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Journal articles on the topic '0954'

Author: Grafiati

Published: 25 July 2024

Last updated: 31 July 2025

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1

Han, Cheongho, Andrzej Udalski, Doeon Kim, et al. "Three microlensing planets with no caustic-crossing features." Astronomy & Astrophysics 650 (June 2021): A89. http://dx.doi.org/10.1051/0004-6361/202140758.

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Aims. We search for microlensing planets with signals exhibiting no caustic-crossing features, considering the possibility that such signals may be missed due to their weak and featureless nature. Methods. For this purpose, we reexamine the lensing events found by the KMTNet survey before the 2019 season. From this investigation, we find two new planetary lensing events, KMT-2018-BLG-1976 and KMT-2018-BLG-1996. We also present the analysis of the planetary event OGLE-2019-BLG-0954, for which the planetary signal was known but no detailed analysis had previously been presented. We identify the

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2

Tanderup, K. "SP-0954 Above the diaphragm." Radiotherapy and Oncology 170 (May 2022): S847. http://dx.doi.org/10.1016/s0167-8140(22)04065-8.

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Gabuzda, D. C., P. Yu Kochanev, and R. I. Kollgaard. "VLBI Observations of Intraday Variability." International Astronomical Union Colloquium 164 (1998): 265–66. http://dx.doi.org/10.1017/s0252921100045486.

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AbstractIntegrated VLA measurements during our 6 cm global VLBI polarization observations of the intraday variable sources 0716+714, 0917+624, and 0954+658 indicate that although there were no significant total intensity variations during the 24-hour VLBI experiment, the polarization for all three sources varied substantially. Independent polarization images made for 2–3 hour segments show that there were no variations on VLBI scales for 0716+714 or 0954+658, but that there were appreciable variations in the VLBI core of 0917+624, which correlate well with the integrated variations in the simu

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Thriveni, Mallegowdanakoppalu C., Sampathkumar Deepa, Ganesan Thanavendan, G. Ravikumar, and B. T. Sreenivasa. "Characterization and Evaluation of Mulberry Genetic Resources for the Identification of Promising Accessions." Indian Journal of Plant Genetic Resources 36, no. 01 (2023): 85–95. http://dx.doi.org/10.61949/0976-1926.2023.v36i01.12.

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Mulberry is a dioecious species but, is usually cultivated as low bush or dwarf tree form by repeated pruning. Apart from its importance in silkworm rearing, it is also valued for its delicious fruits, medicinal properties in infusions, and ornamental shade tree. The conservation of mulberry genetic resources for future use and their subsequent usage in plant breeding are two critical areas of action in any genetic resource management programme. The current study used morphological, reproductive, anatomical, biochemical, propagation, growth, and yield variables to know the potential value of 2

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Bastien, L., R. Théoret, and R. Godbout. "0954 Sleep of Gifted Children Using Actigraphy." Sleep 43, Supplement_1 (2020): A362—A363. http://dx.doi.org/10.1093/sleep/zsaa056.950.

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Abstract Introduction Intellectual giftedness is characterized by an intellectual development superior to peers (QI &gt; 120) while emotional and relational development corresponds to the age norms. Anecdotal reports from parents suggest that they sleep poorly compared to typically developing (TD) peers. We measured sleep of gifted children using actigraphy. Methods Thirteen gifted children (10 boys, mean age = 10.58, SD = 2.11) were studied. Giftedness was identified using Renzulli’s three-factor definition of giftedness conceptualise in terms of above-average ability and high levels of t

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Ahnen, M. L., S. Ansoldi, L. A. Antonelli, et al. "Detection of the blazar S4 0954+65 at very-high-energy with the MAGIC telescopes during an exceptionally high optical state." Astronomy & Astrophysics 617 (September 2018): A30. http://dx.doi.org/10.1051/0004-6361/201832624.

