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| WoS | SCOPUS | Document Type | Document Title | Abstract | Authors | Affiliation | ResearcherID (WoS) | AuthorsID (SCOPUS) | Author Email(s) | Journal Name | JCR Abbreviation | ISSN | eISSN | Volume | Issue | WoS Edition | WoS Category | JCR Year | IF | JCR (%) | FWCI | FWCI Update Date | WoS Citation | SCOPUS Citation | Keywords (WoS) | KeywordsPlus (WoS) | Keywords (SCOPUS) | KeywordsPlus (SCOPUS) | Language | Publication Stage | Publication Year | Publication Date | DOI | JCR Link | DOI Link | WOS Link | SCOPUS Link |
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| ○ | ○ | Article | Hα Reverberation Mapping of the Intermediate-mass Active Galactic Nucleus in NGC 4395 | We present the results of a high-cadence spectroscopic and imaging monitoring campaign of the active galactic nucleus (AGN) of NGC 4395. High signal-to-noise-ratio spectra were obtained at the Gemini-N 8 m telescope using the GMOS integral field spectrograph (IFS) on 2019 March 7 and at the Keck I 10 m telescope using the Low-Resolution Imaging Spectrometer with slit masks on 2019 March 3 and April 2. Photometric data were obtained with a number of 1 m-class telescopes during the same nights. The narrow-line region (NLR) is spatially resolved; therefore, its variable contributions to the slit spectra make the standard procedure of relative flux calibration impractical. We demonstrate that spatially resolved data from the IFS can be effectively used to correct the slit-mask spectral light curves. While we obtained no reliable lag owing to the lack of a strong variability pattern in the light curves, we constrain the broad-line time lag to be less than 3 hr, consistent with the photometric lag of similar to 80 minutes reported by Woo et al. By exploiting the high-quality spectra, we measure the second moment of the broad component of the H alpha emission line to be 586 +/- 19 km s(-1), superseding the lower value reported by Woo et al. Combining the revised line dispersion and the photometric time lag, we update the black hole mass to (1.7 +/- 0.3) x 10(4) M (circle dot). | Cho, Hojin; Woo, Jong-Hak; Treu, Tommaso; Williams, Peter R.; Armen, Stephen F.; Barth, Aaron J.; Bennert, Vardha N.; Cho, Wanjin; Filippenko, Alexei, V; Gallo, Elena; Geum, Jaehyuk; Gonzalez-Buitrago, Diego; Gultekin, Kayhan; Hodges-Kluck, Edmund; Horst, John C.; Hwang, Seong Hyeon; Kang, Wonseok; Kim, Minjin; Kim, Taewoo; Leonard, Douglas C.; Malkan, Matthew A.; Remigio, Raymond P.; Sand, David J.; Shin, Jaejin; Son, Donghoon; Sung, Hyun-il; Vivian, U. | Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea; Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA; San Diego State Univ, Dept Astron, San Diego, CA 92182 USA; Univ Calif Irvine, Dept Phys & Astron, 4129 Frederick Reines Hall, Irvine, CA 92697 USA; Calif Polytech State Univ San Luis Obispo, Phys Dept, San Luis Obispo, CA 93407 USA; Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA; Univ Calif Berkeley, Miller Inst Basic Res Sci, Berkeley, CA 94720 USA; Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA; Kyungpook Natl Univ, Major Astron & Atmospher Sci, Daegu 41566, South Korea; NASA, GSFC, Code 662, Greenbelt, MD 20771 USA; Natl Youth Space Ctr, Goheung 59567, South Korea; Chungbuk Natl Univ, Dept Astron & Space Sci, Cheongju 28644, South Korea; Univ Arizona, Dept Astron, 933 N Cherry Ave, Tucson, AZ 85719 USA; Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85719 USA; Korea Astron & Space Sci Inst, Daejeon 34055, South Korea | ; Kang, Wonseok/KQV-2130-2024; U, Vivian/J-5875-2019; Woo, Jong-Hak/A-2790-2014; Treu, Tommaso/KYP-7127-2024; Malkan, Matthew/IWM-5356-2023 | 55961062600; 7401751171; 7003853565; 57218765930; 57172805700; 36088948300; 35222917400; 57211396825; 34568722000; 7101964055; 57237852600; 55535507600; 59789702500; 18037283600; 55958121600; 57238207300; 55861763100; 56898213300; 57205660055; 7201953982; 7006872661; 57239077400; 6701331349; 55554622900; 35222498700; 24537938900; 45361575500 | woo@astro.snu.ac.kr; | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 921 | 2 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 0.77 | 2025-07-30 | 15 | 15 | CENTRAL BLACK-HOLE; BROAD-LINE REGION; SEYFERT-1 NUCLEUS; VARIABILITY; TELESCOPE; NGC-4395; GALAXIES; STARS; LAGS | English | 2021 | 2021-11 | 10.3847/1538-4357/ac1e92 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||||
| ○ | ○ | Article | KMTNet Nearby Galaxy Survey. III. Deficient Hα Flux in the Extended Disks of Spiral Galaxies | We perform a deep, wide-field imaging survey of nearby galaxies using H alpha and broadband filters to investigate the characteristics of star formation in galaxies. Motivated by the finding that star formation rates (SFRs) derived from H alpha fluxes in dwarf galaxies are systematically lower than those inferred from far-ultraviolet (FUV) fluxes, we attempt to determine whether the same trend exists in the extended disks of two star-forming galaxies. We perform spatially resolved photometry using grid-shaped apertures to measure the FUV and H alpha fluxes of star-forming regions. We also perform spectral energy distribution (SED) fittings using 11 photometric data points (FUV-to-MIR), including data from the literature, to estimate the local properties such as internal attenuation of individual star-forming clumps. Comparing SFRFUV and SFRH alpha , which are converted from the H alpha and FUV fluxes corrected for the local properties, we find that SFRH alpha /SFRFUV tend to decrease as the SFR decreases. We evaluate possible causes of this discrepancy between the two SFRs by restricting parameters in the SED fitting and conclude that deficient H alpha fluxes in the extended disks of galaxies are tightly correlated with recent starbursts. The strong and short starburst, which has been rapidly suppressed over the last 10 Myr, seems to induce a significant discrepancy between the SFRH alpha and SFRFUV. In addition, the recent bursts in the extended disks of galaxies appear to have occurred azimuth-symmetrically, implying that these were likely triggered by gas accretion or internal processes rather than external perturbation. | Byun, Woowon; Sheen, Yun-Kyeong; Seon, Kwang-Il; Ho, Luis C.; Lee, Joon Hyeop; Jeong, Hyunjin; Kim, Sang Chul; Park, Byeong-Gon; Lee, Yongseok; Cha, Sang-Mok; Ko, Jongwan; Kim, Minjin | Korea Astron & Space Sci Inst, Daejeon 34055, South Korea; Univ Sci & Technol, Daejeon 34113, South Korea; Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China; Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China; Kyung Hee Univ, Sch Space Res, Yongin 17104, Kyeonggi, South Korea; Kyungpook Natl Univ, Dept Astron & Atmospher Sci, Daegu 41566, South Korea | ; LEE, YONGSEOK/AAF-3965-2020; Kim, Minjin/AAU-9910-2020 | 57216758314; 23568407100; 6603554666; 57225302746; 57214829257; 16202920600; 26659735200; 7402834628; 36068040300; 13610036800; 18434193800; 56898213300 | mkim@knu.ac.kr; | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 918 | 2 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 0.28 | 2025-07-30 | 7 | 6 | INITIAL MASS FUNCTION; STAR-FORMATION RATES; IONIZING PHOTONS; HIGH-REDSHIFT; STELLAR POPULATION; ULTRAVIOLET DISK; FAR-ULTRAVIOLET; ESCAPE FRACTION; IMAGING SURVEY; SIMPLE-MODEL | English | 2021 | 2021-09 | 10.3847/1538-4357/ac0f00 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||||
