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| 1 | The sentinel node in gynaecological malignancies显示文摘 | Balega J Trappen POV | 2006 | Cancer hnaging2006，6，： | 1 |
| 2 | Primary non-Hodgkin's lymphoma of the uterine cervix successfully treated by neoadjuvant chemotherapy:case report显示文摘 | Szantho A Balega JJ Csapo Z | 2003 | Gynecol Oncol2003，89，1： | 1 |
| 3 | The risk of nodal metastasis in early adenocarcinoma of the uterine cervix显示文摘 | Balega J Michael H Sutton G P | 2004 | Intern J Gynecol Can2004，14，1： | 1 |
| 4 | The sentinel node in gynaecological malignancies显示文摘 | Balega J Van Trappen PO | 2006 | Cancer Lmaging2006，6，： | 1 |
| 5 | Surgical and oncological outcome of total laparoscopic radical hysterectomy in obese women with esrly-stage cervical cancer显示文摘 | Moss EL Balega J Chan KK | 2012 | Int J Gynecol Cancer2012，22，1： | 1 |
| 6 | The risk of nodal metastasis in early adenocarcinoma of the uterine cervix显示文摘 | Balega J Michael H Sutton GP | | 0，，01： | 1 |
| 7 | Surgical and oncological outcome of total laparoscopic radical hysterectomy in obese women with early-stage cervical cancer显示文摘 | Moss EL Balega J Chan KK | 2012 | Int J Gynecol Cancer2012，22，1： | 1 |
| 8 | Primary non-Hodgkin s lymphoma of the uterine cervix successfully treated by neoadju- vantchemotherapy: case report 显示文摘 | SzanthoA Balega JJ Csapo Z | 2003 | Gynecol Oncol2003，89，1： | 1 |
| 9 | The sentinel node in gynaecological malignancies显示文摘 | Balega J Van Trappen PO | 2006 | Cancer Imaging2006，6，： | 1 |
| 10 | The sentinel node in gynaecological malignancies 显示文摘 | Balega J Van Trappen PO | 2006 | Cancer Imaging2006，28，6： | 1 |
| 11 | The risk of nodal metastasis in early adenocarcinoma of the uterine cervix显示文摘 | Balega J Michael H SuRon G P | 2004 | Intemational Journal of Gynecological Cancer2004，14，1： | 1 |
| 12 | The sentinel node in gynaecological malignancies 显示文摘 | Balega J Van Trappen P O | 2006 | Cancer Imaging2006，6，： | 1 |
| 13 | The sentinel node in gynaecological malignancies显示文摘 | Balega J Van Trappen PO | | 0，，06： | 1 |
| 14 | The first results of observations of lunar occultations in different spectral ranges at the 6-m telescope of the SAO RAS显示文摘Observations by the method of lunar occultations at the 6-m telescope of the SAO RAS reach a resolution limit better than 1mas.We have devised a new method of observation,which allows obtaining the curves of lunar occultations simultaneously in different ranges of the visible part of the spectrum,and conducted the first observations using amodified optical system.In January 2019,applying the newmethod,the magnitude differences of the components of the binary star HD 36524 in the R and I bands were measured,which were 1.5 and 1.3mag,respectively,in good agreement with values calculated from the Gaia mission.According to the obtained data,it was determined that with this method it is possible to reach a signal-to-noise ratio of about 5–10 for stars of 10th magnitude.We discuss the applicability of the proposed optical scheme for the study of binary stars. | Ekaterina Shmaylova Vladimir Dyachenko Andrea Richichi Anatoly Beskakotov AleksandrMaksimov Arina Mitrofanova Yuri Balega | 2020 | Research in Astronomy and Astrophysics2020，20，11： | 0 |
| 15 | On the correctness of orbital solutions obtained from a small set of points.Orbit of HIP 53731显示文摘HIP 53731 is a binary consisting of stars of the spectral types K0 and K9.The orbit of this object was constructed previously by Cvetkovic et al.and improved by Tokovinin.It should be noted that there is a 180°ambiguity in the position angles of some published measurements.Speckle interferometric observations were obtained in 2007–2020(21 measurements)at the 6-m telescope of the SAO RAS(BTA)by the authors of this article.The analysis of new data together with previously published ones made it possible to construct an accurate orbit of HIP 53731 and to halve the already known values of the orbital period of the system.As a result of the study,the mass sum,the masses of each component and their spectral types were determined by two independent methods.According to the qualitative classification of orbits,the orbital solution has grade 2–'good'(observations cover more than half of the orbital period and correspond to different phases). | Arina Mitrofanova Vladimir Dyachenko Anatoly Beskakotov Yury Balega Alexander Maksimov Denis Rastegaev Sergey Komarinsky | 2020 | Research in Astronomy and Astrophysics2020，20，11： | 0 |
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