First-Line Therapy for Patients with Advanced Hodgkin’s Lymphoma: Efficacy and Toxicity of Intensive ЕАСОРР-14 Program (NN Blokhin National Medical Cancer Research Center Data)

Aim. To assess the efficacy and toxicity of intensive 6 courses EACOPP-14 treatment with or without radiotherapy (RT) for advanced stages of Hodgkin’s lymphoma (HL). Materials & Methods. From November 2009 to February 2015, 95 patients with advanced stages of HL (IIX–IIE, III–IV) aged between 17 and 50 years (median 29 years) were selected for the participation in the protocol ЛХМосква1-3. The study population consisted of 46.3 % men and 53.7 % women. The results of the treatment were assessed in 91 patients who have received more than 2 courses of EACOPP-14. The follow up period was at least 3 months after the receiving the therapy. Consolidation RT with a total dose of 30 Gy for residual tumor lesions and/or initially large tumors was performed after the chemotherapy. Results. Complete remission was achieved in 82 (90.1 %) patients, partial remission in 2 (2.2 %), and the progression was observed in 7 (7.7 %) patients. The overall 4-year survival rate was 90.8 %, the progression-free survival was 88.2 %. The toxicity of the ЕАСОРР-14 program was slightly lower than that of 8 courses of ВЕАСОРРesc, and was comparable to the toxicity of other modifications of intensified ВЕАСОРР scheme. Hematological toxicity grade 3 and 4 was most commonly observed: leukopenia was observed after 64.9 % of courses, anemia — after 24 % of courses, thrombocytopenia — after 3.8 % of courses. The rate of infections did not singificantly differ and accounted for 24 %. The most frequent non-infectious complications were mucositis (21.1 %) and polyneuropathy (11.7 %). Complications resulted in the change of treatment in only 3 (3.01 %) of patients. The exclusion of bleomycine from the ЕАСОРР-14 program reduced the frequency of RT complications. Grade 3 pulmonitis developed in 4.5 % of cases, while radiation-induce pulmonary fibrosis verified by CT developed in 15.2 % of cases. The ЕАСОРР-14 6 courses program showed its high efficacy both with and without RT, high tolerance and the possibility of full administration for the majority of patients with the various stages of HL. Conclusion. Current research showed the efficacy of treatment without RT for patients with advanced stages of HL with negative PET results and small (< 2.5 cm) residual tumors after intensive ЕАСОРР-14 program. This approach allowed to avoid a number of late treatment complications

Relevance of Positron-Emission Therapy for Optimization of Treatment of Advanced Hodgkin’s Lymphoma Using Intensive ЕАСОРР-14 Program

Aim. To evaluate the relevance of the positron-emission therapy (PET) for optimization of the therapy of advanced Hodgkin’s lymphoma (HL) using the intensive EACOPP-14 program. Materials & Methods. 91 patients with advanced HL (IIX–IIE, III–IV) received the treatment according to the “ЛХМосква1-3” protocol over the period from November 2009 to February 2015, and then the treatment was analyzed. The median age was 29 years (range: 17–50); there were 42 men (46.3 %) and 49 (53.7 %) women. The treatment included 6 cycles of polychemotherapy according to the regimen ЕА(50)СОРР-14 ± radiation therapy. The radiation therapy was performed in 66 patients (72.5 %) after the completion of the chemotherapy. The cumulative focal dose was 30 Gy onto the areas of residual lesions and/or initially large tumor masses. Results. PET performed during the initial HL diagnosing permited to identify new areas of neoplastic lesions without changes in staging and treatment scheme, as well as specify areas and field size of planned radiation consolidation. The paper confirms the prognostic value of the intermediate PET in patients with advanced HL during the intensive first-line chemotherapy. The intensive therapy at the beginning of the treatment program is associated with higher chances for survival for patients with extremely unfavorable prognosis. After completion of the drug therapy, negative PET findings had a higher prognostic value, than the positive ones. The analysis of the relevance of residual tumor dimensions in the PET negative group demonstrated that the relapses were more common, if the residual tumor was more than 4.5 cm (according to CT findings). Conclusion. This study confirmed that it reasonable to discuss the discontinuation of the radiation therapy in patients with advanced HL, negative PET findings and small (< 2.5 cm) residual tumor after the intensive ЕАСОРР-14 program. This tactics permits avoiding a number of delayed complications