| ○ | ○ | Article | Persistent electrical energy generation from organic diodes under constant pressure: Toward organic gravity nanogenerators | Here it is demonstrated that electricity can be continuously generated by pressing organic diodes with the poly(3-hexylthiophene) (P3HT) layers which are sandwiched between indium-tin oxide and aluminum (Al) electrodes. The optimized single devices with the 150-nm-thick P3HT layers are able to generate 60 mu V and 45 mu A by pressing, while persistent voltage (50 mu V) and current (45 mu A) generations are achieved by continuous pressing for 7 days. The charge generation by pressing of organic diodes is supported by the current density-voltage and capacitance measurements, while the friction of pi-orbital electrons in the P3HT chains upon pressing is proposed for the mechanism of persistent electricity generation. Organic diode modules with 14 sub-cells in series deliver ca. 0.4 V and ca. 20 mu W. The present technology is expected to pave the way for next-generation energy conversion devices, organic gravity nanogenerators that enable continuous electricity generation by gravitational forces. | Lee, Sooyong; Kim, Hwajeong; Kim, Youngkyoo | Kyungpook Natl Univ, Organ Nanoelect Lab, Daegu 41566, South Korea; Kyungpook Natl Univ, Sch Appl Chem Engn, KNU Inst Nanophoton Applicat KINPA, Dept Chem Engn, Daegu 41566, South Korea; Kyungpook Natl Univ, Res Inst Environm Sci & Technol, Daegu 41566, South Korea | 55421486100; 15520531700; 10340424400 | ykimm@knu.ac.kr; | ISCIENCE | ISCIENCE | 2589-0042 | 24 | 6 | SCIE | MULTIDISCIPLINARY SCIENCES | 2021 | 6.107 | 19.6 | 0 | 2025-07-30 | 0 | 0 | STORAGE | energy materials; energy resources; energy systems | English | 2021 | 2021-06-25 | 10.1016/j.isci.2021.102546 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||||
| ○ | ○ | Article | Revisiting the Color-Color Selection: Submillimeter and AGN Properties of NUV-r-J Selected Quiescent Galaxies | We examine the robustness of the color-color selection of quiescent galaxies (QGs) against contamination of dusty star-forming galaxies using the latest submillimeter data. We selected 18,304 QG candidates out to z similar to 3 using the commonly adopted NUV-r-J selection based on the high-quality multiwavelength COSMOS2015 catalog. Using extremely deep 450 and 850 mu m catalogs from the latest JCMT SCUBA-2 Large Programs, S2COSMOS and STUDIES, as well as the Atacama Large Millimeter/submillimeter Array submillimeter, VLA 3 GHz, and Spitzer MIPS 24 mu m catalogs, we identified luminous, dusty, star-forming galaxies among the QG candidates. We also conducted stacking analyses in the SCUBA-2 450 and 850 mu m images to look for less-luminous dusty galaxies among the QG candidates. By cross matching to the 24 mu m and 3 GHz data, we were able to identify a subgroup of "IR-radio-bright" QGs that possess strong 450 and 850 mu m stacking signals. The potential contamination of these luminous and less-luminous dusty galaxies accounts for approximately 10% of the color-selected QG candidates. In addition, there exists a spatial correlation between the luminous star-forming galaxies and the QGs at a less than or similar to 60 kpc scale. Finally, we found a high QG fraction among radio active galactic nuclei (AGNs) at z < 1.5. Our data show a strong correlation between QGs and radio AGNs, which may suggest a connection between the quenching process and the radio-mode AGN feedback. | Hwang, Yu-Hsuan; Wang, Wei-Hao; Chang, Yu-Yen; Lim, Chen-Fatt; Chen, Chian-Chou; Gao, Zhen-Kai; Dunlop, James S.; Gao, Yu; Ho, Luis C.; Hwang, Ho Seong; Koprowski, Maciej; Michalowski, Michal J.; Peng, Ying-jie; Shim, Hyunjin; Simpson, James M.; Toba, Yoshiki | Natl Taiwan Univ, Dept Phys, 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan; Acad Sinica, Inst Astron & Astrophys, 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan; Natl Chung Hsing Univ, Dept Phys, Taichung 40227, Taiwan; Natl Cent Univ, Grad Inst Astron, Taoyuan, Taiwan; Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland; Xiamen Univ, Dept Astron, 422 Siming South Rd, Xiamen 361005, Peoples R China; Chinese Acad Sci, Key Lab Radio Astron, Purple Mt Observ, 10 Yuanhua Rd, Nanjing 210023, Peoples R China; Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China; Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China; Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea; Seoul Natl Univ, Dept Phys & Astron, Astron Program, 1 Gwanak Ro, Seoul 08826, South Korea; Nicolaus Copernicus Univ, Inst Astron, Fac Phys Astron & Informat, Grudziadzka 5, PL-87100 Torun, Poland; Adam Mickiewicz Univ, Astron Observ Inst, Fac Phys, PL-60286 Poznan, Poland; Kyungpook Natl Univ, Dept Earth Sci Educ, Deagu 41566, South Korea; Univ Durham, Dept Phys, Ctr Extragalact Astron, Durham, England; Natl Astron Observ Japan, Osawa, Mitaka, Japan; Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto 6068502, Japan; Ehime Univ, Res Ctr Space & Cosm Evolut, 2-5 Bunkyo Cho, Matsuyama, Ehime 7908577, Japan | ; 高, 煜/AGW-4046-2022; Michałowski, Michał/AAQ-4789-2021; Koprowski, Maciej/M-7525-2019; Peng, Yingjie/B-1280-2013; HWANG, Ho/AAS-6010-2020; CHEN, Chian-Chou (TC)/ABB-2819-2020; Chang, Yu-Yen/GLR-5642-2022; Dunlop, James/ADB-7947-2022; Wang, Wei-Hao/ABD-9942-2020; Shim, Hyunjin/LZI-7486-2025 | 57222956871; 8294170500; 55505186100; 57195235890; 44561018400; 57222184106; 7202804202; 55547120397; 35229428100; 15131707100; 56038935500; 15822545300; 25937428700; 14061137700; 55430490600; 37068332400 | whwang@asiaa.sinica.edu.tw; | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 913 | 1 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 0.42 | 2025-07-30 | 8 | 7 | ACTIVE GALACTIC NUCLEI; COSMOLOGY LEGACY SURVEY; STAR-FORMATION RATE; MU-M; OPTICAL SPECTROSCOPY; PASSIVE GALAXIES; MASSIVE GALAXIES; DUSTY GALAXIES; EARLY UNIVERSE; BLACK-HOLES | English | 2021 | 2021-05 | 10.3847/1538-4357/abf11a | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||||
