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arXiv 2024年

作者： Chen, Michael Chun-Yuan Fissel, Laura M. Sadavoy, Sarah I. Rosolowsky, Erik Doi, Yasuo Arzoumanian, Doris Bastien, Pierre Coudé, Simon Di Francesco, James Friesen, Rachel Furuya, Ray S. Hwang, Jihye Inutsuka, Shu-Ichiro Johnstone, Doug Karoly, Janik Kwon, Jungmi Kwon, Woojin Le Gouellec, Valentin J.M. Liu, Hong-Li Mairs, Steve Onaka, Takashi Pattle, Kate Rawlings, Mark G. Tahani, Mehrnoosh Tamura, Motohide Wang, Jia-Wei Department of Physics Engineering Physics and Astronomy Queen’s University KingstonONK7L 3N6 Canada Department of Physics University of Alberta EdmontonABT6G 2E1 Canada Department of Earth Science and Astronomy The University of Tokyo 3-8-1 Komaba Meguro Tokyo153-8902 Japan National Astronomical Observatory of Japan Osawa 2-21-1 Mitaka Tokyo181-8588 Japan Université de Montréal Département de Physique 1375 Avenue Thérèse-Lavoie-Roux MontréalQCH2V 0B3 Canada Department of Earth Environment and Physics Worcester State University WorcesterMA01602 United States Center for Astrophysics | Harvard & Smithsonian 60 Garden Street CambridgeMA02138 United States NRC Herzberg Astronomy and Astrophysics 5071 West Saanich Rd VictoriaBCV9E 2E7 Canada Department of Physics and Astronomy University of Victoria VictoriaBCV8P 5C2 Canada David A. Dunlap Department of Astronomy and Astrophysics University of Toronto 50 St. George Street TorontoONM5S 3H4 Canada Institute of Liberal Arts and Sciences Tokushima University Minami Jousanajima-machi 1-1 Tokushima770-8502 Japan Korea Astronomy and Space Science Institute 776 Daedeokdae-ro Yuseong-gu Daejeon34055 Korea Republic of University of Science and Technology Korea 217 Gajeong-ro Yuseong-gu Daejeon34113 Korea Republic of Department of Physics Graduate School of Science Nagoya University Furo-cho Chikusa-ku Nagoya464-8602 Japan Jeremiah Horrocks Institute University of Central Lancashire PrestonPR1 2HE United Kingdom Department of Astronomy Graduate School of Science The University of Tokyo 7-3-1 Hongo Bunkyo-ku Tokyo113-0033 Japan Department of Earth Science Education Seoul National University 1 Gwanak-ro Gwanak-gu Seoul08826 Korea Republic of SNU Astronomy Research Center Seoul National University 1 Gwanak-ro Gwanak-gu Seoul08826 Korea Republic of NASA Ames Research Center Space Science and Astrobiology Division M.S. 245-6 Moffett FieldCA94035 United States NASA Postdoc

Magnetic fields play an important role in shaping and regulating star formation in molecular clouds. Here, we present one of the first studies examining the relative orientations between magnetic (B) fields and the dust emission, gas column density, and velocity centroid gradients on the 0.02 pc (core) scales, using the BISTRO and VLA+GBT observations of the NGC 1333 star-forming clump. We quantified these relative orientations using the Project Rayleigh Statistic (PRS) and found preferential global parallel alignment between the B field and dust emission gradients, consistent with large-scale studies with Planck. No preferential global alignments, however, are found between the B field and velocity gradients. Local PRS calculated for subregions defined by either dust emission or velocity coherence further revealed that the Bfield does not preferentially align with dust emission gradients in most emission-defined subregions, except in the warmest ones. The velocity-coherent structures, on the other hand, also showed no preferred B field alignments with velocity gradients, except for one potentially bubble-compressed region. Interestingly, the velocity gradient magnitude in NGC 1333 ubiquitously features prominent ripple-like structures that are indicative of magnetohydrodynamic (MHD) waves. Finally, we found B field alignments with the emission gradients to correlate with dust temperature and anticorrelate with column density, velocity dispersion, and velocity gradient magnitude. The latter two anticorrelations suggest that alignments between gas structures and B fields can be perturbed by physical processes that elevate velocity dispersion and velocity gradients, such as infall, accretions, and MHD waves. © 2024, CC BY.

