4,698 results on '"Gu, Q."'
Search Results
2. Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z = 3.95
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Zhou, L, Wang, T, Daddi, E, Coogan, R, Sun, H, Xu, K, Arumugam, V, Jin, S, Liu, D, Lu, S, Sillassen, N, Wang, Y, Shi, Y, Zhang, Z, Tan, Q, Gu, Q, Elbaz, D, Le Bail, A, Magnelli, B, Gómez-Guijarro, C, d’Eugenio, C, Magdis, G, Valentino, F, Ji, Z, Gobat, R, Delvecchio, I, Xiao, M, Strazzullo, V, Finoguenov, A, Schinnerer, E, Rich, RM, Huang, J, Dai, Y, Chen, Y, Gao, F, Yang, T, and Hao, Q
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Astronomical Sciences ,Physical Sciences ,galaxies: clusters: general ,galaxies: evolution ,galaxies: high-redshift ,submillimeter: galaxies ,Astronomical and Space Sciences ,Astronomy & Astrophysics ,Astronomical sciences ,Particle and high energy physics ,Space sciences - Abstract
The study of distant galaxy groups and clusters at the peak epoch of star formation is limited by the lack of a statistically and homogeneously selected and spectroscopically confirmed sample. Recent discoveries of concentrated starburst activities in cluster cores have opened a new window to hunt for these structures based on their integrated IR luminosities. Here, we carry out a large NOEMA (NOrthern Extended Millimeter Array) program targeting a statistical sample of infrared-luminous sources associated with overdensities of massive galaxies at z > 2, the Noema formIng Cluster survEy (NICE). We present the first result from the ongoing NICE survey, a compact group at z = 3.95 in the Lockman Hole field (LH-SBC3), confirmed via four massive (M∗ ≳ 1010.5 M⊙) galaxies detected in the CO(4-3) and [CI](1-0) lines. The four CO-detected members of LH-SBC3 are distributed over a 180 kpc physical scale and the entire structure has an estimated halo mass of ~1013 M⊙ and total star formation rate of ~4000 M⊙ yr-1. In addition, the most massive galaxy hosts a radio-loud active galactic nucleus with L1.4 GHz, rest = 3.0 × 1025 W Hz-1. The discovery of LH-SBC3 demonstrates the feasibility of our method to efficiently identify high-z compact groups or cluster cores undergoing formation. The existence of these starbursting cluster cores up to z ~ 4 provides critical insights into the mass assembly history of the central massive galaxies in clusters.
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- 2024
3. Cordycepin Ameliorates Renal Interstitial Fibrosis by Inhibiting Drp1-Mediated Mitochondrial Fission
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Sun Y, Jin S, Chen J, Zhang J, Lu Y, Gu Q, Yan Z, Chen W, Chen A, Fang Y, Geng W, Xu X, and Song N
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cordycepin ,drp1 ,renal fibrosis ,mitochondrial fission ,uir ,il-6 ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Yingxue Sun,1,* Shi Jin,1,* Jun Chen,2,* Jian Zhang,1 Yufei Lu,1 Qiuyu Gu,1 Zhixin Yan,1 Weize Chen,1 Annan Chen,1 Yi Fang,1 Wenye Geng,3 Xialian Xu,1 Nana Song1 1Department of Nephrology, Zhongshan Hospital, Fudan University; Shanghai Medical Center of Kidney; Shanghai Institute of Kidney and Dialysis; Shanghai Key Laboratory of Kidney and Blood Purification; Hemodialysis Quality Control Center of Shanghai, Shanghai, 200032, People’s Republic of China; 2Department of Pathology, Changzheng Hospital, Naval Military Medical University, Shanghai, 200003, People’s Republic of China; 3Scientific Research Department of Shanghai Medical College, Fudan Zhangjiang Institute, Fudan University, Shanghai, 201203, People’s Republic of China*These authors contributed equally to this workCorrespondence: Xialian Xu; Nana Song, Division of Nephrology, Zhongshan Hospital, Fudan University, Shanghai, People’s Republic of China, Tel +86-021-64041990-2138, Fax +86-021-64038038, Email xu.xialian@zs-hospital.sh.cn; song.nana@zs-hospital.sh.cnObjective: This study aimed to investigate the mechanisms and specific targets of cordycepin in the treatment of renal fibrosis using a unilateral ischemia-reperfusion (UIR) model.Methods: A UIR mouse model was established, followed by intraperitoneal injections of cordycepin and Mdivi-1. Masson’s trichrome staining and PAS staining were used to identify renal tubulointerstitial fibrosis and assess the degree of renal injury. Fibrosis markers and mitochondrial dynamics-related proteins were evaluated using Western blotting, while differential gene expression and pathway enrichment were analyzed by RNA-seq. Molecular docking, molecular dynamics simulations and surface plasmon resonance were conducted to validate the specific binding sites of cordycepin on the target protein Drp1. Immunofluorescence and in vitro experiments further elucidated the therapeutic mechanism of cordycepin.Results: In vivo experiments showed that intraperitoneal injection of cordycepin significantly reduced renal inflammation and fibrosis, lowered serum creatinine levels, and decreased collagen deposition. Transcriptome analysis revealed that cordycepin treatment downregulated the mitochondrial fission pathway and upregulated the mitochondrial fusion pathway. Western blotting showed reduced levels of fibrosis markers α-SMA and FN, as well as downregulation of Drp1, MFF, and Fis1, and upregulation of OPA1 and Mfn2. In vitro, cordycepin inhibited TGF-β-induced injury in NRK-52E cells, reducing Drp1 expression and IL-6 secretion. Crosstalk experiments confirmed that decreased IL-6 levels were crucial for cordycepin anti-fibrotic effects by suppressing fibroblast activation.Conclusion: Cordycepin ameliorates renal fibrosis by targeting Drp1 to inhibit mitochondrial fission in injured renal tubular epithelial cells, reducing IL-6 secretion and inhibiting fibroblast activation.Keywords: cordycepin, Drp1, renal fibrosis, mitochondrial fission, UIR, IL-6
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- 2025
4. Fatal Empyema Thoracis Caused by Nocardia otitidiscaviarum
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Gu Q, Zhou L, Shen X, Xu L, Wu G, Pan W, Lin W, Lv D, Lin L, and Yan S
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severe nocardia pneumonia ,empyema ,drug resistance rate ,drug sensitivity test ,Infectious and parasitic diseases ,RC109-216 - Abstract
Qianqian Gu,* Lingren Zhou,* Xiaofei Shen, Le Xu, Guixian Wu, Weijia Pan, Wenxia Lin, Dongqing Lv, Ling Lin, Shuangquan Yan Department of Respiratory Medicine, Taizhou Hospital of Zhejiang Province Affiliated to Wenzhou Medical University, Taizhou, 317000, People’s Republic of China*These authors contributed equally to this workCorrespondence: Ling Lin; Shuangquan Yan, Hospital of Zhejiang Province affiliated to Wenzhou Medical University, 150 Ximen Street, Taizhou, 317000, People’s Republic of China, Email Linling@enzemed.com; ysq25908712@163.comAbstract: Nocardiosis caused by Nocardia otitidiscaviarum is exceptionally rare and characterized by a high mortality rate. It typically affects immunocompromised patients, resulting in severe pulmonary or disseminated infections, and is notorious for abscess formation. Empyema resulting from nocardiosis is even less common. Early clinical signs and imaging findings lack specificity, culture growth is sluggish, and the absence of an effective serological detection method can delay treatment. We report an 81-year-old patient with chronic obstructive pulmonary disease treated by long-term inhalation of high-dose salmeterol fluticasone. The initial empirical anti-infection treatment proved ineffective, resulting in rapid disease progression before the confirmation of nocardiosis with empyema through cultures of pleural fluid and sputum. Despite active treatment measures, the patient succumbed to severe pulmonary infection, sepsis, and multiple organ failure. A review of the literature, together with clinical experience, indicates that conventional empirical treatment for Nocardia otitidiscaviarum infection may not always be effective due to the escalating rate of drug resistance. Therefore, the primary step in the management of the infection is timely diagnosis using different methods. Furthermore, the identification of the responsible strain followed by conducting drug sensitivity tests is paramount for the successful treatment of this disease.Keywords: severe nocardia pneumonia, empyema, drug resistance rate, drug sensitivity test
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- 2025
5. Unveiling Cuproptosis-Driven Molecular Clusters and Immune Dysregulation in Ankylosing Spondylitis
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Wei B, Wang S, Li S, Gu Q, Yue Q, Tang Z, Zhang J, and Liu W
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ankylosing spondylitis ,cuproptosis ,immune cell infiltration ,machine learning model ,Pathology ,RB1-214 ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Bowen Wei,1,2,* Siwei Wang,1,2,* Suiran Li,1,2,* Qingxiang Gu,3 Qingyun Yue,4 Zhuo Tang,1,2 Jiamin Zhang,1,2 Wei Liu1,2 1Department of Rheumatism and Immunity, First Teaching Hospital of Tianjin University of Traditional Chinese Medicine, Tianjin, People’s Republic of China; 2National Clinical Research Center for Chinese Medicine Acupuncture and Moxibustion, Tianjin, People’s Republic of China; 3Center of Preventive Treatment of Disease, Cangzhou Hospital of Integrated Traditional Chinese and Western of Hebei Province, Cangzhou, Hebei, People’s Republic of China; 4School of Chinese Materia Medica, Beijing University of Chinese Medicine, Beijing, People’s Republic of China*These authors contributed equally to this workCorrespondence: Wei Liu, Email fengshiliuwei@163.comBackground: Ankylosing spondylitis (AS) is a chronic autoimmune disease characterized by inflammation of the sacroiliac joints and spine. Cuproptosis is a newly recognized copper-induced cell death mechanism. Our study explored the novel role of cuproptosis-related genes (CRGs) in AS, focusing on immune cell infiltration and molecular clustering.Methods: By analyzing the peripheral blood gene expression datasets obtained from GSE73754, GSE25101, and GSE11886, we identified the expression patterns of cellular factors and immune infiltration cell related to cuproptosis. Subsequently, we employed weighted gene co-expression network analysis (WGCNA) to identify differentially expressed genes (DEGs) within each cluster and utilized the “GSVA” and “GSEABase” software packages to examine variations in gene sets enriched across various CRG clusters. Finally, we selected the best-performing machine learning model to predict genes associated with AS. Datasets (GSE25101 and GSE73754) and ELISA to assess the expression levels of the five genes and their corresponding proteins.Results: Seven cuproptosis-related DEGs and four immune cell types were identified, revealing significant immune heterogeneity in the immune cell infiltration between the two cuproptosis-related molecular clusters in AS. The eXtreme Gradient Boosting (XGB) model showed the highest predictive accuracy, achieving an area under the receiver operating characteristic curve (AUC) of 0.725, and 5-gene prediction models were established. It showed satisfactory performance in the GSE25101 dataset (AUC = 0.812). According to the blood serum samples of AS patients and controls, PELI1 had a higher expression level (AUC = 0.703, p = 0.07), while ICAM2 and RANGAP1 had lower expression levels (AUC = 0.724, 0.745, and p = 0.011, 0.000, respectively) in AS patients.Conclusion: We explored the correlation of cuproptosis in AS, and developed the optimal machine learning model to identify high-risk genes associated with AS. We also explored the pathogenesis and treatment strategies of AS, targeting PELI1, ICAM2, and RANGAP1.Keywords: ankylosing spondylitis, cuproptosis, immune cell infiltration, machine learning model
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- 2025
6. Evaluating Positional Obstructive Sleep Apnea in Children: Prevalence, Characteristics, and Risk Factors
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Wang Q, Huang G, Wang R, Cao Z, Liang J, Li M, and Gu Q
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obstructive sleep apnea ,pediatric patients ,risk factors ,polysomnography ,sleep position ,sleep-disordered breathing ,Psychiatry ,RC435-571 ,Neurophysiology and neuropsychology ,QP351-495 - Abstract
Qian Wang,1,2,* Guimin Huang,3,* Ruikun Wang,4 Zhilong Cao,5 Jieqiong Liang,1 Mengyao Li,1 Qinglong Gu1,2 1Department of Otolaryngology-Head and Neck Surgery, Capital Institute of Pediatrics, Beijing, People’s Republic of China; 2Graduate School of Peking Union Medical College, Beijing, People’s Republic of China; 3Child Health Big Data Research Center, Capital Institute of Pediatrics, Beijing, People’s Republic of China; 4Capital Institute of Pediatrics-Peking University Teaching Hospital, Beijing, People’s Republic of China; 5School of Software, Beihang University, Beijing, People’s Republic of China*These authors contributed equally to this workCorrespondence: Qinglong Gu, Department of Otolaryngology-Head and Neck Surgery, Capital Institute of Pediatrics, No. 2 Yabao Road, Chaoyang District, Beijing, 100020, People’s Republic of China, Tel +86-13146836613, Email gql71@163.comPurpose: This study investigates the prevalence, risk factors, and clinical characteristics of positional obstructive sleep apnea (POSA) among pediatric patients diagnosed with obstructive sleep apnea (OSA).Patients and Methods: A total of 1,236 children aged 0 to 17 years who underwent nocturnal polysomnography (PSG) and completed the Sleep Questionnaire were included. After excluding those with an AHI < 1, neurological or muscular disorders, or insufficient sleep time in specific positions, 908 patients remained: 158 with POSA and 750 with non-positional OSA (NPOSA). Propensity score matching (PSM) was applied at a 1:2 ratio, resulting in a final sample of 153 POSA and 306 NPOSA patients. Data analyses were performed using R software (version 4.2.3).Results: The prevalence of POSA was 12.8%. After PSM, patients with POSA had a lower overall AHI (8.66 vs 10.30), REM-AHI (14.30 vs 17.40), and NREM-AHI (7.43 vs 8.77) compared to those with NPOSA. POSA patients also had a shorter total sleep time (411 vs 427 minutes), spent less time in the supine position (168 vs 225 minutes), and more time in non-supine positions (241 vs 202 minutes) than NPOSA patients. Additionally, while the supine AHI was higher in POSA patients (15.60 vs 10.30), the non-supine AHI was lower (5.00 vs 11.00) compared to NPOSA patients. The minimum oxygen saturation was slightly higher in POSA patients (0.88 vs 0.87). All differences were statistically significant (P < 0.05). Risk factors for POSA included mild OSA, allergic rhinitis, non-allergic rhinitis, and obesity.Conclusion: The prevalence of POSA in children is lower than in adults, and its severity is less than that of NPOSA. Compared to NPOSA patients, POSA patients had significantly higher AHI during supine sleep and lower AHI during non-supine sleep. POSA patients also spent more time in non-supine positions, suggesting that avoiding supine sleep may help reduce apnea events. These findings highlight the importance of monitoring and managing sleep posture in POSA patients.Keywords: obstructive sleep apnea, pediatric patients, risk factors, polysomnography, sleep position, sleep-disordered breathing
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- 2024
7. The CompactLight Design Study
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D’Auria, G., Adli, E., Aicheler, M., Aksoy, A., Alesini, D., Apsimon, R., Arnsberg, J., Auchettl, R., Bainbridge, A., Balazs, K., Bantekas, D., Bedolla, J., Behtouei, M., Bellaveglia, M., vd Berg, M., Bernhard, A., Bignami, A., Breitenbach, M., Breukers, M., Burt, G., Cai, J., Calvi, M., Cardelli, F., Carpanese, M., Cortes, H. M. Castaneda, Castilla, A., Cianchi, A., Clarke, J., Cowie, L., Croia, M., Cross, A., Danailov, M., Dattoli, G., Deleval, S., Mitri, S. Di, Diomede, M., Dowd, R., Dunning, D., Easton, J., Fang, W., Fatehi, S., Faus-Golfe, A., Ferianis, M., Ferrario, M., Ficcadenti, L., Gallo, A., Gazis, E., Gazis, N., Geometrante, R., Gethmann, J., Gioppo, R., Giribono, A., González-Iglesias, D., Goryashko, V., Grohmann, S., Gu, Q., Han, Y., Hinton, A., Hobi, A., Hoekstra, R., Huang, X., Jacewicz, M., Jones, J., Kaertner, F., Karagiannaki, A., Kokole, M., Kotitsa, R., Kotsopoulos, D., Krasch, B., Latina, A., Lepercq, P., Liu, X., Lucas, T. G., Luiten, O. J., Maheshwari, M., Mahnic, J., Mak, A., Marcos, J., Marin, E., Marinov, K., Martínez, B. G., Mercier, B., Migliorati, M., Milharcic, T., Mostacci, A., Mu noz, R., Musat, V., Mutsaers, P. H. A., Nergiz, Z., Nguyen, F., Nix, L., Palumbo, L., Parodi, M., Pavlica, R., Pellegrino, L., Pereira, D. E., Perez, F., Petralia, A., Piersanti, L., Pockar, J., Pramatari, K., Priem, H., Primozic, U., Rassool, R., Reiche, S., Revilak, P., Richter, S. C., Rochow, R., Rossi, C., Salén, P., Schmidt, T., Schoerling, D., Schulte, D., Scifo, J., Sheehy, S., Shepherd, B., Spataro, B., Stapnes, S., Stragier, X. F. D., Syratchev, I., Tabacco, C., Tan, J., Tanke, E., Taylor, G., Telahi, I., Thompson, N., Trachanas, E., Tzanetou, K. S., Vaccarezza, C., Vainola, J., Vannozzi, A., Volpi, M., Wang, C., Williams, P., Wu, X., Wuensch, W., Yap, J., Zangrando, M., Zhang, K., Zhang, L., Zhao, Y., Zhao, Z., and Zhu, D.