| ○ | ○ | Article | Revisiting the Complex Kinematics of Ionized Gas at the Central Region of NGC 1068: Evidence of an Additional Active Galactic Nucleus? | We present a spatially resolved analysis of ionized gas at the nuclear region of the nearby galaxy NGC 1068. While NGC 1068 has been known to have gas outflows driven by its active galactic nucleus (AGN), more complex kinematical signatures were recently reported, which were inconsistent with rotation or simple biconical outflows. To account for the nature of gas kinematics, we performed a spatially resolved kinematical study, finding a morphologically symmetric pair of approaching and receding gas blobs in the northeast region. The midpoint of the two blobs is located at a distance of 180 pc from the nucleus in the projected plane. The ionized gas at the midpoint shows zero velocity and high velocity dispersion, which are characteristics of an outflow-launching position, as the two sides of a bicone, i.e., approaching and receding outflows are superposed on the line of sight, leading to no velocity shift but high velocity dispersion. We investigate the potential scenario of an additional AGN based on a multiwavelength data set. While there are other possibilities, i.e., X-ray binary or supernova shock, the results from optical spectropolarimetry analysis are consistent with the presence of an additional AGN, which likely originates from a minor merger. | Shin, Jaejin; Woo, Jong-Hak; Kim, Minjin; Wang, Junfeng | Kyungpook Natl Univ, Dept Astron & Atmospher Sci, Daegu 41566, South Korea; Seoul Natl Univ, Dept Phys & Astron, Astron Program, Seoul 08826, South Korea; Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China | Kim, Minjin/AAU-9910-2020; Wang, Junmei/C-8636-2014; Woo, Jong-Hak/A-2790-2014 | 55554622900; 7401751171; 56898213300; 56521216000 | woo@astro.snu.ac.kr; | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 908 | 1 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 0.42 | 2025-07-30 | 6 | 6 | Active galactic nuclei; Spectroscopy | English | 2021 | 2021-02 | 10.3847/1538-4357/abd779 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||||
| ○ | ○ | Article | Space Telescope and Optical Reverberation Mapping Project. IX. Velocity-Delay Maps for Broad Emission Lines in NGC 5548 | In this contribution, we achieve the primary goal of the active galactic nucleus (AGN) STORM campaign by recovering velocity-delay maps for the prominent broad emission lines (Ly alpha, C IV, He II, and H beta) in the spectrum of NGC 5548. These are the most detailed velocity-delay maps ever obtained for an AGN, providing unprecedented information on the geometry, ionization structure, and kinematics of the broad-line region. Virial envelopes enclosing the emission-line responses show that the reverberating gas is bound to the black hole. A stratified ionization structure is evident. The He ii response inside 5-10 lt-day has a broad single-peaked velocity profile. The Ly alpha, C IV, and H beta responses extend from inside 2 to outside 20 lt-day, with double peaks at 2500 km s(-1) in the 10-20 lt-day delay range. An incomplete ellipse in the velocity-delay plane is evident in H beta. We interpret the maps in terms of a Keplerian disk with a well-defined outer rim at R = 20 lt-day. The far-side response is weaker than that from the near side. The line-center delay tau = (R/c)(1 - sin i) approximate to 5 days gives the inclination i approximate to 45 degrees. The inferred black hole mass is (BH) 7 x 10(7) M-circle dot. In addition to reverberations, the fit residuals confirm that emission-line fluxes are depressed during the "BLR Holiday" identified in previous work. Moreover, a helical "Barber-Pole" pattern, with stripes moving from red to blue across the C IV and Ly alpha line profiles, suggests azimuthal structure rotating with a 2 yr period that may represent precession or orbital motion of inner-disk structures casting shadows on the emission-line region farther out. | Horne, Keith; Rosa, G. De; Peterson, B. M.; Barth, A. J.; Ely, J.; Fausnaugh, M. M.; Kriss, G. A.; Pei, L.; Bentz, M. C.; Cackett, E. M.; Edelson, R.; Eracleous, M.; Goad, M. R.; Grier, C. J.; Kaastra, J.; Kochanek, C. S.; Krongold, Y.; Mathur, S.; Netzer, H.; Proga, D.; Tejos, N.; Vestergaard, M.; Villforth, C.; Adams, S. M.; Anderson, M. D.; Arevalo, P.; Beatty, T. G.; Bennert, V. N.; Bigley, A.; Bisogni, S.; Borman, G. A.; Boroson, T. A.; Bottorff, M. C.; Brandt, W. N.; Breeveld, A. A.; Brotherton, M.; Brown, J. E.; Brown, J. S.; Canalizo, G.; Carini, M. T.; Clubb, K. I.; Comerford, J. M.; Corsini, E. M.; Crenshaw, D. M.; Croft, S.; Croxall, K. V.; Bonta, E. Dalla; Deason, A. J.; Dehghanian, M.; Lorenzo-Caceres, A. De; Denney, K. D.; Dietrich, M.; Done, C.; Efimova, N. V.; Evans, P. A.; Ferland, G. J.; Filippenko, A. V.; Flatland, K.; Fox, O. D.; Gardner, E.; Gates, E. L.; Gehrels, N.; Geier, S.; Gelbord, J. M.; Gonzalez, L.; Gorjian, V.; Greene, J. E.; Grupe, D.; Gupta, A.; Hall, P. B.; Henderson, C. B.; Hicks, S.; Holmbeck, E.; Holoien, T. W. -S.; Hutchison, T.; Im, M.; Jensen, J. J.; Johnson, C. A.; Joner, M. D.; Jones, J.; Kaspi, S.; Kelly, P. L.; Kennea, J. A.; Kim, M.; Kim, S.; Kim, S. C.; King, A.; Klimanov, S. A.; Korista, K. T.; Lau, M. W.; Lee, J. C.; Leonard, D. C.; Li, Miao; Lira, P.; Lochhaas, C.; Ma, Zhiyuan; MacInnis, F.; Malkan, M. A.; Manne-Nicholas, E. R.; Mauerhan, J. C.; McGurk, R.; McHardy, I. M.; Montuori, C.; Morelli, L.; Mosquera, A.; Mudd, D.; Muller-Sanchez, F.; Nazarov, S. V.; Norris, R. P.; Nousek, J. A.; Nguyen, M. L.; Ochner, P.; Okhmat, D. N.; Pancoast, A.; Papadakis, I.; Parks, J. R.; Penny, M. T.; Pizzella, A.; Pogge, R. W.; Poleski, R.; Pott, J. -U.; Rafter, S. E.; Rix, H. -W.; Runnoe, J.; Saylor, D. A.; Schimoia, J. S.; Schnuelle, K.; Scott, B.; Sergeev, S. G.; Shappee, B. J.; Shivvers, I.; Siegel, M.; Simonian, G. V.; Siviero, A.; Skielboe, A.; Somers, G.; Spencer, M.; Starkey, D.; Stevens, D. J.; Sung, H. -I.; Tayar, J.; Treu, T.; Turner, C. S.; Uttley, P.; Van Saders, J.; Vican, L.; Villanueva, S.; Weiss, Y.; Woo, J. -H.; Yan, H.; Young, S.; Yuk, H.; Zheng, W.; Zhu, W.; Zu, Y. | Univ St Andrews, SUPA Phys & Astron, St Andrews KY16 9SS, Fife, Scotland; Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA; Ohio State Univ, Dept Astron, 140 W 18th Ave, Columbus, OH 43210 USA; Ohio State Univ, Ctr Cosmol & AstroParticle Phys, 191 West Woodruff Ave, Columbus, OH 43210 USA; Univ Calif Irvine, Dept Phys & Astron, 4129 Frederick Reines Hall, Irvine, CA 92697 USA; MIT, Kavli Inst Space & Astrophys Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA; Georgia State Univ, Dept Phys & Astron, 25 Pk Pl,Suite 605, Atlanta, GA 30303 USA; Wayne State Univ, Dept Phys & Astron, 666 W Hancock St, Detroit, MI 48201 USA; Univ Maryland, Dept Astron, College Pk, MD 20742 USA; Penn State Univ, Dept Astron & Astrophys, Eberly Coll Sci, 525 Davey Lab, University Pk, PA 16802 USA; Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA; Univ Leicester, Dept Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England; Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA; SRON Netherlands Inst Space Res, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands; Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands; Univ Nacl Autonoma Mexico, Inst Astron, Mexico City, DF, Mexico; Tel Aviv Univ, Sch Phys & Astron, Raymond & Beverly Sackler Fac Exact Sci, IL-69978 Tel Aviv, Israel; Univ Nevada, Dept Phys & Astron, 4505 South Maryland Pkwy,Box 454002, Las Vegas, NV 89154 USA; Pontificia Univ Catolica Valparaiso, Inst Fis, Casilla 4059, Valparaiso, Chile; Univ Copenhagen, Niels Bohr Inst, DARK, Jagtvej 128, DK-2200 Copenhagen N, Denmark; Univ Bath, Dept Phys, Bath BA2 7AY, Avon, England; CALTECH, Cahill Ctr Astrophys, Pasadena, CA 91125 USA; Univ Valparaiso, Inst Fis & Astron, Fac Ciencias, Gran Bretana N 1111, Valparaiso, Chile; Penn State Univ, Ctr Exoplanets & Habitable Worlds, University Pk, PA 16802 USA; Calif Polytech State Univ San Luis Obispo, Dept