7,943 results on '"Mao, M"'
Search Results
2. Steering linkage topology design using angle-based block partitioning symmetric model (APSM)
- Author
-
Xu, W. L., He, Z. C., Mao, M., Li, Eric, and Chen, Y. J.
- Published
- 2024
- Full Text
- View/download PDF
3. The Role of the TRPV4 Channel in Intestinal Physiology and Pathology
- Author
-
Liu D, Mao M, Liu W, Xie L, Zhong X, Cao W, and Chen L
- Subjects
trpv4 ,intestinal diseases ,gastrointestinal motility ,sensory transduction ,Pathology ,RB1-214 ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Dandan Liu,1,* Mingli Mao,1,* Wenjia Liu,1 Lihua Xie,1 Xiaolin Zhong,1 Wenyu Cao,2 Ling Chen1 1Department of Metabolism and Endocrinology, The First Affiliated Hospital of University of South China, Hengyang Medical School, University of South China, Hengyang, Hunan, 421001, People’s Republic of China; 2Clinical Anatomy & Reproductive Medicine Application Institute, Hengyang Medical School, University of South China, Hengyang, Hunan, 421001, People’s Republic of China*These authors contributed equally to this workCorrespondence: Ling Chen, The First Affiliated Hospital of University of South China, Department of Endocrinology and Metabolism, Hengyang Medical School, University of South China, Hengyang, Hunan, 421001, People’s Republic of China, Email lingchen-cl@outlook.comAbstract: The transient receptor potential vanilloid 4 channel (TRPV4) is an important member of the TRP superfamily of cation channels. The channel can be activated by different physical and chemical stimuli, such as heat, osmotic, and mechanical stress. It regulates the release of nociceptive peptides (substance P and calcitonin gene-related peptide), and mediates neurogenic inflammation, which indicates the involvement of TRPV4 as a nociceptor. Previous studies show that TRPV4 regulates the contraction of intestinal smooth muscle, mucosal barrier permeability, intestinal ion transport, activation of submucosal enteric neurons, and generation of immune cells. TRPV4 is involved in various pathophysiological activities, and altered TRPV4 expression has been detected in some intestinal diseases (IBD, IBS, intestinal tumors, etc). Evidence indicates that TRPV4 plays a noxious role in intestinal barrier function when the intestine is damaged. This review focuses on the role of the TRPV4 channel in the physiological and pathological functions of the intestine, and evaluates the potential clinical significance to target TRPV4 channel in the treatment of intestinal diseases.Plain Language Summary: TRPV4 is expressed in the intestine and regulates intestinal functions, such as intestinal barrier function, gastrointestinal motility, sensory transduction, and intestinal ion transport. It is upregulated in most intestinal disease models and participates as a negative regulator. TRPV4 inhibition is a potential treatment for intestinal diseases. TRPV4 antagonists also show a positive protective effect on intestinal related diseases. The activation or inhibition of TRPV4 in the treatment of different intestinal diseases has put forward a feasible research direction in the future.Keywords: TRPV4, intestinal diseases, gastrointestinal motility, sensory transduction
- Published
- 2024
4. Effective Dose of Epidural Hydromorphone for Analgesia Following Caesarean Section in Using Modified Dixon Sequential Method
- Author
-
Liu QQ, Mao M, Lin NH, Xu CY, Li Q, Jiang CS, Feng SW, and Yuan HM
- Subjects
key words:hydromorphone ,ropivacaine ,caesarean delivery ,postoperative analgesia ,ed50 ,ed90 ,Medicine (General) ,R5-920 - Abstract
Qiao-Qiao Liu,1,* Mao Mao,1,* Ning-Hua Lin,2,* Chen-Yang Xu,1,* Qian Li,1 Chang-Shuo Jiang,1 Shan-Wu Feng,1 Hong-Mei Yuan1 1Department of Anesthesiology, Women’s Hospital of Nanjing Medical University, Nanjing Women and Children’s Healthcare Hospital, Nanjing, 210004, People’s Republic of China; 2Department of Anesthesiology, Nanjing Drum Tower Hospital, The Affiliated Hospital of Nanjing University Medical School, Nanjing, 210008, People’s Republic of China*These authors contributed equally to this workCorrespondence: Shan-Wu Feng; Hong-Mei Yuan, Department of Anesthesiology, Women’s Hospital of Nanjing Medical University, Nanjing Women and Children’s Healthcare Hospital, No. 123, Tianfei Lane, Mochou Road, Nanjing, Jiangsu, People’s Republic of China, Email Shanwufeng666@163.com; yuanhm667@126.comBackground: A single dose of epidural hydromorphone has been suggested as an alternative method for providing analgesia after caesarean section (CS). Nevertheless, the optimal dosage of epidural hydromorphone for postoperative pain relief following CS has yet to be determined.Methods: This trial included 30 singleton primiparous women undergoing scheduled caesarean delivery, who were recruited to determine doses of epidural hydromorphone using the modified Dixon sequential method. The initial hydromorphone dose was 0.75 mg, with adjustments based on the efficacy of the preceding participant’s dose over 12 hours. Various parameters such as blood pressure, heart rate, respiratory rate, visual analog scale (VAS) pain score, postoperative adverse reactions, and patient satisfaction with analgesic effect were recorded at each time point. The VAS scores were categorized as positive (score > 3) or negative (score ≤ 3). Participants received a single epidural injection of 0.2% ropivacaine 20 mg along with a study dose of hydromorphone. The median effective dose (ED50), 90% effective dose (ED90), and corresponding 95% confidence intervals (CIs) of hydromorphone with ropivacaine for analgesia after caesarean section were calculated using the probit method.Results: The ED90 and ED50 in our population were 1.105 mg (95% CI: 0.825– 2.324 mg) and 0.659 mg (95% CI: 0.434– 0.883 mg), respectively.Conclusion: Epidural hydromorphone can be safely used for postoperative analgesia in patients undergoing caesarean section, and the analgesic effect is satisfactory when the dosage is appropriate.Keywords: hydromorphone, ropivacaine, caesarean delivery, postoperative analgesia, ED50, ED90
- Published
- 2024
5. Sivelestat Sodium Alleviates Ischemia-Reperfusion-Induced Acute Kidney Injury via Suppressing TLR4/Myd88/NF-κB Signaling Pathway in Mice
- Author
-
Wang J, Wu Y, Mao M, Bing H, Sun L, Xu W, Tian W, Xia Z, Jin X, and Chu Q
- Subjects
neutrophil elastase ,ischemia reperfusion injury ,renal dysfunction ,inflammation ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Jie Wang,1 Yuanbo Wu,2 Meng Mao,3 Hailong Bing,1 Liwei Sun,1 Wei Xu,1 Wangli Tian,1 Zhengyuan Xia,4,5 Xiaogao Jin,1,6 Qinjun Chu1 1Department of Anesthesiology and Perioperative Medicine, Zhengzhou Central Hospital Affiliated to Zhengzhou University, Zhengzhou, People’s Republic of China; 2Department of Anesthesiology, Hubei Cancer Hospital, Wuhan, Hubei, People’s Republic of China; 3Center for Advanced Medicine, Zhengzhou Central Hospital Affiliated to Zhengzhou University, Zhengzhou, 450007, People’s Republic of China; 4Department of Anesthesiology, The First Affiliated Hospital, Jinan University, Guangzhou, People’s Republic of China; 5Department of Anesthesiology, The University of Hong Kong, Hong Kong; 6Department of Anesthesiology, The Second Affiliated Hospital of Guangdong Medical University, Zhanjiang, People’s Republic of ChinaCorrespondence: Xiaogao Jin; Qinjun Chu, Email jinxiaoagao@zzu.edu.cn; jimmynetchu@163.comPurpose: We aim to detect the effects of sivelestat on renal ischemia-reperfusion associated with AKI and also explore the underlying mechanism.Materials and Methods: Mice, aged between 8 and 12 weeks, were randomly allocated among four distinct groups, respectively normal saline sham group(C), normal saline surgery group(I), sivelestat (50 mg/kg) sham group(S), sivelestat (50 mg/kg) surgery group(SI) (n=6, each group). In the surgical groups, the renal pedicles of mice were clamped with non-traumatic micro-aneurysm clamps, resulting in ischemia of the kidneys for 45 minutes. This was followed by a period of reperfusion lasting 24 hours. Sham group mice underwent the identical surgery produced without clamping renal pedicles. Mice blood was obtained from eyeballs, and Serum creatinine and blood urea nitrogen levels were measured. After a 24-hour period of reperfusion, the mice were euthanized, and their kidneys were gathered for various analyses, including Western Blot (WB) analysis, RT-PCR, immunofluorescence (IF), hematoxylin and eosin (H&E) staining, and Tunel assay.Results: Pretreatments with sivelestat decreased renal Neutrophil elastase (NE), serum creatinine, and blood urea nitrogen levels after renal ischemia-reperfusion. Sivelestat also reduced histological damage and cell apoptosis in kidneys following ischemia-reperfusion injury (IRI). In addition, the sivelestat administration diminished the levels of mRNA expression of interleukin 6 (IL-6), Macrophage inflammatory protein-2 (MIP-2), monocyte chemoattractant protein-1 (MCP-1), and tumor necrosis factor (TNF)-α in the kidneys during IRI. The kidney tissues of the SI group had significantly mitigated TLR4, Myd88, and NF-κB p-p65 protein expression levels compared to the I group (all P< 0.05).Conclusion: We demonstrated a previously unidentified mechanism that sivelestat effectively attenuates AKI-induced renal dysfunction, possibly through suppressing the TLR4/Myd88/ NF-κB pathway.Keywords: neutrophil elastase, ischemia reperfusion injury, renal dysfunction, inflammation