A change in the optical polarization associated with a gamma-ray flare in the blazar 3C 279

It is widely accepted that strong and variable radiation detected over all accessible energy bands in a number of active galaxies arises from a relativistic, Doppler-boosted jet pointing close to our line of sight. The size of the emitting zone and the location of this region relative to the central supermassive black hole are, however, poorly known, with estimates ranging from light-hours to a light-year or more. Here we report the coincidence of a gamma-ray flare with a dramatic change of optical polarization angle. This provides evidence for co-spatiality of optical and gamma-ray emission regions and indicates a highly ordered jet magnetic field. The results also require a non-axisymmetric structure of the emission zone, implying a curved trajectory for the emitting material within the jet, with the dissipation region located at a considerable distance from the black hole, at about 10^5 gravitational radii.Comment: Published in Nature issued on 18 February 2010. Corresponding authors: Masaaki Hayashida and Greg Madejsk

Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

Aims. We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1, which includes, among other instruments, MAGIC, VERITAS, Whipple 10 m, and Fermi-LAT to cover the gamma-ray range from 0.1 GeV to 20 TeV; RXTE and Swift to cover wavelengths from UV to hard X-rays; and GASP-WEBT, which provides coverage of radio and optical wavelengths. Optical polarization measurements were provided for a fraction of the campaign by the Steward and St. Petersburg observatories. We evaluate the variability of the source and interband correlations, the gamma-ray flaring activity occurring in May 2009, and interpret the results within two synchrotron self-Compton (SSC) scenarios.Methods. The multiband variability observed during the full campaign is addressed in terms of the fractional variability, and the possible correlations are studied by calculating the discrete correlation function for each pair of energy bands where the significance was evaluated with dedicated Monte Carlo simulations. The space of SSC model parameters is probed following a dedicated grid-scan strategy, allowing for a wide range of models to be tested and offering a study of the degeneracy of model-to-data agreement in the individual model parameters, hence providing a less biased interpretation than the "single-curve SSC model adjustment" typically reported in the literature.Results. We find an increase in the fractional variability with energy, while no significant interband correlations of flux changes are found on the basis of the acquired data set. The SSC model grid-scan shows that the flaring activity around May 22 cannot be modeled adequately with a one-zone SSC scenario (using an electron energy distribution with two breaks), while it can be suitably described within a two (independent) zone SSC scenario. Here, one zone is responsible for the quiescent emission from the averaged 4.5-month observing period, while the other one, which is spatially separated from the first, dominates the flaring emission occurring at X-rays and very-high-energy (> 100 GeV, VHE) gamma-rays. The flaring activity from May 1, which coincides with a rotation of the electric vector polarization angle (EVPA), cannot be satisfactorily reproduced by either a one-zone or a two-independent-zone SSC model, yet this is partially affected by the lack of strictly simultaneous observations and the presence of large flux changes on sub-hour timescales (detected at VHE gamma rays).Conclusions. The higher variability in the VHE emission and lack of correlation with the X-ray emission indicate that, at least during the 4.5-month observing campaign in 2009, the highest energy (and most variable) electrons that are responsible for the VHE gamma rays do not make a dominant contribution to the similar to 1 keV emission. Alternatively, there could be a very variable component contributing to the VHE gamma-ray emission in addition to that coming from the SSC scenario. The studies with our dedicated SSC grid-scan show that there is some degeneracy in both the one-zone and the two-zone SSC scenarios probed, with several combinations of model parameters yielding a similar model-to-data agreement, and some parameters better constrained than others. The observed gamma-ray flaring activity, with the EVPA rotation coincident with the first gamma-ray flare, resembles those reported previously for low frequency peaked blazars, hence suggesting that there are many similarities in the flaring mechanisms of blazars with different jet properties

