Yuxuan Zhu

ORCID: 0000-0003-2203-4765
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About
Contact & Profiles
Research Areas
  • Astrophysical Phenomena and Observations
  • Pulsars and Gravitational Waves Research
  • Advanced X-ray Imaging Techniques
  • Gamma-ray bursts and supernovae
  • Particle Detector Development and Performance
  • Astrophysics and Cosmic Phenomena
  • CCD and CMOS Imaging Sensors
  • Calibration and Measurement Techniques
  • X-ray Spectroscopy and Fluorescence Analysis
  • High-pressure geophysics and materials
  • Optical Systems and Laser Technology
  • Biocrusts and Microbial Ecology
  • Tryptophan and brain disorders
  • Mechanics and Biomechanics Studies
  • Nuclear Physics and Applications
  • Algal biology and biofuel production
  • Advanced X-ray and CT Imaging
  • Optical measurement and interference techniques
  • Stress Responses and Cortisol
  • Photosynthetic Processes and Mechanisms
  • Superconducting Materials and Applications
  • Groundwater and Isotope Geochemistry
  • Plant Micronutrient Interactions and Effects
  • Mercury impact and mitigation studies
  • Freshwater macroinvertebrate diversity and ecology

Tianjin Medical University
2024-2025

Tsinghua University
2019-2025

Institute of High Energy Physics
2019-2024

Chinese Academy of Sciences
2019-2024

Institute of Hydrobiology
2021-2023

European Space Agency
2023

Max Planck Institute for Extraterrestrial Physics
2023

Jilin University
2020-2022

University of Chinese Academy of Sciences
2021-2022

Abstract The Follow-up X-ray Telescope (FXT) is one of the two main scientific instruments on board Einstein Probe astronomical satellite, which was launched in 2024 January. FXT focuses energy range 0.3–10 keV and mainly conducts follow-up observations transients burst sources. It consists units completely independent optical system detector (FXT-A FXT-B). focal plane adopts PNCCD provided by Max Planck Institute for Extraterrestrial Physics. designed to have three operating modes with...

10.1088/1538-3873/ad7c7d article EN Publications of the Astronomical Society of the Pacific 2024-10-01

Abstract The 100-m X-ray Test Facility of the Institute High Energy Physics (IHEP) was initially proposed in 2012 for test and calibration detectors Hard Modulation Telescope (HXMT) with capability to support future missions. large instrument chamber connected a long vacuum tube can accommodate mirror, focal plane detector other instruments. sources are installed at end distance 105 m, which provide an almost parallel beam covering 0.2 $$\sim$$ <mml:math...

10.1007/s10686-022-09872-7 article EN cc-by Experimental Astronomy 2022-10-22

The Einstein Probe (EP) is an X-ray astronomical mission mainly devoting to time-domain astronomy. There are two main scientific payloads onboard EP, the Wide Field Telescope (WXT) based on lobster eye optics and Follow-up (FXT). FXT contains Wolter-1 mirrors with a pnCCD detector each focus. total effective area about 600 cm2 energy range 0.3-10 keV. cooled by pulse tube cooler enables high-resolution spectroscopy imaging combined excellent time resolution. It will also have several working...

10.1117/12.2562311 article EN Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray 2020-12-12

Abstract The 100 m long X-ray test facility (100XF for clarity) in Institute of High Energy Physics CAS has been playing an increasingly important role the astronomy field China. 100XF contributing to missions under development, such as Einstein Probe mission. also providing support R&amp;D focusing optics China that will enable future telescopes be realized, enhanced Timing and Polarization (eXTP) A pnCCD-based camera employed at rapidly measure performance optics. In this work, we study...

10.1088/1538-3873/acdf20 article EN Publications of the Astronomical Society of the Pacific 2023-06-01

Periphytic algae exist widely in different waters. However, little is known about periphytic long-distance water diversion channels across watersheds. We investigated the and environmental factors at twenty sampling sites middle route of South-to-North Water Diversion Project (MRP). The dominant species were Desmodesmus intermedius (Hegewald), Calothrix thermalis (Bornet &amp; Flahault), parietina Flahault) Leptolyngbya benthonica (Anagnostidis) (dominance &gt; 0.02) as measured a whole...

