Xue Li

ORCID: 0009-0002-8819-8017
Publications
Citations
Views
---
Saved
---
About
Contact & Profiles
Research Areas
  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Photonic Crystals and Applications
  • Photonic and Optical Devices
  • Astrophysics and Cosmic Phenomena
  • Astro and Planetary Science
  • Dyeing and Modifying Textile Fibers
  • Pulsars and Gravitational Waves Research
  • Auction Theory and Applications
  • Dark Matter and Cosmic Phenomena
  • Astronomical Observations and Instrumentation
  • Magnetic properties of thin films
  • Particle physics theoretical and experimental studies
  • Structural Engineering and Vibration Analysis
  • Adaptive optics and wavefront sensing
  • Advanced Semiconductor Detectors and Materials
  • Soil, Finite Element Methods
  • Semiconductor Quantum Structures and Devices
  • Energy, Environment, Agriculture Analysis
  • Engineering Applied Research
  • Quantum optics and atomic interactions
  • Supply Chain and Inventory Management
  • Galaxies: Formation, Evolution, Phenomena

Tsinghua University
2008-2025

Shenzhen University
2025

Wuhan Textile University
2022-2023

Beijing Foreign Studies University
2022-2023

University of Chinese Academy of Sciences
2007-2022

Beijing Academy of Quantum Information Sciences
2022

Nanjing University of Aeronautics and Astronautics
2022

Shenyang University of Technology
2022

Institute of Physics
2022

Chinese Academy of Sciences
2021-2022

The Korea Invisible Mass Search (KIMS) experiment presents new limits on the weakly interacting massive particle (WIMP)-nucleon cross section using data from an exposure of 3409 kg·d taken with low-background CsI(Tl) crystals at Yangyang Underground Laboratory. most stringent limit spin-dependent interaction for a pure proton case is obtained. DAMA signal region both spin-independent and interactions WIMP masses greater than 20 GeV/c2 excluded by single crystal scintillators.Received 3 April...

10.1103/physrevlett.99.091301 article EN Physical Review Letters 2007-08-28

SARS-CoV (the SARS-Associated Coronavirus) was reported as a novel virus member in the coronavirus family, which cause of severe acute respiratory syndrome. Coronavirus replication occurs through unique mechanism employing Leader sequence transcripts when initiating transcription from genome. Therefore, we cloned SARS-CoV(BJ01), is identical to that identified SARS-CoV(HKU-39849), and constructed specific siRNA targeting sequence. Using EGFP RFP reporter genes fused with sequence,...

10.1038/sj.gt.3302479 article EN other-oa Gene Therapy 2005-03-17

On 2018 Feb. 4.41, the All-Sky Automated Survey for SuperNovae (ASAS-SN) discovered ASASSN-18bt in K2 Campaign 16 field. With a redshift of z=0.01098 and peak apparent magnitude B_{max}=14.31, is nearest brightest SNe Ia yet observed by Kepler spacecraft. Here we present discovery ASASSN-18bt, light curve, pre-discovery data from ASAS-SN Asteroid Terrestrial-impact Last Alert System (ATLAS). The early-time curve has an unprecedented 30-minute cadence photometric precision SN~Ia it...

10.3847/1538-4357/aaec79 article EN The Astrophysical Journal 2018-12-28

Abstract Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically confirmed Type Ia supernova (SN Ia) observed in Kepler field. The data revealed an excess emission its early light curve, allowing us to place interesting constraints on progenitor system. Here we present extensive optical, ultraviolet, and near-infrared photometry, as well dense sampling of optical spectra, for this object. SN relatively normal photometric evolution, with a rise time 18.3 ± 0.3 days Δ m 15 ( B ) =...

10.3847/1538-4357/aaec74 article EN The Astrophysical Journal 2018-12-28

Abstract Larch trees are widely used in afforestation and timber plantations. Yet, little is known on how planted larch cope with increasing drought. We a tree-ring network of 818 from 31 plantations spanning most the distribution Larix principis-rupprechtii to investigate extreme drought influences radial growth northern China. found that summer drought, rather than temperature or precipitation, had strongest relationship throughout region. Drought increased frequency recent decades,...