Покращення роботи кінологічних служб і здоров`я службових собак у правоохоронних органах

Ларіонова І. Т. Покращення роботи кінологічних служб і здоров`я службових собак у правоохоронних органах / Ларіонова І.Т. Слюсар Н.В. // Шляхи покращення професійного рівня працівників кінологічних служб : тези доп. Всеукр. наук.-практ. конф. (Харків, 14 груд. 2018 р.) / МВС України, Харків. нац. ун-т внутр. справ. - Харків, 2018.-Розгядаються питання діяльності кінологічних команд різних підрозділів, питання професійної підготовки вітчизняних кінологів. In the article reviewed with the question of the activities of the cynologists teams of different units. Also questions of professional training of domestic cynologists/ Рассматриваются вопросы деятельности кинологических команд разных подразделений, вопросы профессиональной подготовки отечественных кинологов

The awakening of BL Lacertae: observations by Fermi, Swift and the GASP-WEBT

Since the launch of the Fermi satellite, BL Lacertae has been moderately active at gamma-rays and optical frequencies until 2011 May, when the source started a series of strong flares. The exceptional optical sampling achieved by the GLAST-AGILE Support Program of the Whole Earth Blazar Telescope in collaboration with the Steward Observatory allows us to perform a detailed comparison with the daily gamma-ray observations by Fermi. Discrete correlation analysis between the optical and gamma-ray emission reveals correlation with a time lag of 0 +/- 1 d, which suggests cospatiality of the corresponding jet emitting regions. A better definition of the time lag is hindered by the daily gaps in the sampling of the extremely fast flux variations. In general, optical flares present more structure and develop on longer time-scales than corresponding gamma-ray flares. Observations at X-rays and at millimetre wavelengths reveal a common trend, which suggests that the region producing the mm and X-ray radiation is located downstream from the optical and gamma-ray-emitting zone in the jet. The mean optical degree of polarization slightly decreases over the considered period and in general it is higher when the flux is lower. The optical electric vector polarization angle (EVPA) shows a preferred orientation of about 15 degrees, nearly aligned with the radio core EVPA and mean jet direction. Oscillations around it increase during the 2011-2012 outburst. We investigate the effects of a geometrical interpretation of the long-term flux variability on the polarization. A helical magnetic field model predicts an evolution of the mean polarization that is in reasonable agreement with the observations. These can be fully explained by introducing slight variations in the compression factor in a transverse shock waves model

Multiwavelength behaviour of the blazar OJ 248 from radio to gamma-rays

We present an analysis of the multiwavelength behaviour of the blazar OJ 248 at z = 0.939 in the period 2006-2013. We use low-energy data (optical, near-infrared, and radio) obtained by 21 observatories participating in the Gamma-Ray Large Area Space Telescope (GLAST)-AGILE Support Program of the Whole Earth Blazar Telescope, as well as data from the Swift (optical-UV and X-rays) and Fermi (gamma-rays) satellites, to study flux and spectral variability and correlations among emissions in different bands. We take into account the effect of absorption by the Damped Lyman alpha intervening system at z = 0.525. Two major outbursts were observed in 2006-2007 and in 2012-2013 at optical and near-IR wavelengths, while in the high-frequency radio light curves prominent radio outbursts are visible peaking at the end of 2010 and beginning of 2013, revealing a complex radio-optical correlation. Cross-correlation analysis suggests a delay of the optical variations after the gamma-ray ones of about a month, which is a peculiar behaviour in blazars. We also analyse optical polarimetric and spectroscopic data. The average polarization percentage P is less than 3 per cent, but it reaches similar to 19 per cent during the early stage of the 2012-2013 outburst. A vague correlation of P with brightness is observed. There is no preferred electric vector polarization angle and during the outburst the linear polarization vector shows wide rotations in both directions, suggesting a complex behaviour/structure of the jet and possible turbulence. The analysis of 140 optical spectra acquired at the Steward Observatory reveals a strong Mg ii broad emission line with an essentially stable flux of 6.2 x 10(- 15) erg cm(- 2) s(- 1) and a full width at half-maximum of 2053 km s(- 1)