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Journal articles on the topic 'AKORI'

Author: Grafiati

Published: 4 June 2021

Last updated: 4 February 2022

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1

Polkowski, Wojciech P., and Krzysztof Bujko. "Lizboński akord." Nowotwory. Journal of Oncology 64, no. 3 (2014): 284. http://dx.doi.org/10.5603/njo.2014.0047.

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2

Eremeeva, M. E., M. M. Sturgeon, J. K. Willard, S. E. Karpathy, A. Madan, and G. A. Dasch. "Molecular typing of Rickettsia akari." Russian Journal of Infection and Immunity 10, no. 3 (2020): 497–505. http://dx.doi.org/10.15789/2220-7619-mto-1295.

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Rickettsia akari, an obligately intracellular bacterium, is the causative agent of the cosmopolitan urban disease rickettsialpox. R. akari is an atypical representative of spotted fever group rickettsiae (SFG) as it is associated with rodent mites rather than ticks or fleas; however, only limited information is available about the degree of genetic variability found among isolates of R. akari. We examined 13 isolates of R. akari from humans, rodents and mites in the USA, the former Soviet Union, and the former Yugoslavia made between 1946 and 2003 for diversity in their tandem repeat regions (

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3

Wajongkere, Yuanita, Jullia Titaley, and Yohanes A. R. Langi. "Fungsi Transposisi Modulo dan Penerapannya Pada Pencarian Susunan Tangga Nada dan Tingkatan Akor." d'CARTESIAN 8, no. 1 (2019): 11. http://dx.doi.org/10.35799/dc.8.1.2019.22789.

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Dalam musik, transposisi bertujuan untuk menaik-turunkan nada, nada dasar, dan akor pada sebuah lagu. Penelitian ini bertujuan untuk mencari susunan tangga nada mayor dan minor juga tingkatan akor minor menggunakan fungsi transposisi modulo 12. Data yang digunakan adalah data tentang tangga nada mayor, minor asli, harmonis dan melodis, serta tingkatan akor minor. Setelah ke 12 nada dasar diubah ke bentuk integer model of pitch, dengan memanfaatkan fungsi transposisi , ditemukan keseluruhan susunan tangga nada dimulai dari tangga nada mayor pada nada dasar C#, D, D#, E, F, F#, G, G#, A, A#, dan

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4

Yamauchi, C., S. Fujishima, N. Ikeda, et al. "AKARI-CAS—Online Service for AKARI All-Sky Catalogues." Publications of the Astronomical Society of the Pacific 123, no. 905 (2011): 852–64. http://dx.doi.org/10.1086/660926.

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5

Kaneda, Hidehiro, Daisuke Ishihara, Koudai Kobata, et al. "Processing of Interstellar Dust Grains in Galaxies Revealed by AKARI." Proceedings of the International Astronomical Union 8, S292 (2012): 271–74. http://dx.doi.org/10.1017/s1743921313001348.

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AbstractWith AKARI, we have performed a systematic study of interstellar dust grains in various environments of galaxies. In many cases, the IR emission of dust is an important tool to trace star-forming activities in galaxies. However it is much more than just star-formation tracers. AKARI has revealed the detailed properties of dust grains in regions not relevant to star formation as well, some of which are found not to follow our old empirical knowledge. Because of its unique capabilities, such as near- and far-IR spectroscopy, and all-sky coverage, AKARI has provided new knowledge on the p

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6

Herlina, Linda. "Peningkatan Keterampilan Materi Akord dengan Model Pembelajaran Berkelompok pada Pembelajaran Seni Musik SMA Negeri 1 Kota Sukabumi." Briliant: Jurnal Riset dan Konseptual 4, no. 4 (2019): 488. http://dx.doi.org/10.28926/briliant.v4i4.406.

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Penelitian ini bertujuan untuk dapat memberikan perbaikan pada proses pembelajaran seni musik khususnya pada materi akord yang nantinya akan menjadi bekal saat mereka menganalisis musikalitas dan penyajian musik kontemporer serta berkreasi musik kontemporer. Metode yang digunakan dalam penelitian ini adalah action research atau penelitian tindakan. Adapun temuan penelitian ini yaitu: (1) Proses pelaksanaan pembelajaran materi akord dalam tingkat dengan pengaplikasian pada alat musik keyboard dan gitar menerapkan metode pembelajaran berkelompok (cooperatif learning) dengan tahapan pelaksanaan y

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7

Matsuhara, H., H. Murakami, T. Nakagawa, et al. "AKARI in Orbit—Scientific Potential for Understanding Galaxy Evolution." Proceedings of the International Astronomical Union 2, S235 (2006): 322. http://dx.doi.org/10.1017/s1743921306006879.