关键词： Plasma magnetohydrodynamic waves

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The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray properties and scaling relations of galaxy clusters and groups

arXiv

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arXiv 2021年

作者： Bahar, Y. Emre Bulbul, Esra Clerc, Nicolas Ghirardini, Vittorio Liu, Ang Nandra, Kirpal Pacaud, Florian Chiu, I-Non Comparat, Johan Ider-Chitham, Jacob Klein, Mathias Liu, Teng Merloni, Andrea Migkas, Konstantinos Okabe, Nobuhiro Ramos-Ceja, Miriam E. Reiprich, Thomas H. Sanders, Jeremy S. Schrabback, Tim Max Planck Institute for Extraterrestrial Physics Giessenbachstrasse 1 Garching85748 Germany IRAP Université de Toulouse CNRS UPS CNES Toulouse France Universität Bonn Auf dem Hügel 71 Bonn53121 Germany Tsung-Dao Lee Institute Key Laboratory for Particle Physics Astrophysics and Cosmology Ministry of Education Shanghai Jiao Tong University Shanghai200240 China Universitaets-Sternwarte Muenchen Fakultaet fuer Physik LMU Munich Scheinerstr. 1 Munich81679 Germany Physics Program Graduate School of Advanced Science and Engineering Hiroshima University 1-3-1 Kagamiyama Higashi-Hiroshima Hiroshima739-8526 Japan Hiroshima Astrophysical Science Center Hiroshima University 1-3-1 Kagamiyama Higashi-Hiroshima Hiroshima739-8526 Japan Core Research for Energetic Universe Hiroshima University 1-3-1 Kagamiyama Higashi-Hiroshima Hiroshima739-8526 Japan

Context. Scaling relations link the physical properties of clusters at cosmic scales. They are used to probe the evolution of large-scale structure, estimate observables of clusters, and constrain cosmological parameters through cluster counts. Aims. We investigate the scaling relations between X-ray observables of the clusters detected in the eFEDS field using Spectrum-Roentgen-Gamma/eROSITA observations taking into account the selection effects and the distributions of observables with cosmic time. Methods. We extract X-ray observables (LX, Lbol, T, Mgas, YX) within R500 for the sample of 542 clusters in the eFEDS field. By applying detection and extent likelihood cuts, we construct a subsample of 265 clusters with a contamination level of 500 and core-excised 0.15R500 - R500 apertures for 542 galaxy clusters and groups detected in the eFEDS field. Additionally, we present our best-fit results for the normalization, slope, redshift evolution, and intrinsic scatter parameters of the X-ray scaling relations between LX - T, LX - Mgas, LX - YX, Lbol - T, Lbol - Mgas, Lbol - YX, and Mgas - T. We find that the best-fit slopes significantly deviate from the self-similar model at a > 4σ confidence level, but our results are nevertheless in good agreement with the simulations including non-gravitational physics, and the recent results that take into account selection effects. Conclusions. The strong deviations we find from the self-similar scenario indicate that the non-gravitational effects play an important role in shaping the observed physical state of clusters. This work extends the scaling relations to the low-mass, low-luminosity galaxy cluster and group regime using eFEDS observations, demonstrating the ability of eROSITA to measure emission from the intracluster medium out to R500 with survey-depth exposures and constrain the scaling relations in a wide mass–luminosity–redshift range. Copyright © 2021, The Authors. All rights reserved.

关键词： Surveys

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SARS-CoV-2 infections in certain groups: A review from COVID-19 study cases

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AIP Conference Proceedings 2023年第1期2606卷

作者： Muhammad Mumtaz Adzdzakiy Isnaini Zakiyyah Asyifa Alvira Rifdah Sativa Ahmad Ridha Al Fiqri Anik Budhi Dharmayanthi Anggia Prasetyoputri Sugiyono Saputra 1Graduate Program of Bioscience Faculty of Mathematics and Natural Sciences Universitas Sebelas Maret Jl. Ir. Sutami 36A Surakarta Central Java Indonesia 57126 2Master Program in Biomedical Science Faculty of Medicine Universitas Indonesia Jl. Salemba Raya No. 6 Jakarta Indonesia 10430 3School of Life Science and Technology Bandung Institute of Technology Jl. Ganesa 10 Bandung West Java Indonesia 40132 4Research Center for Biology National Research and Innovation Agency (BRIN) Jl. Raya Jakarta Bogor Km 46 Bogor West Java Indonesia 16911 5Research Center for Biotechnology National Research and Innovation Agency (BRIN) Jl. Raya Jakarta Bogor Km 46 Bogor West Java Indonesia 16911

