subject to significant missing fluxes. This h…

astro-ph.GA2016

CH as a Molecular Gas Tracer and C-Shock Tracer Across a Molecular Cloud Boundary in Taurus

Duo Xu, Di Li

We present new observations of all three ground-state transitions of the methylidyne (CH) radical and all four ground-state transitions of the hydroxyl (OH) radical toward a sharp…

astro-ph.GA2026

Anomalously high deuterium fractionation in a galactic translucent cloud: a challenge to chemical models

Gan Luo, Zhi-Yu Zhang, Thomas G. Bisbas +8

Deuterated (D-) species have long been proposed to diagnose the physical conditions and chemical evolution of cold dense molecular clouds. While deuterium fractionation has been ex…

astro-ph.GA2025

The HASHTAG project II. Giant molecular cloud properties across the M31 disc

Yikai Deng, Zongnan Li, Zhiyuan Li +17

We present a study of giant molecular cloud (GMC) properties in the Andromeda galaxy (M31) using CO(3-2) data from the James Clerk Maxwell Telescope (JCMT) in selected regions acro…

astro-ph.GA2016

Physical properties of CO-dark molecular gas traced by C

Ningyu Tang, Di Li, Carl Heiles +3

Neither HI nor CO emission can reveal a significant quantity of so-called dark gas in the interstellar medium (ISM). It is considered that CO-dark molecular gas (DMG), the molecula…

astro-ph.GA2012

Is the Taurus B213 Region a True Filament?: Observations of Multiple Cyanoacetylene Transitions

Di Li, Paul F. Goldsmith

We have obtained spectra of the J=2-1 and J=10-9 transitions of cyanoacetylene (\hc3n) toward a collection of positions in the most prominent filament, B213, in the Taurus molecula…

astro-ph.GA2023

-enhanced Astrochemistry: the Carbon cycle in extreme galactic conditions

Thomas G. Bisbas, Zhi-Yu Zhang, Eda Gjergo +8

Astrochemistry has been widely developed as a power tool to probe physical properties of the interstellar medium (ISM) in various conditions of the Milky Way (MW) Galaxy, and in ne…

astro-ph.EP2024

FAST Observations of Four Comets to Search for the Molecular Line Emissions between 1.0 and 1.5 GHz Frequencies

Long-Fei Chen, Chao-Wei Tsai, Jian-Yang Li +11

We used the Five-hundred-meter Aperture Spherical radio Telescope (FAST) to search for the molecular emissions in the L-band between 1.0 and 1.5 GHz toward four comets, C/2020 F3 (…

astro-ph.GA2018

HI Observations of Major-Merger Pairs at z = 0: atomic gas and star formation

Pei Zuo, Cong K. Xu, Min S. Yun +3

We present a study of the HI gas content of a large K-band selected sample of 88 close major-merger pairs of galaxies (H-KPAIR) which were observed by . We obtained t…

astro-ph.GA2018

A First Look at BISTRO Observations of The Oph-A core

Jungmi Kwon, Yasuo Doi, Motohide Tamura +119

We present 850 m imaging polarimetry data of the Oph-A core taken with the Submillimeter Common-User Bolometer Array-2 (SCUBA-2) and its polarimeter (POL-2), as part of ou…

cond-mat.mtrl-sci2017

Chemical reaction directed oriented attachment: from precursor particles to new substances

Yongfei Liu, Xiaoying Qin, Yong Yang +11

The oriented attachment (OA) of nanoparticles is an important mechanism for the synthesis of the crystals of inorganic functional materials, and the formation of natural minerals.…

astro-ph.GA2021

Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetry

Chakali Eswaraiah, Di Li, Ray S. Furuya +142

We have obtained sensitive dust continuum polarization observations at 850 m in the B213 region of Taurus using POL-2 on SCUBA-2 at the James Clerk Maxwell Telescope (JCMT), as…

physics.bio-ph2016

Symmetry and size of membrane protein polyhedral nanoparticles

Di Li, Osman Kahraman, Christoph A. Haselwandter

In recent experiments [T. Basta et al., Proc. Natl. Acad. Sci. U.S.A. 111, 670 (2014)] lipids and membrane proteins were observed to self-assemble into membrane protein polyhedral…

astro-ph.HE2026

A Persistently Active Fast Radio Burst source Embedded in an Expanding Supernova Remnant

Chen-Hui Niu, Di Li, Yuan-Pei Yang +21

Fast radio bursts (FRBs) remain one of the most puzzling astrophysical phenomena. While most FRBs are detected only once or sporadically, we present the identification of FRB 20190…

astro-ph.SR2014

350 m map of the Ophiuchus molecular cloud: core mass function

Guoyin Zhang, Di Li, Ashley K. Hyde +3

Stars are born in dense cores of molecular clouds. The core mass function (CMF), which is the mass distribution of dense cores, is important for understanding the stellar initial m…

astro-ph.GA2021

ALMA observations of NGC 6334S. II. Subsonic and Transonic Narrow Filaments in a High-mass Star Formation Cloud

