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| 1 | Role of endoscopic ultrasonography in the loco-regional staging of patients with rectal cancer显示文摘The prognosis of rectal cancer(RC) is strictly related to both T and N stage of the disease at the time of diagnosis. RC staging is crucial for choosing the best multimodal therapy: patients with high risk locally advanced RC(LARC) undergo surgery after neoadjuvant chemotherapy and radiotherapy(NAT); those with low risk LARC are operated on after a preoperative short-course radiation therapy; finally, surgery alone is recommended only for early RC. Several imaging methods are used for staging patients with RC: computerized tomography, magnetic resonance imaging, positron emission tomography, and endoscopic ultrasound(EUS). EUS is highly accurate for the loco-regional staging of RC, since it is capable to evaluate precisely the mural infiltration of the tumor(T), especially in early RC. On the other hand, EUS is less accurate in restaging RC after NAT and before surgery. Finally, EUS is indicated for follow-up of patients operated on for RC, where there is a need for the surveillance of the anastomosis. The aim of this review is to highlight the impact of EUS on the management of patients with RC, evaluating its role in both preoperative staging and follow-up of patients after surgery. | Pietro Marone Mario de Bellis Valentina D'Angelo Paolo Delrio Valentina Passananti Elena Di Girolamo Giovanni Battista Rossi Daniela Rega Maura Claire Tracey Alfonso Mario Tempesta | 2015 | World Journal of Gastrointestinal Endoscopy2015，7，7： | 11 |
| 2 | Predictors of the Use of Physical Therapy Services Among Patients With Rheumatoid Arthritis 显示文摘 | Maura DI Ritu KC Nancy S | 2011 | Physical therapy2011，91，1： | 1 |
| 3 | A Variation in 3′ UTR of hPTP1B Increases Specific Gene Expression and Associates with Insulin Resistance显示文摘 | Rosa Di Paola Lucia Frittitta Giuseppe Miscio Maura Bozzali Roberto Baratta Marta Centra Daniela Spampinato Maria Grazia Santagati Tonino Ercolino Carmela Cisternino Teresa Soccio Sandra Mastroianno Vittorio Tassi Peter Almgren Antonio Pizzuti Riccardo Vi | 2002 | The American Journal of Human Genetics2002，，3： | 1 |
| 4 | Radiation therapy improves treatment outcome in patients with diffuse large B-cell lymphoma显示文摘 | Luigi Marcheselli Raffaella Marcheselli Alessia Bari ElianaValentina Liardo Fortunato Morabito Luca Baldini Maura Brugiatelli Francesco Merli Nicola Di Renzo Stefano Sacchi | 2011 | Leukemia & Lymphoma2011，，10： | 1 |
| 5 | Revascularization on the lateral wall: Long-term angiographic and clinical results of ra dial artery versus right internal thoracic artery grafting显示文摘 | Calafiore AM Di Maura M DAlessandro S | 2002 | J Thorac Cardiovasc Surg2002，123，2： | 1 |
| 6 | OPG and RANKL mRNA and protein expressions in the primary and secondary metaphyseal trabecular bone of PTH-treated rats are independent of that of SOST显示文摘 | Giuliana Silvestrini Paola Ballanti Mariangela Sebastiani Martina Leopizzi Maura Di Vito Ermanno Bonucci | 2008 | Journal of Molecular Histology2008，，2： | 1 |
| 7 | Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534显示文摘We report the radio observations of the eclipsing black widow pulsar J1720-0534, a 3.26 ms pulsar in orbit with a low mass companion of mass 0.029 to 0.034 M⊙. We obtain the phase-connected timing ephemeris and polarization profile of this millisecond pulsar(MSP) using the Five-hundred-meter Aperture Spherical radio Telescope(FAST), the Green Bank Telescope(GBT), and the Parkes Telescope. For the first time from such a system, an oscillatory polarization angle change was observed from a particular eclipse egress with partial depolarization, indicating 10-milliGauss-level reciprocating magnetic fields oscillating in a length scale of 5 ×10^(3)km(assuming an orbital inclination angle of 90°) outside the companion's magnetosphere. The dispersion measure variation observed during the ingresses and egresses shows the rapid raising of the electron density in the shock boundary between the companion's magnetosphere and the surrounding pulsar wind. We suggest that the observed oscillatory magnetic fields originate from the pulsar wind outside the companion's magnetosphere. | Chen-Chen Miao Victoria Blackmon Wei-Wei Zhu Dong-Zi Li Ming-Yu Ge Xiao-Peng You Maura McLaughlin Di Li Na Wang Pei Wang Jia-Rui Niu M.Cruces Jian-Ping Yuan Jun-Tao Bai D.J.Champion Yu-Tong Chen Ming-Min Chi P.C.C.Freire Yi Feng Zhen-Ye Gan M.Kramer Fei-Fei Kou Yu-Xi Li Xue-Li Miao Ling-Qi Meng Chen-Hui Niu Sheng-Nan Sun Zhong-Yi Sun H.M.Tedila Shuang-Qiang Wang Qing-Dong Wu Jing-Bo Wang Zhi-Gang Wen Shen Wang Ya-Biao Wang Cheng-Jie Wang Meng-Yao Xue You-Ling Yue Mao Yuan Ju-Mei Yao Wen-Ming Yan Ru-Shuang Zhao Lei Zhang De Zhao | 2023 | Research in Astronomy and Astrophysics2023，23，10： | 0 |
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