The severe acute respiratory syndrome coronavirus-2 (SARS-CoV-2) has caused the current pandemic of COVID-19 and is highly infectious with relatively high mortality risk. In this study, we reviewed and summarized miscellaneous COVID-19 cases from vulnerable groups, including children and those with comorbidity, reinfections, coinfections and vaccinated individuals, and rapid transmission cases to understand if there are any specific SARS-CoV-2 variants that infect those groups. We concluded that there were no specific variants associated with higher rates of infection within certain groups, rather, they may tend to infect any groups with any immunity levels, regardless of geographical boundaries. A high prevalence of SARS-CoV-2 infection is mainly driven by the ability of viruses with genetic markers that have been associated with higher risks of transmission and immune escape in vulnerable groups. Disease severity is not only influenced by the virus, but also host conditions such as gender, age, comorbidity, and obesity. The likelihood of new emerging SARS-CoV-2 variants resulting from infections in vulnerable groups is high, thus monitoring viral genetic markers and mutations is crucial for outbreak preparedness.

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A therapy game for elementary students with ADHD

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AIP Conference Proceedings 2023年第1期2508卷

作者： Raymond Bahana Edi Abdurachman Ford L. Gaol Tjhin Wiguna Fonny Dameaty Hutagalung Bayu Prakoso Dirgantoro Eko Nugroho 1Computer Science Department BINUS Graduate Program Doctor of Computer Science Bina Nusantara University Jakarta Indonesia 2Faculty of Medicine Universitas Indonesia Depok Indonesia 3Department of Educational Psychology and Counselling Faculty of Education University of Malaya Kuala Lumpur Malaysia 4Graphic Design and New Media Prog. Visual Communication Design Dept. BINUS Northumbria School of Design Bina Nusantara University Jakarta Indonesia 5Kummara Bandung Indonesia

Children with Attention Deficit Hyperactivity Disorder usually have problem to express themselves. Using game as a therapy, they could reduce the problem. A recent study has revealed video games might be an alternative therapy for children with ADHD. This research is to analyze the data that was collected from a prototype game that has been developed and created. The game is created using Construct2. To collect data from the game, back-end web application was created using PHP and MySQL. Several data that have been used in this research paper are score, incorrect house, and incorrect fruit. Ten children with ADHD are involved in this testing, all children are elementary students and never receive any treatment for their ADHD. Before and after the testing, they have been tested by fMRI. The testing consists of 4 weeks of training sessions of about 20-30 minutes almost every day except Sunday or public holiday. Every session contains at least three tutorial or training tasks and four game tasks in a fixed order. In conclusion, the result showed the scores were better when the children with ADHD play with visual instruction rather than with audio instruction.

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The Astrometric Animation of Water Masers towards the Mira Variable BX Cam

arXiv

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arXiv 2022年

作者： Xu, Shuangjing Imai, Hiroshi Yun, Youngjoo Zhang, Bo Rioja, María J. Dodson, Richard Cho, Se-Hyung Kim, Jaeheon Cui, Lang Sobolev, Andrey M. Chibueze, James O. Kim, Dong-Jin Amada, Kei Nakashima, Jun-Ichi Orosz, Gabor Oyadomari, Miyako Oh, Sejin Yonekura, Yoshinori Sun, Yan Mai, Xiaofeng Zhang, Jingdong Wen, Shiming Jung, Taehyun Korea Astronomy and Space Science Institute 776 Daedeok-daero Yuseong-gu Daejeon34055 Korea Republic of Shanghai Astronomical Observatory Chinese Academy of Sciences 80 Nandan Road Shanghai200030 China Graduate School of Science and Engineering Kagoshima University 1-21-35 Korimoto Kagoshima890-0065 Japan Amanogawa Galaxy Astronomy Research Center Graduate School of Science and Engineering Kagoshima University 1-21-35 Korimoto Kagoshima890-0065 Japan Center for General Education Institute for Comprehensive Education Kagoshima University 1-21-30 Korimoto Kagoshima890-0065 Japan ICRAR M468 The University of Western Australia 35 Stirling Hwy CrawleyWA6009 Australia CSIRO Astronomy and Space Science PO Box 1130 BentleyWA6102 Australia Alfonso XII 3 y 5 Madrid28014 Spain Astronomy program Department of Physics and Astronomy Seoul National University Seoul08826 Korea Republic of Republic of Korea Korea Astronomy and Space Science Institute Yuseonggu Daejeon34055 Korea Republic of Xinjiang Astronomical Observatory Chinese Academy of Sciences 150 Science 1-Street Urumqi830011 China Ural Federal University 19 Mira Street Ekaterinburg620002 Russia Centre for Space Research North-West University Potchefstroom2520 South Africa Department of Physics and Astronomy Faculty of Physical Sciences University of Nigeria Carver Building 1 University Road Nsukka Nigeria Massachusetts Institute of Technology Haystack Observatory 99 Millstone Road WestfordMA01886 United States Max-Planck-Institut für Radioastronomie Auf dem Hügel 69 BonnD-53121 Germany School of Physics and Astronomy Sun Yat-sen University 2 Daxue Road Tangjia Guangdong Province Zhuhai China Joint Institute for VLBI ERIC Oude Hoogeveensedijk 4 Dwingeloo7991PD Netherlands Center for Astronomy Ibaraki University 2-1-1 Bunkyo Ibaraki Mito310-8512 Japan Yuquan Rd. Shijingshan Beijing100049 China