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- 2024
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8. Prognostic Value of Ki67 in Epithelial Ovarian Cancer: Post-Neoadjuvant Chemotherapy Ki67 Combined with CA125 Predicting Recurrence
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Liu Y, Gu Q, Xiao Y, Wei X, Wang J, Huang X, and Linghu H
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interval debulking surgery ,progression-free survival ,overall survival ,tumor marker ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Abstract
Yuexi Liu,* Qiuying Gu,* Yao Xiao, Xing Wei, Jinlong Wang, Xiaolan Huang, Hua Linghu Department of Gynecology, The First Affiliated Hospital of Chongqing Medical University, Chongqing, People’s Republic of China*These authors contributed equally to this workCorrespondence: Hua Linghu, Department of Gynecology, The First Affiliated Hospital of Chongqing Medical University, Chongqing, 400016, People’s Republic of China, Email linghuhua@cqmu.edu.cnPurpose: To evaluate Ki67 expression and prognostic value during neoadjuvant chemotherapy (NACT) in advanced epithelial ovarian cancer (EOC).Patients and Methods: 95 patients with advanced EOC receiving NACT followed by interval debulking surgery (IDS) were available for tissue samples from matched pre- and post-therapy specimens. The expression of Ki-67 was evaluated by immunohistochemistry and classified by percentage of stained cells. The optimal cutoff values of the Ki67 were assessed by receiver operating characteristic analysis. Kaplan-Meier analysis, the Log rank test, and Cox regression analysis were carried out to analyze survival.Results: Post-NACT Ki67 was an independent prognostic factor for recurrence by univariate (HR: 1.8, 95% CI: 1.1– 3.0, P-value: 0.023) and multivariate (HR: 1.88, 95% CI: 1.08– 3.26, P-value: 0.025) analysis. Residual disease > 1cm (HR: 2.69, 95% CI: 1.31– 5.54, P-value: 0.0070) and pre-treatment CA125 ≥ 1432 U/mL (HR: 2.00, 95% CI: 1.13– 3.55, P-value: 0.017) were also independent risk factors for progression-free survival (PFS) in multivariate analysis. Post-NACT Ki67 ≥ 20% was an independent risk factor for PFS, however, baseline Ki67 and Ki67 change did not suggest prognostic significance. In patients with high CA125, the median PFS for patients with high postKi67 (median PFS: 15.0 months, 95% CI: 13.4– 16.6 months) was significantly (P-value: 0.013) poorer compared to patients with low postKi67 (median PFS: 30.0 months, 95% CI: 13.5– 46.5 months).Conclusion: Post-NACT Ki67 ≥ 20% was an independent factor associated with poorer PFS in patients with advanced-stage EOC undergoing NACT followed by IDS. The combination of post-NACT Ki67 and pretreatment CA125 could better identify patients with poorer PFS in NACT-administered patients.Keywords: interval debulking surgery, progression-free survival, overall survival, tumor marker
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- 2024
9. Retrospective Analysis of Pyrotinib-Based Therapy for Metastatic Breast Cancer: Promising Efficacy in Combination with Trastuzumab
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Gu Q, Zhu M, Wang Y, and Gu Y
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pyrotinib ,her2 ,metastatic breast cancer ,trastuzumab ,inetetamab ,Neoplasms. Tumors. Oncology. Including cancer and carcinogens ,RC254-282 - Abstract
Qingqing Gu, Mingzhi Zhu, Yanyan Wang, Yuanting Gu The Second Department of Breast Surgery, The First Affiliated Hospital of Zhengzhou University, Zhengzhou, People’s Republic of ChinaCorrespondence: Yuanting Gu; Yanyan Wang, The Second Department of Breast Surgery, The First Affiliated Hospital of Zhengzhou University, Zhengzhou, People’s Republic of China, Tel +86-371-66913114, Fax +86-371-66964992, Email guyuanting2009@163.com; fccwangyy22@zzu.edu.cnPurpose: To evaluate the efficacy and safety of a pyrotinib-based therapy for human epidermal growth factor receptor 2 (HER2)-positive metastatic breast cancer (MBC) in the real world.Methods: Clinical data of 218 patients with HER2-positive MBC who received a pyrotinib-based therapy from January 2020 to March 2023 at the First Affiliated Hospital of Zhengzhou University were retrospectively analyzed.Results: Finally, 195 patients were included in the efficacy cohort. The median progression-free survival (PFS) in the total population is 12.4 months (95% CI, 9.8– 15.0 months). More than half of the patients in the efficacy cohort received pyrotinib mono-targeted therapy (103 cases, 52.8%). Among the remaining patients, 74 (37.9%) patients chose a combined trastuzumab-targeted therapy and 17 (8.7%) chose to combine inetetamab. Median PFS in the pyrotinib group vs pyrotinib plus trastuzumab group was 10.5 months vs 20.1 months (P< 0.001). The median PFS of primary trastuzumab resistance population reached to 20.1 months in pyrotinib plus trastuzumab group. Double-targets’ advantage was also observed in the brain metastases subgroup (17.9 months vs 10.0 months, P=0.386). The patients who received pyrotinib plus inetetamab as second and higher-line treatment reached a median PFS of 7.9 months (95% CI, 4.0– 11.8 months). Forty-one (19.8%) of 207 patients included in the safety cohort experienced grade 3 or higher diarrhea, the most common adverse event in safety analysis, and no adverse event-related deaths.Conclusion: The combination of pyrotinib and trastuzumab demonstrated promising efficacy in the treatment of HER2-positive metastatic breast cancer, including those who had primary resistance to trastuzumab and brain metastases. Pyrotinib plus trastuzumab is expected to be a potent option in the first-line. Additionally, the concurrent administration of pyrotinib and inetetamab could be an alternative to consider in the second and higher-line treatment for metastatic breast cancer. The adverse reactions of pyrotinib were tolerable in general.Keywords: pyrotinib, HER2, metastatic breast cancer, trastuzumab, inetetamab
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- 2024
10. To Investigate the Mechanism of Qinpi Tongfeng Formula in Treating Acute Gouty Arthritis by UHPLC-Q-Orbitrap-MS, Network Pharmacology and Experimental Validation
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Fan Y, Liu W, Jin Y, Lu H, Liu C, Wang A, Gu Q, and Ka Y
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acute gouty arthritis ,qinpi tongfeng formula ,network pharmacology ,uhplc-q-orbitrap-ms ,il-17 signaling pathway ,Pathology ,RB1-214 ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Yihua Fan,1– 3,* Wei Liu,1,2,* Yue Jin,1,2,* Hang Lu,1,2 Chunliu Liu,1,2 Aihua Wang,1,2 Qingxiang Gu,1,2 Yuxiu Ka1,2 1Department of Rheumatism and Immunity, First Teaching Hospital of Tianjin University of Traditional Chinese Medicine, Tianjin, People’s Republic of China; 2National Clinical Research Center for Chinese Medicine Acupuncture and Moxibustion, Tianjin, People’s Republic of China; 3Department of Rheumatism and Immunity, Hospital of Chengdu University of Traditional Chinese Medicine, Chengdu, Sichuan Province, People’s Republic of China*These authors contributed equally to this workCorrespondence: Wei Liu, Email fengshiliuwei@163.comBackground: Acute gouty arthritis (AGA) is characterized by the accumulation of monosodium urate crystals within the joints, leading to inflammation and severe pain. Western medicine treatments have limitations in addressing this condition. Previous studies have shown the efficacy of Qinpi Tongfeng formula (QPTFF) in treating AGA, but further investigation is needed to understand its mechanism of action.Methods: We used ultra-high-performance liquid chromatography tandem Q-Exactive Orbitrap high-resolution mass spectrometry (UHPLC-Q-Orbitrap-MS) to identify compounds in QPTFF. Target proteins regulated by these compounds were obtained from the Traditional Chinese Medicine Systems Pharmacology Database and Analysis Platform, Chemistry Database, and Swiss Target Prediction Database. AGA-related targets were searched and screened from various databases, including Genecards, PharmGKB, Drugbank, etc. Intersection targets of QPTFF and AGA were analyzed for protein–protein interaction networks, GO function enrichment, and KEGG pathway enrichment. We then verified QPTFF’s mechanism of action using an AGA rat model, assessing pathological changes via H&E staining and target expression via ELISA, RT-qPCR, and Western blot.Results: UHPLC-Q-Orbitrap-MS identified 207 compounds in QPTFF, with 55 selected through network pharmacology. Of 589 compound-regulated targets and 1204 AGA-related targets, 183 potential targets were implicated in QPTFF’s treatment of AGA. Main target proteins included IL-1β, NFKBIA, IL-6, TNF, CXCL8, and MMP9, with the IL-17 signaling pathway primarily regulated by QPTFF. Experimental results showed that medium and high doses of QPTFF significantly reduced serum inflammatory factors and MMP-9 expression, and inhibited IL-17A, IL-6, IKK-β, and NF-κB p65 mRNA and protein expression in AGA rats compared to the model group.Conclusion: Key targets of QPTFF include IL-1β, NFKBIA, IL-6, TNF-α, CXCL8, and MMP9. QPTFF effectively alleviates joint inflammation in AGA rats, with high doses demonstrating no liver or kidney toxicity. Its anti-inflammatory mechanism in treating AGA involves the IL-17A/NF-κB p65 signaling pathway.Keywords: acute gouty arthritis, Qinpi Tongfeng formula, network pharmacology, UHPLC-Q-Orbitrap-MS, IL-17 signaling pathway
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- 2024
11. Engineered Exosomes with Growth Differentiation Factor-15 Overexpression Enhance Cardiac Repair After Myocardial Injury
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Zou A, Xiao T, Chi B, Wang Y, Mao L, Cai D, Gu Q, Chen Q, Wang Q, Ji Y, and Sun L
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exosomes ,growth differentiation factor-15 ,telomerase reverse transcriptase ,acute myocardial infarction ,Medicine (General) ,R5-920 - Abstract
Ailin Zou,1,* Tingting Xiao,1,* Boyu Chi,1,2 Yu Wang,1 Lipeng Mao,1,2 Dabei Cai,1,2 Qingqing Gu,1 Qianwen Chen,1 Qingjie Wang,1 Yuan Ji,1 Ling Sun1,2 1Department of Cardiology, the Affiliated Changzhou Second People’s Hospital of Nanjing Medical University, Changzhou, Jiangsu, People’s Republic of China; 2Changzhou Clinical Medical College, Dalian Medical University, Dalian, Liaoning, People’s Republic of China*These authors contributed equally to this workCorrespondence: Ling Sun; Qingjie Wang, Department of Cardiology, the Affiliated Changzhou Second People’s Hospital of Nanjing Medical University, Changzhou, Jiangsu, 213003, People’s Republic of China, Email sunling85125@hotmail.com; wang-qingjie@hotmail.comBackground: Cardiac repair remains a thorny issue for survivors of acute myocardial infarction (AMI), due to the regenerative inertia of myocardial cells. Cell-free therapies, such as exosome transplantation, have become a potential strategy for myocardial injury. The aim of this study was to investigate the role of engineered exosomes in overexpressing Growth Differentiation Factor-15 (GDF-15) (GDF15-EVs) after myocardial injury, and their molecular mechanisms in cardiac repair.Methods: H9C2 cells were transfected with GDF-15 lentivirus or negative control. The exosomes secreted from H9C2 cells were collected and identified. The cellular apoptosis and autophagy of H2O2-injured H9C2 cells were assessed by Western blotting, TUNEL assay, electron microscopy, CCK-8 and caspase 3/7 assay. A rat model of AMI was constructed by ligating the left anterior descending artery. The anti-apoptotic, pro-angiogenic effects of GDF15-EVs treatment, as well as ensuing functional and histological recovery were evaluated. Then, mRNA sequencing was performed to identify the differentially expressed mRNAs after GDF15-EVs treatment.Results: GDF15-EVs inhibited apoptosis and promoted autophagy in H2O2 injured H9C2 cells. GDF15-EVs effectively decreased the infarct area and enhanced the cardiac function in rats with AMI. Moreover, GDF15-EVs hindered inflammatory cell infiltration, inhibited cell apoptosis, and promoted cardiac angiogenesis in rats with AMI. RNA sequence showed that telomerase reverse transcriptase (TERT) mRNA was upregulated in GDF15-EVs-treated H9C2 cells. AMPK signaling was activated after GDF15-EVs. Silencing TERT impaired the protective effects of GDF15-EVs on H2O2-injured H9C2 cells.Conclusion: GDF15-EVs could fulfil their protective effects against myocardial injury by upregulating the expression of TERT and activating the AMPK signaling pathway. GDF15-EVs might be exploited to design new therapies for AMI.Keywords: exosomes, growth differentiation factor-15, telomerase reverse transcriptase, acute myocardial infarction
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- 2024
12. The Transition Region between Brightest Cluster Galaxies and Intra-Cluster Light in Galaxy Groups and Clusters
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Contini, E., Chen, H. Z., and Gu, Q. S.