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AbstractThe AKARI (formerly known as ASTRO-F) mission is the first Japanese satellite dedicated for large area surveys in the infrared (Murakami et al. 2004). AKARI was launched successfully on February 22nd 2006 (JST) from JAXA's Uchinoura Space Centre, Japan. AKARI is now orbiting around the Earth in a Sun-synchronous polar orbit at the altitude of 700 km. The 68.5 cm aperture telescope and scientific instruments are cooled to 6K by liquid Helium and mechanical coolers. The expected liquid Helium holding time is now found to be at least one year after the successful aperture lid-opening on 2

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8

Oyabu, Shinki. "AKARI Infrared Views of AGNs." Proceedings of the International Astronomical Union 5, S267 (2009): 129. http://dx.doi.org/10.1017/s1743921310005909.

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AbstractThe Japanese infrared satellite AKARI has unique capabilities for near-infrared spectroscopy and an all-sky survey in the mid- and far-infrared. We present the recent results on active galactic nuclei that use the unique capabilities of AKARI.

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9

Blain, Andrew W. "WISE AND AKARI." Publications of The Korean Astronomical Society 27, no. 4 (2012): 367–73. http://dx.doi.org/10.5303/pkas.2012.27.4.367.

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10

Ueta, Toshiya, Ryszard Szczerba, Andrew G. Fullard, and Satoshi Takita. "Planetary Nebulae Detected in the AKARI Far-IR All-Sky Survey Maps." Proceedings of the International Astronomical Union 14, S343 (2018): 522–24. http://dx.doi.org/10.1017/s1743921318006452.

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AbstractThe AKARI Far-IR All-Sky Survey (AFASS) maps produced by the AKARI Infrared Astronomical Satellite enabled us to probe the far-IR sky for objects having surface brightnesses greater than a few to a couple of dozen MJy sr−1. Recently, we have verified that, if AFASS-measured fluxes are properly corrected for using the aperture correction method based on the empirical point-spread-function templates derived directly from the AFASS maps, point-source photometry measured from the AFASS maps reproduces fluxes in the AKARI bright source catalogue (BSC). We have surveyed the far-IR sky in the

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11

Usui, Fumihiko, Daisuke Kuroda, Thomas G. MÜLler, et al. "Asteroid Catalog Using AKARI: AKARI/IRC Mid-Infrared Asteroid Survey." Publications of the Astronomical Society of Japan 63, no. 5 (2011): 1117–38. http://dx.doi.org/10.1093/pasj/63.5.1117.

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12

Kim, Seong Jin, Nagisa Oi, Tomotsugu Goto, et al. "Identification of AKARI infrared sources by the Deep HSC Optical Survey: construction of a new band-merged catalogue in the North Ecliptic Pole Wide field." Monthly Notices of the Royal Astronomical Society 500, no. 3 (2020): 4078–94. http://dx.doi.org/10.1093/mnras/staa3359.

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ABSTRACT The North Ecliptic Pole field is a natural deep-field location for many satellite observations. It has been targeted many times since it was surveyed by the AKARI space telescope with its unique wavelength coverage from the near- to mid-infrared (mid-IR). Many follow-up observations have been carried out, making this field one of the most frequently observed areas with a variety of facilities, accumulating abundant panchromatic data from the X-ray to the radio wavelength range. Recently, a deep optical survey with the Hyper Suprime-Cam (HSC) at the Subaru telescope covered the NEP-Wid

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13

Huang, Ting-Chi, Hideo Matsuhara, Tomotsugu Goto, et al. "CFHT MegaPrime/MegaCam u-band source catalogue of the AKARI North Ecliptic Pole Wide field." Monthly Notices of the Royal Astronomical Society 498, no. 1 (2020): 609–20. http://dx.doi.org/10.1093/mnras/staa2459.