- Published
- 2024
6. Characterization of ST15-KL112 Klebsiella pneumoniae Co-Harboring Blaoxa-232 and rmtF in China
- Author
-
Hou B, Zhou Y, Wang W, Shen W, Yu Q, Mao M, Wang S, Ai W, Yu F, and Shao P
- Subjects
blaoxa-232 ,rmtf ,klebsiella pneumoniae ,carbapenemase ,plasmid ,Infectious and parasitic diseases ,RC109-216 - Abstract
Bailong Hou,1,* Ying Zhou,2,* Wei Wang,1 Weifeng Shen,1 Qinlong Yu,1 Minjie Mao,1 Siheng Wang,1 Wenxiu Ai,3 Fangyou Yu,2,3 Pingyang Shao1 1Department of Clinical Laboratory Medicine, The First Hospital of Jiaxing, The Affiliated Hospital of Jiaxing University, Jiaxing, 314000, People’s Republic of China; 2Department of Clinical Laboratory Medicine, Shanghai Pulmonary Hospital, Tongji University School of Medicine, Shanghai, 200000, People’s Republic of China; 3Department of Clinical Laboratory, The First Affiliated Hospital of Wenzhou Medical University, Wenzhou, 325000, People’s Republic of China*These authors contributed equally to this workCorrespondence: Pingyang Shao, Department of Clinical Laboratory Medicine, The First Hospital of Jiaxing, The Affiliated Hospital of Jiaxing University, Jiaxing, 314000, People’s Republic of China, Email spy202001@163.com Fangyou Yu, Department of Clinical Laboratory Medicine, Shanghai Pulmonary Hospital, Tongji University School of Medicine, Shanghai, 200000, People’s Republic of China, Email wzjxyfy@163.comIntroduction: This study aimed to investigate the emergence and characteristics of carbapenem-resistant Klebsiella pneumoniae (CRKP) strains that demonstrate resistance to multiple antibiotics, including aminoglycosides and tigecycline, in a Chinese hospital.Methods: A group of ten CRKP strains were collected from the nine patients in a Chinese hospital. Antimicrobial Susceptibility Testing (AST) and phenotypic inhibition assays precisely assess bacterial antibiotic resistance. Real-time quantitative PCR (RT-qPCR) was used to analyze the mRNA levels of efflux pump genes (acrA/acrB and oqxA/oqxB) and the regulatory gene (ramA). The core-genome tree and PFGE patterns were analyzed to assess the clonal and horizontal transfer expansion of the strains. Whole-genome sequencing was performed on a clinical isolate of K. pneumoniae named Kpn20 to identify key resistance genes and antimicrobial resistance islands (ARI).Results: The CRKP strains showed high resistance to carbapenems, aminoglycosides (CLSI, 2024), and tigecycline (EUCAST, 2024). The mRNA expression levels of efflux pump genes and regulatory genes were detected by RT-qPCR. All 10 isolates had significant differences compared to the control group of ATCC13883. The core-genome tree and PFGE patterns revealed five clusters, indicating clonal and horizontal transfer expansion. Three key resistance genes (blaoxa-232, blaCTX-M-15, and rmtF) were observed in the K. pneumoniae clinical isolate Kpn20. Mobile antibiotic resistance islands were identified containing blaCTX-M-15 and rmtF, with multiple insertion sequences and transposons present. The coexistence of blaoxa-232 and rmtF in a high-risk K. pneumoniae strain was reported. Conjugation assay was utilized to investigate the transferability of blaoxa-232-encoding plasmids horizontally.Conclusion: The study highlights the emergence of ST15-KL112 high-risk CRKP strains with multidrug resistance, including to aminoglycosides and tigecycline. The presence of mobile ARI and clonal and horizontal transfer expansion of strains indicate the threat of transmission of these strains. Future research is needed to assess the prevalence of such isolates and develop effective control measures.Keywords: blaOXA-232, rmtF, Klebsiella pneumoniae, carbapenemase, plasmid
- Published
- 2024
7. Efficacy and Safety of Kuoxin Formula in the Treatment of Dilated Cardiomyopathy-Related Heart Failure: Study Protocol of a Randomized, Double-Blind, Placebo-Controlled, Multi-Center Clinical Trial
- Author
-
Wu Q, An S, Lee R, Gao D, Zhou Y, Peng L, Hu C, Yao L, Zhou C, Zhou L, Gao J, Cao M, Mao M, Li G, Deng B, Xu Y, and Wang Y
- Subjects
dilated cardiomyopathy ,heart failure ,kuoxin formula ,traditional chinese medicine ,clinical trials ,Medicine (General) ,R5-920 - Abstract
Qiong Wu,1,* Shiying An,1,* RueyJyh Lee,1 Dongwen Gao,2 Yinyifan Zhou,1 Longping Peng,1 Chunrui Hu,1 Lei Yao,3 Chang Zhou,4 Li Zhou,5 Junjie Gao,6 Min Cao,1 Meijiao Mao,1 Guanghao Li,1 Bing Deng,1 Yingjia Xu,4 Youhua Wang1 1Department of Cardiology, Longhua Hospital Affiliated to Shanghai University of Traditional Chinese Medicine, Shanghai, People’s Republic of China; 2Department of Ultrasound, Longhua Hospital affiliated to Shanghai University of Traditional Chinese Medicine, Shanghai, People’s Republic of China; 3Department of Cardiology, Yueyang Hospital of Integrated Traditional Chinese and Western Medicine Affiliated to Shanghai University of Traditional Chinese Medicine, Shanghai, People’s Republic of China; 4Department of Cardiology, Shanghai Fifth People’s Hospital Affiliated to Fudan University, Shanghai, People’s Republic of China; 5Department of Cardiology, Shanghai Jiading Nanxiang Hospital, Shanghai, People’s Republic of China; 6Department of Cardiology, Shuguang Hospital Affiliated to Shanghai University of Traditional Chinese Medicine, Shanghai, People’s Republic of China*These authors contributed equally to this workCorrespondence: Yingjia Xu, Shanghai Fifth People’s Hospital, Fudan University, Minhang District, 128 Ruili Road, Shanghai, 200240, People’s Republic of China, Tel +862164308151, Email xuyingjia@5thhospital.com Youhua Wang, Department of cardiology, Longhua Hospital affiliated to Shanghai University of Traditional Chinese Medicine, Xunhui, 725 South Wan-Ping Road, Shanghai, 200032, People’s Republic of China, Tel +862164385700, Email doctorwyh@163.comBackground: Dilated cardiomyopathy (DCM) is a severe heterogeneous cardiomyopathy characterized by cardiac enlargement and declining heart function, often leading to refractory heart failure and life-threatening outcomes, particularly prevalent in China. The challenge lies in the scarcity of targeted therapies with substantial efficacy for DCM. Additionally, traditional anti-heart failure drugs are constrained due to hypotension propensity or limited symptom improvement. Kuoxin Formula (KXF), internally endorsed at Longhua Hospital, demonstrates clear biological evidence for enhancing cardiac function and myocardial remodeling. Previous clinical studies suggest its potential to enhance patients’ quality of life. This trial aims to further evaluate KXF’s safety and efficacy in managing DCM-related heart failure.Methods: This prospective, randomized, double-blind, placebo-controlled, multicenter trial aims to recruit 230 DCM patients from five centers. Participants will be randomly assigned to either KXF or placebo for 12 weeks, with careful monitoring of key indicators and adverse events. The primary outcome measures the proportion of patients with NT-proBNP reduction exceeding 30%. Secondary outcomes include New York Heart Association functional classification, Traditional Chinese Medicine syndrome scores, 6-minute walk test, Lee’s heart failure score, and Minnesota Heart Failure Quality of Life Scale score. Ventricular remodeling will be assessed using cardiac ultrasound and ELISA. Safety metrics and adverse events will be meticulously recorded.Discussion: This study will be the first multicentered research conducted in China that utilizes a randomized, double-blind, placebo-controlled design to investigate the use of TCM in the treatment of DCM. It seeks to develop new theoretical frameworks and provide solid clinical data to support the integration of TCM and modern medicine in treating heart failure in DCM patients.Trial Registration: China Clinical Trial Registry, ChiCTR2300068937. Registered on March 1, 2023. https://www.chictr.org.cn/bin/project/edit?pid=190926.Keywords: dilated cardiomyopathy, heart failure, Kuoxin Formula, traditional Chinese medicine, clinical trials
- Published
- 2024
8. Standardizing a method for functional assessment of neural networks in brain organoids
- Author
-
Oliva, MK, Bourke, J., Kornienko, D., Mattei, C., Mao, M., Kuanyshbek, A., Ovchinnikov, D., Bryson, A., Karle, TJ, Maljevic, S., and Petrou, S.