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Astrophysics - Astrophysics of Galaxies - Abstract
We take advantage of a state-of-art semi analytic model of galaxy formation, and the model presented in \citet{contini21a}, to investigate the mass distribution of Brightest Cluster Galaxies (BCGs) and Intra-Cluster Light (ICL) by addressing two points: (1) the region of transition between a BCG dominated distribution and an ICL dominated one, and; (2) the relation between the total BCG+ICL mass and the ICL one alone. We find the transition radius to be independent of both BCG+ICL and halo masses, with an average of 60$\pm$40 kpc, in good agreement with previous observational measurements, but given the large scatter, it can be considered as a sort of physical separation between the two components only on cluster scale. From the analysis of $M_{ICL}-M_{BCG+ICL}$ relation, we build a method able to extract the ICL mass directly from the knowledge of the BCG+ICL one. Given the large scatter on low mass systems, such method under/overpredicts the true value of the ICL in a significant way, up to a factor of three in the worst cases. On the other hand, for $\log M_{BCG+ICL}>12$ or $\log M_{Halo}>14$, the difference between the true value and the one extracted from the $M_{ICL}-M_{BCG+ICL}$ relation ranges between $\pm$30\%. We therefore suggest this relation as a reliable test for observational works aiming to isolate the ICL from the BCG, for systems hosted by haloes on cluster scale., Comment: 12 pages, 2 tables and 5 figures. Accepted for publications in ApJ. Small corrections after proof
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- 2022
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13. Neutrophil Percentage as a Potential Biomarker of Acute Kidney Injury Risk and Short-Term Prognosis in Patients with Acute Myocardial Infarction in the Elderly
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Chen Q, Gu Q, Yin A, Cai D, Xiao T, Wang Y, Ji Y, Wang Q, Wei J, and Sun L
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neutrophil percentage ,acute kidney injury ,acute myocardial infarction ,Geriatrics ,RC952-954.6 - Abstract
Qianwen Chen,1,* Qingqing Gu,1,* Anwen Yin,2,* Dabei Cai,1 Tingting Xiao,1 Yu Wang,1 Yuan Ji,1 Qingjie Wang,1 Jun Wei,3 Ling Sun1 1Department of Cardiology, the Affiliated Changzhou Second People’s Hospital of Nanjing Medical University, Changzhou, Jiangsu, 213000, People’s Republic of China; 2Department of Cardiology, the Affiliated Wuxi People’s Hospital of Nanjing Medical University, Wuxi, Jiangsu, 214023, People’s Republic of China; 3Department of Cardiovascular Surgery, the First Affiliated Hospital of Wannan Medical College, Wuhu, Anhui, 241000, People’s Republic of China*These authors contributed equally to this workCorrespondence: Qingjie Wang; Ling Sun, Department of Cardiology, the Affiliated Changzhou Second People’s Hospital of Nanjing Medical University, 29 Xinglong Alley, Changzhou, Jiangsu, 213003, People’s Republic of China, Email wang-qingjie@hotmail.com; sunling85125@hotmail.comObjective: This study aimed to explore the association of preoperative neutrophil percentage (NEUT%) with the risk of acute kidney injury (AKI) in patients with acute myocardial infarction (AMI) having undergone coronary interventional therapy.Methods: A single-center, retrospective and observational study was conducted. From December 2012 to June 2021, patients with AMI were enrolled and divided into AKI group and non-AKI group. The NEUT% in the two groups was compared. The association between NEUT% with the risk of post-AMI AKI was analyzed by univariate and multivariable logistic regression. Kaplan-Meier survival curve was drawn to evaluate the prognostic ability of NEUT% for short-term all-cause death following AMI.Results: A total of 3001 consecutive patients were enrolled with an average age of 64.38 years. AKI occurred in 327 (10.9%) patients. The NEUT% was higher in the AKI group than in the non-AKI group ([76.65± 11.43]% versus [73.22± 11.83]%, P< 0.001). NEUT% was also identified as an independent risk factor for AKI in AMI patients after adjustment (OR=1.021, 95% CI: 1.010– 1.033, P < 0.001). Compared with those at the lowest quartile of NEUT%, the patients at quartiles 2– 4 had a higher risk of AKI (P for trend = 0.003). The odds of AKI increased by 29.0% as NEUT% increased by 1 standard deviation (OR=1.290, 95% CI: 1.087– 1.531, P = 0.004). After a median of 35 days follow-up, 93 patients died. Patients with a higher NEUT% presented a higher risk of all-cause death after AMI (Log rank: χ2 =24.753, P< 0.001).Conclusion: In AMI patients, the peripheral blood NEUT% was positively associated with the odds of AKI and short-term all-cause mortality. NEUT% may provide physicians with more information about disease development and prognosis.Keywords: neutrophil percentage, acute kidney injury, acute myocardial infarction
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- 2024
14. Clozapine-Induced Severe Toxicity: Exploring the Pharmacokinetic Profile of Clozapine and Its Significance in Hemodynamic Instability – A Case Report
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Yu ZX, Pi Y, Chen MK, Dong DJ, and Gu Q
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clozapine ,toxicity ,pulse index continuous cardiac output ,picco ,hemoperfusion ,hp ,Medicine (General) ,R5-920 - Abstract
Zhu-Xi Yu, Yang Pi, Mei-Kai Chen, Dan-Jiang Dong, Qin Gu Department of Critical Care Medicine, the Affiliated Drum Tower Hospital of Nanjing University Medical School, Nanjing, Jiangsu, 21008, People’s Republic of ChinaCorrespondence: Qin Gu, Department of Critical Care Medicine, the Affiliated Drum Tower Hospital of Nanjing University Medical school, Nanjing, Jiangsu, 21008, People’s Republic of China, Tel +86-13705150348, Email guqin123456202206@163.comAbstract: Hemodynamic instability in patients with clozapine intoxication can indirectly reflect the serum concentration of clozapine.We have described a case of a 32-year-old pregnant woman who developed life-threatening clozapine toxicity at 28 weeks of gestation. The levels of clozapine and norclozapine in the serum were high. We initiated hemoperfusion(HP) and other detoxification therapies to remove the drug. The patient had severely dilated peripheral blood vessels, which led to cardiac symptoms such as fatal hypotension and uncontrollable tachycardia, resulting in very high cardiac output and elevated Central venous oxygen saturation (ScvO2). Pharmacological intervention significantly improved the hemodynamics.In light of our observations in the ongoing case, we posit that evaluating hemodynamic parameters before and after blood detoxification could serve as a valuable means to gauge effectiveness and provide guidance for treatment.Keywords: clozapine, toxicity, pulse index continuous cardiac output, PICCO, hemoperfusion, HP
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- 2024
15. Efficacy and Safety of Hydrogen Therapy in Patients with Early-Stage Interstitial Lung Disease: A Single-Center, Randomized, Parallel-Group Controlled Trial
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Tang C, Wang L, Chen Z, Yang J, Gao H, Guan C, Gu Q, He S, Yang F, Chen S, Ma L, Zhang Z, Zhao Y, Tang L, Xu Y, Hu Y, and Luo X
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hydrogen ,n-acetylcysteine ,interstitial lung disease ,therapeutic effects ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Chang Tang,1,2,* Lanting Wang,1,2,* Zihua Chen,1,2,* Jin Yang,1,2 Haiqing Gao,1,2 Chenggong Guan,1,2 Qiaozhi Gu,1,2 Shan He,1,2 Fanping Yang,1,2 Shengan Chen,1,2 Li Ma,1,2 Zhen Zhang,1,2 Ying Zhao,1,2 Lin Tang,1,2 Yu Xu,1,2 Yue Hu,3 Xiaoqun Luo1,2 1Department of Allergy & Immunology, Huashan Hospital Affiliated to Fudan University, Shanghai, People’s Republic of China; 2Department of Dermatology, Huashan Hospital Affiliated to Fudan University, Shanghai, People’s Republic of China; 3Department of Clinical Laboratory, Huashan Hospital Affiliated to Fudan University, Shanghai, People’s Republic of China*These authors contributed equally to this workCorrespondence: Xiaoqun Luo, 12 Wulumuqi Zhong Road, Jing’an District, Shanghai, People’s Republic of China, Tel +86 13918825230, Email luoxiaoqun913@126.comPurpose: Several in vivo experiments have shown that molecular hydrogen is a promising therapeutic agent for interstitial lung diseases (ILD). In this study, hydrogen therapy was investigated to determine whether it is superior to N-Acetylcysteine (NAC) for the treatment of patients with early-stage ILD.Patients and Methods: A prospective, single-center, randomized, controlled clinical trial was conducted in 87 patients with early-stage ILD. Hydrogen or NAC therapy was randomly assigned (1:1 ratio) to the eligible patients. The primary endpoint was the change in the high-resolution computed tomography (HRCT) and composite physiologic index (CPI) scores from baseline to week 48. Pulmonary function was evaluated as a secondary endpoint, and adverse events were recorded for safety analysis.Results: The rate of HRCT image improvement from the baseline in the HW group (63.6%) was higher than that in the NAC group (39.5%). A significant decrease in CPI and improvement in DLCO-sb were observed in the hydrogen group compared with those in the control group. Changes in other pulmonary function parameters, including FVC, FEV1, FEV1/FVC%, and TLC, were not significantly different between the two groups. Adverse events were reported in 7 (15.9%) patients in the HW group and 10 (23.3%) patients in the NAC group, but the difference was not significant (P=0.706).Conclusion: Hydrogen therapy exhibits superior efficacy and acceptable safety compared with NAC therapy in patients with early-stage ILD.Keywords: hydrogen, N-acetylcysteine, interstitial lung disease, therapeutic effects
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- 2023
16. APOL1 Induces Pyroptosis of Fibroblasts Through NLRP3/Caspase-1/GSDMD Signaling Pathway in Ulcerative Colitis
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Zhu F, Li S, Gu Q, Xie N, and Wu Y
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apolipoprotein l1 ,pyroptosis ,fibroblasts ,gasdermin-d ,ulcerative colitis ,Pathology ,RB1-214 ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Fangqing Zhu,1 Sheng Li,2 Qiuping Gu,1 Ningsheng Xie,1 Yinxia Wu3 1Department of Gastroenterology, Ganzhou People’s Hospital, Ganzhou, Jiangxi, 341000, People’s Republic of China; 2Department of Gastroenterology, Yuebei People’s Hospital, Shantou University Medical College, Shaoguan, Guangdong, 512026, People’s Republic of China; 3Department of Rehabilitation, Ganzhou People’s Hospital, Ganzhou, Jiangxi, 341000, People’s Republic of ChinaCorrespondence: Fangqing Zhu; Yinxia Wu, Email wanliqingkong0707@163.com; xiaflora0608@163.comBackground: Pyroptosis is a form of proinfammatory gasdermin-mediated programmed cell death. Abnormal infammation in the intestine is a critical risk factor for Ulcerative colitis (UC). However, at present, it is not clear whether pyroptosis of colonic fibroblasts is involved in the pathogenesis and progression of UC.Methods: In this study, key genes associated with UC were identified by bioinformatics analysis. Datasets were downloaded from the Gene Expression Omnibus (GEO) database (GSE193677). The differentially expressed genes were analyzed, and the hub genes were screened by weighted gene co-expression network analysis (WGCNA) and differentially expressed genes. We also downloaded the dataset from GEO for single-cell RNA sequencing (GSE231993). The expression of key genes was verified by immunohistochemistry, immunofluorescence and Western blot, and the specific pathways of key genes inducing pyroptosis in cell lines were explored.Results: The results of bioinformatics analysis showed that the expression of APOL1 and CXCL1 in UC tissues was significantly higher than that in normal tissues. The results of single-cell analysis showed that the two genes were co-localized to fibroblasts. These results were consistent with the results of immunohistochemistry and immunofluorescence colocalization in human intestinal mucosa specimens. Furthermore, APOL1 overexpression induced NLRP3-caspase1-GSDMD-mediated pyroptosis of fibroblasts, which was confirmed by Western blot.Conclusion: APOL1 induces pyroptosis of fibroblasts mediated by NLRP3-Caspase1-GSDMD signaling pathway and promote the release of chemokines CXCL1. Fibroblasts may play a crucial role in the pathogenesis and progression of UC.Keywords: apolipoprotein L1, pyroptosis, fibroblasts, gasdermin-D, Ulcerative colitis
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- 2023
17. The Relationship Between the Expression of CRBN in Peripheral Blood and the Severity and Prognosis of Adult Sepsis
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Kuang Z and Gu Q
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sepsis ,cereblon protein ,prognosis ,severity ,Medicine (General) ,R5-920 - Abstract
Zhiming Kuang,1 Qiuping Gu1,2 1Department of Critical Care Medicine, Ganzhou People’s Hospital, Ganzhou, Jiangxi Province, 341000, People’s Republic of China; 2Department of Gastroenterology, Ganzhou People’s Hospital, Ganzhou, Jiangxi Province, 341000, People’s Republic of ChinaCorrespondence: Qiuping Gu, Department of Gastroenterology, Ganzhou People’s Hospital, No. 16, Meiguan Avenue, Zhanggong District, Ganzhou City, Jiangxi Province, People’s Republic of China, Tel +86-18214932018, Email zhangdi2@mail.sdufe.edu.cnObjective: To investigate the correlation between the expression of cereblon (CRBN) protein in peripheral blood and the severity and prognosis of sepsis.Methods: A total of 130 patients with sepsis admitted to our hospital were selected as the observation subjects (sepsis group). The patients were divided into mild group, moderate group and severe group according to their conditions. The patients were divided into survival group and death group according to their living conditions within 28 days after admission. 130 health individuals were selected as the control group. The levels of CRBN mRNA, CRP and PCT in peripheral blood were detected.Results: The levels of serum CRBN mRNA, CRP, and PCT in patients with sepsis were higher than those in the control group (P< 0.05); As the condition worsens, the levels of CRBN mRNA, CRP, and PCT gradually increase, and there are statistically significant differences among patients with mild, moderate, and severe sepsis; Correlation analysis showed that the expression of CRBN mRNA in sepsis patients was positively correlated with CRP, PCT levels, APACHE II score and SOFA score (P< 0.05); the 28-day cumulative survival rate of patients with high CRBN mRNA expression was significantly lower than that of patients with low CRBN mRNA expression (P< 0.05); compared with the survival group, the levels of serum CRBN mRNA, CRP and PCT in the death group were significantly higher (P< 0.05); the AUC of death in sepsis patients diagnosed by CRBN mRNA, CRP and PCT was 0.961, the combined diagnostic efficacy was higher than that of single detection (P< 0.05).Conclusion: The expression level of CRBN in the peripheral blood of patients with sepsis is increased, which is related to the severity and prognosis of the patients. The combination of CRP and PCT has certain diagnostic value for the death of sepsis patients.Keywords: sepsis, cereblon protein, prognosis, severity
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- 2023
18. Combination of NK and Other Immune Markers at Early Phase Stratify the Risk of Sepsis Patients: A Retrospective Study
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Hu Z, Dong D, Peng F, Zhou X, Sun Q, Chen H, Chang W, Gu Q, Xie J, and Yang Y
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sepsis ,immune dysfunction ,natural killer cell ,hla-dr ,t cell ,Pathology ,RB1-214 ,Therapeutics. Pharmacology ,RM1-950 - Abstract
Zihan Hu,1,* Danjiang Dong,2,* Fei Peng,1,* Xing Zhou,1 Qin Sun,1 Hui Chen,1,3 Wei Chang,1 Qin Gu,2,* Jianfeng Xie,1,* Yi Yang1,* 1Jiangsu Provincial Key Laboratory of Critical Care Medicine, Department of Critical Care Medicine, Zhongda Hospital, School of Medicine, Southeast University, Nanjing, 210009, People’s Republic of China; 2Department of Critical Care Medicine, Nanjing Drum Tower Hospital, The Affiliated Hospital of Nanjing University Medical School, Nanjing, People’s Republic of China; 3Department of Critical Care Medicine, The First Affiliated Hospital of Soochow University, Soochow University, Suzhou, 215000, People’s Republic of China*These authors contributed equally to this workCorrespondence: Jianfeng Xie; Qin Gu, Department of Critical Care Medicine, Zhongda Hospital, School of medicine, Southeast University, 87 Dingjiaqiao Road, Nanjing, 210009, People’s Republic of China, Tel/Fax +00862583262500, Email xie820405@126.com; guqinicu012323@126.comPurpose: Immune dysfunction plays a pivotal role in sepsis pathogenesis. Previous studies have revealed the crucial role of T cells and human leukocyte antigen-DR (HLA-DR) in sepsis. However, the function of natural killer (NK) cells remains unclear. This study aimed to investigate whether NK cells are associated with sepsis prognosis. In addition, we aimed to explore the interrelation and influence between NK and other immunological features in patients with sepsis.Patients and Methods: This retrospective, observational study included patients with sepsis from two hospitals in mainland China. The clinical characteristics and immune results during the early phase were collected. Patients were classified according to the level of immune cells to analyze the relationship between immunological features and 28-day mortality.Results: A total of 984 patients were included in this study. Non-survivors were older and had lower levels of lymphocytes, monocytes, NK cells, HLA-DR, and T cells. Patients were classified into eight groups according to their levels of NK cells, HLA-DR, and T cells. Only patients with decreased NK and T cell counts showed a significant increase in 28-day mortality. An increase in CD8+ T cells was correlated with the alleviation of 28-day mortality only among patients with high NK cell levels.Conclusion: This study provides novel insights into the association between NK cells and 28-day mortality as well as the interrelation between NK cells and other immune cells in sepsis. The relationship between CD8+ T cells and 28-day mortality in sepsis is dependent on NK cell count.Keywords: sepsis, immune dysfunction, natural killer cell, HLA-DR, T cell
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- 2023
19. Dust polarized emission observations of NGC 6334; BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network
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Arzoumanian, D., Furuya, R., Hasegawa, T., Tahani, M., Sadavoy, S., Hull, C. L. H., Johnstone, D., Koch, P. M., Inutsuka, S. -i., Doi, Y., Hoang, T., Onaka, T., Iwasaki, K., Shimajiri, Y., Inoue, T., Peretto, N., André, P., Bastien, P., Berry, D., Chen, H. -R. V., Di Francesco, J., Eswaraiah, C., Fanciullo, L., Fissel, L. M., Hwang, J., Kang, J. -h., Kim, G., Kim, K. -T., Kirchschlager, F., Kwon, W., Lee, C. W., Liu, H. -L., Lyo, A. -R., Pattle, K., Soam, A., Tang, X., Whitworth, A., Ching, T. -C., Coudé, S., Wang, J. -W., Ward-Thompson, D., Lai, S. -P., Qiu, K., Bourke, T. L., Byun, D. -Y., Chen, M., Chen, Z., Chen, W. P., Cho, J., Choi, Y., Choi, M., Chrysostomou, A., Chung, E. J., Dai, S., Diep, P. N., Duan, H. -Y., Duan, Y., Eden, D., Fiege, J., Franzmann, E., Friberg, P., Fuller, G., Gledhill, T., Graves, S., Greaves, J., Griffin, M., Gu, Q., Han, I., Hatchell, J., Hayashi, S., Houde, M., Jeong, I. -G., Kang, M., Kang, S. -j., Kataoka, A., Kawabata, K., Kemper, F., Kim, M. -R., Kim, K. H., Kim, J., Kim, S., Kirk, J., Kobayashi, M. I. N., Konyves, V., Kusune, T., Kwon, J., Lacaille, K., Law, C. -Y., Lee, C. -F., Lee, Y. -H., Lee, S. -S., Lee, H., Lee, J. -E., Li, H. -b., Li, D., Liu, J., Liu, T., Liu, S. -Y., Lu, X., Mairs, S., Matsumura, M., Matthews, B., Moriarty-Schieven, G., Nagata, T., Nakamura, F., Nakanishi, H., Ngoc, N. B., Ohashi, N., Park, G., Parsons, H., Pyo, T. -S., Qian, L., Rao, R., Rawlings, J., Rawlings, M., Retter, B., Richer, J., Rigby, A., Saito, H., Savini, G., Scaife, A., Seta, M., Shinnaga, H., Tamura, M., Tang, Y. -W., Tomisaka, K., Tram, L. N., Tsukamoto, Y., Viti, S., Wang, H., Xie, J., Yen, H. -W., Yoo, H., Yuan, J., Yun, H. -S., Zenko, T., Zhang, G., Zhang, C. -P., Zhang, Y., Zhou, J., Zhu, L., de Looze, I., Dowell, C. D., Eyres, S., Falle, S., Friesen, R., Robitaille, J. -F., and van Loo, S.