Phys, San Luis Obispo, CA 93407 USA; Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA; INAF IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy; Crimean Astrophys Observ, UA-298409 P O Nauchny, Crimea, Ukraine; Las Cumbres Observ Global Telescope Network, 6740 Cortona Dr,Suite 102, Goleta, CA 93117 USA; Southwestern Univ, Fountainwood Observ, Dept Phys, FJS 149,1011 E Univ Ave, Georgetown, TX 78626 USA; Penn State Univ, Dept Phys, 104 Davey Lab, University Pk, PA 16802 USA; Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England; Univ Wyoming, Dept Phys & Astron, 1000 E Univ Ave, Laramie, WY 82071 USA; Univ Missouri, Dept Phys & Astron, Columbia, MO 65211 USA; Univ Calif Santa Cruz, Dept Astron & Astrophys, 1156 High St, Santa Cruz, CA 95064 USA; Univ Calif Riverside, Dept Phys & Astron, Riverside, CA 92521 USA; Western Kentucky Univ, Dept Phys & Astron, 1906 Coll Hts Blvd 11077, Bowling Green, KY 42101 USA; Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA; Univ Padua, Dipartimento Fis & Astron G Galilei, Vicolo Osservatorio 3, I-35122 Padua, Italy; INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy; Univ Calif Santa Cruz, Dept Astron & Astrophys, 1156 High St, Santa Cruz, CA 95064 USA; Univ Durham, Inst Computat Cosmol, Dept Phys, South Rd, Durham DH1 3LE, England; Univ Kentucky, Dept Phys & Astron, Lexington, KY 40506 USA; Inst Astrofis Canarias, Calle Via Lactea S-N, E-38205 Tenerife, Spain; Worcester State Univ, Dept Earth Environm & Phys, Worcester, MA 01602 USA; Univ Durham, Dept Phys, Ctr Extragalact Astron, South Rd, Durham DH1 3LE, England; Pulkovo Observ, St Petersburg 196140, Russia; Univ Calif Berkeley, Miller Inst Basic Res Sci, Berkeley, CA 94720 USA; San Diego State Univ, Dept Astron, San Diego, CA 92182 USA; Oakwood Sch, 105 John Wilson Way, Morgan Hill, CA 95037 USA; Univ Reading, Sch Biol Sci, Reading RG6 6AS, Berks, England; Lick Observ, POB 85, Mt Hamilton, CA 95140 USA; NASA, Goddard Space Flight Ctr, Astrophys Sci Div, Mail Code 661, Greenbelt, MD 20771 USA; Inst Astrofis Canarias, E-38200 Tenerife, Spain; Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain; Gran Telescopio Canarias GRANTECAN, E-38205 Tenerife, Spain; Spectral Sci Inc, 4 Fourth Ave, Burlington, MA 01803 USA; Eureka Sci Inc, 2452 Delmer St Suite 100, Oakland, CA 94602 USA; CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA; Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA; Morehead State Univ, Ctr Space Sci, 235 Martindale Dr, Morehead, KY 40351 USA; York Univ, Dept Phys & Astron, Toronto, ON M3J 1P3, Canada; CALTECH, IPAC, Mail Code 100-22,1200 East Calif Blvd, Pasadena, CA 91125 USA; Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA; Carnegie Observ, 813 Santa Barbara St, Pasadena, CA 91101 USA; Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA; Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA; Seoul Natl Univ, Dept Phys & Astron, Astron Program, Seoul, South Korea; Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA; Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA; Brigham Young Univ, Dept Phys & Astron, N283 ESC, Provo, UT 84602 USA; Technion, Phys Dept, IL-32000 Haifa, Israel; Univ Minnesota, Sch Phys & Astron, Minnesota Inst Astrophys, 116 Church St S-E, Minneapolis, MN 55455 USA; Korea Astron & Space Sci Inst, Daejeon, South Korea; Kyungpook Natl Univ, Dept Astron & Atmospher Sci, Daegu 41566, South Korea; Univ Surrey, Dept Phys, Guildford GU2 7XH, Surrey, England; Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia; Western Michigan Univ, Dept Phys, 1120 Everett Tower, Kalamazoo, MI 49008 USA; Columbia Univ, Dept Astron, 550 W 120th St, New York, NY 10027 USA; Univ Chile, Dept Astron, Camino Observ 1515, Santiago, Chile; Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA; Univ Southampton, Southampton SO17 1BJ, Hants, England; Univ Insubria, DiSAT, Via Valleggio 11, I-22100 Como, Italy; Univ Atacama, Inst Astron & Ciencias Planetarias, Copiapo, Chile; US Naval Acad, Dept Phys, Annapolis, MD 21403 USA; Univ Memphis, Dept Phys & Mat Sci, 3720 Alumni Ave, Memphis, TN 38152 USA; Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA; Univ Crete, Dept Phys, GR-71003 Iraklion, Greece; Univ Crete, Inst Theoret & Computat Phys, GR-71003 Iraklion, Greece; Fdn Res & Technol, IESL, GR-71110 Iraklion, Greece; Louisiana State Univ, Dept Phys & Astron, Nicholson Hall,Tower Dr, Baton Rouge, LA 70803 USA; Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany; Univ Haifa, Dept Phys, Fac Nat Sci, IL-31905 Haifa, Israel; Univ Michigan, Dept Astron, 1085 S Univ Ave, Ann Arbor, MI 48109 USA; Vanderbilt Univ, Dept Phys & Astron, 6301 Stevenson Circle, Nashville, TN 37235 USA; Lab Interinst E Astron, Rua Gen Jose Cristino,77 Vasco Gama, Rio De Janeiro, RJ, Brazil; Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA; Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA; Univ Amsterdam, Astron Inst Anton Pannekoek, Postbus 94249, NL-1090 GE Amsterdam, Netherlands; Shanghai Jiao Tong Univ, 800 Dongchuan Rd, Shanghai 200240, Peoples R China | ; Grupe, Dirk/JVT-4185-2024; Zhu, Wei/JDP-0387-2023; Brandt, William/N-2844-2015; Im, Myungshin/B-3436-2013; Poleski, Radoslaw/AAM-7565-2021; Micheli, Marco/H-7598-2015; Adams, Scott/KIC-4492-2024; Treu, Tommaso/KYP-7127-2024; done, chris/D-4605-2016; Morelli, Lorenzo/AAX-2452-2021; Evans, Philip/JJC-1668-2023; Lira, Paulina/G-8536-2016; Kim, Minjin/AAU-9910-2020; Norris, Ray/JQI-5303-2023; Papadakis, Iossif/C-3235-2011; Netzer, Hagai/AAA-1835-2019; Peterson, Bradley/G-8226-2012; bonta, Elena/HZL-3516-2023; Li, Miao/AAL-6344-2021; Malkan, Matthew/IWM-5356-2023; Klimanov, Sergei/O-7827-2017; Kim, Stacy/HKF-3776-2023; Woo, Jong-Hak/A-2790-2014; Kennea, Jamie/AAF-2090-2019; Gupta, Anjali/HCH-5986-2022; Corsini, Enrico/AAE-1229-2021; Norris, Ray/A-1316-2008; Skielboe, Andreas/E-6243-2015; Lecoanet, Daniel/Y-4061-2019; Efimova, Natalia/I-2196-2013; Krongold, Yair/AAF-2844-2021; Vestergaard, Marianne/M-5247-2014; Penny, Matthew/AGE-0251-2022; Zu, Ying/ABE-1449-2022; Ma, ZhiYuan/GWN-1061-2022; Sergeyev, Sergey/LWH-7849-2024; Ferland, Gary/AFO-6311-2022; King, Andrew/AAS-4216-2021 | 55172662700; 56708167000; 16219777200; 36088948300; 55542009800; 55767439500; 7006072785; 55340311200; 7007172911; 8302847800; 57213232100; 7006250694; 10241897600; 23488608100; 7006511205; 35242747200; 6603127332; 7402610198; 36094846500; 6701789863; 24449720000; 43361722900; 24073775000; 23491705100; 57203331731; 14818934200; 25521379400; 35222917400; 57193699379; 57190802646; 55936419600; 57202954730; 7006617490; 35247682800; 6603460192; 56312481000; 57193701812; 55933048000; 6601959161; 7103191551; 24536972800; 7005041163; 7005674273; 55665128500; 14522085200; 8283329500; 57206712686; 25927011900; 57209887790; 23088009300; 15749792200; 24758008000; 35595494700; 7005798085; 57202328232; 35503330500; 34568722000; 56942413300; 57226394283; 55875326400; 35476049700; 57217578289; 13409026300; 6506351764; 59572965100; 6701360960; 7402743629; 57204299797; 55491981200; 35356071700; 41461135600; 57000000200; 57193691310; 56010513200; 57188864446; 7004267711; 56970247900; 57223328232; 6603675694; 