- Published
- 2024
- Full Text
- View/download PDF
9. Research Trends and Hot Spots of Allopregnanolone Research in the Last 20 Years: A Bibliometric Analysis
- Author
-
Guo K, Mao M, Zhang S, Xu S, Zhao L, Wang X, and Feng S
- Subjects
allopregnanolone ,vosviewer ,citespace ,bibliometric analysis ,research trend ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Kunlin Guo,* Mingjie Mao,* Susu Zhang, Shiqin Xu, Liping Zhao, Xian Wang, Shanwu Feng Department of Anesthesiology, Women’s Hospital of Nanjing Medical University, Nanjing Maternity and Child Health Care Hospital, Nanjing, Jiangsu Province, People’s Republic of China*These authors contributed equally to this workCorrespondence: Xian Wang; Shanwu Feng, Department of Anesthesiology, Women’s Hospital of Nanjing Medical University, Nanjing Maternity and Child Health Care Hospital, No. 123, Mochou Road, Tianfei Lane, Nanjing, Jiangsu Province, 210004, People’s Republic of China, Tel +86-25-13770723174 ; +86-25-13921426351, Fax +82-25-52226530, Email wangxian2002@126.com; iamfsw@163.comBackground: Allopregnanolone is a kind of neuroactive steroid or neurosteroid in the central nervous system that acts as an endogenenous GABAA receptor positive modulator. However, at present, no comprehensive bibliometric analysis regarding allopregnanolone research is available. In our study, we intend to analyze the research trends and hot spots related to allopregnanolone in the past 20 years.Methods: We searched for allopregnanolone related articles and reviews between 2004 and 2023 from the Web of Science Core Collection database. Then, the bibliometric analysis was conducted using VOSviewer, CiteSpace, Microsoft Excel 2019, as well as the online bibliometric analysis platform (http://bibliometric.com/).Results: A total of 1841 eligible publications were identified. The number of annual publications and citations was generally on the rise. Among countries, the United States ranked first in overall publications, citations, international cooperation, and the number of research institutions. The University of North Carolina was the most active institution, conducting numerous preclinical and clinical work that focusing on allopregnanolone treatment for diverse psychiatric or neurologic disorders. As for authors, Dr. Frye CA, Morrow AL, and Pinna G were identified as the top three prolific scholars due to their great publications and citations. Based on the publication clusters and citation bursts analysis, the keyword co-occurrence network, the strongest citation bursts, and co-cited references analysis, the hot spots in recent years included “depression”, “postpartum depression”, “GABAA receptor”, and so on.Conclusion: Allopregnanolone is still a popular area of research, and the United States leads the way in this area. Dr. Frye CA, Morrow AL, Pinna G, and their teams contributed greatly to the mechanism study and translation study of allopregnanolone. The use of allopregnanolone for the treatment of psychiatric or neurologic disorders, especially postpartum depression, is the current hot spot. However, the underlying mechanisms of anti-depression are still not clear, deserving more in-depth research.Keywords: allopregnanolone, VOSviewer, CiteSpace, bibliometric analysis, research trend
- Published
- 2023
10. Patterns of Drug Resistance and Bacterial Pathogen Distribution in Patients with Urinary Tract Infections in the Jiaxing Region from 2020 to 2022
- Author
-
Niu X, Hou B, Yang L, Wang W, Yu Q, Mao M, and Shen W
- Subjects
antibiotic resistance ,urinary tract infections ,pathogenic bacteria ,urine culture ,Infectious and parasitic diseases ,RC109-216 - Abstract
Xiaoqin Niu, Bolong Hou, Lunyun Yang, Wei Wang, Qinlong Yu, Minjie Mao, Weifeng Shen Department of Clinical Laboratory, The First Hospital of Jiaxing, The Affiliated Hospital of Jiaxing University, Jiaxing, 314000, People’s Republic of ChinaCorrespondence: Weifeng Shen, Department of Clinical Laboratory, The First Hospital of Jiaxing, The Affiliated Hospital of Jiaxing University, No. 1882, Zhonghuan South Road, Nanhu District, Jiaxing, Zhejiang, 314000, People’s Republic of China, Tel +86-18868345828, Email jyzhy526@163.comBackground: Urinary tract infections (UTIs) and the antibiotic resistance of pathogenic bacteria pose severe threats to public health in the current healthcare environment.Objective: The purpose of this study was to assess the frequency distribution of bacterial pathogens causing UTIs as well as the characteristics of antibiotic susceptibility and resistance.Methods: The retrospective study was conducted on 32,391 samples of midstream urine culture from January 1, 2020, to December 31, 2022, in Jiaxing. Bacteria were cultivated on blood agar and identified using MALDI-TOF, and their susceptibility to different antibiotics was assessed using the Kirby-Bauer disk diffusion method and drug sensitivity reaction cards. The SPSS 22 software was used for data analysis. Bivariate logistic regression was used to analyze the risk factors for multidrug resistance.Results: The total number of positive growth samples was 5378 (16.6%), including 3206 females (59.6%) and 2172 males (40.4%). The four most common urinary pathogens were Escherichia coli (39.2%), Enterococcus faecalis (12.4%), Klebsiella pneumoniae (7.6%), and Enterococcus faecium (7.6%). As far as antibiotic resistance was concerned, Escherichia coli had a greater than 50% resistance rate to ampicillin (76.1%), ciprofloxacin (58.6%), and levofloxacin (51.2%). The multidrug resistance rate was high (41.8%). Low levels of resistance were seen to ertapenem (0.1%), imipenem (0.7%), meropenem (0.7%), piperacillin/tazobactam (0.7%), and nitrofurantoin (1.8%). Klebsiella pneumoniae was highly sensitive to ertapenem (100%). The resistance rates to nitrofurantoin, ceftriaxone, and ciprofloxacin were 37.4%, 37.1%, and 35.1%, respectively. Up to 41% of Escherichia coli strains and 26% of Klebsiella pneumoniae strains produced extended-spectrum lactamases (ESBL). Two species of enterococci were highly sensitive to tigecycline and linezolid (100%), and a small number of norvancomycin-resistant strains (0.2%/two strains) were found.Conclusion: Escherichia coli and Enterococcus faecium were the most common urinary pathogens in this study. The isolated pathogens showed different sensitivity patterns. Antibiotics should be selected reasonably according to the sensitivity mode of pathogenic bacteria to effectively treat and prevent urinary tract infections.Keywords: antibiotic resistance, urinary tract infections, pathogenic bacteria, urine culture
- Published
- 2023
11. BONE MARROW-DERIVED MESENCHYMAL STEM CELL THERAPY IN CHRONIC KIDNEY DISEASE: AN EARLY PHASE CLINICAL TRIAL
- Author
-
Elhusseiny, K., primary, Alatta, L., additional, Snow, Z.K., additional, Skaff, C., additional, Yin, M., additional, Aslam, N., additional, Porter, I., additional, Mao, M., additional, Trautman, C., additional, Baker, L., additional, Manohar, S., additional, Chebib, F., additional, Lorenz, E., additional, and Hickson, L., additional
- Published
- 2024
- Full Text
- View/download PDF
12. Refining the origins of the gamma-ray binary 1FGL J1018.6-5856
- Author
-
Marcote, B., Ribó, M., Paredes, J. M., Mao, M. Y., and Edwards, P. G.
- Subjects
Astrophysics - High Energy Astrophysical Phenomena - Abstract
Gamma-ray binaries are systems composed of a massive star and a compact object that exhibit emission from radio to very high energy gamma rays. They are ideal laboratories to study particle acceleration and a variety of physical processes that vary as a function of the orbital phase. We aim to study the radio emission of the gamma-ray binary 1FGL J1018.6-5856 to constrain the emitting region and determine the peculiar motion of the system within the Galaxy to clarify its origin by analyzing an observation with the Australian Long Baseline Array at 8.4~GHz. We combined these data with the optical Gaia DR2 and UCAC4 catalogs to consolidate the astrometry information therein. 1FGL J1018.6-5856 shows compact radio emission ($< 3$ mas or $\lesssim 20$ au at $\sim 6.4$ kpc distance), implying a brightness temperature of $\gtrsim 5.6 \times 10^6$ K, and confirming its nonthermal origin. We report consistent results between the proper motion reported by Gaia DR2 and the positions obtained from the Gaia, UCAC4, and LBA data. We also determined the distance to 1FGL J1018.6-5856 to be $6.4_{-0.7}^{+ 1.7}$ kpc. Together with the radial velocity of the source we computed its three-dimensional proper and peculiar motion within the Galaxy. We obtained a peculiar motion on its regional standard of rest (RSR) frame of $|u| = 45_{-9}^{+30}$ km s$^{-1}$, with the system moving away from the Galactic plane. In the simplest scenario of a symmetric stellar core collapse we estimate a mass loss of $ 4 \lesssim \Delta M \lesssim 9$ M$_{\odot}$ during the creation of the compact object. 1FGL J1018.6-5856 exhibits compact radio emission similar to that detected in other gamma-ray binaries. We provide the first accurate peculiar motion estimations of the system and place it within the Galaxy. The obtained motion and distance excludes its physical relation with the supernova remnant G284.3-1.8., Comment: 8 pages, 7 figures, Accepted for publication by A&A
- Published
- 2018
- Full Text
- View/download PDF
13. A subarcsecond near-infrared view of massive galaxies at z > 1 with Gemini Multiconjugate Adaptive Optics
- Author
-
Lacy, M., Nyland, K., Mao, M., Jagannathan, P., Pforr, J., Ridgway, S. E., Afonso, J., Farrah, D., Guarnieri, P., Gonzales-Solares, E., Jarvis, M. J., Maraston, C., Nielsen, D. M., Petric, A. O., Sajina, A., Surace, J. A., and Vaccari, M.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
We present images taken using the Gemini South Adaptive Optics Imager (GSAOI) with the Gemini Multiconjugate Adaptive Optics System (GeMS) in three 2 arcmin$^2$ fields in the Spitzer Extragalactic Representative Volume Survey. These GeMS/GSAOI observations are among the first $\approx 0.1^{''}$ resolution data in the near-infrared spanning extragalactic fields exceeding $1.5^{\prime}$ in size. We use these data to estimate galaxy sizes, obtaining results similar to those from studies with the Hubble Space Telescope, though we find a higher fraction of compact star forming galaxies at $z>2$. To disentangle the star-forming galaxies from active galactic nuclei (AGN), we use multiwavelength data from surveys in the optical and infrared, including far-infrared data from Herschel, as well as new radio continuum data from the Australia Telescope Compact Array and Very Large Array. We identify ultraluminous infrared galaxies (ULIRGs) at $z \sim 1-3$, which consist of a combination of pure starburst galaxies and Active Galactic Nuclei (AGN)/starburst composites. The ULIRGs show signs of recent merger activity, such as highly disturbed morphologies and include a rare candidate triple AGN. We find that AGN tend to reside in hosts with smaller scale sizes than purely star-forming galaxies of similar infrared luminosity. Our observations demonstrate the potential for MCAO to complement the deeper galaxy surveys to be made with the James Webb Space Telescope., Comment: 20 pages, AJ, in press