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ABSTRACT The $AKARI$ infrared (IR) space telescope conducted two surveys (Deep and Wide) in the North Ecliptic Pole (NEP) field to find more than 100 000 IR sources using its infrared camera (IRC). IRC’s nine filters, which cover wavebands from 2 to 24 μm continuously, make $AKARI$ unique in comparison with other IR observatories such as $Spitzer$ or $WISE$. However, studies of the $AKARI$ NEP-Wide field sources had been limited due to the lack of follow-up observations in the ultraviolet (UV) and optical. In this work, we present the Canada–France–Hawaii Telescope MegaPrime/MegaCam u-band sou

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14

Tika Setiarini, Agnes, Agoeng Prasetyo, and Suryati Suryati. "Analisis dan Interpretasi Lagu Desafinado karya Antonio Carlos Jobim." PROMUSIKA 4, no. 1 (2016): 13–20. http://dx.doi.org/10.24821/promusika.v4i1.2268.

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Studi ini membahas musik Jazz Latin dari Jobim yang merupakan percampuran antara musik jazz dan musik latin. Pada musik ini jazz dengan variasi akor yang beragam digabungkan dengan musik latin yang kaya akan permainan ritmis alat musik perkusi. Irama musik latin jazz yang bermacam-macam membuat musik ini mendapatkan apresiasi yang tinggi. Lagu Desafinado ciptaan Antonio Carlos Jobim adalah salah satu lagu standart latin jazz yang sangat terkenal.Desafinado memiliki banyak hal yang menarik untuk diteliti, yaitu dari bentuk lagu, progresi akor, dan interpretasi lirik lagu. Analisis yang dilakuka

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15

Yuan, Fang-Ting, Tsutomu T. Takeuchi, Véronique Buat, et al. "AKARI/IRC broadband mid-infrared data as an indicator of the Star Formation Rate." Proceedings of the International Astronomical Union 7, S284 (2011): 357–59. http://dx.doi.org/10.1017/s1743921312009416.

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AbstractWith the goal of constructing Star-Formation Rates (SFR) from AKARI Infrared Camera (IRC) data, we analyzed an IR-selected GALEX-SDSS-2MASS-AKARI(IRC & Far-Infrared Surveyor) sample of 153 nearby galaxies. The far-infrared fluxes were obtained from AKARI diffuse maps to correct the underestimation for extended sources raised by PSF photometry. SFRs of these galaxies were derived using the SED fitting program CIGALE. In spite of complicated features contained in these bands, both the S9W and L18W emissions correlate with the SFR of galaxies. The SFR calibrations using S9W and L18W a

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Eremeeva, M. E., and K. Muniz-Rodriguez. "Rickettsialpox — a rare but not extinct disease: review of the literature and new directions." Russian Journal of Infection and Immunity 10, no. 3 (2020): 477–85. http://dx.doi.org/10.15789/2220-7619-rar-1294.

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Rickettsialpox is an urban zoonosis caused by Rickettsia akari. To date R. akari is the only well-characterized mite-borne member of the spotted fever group. It is transmitted by the mouse mite, Liponyssoides sanguineus, commonly found on peridomestic rodents. While the disease was first discovered in New York City in 1946, a few years later a similar outbreak occurred in the Ukraine SSR. Numerous serosurveys and diagnosis of sporadic cases of rickettsialpox suggest its global distribution; however, the actual contemporary geography of rickettsialpox and its incidence are unknown. Rickettsialp

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17

Sedgwick, Chris, Stephen Serjeant, Chris Pearson, et al. "Far Infrared Luminosity Function of Local Galaxies in the AKARI Deep Field South." Proceedings of the International Astronomical Union 7, S284 (2011): 289–91. http://dx.doi.org/10.1017/s1743921312009271.

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AbstractWe present the first far-infrared luminosity function in the AKARI Deep Field South, a premier deep field of the AKARI Space Telescope, using spectroscopic redshifts obtained with AAOmega. To date, we have found spectroscopic redshifts for 389 galaxies in this field and have measured the local (z<0.25) 90 μm luminosity function using about one-third of these redshifts. The results are in reasonable agreement with recent theoretical predictions.

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18

Aston, D. A. "Akoris. Report of the Excavations at Akoris in Middle Egypt, 1981-1992." Journal of Egyptian Archaeology 83 (1997): 238. http://dx.doi.org/10.2307/3822476.

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19

Marton, G., L. V. Tóth, L. G. Balázs, et al. "A selection of AKARI FIS BSC extragalactic objects." Proceedings of the International Astronomical Union 11, S319 (2015): 101. http://dx.doi.org/10.1017/s1743921315010297.

