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pro vyhledávání: '"OGURA, K."'
Autor:
Pirozhkov, A. S., Sagisaka, A., Ogura, K., Vishnyakov, E. A., Shatokhin, A. N., Armstrong, C. D., Esirkepov, T. Zh., Izquierdo, B. Gonzalez, Pikuz, T. A., Hadjisolomou, P., Alkhimova, M. A., Arran, C., Tsygvintsev, I. P., Valenta, P., Pikuz, S. A., Yan, W., Jeong, T. M., Singh, S., Finke, O., Grittani, G., Nevrkla, M., Lazzarini, C., Velyhan, A., Hayakawa, T., Fukuda, Y., Koga, J. K., Ishino, M., Kondo, Ko., Miyasaka, Y., Kon, A., Nishikino, M., Nosach, Y. V., Khikhlukha, D., Kolesnikov, A. O., Ragozin, E. N., Gasilov, V. A., Kumar, D., Nejdl, J., Sasorov, P. V., Weber, S., Margarone, D., Kato, Y., Korn, G., Kiriyama, H., Kondo, K., Ridgers, C., Kawachi, T., Kando, M., Bulanov, S. V.
Gamma rays consist of high-energy photons that selectively interact with nuclei, induce and mediate nuclear reactions and elementary particle interactions, and exceed x-rays in penetrating power and thus are indispensable for analysis and modificatio
Externí odkaz:
http://arxiv.org/abs/2410.06537
Publikováno v:
Experiments in Fluids Volume 65, article number 102 (2024)
Pressure-sensitive paint (PSP) was applied to the surface of a NACA0012 airfoil to investigate pressure fluctuations associated with trailing edge (TE) noise under low-velocity flow conditions. The primary focus is to assess the feasibility of employ
Externí odkaz:
http://arxiv.org/abs/2407.04233
Autor:
Pirozhkova, M. S., Ogura, K., Sagisaka, A., Esirkepov, T. Zh., Faenov, A. Ya., Pikuz, T. A., Kotaki, H., Hayashi, Y., Fukuda, Y., Koga, J. K., Bulanov, S. V., Daido, H., Hasegawa, N., Ishino, M., Nishikino, M., Koike, M., Kawachi, T., Kiriyama, H., Kando, M., Neely, D., Pirozhkov, A. S.
High-order harmonics are ubiquitous in nature and present in electromagnetic, acoustic, and gravitational waves. They are generated by periodic nonlinear processes or periodic high-frequency pulses. However, this periodicity is often inexact, such as
Externí odkaz:
http://arxiv.org/abs/2306.01018
Autor:
Sinha, Tirthendu, Sharma, Saurabh, Panwar, Neelam, Matsunaga, N., Ogura, K., Kobayashi, N., Yadav, R. K., Ghosh, A., Pandey, R., Bisht, P. S.
We present the results from our time-series imaging data taken with the 1.3m Devasthal fast optical telescope and 0.81m Tenagara telescope in $V$, $R_{c}$, $I_{c}$ bands covering an area of $\sim18^\prime.4\times 18^\prime.4$ towards the star-forming
Externí odkaz:
http://arxiv.org/abs/2108.02107
Autor:
Sinha, Tirthendu, Sharma, Saurabh, Pandey, A. K., Yadav, R. K., Ogura, K., Matsunaga, N., Kobayashi, N., Bisht, P. S., Pandey, R., Ghosh, A.
We present multi-epoch deep ($\sim$20 mag) $I_{c}$~band photometric monitoring of the Sh 2-170 star-forming region to understand the variability properties of pre-main-sequence (PMS) stars. We report identification of 47 periodic and 24 non-periodic
Externí odkaz:
http://arxiv.org/abs/2001.08892
New observations in the $VI$ bands along with archival data from the 2MASS and $WISE$ surveys have been used to generate a catalog of young stellar objects (YSOs) covering an area of about $6^\circ\times6^\circ$ in the Auriga region centered at $l\si
Externí odkaz:
http://arxiv.org/abs/1912.11789
Akademický článek
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Autor:
Panwar, Neelam, Pandey, A. K., Samal, Manash R., Battinelli, Paolo, Ogura, K., Ojha, D. K., Chen, W. P., Singh, H. P.
Berkeley 59 is a nearby ($\sim$1 kpc) young cluster associated with the Sh2-171 H{\sc ii} region. We present deep optical observations of the central $\sim$2.5$\times$2.5 pc$^2$ area of the cluster, obtained with the 3.58-m Telescopio Nazionale Galil
Externí odkaz:
http://arxiv.org/abs/1711.09353
Autor:
Panwar, Neelam, Samal, M. R., Pandey, A. K., Jose, J., Chen, W. P., Ojha, D. K., Ogura, K., Singh, H. P., Yadav, R. K.
W4 is a giant H{\sc ii} region ionized by the OB stars of the cluster IC~1805. The H{\sc ii} region/cluster complex has been a subject of numerous investigations as it is an excellent laboratory for studying the feedback effect of massive stars on th
Externí odkaz:
http://arxiv.org/abs/1703.03604
Autor:
Sharma, Saurabh, Pandey, A. K., Ojha, D. K., Bhatt, Himali, Ogura, K., Kobayashi, N., Yadav, R., Pandey, J. C.
Deep optical photometric data on the NGC 7538 region were collected and combined with archival data sets from $Chandra$, 2MASS and {\it Spitzer} surveys in order to generate a new catalog of young stellar objects (YSOs) including those not showing IR
Externí odkaz:
http://arxiv.org/abs/1701.00975