46161347700; 7004725504; 25641134600; 10240135000; 56898213300; 57193702961; 26659735200; 56226004000; 6506581878; 57195693154; 55892840900; 44561285600; 7201953982; 57218259851; 7004380328; 57191281517; 56271785800; 57188862518; 7006872661; 35748755100; 8567321700; 35503513100; 7004698784; 35732309200; 15830351600; 35185478700; 56152100500; 14825359600; 16033756000; 57203761212; 55943988000; 8895449400; 16242110900; 54783071500; 36624101000; 22935453600; 20436555600; 36926032900; 6603938087; 35243272000; 16507612700; 7003480487; 16025343300; 35350466600; 51665761600; 56414526400; 55123116000; 37077982900; 56707598000; 7101928440; 38362184400; 44561605900; 7402331052; 55660997900; 55880601100; 55078382500; 55893172100; 56200618500; 57168772200; 55835005200; 58709627600; 55603167100; 7003853565; 56413968600; 57206439738; 36714576300; 37003120400; 36638690700; 57188862618; 7401751171; 55730037700; 56956181600; 57191892016; 7403566199; 57171299700; 37032950700 | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 907 | 2 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 2.87 | 2025-07-30 | 47 | 48 | TERM PROFILE VARIABILITY; ACTIVE GALACTIC NUCLEUS; RADIATION PRESSURE; MASS; CONTINUUM; REGIONS; DISC | English | 2021 | 2021-02 | 10.3847/1538-4357/abce60 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||||
| ○ | ○ | Article | Strong Correlation between Fe ii/Mg ii Ratio and Eddington Ratio of Type 1 Active Galactic Nuclei | The Fe ii/Mg ii line flux ratio has been used as an indicator of the Fe/Mg abundance ratio in the broad-line region (BLR) of active galactic nuclei (AGNs). On the basis of archival rest-frame UV spectra obtained via the Hubble Space Telescope and the Sloan Digital Sky Survey, we investigate the Fe ii/Mg ii ratios of type 1 AGNs at z < 2. Over wide dynamic ranges of AGN properties (i.e., black hole mass, AGN luminosity, and Eddington ratio), we confirm that the Fe ii/Mg ii ratio strongly correlates with Eddington ratio but not with black hole mass, AGN luminosity, or redshift. Our results suggest that the metallicity in the BLR are physically related to the accretion activity of AGNs, but not to the global properties of galaxies (i.e., galaxy mass and luminosity). With regard to the relation between the BLR metallicity and the accretion rate of AGNs, we discuss that metal cooling may play an important role in enhancing the gas inflow into the central region of host galaxies, resulting in the high accretion rate of AGNs. | Shin, Jaejin; Woo, Jong-Hak; Nagao, Tohru; Kim, Minjin; Bahk, Hyeonguk | Kyungpook Natl Univ, Dept Astron & Atmospher Sci, Daegu 41566, South Korea; Seoul Natl Univ, Dept Phys & Astron, Astron Program, Seoul 08826, South Korea; Ehime Univ, Res Ctr Space & Cosm Evolut, Bunkyo Cho 2-5, Matsuyama, Ehime 7908577, Japan | Kim, Minjin/AAU-9910-2020; Woo, Jong-Hak/A-2790-2014 | 55554622900; 7401751171; 7401489546; 56898213300; 57209303353 | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 917 | 2 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 0.42 | 2025-07-30 | 7 | 7 | BLACK-HOLE MASS; NEAR-INFRARED SPECTROSCOPY; EMISSION-LINE PROPERTIES; MG II; METALLICITY RELATION; CHEMICAL EVOLUTION; REDSHIFT QUASARS; STAR-FORMATION; ACCRETION RATE; IRON EMISSION | English | 2021 | 2021-08 | 10.3847/1538-4357/ac0adf | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||||
| ○ | ○ | Article | Supernova Model Discrimination with Hyper-Kamiokande | Core-collapse supernovae are among the most magnificent events in the observable universe. They produce many of the chemical elements necessary for life to exist and their remnants-neutron stars and black holes-are interesting astrophysical objects in their own right. However, despite millennia of observations and almost a century of astrophysical study, the explosion mechanism of core-collapse supernovae is not yet well understood. Hyper-Kamiokande is a next-generation neutrino detector that will be able to observe the neutrino flux from the next galactic core-collapse supernova in unprecedented detail. We focus on the first 500 ms of the neutrino burst, corresponding to the accretion phase, and use a newly-developed, high-precision supernova event generator to simulate Hyper-Kamiokande's response to five different supernova models. We show that Hyper-Kamiokande will be able to distinguish between these models with high accuracy for a supernova at a distance of up to 100 kpc. Once the next galactic supernova happens, this ability will be a powerful tool for guiding simulations toward a precise reproduction of the explosion mechanism observed in nature. | Abe, K.; Adrich, P.; Aihara, H.; Akutsu, R.; Alekseev, I; Ali, A.; Ameli, F.; Anghel, I; Anthony, L. H., V; Antonova, M.; Araya, A.; Asaoka, Y.; Ashida, Y.; Aushev, V; Ballester, F.; Bandac, I; Barbi, M.; Barker, G. J.; Barr, G.; Batkiewicz-Kwasniak, M.; Bellato, M.; Berardi, V; Bergevin, M.; Bernard, L.; Bernardini, E.; Berns, L.; Bhadra, S.; Bian, J.; Blanchet, A.; Blaszczyk, F. D. M.; Blondel, A.; Boiano, A.; Bolognesi, S.; Bonavera, L.; Booth, N.; Borjabad, S.; Boschi, T.; Bose, D.; Bozza, C.; Bravar, A.; Bravo-Berguno, D.; Bronner, C.; Brown, L.; Bubak, A.; Buchowicz, A.; Avanzini, M. Buizza; Cafagna, F. S.; Calabria, N. F.; Calvo-Mozota, J. M.; Cao, S.; Cartwright, S. L.; Carroll, A.; Catanesi, M. G.; Cebrian, S.; Chabera, M.; Chakraborty, S.; Checchia, C.; Choi, J. H.; Choubey, S.; Cicerchia, M.; Coleman, J.; Collazuol, G.; Cook, L.; Cowan, G.; Cuen-Rochin, S.; Danilov, M.; Daz Lopez, G.; De la Fuente, E.; de Perio, P.; De Rosa, G.; Dealtry, T.; Densham, C. J.; Dergacheva, A.; Deshmukh, N.; Devi, M. M.; Di Lodovico, F.; Di Meo, P.; Di Palma, I; Doyle, T. A.; Drakopoulou, E.; Drapier, O.; Dumarchez, J.; Dunne, P.; Dziewiecki, M.; Eklund, L.; El Hedri, S.; Ellis, J.; Emery, S.; Esmaili, A.; Esteve, R.; Evangelisti, A.; Feely, M.; Fedotov, S.; Feng, J.; Fernandez, P.; Fernandez-Martinez, E.; Ferrario, P.; Ferrazzi, B.; Feusels, T.; Finch, A.; Finley, C.; Fiorentini, A.; Fiorillo, G.; Fitton, M.; Frankiewicz, K.; Friend, M.; Fujii, Y.; Fukuda, Y.; Galinski, G.; Gao, J.; Garde, C.; Garfagnini, A.; Garode, S.; Gialanella, L.; Giganti, C.; Gomez-Cadenas, J. J.; Gonin, M.; Gonzalez-Nuevo, J.; Gorin, A.; Gornea, R.; Gousy-Leblanc, V; Gramegna, F.; Grassi, M.; Grella, G.; Guigue, M.; Gumplinger, P.; Hadley, D. R.; Harada, M.; Hartfiel, B.; Hartz, M.; Hassani, S.; Hastings, N. C.; Hayato, Y.; Hernando-Morata, J. A.; Herrero, V; Hill, J.; Hiraide, K.; Hirota, S.; Holin, A.; Horiuchi, S.; Hoshina, K.; Hultqvist, K.; Iacob, F.; Ichikawa, A. K.; Ibnsalih, W. Idrissi; Iijima, T.; Ikeda, M.; Inomoto, M.; Inoue, K.; Insler, J.; Ioannisian, A.; Ishida, T.; Ishidoshiro, K.; Ishino, H.; Ishitsuka, M.; Ito, H.; Ito, S.; Itow, Y.; Iwamoto, K.; Izmaylov, A.; Izumi, N.; Izumiyama, S.; Jakkapu, M.; Jamieson, B.; Jang, H., I; Jang, J. S.; Jenkins, S. J.; Jeon, S. H.; Jiang, M.; Jo, H. S.; Jonsson, P.; Joo, K. K.; Kajita, T.; Kakuno, H.; Kameda, J.; Kano, Y.; Kalaczynski, P.; Karlen, D.; Kasperek, J.; Kataoka, Y.; Kato, A.; Katori, T.; Kazarian, N.; Kearns, E.; Khabibullin, M.; Khotjantsev, A.; Kikawa, T.; Kikec, M.; Kim, J. H.; Kim, J. Y.; Kim, S. B.; Kim, S. Y.; King, S.; Kinoshita, T.; Kisiel, J.; Klekotko, A.; Kobayashi, T.; Koch, L.; Koga, M.; Koerich, L.; Kolev, N.; Konaka, A.; Kormos, L. L.; Koshio, Y.; Korzenev, A.; Kotsar, Y.; Kouzakov, K. A.; Kowalik, K. L.; Kravchuk, L.; Kryukov, A. P.; Kudenko, Y.; Kumita, T.; Kurjata, R.; Kutter, T.; Kuze, M.; Kwak, K.; La