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Aims. The very high energy (VHE ≳100 GeV) γ-ray MAGIC observations of the blazar S4 0954+65, were triggered by an exceptionally high flux state of emission in the optical. This blazar has a disputed redshift of z = 0.368 or z ≥ 0.45 and an uncertain classification among blazar subclasses. The exceptional source state described here makes for an excellent opportunity to understand physical processes in the jet of S4 0954+65 and thus contribute to its classification. Methods. We investigated the multiwavelength (MWL) light curve and spectral energy distribution (SED) of the S4 0954+65 blazar dur

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González, J. Becerra, J. A. Acosta-Pulido, W. Boschin, et al. "Optical spectral characterization of the gamma-ray blazars S4 0954+65, TXS 1515−273, and RX J0812.0+0237." Monthly Notices of the Royal Astronomical Society 504, no. 4 (2021): 5258–69. http://dx.doi.org/10.1093/mnras/stab1274.

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ABSTRACT The study of gamma-ray blazars is usually hindered due to the lack of information on their redshifts and on their low-energy photon fields. This information is key to understand the effect on the gamma-ray absorption due to either extragalactic background light and/or intrinsic absorption and emission processes. All this information has also an impact on the determination of the location of the emitting region within the relativistic jets. In this work, a new optical spectroscopic characterization is presented for three gamma-ray blazars: S4 0954+65, TXS 1515−273, and RX J0812.0+0237.

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Гаген-Торн, В. А., В. М. Ларионов, А. А. Архаров та ін. "Оптическая переменность блазара S4 0954+658 в 2008–2012 гг." Астрономический журнал 92, № 06 (2015): 514–26. http://dx.doi.org/10.7868/s0004629915050035.

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Vlasyuk, V. V., Yu V. Sotnikova, A. E. Volvach, et al. "Optical and Radio Variability of the Blazar S4 0954+658." Astrophysical Bulletin 78, no. 4 (2023): 464–86. http://dx.doi.org/10.1134/s1990341323600229.

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10

Morozova, Daria, Valeri Larionov, Svetlana Jorstad, et al. "Optical Outburst of the Blazar S4 0954+658 in Early 2015." Galaxies 4, no. 3 (2016): 24. http://dx.doi.org/10.3390/galaxies4030024.

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11

Hagen-Thorn, V. A., V. M. Larionov, A. A. Arkharov, et al. "Optical variability of the blazar S4 0954+658 in 2008–2012." Astronomy Reports 59, no. 6 (2015): 551–62. http://dx.doi.org/10.1134/s1063772915050030.

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12

Вольвач, А. Е., В. С. Бычкова, М. Г. Ларионов та ін. "Нестационарное излучение блазара S4 0954+658 в широком диапазоне длин волн". Астрономический журнал 93, № 12 (2016): 1012–22. http://dx.doi.org/10.7868/s0004629916120069.

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13

Cox, Rebecca, Brandon Aylward, Isabella Macarelli, and Michele Okun. "0954 Associations Between Sleep Duration and Timing and Postpartum Anxiety Symptoms." SLEEP 47, Supplement_1 (2024): A409. http://dx.doi.org/10.1093/sleep/zsae067.0954.

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Abstract Introduction Postpartum anxiety is understudied and underdiagnosed in postpartum women, despite being more common than postpartum depression. Given associations between postpartum anxiety and adverse maternal and infant outcomes, it is crucial to identify patterns and predictors of postpartum anxiety. We examined the associations between sleep duration and timing and postpartum anxiety over 6 months following delivery. Methods Pregnant women (n=147; 30-39 weeks) with a history of depression completed the Pittsburgh Sleep Quality Index (PSQI), Edinburgh Postnatal Depression Scale, and

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14

O'SULLIVAN, S. P., and D. C. GABUZDA. "PARSEC-SCALE INVESTIGATION OF THE MAGNETIC FIELD STRUCTURE OF SEVERAL AGN JETS." International Journal of Modern Physics D 17, no. 09 (2008): 1553–60. http://dx.doi.org/10.1142/s0218271808013145.