- Published
- 2018
- Full Text
- View/download PDF
14. Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [CI]
- Author
-
Emonts, B. H. C., Lehnert, M. D., Dannerbauer, H., De Breuck, C., Villar-Martin, M., Miley, G. K., Allison, J. R., Gullberg, B., Hatch, N. A., Guillard, P., Mao, M. Y., and Norris, R. P.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
The circumgalactic medium (CGM) of the massive Spiderweb Galaxy, a conglomerate of merging proto-cluster galaxies at z=2.2, forms an enriched interface where feedback and recycling act on accreted gas. This is shown by observations of [CI], CO(1-0) and CO(4-3) performed with the Atacama Large Millimeter Array (ALMA) and Australia Telescope Compact Array (ATCA). [CI] and CO(4-3) are detected across ~50 kpc, following the distribution of previously detected low-surface-brightness CO(1-0) across the CGM. This confirms our previous results on the presence of a cold molecular halo. The central radio galaxy MRC1138-262 shows a very high global $L'_{\rm CO(4-3)}$/$L'_{\rm CO(1-0)}$ ~ 1, suggesting that mechanisms other than FUV-heating by star formation prevail at the heart of the Spiderweb Galaxy. Contrary, the CGM has $L'_{\rm CO(4-3)}$/$L'_{\rm CO(1-0)}$ and $L'_{\rm [CI]}$/$L'_{\rm CO(1-0)}$ similar to the ISM of five galaxies in the wider proto-cluster, and its carbon abundance, $X_{\rm [CI]}$/$X_{\rm H2}$, resembles that of the Milky Way and starforming galaxies. The molecular CGM is thus metal-rich and not diffuse, confirming a link between the cold gas and in-situ star formation. Thus, the Spiderweb Galaxy grows not directly through accretion of gas from the cosmic web, but from recycled gas in the GCM., Comment: Accepted for publication as a Letter in MNRAS (5 pages, 4 figures)
- Published
- 2018
- Full Text
- View/download PDF
15. Palmitate Induces Mitochondrial Energy Metabolism Disorder and Cellular Damage via the PPAR Signaling Pathway in Diabetic Cardiomyopathy
- Author
-
Zhang X, Mao M, and Zuo Z
- Subjects
diabetic cardiomyopathy ,lipotoxicity ,mitochondrial energy metabolism ,cell ,Specialties of internal medicine ,RC581-951 - Abstract
Xianyu Zhang, Min Mao, Zhong Zuo Department of Cardiology, The First Affiliated Hospital of Chongqing Medical University, Chongqing, 400016, People’s Republic of ChinaCorrespondence: Zhong Zuo, Department of Cardiology, The First Affiliated Hospital of Chongqing Medical University, No. 1, Medical College Road, Yuzhong District, Chongqing, 400016, People’s Republic of China, Email zuozhong@hospital.cqmu.edu.cnPurpose: To establish an in vitro lipotoxicity model with mouse cardiomyocytes (MCMs) and investigate the molecular mechanism of the peroxisome proliferator-activated receptors (PPAR) signaling on mitochondrial energy metabolism disorder and cellular injury in diabetic cardiomyopathy (DCM).Methods: Gene ontology (GO) and Kyoto Encyclopedia of Genes and Genomes (KEGG) analyses were performed on the differentially expressed genes (DEGs) of DCM. CCK-8 method was used to detect the proliferation inhibition effect of palmitate (PA) on MCMs. Oil red O staining and mRNA levels of CD36 were used to verify intracellular lipid accumulation. DCFH-DA method was used to determine the content of intracellular reactive oxygen species (ROS), and ATP levels were detected by the ATP Detection Kit. Transmission electron microscope (TEM) was used to observe the mitochondrial structure. Western blot was used to detect the expression levels of PPARα, PPARγ, P-mTOR, mTOR, PGC-1α, UCP2, and BNP. In addition, the expression of PPARγ was also detected by cellular immunofluorescence staining. BNP levels were detected by qRT-PCR and the ELISA Kit.Results: KEGG pathway analysis combined with GO analysis has shown that PPAR signaling played a significant regulatory role in mitochondrial biogenesis and fatty acid metabolism in DCM. Then, MCMs stimulated with PA for 24 h were selected as an in vitro lipotoxicity model. PA decreased cell viability, cell membrane shrinkage, and lipid accumulation. Meanwhile, PA-induced increase in cellular ROS led to ATP generation reduction and mitochondrial damage. Furthermore, the expression levels of p-mTOR- PPARα/γ were decreased, and the expressions of PGC-1α and UCP2 were increased. The levels of BNP were elevated, demonstrating PA impaired cardiomyocytes.Conclusion: Mitochondrial energy metabolism obstacle and cell injury appeared in cardiac lipotoxicity of DCM, associated with lipid accumulation and increased ROS, indicating a crosstalk with the PPAR pathway mediated mechanism.Keywords: diabetic cardiomyopathy, lipotoxicity, mitochondrial energy metabolism, cell damage, PPAR
- Published
- 2022
16. Survival Risk Analysis of Small Cell Lung Cancer Patients with Pre-Existing Type 2 Diabetes Mellitus: A Single-Center Retrospective Cohort Study
- Author
-
Ding J, Li X, Ge J, Gong Y, Zhou Y, Xiao J, Yang Q, Chen J, and Mao M
- Subjects
type 2 diabetes mellitus ,small cell lung cancer ,distant metastasis ,insulin ,overall survival ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Abstract
Jing Ding,1 Xudong Li,1 Jun Ge,1 Yuanqian Gong,1 Ya Zhou,1 Juan Xiao,1 Qin Yang,2 Jing Chen,1 Mian Mao3 1Department of Medical Oncology, Sichuan Cancer Hospital & Institute, Sichuan Cancer Center, School of Medicine, University of Electronic Science and Technology of China, Chengdu, Sichuan, People’s Republic of China; 2Department of Oncology, Bazhong Central Hospital, Bazhong, Sichuan, People’s Republic of China; 3Department of Pharmacy, Sichuan Cancer Hospital & Institute, Sichuan Cancer Center, School of Medicine, University of Electronic Science and Technology of China, Chengdu, Sichuan, People’s Republic of ChinaCorrespondence: Mian Mao, Tel/Fax +86-28-85420311, Email maokefei_0703@163.comPurpose: We aimed to investigate the clinicopathological characteristics and survival risk factors in small cell lung cancer (SCLC) patients with preexisting type 2 diabetes mellitus (preDM).Patients and Methods: All patients with SCLC admitted to our hospital between January 2013 and August 2018 were followed up until August 2020 and retrospectively analyzed. Clinical characteristics of SCLC patients with and without preDM were extracted. Cox proportional hazards models were conducted to identify potential independent prognostic factors.Results: Of 628 eligible individuals, 88 individuals had preDM. preDM was independently significantly associated with distant metastasis in all SCLC patients (p =0.016, OR=1.80, 95% CI 1.11– 2.91), while preDM did not affect the outcome of SCLC patients (p=0.803, HR=1.04, 95% CI 0.79– 1.36) by multivariate analysis. In the preDM group, the median overall survival (OS) was shorter in the insulin group than in the non insulin group (13.93 months versus 21.77 months, p=0.024). Multivariate analysis identified that insulin treatment was an independent unfavorable factor associated with OS (p =0.009, HR=2.10, 95% CI 1.19– 3.64). In addition, poorer performance status (PS) and liver metastasis were also independent unfavorable prognostic factors (all p< 0.01), while thoracic therapy significantly improved OS and decreased mortality risk in diabetic patients with SCLC (p< 0.05).Conclusion: preDM may promote distant metastasis of SCLC while it is insulin therapy and not preDM which adversely affects the prognosis of SCLC patients. These findings indicate that enhancing blood glucose control and reducing insulin analog use may be essential to the improvement of the long-term survival of the diabetic population with SCLC.Keywords: type 2 diabetes mellitus, small cell lung cancer, distant metastasis, insulin, overall survival
- Published
- 2022
17. Molecular Gas in the Halo Fuels the Growth of a Massive Cluster Galaxy at High Redshift
- Author
-
Emonts, B. H. C., Lehnert, M. D., Villar-Martin, M., Norris, R. P., Ekers, R. D., van Moorsel, G. A., Dannerbauer, H., Pentericci, L., Miley, G. K., Allison, J. R., Sadler, E. M., Guillard, P., Carilli, C. L., Mao, M. Y., Rottgering, H. J. A., De Breuck, C., Seymour, N., Gullberg, B., Ceverino, D., Jagannathan, P., Vernet, J., and Indermuehle, B. T.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
The largest galaxies in the Universe reside in galaxy clusters. Using sensitive observations of carbon-monoxide, we show that the Spiderweb Galaxy -a massive galaxy in a distant protocluster- is forming from a large reservoir of molecular gas. Most of this molecular gas lies between the protocluster galaxies and has low velocity dispersion, indicating that it is part of an enriched inter-galactic medium. This may constitute the reservoir of gas that fuels the widespread star formation seen in earlier ultraviolet observations of the Spiderweb Galaxy. Our results support the notion that giant galaxies in clusters formed from extended regions of recycled gas at high redshift., Comment: Published in Science on 2 Dec 2016 (accepted 21 Oct 2016), 20 pages, 5 figures, 3 tables. Contains minor copy-editing differences with published version
- Published
- 2016
- Full Text
- View/download PDF
18. First-Line Anlotinib Combined with Stereotactic Body Radiation Therapy for an Octogenarian with Pulmonary Carcinosarcoma
- Author
-
Liang L, Chen T, Ren T, Mao M, Wang K, Tang C, Xiao J, Jia H, Chen W, Wang Q, and Li T
- Subjects
pulmonary carcinosarcoma ,sbrt ,anlotini ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Abstract
Long Liang,1,* Taiyu Chen,2,* Tao Ren,3 Mian Mao,4 Keli Wang,5 Chunhan Tang,2 Juan Xiao,1 Hongyuan Jia,1 Wenli Chen,1 Qifeng Wang,1 Tao Li1 1Department of Radiation Oncology, Sichuan Cancer Hospital and Institution, Sichuan Cancer Center, School of Medicine, University of Electronic Science and Technology of China, Radiation Oncology Key Laboratory of Sichuan Province, Chengdu, People’s Republic of China; 2Clinical Medical College of Chengdu Medical College, Chengdu, 610500, People’s Republic of China; 3Oncology Department, Clinical Medical College and The First Affiliated Hospital of Chengdu Medical College, Chengdu, 610500, People’s Republic of China; 4Department of Pharmacy, Sichuan Cancer Hospital & Institute, Sichuan Cancer Center, School of Medicine, University of Electronic Science and Technology of China, Chengdu, People’s Republic of China; 5Clinical Medical College of Southwest Medical University, Luzhou, 646000, People’s Republic of China*These authors contributed equally to this workCorrespondence: Tao Li Tel/Fax +86 2885420173Email litaoxmf@126.comAbstract: Pulmonary carcinosarcoma (PC) is a rare and highly malignant type of non-small cell lung cancer (NSCLC) that is insensitive to radiotherapy and chemotherapy and has a poor prognosis. Here, we report a case of an 88-year-old patient with inoperable PC and a history of cerebral infarction who was treated with first-line anlotinib combined with stereotactic body radiation therapy (SBRT). The therapeutic response has sustained for 10 months. Our work suggests that SBRT combined with anlotinib may be a safe and effective treatment strategy for octogenarians with PC.Keywords: pulmonary carcinosarcoma, SBRT, anlotini