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Astrophysics - Astrophysics of Galaxies - Abstract
[Abridged] Filaments and hubs have received special attention recently thanks to studies showing their role in star formation. While the column density and velocity structures of both filaments and hubs have been studied, their magnetic fields (B-field) are not yet characterized. We aim to understand the role of the B-field in the dynamical evolution of the NGC 6334 hub-filament network. We present new observations of the dust polarized emission at 850$\mu$m towards NGC 6334 obtained with the JCMT/POL-2. We study the distribution and dispersion of the polarized intensity ($PI$), the polarization fraction ($PF$), and the B-field angle ($\theta_{B}$). We derive the power spectrum of the intensity and $\theta_{B}$ along the ridge crest. Our analyses show a complex B-field structure when observed over the whole region ($\sim10$ pc), however, at smaller scales ($\sim1$ pc), $\theta_{B}$ varies coherently along the filaments. The observed power spectrum of $\theta_{B}$ can be well represented with a power law function with a slope $-1.33\pm0.23$, which is $\sim20\%$ shallower than that of $I$. This result is compatible with the properties of simulated filaments and may indicate the processes at play in the formation of filaments. $\theta_{B}$ rotates from being mostly perpendicular to the filament crests to mostly parallel as they merge with the hubs. This variation of $\theta_{B}$ may be tracing local velocity flows of matter in-falling onto the hubs. Our analysis suggests a variation of the energy balance along the crests of these filaments, from magnetically critical/supercritical at their far ends to magnetically subcritical near the hubs. We detect an increase of $PF$ towards the high-column density star cluster-forming hubs that may result from the increase of grain alignment efficiency due to stellar radiation from the newborn stars., Comment: Accepted for publication in Astronomy & Astrophysics
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- 2020
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20. The Tenth Visual Object Tracking VOT2022 Challenge Results
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Kristan, Matej, Leonardis, Aleš, Matas, Jiří, Felsberg, Michael, Pflugfelder, Roman, Kämäräinen, Joni-Kristian, Chang, Hyung Jin, Danelljan, Martin, Zajc, Luka Čehovin, Lukežič, Alan, Drbohlav, Ondrej, Björklund, Johanna, Zhang, Yushan, Zhang, Zhongqun, Yan, Song, Yang, Wenyan, Cai, Dingding, Mayer, Christoph, Fernández, Gustavo, Ben, Kang, Bhat, Goutam, Chang, Hong, Chen, Guangqi, Chen, Jiaye, Chen, Shengyong, Chen, Xilin, Chen, Xin, Chen, Xiuyi, Chen, Yiwei, Chen, Yu-Hsi, Chen, Zhixing, Cheng, Yangming, Ciaramella, Angelo, Cui, Yutao, Džubur, Benjamin, Dasari, Mohana Murali, Deng, Qili, Dhar, Debajyoti, Di, Shangzhe, Nardo, Emanuel Di, Du, Daniel K., Dunnhofer, Matteo, Fan, Heng, Feng, Zhenhua, Fu, Zhihong, Gao, Shang, Gorthi, Rama Krishna, Granger, Eric, Gu, Q. H., Gupta, Himanshu, He, Jianfeng, He, Keji, Huang, Yan, Jangid, Deepak, Ji, Rongrong, Jiang, Cheng, Jiang, Yingjie, Lawin, Felix Järemo, Kang, Ze, Kiran, Madhu, Kittler, Josef, Lai, Simiao, Lan, Xiangyuan, Lee, Dongwook, Lee, Hyunjeong, Lee, Seohyung, Li, Hui, Li, Ming, Li, Wangkai, Li, Xi, Li, Xianxian, Li, Xiao, Li, Zhe, Lin, Liting, Ling, Haibin, Liu, Bo, Liu, Chang, Liu, Si, Lu, Huchuan, Cruz, Rafael M. O., Ma, Bingpeng, Ma, Chao, Ma, Jie, Ma, Yinchao, Martinel, Niki, Memarmoghadam, Alireza, Micheloni, Christian, Moallem, Payman, Nguyen-Meidine, Le Thanh, Pan, Siyang, Park, ChangBeom, Paudel, Danda, Paul, Matthieu, Peng, Houwen, Robinson, Andreas, Rout, Litu, Shan, Shiguang, Simonato, Kristian, Song, Tianhui, Song, Xiaoning, Sun, Chao, Sun, Jingna, Tang, Zhangyong, Timofte, Radu, Tsai, Chi-Yi, Gool, Luc Van, Verma, Om Prakash, Wang, Dong, Wang, Fei, Wang, Liang, Wang, Liangliang, Wang, Lijun, Wang, Limin, Wang, Qiang, Wu, Gangshan, Wu, Jinlin, Wu, Xiaojun, Xie, Fei, Xu, Tianyang, Xu, Wei, Xu, Yong, Xu, Yuanyou, Xue, Wanli, Xun, Zizheng, Yan, Bin, Yang, Dawei, Yang, Jinyu, Yang, Wankou, Yang, Xiaoyun, Yang, Yi, Yang, Yichun, Yang, Zongxin, Ye, Botao, Yu, Fisher, Yu, Hongyuan, Yu, Jiaqian, Yu, Qianjin, Yu, Weichen, Ze, Kang, Zhai, Jiang, Zhang, Chengwei, Zhang, Chunhu, Zhang, Kaihua, Zhang, Tianzhu, Zhang, Wenkang, Zhang, Zhibin, Zhang, Zhipeng, Zhao, Jie, Zhao, Shaochuan, Zheng, Feng, Zheng, Haixia, Zheng, Min, Zhong, Bineng, Zhu, Jiawen, Zhu, Xuefeng, Zhuang, Yueting, Goos, Gerhard, Founding Editor, Hartmanis, Juris, Founding Editor, Bertino, Elisa, Editorial Board Member, Gao, Wen, Editorial Board Member, Steffen, Bernhard, Editorial Board Member, Yung, Moti, Editorial Board Member, Karlinsky, Leonid, editor, Michaeli, Tomer, editor, and Nishino, Ko, editor
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- 2023
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21. The Roles of Mass and Environment in the Quenching of Galaxies. II
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Contini, E., Gu, Q., Ge, X., Rhee, J., Yi, S. K., and Kang, X.
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Astrophysics - Astrophysics of Galaxies - Abstract
We take advantage of an analytic model of galaxy formation coupled to the merger tree of an N-body simulation to study the roles of environment and stellar mass in the quenching of galaxies. The model has been originally set in order to provide the observed evolution of the stellar mass function as well as reasonable predictions of the star formation rate-stellar mass relation, from high redshift to the present time. We analyse the stellar mass and environmental quenching efficiencies and their dependence on stellar mass, halo mass (taken as a proxy for the environment) and redshift. Our analysis shows that the two quenching efficiencies are redshift, stellar and halo mass dependent, and that the halo mass is also a good proxy for the environment. The environmental quenching increases with decreasing redshift and is inefficient below $\log M_* \sim 9.5$, reaches the maximum value at $\log M_* \sim 10.5$, and decreases again, becoming poorly efficient at very high stellar mass ($\log M_* \gtrsim 11.5$). Central and satellites galaxies are mass quenched differently: for the former, the quenching efficiency depends very weakly on redshift, but strongly on stellar mass; for the latter, it strongly depends on both stellar mass and redshift in the range $10\lesssim \log M_* \lesssim 11$. According to the most recent observational results, we find that the two quenching efficiencies are not separable: intermediate mass galaxies are environmental quenched faster, as well as intermediate/massive galaxies in more massive haloes. At stellar masses lower than $\log M_* \lesssim 9.5$ both quenching mechanisms become inefficient, independently of the redshift., Comment: 13 pages, 8 figures, accepted for publication in ApJ, minor revision after Proof correction
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- 2020
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22. Effect of PD-L1 Expression for the PD-1/L1 Inhibitors on Non-small Cell Lung Cancer: A Meta-analysis Based on Randomised Controlled Trials
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Xu, Z., Liang, J., Fu, R., Yang, L., Xin Chen, Y., Ren, W., Lu, Y., Qiu, X., and Gu, Q.
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- 2023
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23. Experimental evidence of crystal symmetry protection for the topological nodal line semimetal state in ZrSiS
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Gu, C. C., Hu, J., Chen, X. L., Guo, Z. P., Fu, B. T., Zhou, Y. H., An, C., Zhou, Y., Zhang, R. R., Xi, C. Y., Gu, Q. Y., Park, C., Shu, H. Y., Yang, W. G., Pi, L., Zhang, Y. H., Yao, Y. G., Yang, Z. R., Zhou, J. H., Sun, J., Mao, Z. Q., and Tian, M. L.
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Condensed Matter - Materials Science - Abstract
Tunable symmetry breaking plays a crucial role for the manipulation of topological phases of quantum matter. Here, through combined high-pressure magneto-transport measurements, Raman spectroscopy, and X-ray diffraction, we demonstrate a pressure-induced topological phase transition in nodal-line semimetal ZrSiS. Symmetry analysis and first-principles calculations suggest that this pressure-induced topological phase transition may be attributed to weak lattice distortions by non-hydrostatic compression, which breaks some crystal symmetries, such as the mirror and inversion symmetries. This finding provides some experimental evidence for crystal symmetry protection for the topological semimetal state, which is at the heart of topological relativistic fermion physics., Comment: 27 pages, 17 figures
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- 2019
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24. The Roles of Mass and Environment in the Quenching of Galaxies
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Contini, E., Gu, Q., Kang, X., Rhee, J., and Yi, S. K.
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Astrophysics - Astrophysics of Galaxies - Abstract
We study the roles of stellar mass and environment in quenching the star formation activity of a large set of simulated galaxies by taking advantage of an analytic model coupled to the merger tree extracted from an N-body simulation. The analytic model has been set to match the evolution of the global stellar mass function since redshift $z\sim 2.3$ and give reasonable predictions of the star formation history of galaxies at the same time. We find that stellar mass and environment play different roles: the star formation rate/specific star formation rate-$M_*$ relations are independent of the environment (defined as the halo mass) at any redshift probed, $0
1$ as generally claimed, while the environment has a minimal role. All the physical processes linked to the environment must act on very short timescales, such that they do not influence the star formation of active galaxies, but increase the probability of a given galaxy to become quiescent., Comment: 13 pages, 8 figures, accepted for publication in ApJ - Published
- 2019
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25. Exploring the origin of multiwavelength activities of high-redshift FSRQ PKS 1502+106 during 2014-2018
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Ding, N., Gu, Q. S., Geng, X. F., Xiong, Ding-Rong, Xue, R., Wang, X. Y., and Guo, X. T.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The origin of the multi-band activities (outbursts/flares) of blazars is still a heavily debated topic. Shock and magnetic reconnection have long been considered as possible triggers for the multi-band activities. In this paper, we present an exploration of the origin of multi-band activities for a high-redshift (z =1.8385) FSRQ PKS 1502+106. Utilizing multi-band data from radio to $\gamma$-ray and optical polarization observations, we investigate two dramatic activities in detail: a $\gamma$-ray dominated outburst in 2015 and an optical dominated outburst in 2017. Our main results are as follows. (I) A fast $\gamma$-ray flare with a flux-doubling time-scale as short as 1-hr in 2015 is discovered. Based on the variability time-scale, the physical parameters of the flaring region (e.g, minimum Doppler factor, emission region size, etc.) are constrained. At the peak of the flare, the $\gamma$-ray spectrum hardens to $\Gamma_{\gamma} = 1.82\pm0.04$ and exhibits an obvious curvature/break characteristic that is caused by the typical "cooling break". Modelings of multi-band SEDs reveal a very hard electronic energy spectrum with the electronic spectral index of $1.07\pm0.53$. This result suggests that this fast $\gamma$-ray flare may be triggered by magnetic reconnection. (II) During the outburst in 2017, the optical polarization degree and optical fluxes show a very tight correlation. By analyzing Stokes parameters of polarization observations, our results show that this outburst could be triggered by a transverse shock with a compression ratio of $\eta> 2.2$, and the magnetic field intensity of the shock emission region is about $0.032$ G., Comment: 18 pages, 13 figures, 5 tables, accepted by ApJ
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- 2019
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26. Discovery of four apparently cold dusty galaxies at z=3.62-5.85 in the COSMOS field: direct evidence of CMB impact on high-redshift galaxy observables
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Jin, S., Daddi, E., Magdis, G. E., Liu, D., Schinnerer, E., Papadopoulos, P. P., Gu, Q., Gao, Y., and Calabro, A.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We report Atacama Large Millimetre Array (ALMA) observations of four high-redshift dusty star-forming galaxy candidates selected from far-Infrared (FIR)/submm observations in the COSMOS field. We securely detect all galaxies in the continuum and spectroscopically confirm them at z=3.62--5.85 using ALMA 3mm line scans, detecting multiple CO and/or [CI] transitions. This includes the most distant dusty galaxy currently known in the COSMOS field, ID85001929 at z=5.847. These redshifts are lower than we had expected as these galaxies have substantially colder dust temperatures (i.e., their SEDs peak at longer rest frame wavelengths) than most literature sources at z>4. The observed cold dust temperatures are best understood as evidence for optically thick dust continuum in the FIR, rather than the result of low star formation efficiency with rapid metal enrichment. We provide direct evidence that, given their cold spectral energy distributions, CMB plays a significant role biasing their observed Rayleigh-Jeans (RJ) slopes to unlikely steep values and, possibly, reducing their CO fluxes by a factor of two. We recover standard RJ slopes when the CMB contribution is taken into account. High resolution ALMA imaging shows compact morphology and evidence for mergers. This work reveals a population of cold dusty star-forming galaxies that were under-represented in current surveys, and are even colder than typical Main Sequence galaxies at the same redshift. High FIR dust optical depth might be a widespread feature of compact starbursts at any redshift., Comment: 13 pages, 8 figures, 4 tables, accepted for publication in ApJ
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- 2019
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27. The Compact Linear Collider (CLIC) - 2018 Summary Report