We report VLBI monitoring observations of the 22 GHz water (H2O) masers around the Mira variable BX Cam, which were carried out as a part of the EAVN Synthesis of Stellar Maser Animations (ESTEMA) project. Data of 37 epochs in total were obtained from 2018 May to 2021 June with a time interval of 3–4 weeks, spanning approximately three stellar pulsation periods (P =∼440 d). In particular, the dual-beam system equipped on the VERA stations was used to measure the kinematics and parallaxes of the H2O maser features. The measured parallax, π = 1.79 ± 0.08 mas, is consistent with Gaia EDR3 and previously measured VLBI parallaxes within a 1-σ error level. The position of the central star was estimated, based on both the Gaia EDR3 data and the center position of the ring-like 43 GHz silicon-monoxide (SiO) maser distribution imaged with the KVN. The three-dimensional H2O maser kinematics indicates that the circumstellar envelope is expanding at a velocity of 13 ± 4 km s−1, while there are asymmetries in both the spatial and velocity distributions of the maser features. Furthermore, the H2O maser animation achieved by our dense monitoring program manifests the propagation of shock waves in the circumstellar envelope of BX Cam. © 2022, CC BY.

关键词： Stars

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SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 µm and Data Release for the COSMOS Field

arXiv

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arXiv 2024年

作者： Gao, Zhen-Kai Lim, Chen-Fatt Wang, Wei-Hao Chen, Chian-Chou Smail, Ian Chapman, Scott C. Zheng, Xian Zhong Shim, Hyunjin Kodama, Tadayuki Ao, Yiping Chang, Siou-Yu Clements, David L. Dunlop, James S. Ho, Luis C. Hsu, Yun-Hsin Hwang, Chorng-Yuan Hwang, Ho Seong Koprowski, M.P. Scott, Douglas Serjeant, Stephen Toba, Yoshiki Urquhart, Sheona A. No. 1 Section 4 Roosevelt Rd. Taipei10617 Taiwan Graduate Institute of Astronomy National Central University 300 Zhongda Road Zhongli Taoyuan32001 Taiwan Centre for Extragalactic Astronomy Department of Physics Durham University South Road DurhamDH1 3LE United Kingdom Department of Physics and Atmospheric Science Dalhousie University Halifax HalifaxNSB3H 3J5 Canada Purple Mountain Observatory Key Laboratory for Radio Astronomy Chinese Academy of Sciences 10 Yuanhua Road Nanjing210023 China School of Astronomy and Space Science University of Science and Technology of China Anhui Hefei230026 China Department of Earth Science Education Kyungpook National University 80 Daehak-ro Buk-gu Daegu41566 Korea Republic of Astronomical Institute Tohoku University 6-3 Aramaki Aoba Miyagi Sendai980-8578 Japan Institute of Astronomy Department of Physics National Tsing Hua University Hsinchu30013 Taiwan Imperial College London Blackett Laboratory Prince Consort Road LondonSW7 2AZ United Kingdom SUPA Institute for Astronomy University of Edinburgh Royal Observatory EdinburghEH9 3HJ United Kingdom Kavli Institute for Astronomy and Astrophysics Peking University Beijing100871 China Department of Astronomy School of Physics Peking University Beijing100871 China Department of Philosophy National Taiwan University No. 1 Section 4 Roosevelt Rd. Taipei10617 Taiwan Astronomy Program Department of Physics and Astronomy Seoul National University 1 Gwanak-ro Gwanak-gu Seoul08826 Korea Republic of SNU Astronomy Research Center Seoul National University 1 Gwanak-ro Gwanak-gu Seoul08826 Korea Republic of Institute of Astronomy Faculty of Physics Astronomy and Informatics Nicolaus Copernicus University Grudziadzka 5 Torun87-100 Poland Department of Physics and Astronomy University of British Columbia 6224 Agricultural Road VancouverBCV6T 1Z1 Canada School of Physical Sciences The Open University Milton KeynesMK7 6AA United Kingdom