10.1088/1748-9326/abd214 article EN cc-by Environmental Research Letters 2020-12-10

We present our photometric and spectroscopic observations on the peculiar transient AT2018cow. The multi-band photometry covers from peak to $\sim$70 days spectroscopy ranges 5 $\sim$50 days. rapid rise ($t_{\mathrm{r}}$$\lesssim$2.9 days), high luminosity ($M_{V,\mathrm{peak}}\sim-$20.8 mag) fast decline after make AT2018cow stand out of any other optical transients. While we find that its light curves show resemblance those type Ibn supernovae. Moreover, spectral energy distribution...

10.3847/1538-4357/abdeba article EN The Astrophysical Journal 2021-03-01

ABSTRACT Background Cachexia is a wasting syndrome associated with imbalanced energy metabolism and loss of adipose muscle tissues contributes to morbidity mortality in ageing as well patients severe chronic diseases, including cancer. At present, there are no treatments addressing cachexia that have reached validation be used the clinic. In this study, we investigate protective role SIRT6, an important regulator homeostasis health preservation, against Lewis lung carcinoma (LLC)–induced...

10.1002/jcsm.13734 article EN cc-by Journal of Cachexia Sarcopenia and Muscle 2025-02-01

We aim to participate in the calibration of X-ray photon count rate halo mass scaling relation galaxy clusters selected first eROSITA All-Sky Survey on western Galactic hemisphere (eRASS1) using weak-lensing (WL) data from fourth release Kilo-Degree (KiDS-1000) . therefore measured radial shear profiles around eRASS1 background galaxies KiDS-1000 as well cluster member contamination. Furthermore, we provide consistency checks with other stage-III surveys that take part Dark Energy Year 3...

10.1051/0004-6361/202449599 article EN cc-by Astronomy and Astrophysics 2025-02-25

Near-infrared II (NIR-II) microscopy, which enables in vivo deep-tissue visualization of vasculature and cell activities, has been a promising tool for understanding physiological mechanisms. However, the volumetric image speed current NIR-II microscopy is hindered by scanning strategy, causing limitations observing instantaneous biological dynamics 3D space. Here, we developed light-field (LFM) based on selective illumination self-supervised implicit neural representation...

10.1101/2025.03.16.643569 preprint EN bioRxiv (Cold Spring Harbor Laboratory) 2025-03-17

Despite cisplatin has been widely used in the treatment of various cancers, noteworthy nephrotoxicity greatly constrained its clinical value. For this reason, finding novel targeted therapies to attenuate should be pretty significant. Our previous study found that histone deacetylase sirtuin 6 (SIRT6) could an ideal target for cisplatin-induced acute kidney injury. In study, we explored protective effects ellagic acid, a natural polyphenol compound activates SIRT6, on nephrotoxicity....

10.1016/j.fshw.2023.03.043 article EN cc-by-nc-nd Food Science and Human Wellness 2023-04-05

ABSTRACT SN 2018hti is a Type I superluminous supernova (SLSN I) with an absolute g-band magnitude of −22.2 at maximum brightness, discovered by the Asteroid Terrestrial-impact Last Alert System in metal-poor galaxy redshift 0.0612. We present extensive photometric and spectroscopic observations this supernova, covering phases from ∼−35 d to more than +340 r-band maximum. Combining our BVgri-band photometry Swift UVOT optical/ultraviolet photometry, we calculated peak luminosity as ∼3.5 ×...

10.1093/mnras/staa1918 article EN Monthly Notices of the Royal Astronomical Society 2020-07-03

Tsinghua University-Ma Huateng Telescopes for Survey (TMTS), located at Xinglong Station of NAOC, has a field view upto 18 deg^2. The TMTS started to monitor the LAMOST sky areas since 2020, with uninterrupted observations lasting about 6 hours on average each area and cadence 1 minute. Here we introduce data analysis preliminary scientific results first-year observations, which covered 188 plates ( 1970 deg^2). These have generated over 4.9 million light curves, least 100 epochs them....

10.1093/mnras/stab2812 article EN Monthly Notices of the Royal Astronomical Society 2021-09-30

Time-domain (TD) spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) can provide accurate and high-cadence radial velocities (RVs). In this work, we search for binaries with compact components RV monitoring method by using LAMOST TD survey of four $K$2 plates. Three binary systems including an unseen white dwarf or neutron star are found. For each system, estimate stellar parameters visible orbital parameters, finally calculate mass function minimum...