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AbstractThe point sources in the Bright Source Catalogue (BSC) of the AKARI Far–Infrared Surveyor (FIS) were classified based on their far–IR and mid–IR fluxes and colours using Quadratic Discriminant Analysis method (QDA) and Support Vector Machines (SVM). The reliability of our results show that we can successfully separate galactic and extragalactic AKARI point sources in the multidimensional space of fluxes and colours. However, differentiating among the extragalactic sub–types needs further information.

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Miyaji, Takamitsu. "X-ray - Infrared relation of AGNs and search for highly obscured accretion in the AKARI NEP Field." Proceedings of the International Astronomical Union 15, S341 (2019): 172–76. http://dx.doi.org/10.1017/s1743921319002540.

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AbstractThe infrared Astronomical Satellite AKARI conducted deep (∼0.4 deg2) and wide (∼ 5.4 deg2) surveys around the North Ecliptic Pole (NEP) with its InfraRed Camera (IRC) with nine filters continuously covering the 2–25 μm range. These photometric bands include three filters that fill the “ Spitzer gap” between the wavelength coverages of IRAC and MIPS. This unique feature has enabled us to make sensitive mid-infrared detection of AGN candidates at z∼1-2, based on the Spectral Energy Distribution (SED) fitting including hot dust emission in the AGN torus. This enables us to compare X-rays

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21

Radulovic, S., P. W. Price, M. S. Beier, J. Gaywee, J. A. Macaluso, and A. Azad. "Rickettsia-Macrophage Interactions: Host Cell Responses to Rickettsia akari and Rickettsia typhi." Infection and Immunity 70, no. 5 (2002): 2576–82. http://dx.doi.org/10.1128/iai.70.5.2576-2582.2002.

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ABSTRACT The existence of intracellular rickettsiae requires entry, survival, and replication in the eukaryotic host cells and exit to initiate new infection. While endothelial cells are the preferred target cells for most pathogenic rickettsiae, infection of monocytes/macrophages may also contribute to the establishment of rickettsial infection and resulting pathogenesis. We initiated studies to characterize macrophage-Rickettsia akari and -Rickettsia typhi interactions and to determine how rickettsiae survive within phagocytic cells. Flow cytometry, microscopic analysis, and LDH release demo

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Kusumawati, Heni. "KREATIVITAS DALAM PEMBUATAN ARANSEMEN MUSIK SEKOLAH." Imaji 14, no. 1 (2016): 57–64. http://dx.doi.org/10.21831/imaji.v14i1.9534.

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Kreativitas merupakan sarana untuk mengungkapkan ekspresi, imajinasi dan apresiasi dalam bermusik. Salah satu kegiatan pembelajaran seni budaya/seni musik adalah mengekspresikan diri melalui karya seni dengan pembuatan aransemen musik sekolah. Aransemen merupakan kegiatan kreatif dalam mengolah dan mengembangkan elemen-elemen musik menjadi sebuah karya baru. Adapun tahapan dalam pembuatan aransemen sederhana untuk musik sekolah diantaranya adalah: 1) Menentukan lagu yang akan di aransemen, 2) Mengolah pola ritme/harga nada/irama/durasi notasi, 3) Menentukan Akor, 4) Menulis melodi, 5) Progresi

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Weiss, Jernej. "Josip Procházka (1874–1956) kot »češko-slovenski« skladatelj samospevov." Musicological Annual 42, no. 2 (2006): 73–85. http://dx.doi.org/10.4312/mz.42.2.73-85.

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Avtor pričujočega prispevka skuša s primerjalno analizo določiti bistvene kompozicijsko-tehnične značilnosti in estetske usmeritve v enajstih samospevih Josipa Procházke, objavljenih v reviji Novi akordi, ki jih je skladatelj napisal za časa njegovega glasbeno-pedagoškega delovanja na Slovenskem. V želji po določitvi vloge in pomena omenjenih samospevov v širšem ustvarjalnem kontekstu samospeva na Slovenskem pa se avtor pričujočega prispevka kritično opredeli do razumevanja napredka v funkciji utrjevanja nacionalne samobitnosti, ki je zdi se pomembno zarisalo meje uredniški politiki v navidez

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Tóth, L. V., Y. Doi, S. Pinter, et al. "The structure of the ISM in the Zone of Avoidance by high-resolution multi-wavelength observations." Proceedings of the International Astronomical Union 12, S333 (2017): 162–65. http://dx.doi.org/10.1017/s1743921317011541.