Commara, M.; Labarga, L.; Lagoda, J.; James, M. Lamers; Lamoureux, M.; Laveder, M.; Lavitola, L.; Lawe, M.; Learned, J. G.; Lee, J.; Leitner, R.; Lezaun, V; Lim, I. T.; Lindner, T.; Litchfield, R. P.; Long, K. R.; Longhin, A.; Loverre, P.; Lu, X.; Ludovici, L.; Maekawa, Y.; Magaletti, L.; Magar, K.; Mahn, K.; Makida, Y.; Malek, M.; Malinsky, M.; Marchi, T.; Maret, L.; Mariani, C.; Marinelli, A.; Martens, K.; Marti, Ll; Martin, J. F.; Martin, D.; Marzec, J.; Matsubara, T.; Matsumoto, R.; Matsuno, S.; Matusiak, M.; Mazzucato, E.; McCarthy, M.; McCauley, N.; McElwee, J.; McGrew, C.; Mefodiev, A.; Medhi, A.; Mehta, P.; Mellet, L.; Menjo, H.; Mermod, P.; Metelko, C.; Mezzetto, M.; Migenda, J.; Migliozzi, P.; Mijakowski, P.; Miki, S.; Miller, E. W.; Minakata, H.; Minamino, A.; Mine, S.; Mineev, O.; Mitra, A.; Miura, M.; Moharana, R.; Mollo, C. M.; Mondal, T.; Mongelli, M.; Monrabal, F.; Moon, D. H.; Moon, C. S.; Mora, F. J.; Moriyama, S.; Mueller, Th A.; Munteanu, L.; Murase, K.; Nagao, Y.; Nakadaira, T.; Nakagiri, K.; Nakahata, M.; Nakai, S.; Nakajima, Y.; Nakamura, K.; Nakamura, Ki; Nakamura, H.; Nakano, Y.; Nakaya, T.; Nakayama, S.; Nakayoshi, K.; Machado, L. Nascimento; Naseby, C. E. R.; Navarro-Garcia, B.; Needham, M.; Nicholls, T.; Niewczas, K.; Nishimura, Y.; Noah, E.; Nova, F.; Nugent, J. C.; Nunokawa, H.; Obrebski, W.; Ochoa-Ricoux, J. P.; O'Connor, E.; Ogawa, N.; Ogitsu, T.; Ohta, K.; Okamoto, K.; O'Keeffe, H. M.; Okumura, K.; Onishchuk, Y.; Orozco-Luna, F.; Oshlianskyi, A.; Ospina, N.; Ostrowski, M.; O'Sullivan, E.; O'Sullivan, L.; Ovsiannikova, T.; Oyama, Y.; Ozaki, H.; Pac, M. Y.; Paganini, P.; Palladino, V; Paolone, V; Pari, M.; Parsa, S.; Pasternak, J.; Pastore, C.; Pastuszak, G.; Patel, D. A.; Pavin, M.; Payne, D.; Pena-Garay, C.; Pidcott, C.; Guerra, E. Pinzon; Playfer, S.; Pointon, B. W.; Popov, A.; Popov, B.; Porwit, K.; Posiadala-Zezula, M.; Poutissou, J-M; Pozimski, J.; Pronost, G.; Prouse, N. W.; Przewlocki, P.; Quilain, B.; Quiroga, A. A.; Radicioni, E.; Radics, B.; Rajda, P. J.; Renner, J.; Rescigno, M.; Retiere, F.; Ricciardi, G.; Riccio, C.; Richards, B.; Rondio, E.; Rose, H. J.; Roskovec, B.; Roth, S.; Rott, C.; Rountree, S. D.; Rubbia, A.; Ruggeri, A. C.; Ruggles, C.; Russo, S.; Rychter, A.; Ryu, D.; Sakashita, K.; Samani, S.; Sanchez, F.; Sanchez, M. L.; Sanchez, M. C.; Sano, S.; Santos, J. D.; Santucci, G.; Sarmah, P.; Sashima, I; Sato, K.; Scott, M.; Seiya, Y.; Sekiguchi, T.; Sekiya, H.; Seo, J. W.; Seo, S. H.; Sgalaberna, D.; Shaikhiev, A.; Shan, Z.; Shaykina, A.; Shimizu, I; Shin, C. D.; Shinoki, M.; Shiozawa, M.; Sinnis, G.; Skrobova, N.; Skwarczynski, K.; Smy, M. B.; Sobczyk, J.; Sobel, H. W.; Soler, F. J. P.; Sonoda, Y.; Spina, R.; Spisso, B.; Spradlin, P.; Stankevich, K. L.; Stawarz, L.; Stellacci, S. M.; Stopa, K.; Studenikin, A., I; Suarez Gomez, S. L.; Suganuma, T.; Suvorov, S.; Suwa, Y.; Suzuki, A. T.; Suzuki, S. Y.; Suzuki, Y.; Svirida, D.; Svoboda, R.; Taani, M.; Tada, M.; Takeda, A.; Takemoto, Y.; Takenaka, A.; Taketa, A.; Takeuchi, Y.; Takhistov, V; Tanaka, H.; Tanaka, H. A.; Tanaka, H., I; Tanaka, M.; Tashiro, T.; Thiesse, M.; Thompson, L. F.; Toledo, J.; Tomatani-Sanchez, A. K.; Tortone, G.; Tsui, K. M.; Tsukamoto, T.; Tzanov, M.; Uchida, Y.; Vagins, M. R.; Valder, S.; Valentino, V.; Vasseur, G.; Vijayvargi, A.; Vilela, C.; Vinning, W. G. S.; Vivolo, D.; Vladisavljevic, T.; Vogelaar, R. B.; Vyalkov, M. M.; Wachala, T.; Walker, J.; Wark, D.; Wascko, M. O.; Wendell, R. A.; Wilkes, R. J.; Wilking, M. J.; Wilson, J. R.; Wronka, S.; Xia, J.; Xie, Z.; Xin, T.; Yamaguchi, Y.; Yamamoto, K.; Yanagisawa, C.; Yano, T.; Yen, S.; Yershov, N.; Yeum, D. N.; Yokoyama, M.; Yonenaga, M.; Yoo, J.; Yu, I; Yu, M.; Zakrzewski, T.; Zaldivar, B.; Zalipska, J.; Zaremba, K.; Zarnecki, G.; Ziembicki, M.; Zietara, K.; Zito, M.; Zsoldos, S. | Univ Tokyo, Inst Cosm Ray Res, Kamioka Observ, Kamioka, Akita, Japan; Univ Tokyo, Univ Tokyo Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba, Japan; Univ Tokyo, Next Generat Neutrino Sci Org, Kamioka, Akita, Japan; Natl Ctr Nucl Res, Warsaw, Poland; Univ Tokyo, Dept Phys, Tokyo, Japan; TRIUMF, Vancouver, BC, Canada; Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia; Kyoto Univ, Dept Phys, Kyoto, Japan; Univ Sapienza, Dipartimento Fis, Sez Roma, Ist Nazl Fis Nucl, Rome, Italy; Iowa State Univ, Dept Phys & Astron, Ames, IA USA; Imperial Coll London, Dept Phys, London, England; Russian Acad Sci, Inst Nucl Res, Moscow, Russia; Univ Tokyo, Earthquake Res Inst, Tokyo, Japan; Kyiv Natl Univ, Dept Nucl Phys, Kiev, Ukraine; Univ Politecn Valencia, Inst Instrumentac Imagen Mol I3M, Valencia, Spain; Lab Subterraneo Canfranc, Canfranc Estn, Spain; Univ Regina, Dept Phys, Regina, SK, Canada; Univ Warwick, Dept Phys, Coventry, W Midlands, England; Univ Oxford, Dept Phys, Oxford, England; H Niewodniczanski Inst Nucl Phys PAN, Krakow, Poland; Ist Nazl Fis Nucl, Sez Padova, Padua, Italy; Univ & Politecn Bari, Bari, Italy; Univ Calif Davis, Dept Phys, Davis, CA 95616 USA; Ecole Polytech, Lab Leprince Ringuet, IN2P3 CNRS, Palaiseau, France; Tokyo Inst Technol, Dept Phys, Tokyo, Japan; York Univ, Dept Phys & Astron, Toronto, ON, Canada; Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA; Sorbonne Univ, Lab Phys Nucl & Hautes Energie, IN2P3 CNRS, Paris, France; Boston Univ, Dept Phys, 590 Commonwealth Ave, Boston, MA 02215 USA; Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy; Univ Paris Saclay, CEA, IRFU, Gif Sur Yvette, France; Univ Oviedo, Appl Math Modeling Grp, Dept Phys, Oviedo, Spain; Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada; Kings Coll London, Dept Phys, Strand Bldg, London, England; SN Bose Natl Ctr Basic Sci, Kolkata, India; Univ Salerno, Fisciano, Italy; Ist Nazl Fis Nucl, Grp Collegato Salerno, Fisciano, Italy; Univ Geneva, Sect Phys, DPNC, Geneva, Switzerland; Univ Autonoma Madrid, Dept Theoret Phys, Madrid, Spain; Univ Silesia Katowice, A Chelkowski Inst Phys, Katowice, Poland; Warsaw Univ Technol, Inst Radioelect & Multimedia Technol, Warsaw, Poland; Univ Federico II Napoli, Dipartimento Fis, Naples, Italy; High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki, Japan; J PARC Ctr, Tokai, Ibaraki, Japan; Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England; Univ Liverpool, Dept Phys, Liverpool, Merseyside, England; Univ Zaragoza, Ctr Astroparticulas & Fis Altas Energias CAPA, Zaragoza, Spain; Indian Inst Technol Guwahati, Gauhati, India; Dongshin Univ, Lab High Energy Phys, Naju, South Korea; KTH Royal Inst Technol, Dept Phys, Stockholm, Sweden; Ist Nazl Fis Nucl, Lab Nazl Legnaro, Legnaro, PD, Italy; Univ Edinburgh, Sch Phys & Astron, Edinburgh, Midlothian, Scotland; Univ Autonoma Sinaloa, Culiacan, Sinaloa, Mexico; Univ Santiago de Compostela, Inst Gallego Fis Altas Energias, Campus