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Multi-frequency (4.6, 5, 5.5, 8, 8.8, 13, 15, 22 & 43 GHz) polarization observations of six "blazars" were obtained on the American Very Long Baseline Array (VLBA) over a 24-hr period on 2 July 2006. Observing at several frequencies, separated by short and long intervals, enabled reliable determination of the distribution of Faraday rotation on a range of scales. In all cases the magnitude of the RM increases in the higher frequency observations, implying that the electron density and/or magnetic field strength is increasing as we get closer to the central engine. After correcting for Fara

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15

Fiedler, Ralph, Brian Dennison, and Kenneth Johnston. "Extreme Scattering Events." Symposium - International Astronomical Union 129 (1988): 301–2. http://dx.doi.org/10.1017/s0074180900134771.

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Dally flux density measurements of 36 extragalactic radio sources over a seven year period, obtained by the Green Bank interferometer, reveal several unusual minima in the light curves that do not follow typical source variations (Fiedler et al. 1987). The most significant departure from typical source variability occurred at both frequencies in the quasar 0954+658 between 1980.95 and 1981.3. Refractive focussing by small scale inhomogeneities in an ionized structure in the interstellar medium appears to be the most likely explanation.

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Bachev, Rumen, Anton Strigachev, Evgeni Semkov, et al. "The Extremes in Intra-Night Blazar Variability: The S4 0954+65 Case." Galaxies 4, no. 3 (2016): 13. http://dx.doi.org/10.3390/galaxies4030013.

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17

Cimò, Giuseppe, T. Beckert, T. P. Krichbaum, et al. "A Very Rapid Extreme Scattering Event in the IDV Source 0954+658." Publications of the Astronomical Society of Australia 19, no. 1 (2002): 10–13. http://dx.doi.org/10.1071/as01097.

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AbstractExtreme scattering events (ESEs) are dramatic variations of the flux density at gigahertz frequencies caused by ray path distortions within an isolated inhomogeneity (‘plasma lens’) in the interstellar medium. These events are characterised by a deep flux density minimum in the light curve with, in some cases, surrounding maxima. The variability time scales range from weeks to months. These phenomena show a strong frequency dependence, in which the variability amplitudes increase with wavelength. During an intraday variability (IDV) monitoring project (March 2000), a feature resembling

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18

Morozova, D. A., V. M. Larionov, I. S. Troitsky, et al. "THE OUTBURST OF THE BLAZAR S4 0954+658 IN 2011 MARCH-APRIL." Astronomical Journal 148, no. 3 (2014): 42. http://dx.doi.org/10.1088/0004-6256/148/3/42.

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19

Leroi, N., A. Noel, S. Blacher, E. Lenaerts, P. Coucke, and P. Martinive. "PO-0954: Impact of neoadjuvant radiotherapy on tumor inflammatory microenvironment and metastases." Radiotherapy and Oncology 111 (2014): S128. http://dx.doi.org/10.1016/s0167-8140(15)31072-0.

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20

Kishore, Shubham, Alok C. Gupta, and Paul J. Wiita. "Detection of Quasiperiodic Oscillations in the Blazar S4 0954+658 with TESS." Astrophysical Journal 943, no. 1 (2023): 53. http://dx.doi.org/10.3847/1538-4357/aca809.

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Abstract We report the detection of several quasiperiodicities around 0.6–2.5 days in the optical emission of the blazar S4 0954+658. The source was observed by the Transiting Exoplanet Survey Satellite in six sectors and it showed these features in all but one of them, with a quasiperiodic oscillation of 1.52 days apparently present in portions of four of them. We used the generalized Lomb–Scargle periodogram method to search for significant signals and we confirmed them using a weighted wavelet transform for time–frequency domain analyses. We discuss several possible explanations for these r

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21

Marchenko, S. G., A. P. Marscher, J. R. Mattox, A. E. Wehrle та W. Xu. "Multi-Epoch VLBA Observations of γ-Ray Bright Blazars". International Astronomical Union Colloquium 164 (1998): 67–68. http://dx.doi.org/10.1017/s0252921100044560.