Shanghuo Li, Patricio Sanhueza, Chang Won Lee +22

We present a study of narrow filaments toward a massive infrared dark cloud, NGC 6334S, using the Atacama Large Millimeter/submillimeter Array (ALMA). Thirteen gas filaments are id…

astro-ph.HE2026

Indication for Decreasing Dispersion Measure in the Population of Repeating Fast Radio Bursts and Connection to Young Supernova Remnant Expansion

Xiang-han Cui, Cheng-min Zhang, Di Li +8

Fast Radio Bursts (FRBs) are millisecond-duration, highly energetic radio transients of uncertain origin. Repeating FRBs provide an excellent population for investigating their nat…

astro-ph.HE2022

Frequency-dependent polarization of repeating fast radio bursts-implications for their origin

Yi Feng, Di Li, Yuan-Pei Yang +23

The polarization of fast radio bursts (FRBs), bright astronomical transients, contains crucial information about their environments. We report polarization measurements of five rep…

astro-ph.IM2016

The Five-hundred-meter Aperture Spherical Radio Telescope (FAST) Project

Di Li, Zhichen Pan

The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is a Chinese mega-science project funded by the National Development and Reform Commission (NDRC) of the People's R…

astro-ph.HE2024

The arrival time and energy of FRBs traverse the time-energy bivariate space like a Brownian motion

Yong-Kun Zhang, Di Li, Yi Feng +5

The origin of fast radio bursts (FRBs), the brightest cosmic explosion in radio bands, remains unknown. We introduce here a novel method for a comprehensive analysis of active FRBs…

astro-ph.CO2025

A stringent constraint on the fractional change of proton g-factor

Renzhi Su, Stephen J. Curran, Jeremy Darling +5

We report a constraint on the cosmological variation of the proton g-factor, . By comparing the measured redshifts between \mbox{H\,{\sc i}} 21 cm and OH 18 cm lines observed…

astro-ph.HE2022

Radio detection of an elusive millisecond pulsar in the Globular Cluster NGC 6397

Lei Zhang, Alessandro Ridolfi, Harsha Blumer +32

We report the discovery of a new 5.78 ms-period millisecond pulsar (MSP), PSR J1740-5340B (NGC 6397B), in an eclipsing binary system discovered with the Parkes radio telescope (now…

astro-ph.SR2015

Sulfur-Bearing Molecules In Massive Star-Forming Regions: Observations Of OCS, CS, H2S and SO

Juan Li, Junzhi Wang, Qingfeng Zhu +2

We studied sulfur chemistry of massive star-forming regions through single-dish submillimeter spectroscopy. OCS, O13CS, 13CS, H2S and SO transitions were observed toward a sample o…

astro-ph.GA2026

The ALMA-QUARKS Survey: Properties of Hot Molecular Fragments in the Massive Protocluster IRAS 17233-3606

Li Chen, Sheng-Li Qin, Dongting Yang +29

To investigate the physical mechanisms of fragmentation within the hot molecular core of the massive protocluster IRAS 17233-3606 (G351.78-0.54), we carried out a detailed analysis…

astro-ph.GA2021

Molecular Cloud Cores with High Deuterium Fractions: Nobeyama Mapping Survey

Ken'ichi Tatematsu, Gwanjeong Kim, Tie Liu +35

We present the results of on-the-fly mapping observations of 44 fields containing 107 SCUBA-2 cores in the emission lines of molecules, NH, HCN, and CCS at 8294 GHz…

astro-ph.GA2016

Cloud Structure of Galactic OB Cluster Forming Regions from Combining Ground and Space Based Bolometric Observations

Yuxin Lin, Hauyu Baobab Liu, Di Li +13

We have developed an iterative procedure to systematically combine the millimeter and submillimeter images of OB cluster-forming molecular clouds, which were taken by ground based…

astro-ph.GA2025

The evolution of CH in Planck Galactic Cold Clumps

Gan Luo, Arshia M. Jacob, Marco Padovani +6

Methylidyne (CH) has long been considered a reliable tracer of molecular gas in the low-to-intermediate extinction range. Although extended CH 3.3 GHz emission is commonly observed…

astro-ph.GA2019

Revealing The CO X-factor In Dark Molecular Gas through Sensitive ALMA Absorption Observations

Gan Luo, Di Li, Ningyu Tang +11

Carbon-bearing molecules, particularly CO, have been widely used as tracers of molecular gas in the interstellar medium (ISM). In this work, we aim to study the properties of molec…

astro-ph.GA2021

A Low-mass Cold and Quiescent Core Population in a Massive Star Protocluster

Shanghuo Li, Xing Lu, Qizhou Zhang +24

Pre-stellar cores represent the initial conditions of star formation. Although these initial conditions in nearby low-mass star-forming regions have been investigated in detail, su…