We present confusion-limited SCUBA-2 450-µm observations in the COSMOS-CANDELS region as part of the JCMT Large program, SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). Our maps at 450 and 850 µm cover an area of 450 arcmin2. We achieved instrumental noise levels of σ450 = 0.59 mJy beam−1 and σ850 = 0.09 mJy beam−1 in the deepest area of each map. The corresponding confusion noise levels are estimated to be 0.65 and 0.36 mJy beam−1. Above the 4 (3.5) σ threshold, we detected 360 (479) sources at 450 µm and 237 (314) sources at 850 µm. We derive the deepest blank-field number counts at 450 µm, covering the flux-density range of 2 to 43 mJy. These are in agreement with other SCUBA-2 blank-field and lensing-cluster observations, but are lower than various model counts. We compare the counts with those in other fields and find that the field-to-field variance observed at 450 µm at the R = 6′ scale is consistent with Poisson noise, so there is no evidence of strong 2-D clustering at this scale. Additionally, we derive the integrated surface brightness at 450 µm down to 2.1 mJy to be (Equation presented) Jy deg−2, contributing to (41±4)% of the 450-µm extragalactic background light (EBL) measured by COBE and Planck. Our results suggest that the 450-µm EBL may be fully resolved at (Equation presented) mJy, which extremely deep lensing-cluster observations and next-generation submillimeter instruments with large aperture sizes may be able to achieve. © 2024, CC BY.

关键词： Galaxies

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Identification of single- and double-well coherence-incoherence patterns by the binary distance matrix

arXiv

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arXiv 2022年

作者： dos Santos, Vagner Sales, Matheus Rolim Muni, Sishu Shankar Szezech, José D. Batista, Antonio Marcos Yanchuk, Serhiy Kurths, Jürgen Department of Mathematics and Statistics State University of Ponta Grossa PR Ponta Grossa84030-900 Brazil Ciências Exatas Naturais e Engenharias Centro Universitário UNIFATEB PR Telêmaco Borba84266-010 Brazil Graduate Program in Sciences/Physics State University of Ponta Grossa PR Ponta Grossa84030-900 Brazil Potsdam Institute for Climate Impact Research Leibniz Association P.O. Box 6012 03 PotsdamD-14412 Germany Institute of Mathematics Humboldt University Berlin Berlin12489 Germany Department of Physical Sciences Indian Institute of Science Education and Research Kolkata West Bengal Mohanpur741246 India Institute of Physics Humboldt University Berlin Berlin10099 Germany Division of Dynamics Lodz University of Technology Stefanowskiego 1/15 Lodz90-924 Poland

The study of chimera states or, more generally, coherence-incoherence patterns has led to the development of several tools for their identification and characterization. In this work, we extend the eigenvalue decomposition method to distinguish between single-well and double-well patterns. By applying our method, we are able to identify the following four types of dynamical patterns in a ring of nonlocally coupled Chua circuits and nonlocally coupled cubic maps: single-well cluster, single-well coherence-incoherence pattern, double-well cluster, and double-well coherence-incoherence. In a ring-star network of Chua circuits, we investigate the influence of adding a central node on the spatio-temporal patterns. Our results show that increasing the coupling with the central node favors the occurrence of single-well coherence-incoherence states. We observe that the boundaries of the attraction basins resemble fractal and riddled structures. © 2022, CC BY-NC-SA.