Sur, Santiago De Compostela, Spain; Univ Guadalajara, Dept Fis, CUCEI, Guadalajara, Jalisco, Mexico; Univ Guadalajara, IT PhD Program, CUCEA, Guadalajara, Jalisco, Mexico; Univ Lancaster, Phys Dept, Lancaster, England; Harwell Oxford, Rutherford Appleton Lab, STFC, Warrington, Cheshire, England; Daresbury Lab, Warrington, Cheshire, England; Vishwakarma Inst Informat Technol, Pune, Maharashtra, India; Tezpur Univ, Dept Phys, Sonitpur, India; Univ Glasgow, Sch Phys & Astron, Glasgow, Lanark, Scotland; Pontificia Univ Catolica Rio de Janeiro, Dept Fis, Rio De Janeiro, Brazil; Donostia Int Phys Ctr, Basque Country, Spain; Ikerbasque Fdn, Basque Country, Spain; Univ British Columbia, Dept Phys & Astron, Vancouver, BC, Canada; Stockholm Univ, Oskar Klein Ctr, Stockholm, Sweden; Stockholm Univ, Dept Phys, Stockholm, Sweden; Miyagi Univ Educ, Dept Phys, Sendai, Miyagi, Japan; Univ Campania L Vanvitelli, Naples, Italy; Carleton Univ, Dept Phys, Ottawa, ON, Canada; Okayama Univ, Dept Phys, Okayama, Japan; Calif State Univ Carson, Dept Phys, Carson, CA USA; Virginia Tech, Ctr Neutrino Phys, Blacksburg, VA USA; Nagoya Univ, Grad Sch Sci, Nagoya, Aichi, Japan; Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi, Japan; Tokyo Univ Sci, Dept Phys, Chiba, Japan; Tohoku Univ, Res Ctr Neutrino Sci, Sendai, Miyagi, Japan; Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA; Inst Theoret Phys & Modeling, Yerevan, Armenia; Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi, Japan; SOKENDAI Grad Univ Adv Studies, Tokai, Ibaraki, Japan; Univ Winnipeg, Dept Phys, Winnipeg, MB, Canada; Seoyeong Univ, Dept Fire Safety, Gwangju, South Korea; Gwangju Inst Sci & Technol, GIST Coll, Gwangju, South Korea; Sungkyunkwan Univ, Dept Phys, Suwon, South Korea; Kyungpook Natl Univ, Dept Phys, Daegu, South Korea; Chonnam Natl Univ, Dept Phys, Gwangju, South Korea; Univ Tokyo, Res Ctr Cosm Neutrinos, Inst Cosm Ray Res, Kashiwa, Chiba, Japan; Tokyo Metropolitan Univ, Dept Phys, Tokyo, Japan; AGH Univ Sci & Technol, Fac Comp Sci Elect & Telecommun, Krakow, Poland; Seoul Natl Univ, Dept Phys & Astron, Seoul, South Korea; Kobe Univ, Dept Phys, Kobe, Hyogo, Japan; Moscow State Univ, Dept Theoret Phys, Moscow, Russia; Ulsan Natl Inst Sci & Technol, Dept Phys, Ulsan, South Korea; Univ Hawaii, Dept Phys & Astron, Honolulu, HI USA; Charles Univ Prague, FMF, IPNP, Prague, Czech Republic; Keio Univ, Dept Phys, Yokohama, Kanagawa, Japan; Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA; Univ Toronto, Dept Phys, Toronto, ON, Canada; SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA; UAM CSIC, Inst Fis Teor, Madrid, Spain; Yokohama Natl Univ, Fac Engn, Yokohama, Kanagawa, Japan; Indian Inst Technol Jodhpur, Dept Phys, Karwar, Rajasthan, India; Penn State Univ, Dept Phys, 104 Davey Lab, University Pk, PA 16802 USA; Wroclaw Univ, Fac Phys & Astron, Wroclaw, Poland; Stockholm Univ, Dept Astron, Stockholm, Sweden; Jagiellonian Univ, Astron Observ, Krakow, Poland; Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden; Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA; British Columbia Inst Technol, Phys Dept, Burnaby, BC, Canada; Univ Warsaw, Fac Phys, Warsaw, Poland; Swiss Fed Inst Technol, Inst Particle & Astroparticle Phys, Zurich, Switzerland; Rhein Westfal TH Aachen, Phys Inst 3, Aachen, Germany; Osaka City Univ, Dept Phys, Osaka, Japan; Los Alamos Natl Lab, Los Alamos, NM USA; Kyoto Sangyo Univ, Dept Astrophys & Atmospher Sci, Kyoto, Japan; Univ Tokyo, Tokyo, Japan; Tecnol Monterrey, Escuela Ingn & Ciencias, Zapopan, Jalisco, Mexico; Univ Washington, Dept Phys, Seattle, WA 98195 USA; Korea Inst Sci & Technol, Dept Phys, Daejeon, South Korea; Indian Inst Technol Kharagpur, Dept Phys, Kharagpur, W Bengal, India | Roth, Stefan/J-2757-2016; Kryukov, Alexander/G-8076-2012; Adrich, Przemyslaw/Z-2202-2019; Lindner, Thomas/AAG-4863-2021; Mefodiev, Aleksandr/AAC-3716-2021; 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Kim, Ji.hwan/AAN-9424-2021; Zsoldos, Stephane/KDP-1422-2024; Kouzakov, Konstantin/P-5545-2019; Toledo, Jose/E-2571-2018; Fernandez-Martinez, Enrique/Q-5780-2019; Alekseev, Igor/J-8070-2014; Sobel, Henry/A-4369-2011; Bandac, Iulian/ABG-6750-2020; Aushev, Volodymyr/AAS-8421-2020; Popov, Artem/JQT-3392-2023; Cafagna, Francesco/A-9299-2010; Seo, Seon/K-9250-2014; Radics, Balint/AAN-2721-2020; Calabria, Nicola Fulvio/HWQ-4671-2023; Ricciardi, Giulia/H-3649-2011; Kisiel, Jan/G-9321-2012; Cuen-Rochin, Saul/AGH-5071-2022; Wilkes, R.Jeffrey/E-6011-2013; Sobczyk, Jan/C-9761-2016; Batkiewicz-Kwasniak, Marcela/M-8644-2018; Mineev, Oleg/AAG-9458-2021; Bozza, Cristiano/JXM-4910-2024; Cao, Son/LUW-8022-2024; Vivolo, Daniele/AAC-5805-2020; Aihara, Hiroaki/F-3854-2010; Gorin, Aleksandr/AAC-3143-2021; Svirida, Dmitry/R-4909-2016; de la Fuente, Eduardo/B-5170-2018; Iijima, Toru/LNR-4469-2024; Ballester Merelo, Francisco/Y-9526-2018; Nunokawa, Hiroshi/AAX-9444-2021; de la Fuente Acosta, Eduardo/B-5170-2018; Roskovec, Bedřich/AAJ-4016-2021; Khabibullin, Marat/O-1076-2013; Monrabal, Francesc/R-5374-2018; Koerich, Leonardo/J-7004-2014; IZUMI, Nobuhiko/J-8487-2016; Berardi, Vincenzo/AAA-3087-2020; Hiraide, Katsuki/A-4479-2011; Zaldivar, Bryan/AAI-1332-2019; Marzec, Janusz/H-1129-2019; Fiorillo, Giuliana/A-2248-2012; Collazuol, Gianmaria/C-5670-2012; Fernandez, Pablo/AAA-8737-2020; Tetsuro, Kumita/R-7771-2017; Kalaczyński, Piotr/P-8189-2019; Sgalaberna, Davide/AEU-4781-2022; Danilov, Mikhail/C-5380-2014; Suzuki, Alfredo/B-7322-2014; Bernardini, Elisa/AAA-4810-2020; Pereira Ferrazzi, Bruno/D-8613-2016; Migliozzi, Pasquale/I-6427-2015; Stankevich, Konstantin/AAL-8525-2020; Shaikhiev, Artur/N-7594-2016; Stellacci, Simona/AAM-6601-2021; Toledo Alarcon, Jose Francisco/E-2571-2018; Kuze, Masahiro/V-4251-2018; Dergacheva, Anna/AAG-9701-2021; Matusiak, Michal/AAB-4598-2019; Fernandez-Martinez, Enrique/L-2919-2013; Gonzalez-Nuevo, Joaquin/I-3562-2014; Leitner, Rupert/C-2004-2017; James, Megan/IWE-1268-2023; Malinsky, Milan/J-4087-2019; Yano, Takatomi/KDN-3830-2024; Kravchuk, Leonid/L-4317-2017; Bubak, Arkadiusz/F-5902-2013; Katori, Teppei/S-8685-2019; Vilela, Cristovao/AAK-7654-2021; Patel, Divya/JTS-9886-2023; Quiroga, Alexander/MSY-4005-2025; Pena Garay, Carlos/H-5769-2018; Sanchez, Maria Luisa/N-7389-2013 | 35316842700; 13609522800; 26431253400; 57191279607; 7004810214; 57191253786; 7004440709; 58378793600; 57195331264; 57188829285; 7006379524; 7005503172; 57224769890; 6602773267; 59569332600; 6508172339; 7006694639; 7202030397; 7102234805; 57208582625; 6603078804; 7006563072; 9840261300; 57203392800; 57188547921; 57203321898; 10040410200; 55436856500; 57203395818; 37074161900; 7004379668; 6603201393; 24478500100; 15843147700; 57198148175; 16302935100; 57211819211; 26642396600; 7201526906; 55891479200; 7004096230; 57211850375; 35620085700; 57222066439; 6602784103; 6508217550; 26423574600; 7004393799; 57207571126; 57221140472; 53983767600; 35314572000; 57215562596; 56568520400; 7004492021; 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7005259274; 56419646100; 57213957623; 8364191700; 35227915400; 54791523400; 35227856600; 35227850400; 57218345630; 7004178005; 57200802877; 