- Published
- 2022
19. Graphene Oxide-Copper Nanocomposites Suppress Cariogenic Streptococcus mutans Biofilm Formation
- Author
-
Mao M, Zhang W, Huang Z, Huang J, Wang J, Li W, and Gu S
- Subjects
graphene oxide-copper nanocomposites ,anti-biofilm ,streptococcus mutans ,exopolysaccharides ,dental caries ,Medicine (General) ,R5-920 - Abstract
Mengying Mao,1– 3 Wenjie Zhang,2– 4 Zhengwei Huang,1– 3 Jing Huang,1– 3 Jia Wang,1– 3 Weiping Li,1– 3 Shensheng Gu1– 3 1Department of Endodontics, Shanghai Ninth People’s Hospital, College of Stomatology, Shanghai Jiao Tong University School of Medicine, Shanghai, People’s Republic of China; 2National Clinical Research Center for Oral Diseases, Shanghai, People’s Republic of China; 3Shanghai Key Laboratory of Stomatology & Shanghai Research Institute of Stomatology, Shanghai, People’s Republic of China; 4Department of Prosthodontics, Oral Bioengineering and Regenerative Medicine Lab, Shanghai Ninth People’s Hospital, College of Stomatology, Shanghai Jiao Tong University School of Medicine, Shanghai, People’s Republic of ChinaCorrespondence: Shensheng GuDepartment of Endodontics, Shanghai Ninth People’s Hospital, College of Stomatology, Shanghai Jiao Tong University School of Medicine, 639 Zhizaoju Road, Shanghai, 200011, People’s Republic of ChinaEmail gss2m9h@163.comWeiping LiShanghai Ninth People’s Hospital, College of Stomatology, Shanghai Jiao Tong University School of Medicine, 639 Zhizaoju Road, Shanghai, 200011, People’s Republic of ChinaEmail wp_li95814@163.comIntroduction: Dental caries is a biofilm-dependent disease that largely relies on the ability of Streptococcus mutans to synthesize exopolysaccharide matrix. Graphene oxide-based metal nanomaterials, as the derivatives of graphene, are potent agents against pathogens by their impressive antibacterial and anti-biofilm biofunctions. Previously, we fabricated the novel graphene oxide-copper nanocomposites (GO-Cu), maintaining a long-term release of copper nanoparticles. Here, the biofunctionalization of GO-Cu nanocomposites against cariogenic S. mutans is investigated.Methods: Growth curve observation and colony forming units counting were applied to detect the antibacterial effect of GO-Cu nanocomposites on S. mutans. Scanning electron microscopy and the crystal violet assay were used to detect nanocomposite effects on biofilm forming ability. The production and distribution of exopolysaccharides within biofilm was analyzed and the expression of genes required for biofilm formation was explored. Moreover, the regulatory landscape of GO-Cu nanocomposites on S. mutans pathogenicity was probed.Results: It has been found that GO-Gu nanocomposites were antibacterial to S. mutans and 10 μg/mL GO-Cu nanocomposites could inhibit the bacteria bioactivity instead of killing them. The biomass of S. mutans biofilm was significantly reduced when treated with 10 μg/mL GO-Cu nanocomposites. Also, 10 μg/mL GO-Cu nanocomposites could alter the biofilm architecture and impair exopolysaccharides production and distribution, and dysregulated the expression of exopolysaccharide-associated genes.Conclusion: In all, we found low-dose GO-Cu nanocomposites could disrupt exopolysaccharide matrix assembly and further impair optimal biofilm development with minimal cytotoxicity. Therefore, GO-Cu nanocomposites can open up a new avenue for the development of alternative anti-caries biomaterials.Keywords: graphene oxide-copper nanocomposites, anti-biofilm, Streptococcus mutans, exopolysaccharides, dental caries
- Published
- 2021
20. Store-Operated Calcium Channels Contribute to Remifentanil-Induced Postoperative Hyperalgesia via Phosphorylation of CaMKIIα in Rats
- Author
-
Zhou Z, Mao M, Cai X, Zhu W, and Sun J
- Subjects
remifentanil ,hyperalgesia ,soccs ,camkiiα ,Medicine (General) ,R5-920 - Abstract
Zhenhui Zhou,1,* Meng Mao,2,* Xuechun Cai,1 Wei Zhu,1 Jie Sun3 1Department of Anesthesiology and Perioperative Medicine, The First Affiliated Hospital of Nanjing Medical University, Nanjing, Jiangsu, People’s Republic of China; 2Department of Anesthesiology, The Affiliated Stomatological Hospital of Nanjing Medical University, Nanjing, Jiangsu, People’s Republic of China; 3Department of Anesthesiology, Zhongda Hospital, Medical School, Southeast University, Nanjing, Jiangsu, People’s Republic of China*These authors contributed equally to this workCorrespondence: Jie SunDepartment of Anesthesiology, Zhongda Hospital, Medical School, Southeast University, Nanjing, 210009, People’s Republic of ChinaTel +8615895971012Email dgsunjie@hotmail.comWei ZhuDepartment of Anesthesiology and Perioperative Medicine, The First Affiliated Hospital of Nanjing Medical University, Nanjing, 210009, People’s Republic of ChinaTel +8618905182820Email zhuweijsph@163.comPurpose: The mechanisms of remifentanil-induced postoperative hyperalgesia (RIPH) remain unclear. Store-operated calcium channels (SOCCs) are mainly comprised of stromal interaction molecules 1 (STIM1) and pore-forming subunits (Orai1). They were found to take a pivotal part in Ca2+-dependent procedures and involved in the development of central sensitization and pain. Ca2+/calmodulin-dependent protein kinase IIα (CaMKIIα), regulated by Ca2+/calmodulin complex, has been shown to have a crucial role in RIPH. This study aims to determine whether SOCCs contribute to RIPH via activating CaMKIIα.Materials and Methods: Intra-operative infusion of remifentanil (1.0 μg kg− 1 min− 1, 60 min) was used to establish a RIPH rat model. The SOCCs blocker (YM-58483) was applied intrathecally to confirm the results. Animal behavioral tests including paw withdrawal thermal latency (PWTL) and paw withdrawal mechanical threshold (PWMT) were performed at − 24, 2, 6, 24, 48 h after incision and remifentanil treatments. The protein expression of STIM1, Orai1, CaMKIIα, and p-CaMKIIα was assayed with Western blot, and the number of STIM1 and Orai1 positive cells was shown by immunofluorescence.Results: Remifentanil administration significantly induced postoperative mechanical and thermal hyperalgesia, as well as increased STIM1 and Orai1 protein expression in the spinal dorsal horn. Furthermore, the intrathecal administration of YM-58483 effectively alleviated remifentanil-induced postoperative mechanical and thermal hyperalgesia according to the behavioral tests. In addition, YM-58483 suppressed the phosphorylation of CaMKIIα but had no effect on the expression of STIM1 and Orai1.Conclusion: Our study demonstrated that SOCCs are involved in RIPH. The over-expressed STIM1 and Orai1 in the spinal cord contribute to RIPH via mediating the phosphorylation of CaMKIIα. Blockade of SOCCs may provide an effective therapeutic approach for RIPH.Keywords: remifentanil, hyperalgesia, SOCCs, CaMKIIα
- Published
- 2021
21. The Discovery of a Low-Luminosity SPIRAL DRAGN
- Author
-
Mulcahy, D. D., Mao, M. Y., Mitsuishi, I., Scaife, A. M. M., Clarke, A. O., Babazaki, Y., Kobayashi, H., Suganuma, R., Matsumoto, H., and Tawara, Y.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
Standard galaxy formation models predict that large-scale double-lobed radio sources, known as DRAGNs, will always be hosted by elliptical galaxies. In spite of this, in recent years a small number of spiral galaxies have also been found to host such sources. These so-called spiral DRAGNs are still extremely rare, with only $\sim 5$ cases being widely accepted. Here we report on the serendipitous discovery of a new spiral DRAGN in data from the Giant Metrewave Radio Telescope (GMRT) at 322 MHz. The host galaxy, MCG+07-47-10, is a face-on late-type Sbc galaxy with distinctive spiral arms and prominent bulge suggesting a high black hole mass. Using WISE infra-red and GALEX UV data we show that this galaxy has a star formation rate of 0.16-0.75 M$_{\odot}$yr$^{-1}$, and that the radio luminosity is dominated by star-formation. We demonstrate that this spiral DRAGN has similar environmental properties to others of this class, but has a comparatively low radio luminosity of $L_{\rm 1.4GHz}$ = 1.12$\times$10$^{22}$ W Hz$^{-1}$, two orders of magnitude smaller than other known spiral DRAGNs. We suggest that this may indicate the existence of a previously unknown low-luminosity population of spiral DRAGNS., Comment: 4 pages, Accepted for publication in Astronomy and Astrophysics
- Published
- 2016
- Full Text
- View/download PDF
22. Investigation of the treatment modality in primary lymphoma of the salivary glands
- Author
-
Zhang, Y.-Y., Mao, M.-H., Feng, Z.-E., Li, J.-Z., Qin, L.-Z., and Han, Z.-X.
- Published
- 2021
- Full Text
- View/download PDF
23. Plis de passage in the superior temporal sulcus: Morphology and local connectivity
- Author
-
Bodin, C., Pron, A., Le Mao, M., Régis, J., Belin, P., and Coulon, O.
- Published
- 2021
- Full Text
- View/download PDF
24. ATLAS - I. Third Release of 1.4 GHz Mosaics and Component Catalogues
- Author
-
Franzen, T. M. O., Banfield, J. K., Hales, C. A., Hopkins, A., Norris, R. P., Seymour, N., Chow, K. E., Herzog, A., Huynh, M. T., Lenc, E., Mao, M. Y., and Middelberg, E.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
We present the third data release from the Australia Telescope Large Area Survey (ATLAS). These data combine the observations at 1.4 GHz before and after upgrades to the Australia Telescope Compact Array reaching a sensitivity of 14 microJy/beam in 3.6 deg^2 over the Chandra Deep Field South (CDFS) and of 17 microJy/beam in 2.7 deg^2 over the European Large Area ISO Survey South 1 (ELAIS-S1). We used a variety of array configurations to maximise the uv coverage resulting in a resolution of 16 by 7 arcsec in CDFS and of 12 by 8 arcsec in ELAIS-S1. After correcting for peak bias and bandwidth smearing, we find a total of 3034 radio source components above 5 sigma in CDFS, of which 514 (17 per cent) are considered to be extended. The number of components detected above 5 sigma in ELAIS-S1 is 2084, of which 392 (19 per cent) are classified as extended. The catalogues include reliable spectral indices (delta alpha < 0.2) between 1.40 and 1.71 GHz for ~350 of the brightest components., Comment: 19 pages, 11 figures, MNRAS accepted
- Published
- 2015
- Full Text
- View/download PDF
25. What Powers Lyman alpha Blobs?
- Author
-
Ao, Y., Matsuda, Y., Beelen, A., Henkel, C., Cen, R., De Breuck, C., Francis, P., Kovacs, A., Lagache, G., Lehnert, M., Mao, M., Menten, K. M., Norris, R., Omont, A., Tatemastu, K., Weiss, A., and Zheng, Z.