10.3390/w14060914 article EN Water 2022-03-15

Astrocytes are the primary cell type in central nervous system, responsible for maintaining stability of brain’s internal environment and supporting neuronal functions. Researches have demonstrated close relationship between astrocytes pathophysiology etiology major depressive disorder. However, regulatory mechanisms during depression remain unclear. The aim this study is to examine alterations calcium signaling dorsal raphe nucleus (DRN), neurons both DRN medial prefrontal cortex (mPFC),...

10.1155/bn/8890705 article EN cc-by Behavioural Neurology 2025-01-01

Abstract The Einstein Probe (EP) mission, launched in 2024 January, is a time-domain X-ray satellite designed to discover and study transient burst sources while investigating electromagnetic counterparts gravitational waves. To achieve precise observations, EP features the Follow-up Telescope (FXT), equipped with two Wolter-I type mirrors for imaging within 1 square degree field of view. A specialized Ray-Tracing package FXT (RTF) was developed assess mirrors’ performance used FXT. By...

10.1088/1538-3873/adc0c0 article EN Publications of the Astronomical Society of the Pacific 2025-04-01

Background Apalutamide is used in the treatment of castration-resistant prostate cancer. A simple, specific, selective, and effective liquid chromatography–tandem mass spectrometry method for quantifying apalutamide its active metabolite concentration human plasma was developed validated according to FDA EMA validation guidelines. Methods total 24 patients diagnosed with desmoplasia-resistant cancer (NM-CRPC) were recruited. Blood samples drawn after 4 weeks’ administration at a dose 180 mg...

10.3389/fphar.2025.1510583 article EN cc-by Frontiers in Pharmacology 2025-05-19

The nested Wolter-I type focusing mirror is widely used in the field of X-ray astronomy. thin-shell mirrors produced by electroforming replication method will introduce various shape errors during fabricating and assembling process. This study introduces a non-analytical 3D geometrical ray tracing algorithm capable predicting optical performance for large deformations. algorithm's implementation involves error reconstruction, light source simulation, calculation. Experimental simulation...

10.1364/oe.497987 article EN cc-by Optics Express 2023-08-24

10.1016/j.nima.2022.166465 article EN Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 2022-02-15

The South-to-North Water Division Middle Route Project (MRP) is currently the longest inter-basin water diversion project in world. It benefits a large population and its quality has attracted much attention. In this study, seasonal investigations on 11 sampling sites along MRP were conducted from 2018 to 2019; temperature, pH, turbidity, transparency, COD Mn , dissolved oxygen, total phosphorus, phosphate, nitrogen, ammonia, nitrate, chlorophyll determined synchronously. Single leakage...

10.3389/fenvs.2023.945884 article EN cc-by Frontiers in Environmental Science 2023-03-20

The Follow-up X-ray Telescope (FXT), a key payload onboard the Einstein Probe sallite (EP), is equipped with Wolter-I x-ray focusing mirror system. We introduce principle of such system and analyze influence gap in multishell nested FXT on effective area, stray-light ratio, vignetting. To ensure that no occlusion occurs within adjacent shells minimize size set to optimized value for corresponding shell. finished design 54-shell according these results. optical performance was then simulated...

10.1117/1.oe.60.2.025102 article EN Optical Engineering 2021-02-13

Abstract CCD236 is a new generation swept charge device (SCD) developed by e2v. It designed for the Low Energy Telescope (LE) onboard Hard X-ray Modulation (HXMT). The spectrum of detector convolution result incident and energy response detector. One can obtain accurate quantities fitting model with response. According to two-dimensional interpolation method, an matrix generated using calibration data obtained low facility located at Institute High Physics. accuracy better than 0.2 eV, full...

10.1088/1748-0221/16/05/p05016 article EN Journal of Instrumentation 2021-05-01
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