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CLIC, The, collaborations, CLICdp, Charles, T. K., Giansiracusa, P. J., Lucas, T. G., Rassool, R. P., Volpi, M., Balazs, C., Afanaciev, K., Makarenko, V., Patapenka, A., Zhuk, I., Collette, C., Boland, M. J., Hoffman, A. C. Abusleme, Diaz, M. A., Garay, F., Chi, Y., He, X., Pei, G., Pei, S., Shu, G., Wang, X., Zhang, J., Zhao, F., Zhou, Z., Chen, H., Gao, Y., Huang, W., Kuang, Y. P., Li, B., Li, Y., Meng, X., Shao, J., Shi, J., Tang, C., Wang, P., Wu, X., Zha, H., Ma, L., Han, Y., Fang, W., Gu, Q., Huang, D., Huang, X., Tan, J., Wang, Z., Zhao, Z., Uggerhøj, U. I., Wistisen, T. N., Aabloo, A., Aare, R., Kuppart, K., Vigonski, S., Zadin, V., Aicheler, M., Baibuz, E., Brücken, E., Djurabekova, F., Eerola, P., Garcia, F., Haeggström, E., Huitu, K., Jansson, V., Kassamakov, I., Kimari, J., Kyritsakis, A., Lehti, S., Meriläinen, A., Montonen, R., Nordlund, K., Österberg, K., Saressalo, A., Väinölä, J., Veske, M., Farabolini, W., Mollard, A., Peauger, F., Plouin, J., Bambade, P., Chaikovska, I., Chehab, R., Delerue, N., Davier, M., Faus-Golfe, A., Irles, A., Kaabi, W., LeDiberder, F., Pöschl, R., Zerwas, D., Aimard, B., Balik, G., Blaising, J. -J., Brunetti, L., Chefdeville, M., Dominjon, A., Drancourt, C., Geoffroy, N., Jacquemier, J., Jeremie, A., Karyotakis, Y., Nappa, J. M., Serluca, M., Vilalte, S., Vouters, G., Bernhard, A., Bründermann, E., Casalbuoni, S., Hillenbrand, S., Gethmann, J., Grau, A., Huttel, E., Müller, A. -S., Peiffer, P., Perić, I., de Jauregui, D. Saez, Emberger, L., Graf, C., Simon, F., Szalay, M., van der Kolk, N., Brass, S., Kilian, W., Alexopoulos, T., Apostolopoulos, T., Gazis, E. N., Gazis, N., Kostopoulos, V., Kourkoulis, S., Heilig, B., Lichtenberger, J., Shrivastava, P., Dayyani, M. K., Ghasem, H., Hajari, S. S., Shaker, H., Ashkenazy, Y., Popov, I., Engelberg, E., Yashar, A., Abramowicz, H., Benhammou, Y., Borysov, O., Borysova, M., Levy, A., Levy, I., Alesini, D., Bellaveglia, M., Buonomo, B., Cardelli, A., Diomede, M., Ferrario, M., Gallo, A., Ghigo, A., Giribono, A., Piersanti, L., Stella, A., Vaccarezza, C., de Blas, J., Franceschini, R., D'Auria, G., Di Mitri, S., Abe, T., Aryshev, A., Fukuda, M., Furukawa, K., Hayano, H., Higashi, Y., Higo, T., Kubo, K., Kuroda, S., Matsumoto, S., Michizono, S., Naito, T., Okugi, T., Shidara, T., Tauchi, T., Terunuma, N., Urakawa, J., Yamamoto, A., Raboanary, R., Luiten, O. J., Stragier, X. F. D., Hart, R., van der Graaf, H., Eigen, G., Adli, E., Lindstrøm, C. A., Lillestøl, R., Malina, L., Pfingstner, J., Sjobak, K. N., Ahmad, A., Hoorani, H., Khan, W. A., Bugiel, S., Bugiel, R., Firlej, M., Fiutowski, T. A., Idzik, M., Moroń, J., Świentek, K. P., de Renstrom, P. Brückman, Krupa, B., Kucharczyk, M., Lesiak, T., Pawlik, B., Sopicki, P., Turbiarz, B., Wojtoń, T., Zawiejski, L. K., Kalinowski, J., Nowak, K., Żarnecki, A. F., Firu, E., Ghenescu, V., Neagu, A. T., Preda, T., Zgura, I. S., Aloev, A., Azaryan, N., Boyko, I., Budagov, J., Chizhov, M., Filippova, M., Glagolev, V., Gongadze, A., Grigoryan, S., Gudkov, D., Karjavine, V., Lyablin, M., Nefedov, Yu., Olyunin, A., Rymbekova, A., Samochkine, A., Sapronov, A., Shelkov, G., Shirkov, G., Soldatov, V., Solodko, E., Trubnikov, G., Tyapkin, I., Uzhinsky, V., Vorozhtov, A., Zhemchugov, A., Levichev, E., Mezentsev, N., Piminov, P., Shatilov, D., Vobly, P., Zolotarev, K., Jelisavčić, I. Božović, Kačarević, G., Dumbelović, G. Milutinović, Pandurović, M., Radulović, M., Stevanović, J., Vukasinović, N., Lee, D. -H., Ayala, N., Benedetti, G., Guenzel, T., Iriso, U., Marti, Z., Perez, F., Pont, M., Trenado, J., Ruiz-Jimeno, A., Vila, I., Calero, J., Dominguez, M., Garcia-Tabares, L., Gavela, D., Lopez, D., Toral, F., Gutierrez, C. Blanch, Boronat, M., Esperante, D., Fullana, E., Fuster, J., García, I., Gimeno, B., Lopez, P. Gomis, González, D., Perelló, M., Ros, E., Villarejo, M. A., Vnuchenko, A., Vos, M., Borgmann, Ch., Brenner, R., Ekelöf, T., Jacewicz, M., Olvegård, M., Ruber, R., Ziemann, V., Aguglia, D., Gonzalvo, J. Alabau, Leon, M. Alcaide, Tehrani, N. Alipour, Anastasopoulos, M., Andersson, A., Andrianala, F., Antoniou, F., Apyan, A., Arominski, D., Artoos, K., Assly, S., Atieh, S., Baccigalupi, C., Sune, R. Ballabriga, Caballero, D. Banon, Barnes, M. J., Garcia, J. Barranco, Bartalesi, A., Bauche, J., Bayar, C., Belver-Aguilar, C., Morell, A. Benot, Bernardini, M., Bett, D. R., Bettoni, S., Bettencourt, M., Bielawski, B., Garcia, O. Blanco, Kraljevic, N. Blaskovic, Bolzon, B., Bonnin, X. A., Bozzini, D., Branger, E., Brondolin, E., Brunner, O., Buckland, M., Bursali, H., Burkhardt, H., Caiazza, D., Calatroni, S., Campbell, M., Lasheras, N. Catalan, Cassany, B., Castro, E., Soares, R. H. Cavaleiro, Bastos, M. Cerqueira, Cherif, A., Chevallay, E., Cilento, V., Corsini, R., Costa, R., Cure, B., Curt, S., Gobbo, A. Dal, Dannheim, D., Daskalaki, E., Deacon, L., Degiovanni, A., De Michele, G., De Oliveira, L., Romano, V. Del Pozo, Delahaye, J. P., Delikaris, D., de Almeida, P. G. Dias, Dobers, T., Doebert, S., Doytchinov, I., Draper, M., Ramos, F. Duarte, Duquenne, M., Plaja, N. Egidos, Elsener, K., Esberg, J., Esposito, M., Evans, L., Fedosseev, V., Ferracin, P., Fiergolski, A., Foraz, K., Fowler, A., Friebel, F., Fuchs, J-F., Gaddi, A., Gamba, D., Fajardo, L. Garcia, Morales, H. Garcia, Garion, C., Gasior, M., Gatignon, L., Gayde, J-C., Gerbershagen, A., Gerwig, H., Giambelli, G., Gilardi, A., Goldblatt, A. N., Anton, S. Gonzalez, Grefe, C., Grudiev, A., Guerin, H., Guillot-Vignot, F. G., Gutt-Mostowy, M. L., Lutz, M. Hein, Hessler, C., Holma, J. K., Holzer, E. B., Hourican, M., Hynds, D., Ikarios, E., Levinsen, Y. Inntjore, Janssens, S., Jeff, A., Jensen, E., Jonker, M., Kamugasa, S. W., Kastriotou, M., Kemppinen, J. M. K., Khan, V., Kieffer, R. B., Klempt, W., Kokkinis, N., Kossyvakis, I., Kostka, Z., Korsback, A., Platia, E. Koukovini, Kovermann, J. W., Kozsar, C-I., Kremastiotis, I., Kröger, J., Kulis, S., Latina, A., Leaux, F., Lebrun, P., Lefevre, T., Leogrande, E., Linssen, L., Liu, X., Cudie, X. Llopart, Magnoni, S., Maidana, C., Maier, A. A., Durand, H. Mainaud, Mallows, S., Manosperti, E., Marelli, C., Lacoma, E. Marin, Marsh, S., Martin, R., Martini, I., Martyanov, M., Mazzoni, S., Mcmonagle, G., Mether, L. M., Meynier, C., Modena, M., Moilanen, A., Mondello, R., Cabral, P. B. Moniz, Irazabal, N. Mouriz, Munker, M., Muranaka, T., Nadenau, J., Navarro, J. G., Quirante, J. L. Navarro, Del Busto, E. Nebo, Nikiforou, N., Ninin, P., Nonis, M., Nisbet, D., Nuiry, F. X., Nürnberg, A., Ögren, J., Osborne, J., Ouniche, A. C., Pan, R., Papadopoulou, S., Papaphilippou, Y., Paraskaki, G., Pastushenko, A., Passarelli, A., Patecki, M., Pazdera, L., Pellegrini, D., Pepitone, K., Codina, E. Perez, Fontenla, A. Perez, Persson, T. H. B., Petrič, M., Pitman, S., Pitters, F., Pittet, S., Plassard, F., Popescu, D., Quast, T., Rajamak, R., Redford, S., Remandet, L., Renier, Y., Rey, S. F., Orozco, O. Rey, Riddone, G., Castro, E. Rodriguez, Roloff, P., Rossi, C., Rossi, F., Rude, V., Ruehl, I., Rumolo, G., Sailer, A., Sandomierski, J., Santin, E., Sanz, C., Bedolla, J. Sauza, Schnoor, U., Schmickler, H., Schulte, D., Senes, E., Serpico, C., Severino, G., Shipman, N., Sicking, E., Simoniello, R., Skowronski, P. K., Mompean, P. Sobrino, Soby, L., Sollander, P., Solodko, A., Sosin, M. P., Spannagel, S., Sroka, S., Stapnes, S., Sterbini, G., Stern, G., Ström, R., Stuart, M. J., Syratchev, I., Szypula, K., Tecker, F., Thonet, P. A., Thrane, P., Timeo, L., Tiirakari, M., Garcia, R. Tomas, Tomoiaga, C. I., Valerio, P., Vaňát, T., Vamvakas, A. L., Van Hoorne, J., Viazlo, O., Pinto, M. Vicente Barreto, Vitoratou, N., Vlachakis, V., Weber, M. A., Wegner, R., Wendt, M., Widorski, M., Williams, O. E., Williams, M., Woolley, B., Wuensch, W., Wulzer, A., Uythoven, J., Xydou, A., Yang, R., Zelios, A., Zhao, Y., Zisopoulos, P., Benoit, M., Sultan, D M S, Riva, F., Bopp, M., Braun, H. H., Craievich, P., Dehler, M., Garvey, T., Pedrozzi, M., Raguin, J. Y., Rivkin, L., Zennaro, R., Guillaume, S., Rothacher, M., Aksoy, A., Nergiz, Z., Yavas, Ö., Denizli, H., Keskin, U., Oyulmaz, K. Y., Senol, A., Ciftci, A. K., Baturin, V., Karpenko, O., Kholodov, R., Lebed, O., Lebedynskyi, S., Mordyk, S., Musienko, I., Profatilova, Ia., Storizhko, V., Bosley, R. R., Price, T., Watson, M. F., Watson, N. K., Winter, A. G., Goldstein, J., Green, S., Marshall, J. S., Thomson, M. A., Xu, B., You, T., Gillespie, W. A., Spannowsky, M., Beggan, C., Martin, V., Zhang, Y., Protopopescu, D., Robson, A., Apsimon, R. J., Bailey, I., Burt, G. C., Dexter, A. C., Edwards, A. V., Hill, V., Jamison, S., Millar, W. L., Papke, K., Casse, G., Vossebeld, J., Aumeyr, T., Bergamaschi, M., Bobb, L., Bosco, A., Boogert, S., Boorman, G., Cullinan, F., Gibson, S., Karataev, P., Kruchinin, K., Lekomtsev, K., Lyapin, A., Nevay, L., Shields, W., Snuverink, J., Towler, J., Yamakawa, E., Boisvert, V., West, S., Jones, R., Joshi, N., Bett, D., Bodenstein, R. M., Bromwich, T., Burrows, P. N., Christian, G. B., Gohil, C., Korysko, P., Paszkiewicz, J., Perry, C., Ramjiawan, R., Roberts, J., Coates, T., Salvatore, F., Bainbridge, A., Clarke, J. A., Krumpa, N., Shepherd, B. J. A., Walsh, D., Chekanov, S., Demarteau, M., Gai, W., Liu, W., Metcalfe, J., Power, J., Repond, J., Weerts, H., Xia, L., Zupan, J., Wells, J. D., Zhang, Z., Adolphsen, C., Barklow, T., Dolgashev, V., Franzi, M., Graf, N., Hewett, J., Kemp, M., Kononenko, O., Markiewicz, T., Moffeit, K., Neilson, J., Nosochkov, Y., Oriunno, M., Phinney, N., Rizzo, T., Tantawi, S., Wang, J., Weatherford, B., White, G., and Woodley, M.
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Physics - Accelerator Physics - Abstract
The Compact Linear Collider (CLIC) is a TeV-scale high-luminosity linear $e^+e^-$ collider under development at CERN. Following the CLIC conceptual design published in 2012, this report provides an overview of the CLIC project, its current status, and future developments. It presents the CLIC physics potential and reports on design, technology, and implementation aspects of the accelerator and the detector. CLIC is foreseen to be built and operated in stages, at centre-of-mass energies of 380 GeV, 1.5 TeV and 3 TeV, respectively. CLIC uses a two-beam acceleration scheme, in which 12 GHz accelerating structures are powered via a high-current drive beam. For the first stage, an alternative with X-band klystron powering is also considered. CLIC accelerator optimisation, technical developments and system tests have resulted in an increased energy efficiency (power around 170 MW) for the 380 GeV stage, together with a reduced cost estimate at the level of 6 billion CHF. The detector concept has been refined using improved software tools. Significant progress has been made on detector technology developments for the tracking and calorimetry systems. A wide range of CLIC physics studies has been conducted, both through full detector simulations and parametric studies, together providing a broad overview of the CLIC physics potential. Each of the three energy stages adds cornerstones of the full CLIC physics programme, such as Higgs width and couplings, top-quark properties, Higgs self-coupling, direct searches, and many precision electroweak measurements. The interpretation of the combined results gives crucial and accurate insight into new physics, largely complementary to LHC and HL-LHC. The construction of the first CLIC energy stage could start by 2026. First beams would be available by 2035, marking the beginning of a broad CLIC physics programme spanning 25-30 years., Comment: 112 pages, 59 figures; published as CERN Yellow Report Monograph Vol. 2/2018; corresponding editors: Philip N. Burrows, Nuria Catalan Lasheras, Lucie Linssen, Marko Petri\v{c}, Aidan Robson, Daniel Schulte, Eva Sicking, Steinar Stapnes
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- 2018
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28. Variability-selected low-luminosity active galactic nuclei candidates in the 7 Ms Chandra Deep Field-South
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Ding, N., Luo, B., Brandt, W. N., Paolillo, M., Yang, G., Lehmer, B. D., Shemmer, O., Schneider, D. P., Tozzi, P., Xue, Y. Q., Zheng, X. C., Gu, Q. S., Koekemoer, A. M., Vignali, C., Vito, F., and Wang, J. X.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Astrophysics of Galaxies - Abstract
In deep X-ray surveys, active galactic nuclei (AGNs) with a broad range of luminosities have been identified. However, cosmologically distant low-luminosity AGN (LLAGN, $L_{\mathrm{X}} \lesssim 10^{42}$ erg s$^{-1}$) identification still poses a challenge due to significant contamination from host galaxies. Based on the 7 Ms Chandra Deep Field-South (CDF-S) survey, the longest timescale ($\sim 17$ years) deep X-ray survey to date, we utilize an X-ray variability selection technique to search for LLAGNs that remain unidentified among the CDF-S X-ray sources. We find 13 variable sources from 110 unclassified CDF-S X-ray sources. Except for one source which could be an ultraluminous X-ray source, the variability of the remaining 12 sources is most likely due to accreting supermassive black holes. These 12 AGN candidates have low intrinsic X-ray luminosities, with a median value of $7 \times10^{40}$ erg s$^{-1}$. They are generally not heavily obscured, with an average effective power-law photon index of 1.8. The fraction of variable AGNs in the CDF-S is independent of X-ray luminosity and is only restricted by the total number of observed net counts, confirming previous findings that X-ray variability is a near-ubiquitous property of AGNs over a wide range of luminosities. There is an anti-correlation between X-ray luminosity and variability amplitude for high-luminosity AGNs, but as the luminosity drops to $\lesssim 10^{42}$ erg s$^{-1}$, the variability amplitude no longer appears dependent on the luminosity. The entire observed luminosity-variability trend can be roughly reproduced by an empirical AGN variability model based on a broken power-law power spectral density function., Comment: 18 pages, 11 figures, accepted for publication in ApJ
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- 2018
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29. An improved boundary condition at a low grid resolution and Reynolds number
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Burel, T. and Gu, Q.
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Physics - Fluid Dynamics ,Physics - Computational Physics - Abstract
Complex geometries can be easily treated using the well-known full-way and half-way bounce-back rules. However, the accuracy of the full-way bounce-back rule is one order lower than the half-way bounce-back rule. Moreover, when the walls are not aligned with the lattices, the errors increase. Including the collision operator on the walls with the full-way bounce-back rule leads to an improvement of the accuracy of the pressure-drop, but, a loss of momentum is observed on concave corners. We propose to improve the momentum conservation by adding an extrapolation of the density by the inverse distance weighting at concave corners. The technique is shown to give a second-order accuracy at a lower grid resolution, thus, the computational cost can be reduced.