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Lyman alpha blobs (LABs) are spatially extended lyman alpha nebulae seen at high redshift. The origin of Lyman alpha emission in the LABs is still unclear and under debate. To study their heating mechanism(s), we present Australia Telescope Compact Array (ATCA) observations of the 20 cm radio emission and Herschel PACS and SPIRE measurements of the far-infrared (FIR) emission towards the four LABs in the protocluster J2143-4423 at z=2.38. Among the four LABs, B6 and B7 are detected in the radio with fluxes of 67+/-17 microJy and 77+/-16 microJy, respectively, and B5 is marginally detected at 3 sigma (51+/-16 microJy). For all detected sources, their radio positions are consistent with the central positions of the LABs. B6 and B7 are obviously also detected in the FIR. By fitting the data with different templates, we obtained redshifts of 2.20$^{+0.30}_{-0.35}$ for B6 and 2.20$^{+0.45}_{-0.30}$ for B7 which are consistent with the redshift of the lyman alpha emission within uncertainties, indicating that both FIR sources are likely associated with the LABs. The associated FIR emission in B6 and B7 and high star formation rates strongly favor star formation in galaxies as an important powering source for the lyman alpha emission in both LABs. However, the other two, B1 and B5, are predominantly driven by the active galactic nuclei or other sources of energy still to be specified, but not mainly by star formation. In general, the LABs are powered by quite diverse sources of energy., Comment: 7 pages and 3 figurs, accepted by A&A
- Published
- 2015
- Full Text
- View/download PDF
26. Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection
- Author
-
Banfield, J. K., Wong, O. I., Willett, K. W., Norris, R. P., Rudnick, L., Shabala, S. S., Simmons, B. D., Snyder, C., Garon, A., Seymour, N., Middelberg, E., Andernach, H., Lintott, C. J., Jacob, K., Kapinska, A. D., Mao, M. Y., Masters, K. L., Jarvis, M. J., Schawinski, K., Paget, E., Simpson, R., Klockner, H. R., Bamford, S., Burchell, T., Chow, K. E., Cotter, G., Fortson, L., Heywood, I., Jones, T. W., Kaviraj, S., Lopez-Sanchez, A. R., Maksym, W. P., Polsterer, K., Borden, K., Hollow, R. P., and Whyte, L.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
We present results from the first twelve months of operation of Radio Galaxy Zoo, which upon completion will enable visual inspection of over 170,000 radio sources to determine the host galaxy of the radio emission and the radio morphology. Radio Galaxy Zoo uses $1.4\,$GHz radio images from both the Faint Images of the Radio Sky at Twenty Centimeters (FIRST) and the Australia Telescope Large Area Survey (ATLAS) in combination with mid-infrared images at $3.4\,\mu$m from the {\it Wide-field Infrared Survey Explorer} (WISE) and at $3.6\,\mu$m from the {\it Spitzer Space Telescope}. We present the early analysis of the WISE mid-infrared colours of the host galaxies. For images in which there is $>\,75\%$ consensus among the Radio Galaxy Zoo cross-identifications, the project participants are as effective as the science experts at identifying the host galaxies. The majority of the identified host galaxies reside in the mid-infrared colour space dominated by elliptical galaxies, quasi-stellar objects (QSOs), and luminous infrared radio galaxies (LIRGs). We also find a distinct population of Radio Galaxy Zoo host galaxies residing in a redder mid-infrared colour space consisting of star-forming galaxies and/or dust-enhanced non star-forming galaxies consistent with a scenario of merger-driven active galactic nuclei (AGN) formation. The completion of the full Radio Galaxy Zoo project will measure the relative populations of these hosts as a function of radio morphology and power while providing an avenue for the identification of rare and extreme radio structures. Currently, we are investigating candidates for radio galaxies with extreme morphologies, such as giant radio galaxies, late-type host galaxies with extended radio emission, and hybrid morphology radio sources., Comment: Accepted to MNRAS, 17 pages, 13 figures, 1 table. Higher resolution figures available with MNRAS publication or contact author
- Published
- 2015
- Full Text
- View/download PDF
27. A CO-rich merger shaping a powerful and hyper-luminous infrared radio galaxy at z=2: the Dragonfly Galaxy
- Author
-
Emonts, B. H. C., Mao, M. Y., Stroe, A., Pentericci, L., Villar-Martin, M., Norris, R. P., Miley, G., De Breuck, C., van Moorsel, G. A., Lehnert, M. D., Carilli, C. L., Rottgering, H. J. A., Seymour, N., Sadler, E. M., Ekers, R. D., Drouart, G., Feain, I., Colina, L., Stevens, J., and Holt, J.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
In the low-redshift Universe, the most powerful radio sources are often associated with gas-rich galaxy mergers or interactions. We here present evidence for an advanced, gas-rich (`wet') merger associated with a powerful radio galaxy at a redshift of z~2. This radio galaxy, MRC 0152-209, is the most infrared-luminous high-redshift radio galaxy known in the southern hemisphere. Using the Australia Telescope Compact Array, we obtained high-resolution CO(1-0) data of cold molecular gas, which we complement with HST/WFPC2 imaging and WHT long-slit spectroscopy. We find that, while roughly M(H2) ~ 2 x 10$^{10}$ M$_{\odot}$ of molecular gas coincides with the central host galaxy, another M(H2) ~ 3 x 10$^{10}$ M$_{\odot}$ is spread across a total extent of ~60 kpc. Most of this widespread CO(1-0) appears to follow prominent tidal features visible in the rest-frame near-UV HST/WFPC2 imaging. Ly$\alpha$ emission shows an excess over HeII, but a deficiency over L(IR), which is likely the result of photo-ionisation by enhanced but very obscured star formation that was triggered by the merger. In terms of feedback, the radio source is aligned with widespread CO(1-0) emission, which suggests that there is a physical link between the propagating radio jets and the presence of cold molecular gas on scales of the galaxy's halo. Its optical appearance, combined with the transformational stage at which we witness the evolution of MRC 0152-209, leads us to adopt the name `Dragonfly Galaxy'., Comment: Accepted for publication in MNRAS (12 pages, 5 figures)
- Published
- 2015
- Full Text
- View/download PDF
28. Intestinal Translocation of Live Porphyromonas gingivalis Drives Insulin Resistance
- Author
-
Niu, C., primary, Lv, W., additional, Zhu, X., additional, Dong, Z., additional, Yuan, K., additional, Jin, Q., additional, Zhang, P., additional, Li, P., additional, Mao, M., additional, Dong, T., additional, Chen, Z., additional, Luo, J., additional, Hou, L., additional, Zhang, C., additional, Hao, K., additional, Chen, S., additional, and Huang, Z., additional
- Published
- 2024
- Full Text
- View/download PDF
29. Is there a role for chemotherapy and radiation in the treatment of patients with low-grade myofibroblastic sarcoma?
- Author
-
Xu, Y., Xu, G., Wang, X., Mao, M., Wu, H., Baklaushev, V. P., Chekhonin, V. P., Peltzer, K., Wang, G., and Zhang, C.
- Published
- 2021
- Full Text
- View/download PDF
30. Electro-osmotic flow through a nanopore
- Author
-
Mao, M., Sherwood, J. D., and Ghosal, S.
- Subjects
Physics - Fluid Dynamics ,Condensed Matter - Soft Condensed Matter - Abstract
Electroosmotic pumping of fluid through a nanopore that traverses an insulating membrane is considered. The density of surface charge on the membrane is assumed uniform, and sufficiently low for the Poisson-Boltzmann equation to be linearized. The reciprocal theorem gives the flow rate generated by an applied weak electric field, expressed as an integral over the fluid volume. For a circular hole in a membrane of zero thickness, an analytical result is possible up to quadrature. For a membrane of arbitrary thickness, the full Poisson--Nernst--Planck--Stokes system of equations is solved numerically using a finite volume method. The numerical solution agrees with the standard analytical result for electro-osmotic flux through a long cylindrical pore when the membrane thickness is large compared to the hole diameter. When the membrane thickness is small, the flow rate agrees with that calculated using the reciprocal theorem., Comment: 16 pages, 6 figures
- Published
- 2014
- Full Text
- View/download PDF
31. ATLAS 1.4 GHz Data Release 2 -- I. Observations of the CDF-S and ELAIS-S1 fields and methods for constructing differential number counts
- Author
-
Hales, C. A., Norris, R. P., Gaensler, B. M., Middelberg, E., Chow, K. E., Hopkins, A. M., Huynh, M. T., Lenc, E., and Mao, M. Y.
- Subjects
Astrophysics - Astrophysics of Galaxies - Abstract
This is the first of two papers describing the second data release (DR2) of the Australia Telescope Large Area Survey (ATLAS) at 1.4 GHz, which comprises deep wide-field observations in total intensity, linear polarization, and circular polarization over the Chandra Deep Field-South and European Large Area Infrared Space Observatory Survey-South 1 regions. DR2 improves upon the first data release by maintaining consistent data reductions across the two regions, including polarization analysis, and including differential number counts in total intensity and linear polarization. Typical DR2 sensitivities across the mosaicked multi-pointing images are 30 uJy/beam at approximately 12"x6" resolution over a combined area of 6.4 square degrees. In this paper we present detailed descriptions of our data reduction and analysis procedures, including corrections for instrumental effects such as positional variations in image sensitivity, bandwidth smearing with a non-circular beam, and polarization leakage, and application of the BLOBCAT source extractor. We present the DR2 images and catalogues of components (discrete regions of radio emission) and sources (groups of physically associated radio components). We describe new analytic methods to account for resolution bias and Eddington bias when constructing differential number counts of radio components., Comment: 40 pages, 27 figures, 5 tables. Quality of some figures reduced. Accepted for publication in MNRAS
- Published
- 2014
- Full Text
- View/download PDF
32. CO(1-0) survey of high-z radio galaxies: alignment of molecular halo gas with distant radio sources
- Author
-
Emonts, B. H. C., Norris, R. P., Feain, I., Mao, M. Y., Ekers, R. D., Miley, G., Seymour, N., Roettgering, H. J. A., Villar-Martin, M., Sadler, E. M., Carilli, C. L., Mahony, E. K., de Breuck, C., Stroe, A., Pentericci, L., van Moorsel, G. A., Drouart, G., Ivison, R. J., Greve, T. R., Humphrey, A., Wylezalek, D., and Tadhunter, C. N.