关键词： Timing circuits

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Calycosin Enhances Heat Shock Related-Proteins in H9c2 Cells to Modulate Survival and Apoptosis against Heat Shock

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The American journal of Chinese medicine 2024年第4期52卷 1173-1193页

作者： Pei-Fang Lai Ramasamy Mahendran Bruce Chi-Kang Tsai Cheng-You Lu Chia-Hua Kuo Kuan-Ho Lin Shang-Yeh Lu Yu-Ling Wu Yung-Ming Chang Wei-Wen Kuo Chih-Yang Huang Department of Emergency Medicine Hualien Tzu Chi Hospital Buddhist Tzu Chi Medical Foundation Hualien 970 Taiwan. Department of Medicine Tzu Chi University Hualien 970 Taiwan. Cardiovascular and Mitochondrial Related Disease Research Center Hualien Tzu Chi Hospital Buddhist Tzu Chi Medical Foundation Hualien 970 Taiwan. Department of Post-Baccalaureate Medicine College of Medicine National Chung Hsing University Taichung 402 Taiwan. Laboratory of Exercise Biochemistry University of Taipei Taipei 111 Taiwan. Institute of Sports Sciences University of Taipei Taipei 111 Taiwan. School of Physical Education and Sports Science Soochow University Suzhou 215021 China. Department of Kinesiology and Health College of William and Mary Williamsburg VA 23185 USA. Department of Emergency Medicine China Medical University Hospital Taichung 404 Taiwan. College of Medicine China Medical University Taichung 406 Taiwan. Division of Cardiovascular Medicine Department of Internal Medicine China Medical University Hospital Taichung 404 Taiwan. The School of Chinese Medicine for Post-Baccalaureate I-Shou University 840 Kaohsiung Taiwan. Chinese Medicine Department E-DA Hospital Kaohsiung 824 Taiwan. 1PT Biotechnology Co. Ltd. Taichung 433 Taiwan. Department of Biological Science and Technology College of Life Sciences China Medical University Taichung 406 Taiwan. Ph.D. Program for Biotechnology Industry China Medical University Taichung 406 Taiwan. School of Pharmacy China Medical University Taichung 406 Taiwan. Graduate Institute of Biomedical Sciences China Medical University Taichung 406 Taiwan. Department of Medical Laboratory Science and Biotechnology Asia University Taichung 413 Taiwan. Center of General Education Buddhist Tzu Chi Medical Foundation Tzu Chi University of Science and Technology Hualien 970 Taiwan. Department of Medical Research China Medical University Hospital China Medical University Taichung 404 Taiwan.

Heat shock proteins (HSPs), which function as chaperones, are activated in response to various environmental stressors. In addition to their role in diverse aspects of protein production, HSPs protect against harmful protein-related stressors. Calycosin exhibits numerous beneficial properties. This study aims to explore the protective effects of calycosin in the heart under heat shock and determine its underlying mechanism. H9c2 cells, western blot, TUNEL staining, flow cytometry, and immunofluorescence staining were used. The time-dependent effects of heat shock analyzed using western blot revealed increased HSP expression for up to 2[Formula: see text]h, followed by protein degradation after 4[Formula: see text]h. Hence, a heat shock damage duration of 4[Formula: see text]h was chosen for subsequent investigations. Calycosin administered post-heat shock demonstrated dose-dependent recovery of cell viability. Under heat shock conditions, calycosin prevented the apoptosis of H9c2 cells by upregulating HSPs, suppressing p-JNK, enhancing Bcl-2 activation, and inhibiting cleaved caspase 3. Calycosin also inhibited Fas/FasL expression and activated cell survival markers (p-PI3K, p-ERK, p-Akt), indicating their cytoprotective properties through PI3K/Akt activation and JNK inhibition. TUNEL staining and flow cytometry confirmed that calycosin reduced apoptosis. Moreover, calycosin reversed the inhibitory effects of quercetin on HSF1 and Hsp70 expression, illustrating its role in enhancing Hsp70 expression through HSF1 activation during heat shock. Immunofluorescence staining demonstrated HSF1 translocation to the nucleus following calycosin treatment, emphasizing its cytoprotective effects. In conclusion, calycosin exhibits pronounced protective effects against heat shock-induced damages by modulating HSP expression and regulating key signaling pathways to promote cell survival in H9c2 cells.