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- 2018
30. A holistic perspective on the dynamics of G035.39-00.33: the interplay between gas and magnetic fields
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Liu, Tie, Li, Pak Shing, Juvela, Mika, Kim, Kee-Tae, Evans II, Neal J., Di Francesco, James, Liu, Sheng-Yuan, Yuan, Jinghua, Tatematsu, Ken'ichi, Zhang, Qizhou, Ward-Thompson, Derek, Fuller, Gary, Goldsmith, Paul F., Koch, P. M., Sanhueza, Patricio, Ristorcelli, I., Kang, Sung-ju, Chen, Huei-Ru, Hirano, N., Wu, Yuefang, Sokolov, Vlas, Lee, Chang Won, White, Glenn J., Wang, Ke, Eden, David, Li, Di, Thompson, Mark, Pattle, Kate M, Soam, Archana, Nasedkin, Evert, Kim, Jongsoo, Kim, Gwanjeong, Lai, Shih-Ping, Park, Geumsook, Qiu, Keping, Zhang, Chuan-Peng, Alina, Dana, Eswaraiah, Chakali, Falgarone, Edith, Fich, Michel, Greaves, Jane, Gu, Q. -L., Kwon, Woojin, Li, Hua-bai, Malinen, Johanna, Montier, Ludovic, Parsons, Harriet, Qin, Sheng-Li, Rawlings, Mark G., Ren, Zhi-Yuan, Tang, Mengyao, Tang, Y. -W., Toth, L. V., Wang, Jiawei, Wouterloot, Jan, Yi, H. -W., and Zhang, H. -W.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Solar and Stellar Astrophysics - Abstract
Magnetic field is one of the key agents that play a crucial role in shaping molecular clouds and regulating star formation, yet the complete information on the magnetic field is not well constrained due to the limitations in observations. We study the magnetic field in the massive infrared dark cloud G035.39-00.33 from dust continuum polarization observations at 850 $\micron$ with SCUBA-2/POL-2 at JCMT. The magnetic field tends to be perpendicular to the densest part of the main filament (F$_{M}$), whereas it has a less defined relative orientation in the rest of the structure, where it tends to be parallel to some diffuse regions. A mean plane-of-the-sky magnetic field strength of $\sim$50 $\mu$G for F$_{M}$ is obtained using Davis-Chandrasekhar-Fermi method. Based on $^{13}$CO (1-0) line observations, we suggest a formation scenario of F$_{M}$ due to large-scale ($\sim$10 pc) cloud-cloud collision. Using additional NH$_3$ line data, we estimate that F$_{M}$ will be gravitationally unstable if it is only supported by thermal pressure and turbulence. The northern part of F$_{M}$, however, can be stabilized by a modest additional support from the local magnetic field. The middle and southern parts of F$_{M}$ are likely unstable even if the magnetic field support is taken into account. We claim that the clumps in F$_{M}$ may be supported by turbulence and magnetic fields against gravitational collapse. Finally, we identified for the first time a massive ($\sim$200 M$_{\sun}$), collapsing starless clump candidate, "c8", in G035.39-00.33. The magnetic field surrounding "c8" is likely pinched, hinting at an accretion flow along the filament., Comment: Published on ApJ, 27 pages
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- 2018
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31. Radio selection of the most distant galaxy clusters
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Daddi, E., Jin, S., Strazzullo, V., Sargent, M. T., Wang, T., Ferrari, C., Schinnerer, E., Smolcic, V., Calabro, A., Coogan, R., Delhaize, J., Delvecchio, I., Elbaz, D., Gobat, R., Gu, Q., Liu, D., Novak, M., and Valentino, F.
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Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
We show that the most distant X-ray detected cluster known to date, ClJ1001 at z=2.506, hosts a strong overdensity of radio sources. Six of them are individually detected (within 10") in deep 0.75" resolution VLA 3GHz imaging, with S(3GHz)>8uJy. Of the six, AGN likely affects the radio emission in two galaxies while star formation is the dominant source powering the remaining four. We searched for cluster candidates over the full COSMOS 2-square degree field using radio-detected 3GHz sources and looking for peaks in Sigma5 density maps. ClJ1001 is the strongest overdensity by far with >10sigma, with a simple z_phot>1.5 preselection. A cruder photometric rejection of z<1 radio foregrounds leaves ClJ1001 as the second strongest overdensity, while even using all radio sources ClJ1001 remains among the four strongest projected overdensities. We conclude that there are great prospects for future, deep and wide-area radio surveys to discover large samples of the first generation of forming galaxy clusters. In these remarkable structures widespread star formation and AGN activity of massive galaxy cluster members, residing within the inner cluster core, will ultimately lead to radio continuum as one of the most effective means for their identification, with detection rates expected in the ballpark of 0.1-1 per square degree at z>2.5. Samples of hundreds such high-redshift clusters could potentially constrain cosmological parameters and test cluster and galaxy formation models., Comment: ApJ Letters in press
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- 2017
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32. Crystal structure and thermochromic behavior of the quasi-0D lead-free organic-inorganic hybrid compounds (C7H9NF)8M4I16 (M = Bi, Sb)
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Zhao, X.C., Fu, Y.K., Lei, Y.L., Wong-Ng, Winnie, Wang, C., Gu, Q., Zhou, W., Wang, S.Y., and Liu, W.F.
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- 2022
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33. Unraveling the Role of Base and Catalyst Polarization in Alcohol Oxidation on Au and Pt in Water
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Gu, Q, Sautet, P, and Michel, C
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Aerobic alcohol oxidation ,density functional theory ,basic aqueous environment ,catalyst promotion ,Au ,Pt ,Inorganic Chemistry ,Organic Chemistry ,Chemical Engineering - Abstract
Alcohol oxidation by O2 to carboxylic acid can be operated in water using noble-metal catalysts, but relies on the undesirable addition of a base such as sodium hydroxide. Using periodic density functional theory (DFT), we built a model including the chemisorption of hydroxide anion at the metal/water interface to rationalize the pivotal role of the added base on the catalytic activity. We demonstrate that the role of the base is to polarize the surface and that a similar promotion could be obtained by tuning the electronic properties of additives, alloy, and support.
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- 2018
34. AGN-Host Connection at 0.5 < z < 2.5: A rapid evolution of AGN fraction in red galaxies during the last 10 Gyr
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Wang, Tao, Elbaz, D., Alexander, D. M., Xue, Y. Q., Gabor, J. M., Juneau, S., Schreiber, C., Zheng, X-Z., Wuyts, S., Shi, Y., Daddi, E., Shu, X-W., Fang, G-W., Huang, J-S., Luo, B., and Gu, Q-S.
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Astrophysics - Astrophysics of Galaxies - Abstract
We explore the dependence of the incidence of moderate-luminosity ($L_{X} = 10^{41.9-43.7}$ erg s$^{-1}$) AGNs and the distribution of their accretion rates on host color at 0.5 < z < 2.5, using deep X-ray data in GOODS fields. We use extinction-corrected rest-frame U-V colors to divide both AGN hosts and non-AGN galaxies into red sequence (quiescent), green valley (transition), and blue cloud (star-forming) populations. We find that both the AGN fraction at fixed stellar mass and its evolution with redshift are dependent on host colors. Most notably, red galaxies have the lowest AGN fraction (~5\%) at z~1 yet with most rapid redshift evolution, increasing by a factor of 5 (~24\%) at z~2. Green galaxies exhibit the highest AGN fraction across all redshifts, which is most pronounced at z~2 with more than half of them hosting an AGN at $M_{*} > 10^{10.6} M_{\odot}$. Together with the high AGN fraction in red galaxies at z~2, this indicates that X-ray AGNs could be important in both transforming blue galaxies into red ones and subsequently maintaining their quiescence at high redshift. Furthermore, consistent with low-redshift studies, we find that the probability of hosting an AGN in the total galaxy population can be characterized by a universal Eddington ratio ($p(\lambda_{Edd}) \sim \lambda_{Edd}^{-0.4}$) and a moderate redshift evolution. Yet consistent with their different AGN fractions, different populations appear to also have different $p(\lambda_{Edd})$ with red galaxies exhibiting more rapid redshift evolution than green and blue ones. Evidence for a steeper power law of $p(\lambda_{Edd})$ in red galaxies is also presented, though larger samples are needed to confirm. These results suggest that the AGN accretion or the growth of supermassive black holes is related to their host properties, and may also influence their hosts in a different mode dependent on the host color., Comment: A&A, in press
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- 2016
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35. The Chandra Deep Field-South Survey: 7 Ms Source Catalogs
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Luo, B., Brandt, W. N., Xue, Y. Q., Lehmer, B., Alexander, D. M., Bauer, F. E., Vito, F., Yang, G., Basu-Zych, A. R., Comastri, A., Gilli, R., Gu, Q. -S., Hornschemeier, A. E., Koekemoer, A., Liu, T., Mainieri, V., Paolillo, M., Ranalli, P., Rosati, P., Schneider, D. P., Shemmer, O., Smail, I., Sun, M., Tozzi, P., Vignali, C., and Wang, J. -X.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present X-ray source catalogs for the $\approx7$ Ms exposure of the Chandra Deep Field-South (CDF-S), which covers a total area of 484.2 arcmin$^2$. Utilizing WAVDETECT for initial source detection and ACIS Extract for photometric extraction and significance assessment, we create a main source catalog containing 1008 sources that are detected in up to three X-ray bands: 0.5-7.0 keV, 0.5-2.0 keV, and 2-7 keV. A supplementary source catalog is also provided including 47 lower-significance sources that have bright ($K_s\le23$) near-infrared counterparts. We identify multiwavelength counterparts for 992 (98.4%) of the main-catalog sources, and we collect redshifts for 986 of these sources, including 653 spectroscopic redshifts and 333 photometric redshifts. Based on the X-ray and multiwavelength properties, we identify 711 active galactic nuclei (AGNs) from the main-catalog sources. Compared to the previous $\approx4$ Ms CDF-S catalogs, 291 of the main-catalog sources are new detections. We have achieved unprecedented X-ray sensitivity with average flux limits over the central $\approx1$ arcmin$^2$ region of $\approx1.9\times10^{-17}$, $6.4\times10^{-18}$, and $2.7\times10^{-17}$ erg cm$^{-2}$ s$^{-1}$ in the three X-ray bands, respectively. We provide cumulative number-count measurements observing, for the first time, that normal galaxies start to dominate the X-ray source population at the faintest 0.5-2.0 keV flux levels. The highest X-ray source density reaches $\approx50\,500$ deg$^{-2}$, and $47\%\pm4\%$ of these sources are AGNs ($\approx23\,900$ deg$^{-2}$)., Comment: 31 pages, 31 figures, 8 tables, ApJS in press, minor text updates; full-resolution PDF version and data products available at http://www.astro.psu.edu/users/niel/cdfs/cdfs-chandra.html
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- 2016
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36. Updated baseline for a staged Compact Linear Collider
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CLIC, The, collaborations, CLICdp, Boland, M. J., Felzmann, U., Giansiracusa, P. J., Lucas, T. G., Rassool, R. P., Balazs, C., Charles, T. K., Afanaciev, K., Emeliantchik, I., Ignatenko, A., Makarenko, V., Shumeiko, N., Patapenka, A., Zhuk, I., Hoffman, A. C. Abusleme, Gutierrez, M. A. Diaz, Gonzalez, M. Vogel, Chi, Y., He, X., Pei, G., Pei, S., Shu, G., Wang, X., Zhang, J., Zhao, F., Zhou, Z., Chen, H., Gao, Y., Huang, W., Kuang, Y. P., Li, B., Li, Y., Shao, J., Shi, J., Tang, C., Wu, X., Ma, L., Han, Y., Fang, W., Gu, Q., Huang, D., Huang, X., Tan, J., Wang, Z., Zhao, Z., Laštovička, T., Uggerhoj, U., Wistisen, T. N., Aabloo, A., Eimre, K., Kuppart, K., Vigonski, S., Zadin, V., Aicheler, M., Baibuz, E., Brücken, E., Djurabekova, F., Eerola, P., Garcia, F., Haeggström, E., Huitu, K., Jansson, V., Karimaki, V., Kassamakov, I., Kyritsakis, A., Lehti, S., Meriläinen, A., Montonen, R., Niinikoski, T., Nordlund, K., Österberg, K., Parekh, M., Törnqvist, N. A., Väinölä, J., Veske, M., Farabolini, W., Mollard, A., Napoly, O., Peauger, F., Plouin, J., Bambade, P., Chaikovska, I., Chehab, R., Davier, M., Kaabi, W., Kou, E., LeDiberder, F., Pöschl, R., Zerwas, D., Aimard, B., Balik, G., Baud, J. -P., Blaising, J. -J., Brunetti, L., Chefdeville, M., Drancourt, C., Geoffroy, N., Jacquemier, J., Jeremie, A., Karyotakis, Y., Nappa, J. M., Vilalte, S., Vouters, G., Bernard, A., Peric, I., Gabriel, M., Simon, F., Szalay, M., van der Kolk, N., Alexopoulos, T., Gazis, E. N., Gazis, N., Ikarios, E., Kostopoulos, V., Kourkoulis, S., Gupta, P. D., Shrivastava, P., Arfaei, H., Dayyani, M. K., Ghasem, H., Hajari, S. S., Shaker, H., Ashkenazy, Y., Abramowicz, H., Benhammou, Y., Borysov, O., Kananov, S., Levy, A., Levy, I., Rosenblat, O., D'Auria, G., Di Mitri, S., Abe, T., Aryshev, A., Higo, T., Makida, Y., Matsumoto, S., Shidara, T., Takatomi, T., Takubo, Y., Tauchi, T., Toge, N., Ueno, K., Urakawa, J., Yamamoto, A., Yamanaka, M., Raboanary, R., Hart, R., van der Graaf, H., Eigen, G., Zalieckas, J., Adli, E., Lillestøl, R., Malina, L., Pfingstner, J., Sjobak, K. N., Ahmed, W., Asghar, M. I., Hoorani, H., Bugiel, S., Dasgupta, R., Firlej, M., Fiutowski, T. A., Idzik, M., Kopec, M., Kuczynska, M., Moron, J., Swientek, K. P., Daniluk, W., Krupa, B., Kucharczyk, M., Lesiak, T., Moszczynski, A., Pawlik, B., Sopicki, P., Wojtoń, T., Zawiejski, L., Kalinowski, J., Krawczyk, M., Żarnecki, A. F., Firu, E., Ghenescu, V., Neagu, A. T., Preda, T., Zgura, I-S., Aloev, A., Azaryan, N., Budagov, J., Chizhov, M., Filippova, M., Glagolev, V., Gongadze, A., Grigoryan, S., Gudkov, D., Karjavine, V., Lyablin, M., Olyunin, A., Samochkine, A., Sapronov, A., Shirkov, G., Soldatov, V., Solodko, A., Solodko, E., Trubnikov, G., Tyapkin, I., Uzhinsky, V., Vorozhtov, A., Levichev, E., Mezentsev, N., Piminov, P., Shatilov, D., Vobly, P., Zolotarev, K., Jelisavcic, I. Bozovic, Kacarevic, G., Lukic, S., Milutinovic-Dumbelovic, G., Pandurovic, M., Iriso, U., Perez, F., Pont, M., Trenado, J., Aguilar-Benitez, M., Calero, J., Garcia-Tabares, L., Gavela, D., Gutierrez, J. L., Lopez, D., Toral, F., Moya, D., Jimeno, A. Ruiz, Vila, I., Argyropoulos, T., Gutierrez, C. Blanch, Boronat, M., Esperante, D., Faus-Golfe, A., Fuster, J., Martinez, N. Fuster, Muñoz, N. Galindo, García, I., Navarro, J. Giner, Ros, E., Vos, M., Brenner, R., Ekelöf, T., Jacewicz, M., Ögren, J., Olvegård, M., Ruber, R., Ziemann, V., Aguglia, D., Tehrani, N. Alipour, Andersson, A., Andrianala, F., Antoniou, F., Artoos, K., Atieh, S., Sune, R. Ballabriga, Barnes, M. J., Garcia, J. Barranco, Bartosik, H., Belver-Aguilar, C., Morell, A. Benot, Bett, D. R., Bettoni, S., Blanchot, G., Garcia, O. Blanco, Bonnin, X. A., Brunner, O., Burkhardt, H., Calatroni, S., Campbell, M., Lasheras, N. Catalan, Bastos, M. Cerqueira, Cherif, A., Chevallay, E., Constance, B., Corsini, R., Cure, B., Curt, S., Dalena, B., Dannheim, D., De Michele, G., De Oliveira, L., Deelen, N., Delahaye, J. P., Dobers, T., Doebert, S., Draper, M., Ramos, F. Duarte, Dubrovskiy, A., Elsener, K., Esberg, J., Esposito, M., Fedosseev, V., Ferracin, P., Fiergolski, A., Foraz, K., Fowler, A., Friebel, F., Fuchs, J-F., Rojas, C. A. Fuentes, Gaddi, A., Fajardo, L. Garcia, Morales, H. Garcia, Garion, C., Gatignon, L., Gayde, J-C., Gerwig, H., Goldblatt, A. N., Grefe, C., Grudiev, A., Guillot-Vignot, F. G., Gutt-Mostowy, M. L., Hauschild, M., Hessler, C., Holma, J. K., Holzer, E., Hourican, M., Hynds, D., Levinsen, Y. Inntjore, Jeanneret, B., Jensen, E., Jonker, M., Kastriotou, M., Kemppinen, J. M. K., Kieffer, R. B., Klempt, W., Kononenko, O., Korsback, A., Platia, E. Koukovini, Kovermann, J. W., Kozsar, C-I., Kremastiotis, I., Kulis, S., Latina, A., Leaux, F., Lebrun, P., Lefevre, T., Linssen, L., Cudie, X. Llopart, Maier, A. A., Durand, H. Mainaud, Manosperti, E., Marelli, C., Lacoma, E. Marin, Martin, R., Mazzoni, S., Mcmonagle, G., Mete, O., Mether, L. M., Modena, M., Münker, R. M., Muranaka, T., Del Busto, E. Nebot, Nikiforou, N., Nisbet, D., Nonglaton, J-M., Nuiry, F. X., Nürnberg, A., Olvegard, M., Osborne, J., Papadopoulou, S., Papaphilippou, Y., Passarelli, A., Patecki, M., Pazdera, L., Pellegrini, D., Pepitone, K., Codina, E. Perez, Fontenla, A. Perez, Persson, T. H. B., Petrič, M., Pitters, F., Pittet, S., Plassard, F., Rajamak, R., Redford, S., Renier, Y., Rey, S. F., Riddone, G., Rinolfi, L., Castro, E. Rodriguez, Roloff, P., Rossi, C., Rude, V., Rumolo, G., Sailer, A., Santin, E., Schlatter, D., Schmickler, H., Schulte, D., Shipman, N., Sicking, E., Simoniello, R., Skowronski, P. K., Mompean, P. Sobrino, Soby, L., Sosin, M. P., Sroka, S., Stapnes, S., Sterbini, G., Ström, R., Syratchev, I., Tecker, F., Thonet, P. A., Timeo, L., Timko, H., Garcia, R. Tomas, Valerio, P., Vamvakas, A. L., Vivoli, A., Weber, M. A., Wegner, R., Wendt, M., Woolley, B., Wuensch, W., Uythoven, J., Zha, H., Zisopoulos, P., Benoit, M., Pinto, M. Vicente Barreto, Bopp, M., Braun, H. H., Divall, M. Csatari, Dehler, M., Garvey, T., Raguin, J. Y., Rivkin, L., Zennaro, R., Aksoy, A., Nergiz, Z., Pilicer, E., Tapan, I., Yavas, O., Baturin, V., Kholodov, R., Lebedynskyi, S., Miroshnichenko, V., Mordyk, S., Profatilova, I., Storizhko, V., Watson, N., Winter, A., Goldstein, J., Green, S., Marshall, J. S., Thomson, M. A., Xu, B., Gillespie, W. A., Pan, R., Tyrk, M. A, Protopopescu, D., Robson, A., Apsimon, R., Bailey, I., Burt, G., Constable, D., Dexter, A., Karimian, S., Lingwood, C., Buckland, M. D., Casse, G., Vossebeld, J., Bosco, A., Karataev, P., Kruchinin, K., Lekomtsev, K., Nevay, L., Snuverink, J., Yamakawa, E., Boisvert, V., Boogert, S., Boorman, G., Gibson, S., Lyapin, A., Shields, W., Teixeira-Dias, P., West, S., Jones, R., Joshi, N., Bodenstein, R., Burrows, P. N., Christian, G. B., Gamba, D., Perry, C., Roberts, J., Clarke, J. A., Collomb, N. A., Jamison, S. P., Shepherd, B. J. A., Walsh, D., Demarteau, M., Repond, J., Weerts, H., Xia, L., Wells, J. D., Adolphsen, C., Barklow, T., Breidenbach, M., Graf, N., Hewett, J., Markiewicz, T., McCormick, D., Moffeit, K., Nosochkov, Y., Oriunno, M., Phinney, N., Rizzo, T., Tantawi, S., Wang, F., Wang, J., White, G., and Woodley, M.