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AbstractWe have investigated the sub-milliarcsecond scale structure of 41 γ-ray bright blazars with the VLBA at frequencies of 22, 43, and occasionally 8.4 GHz. All of the blazars have dominant, unresolved (less than 0.1 to 0.2 milliarcsec) cores, with the exception of 0954+556, which has no structure apparent on scales less than about 1 milliarcsec. Some have prominent jets, others show only faint secondary components or no non-core structure at all. Apparent velocities have been measured for 13 sources. These range from no detected motion to > 25c.

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22

Sousa, F., I. Azevedo, D. Moreira, et al. "PO-0954: Occult Primary Breast Carcinoma with axillary involvement: two different treatment approaches." Radiotherapy and Oncology 152 (November 2020): S510. http://dx.doi.org/10.1016/s0167-8140(21)00972-5.

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23

Volvach, A. E., L. N. Volvach, and M. G. Larionov. "Parameters of binary systems in 0235+164, 0528+134 and 0954+658 blazars." Infocommunications and Radio Technologies 1, no. 1 (2018): 7–16. http://dx.doi.org/10.15826/icrt.2018.01.1.01.

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24

Ivanenko, A., L. Kek, and J. Grosrenaud. "0954 LONG-TERM USE OF MODAFINIL AND ARMODAFINIL IN PEDIATRIC PATIENTS WITH NARCOLEPSY." Sleep 40, suppl_1 (2017): A354—A355. http://dx.doi.org/10.1093/sleepj/zsx050.953.

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25

Hartt, William H. "Analytical Evaluation of Time-to-Corrosion for Chloride-Exposed Reinforced Concrete with an Admixed Corrosion Inhibitor: Part 2—Consideration of Diffusional Inhibitor Egress." CORROSION 70, no. 2 (2014): 156–65. http://dx.doi.org/10.5006/0954.

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26

Raiteri, C. M., M. Villata, V. M. Larionov, et al. "The complex variability of blazars: time-scales and periodicity analysis in S4 0954+65." Monthly Notices of the Royal Astronomical Society 504, no. 4 (2021): 5629–46. http://dx.doi.org/10.1093/mnras/stab1268.

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ABSTRACT Among active galactic nuclei, blazars show extreme variability properties. We here investigate the case of the BL Lac object S4 0954+65 with data acquired in 2019–2020 by the Transiting Exoplanet Survey Satellite (TESS) and by the Whole Earth Blazar Telescope (WEBT) Collaboration. The 2-min cadence optical light curves provided by TESS during three observing sectors of nearly 1 month each allow us to study the fast variability in great detail. We identify several characteristic short-term time-scales, ranging from a few hours to a few days. However, these are not persistent, as they d

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Papadakis, I. E., V. Samaritakis, P. Boumis, and J. Papamastorakis. "Multi-band optical micro-variability observations of the BL Lac object S4 0954+658." Astronomy & Astrophysics 426, no. 2 (2004): 437–43. http://dx.doi.org/10.1051/0004-6361:20040446.

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28

Landoni, M., R. Falomo, A. Treves, R. Scarpa, and D. Reverte Payá. "WHAT IS THE REDSHIFT OF THE GAMMA-RAY BL LAC SOURCE S4 0954+65?" Astronomical Journal 150, no. 6 (2015): 181. http://dx.doi.org/10.1088/0004-6256/150/6/181.

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29

Gabuzda, D. C., P. Y. Kochenov, R. I. Kollgaard, and T. V. Cawthorne. "VLBI and VLA observations of intraday polarization variability in 0917+624 and 0954+658." Monthly Notices of the Royal Astronomical Society 315, no. 2 (2000): 229–40. http://dx.doi.org/10.1046/j.1365-8711.2000.03400.x.

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30

Bajkova, Anisa T., and Alexander B. Pushkarev. "Multifrequency synthesis algorithm based on the generalized maximum entropy method: application to 0954+658." Monthly Notices of the Royal Astronomical Society 417, no. 1 (2011): 434–43. http://dx.doi.org/10.1111/j.1365-2966.2011.19280.x.