关键词： Astragalus Membranaceus Calycosin Cardiomyocyte Heart Protection Heat Shock Heat Shock-Related Protein

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Upcycling waste polyethylene terephthalate (PET) bottles into high-performance activated carbon for electrochemical desalination

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Chemosphere 2024年 364卷 143029页

作者： Jhen-Cih Wu Jui-Yao Chang Xiangzhou Yuan Eakalak Khan Yong Sik Ok Chia-Hung Hou Graduate Institute of Environmental Engineering National Taiwan University No. 1 Sec. 4 Roosevelt Road Taipei 10617 Taiwan. Korea Biochar Research Center APRU Sustainable Waste Management Program & Division of Environmental Science and Ecological Engineering Korea University Seoul 02841 South Korea Ministry of Education of Key Laboratory of Energy Thermal Conversion and Control School of Energy and Environment Southeast University Nanjing 210096 China. Department of Civil and Environmental Engineering and Construction University of Nevada Las Vegas Las Vegas NV 89154 USA. Korea Biochar Research Center APRU Sustainable Waste Management Program & Division of Environmental Science and Ecological Engineering Korea University Seoul 02841 South Korea. Electronic address: yongsikok@korea.ac.kr. Graduate Institute of Environmental Engineering National Taiwan University No. 1 Sec. 4 Roosevelt Road Taipei 10617 Taiwan Research Center for Future Earth National Taiwan University No. 1 Sec. 4. Roosevelt Rd. Taipei 10617 Taiwan. Electronic address: chiahunghou@ntu.edu.tw.

Upcycling waste polyethylene terephthalate (PET) bottles has attracted intensive research interests. This simultaneously alleviates plastic pollution and achieves a waste-to-resource strategy. Waste PET water bottles were used to fabricate value-added activated carbon (AC) electrodes for capacitive deionization (CDI). The KOH activation temperature (greater than 700 °C) prominently affected the physi-chemical properties and desalination performance of PET-derived activated carbons (PET-AC). Profiting from a large Brunauer-Emmet-Teller specific surface area (1448 m g) with a good mesoporous structure (the ratio of the mesopore volume to the total pore volume was 41.3%), PET-AC-1000 (activated at 1000 °C) possessed a huge specific capacitance of 108 F g for capacitive ion storage. Moreover, when utilized as the electrode material in single-pass CDI, PET-AC-1000 exhibited a maximum electrosorption capacity of 10.82 ± 0.11 mg g and a low level of energy consumption (0.07 kWh mol), associated with good electrochemical charging-discharging cyclic stability. The results provide a promising facile approach to tackle the challenge of plastic pollution and promote the advancement of electrode materials for economic affordable and energy-efficient electrochemical desalination process, which meets the United Nations (UN) sustainable development goals (SDGs).

关键词： Activated carbon Capacitive deionization Circular economy Polyethylene terephthalate waste Sustainable development goals 6 (SDG6) Clean water and sanitation

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JASMINE: Near-Infrared Astrometry and Time Series Photometry science