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Physics - Accelerator Physics ,High Energy Physics - Experiment - Abstract
The Compact Linear Collider (CLIC) is a multi-TeV high-luminosity linear e+e- collider under development. For an optimal exploitation of its physics potential, CLIC is foreseen to be built and operated in a staged approach with three centre-of-mass energy stages ranging from a few hundred GeV up to 3 TeV. The first stage will focus on precision Standard Model physics, in particular Higgs and top-quark measurements. Subsequent stages will focus on measurements of rare Higgs processes, as well as searches for new physics processes and precision measurements of new states, e.g. states previously discovered at LHC or at CLIC itself. In the 2012 CLIC Conceptual Design Report, a fully optimised 3 TeV collider was presented, while the proposed lower energy stages were not studied to the same level of detail. This report presents an updated baseline staging scenario for CLIC. The scenario is the result of a comprehensive study addressing the performance, cost and power of the CLIC accelerator complex as a function of centre-of-mass energy and it targets optimal physics output based on the current physics landscape. The optimised staging scenario foresees three main centre-of-mass energy stages at 380 GeV, 1.5 TeV and 3 TeV for a full CLIC programme spanning 22 years. For the first stage, an alternative to the CLIC drive beam scheme is presented in which the main linac power is produced using X-band klystrons., Comment: 57 pages, 27 figures, 12 tables, published as CERN Yellow Report. Updated version: Minor layout changes for print version
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- 2016
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37. Molecular conformations of DNA targets captured by model nanoarrays
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Hao, X, Josephs, EA, Gu, Q, and Ye, T
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Genetics ,Good Health and Well Being ,DNA Probes ,Molecular Conformation ,Nanotechnology ,Physical Sciences ,Chemical Sciences ,Technology ,Nanoscience & Nanotechnology - Abstract
An open question in single molecule nanoarrays is how the chemical and morphological heterogeneities of the solid support affect the properties of biomacromolecules. We generated arrays that allowed individually-resolvable DNA molecules to interact with tailored surface heterogeneities and revealed how molecular conformations are impacted by surface interactions.
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- 2017
38. Modulation on the electrical and optical properties of Na and Rh co-doped Ruddlesden-Popper layered Ca3Ti2O7
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Gu, Q., Liu, W. F., Wong-Ng, Winnie, Wu, X. X., Wang, C., Zhou, W., and Wang, S. Y.
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- 2021
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39. The Value of Relative Size in the Ultrasound Diagnosis of Follicular Thyroid Neoplasm
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Zhang S, Huang L, Huang Q, Wei W, Xie L, Zeng J, Gu Q, Chen L, and Chen S
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follicular thyroid neoplasm ,nodular goiter ,size ,ultrasonography ,Medicine (General) ,R5-920 - Abstract
Sufang Zhang,1,* Liyan Huang,1,* Qingshan Huang,2,* Weili Wei,1 Lijun Xie,1 Jinshu Zeng,1 Qiuyang Gu,1 Ling Chen,1 Shuqiang Chen1 1Department of Ultrasound, The First Affiliated Hospital of Fujian Medical University, Fuzhou, 350005, People’s Republic of China; 2Musculoskeletal Tumor Center, Peking University People’s Hospital, Beijing, 100044, People’s Republic of China*These authors contributed equally to this workCorrespondence: Shuqiang ChenDepartment of Ultrasound, The First Affiliated Hospital of Fujian Medical University, Fuzhou, 350005, People’s Republic of ChinaTel/Fax +86-591-87981961Email chenshu0518@163.comPurpose: Ultrasonography as the first choice for thyroid nodules is still difficult to distinguish between solid follicular thyroid neoplasm (FTN) and solid nodular goiter (NG). We tried to investigate the value of relative size (M/S, M: the maximum diameter of target nodule, S: the maximum diameter of the largest of the remaining nodules) that may help to differentiate FTN from NG.Methods: T test and chi-square test were used to retrospectively analyze the differences of the clinical and ultrasonographic characteristics between FTN and NG in 422 cases in our hospital. T test was used to analyze the difference of M/S value in the two kinds of nodules. ROC was used to evaluate the accuracy of M/S value in distinguishing the two.Results: There were statistically significant differences in age, echogenicity, calcification, peripheral halo and blood supply between the two. The M/S value is not only significantly different in the two kinds of nodules but also can be used as a quantitative indicator to guide ultrasound diagnosis. ROC analysis showed that the cutoff point and AUC of M/S value were 1.94 and 0.709, respectively.Conclusion: In the ultrasound diagnosis of multiple thyroid nodules, the M/S value can better distinguish FTN and NG. We need to be aware of FTN when the M/S value of the nodule is greater than 2.Keywords: follicular thyroid neoplasm, nodular goiter, size, ultrasonography
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- 2021
40. The Intrapleural Bridge Connection is One of the Reasons for Unknown Localized Pleural Adhesion
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Gu Q, Deng X, Li Z, Wang J, Hu C, Lei S, and Cai X
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pleural adhesion ,bridge connection ,physiological variation ,image ,thoracoscope. ,Medicine (General) ,R5-920 - Abstract
Qihua Gu,1,2 Xinhao Deng,1,2 Zhao Li,1,2 Jing Wang,3 Chengping Hu,1,2 Shuhua Lei,1,2 Xiaoling Cai1,2 1Department of Respiratory Medicine, Xiangya Hospital Affiliated to Central South University, Changsha, Hunan Province, 410008, People’s Republic of China; 2Key Cite of National Clinical Research Center for Respiratory Disease, Changsha, Hunan Province, 410008, People’s Republic of China; 3Department of Pathology, Xiangya Hospital Affiliated to Central South University, Changsha, Hunan Province, 410008, People’s Republic of ChinaCorrespondence: Qihua Gu Tel +86 15973196025Email guqh06@163.comBackground: Simple signs of local pleural adhesion are often found in people during a physical examination. In the present study, we aimed to clarify whether the merely localized pleural adhesion was just caused by previous pleural inflammation or physiological variation.Materials and Methods: Chest X-ray image materials were collected to analyze the incidence of simple pleural adhesions. Moreover, the causes of these simple pleural adhesions were further analyzed using thoracoscopy under direct vision and biopsy data.Results: In all 2218 chest X-ray images, 68 cases were found to have pleural lesions (3.07%), including 15 cases of localized pleural adhesion only. Subsequently, we analyzed the characteristics of 70 cases of pleural lesions using thoracoscopy. In two lung cancer patients with pleural metastasis, we found an unusual pleural junction. This connective strip was smooth and free of inflammation, resembling the normal pleura.Conclusion: Some of these purely localized pleural adhesions might be attributed to previous inflammation. However, there was still at least a possibility that there must be a physiological pleural junction, which could be the cause of the purely localized pleural adhesion shown in the chest radiograph.Keywords: pleural adhesion, bridge connection, physiological variation, image, thoracoscope
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- 2021
41. Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z = 3.95
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Zhou, L., primary, Wang, T., additional, Daddi, E., additional, Coogan, R., additional, Sun, H., additional, Xu, K., additional, Arumugam, V., additional, Jin, S., additional, Liu, D., additional, Lu, S., additional, Sillassen, N., additional, Wang, Y., additional, Shi, Y., additional, Zhang, Z., additional, Tan, Q., additional, Gu, Q., additional, Elbaz, D., additional, Le Bail, A., additional, Magnelli, B., additional, Gómez-Guijarro, C., additional, d’Eugenio, C., additional, Magdis, G., additional, Valentino, F., additional, Ji, Z., additional, Gobat, R., additional, Delvecchio, I., additional, Xiao, M., additional, Strazzullo, V., additional, Finoguenov, A., additional, Schinnerer, E., additional, Rich, R. M., additional, Huang, J., additional, Dai, Y., additional, Chen, Y., additional, Gao, F., additional, Yang, T., additional, and Hao, Q., additional
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- 2024
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42. Modeling Warm Absorption in HST/COS Spectrum of Mrk 290 with XSTAR
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Zhang, S. N., Ji, L., Kallman, T. R., Yao, Y. S., Froning, C. S., Gu, Q. S., and Kriss, G. A.
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Astrophysics - Astrophysics of Galaxies - Abstract
We present a new method to model a HST/COS spectrum, aimed to analyze intrinsic UV absorption from the outflow of Mrk 290, a Seyfert I galaxy. We use newly updated XSTAR to generate photoionization models for the intrinsic absorption from the AGN outflow, the line emission from the AGN broad and narrow line regions, and the local absorption from high velocity clouds and Galactic interstellar medium. The combination of these physical models accurately fit the COS spectrum. Three intrinsic absorbers outflowing with velocities ~500 km/s are identified, two of which are found directly from two velocity components of the N V and C IV doublets, while the third is required by the extra absorption in the Lyman alpha. Their outflow velocities, ionization states and column densities are consistent with the lowest and moderately ionization warm absorbers (WAs) in the X-ray domain found by Chandra observations, suggesting an one-to-one correspondence between the absorbing gas in the UV and X-ray bands. The small turbulent velocities of the WAs (v_turb~<100 km/s) support our previous argument from the X-ray study that the absorbers originate from the inner side of the torus due to thermal evaporation. Given the covering fractions of ~65% for the three WAs, we deduce that the lengths and the thicknesses of the WAs are comparable, which indicates that the geometry of WAs are more likely clouds rather than flat and thin layers. In addition, the modeling of the broad line emission suggests a higher covering fraction of clouds when they are very closer to the black hole., Comment: 14 pages, 7 figures; Accepted for publication in MNRAS
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- 2014
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43. Finite Element Analysis for Predicting Skin Pharmacokinetics of Nano Transdermal Drug Delivery System Based on the Multilayer Geometry Model
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Gu Y, Gu Q, Yang Q, Yang M, Wang S, and Liu J
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nano transdermal drug delivery system ,skin pharmacokinetics ,finite element analysis ,multilayer geometry model ,diffusion coefficient ,paeonol nanoemulsion ,Medicine (General) ,R5-920 - Abstract
Yongwei Gu,1– 3,* Qing Gu,4,* Qing Yang,1,2 Meng Yang,3 Shengzhang Wang,5 Jiyong Liu1– 3 1Department of Pharmacy, Fudan University Shanghai Cancer Center, Shanghai 200032, People’s Republic of China; 2Department of Oncology, Shanghai Medical College, Fudan University, Shanghai 200032, People’s Republic of China; 3Department of Pharmacy, Changhai Hospital, Second Military Medical University, Shanghai 200433, People’s Republic of China; 4Department of Pharmacy, Jingan District Zhabei Central Hospital, Shanghai 200070, People’s Republic of China; 5Institute of Biomechanics, Department of Aeronautics and Astronautics, Fudan University, Shanghai 200433, People’s Republic of China*These authors contributed equally to this workCorrespondence: Shengzhang WangDepartment of Aeronautics and Astronautics, Institute of Biomechanics, Fudan University, Shanghai 200433, People’s Republic of ChinaTel/Fax +86-21-65647825Email szwang@fudan.edu.cnJiyong LiuDepartment of Pharmacy, Fudan University Shanghai Cancer Center, Shanghai 200032, People’s Republic of China; Department of Oncology, Shanghai Medical College, Fudan University, Shanghai 200032, People’s Republic of ChinaTel/Fax +86-21-64175590Email liujiyong@fudan.edu.cnBackground: Skin pharmacokinetics is an indispensable indication for studying the drug fate after administration of transdermal drug delivery systems (TDDS). However, the heterogeneity and complex skin structured with stratum corneum, viable epidermis, dermis, and subcutaneous tissue inevitably leads the drug diffusion coefficient (Kp) to vary depending on the skin depth, which seriously limits the development of TDDS pharmacokinetics in full thickness skin.Methods: A multilayer geometry skin model was established and the Kp of drug in SC, viable epidermis, and dermis was obtained using the technologies of molecular dynamics simulation, in vitro permeation experiments, and in vivo microdialysis, respectively. Besides, finite element analysis (FEA) based on drug Kps in different skin layers was applied to simulate the paeonol nanoemulsion (PAE-NEs) percutaneous dynamic penetration process in two and three dimensions. In addition, PAE-NEs skin pharmacokinetics profile obtained by the simulation was verified by in vivo experiment.Results: Coarse-grained modeling of molecular dynamic simulation was successfully established and the Kp of PAE in SC was 2.00× 10− 6 cm2/h. The Kp of PAE-NE in viable epidermis and in dermis detected using penetration test and microdialysis probe technology, was 1.58× 10− 5 cm2/h and 3.20× 10− 5 cm2/h, respectively. In addition, the results of verification indicated that PAE-NEs skin pharmacokinetics profile obtained by the simulation was consistent with that by in vivo experiment.Discussion: This study demonstrated that the FEA combined with the established multilayer geometry skin model could accurately predict the skin pharmacokinetics of TDDS.Keywords: nano transdermal drug delivery system, skin pharmacokinetics, finite element analysis, multilayer geometry model, diffusion coefficient, paeonol nanoemulsion
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- 2020
44. Noema formIng Cluster survEy (NICE):Discovery of a starbursting galaxy group with a radio-luminous core at z = 3.95
- Author
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Zhou, L., Wang, T., Daddi, E., Coogan, R., Sun, H., Xu, K., Arumugam, V., Jin, S., Liu, D., Lu, S., Sillassen, N., Wang, Y., Shi, Y., Zhang, Z., Tan, Q., Gu, Q., Elbaz, D., Le Bail, A., Magnelli, B., Gómez-guijarro, C., D’eugenio, C., Magdis, G., Valentino, F., Ji, Z., Gobat, R., Delvecchio, I., Xiao, M., Strazzullo, V., Finoguenov, A., Schinnerer, E., Rich, R. M., Huang, J., Dai, Y., Chen, Y., Gao, F., Yang, T., Hao, Q., Zhou, L., Wang, T., Daddi, E., Coogan, R., Sun, H., Xu, K., Arumugam, V., Jin, S., Liu, D., Lu, S., Sillassen, N., Wang, Y., Shi, Y., Zhang, Z., Tan, Q., Gu, Q., Elbaz, D., Le Bail, A., Magnelli, B., Gómez-guijarro, C., D’eugenio, C., Magdis, G., Valentino, F., Ji, Z., Gobat, R., Delvecchio, I., Xiao, M., Strazzullo, V., Finoguenov, A., Schinnerer, E., Rich, R. M., Huang, J., Dai, Y., Chen, Y., Gao, F., Yang, T., and Hao, Q.