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AbstractWe estimate the column density of the Galactic foreground interstellar medium (GFISM) in the direction of extragalactic sources. All-sky AKARI FIS infrared sky survey data might be used to trace the GFISM with a resolution of 2 arcminutes. The AKARI based GFISM hydrogen column density estimates are compared with similar quantities based on HI 21cm measurements of various resolution and of Planck results. High spatial resolution observations of the GFISM may be important recalculating the physical parameters of gamma-ray burst (GRB) host galaxies using the updated foreground parameters.

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Pepiak, A., A. Solarz, A. Pollo, T. T. Takeuchi, W. Jurusik, and AKARI Team AKARI Team. "RADIO EMISSION FROM AKARI GALAXIES." Publications of The Korean Astronomical Society 27, no. 4 (2012): 339–41. http://dx.doi.org/10.5303/pkas.2012.27.4.339.

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Nagayama, T., T. Kokusho, and H. Kaneda. "SYNERGY BETWEEN IRSF AND AKARI." Publications of The Korean Astronomical Society 27, no. 4 (2012): 381–82. http://dx.doi.org/10.5303/pkas.2012.27.4.381.

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27

Barthel, Peter. "AGN WITH AKARI AND HERSCHEL." Publications of The Korean Astronomical Society 32, no. 1 (2017): 179–83. http://dx.doi.org/10.5303/pkas.2017.32.1.179.

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Murakami, Hiroshi, Hajime Baba, Peter Barthel, et al. "The Infrared Astronomical Mission AKARI." Publications of the Astronomical Society of Japan 59, sp2 (2007): S369—S376. http://dx.doi.org/10.1093/pasj/59.sp2.s369.

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Onaka, Takashi, and Alberto Salama. "AKARI: space infrared cooled telescope." Experimental Astronomy 27, no. 1-2 (2009): 9–17. http://dx.doi.org/10.1007/s10686-009-9168-3.

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&NA;, &NA;. "Allergan Deals Paremyd to Akorn." Optometry and Vision Science 75, no. 4 (1998): 240. http://dx.doi.org/10.1097/00006324-199804000-00012.

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Bertout, C. "Special feature on AKARI results." Astronomy and Astrophysics 514 (May 2010): E1. http://dx.doi.org/10.1051/0004-6361/201014744.

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Aston, D. A. "Book Review: Akoris. Report of the Excavations at Akoris in Middle Egypt, 1981–1992." Journal of Egyptian Archaeology 83, no. 1 (1997): 238–40. http://dx.doi.org/10.1177/030751339708300122.

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33

Komugi, Shinya, Yasuo Doi, Makoto Hattori, et al. "The AKARI Far-Infrared Surveyor (FIS): all–sky Diffuse Map." Proceedings of the International Astronomical Union 6, S277 (2010): 1–4. http://dx.doi.org/10.1017/s1743921311022332.

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AbstractThe infrared astronomical satellite AKARI performed an all sky survey at six infrared bands. We report here on the calibration of the all-sky image data, observed in the four long wavelength bands with the FIS instrument (AKARI Far-infrared All Sky Survey : AFASS). The preliminary image attains a calibration uncertainty and sensitivity of better than ~ 30% and ~ 10 MJy str−1, respectively, for all four bands. The point spread function (PSF) is obtained via a stacking technique. The data are shown to be useful for exploring the internal structure and dust spectral energy distributions (

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Kaestri, Veronica Yoni. "Perancangan Aransemen Lagu Suwe Ora Jamu dan Cublak-Cublak Suweng Ditinjau Dari Perspektif Ilmu Harmoni Dasar." Resital: Jurnal Seni Pertunjukan 22, no. 1 (2021): 36–47. http://dx.doi.org/10.24821/resital.v22i1.4696.

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Aransemen musik merupakan suatu kreatifitas seorang arranger untuk mengekspresikan ide kreatifnya yang dituangkan dalam sebuah lagu, dimana tidak mengubah bentuk lagu aslinya. Sebagai arranger harus menguasai teori musik yang didalamnya terdapat ritme, melodi dan harmoni. Dalam pembuatan aransemen harus melihat siapakah yang akan memainkan aransemen, tingkat kemampuan pemain, ambitus suara, dan ciri khas nuansa lagu misalnya dalam lagu tradisional. Pembuatan aransemen ini merupakan suatu kreatifitas musisi untuk menuangkan ide-idenya. Metode yang digunakan adalah metode eksperimen dan mengacu

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Alí-Lagoa, V., T. G. Müller, F. Usui, and S. Hasegawa. "The AKARI IRC asteroid flux catalogue: updated diameters and albedos." Astronomy & Astrophysics 612 (April 2018): A85. http://dx.doi.org/10.1051/0004-6361/201731806.