10.3847/1538-4357/ac8f29 article EN cc-by The Astrophysical Journal 2022-10-01

Structural coloration as the most possible way to realize ecofriendly dying process for textiles or fabrics has attracted significant attention in past decades. However, photonic crystals (PCs) are a typical example of materials with structural color usually located on surface textiles, which make them not stable when rubbed, bent, washed due weak interaction between PC coatings and fabrics. Here, double networks were constructed first time via hydrogen bond by introducing tannic acid (TA)...

10.1021/acsami.2c20581 article EN ACS Applied Materials & Interfaces 2023-02-07

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through first 180 days. does not show signs of narrow, high-ionization emission lines in early optical spectra, yet lightcurve evolution suggests that an extra energy source circumstellar medium (CSM) interaction must be for at least 2 days explosion. Modeling indicates a ~500R$_{\odot}$ progenitor radius, consistent with rather compact red...

10.3847/1538-4357/ab43e3 article EN The Astrophysical Journal 2019-11-01

Little is known about the diversity in light curves of GRB-SNe, including whether curve SN 1998bw can be used as a representative template or there luminosity-decline rate relation akin to that SNe Ia. In this paper, we aim obtain well-constrained GRB-SNe without assumption empirical parametric templates and investigate peak brightness correlates with other parameters such shape time peak. We select eight redshift range 0.0085 0.606, which are firmly associated GRBs. The these well sampled...

10.48550/arxiv.1407.3506 preprint EN other-oa arXiv (Cornell University) 2014-01-01

We investigate the temperature dependence of $g$ factor in two-dimensional (2D) ferromagnet ${\mathrm{CrSiTe}}_{3}$ by combining three-dimensional vector-ferromagnetic resonance (FMR) experiments. It is shown from angular that dramatic shift near critical originates interplay enhanced magnetic fluctuations and anisotropic spin interactions 2D magnetism. The crossover isotropic to for $T\ensuremath{\rightarrow}{T}_{c}$ yields anomalously parallel pumped excitations. In regime, field...

10.1103/physrevb.106.054427 article EN Physical review. B./Physical review. B 2022-08-22

We report estimates of the cosmological parameters $\Omega_m$ and $\Omega_{\Lambda}$ obtained using supernovae (SNe) associated with gamma-ray bursts (GRBs) at redshifts up to 0.606. Eight high-fidelity GRB-SNe well-sampled light curves across peak are used. correct their magnitudes for a luminosity-decline rate relation turn them into accurate standard candles dispersion $\sigma = 0.18$ mag. also estimate peculiar velocity low-redshift host galaxy SN 1998bw, constrained simulations. In flat...

10.1088/2041-8205/796/1/l4 article EN The Astrophysical Journal Letters 2014-10-31

ABSTRACT We present optical and ultraviolet photometry, as well spectra, for the type II supernova (SN) 2015bf. Our observations cover phases from ∼2 to ∼200 d after explosion. The first spectrum is characterized by a blue continuum with blackbody temperature of ∼24 000 K flash-ionized emission lines. After about 1 week, spectra SN 2015bf evolve like those regular II. From luminosity narrow component H α, we deduce that mass-loss rate larger than ${\sim}3.7\times 10^{-3}\, {\rm M_\odot \,...

10.1093/mnras/stab1550 article EN Monthly Notices of the Royal Astronomical Society 2021-05-26

Time delays of gravitationally lensed sources can be used to constrain the mass model a deflector and determine cosmological parameters. We here present an analysis time-delay distribution multiply imaged behind 17 strong lensing galaxy clusters with well-calibrated models. find that for time less than 1000 days, at z = 3.0, their logarithmic probability functions are well represented by P(log Δt) 5.3 × 10−4Δt/M2502, 0.77, where M250 is projected cluster inside 250 kpc (in 1014M☉), power-law...

10.1088/1475-7516/2012/11/015 article EN Journal of Cosmology and Astroparticle Physics 2012-11-07

Structural colored aramid fabric with bright colors and good photocatalytic properties was constructed.

10.1039/d2sm01373h article EN Soft Matter 2022-12-14
Coming Soon ...