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31

Wang, Y., S. Tadimalla, L. Holloway, and A. Haworth. "MO-0954 Impact of androgen deprivation therapy on Imaging treatment response following prostate radiotherapy." Radiotherapy and Oncology 182 (May 2023): S802—S803. http://dx.doi.org/10.1016/s0167-8140(23)08494-3.

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32

Zhao, P. Y., T. S. Li, S. Shanmugam, S. Kathannan, R. X. Lan, and I. H. Kim. "0954 Effect of dietary flaxseed oil on growth performance, nutrient digestibility, blood profiles, and meat quality in pigs." Journal of Animal Science 94, suppl_5 (2016): 459. http://dx.doi.org/10.2527/jam2016-0954.

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33

Volvach, A. E., V. S. Bychkova, M. G. Larionov, et al. "Non-stationary emission of the blazar S4 0954+658 over a wide range of wavelength." Astronomy Reports 60, no. 12 (2016): 1035–45. http://dx.doi.org/10.1134/s1063772916120052.

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34

Schleicher, U., M. Türker, E. Bosch, W. Hürter, L. Paas, and A. Sauerwald. "PO-0954: Breast IORT by HDR-afterloading with a balloon catheter applicator is well tolerated." Radiotherapy and Oncology 106 (March 2013): S368. http://dx.doi.org/10.1016/s0167-8140(15)33260-6.

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35

Jiang, L., S. Lu, J. Lu, et al. "PO-0954 A Prediction Model of Acute Esophageal Toxicity in Esophageal Squamous Cell Carcinoma Patients." Radiotherapy and Oncology 133 (April 2019): S516—S517. http://dx.doi.org/10.1016/s0167-8140(19)31374-x.

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36

Sjöberg, F., D. Malipatlolla, G. Steineck, and C. Bull. "PO-0954: A model to study long-term impact of radiation towards the colorectal area." Radiotherapy and Oncology 123 (May 2017): S527—S528. http://dx.doi.org/10.1016/s0167-8140(17)31391-9.

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37

Gong, Yunlu, Shiting Tian, Liancheng Zhou, Tingfeng Yi та Jun Fang. "Two Transient Quasi-periodic Oscillations in γ-Ray Emission from the Blazar S4 0954+658". Astrophysical Journal 949, № 2 (2023): 39. http://dx.doi.org/10.3847/1538-4357/acca7b.

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Abstract In this work, we report periodicity search analyses in the gamma-ray light curve of the blazar S4 0954+658 in monitoring undertaken by the Fermi Large Area Telescope. Four analytical methods and a tool are adopted to detect any periodic flux modulation and corresponding significance level, revealing: (i) a quasi-periodic oscillation (QPO) of 66 days with a significance level of >5σ spanning over 600 days from 2015 to 2016 (MJD 57,145–57,745), resulting in continuous observation of nine cycles, which is one of the longest cycles discerned in blazar gamma-ray light curves; (ii) a pos

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38

Bratland, Å., H. A. Eide, and J. A. Kyte. "PO-0954 REPORT; REirradiation and PD-1 blockade On Recurrent squamous cell head and neck Tumors." Radiotherapy and Oncology 161 (August 2021): S795. http://dx.doi.org/10.1016/s0167-8140(21)07405-3.

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39

Mukherjee, R., H. D. Aller, M. F. Aller, et al. "EGRET gamma-ray sources: GRO J0744+54 and GRO J0957+65 (= BL Lacertae object 0954+658)." Astrophysical Journal 445 (May 1995): 189. http://dx.doi.org/10.1086/175685.

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Ciardo, D., M. A. Gerardi, S. Vigorito, et al. "PO-0954: Evaluation of specific and general-purpose atlases for automatic segmentation in breast cancer radiotherapy." Radiotherapy and Oncology 115 (April 2015): S502—S503. http://dx.doi.org/10.1016/s0167-8140(15)40946-6.