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The AKARI IRC all-sky survey provided more than twenty thousand thermal infrared observations of over five thousand asteroids. Diameters and albedos were obtained by fitting an empirically calibrated version of the standard thermal model to these data. After the publication of the flux catalogue in October 2016, our aim here is to present the AKARI IRC all-sky survey data and discuss valuable scientific applications in the field of small body physical properties studies. As an example, we update the catalogue of asteroid diameters and albedos based on AKARI using the near-Earth asteroid therma

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Oi, Nagisa, Tomotsugu Goto, Hideo Matsuhara, et al. "Subaru/HSC deep optical imaging of infrared sources in the AKARI North Ecliptic Pole-Wide field." Monthly Notices of the Royal Astronomical Society 500, no. 4 (2020): 5024–42. http://dx.doi.org/10.1093/mnras/staa3080.

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ABSTRACT We present a five-broad-band (grizy) photometric catalogue of Subaru/Hyper Suprime-Cam (HSC) optical imaging observations at around the North Ecliptic Pole (NEP) where the AKARI infrared (IR) satellite conducted a large survey (NEP-Wide survey). The observations cover almost all the NEP-Wide survey field down to the depth of 28.1, 26.8, 26.3, 25.5, and 25.0 mag (5σ) at grizy, respectively. The five-band HSC catalogue contains about 2.6 million objects, and 70 959 AKARI NEP-Wide counterpart sources are identified in the catalogue. We added existing supplementary catalogues from the u b

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Tóth, L. Viktor, Sarolta Zahorecz, Gábor Marton, et al. "Pattern analysis of young stellar clusters." Proceedings of the International Astronomical Union 8, S292 (2012): 113. http://dx.doi.org/10.1017/s1743921313000732.

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Kaneda, H., T. Suzuki, T. Onaka, et al. "AKARI Far-Infrared View of Nearby Galaxies." Proceedings of the International Astronomical Union 5, H15 (2009): 414. http://dx.doi.org/10.1017/s1743921310010021.

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Kaneda, H., T. Onaka, T. Kitayama, Y. Okada, and I. Sakon. "Mid- and Far-Infrared Study of X-ray-emitting Dusty Elliptical Galaxies." Proceedings of the International Astronomical Union 2, S235 (2006): 211. http://dx.doi.org/10.1017/s174392130600617x.

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Onaka, Takashi, Tamami I. Mori, Itsuki Sakon, Fumihiko Usui, Ronin Wu, and Takashi Shimonishi. "AKARI NIR spectroscopy of interstellar ices." Proceedings of the International Astronomical Union 11, A29A (2015): 319–20. http://dx.doi.org/10.1017/s1743921316003161.

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AbstractThe Infrared Camera (IRC) onboard AKARI has a near-infrared (2--5μm) spectroscopic capability with high sensitivity that allows us to study the major ice components in various objects. In particular, H2O and CO2 ice absorption features have been detected towards nearby galaxies, including several young stellar objects (YSOs) in the Large Magellanic Cloud (LMC), as well as a number of HII region-PDR complexes for the first time by IRC spectroscopy. While observations in the LMC show a high ratio (~0.34) of the CO2 to H2O ice column densities, the ratios in Galactic HII-region-PDR comple

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Onaka, Takashi. "AKARI OBSERVATIONS OF THE INTERSTELLAR MEDIUM." Publications of The Korean Astronomical Society 27, no. 4 (2012): 187–93. http://dx.doi.org/10.5303/pkas.2012.27.4.187.

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Osman, Hassan. "An Unpublished Water Cistern at Akoris." مجلة کلیة السیاحة والفنادق - جامعة مدینة السادات 1, no. 2 (2017): 99–112. http://dx.doi.org/10.21608/mfth.2017.26097.

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Балан, П. Г. "Зоогеографічна характеристика церконід (Akari, Mesostigmata) України". Вісник Київського університету. Хіміко-біологічні науки та науки про землю, Вип. 3 (1991): 35–37.