arXiv

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arXiv 2023年

作者： Kawata, Daisuke Kawahara, Hajime Gouda, Naoteru Secrest, Nathan J. Kano, Ryouhei Kataza, Hirokazu Isobe, Naoki Ohsawa, Ryou Usui, Fumihiko Yamada, Yoshiyuki Graham, Alister W. Pettitt, Alex R. Asada, Hideki Baba, Junichi Bekki, Kenji Dorland, Bryan N. Fujii, Michiko Fukui, Akihiko Hattori, Kohei Hirano, Teruyuki Kamizuka, Takafumi Kashima, Shingo Kawanaka, Norita Kawashima, Yui Klioner, Sergei A. Kodama, Takanori Koshimoto, Naoki Kotani, Takayuki Kuzuhara, Masayuki Levine, Stephen E. Majewski, Steven R. Masuda, Kento Matsunaga, Noriyuki Miyakawa, Kohei Miyoshi, Makoko Morihana, Kumiko Nishi, Ryoichi Notsu, Yuta Omiya, Masashi Sanders, Jason Tanikawa, Ataru Tsujimoto, Masahiro Yano, Taihei Aizawa, Masataka Arimatsu, Ko Biermann, Michael Boehm, Celine Chiba, Masashi Debattista, Victor P. Gerhard, Ortwin Hirabayashi, Masayuki Hobbs, David Ikenoue, Bungo Izumiura, Hideyuki Jordi, Carme Kohara, Naoki Löffler, Wolfgang Luri, Xavier Mase, Ichiro Miglio, Andrea Mitsuda, Kazuhisa Newswander, Trent Nishiyama, Shogo Obuchi, Yoshiyuki Ootsubo, Takafumi Ouchi, Masami Ozaki, Masanobu Perryman, Michael Prusti, Timo Ramos, Pau Read, Justin I. Rich, R. Michael Schönrich, Ralph Shikauchi, Minori Shimizu, Risa Suematsu, Yoshinori Tada, Shotaro Takahashi, Aoi Tatekawa, Takayuki Tatsumi, Daisuke Tsujimoto, Takuji Tsuzuki, Toshihiro Urakawa, Seitaro Uraguchi, Fumihiro Utsunomiya, Shin Van Eylen, Vincent van Leeuwen, Floor Wada, Takehiko Walton, Nicholas A. National Astronomical Observatory of Japan 2-21-1 Osawa Mitaka Tokyo181-8588 Japan Mullard Space Science Laboratory University College London Holmbury St. Mary Dorking SurreyRH5 6NT United Kingdom Institute of Space and Astronautical Science Japan Aerospace Exploration Agency 3-1-1 Yoshinodai Chuo-ku Kanagawa Sagamihara252-5210 Japan Astronomical Science Program Graduate Institute for Advanced Studies SOKENDAI 2-21-1 Osawa Mitaka Tokyo181-1855 Japan U.S. Naval Observatory 3450 Massachusetts Ave NW WashingtonDC20392-5420 United States Department of Physics Kyoto University Kitashirakawa-oiwake-cho Sakyo-ku Kyoto606-8502 Japan Centre for Astrophysics and Supercomputing Swinburne University of Technology HawthornVIC3122 Australia Department of Physics and Astronomy California State University Sacramento 6000 J Street SacramentoCA95819-6041 United States Graduate School of Science and Technology Hirosaki University Aomori036-8561 Japan Graduate School of Science and Engineering Kagoshima University 1-21-35 Korimoto Kagoshima890-0065 Japan International Centre for Radio Astronomy Research The University of Western Australia 7 Fairway CrawleyWA6009 Australia Department of Astronomy Graduate School of Science The University of Tokyo 7-3-1 Hongo Bunkyo-ku Tokyo113-0033 Japan Department of Earth and Planetary Science Graduate School of Science The University of Tokyo 7-3-1 Hongo Bunkyo-ku Tokyo113-0033 Japan Institute of Statistical Mathematics 10-3 Midoricho Tachikawa Tokyo190-8562 Japan Astrobiology Center 2-21-1 Osawa Mitaka Tokyo181-8588 Japan Institute of Astronomy Graduate School of Science The University of Tokyo 2-21-1 Osawa Mitaka Tokyo181-0015 Japan Center for Gravitational Physics and Quantum Information Yukawa Institute for Theoretical Physics Kyoto University Kitashirakawa-oiwake-cho Sakyo-ku Kyoto606-8502 Japan Cluster for Pioneering Research RIKEN 2-1 Hirosawa Saitama Wako351-0198 Japan Lohrmann Observ

Japan Astrometry Satellite Mission for INfrared Exploration (JASMINE) is a planned M-class science space mission by the Institute of Space and Astronautical science, the Japan Aerospace Exploration Agency. JASMINE has two main science goals. One is the Galactic archaeology with Galactic Center Survey, which aims to reveal the Milky Way's central core structure and formation history from Gaia-level (∼25 µas) astrometry in the Near-Infrared (NIR) Hw-band (1.0-1.6 µm). The other is the Exoplanet Survey, which aims to discover transiting Earth-like exoplanets in the habitable zone from NIR time-series photometry of M dwarfs when the Galactic center is not accessible. We introduce the mission, review many science objectives, and present the instrument concept. JASMINE will be the first dedicated NIR astrometry space mission and provide precise astrometric information of the stars in the Galactic center, taking advantage of the significantly lower extinction in the NIR. The precise astrometry is obtained by taking many short-exposure images. Hence, the JASMINE Galactic center survey data will be valuable for studies of exoplanet transits, asteroseismology, variable stars and microlensing studies, including discovery of (intermediate mass) black holes. We highlight a swath of such potential science, and also describe synergies with other missions. © 2023, CC BY.

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