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41

Bachev, Rumen. "Violent intranight optical variability of the blazar S4 0954+65 during its unprecedented 2015 February outburst." Monthly Notices of the Royal Astronomical Society: Letters 451, no. 1 (2015): L21—L24. http://dx.doi.org/10.1093/mnrasl/slv059.

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42

Calderone, G., G. Ghisellini, M. Colpi та M. Dotti. "B2 0954+25A: a typical Fermi blazar or a γ-ray loud Narrow Line Seyfert 1≟". Monthly Notices of the Royal Astronomical Society 424, № 4 (2012): 3081–93. http://dx.doi.org/10.1111/j.1365-2966.2012.21456.x.

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43

Taheruzzaman, K., A. Akhundlu, T. Suzuki, et al. "0954 MPZL3 is a novel, therapeutically targetable mitochondrial regulator of human sebaceous gland homeostasis and function." Journal of Investigative Dermatology 145, no. 8 (2025): S165. https://doi.org/10.1016/j.jid.2025.06.970.

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44

Apolle, R., M. Rehm, J. Thiele, S. Brückner, J. Hampe, and E. Troost. "PO-0954: Fiducial markers and daily kV imaging improve patient setup during proton RT of esophageal cancer." Radiotherapy and Oncology 127 (April 2018): S521—S522. http://dx.doi.org/10.1016/s0167-8140(18)31264-7.

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45

Costa, P., A. M. N. Syed, H. Chang, et al. "PO-0954: Early results of a multi-center trial of IORT using electronic brachytherapy for breast cancer." Radiotherapy and Oncology 119 (April 2016): S464. http://dx.doi.org/10.1016/s0167-8140(16)32204-6.

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46

Kesavadev, J., B. Saboo, S. R. Joshi, et al. "IDF2022-0954 Points in Range (PIR) as an alternative to Time in Range in Resource limited settings." Diabetes Research and Clinical Practice 197 (March 2023): 110358. http://dx.doi.org/10.1016/j.diabres.2023.110358.

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47

SHIN, I. G., Y. H. RYU, A. UDALSKI, et al. "A SUPER-JUPITER MICROLENS PLANET CHARACTERIZED BY HIGH-CADENCE KMTNET MICROLENSING SURVEY OBSERVATIONS OF OGLE-2015-BLG-0954." Journal of The Korean Astronomical Society 49, no. 3 (2016): 73–81. http://dx.doi.org/10.5303/jkas.2016.49.3.73.

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48

Okuda, Shoki, Jumpei Tetsuka, Kenichi Takahashi, Yasuo Toda, Takekazu Kubo, and Shigeru Tokita. "0954 Association between Sleep Disturbance in Alzheimer's Disease Patients and Burden on and Health Status of Their Caregivers." Sleep 42, Supplement_1 (2019): A383—A384. http://dx.doi.org/10.1093/sleep/zsz067.952.

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Mikuš, Tomislav, Lidija Kozačinski, Željka Cvrtila, et al. "The influence of season and age on the levels of lipids, lipoproteins and enzymes in the serum of Lička pramenka sheep." Veterinarski arhiv 91, no. 1 (2021): 31–37. http://dx.doi.org/10.24099/vet.arhiv.0954.

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This study aimed to identify seasonal and age related variability in triglycerides (TRI), paraoxonase (PON), stimulated PON (PON I) and cholesterol (CHOL, HDL, LDL) in extensively reared Lička pramenka sheep. The study was conducted 30 randomly chosen non-gravid Lička pramenka sheep on an extensive farm, grouped into three age groups in the Karlovac County, Croatia. Blood was collected by venepuncture of the jugular vein, twice in one year - the first sampling in spring (April) and the second in autumn (October). The results showed that age had no significant effect on any of the investigated

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Mdodo, Rennatus, Emma L. Frazier, Shanta R. Dube, et al. "Cigarette Smoking Prevalence Among Adults With HIV Compared With the General Adult Population in the United States." Annals of Internal Medicine 162, no. 5 (2015): 335. http://dx.doi.org/10.7326/m14-0954.

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