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44

Балан, П. Г. "Зоогеографічна характеристика церконід (Akari, Mesostigmata) України". Вісник Київського університету. Хіміко-біологічні науки та науки про землю, Вип. 3 (1991): 35–37.

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Murata, K., H. Matsuhara, T. Wada, et al. "AKARI North Ecliptic Pole Deep Survey." Astronomy & Astrophysics 559 (November 2013): A132. http://dx.doi.org/10.1051/0004-6361/201321505.

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Kovács, Tímea, Denis Burgarella, Hidehiro Kaneda, et al. "PAHs and star formation in ELAIS N1 as seen by AKARI." Proceedings of the International Astronomical Union 15, S352 (2019): 241–42. http://dx.doi.org/10.1017/s1743921319009128.

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AbstractWe have examined the relationship between star formation and polycyclic aromatic hydrocarbons (PAHs) by fitting the spectral energy distributions (SED) of AKARI selected galaxies. PAHs are excited by the ultraviolet (UV) photons of young stars and can trace star formation in galaxies, but they are disassociated by the strong UV radiation in starbursts. AKARI covered the mid-infrared, where the PAHs emit their radiation, with a high density of photometric bands. These observations allow us to estimate the star formation rate and the PAH mass fraction of the dust in galaxies. In the futu

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Im, Myungshin. "QSONG: Supermassive Black Holes in Quasars at World's End." Proceedings of the International Astronomical Union 5, S267 (2009): 40–45. http://dx.doi.org/10.1017/s1743921310005545.

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AbstractWe present the initial results of the AKARI mission program QSONG (Quasar Spectroscopic Observation with NIR Grism). QSONG utilizes the unique AKARI capability of performing spectroscopic observations at 2.5–5 μm, with the aim of understanding the mass evolution of ~200 quasars at 3.4 < z < 6.5 from their rest-frame optical spectra. The program also studies the rest-frame NIR spectra of 99 well-studied quasars at low redshift (z < 0.5) and 10 red quasars. With the high-redshift QSONG observations, we detect and resolve redshifted optical lines such as Hα for the first time at

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Ita, Yoshifusa, Takashi Onaka, and Daisuke Kato. "AKARI IRC survey of the Large Magellanic Cloud: A new feature in the infrared color—magnitude diagram." Proceedings of the International Astronomical Union 4, S256 (2008): 9–13. http://dx.doi.org/10.1017/s1743921308028184.

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AbstractWe observed an area of 10 deg2 of the Large Magellanic Cloud using the Infrared Camera on board AKARI. The observations were carried out using five imaging filters (3, 7, 11, 15, and 24 μm) and a dispersion prism (2 − 5 μm, λ/Δλ ~ 20) equipped in the IRC. The 11 and 15 μm data, which are unique to AKARI IRC, allow us to construct color-magnitude diagrams that are useful to identify stars with circumstellar dust. We found a new sequence in the color-magnitude diagram, which is attributed to red giants with luminosity fainter than that of the tip of the first red giant branch. We suggest

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Kaneda, Hidehiro, Takashi Onaka, Itsuki Sakon, Hiroko Matsumoto, and Toyoaki Suzuki. "Polycyclic aromatic hydrocarbons in elliptical galaxies." Proceedings of the International Astronomical Union 4, S251 (2008): 247–48. http://dx.doi.org/10.1017/s1743921308021674.

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AbstractWe have observed 18 nearby dusty elliptical galaxies in the near- to far-infrared with Spitzer and AKARI. We have found that polycyclic aromatic hydrocarbons are present in 14 out of the 18 elliptical galaxies.

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Yang(杨光), G., M. Boquien, V. Buat, et al. "x-cigale: fitting AGN/galaxy SEDs from X-ray to infrared." Monthly Notices of the Royal Astronomical Society 491, no. 1 (2019): 740–57. http://dx.doi.org/10.1093/mnras/stz3001.

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ABSTRACT Code Investigating GALaxy Emission (cigale) is a powerful multiwavelength spectral energy distribution (SED) fitting code for extragalactic studies. However, the current version of cigale is not able to fit X-ray data, which often provide unique insights into active galactic nucleus (AGN) intrinsic power. We develop a new X-ray module for cigale, allowing it to fit SEDs from the X-ray to infrared (IR). We also improve the AGN fitting of cigale from UV-to-IR wavelengths. We implement a modern clumpy two-phase torus model, skirtor. To account for moderately extincted type 1 AGNs, we imp

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