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a CO(1-0) survey for cold molecular gas in a representative sample of 13 high-z radio galaxies (HzRGs) at 1.4
- Published
- 2013
- Full Text
- View/download PDF
33. Prediction of Poor Outcomes in Patients with Colorectal Cancer: Elevated Preoperative Prothrombin Time (PT) and Activated Partial Thromboplastin Time (APTT)
- Author
-
Zhang L, Ye J, Luo Q, Kuang M, Mao M, Dai S, and Wang X
- Subjects
pt ,aptt ,crc ,prognosis ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Abstract
Lin Zhang,1,2,* Juan Ye,2– 4,* Qiuyun Luo,2 Miaohuan Kuang,1 Minjie Mao,1 Shuqin Dai,1 Xueping Wang1 1Department of Clinical Laboratory, Sun Yat-Sen University Cancer Center, State Key Laboratory of Oncology in South China, Collaborative Innovation Center for Cancer Medicine, Guangzhou, Guangdong 510060, People’s Republic of China; 2Department of Experimental Research, Sun Yat-Sen University Cancer Center, State Key Laboratory of Oncology in South China, Collaborative Innovation Center for Cancer Medicine, Guangzhou, Guangdong, People’s Republic of China; 3Department of Infectious Diseases, The Fifth Affiliated Hospital of Sun Yat-Sen University, Zhuhai, Guangdong, People’s Republic of China; 4Department of Oncology, Affiliated Hospital of Zunyi Medical University, Zunyi, Guizhou, People’s Republic of China*These authors contributed equally to this workCorrespondence: Xueping Wang; Shuqin Dai Tel/ Fax +86 20 8734 3438Email wangxuep@sysucc.org.cn; daishq@sysucc.org.cnBackground and Objective: Tools for the non-invasive assessment of colorectal cancer (CRC) prognosis have profound significance. Although plasma coagulation tests have been investigated in a variety of tumours, the prognostic value of the prothrombin time (PT) and activated partial thromboplastin time (APTT) in CRC has not been discussed. Our study objective was to explore the prognostic significance of preoperative PT and APTT in CRC patients.Patients and Methods: A retrospective analysis of preoperative coagulation indexes including PT, PTA, INR, APTT, FIB, TT, PLT, NLR and PLR in 250 patients with CRC was performed. Kaplan–Meier and multivariate Cox regression analysis were used to demonstrate the prognostic value of these preoperative coagulation indexes.Results: The overall survival (OS, p< 0.05) and disease-free survival (DFS, p< 0.05) of CRC patients with lower PT and APTT levels were significantly prolonged. Based on univariate analysis, PT levels (p< 0.001, p< 0.001), PTA levels (p=0.001, p=0.001), APTT levels (p=0.001, p< 0.001), INR levels (p< 0.001, p< 0.001), fibrinogen levels (p=0.032, p=0.036), tumour status (p=0.005, p=0.003), nodal status (p< 0.001, p< 0.001), metastasis status (p< 0.001, p< 0.001) and TNM stages (p< 0.001, p< 0.001) were remarkably associated with DFS and OS. Multivariate Cox regression analysis suggested that the levels of PT (HR: 2.699, p=0.006) and APTT (HR: 1.942, p=0.015), metastasis status (HR: 2.091, p= 0.015) and TNM stage (HR: 7.086, p=0.006) were independent predictors of survival in CRC. In the whole cohort, the enrolled patients were then divided into three groups according to their PT and APTT levels. The OS and DFS differed notably among the low-risk (PT< 11.85 sec and APTT< 25.85 sec), medium-risk (PT≥ 11.85 sec or APTT≥ 25.85 sec), and high-risk (PT≥ 11.85 sec and APTT≥ 25.85 sec) groups.Conclusion: Elevated levels of preoperative PT and APTT were predictors of poor outcomes in CRC patients. Moreover, the combination of preoperative PT and APTT can be a new prognostic stratification approach for more precise clinical staging of CRC.Keywords: PT, APTT, CRC, prognosis
- Published
- 2020
34. CO(1-0) detection of molecular gas in the massive Spiderweb Galaxy (z=2)
- Author
-
Emonts, B. H. C., Feain, I., Roettgering, H. J. A., Miley, G., Seymour, N., Norris, R. P., Carilli, C. L., Villar-Martin, M., Mao, M. Y., Sadler, E. M., Ekers, R. D., van Moorsel, G. A., Ivison, R. J., Pentericci, L., Tadhunter, C. N., and Saikia, D. J.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The high-redshift radio galaxy MRC 1138-262 (`Spiderweb Galaxy'; z = 2.16), is one of the most massive systems in the early Universe and surrounded by a dense `web' of proto-cluster galaxies. Using the Australia Telescope Compact Array, we detected CO(1-0) emission from cold molecular gas -- the raw ingredient for star formation -- across the Spiderweb Galaxy. We infer a molecular gas mass of M(H2) = 6x10^10 M(sun) (for M(H2)/L'(CO)=0.8). While the bulk of the molecular gas coincides with the central radio galaxy, there are indications that a substantial fraction of this gas is associated with satellite galaxies or spread across the inter-galactic medium on scales of tens of kpc. In addition, we tentatively detect CO(1-0) in the star-forming proto-cluster galaxy HAE 229, 250 kpc to the west. Our observations are consistent with the fact that the Spiderweb Galaxy is building up its stellar mass through a massive burst of widespread star formation. At maximum star formation efficiency, the molecular gas will be able to sustain the current star formation rate (SFR ~ 1400 M(sun)/yr, as traced by Seymour et al.) for about 40 Myr. This is similar to the estimated typical lifetime of a major starburst event in infra-red luminous merger systems., Comment: 7 pages, 3 figures - accepted for publication in MNRAS
- Published
- 2013
- Full Text
- View/download PDF
35. Comparison and analysis of flexural behavior of steel-bamboo composite beams based on different kinds of bamboo plates
- Author
-
Zhang, J.L., primary, Mao, M., additional, and Li, Y.S., additional
- Published
- 2021
- Full Text
- View/download PDF
36. The ATLAS 5.5 GHz survey of the Extended Chandra Deep Field South: Catalogue, Source Counts and Spectral Indices
- Author
-
Huynh, M. T., Hopkins, A. M., Lenc, E., Mao, M. Y., Middelberg, E., Norris, R. P., and Randall, K. E.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Star forming galaxies are thought to dominate the sub-mJy radio population, but recent work has shown that low luminosity AGN can still make a significant contribution to the faint radio source population. Spectral indices are an important tool for understanding the emission mechanism of the faint radio sources. We have observed the extended Chandra Deep Field South at 5.5 GHz using a mosaic of 42 pointings with the Australia Telescope Compact Array (ATCA). Our image reaches an almost uniform sensitivity of ~12 microJy rms over 0.25 deg^2 with a restoring beam of 4.9 x 2.0 arcsec, making it one of the deepest 6cm surveys to date. We present the 5.5 GHz catalogue and source counts from this field. We take advantage of the large amounts of ancillary data in this field to study the 1.4 to 5.5 GHz spectral indices of the sub-mJy population. For the full 5.5 GHz selected sample we find a flat median spectral index, alpha_med = -0.40, which is consistent with previous results. However, the spectral index appears to steepen at the faintest flux density levels (S_{5.5 GHz} < 0.1 mJy), where alpha_med = -0.68. We performed stacking analysis of the faint 1.4 GHz selected sample (40 < S_{1.4 GHz} < 200 microJy) and also find a steep average spectral index, alpha = -0.8, consistent with synchrotron emission. We find a weak trend of steepening spectral index with redshift. Several young AGN candidates are identified using spectral indices, suggesting Gigahertz Peaked Spectrum (GPS) sources are as common in the mJy population as they are at Jy levels., Comment: 18 pages, 16 figures, accepted for publication in MNRAS
- Published
- 2012
- Full Text
- View/download PDF
37. EMU: Evolutionary Map of the Universe
- Author
-
Norris, Ray P., Hopkins, A. M., Afonso, J., Brown, S., Condon, J. J., Dunne, L., Feain, I., Hollow, R., Jarvis, M., Johnston-Hollitt, M., Lenc, E., Middelberg, E., Padovani, P., Prandoni, I., Rudnick, L., Seymour, N., Umana, G., Andernach, H., Alexander, D. M., Appleton, P. N., Bacon, D., Banfield, J., Becker, W., Brown, M. J. I., Ciliegi, P., Jackson, C., Eales, S., Edge, A. C., Gaensler, B. M., Giovannini, G., Hales, C. A., Hancock, P., Huynh, M. Y., Ibar, E., Ivison, R. J., Kennicutt, R., Kimball, Amy E., Koekemoer, A. M., Koribalski, B. S., López-Sánchez, Á. R., Mao, M. Y., Murphy, T., Messias, H., Pimbblet, K. A., Raccanelli, A., Randall, K. E., Reiprich, T. H., Roseboom, I. G., Röttgering, H., Saikia, D. J., Sharp, R. G., Slee, O. B., Smail, Ian, Thompson, M. A., Urquhart, J. S., Wall, J. V., and Zhao, G. -B.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
EMU is a wide-field radio continuum survey planned for the new Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep (rms ~ 10 microJy/beam) radio continuum survey of the entire Southern Sky at 1.3 GHz, extending as far North as +30 degrees declination, with a resolution of 10 arcsec. EMU is expected to detect and catalogue about 70 million galaxies, including typical star-forming galaxies up to z~1, powerful starbursts to even greater redshifts, and AGNs to the edge of the visible Universe. It will undoubtedly discover new classes of object. This paper defines the science goals and parameters of the survey, and describes the development of techniques necessary to maximise the science return from EMU., Comment: Accepted by PASA; see http://www.atnf.csiro.au/people/rnorris/papers/n252.pdf for higher-resolution figures
- Published
- 2011
- Full Text
- View/download PDF
38. The Australia Telescope Compact Array Broadband Backend (CABB)
- Author
-
Wilson, Warwick E., Ferris, R. H., Axtens, P., Brown, A., Davis, E., Hampson, G., Leach, M., Roberts, P., Saunders, S., Koribalski, B. S., Caswell, J. L., Lenc, E., Stevens, J., Voronkov, M. A., Wieringa, M. H., Brooks, K., Edwards, P. G., Ekers, R. D., Emonts, B., Hindson, L., Johnston, S., Maddison, S. T., Mahony, E. K., Malu, S. S., Massardi, M., Mao, M. Y., McConnell, D., Norris, R. P., Schnitzeler, D., Subrahmanyan, R., Urquhart, J. S., Thompson, M. A., and Wark, R. M.
- Subjects
Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies ,Astrophysics - Solar and Stellar Astrophysics - Abstract
Here we describe the Compact Array Broadband Backend (CABB) and present first results obtained with the upgraded Australia Telescope Compact Array (ATCA). The 16-fold increase in observing bandwidth, from 2 x 128 MHz to 2 x 2048 MHz, high bit sampling, and addition of 16 zoom windows (each divided into a further 2048 channels) provide major improvements for all ATCA observations. The benefits of the new system are: (1) hugely increased radio continuum and polarization sensitivity as well as image fidelity, (2) substantially improved capability to search for and map emission and absorption lines over large velocity ranges, (3) simultaneous multi-line and continuum observations, (4) increased sensitivity, survey speed and dynamic range due to high-bit sampling, and (5) high velocity resolution, while maintaining full polarization output. The new CABB system encourages all observers to make use of both spectral line and continuum data to achieve their full potential. Given the dramatic increase of the ATCA capabilities in all bands (ranging from 1.1 to 105 GHz) CABB enables scientific projects that were not feasible before the upgrade, such as simultaneous observations of multiple spectral lines, on-the-fly mapping, fast follow-up of radio transients (e.g., the radio afterglow of new supernovae) and maser observations at high velocity resolution and full polarization. The first science results presented here include wide-band spectra, high dynamic-range images, and polarization measurements, highlighting the increased capability and discovery potential of the ATCA., Comment: 27 pages, 34 figures, MNRAS, accepted
- Published
- 2011
- Full Text
- View/download PDF
39. Molecular CO(1-0) gas in the z~2 radio galaxy MRC 0152-209
- Author
-
Emonts, B. H. C., Feain, I., Mao, M. Y., Norris, R. P., Miley, G., Ekers, R. D., Villar-Martin, M., Rottgering, H. J. A., Sadler, E. M., Rees, G., Morganti, R., Saikia, D. J., Oosterloo, T. A., Stevens, J. B., and Tadhunter, C. N.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We report the detection of molecular CO(1-0) gas in the high-z radio galaxy MRC 0152-209 (z = 1.92) with the Australia Telescope Compact Array Broadband Backend (ATCA/CABB). This is the third known detection of CO(1-0) in a high-z radio galaxy to date. CO(1-0) is the most robust tracer of the overall molecular gas content (including the wide-spread, low-density and subthermally excited component), hence observations of CO(1-0) are crucial for studying galaxy evolution in the Early Universe. We derive L'(CO) = (6.6 +- 2.0) x 10^10 K km/s pc^2 for MRC 0152-209, which is comparable to that derived from CO(1-0) observations of several high-z submillimetre and starforming BzK galaxies. The CO(1-0) traces a total molecular hydrogen mass of M(H2) = 5 x 10^10 (alpha_x/0.8) Msun. MRC 0152-209 is an infra-red bright radio galaxy, in which a large reservoir of cold molecular gas has not (yet) been depleted by star formation or radio source feedback. Its compact radio source is reliably detected at 40 GHz and has a steep spectral index of alpha = -1.3 between 1.4 and 40 GHz (4-115 GHz in the galaxy's rest-frame). MRC 0152-209 is part of an ongoing systematic ATCA/CABB survey of CO(1-0) in high-z radio galaxies between 1.7 < z < 3., Comment: Accepted for publication in ApJL -- 8 pages, 3 figures
- Published
- 2011
- Full Text
- View/download PDF
40. Are the infrared-faint radio sources pulsars?
- Author
-
Cameron, A. D., Keith, M. J., Hobbs, G., Norris, R. P., Mao, M. Y., and Middelberg, E.