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- 2024
45. The CompactLight Design Study
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D'Auria, G., Adli, E., Aicheler, M., Aksoy, A., Alesini, D., Apsimon, R., Arnsberg, J., Auchettl, R., Bainbridge, A., Balazs, K., Bantekas, D., Bedolla, J., Behtouei, M., Bellaveglia, M., Vd Berg, M., Bernhard, A., Bignami, A., Breitenbach, M., Breukers, M., Burt, G., Cai, J., Calvi, M., Cardelli, F., Carpanese, M., Cortes, H. M. Castaneda, Castilla, A., Cianchi, A., Clarke, J., Cowie, L., Croia, M., Cross, A., Danailov, M., Dattoli, G., Deleval, S., Mitri, S. Di, Diomede, M., Dowd, R., Dunning, D., Easton, J., Fang, W., Fatehi, S., Faus-Golfe, A., Ferianis, M., Ferrario, M., Ficcadenti, L., Gallo, A., Gazis, E., Gazis, N., Geometrante, R., Gethmann, J., Gioppo, R., Giribono, A., Gonzalez-Iglesias, D., Goryashko, Vitaliy, Grohmann, S., Gu, Q., Han, Y., Hinton, A., Hobi, A., Hoekstra, R., Huang, X., Jacewicz, Marek, Jones, J., Kaertner, F., Karagiannaki, A., Kokole, M., Kotitsa, R., Kotsopoulos, D., Krasch, B., Latina, A., Lepercq, P., Liu, X., Lucas, T. G., Luiten, O. J., Maheshwari, M., Mahnic, J., Mak, Alan, Marcos, J., Marin, E., Marinov, K., Martinez, B. G., Mercier, B., Migliorati, M., Milharcic, T., Mostacci, A., Mu Noz, R., Musat, V., Mutsaers, P. H. A., Nergiz, Z., Nguyen, F., Nix, L., Palumbo, L., Parodi, M., Pavlica, R., Pellegrino, L., Pereira, D. E., Perez, F., Petralia, A., Piersanti, L., Pockar, J., Pramatari, K., Priem, H., Primozic, U., Rassool, R., Reiche, S., Revilak, P., Richter, S. C., Rochow, R., Rossi, C., Salén, Peter, Schmidt, T., Schoerling, D., Schulte, D., Scifo, J., Sheehy, S., Shepherd, B., Spataro, B., Stapnes, S., Stragier, X. F. D., Syratchev, I., Tabacco, C., Tan, J., Tanke, E., Taylor, G., Telahi, I., Thompson, N., Trachanas, E., Tzanetou, K. S., Vaccarezza, C., Vainola, J., Vannozzi, A., Volpi, M., Wang, C., Williams, P., Wu, X., Wuensch, W., Yap, J., Zangrando, M., Zhang, K., Zhang, L., Zhao, Y., Zhao, Z., Zhu, D., D'Auria, G., Adli, E., Aicheler, M., Aksoy, A., Alesini, D., Apsimon, R., Arnsberg, J., Auchettl, R., Bainbridge, A., Balazs, K., Bantekas, D., Bedolla, J., Behtouei, M., Bellaveglia, M., Vd Berg, M., Bernhard, A., Bignami, A., Breitenbach, M., Breukers, M., Burt, G., Cai, J., Calvi, M., Cardelli, F., Carpanese, M., Cortes, H. M. Castaneda, Castilla, A., Cianchi, A., Clarke, J., Cowie, L., Croia, M., Cross, A., Danailov, M., Dattoli, G., Deleval, S., Mitri, S. Di, Diomede, M., Dowd, R., Dunning, D., Easton, J., Fang, W., Fatehi, S., Faus-Golfe, A., Ferianis, M., Ferrario, M., Ficcadenti, L., Gallo, A., Gazis, E., Gazis, N., Geometrante, R., Gethmann, J., Gioppo, R., Giribono, A., Gonzalez-Iglesias, D., Goryashko, Vitaliy, Grohmann, S., Gu, Q., Han, Y., Hinton, A., Hobi, A., Hoekstra, R., Huang, X., Jacewicz, Marek, Jones, J., Kaertner, F., Karagiannaki, A., Kokole, M., Kotitsa, R., Kotsopoulos, D., Krasch, B., Latina, A., Lepercq, P., Liu, X., Lucas, T. G., Luiten, O. J., Maheshwari, M., Mahnic, J., Mak, Alan, Marcos, J., Marin, E., Marinov, K., Martinez, B. G., Mercier, B., Migliorati, M., Milharcic, T., Mostacci, A., Mu Noz, R., Musat, V., Mutsaers, P. H. A., Nergiz, Z., Nguyen, F., Nix, L., Palumbo, L., Parodi, M., Pavlica, R., Pellegrino, L., Pereira, D. E., Perez, F., Petralia, A., Piersanti, L., Pockar, J., Pramatari, K., Priem, H., Primozic, U., Rassool, R., Reiche, S., Revilak, P., Richter, S. C., Rochow, R., Rossi, C., Salén, Peter, Schmidt, T., Schoerling, D., Schulte, D., Scifo, J., Sheehy, S., Shepherd, B., Spataro, B., Stapnes, S., Stragier, X. F. D., Syratchev, I., Tabacco, C., Tan, J., Tanke, E., Taylor, G., Telahi, I., Thompson, N., Trachanas, E., Tzanetou, K. S., Vaccarezza, C., Vainola, J., Vannozzi, A., Volpi, M., Wang, C., Williams, P., Wu, X., Wuensch, W., Yap, J., Zangrando, M., Zhang, K., Zhang, L., Zhao, Y., Zhao, Z., and Zhu, D.
- Abstract
CompactLight is a Design Study funded by the European Union under the Horizon 2020 research and innovation funding programme, with Grant Agreement No. 777431. CompactLight was conducted by an International Collaboration of 23 international laboratories and academic institutions, three private companies, and five third parties. The project, which started in January 2018 with a duration of 48 months, aimed to design an innovative, compact, and cost-effective hard X-ray FEL facility complemented by a soft X-ray source to pave the road for future compact accelerator-based facilities. The result is an accelerator that can be operated at up to 1 kHz pulse repetition rate, beyond today's state of the art, using the latest concepts for high brightness electron photoinjectors, very high gradient accelerating structures in X-band, and novel short-period undulators. In this report, we summarize the main deliverable of the project: the CompactLight Conceptual Design Report, which overviews the current status of the design and addresses the main technological challenges.
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- 2024
- Full Text
- View/download PDF
46. A quantum coherent spin in hexagonal boron nitride at ambient conditions.
- Author
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Stern, HL, M Gilardoni, C, Gu, Q, Eizagirre Barker, S, Powell, OFJ, Deng, X, Fraser, SA, Follet, L, Li, C, Ramsay, AJ, Tan, HH, Aharonovich, I, Atatüre, M, Stern, HL, M Gilardoni, C, Gu, Q, Eizagirre Barker, S, Powell, OFJ, Deng, X, Fraser, SA, Follet, L, Li, C, Ramsay, AJ, Tan, HH, Aharonovich, I, and Atatüre, M
- Abstract
Solid-state spin-photon interfaces that combine single-photon generation and long-lived spin coherence with scalable device integration-ideally under ambient conditions-hold great promise for the implementation of quantum networks and sensors. Despite rapid progress reported across several candidate systems, those possessing quantum coherent single spins at room temperature remain extremely rare. Here we report quantum coherent control under ambient conditions of a single-photon-emitting defect spin in a layered van der Waals material, namely, hexagonal boron nitride. We identify that the carbon-related defect has a spin-triplet electronic ground-state manifold. We demonstrate that the spin coherence is predominantly governed by coupling to only a few proximal nuclei and is prolonged by decoupling protocols. Our results serve to introduce a new platform to realize a room-temperature spin qubit coupled to a multiqubit quantum register or quantum sensor with nanoscale sample proximity.
- Published
- 2024
47. Understanding the charge transfer effects of single atoms for boosting the performance of Na-S batteries.
- Author
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Lei, Y-J, Lu, X, Yoshikawa, H, Matsumura, D, Fan, Y, Zhao, L, Li, J, Wang, S, Gu, Q, Liu, H-K, Dou, S-X, Devaraj, S, Rojo, T, Lai, W-H, Armand, M, Wang, Y-X, Wang, G, Lei, Y-J, Lu, X, Yoshikawa, H, Matsumura, D, Fan, Y, Zhao, L, Li, J, Wang, S, Gu, Q, Liu, H-K, Dou, S-X, Devaraj, S, Rojo, T, Lai, W-H, Armand, M, Wang, Y-X, and Wang, G
- Abstract
The effective flow of electrons through bulk electrodes is crucial for achieving high-performance batteries, although the poor conductivity of homocyclic sulfur molecules results in high barriers against the passage of electrons through electrode structures. This phenomenon causes incomplete reactions and the formation of metastable products. To enhance the performance of the electrode, it is important to place substitutable electrification units to accelerate the cleavage of sulfur molecules and increase the selectivity of stable products during charging and discharging. Herein, we develop a single-atom-charging strategy to address the electron transport issues in bulk sulfur electrodes. The establishment of the synergistic interaction between the adsorption model and electronic transfer helps us achieve a high level of selectivity towards the desirable short-chain sodium polysulfides during the practical battery test. These finding indicates that the atomic manganese sites have an enhanced ability to capture and donate electrons. Additionally, the charge transfer process facilitates the rearrangement of sodium ions, thereby accelerating the kinetics of the sodium ions through the electrostatic force. These combined effects improve pathway selectivity and conversion to stable products during the redox process, leading to superior electrochemical performance for room temperature sodium-sulfur batteries.
- Published
- 2024
48. Effects of stir-frying on the processing characteristics and in vitro digestion of oat flour during storage
- Author
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Zhang, Y, Zhang, M, Huo, R, Bai, X, Wang, P, Gu, Q, Zhang, Y, Zhang, M, Huo, R, Bai, X, Wang, P, and Gu, Q
- Published
- 2024
49. Orientational mercury removal from aqueous solution using three-dimensionally structured CuxS nanocluster anchored attapulgite
- Author
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Dai, G., Huang, J., (0000-0002-4764-7827) Ding, W., Qiu, L., Zhang, W., Gu, Q., Wang, Z., Hu, Z., Quan, C., Li, P., Dai, G., Huang, J., (0000-0002-4764-7827) Ding, W., Qiu, L., Zhang, W., Gu, Q., Wang, Z., Hu, Z., Quan, C., and Li, P.
- Abstract
Toxic mercury-containing wastewater emitted from mining and nonferrous metallurgy seriously threatens human health and aquatic ecosystem. Effective mercury removal interfered with other coexisting metal ions in wastewater poses major challenges, requiring simple and sustainable methods. In this work, a novel three-dimensional (3D) CuxS nanocluster-anchored attapulgite (ATP@CuxS) is tailored for orientational mercury adsorption from diluted mercury-containing wastewater. The prepared ATP@CuxS adsorbent exhibited an unparalleled Hg2+ adsorption capacity of 746.48 mg g-1 among ever-reported clay-based adsorbents. Mercury-containing wastewater with an initial concentration of 5 mg L-1, and solution pH of 6.5 was ~100% removed within 20 min, and no interference by coexisting anionic and cation ions was observed. In the determination of the adsorption mechanism, in-situ intercalation and vulcanization of Cu2+ on ATP base constructs nanoclusters shaped CuxS that provide abundant active sites for Hg2+ adsorption. The negatively charged ATP facilitates positive Cu2+ immobilization on its surface followed by inorganic sulfide generation. This interfacial electrical compatibility makes a compact and stable composite. 33 Hydrophilic ATP modulated the uniform dispersion performance of ATP@CuxS, and 34 the dense CuxS package contributed to easier sedimentation and recovery after Hg2+ 35 adsorption in water. Furthermore, Hg2+ removal efficiency was maintained at 70% after 36 8 times repetitions, indicating a gentle feasibility as a mass-generated adsorbent. The 37 proposed interface engineering from the perspective of micro-interface electrical 38 compatibility creates an attractive and easily accessible system that combines efficiency, 39 capacity, selectivity, and reusability for orientational removing Hg2+ from wastewater.
- Published
- 2024
50. The Properties of H{\alpha} Emission-Line Galaxies at z = 2.24
- Author
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An, F. X., Zheng, X. Z., Wang, W. -H., Huang, J. -S., Kong, X., Wang, J. -X., Fang, G. W., Zhu, F., Gu, Q. -S., Wu, H., Hao, L., and Xia, X. -Y.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
Using deep narrow-band $H_2S1$ and $K_{s}$-band imaging data obtained with CFHT/WIRCam, we identify a sample of 56 H$\alpha$ emission-line galaxies (ELGs) at $z=2.24$ with the 5$\sigma$ depths of $H_2S1=22.8$ and $K_{s}=24.8$ (AB) over 383 arcmin$^{2}$ area in the ECDFS. A detailed analysis is carried out with existing multi-wavelength data in this field. Three of the 56 H$\alpha$ ELGs are detected in Chandra 4 Ms X-ray observation and two of them are classified as AGNs. The rest-frame UV and optical morphologies revealed by HST/ACS and WFC3 deep images show that nearly half of the H$\alpha$ ELGs are either merging systems or with a close companion, indicating that the merging/interacting processes play a key role in regulating star formation at cosmic epoch z=2-3; About 14% are too faint to be resolved in the rest-frame UV morphology due to high dust extinction. We estimate dust extinction from SEDs. We find that dust extinction is generally correlated with H$\alpha$ luminosity and stellar mass (SM). Our results suggest that H$\alpha$ ELGs are representative of star-forming galaxies (SFGs). Applying extinction correction for individual objects, we examine the intrinsic H$\alpha$ luminosity function (LF) at $z=2.24$, obtaining a best-fit Schechter function characterized by a faint-end slope of $\alpha=-1.3$. This is shallower than the typical slope of $\alpha \sim -1.6$ in previous works based on constant extinction correction. We demonstrate that this difference is mainly due to the different extinction corrections. The proper extinction correction is thus key to recovering the intrinsic LF as the extinction globally increases with H$\alpha$ luminosity. Moreover, we find that our H$\alpha$ LF mirrors the SM function of SFGs at the same cosmic epoch. This finding indeed reflects the tight correlation between SFR and SM for the SFGs, i.e., the so-called main sequence., Comment: 15 pages, 12 figures, 2 tables, Received 2013 October 11; accepted 2014 February 13; published 2014 March 18 by ApJ
- Published
- 2014
- Full Text
- View/download PDF
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