- Subjects
Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Infrared-Faint Radio Sources (IFRS) are objects which are strong at radio wavelengths but undetected in sensitive Spitzer observations at infrared wavelengths. Their nature is uncertain and most have not yet been associated with any known astrophysical object. One possibility is that they are radio pulsars. To test this hypothesis we undertook observations of 16 of these sources with the Parkes Radio Telescope. Our results limit the radio emission to a pulsed flux density of less than 0.21 mJy (assuming a 50% duty cycle). This is well below the flux density of the IFRS. We therefore conclude that these IFRS are not radio pulsars., Comment: 4 pages, accepted for publication in MNRAS
- Published
- 2011
- Full Text
- View/download PDF
41. CO observations of high-z radio galaxies MRC 2104-242 and MRC 0943-242: spectral-line performance of the Compact Array Broadband Backend
- Author
-
Emonts, B. H. C., Norris, R. P., Feain, I., Miley, G., Sadler, E. M., Villar-Martin, M., Mao, M. Y., Oosterloo, T. A., Ekers, R. D., Stevens, J. B., Wieringa, M. H., Coppin, K. E. K., and Tadhunter, C. N.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present the first 7-millimetre observations of two high-redshift, Lya-bright radio galaxies (MRC 2104-242 and MRC 0943-242) performed with the 2 x 2 GHz instantaneous bandwidth of the Compact Array Broadband Backend (CABB) at the Australia Telescope Compact Array (ATCA). The aim was to search for 12CO(1-0) emission in these systems and test the millimetre capabilities of CABB for performing spectral line observations at high redshifts. We show that the stable band and enhanced velocity coverage of CABB, combined with hybrid array configurations, provide the ATCA with excellent 7-mm capabilities that allow reliable searches for the ground transition of CO at high redshifts. In this paper we explicitly discuss the calibration procedures used to reach our results. We set a firm upper limit to the mass of molecular gas in MRC 2104-242 (z = 2.5) of M(H2) < 2 x 10^10 (alpha_x/0.8) M_sun. For MRC 0943-242 (z=2.9) we derive an upper limit of M(H2) < 6 x 10^10 (alpha_x/0.8) M_sun. We also find a tentative 3-sigma CO detection in the outer part of the giant Lya halo that surrounds MRC 0943-242. The 30-33 GHz radio continuum of MRC 2104-242 and MRC 0943-242 is reliably detected. Both radio sources show a spectral index of alpha ~ -1.5 between 1.4 and 30 GHz, with no evidence for spectral curvature within this range of frequencies., Comment: Accepted for publication in MNRAS -- 11 pages, 6 figures (full resolution version available at http://www.atnf.csiro.au/people/~emo004/Emonts_COinHzRG_apr11.pdf)
- Published
- 2011
- Full Text
- View/download PDF
42. The ATLAS Survey of the CDFS and ELAIS-S1 Fields
- Author
-
Lenc, E., Norris, R., Hales, C., Randall, K., Hopkins, A., Sharp, R., Huynh, M., Mao, M., and Middelberg, E.
- Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The first phase of the ATLAS (Australia Telescope Large Area Survey) project surveyed a total 7 square degrees down to 30 micro Jy rms at 1.4 GHz and is the largest sensitive radio survey ever attempted. We report on the scientific achievements of ATLAS to date and plans to extend the project as a path finder for the proposed EMU (Evolutionary map of the Universe) project which has been designed to use ASKAP (Australian Square Kilometre Array Pathfinder)., Comment: 4 pages, 3 figures
- Published
- 2009
43. The PULSE@Parkes project: A new observing technique for long-term pulsar monitoring
- Author
-
Hobbs, G., Hollow, R., Champion, D., Khoo, J., Yardley, D., Carr, M., Keith, M., Jenet, F., Amy, S., Burgay, M., Burke-Spolaor, S., Chapman, J., Danaia, L., Homewood, B., Kovacevic, A., Mao, M., McKinnon, D., Mulcahy, M., Oslowski, S., and van Straten, W.
- Subjects
Astrophysics - Solar and Stellar Astrophysics - Abstract
The PULSE@Parkes project has been designed to monitor the rotation of radio pulsars over time spans of days to years. The observations are obtained using the Parkes 64-m and 12-m radio telescopes by Australian and international high school students. These students learn the basis of radio astronomy and undertake small projects with their observations. The data are fully calibrated and obtained with the state-of-the-art pulsar hardware available at Parkes. The final data sets are archived and are currently being used to carry out studies of 1) pulsar glitches, 2) timing noise, 3) pulse profile stability over long time scales and 4) the extreme nulling phenomenon. The data are also included in other projects such as gamma-ray observatory support and for the Parkes Pulsar Timing Array project. In this paper we describe the current status of the project and present the first scientific results from the Parkes 12-m radio telescope. We emphasise that this project offers a straightforward means to enthuse high school students and the general public about radio astronomy while obtaining scientifically valuable data sets., Comment: accepted for publication by PASA
- Published
- 2009
- Full Text
- View/download PDF
44. Allelic heterogeneity contributes to variability in ocular dysgenesis, myopathy and brain malformations caused by Col4a1 and Col4a2 mutations
- Author
-
Gould, Douglas, Kuo, DS, Labelle-Dumais, C, Mao, M, Jeanne, M, Kauffman, WB, Allen, J, Favor, J, and Gould, DB
- Published
- 2014
45. Safety and Efficacy of Spatially Fractionated Radiation Therapy Using Lattice Radiation for Metastatic and/or Bulky Disease
- Author
-
Li, A., primary, Mao, M., additional, and Xu, B., additional
- Published
- 2023
- Full Text
- View/download PDF
46. The first VLBI image of an Infrared-Faint Radio Source
- Author
-
Middelberg, E., Norris, R. P., Tingay, S., Mao, M. Y., Phillips, C. J., and Hotan, A. W.
- Subjects
Astrophysics - Abstract
Context: To investigate the joint evolution of active galactic nuclei and star formation in the Universe. Aims: In the 1.4 GHz survey with the Australia Telescope Compact Array of the Chandra Deep Field South and the European Large Area ISO Survey - S1 we have identified a class of objects which are strong in the radio but have no detectable infrared and optical counterparts. This class has been called Infrared-Faint Radio Sources, or IFRS. 53 sources out of 2002 have been classified as IFRS. It is not known what these objects are. Methods: To address the many possible explanations as to what the nature of these objects is we have observed four sources with the Australian Long Baseline Array. Results: We have detected and imaged one of the four sources observed. Assuming that the source is at a high redshift, we find its properties in agreement with properties of Compact Steep Spectrum sources. However, due to the lack of optical and infrared data the constraints are not particularly strong., Comment: Accepted for publication in Astronomy and Astrophysics, 5 pages, needs aa.cls
- Published
- 2008
- Full Text
- View/download PDF
47. Total endoscopic thyroidectomy versus conventional open thyroidectomy in thyroid cancer: a systematic review and meta-analysis
- Author
-
Chen C, Huang S, Huang A, Jia Y, Wang J, Mao M, Zhou J, and Wang L
- Subjects
Endoscopic thyroidectomy ,Conventional open thyroidectomy ,Papillary thyroid carcinoma ,Meta-analysis ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Cong Chen,1,2 Shumin Huang,3 Aihua Huang,1,2 Yunlu Jia,1,2 Ji Wang,1,2 Misha Mao,1,2 Jichun Zhou,1,2 Linbo Wang1,2 1Department of Surgical Oncology, Sir Run Run Shaw Hospital, Zhejiang University School of Medicine, Hangzhou, China; 2Biomedical Research Center and Key Laboratory of Biotherapy of Zhejiang Province, Hangzhou, China; 3Department of Pediatric Health Care, The Children’s Hospital, Zhejiang University School of Medicine, Hangzhou, China Background: Despite the considerable experience gained thus far using endoscopic technologies, the role of total endoscopic thyroidectomy (ET) for papillary thyroid cancer (PTC) remains controversial. We conducted a systematic review and meta-analysis to investigate the safety and effectiveness of total ET compared with conventional open thyroidectomy (OT) in PTC. Methods: A systematic search was conducted using the PubMed, Embase and Cochrane Library electronic databases up to March 2018. The quality of included studies was evaluated using the Newcastle–Ottawa Scale. Review Manager software version 5.3 was used for the meta-analysis. Results: Twelve studies including 2,672 patients were ultimately included in the systematic review and meta-analysis. ET was associated with longer operative time (P
- Published
- 2018
48. Towards a global cancer knowledge network: dissecting the current international cancer genomic sequencing landscape
- Author
-
Vis, D.J., Lewin, J., Liao, R.G., Mao, M., Andre, F., Ward, R.L., Calvo, F., Teh, B.T., Camargo, A.A., Knoppers, B.M., Sawyers, C.L., Wessels, L.F.A., Lawler, M., Siu, L.L., and Voest, E.
- Published
- 2017
- Full Text
- View/download PDF
49. Co-effect of microstructure and surface constraints on plastic deformation in micro- and mesoscaled forming process
- Author
-
Mao, M. Y., Peng, L. F., Fu, M. W., and Lai, X. M.
- Published
- 2018
- Full Text
- View/download PDF
50. Effects of Solid Solution Treatments on the Microstructure and Mechanical Properties of a Nanoscale Precipitate-Strengthened Ferritic Steel
- Author
-
Zhao, Y., Guo, H., Xu, S. S., Mao, M. J., Chen, L., Gokhman, O., and Zhang, Z. W.
- Published
- 2018
- Full Text
- View/download PDF
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.