57216488079; 59851216500; 55446744500; 34572754800; 35227869500; 57217506867; 35315071900; 35461760500; 57198647173; 57221140913; 35461328700; 57191479169; 57221146456; 57222063114; 56050521600; 24077601800; 35227970200; 55499774700; 8719197000; 57209319687; 7202469827; 57212670640; 16646930100; 57222071586; 57208573431; 7202212489; 56191820400; 57219787001; 24071933100; 8630676300; 57192182484; 57219794859; 6602714744; 7003749196; 57194426867; 55217173800; 57191488233; 56227897900; 57192837686; 35227961100; 57203396608; 35243922200; 55453339300; 57222070803; 6603029548; 57194109845; 57221150748; 57188827382; 15823196300; 57201839222; 57214923578; 55546264300; 6602114983; 7004257392; 57194320179; 57205642820; 35228176800; 56967652300; 57199194235; 56042471600; 59317777600; 56166444000; 55508216000; 57191272690; 57714569800; 57225875741; 57221141307; 57193893003; 35315137400; 56229202900; 57221148620; 6503884494; 56963525800; 57216231240; 6506254435; 57189229483; 6701650464; 57213620331; 7003776359; 35353976400; 57221142645; 56044081600; 57198865806; 55514765000; 57193904072; 6603098471; 57221140763; 15123454000; 57214383982; 7004772244; 6603085091; 35228290900; 57205875475; 6507380356; 57198231124; 8977997200; 57295741200; 57222079561; 56865663000; 55865009800; 59843779100; 14624679600; 55968950500; 7402687244; 8387485300; 57201617583; 55743752400; 57193333004; 59067101600; 35228244700; 56156643200; 57221151144; 51462236400; 55936708500; 6603387833; 57204472898; 16680503100; 54416814100; 35228232200; 57159999800 | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 916 | 1 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 3.51 | 2025-07-30 | 57 | 60 | CORE-COLLAPSE SUPERNOVAE; EQUATION-OF-STATE; NEUTRINO BURST; RADIATION HYDRODYNAMICS; MAGELLANIC-CLOUD; OSCILLATIONS; EVOLUTION; SIMULATIONS; EXPLOSION; MATTER | English | 2021 | 2021-07 | 10.3847/1538-4357/abf7c4 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||||
| ○ | ○ | Article | The Diverse Morphology, Stellar Population, and Black Hole Scaling Relations of the Host Galaxies of Nearby Quasars | We present rest-frame B and I imaging of 35 low-redshift (z < 0.5) Palomar-Green quasars using the Hubble Space Telescope Wide Field Camera 3. We perform multicomponent two-dimensional image decomposition to separate the host galaxy from its bright active nucleus, characterize its morphology, and measure its photometric properties. Special care is devoted to quantifying the structural parameters of the galaxy bulge, determining its B.-.I color, and estimating its stellar mass. Roughly half of the sample, comprising the less luminous (L-5100 less than or similar to 10(45) erg s(-1)) but most high Eddington ratio quasars, reside in disk galaxies that are often barred and possess pseudo bulges. The large stellar masses, large effective radii, and faint surface brightnesses suggest that the host galaxies of the most luminous quasars are mostly ellipticals. Major mergers constitute only a small percentage (less than or similar to 20%) of our sample. Our quasar sample roughly obeys the scaling relations between black hole mass and host galaxy (bulge, core, total) stellar mass. Hosts with black holes more massive than similar to 10(8) M-circle dot. behave similarly to classical bulges and early-type galaxies, while those with less massive black holes, particularly the narrow-line Seyfert 1s, are consistent with pseudo bulges in late-type galaxies. The host galaxy bulges, irrespective of whether they are classical or pseudo, follow a relatively tight inverse relation between the effective radius and the mean effective surface brightness of inactive classical bulges and ellipticals. We argue that pseudo bulges experience recent or ongoing nuclear star formation. | Zhao, Yulin; Ho, Luis C.; Shangguan, Jinyi; Kim, Minjin; Zhao, Dongyao; Gao, Hua | Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China; Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China; Max Planck Inst Extraterr Phys MPE, Giessenbachstr, D-85748 Garching, Germany; Kyungpook Natl Univ, Dept Astron & Atmospher Sci, Daegu 702701, South Korea; Korea Astron & Space Sci Inst, Daejeon 305348, South Korea; Beijing Acad Sci & Technol, Beijing Planetarium, Beijing 100044, Peoples R China; Univ Tokyo, Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan | ; Kim, Minjin/AAU-9910-2020; Gao, Hua/AAE-1094-2021 | 57209312530; 35229428100; 57189698112; 56898213300; 57193530070; 57754348800 | shangguan@mpe.mpg.de; | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 911 | 2 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 2.03 | 2025-07-30 | 33 | 31 | ACTIVE GALACTIC NUCLEI; REVERBERATION MAPPING PROJECT; MOLECULAR GAS CONTENT; BULGE MASS RELATION; STAR-FORMATION; ENERGY-DISTRIBUTIONS; LUMINOSITY FUNCTION; ELLIPTIC GALAXIES; BAND LUMINOSITIES; CLASSICAL BULGES | English | 2021 | 2021-04 | 10.3847/1538-4357/abe8d4 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||||
| ○ | ○ | Article | The JCMT BISTRO Survey: An 850/450 μm Polarization Study of NGC 2071IR in Orion B | We present the results of simultaneous 450 mu m and 850 mu m polarization observations toward the massive star-forming region NGC 2071IR, a target of the BISTRO (B-fields in STar-forming Region Observations) Survey, using the POL-2 polarimeter and SCUBA-2 camera mounted on the James Clerk Maxwell Telescope. We find a pinched magnetic field morphology in the central dense core region, which could be due to a rotating toroidal disklike structure and a bipolar outflow originating from the central young stellar object IRS 3. Using the modified Davis-Chandrasekhar-Fermi method, we obtain a plane-of-sky magnetic field strength of 563 +/- 421 mu G in the central similar to 0.12 pc region from 850 mu m polarization data. The corresponding magnetic energy density of 2.04 x 10(-8) erg cm(-3) is comparable to the turbulent and gravitational energy densities in the region. We find that the magnetic field direction is very well aligned with the whole of the IRS 3 bipolar outflow structure. We find that the median value of polarization fractions is 3.0% at 450 mu m in the central 3 ' region, which is larger than the median value of 1.2% at 850 mu m. The trend could be due to the better alignment of warmer dust in the strong radiation environment. We also find that polarization fractions decrease with intensity at both wavelengths, with slopes, determined by fitting a Rician noise model of 0.59 +/- 0.03 at 450 mu m and 0.36 +/- 0.04 at 850 mu m, respectively. We think that the shallow slope at 850 mu m is due to grain alignment at the center being assisted by strong radiation from the central young stellar objects. | Lyo, A-Ran; Kim, Jongsoo; Sadavoy, Sarah; Johnstone, Doug; Berry, David; Pattle, Kate; Kwon, Woojin; Bastien, Pierre; Onaka, Takashi; Di Francesco, James; Kang, Ji-Hyun; Furuya, Ray; Hull, Charles L. H.; Tamura, Motohide; Koch, Patrick M.; Ward-Thompson, Derek; Hasegawa, Tetsuo; Hoang, Thiem; Arzoumanian, Doris; Lee, Chang Won; Lee, Chin-Fei; Byun, Do-Young; Kirchschlager, Florian; Doi, Yasuo; Kim, Kee-Tae; Hwang, Jihye; Pham Ngoc Diep; Fanciullo, Lapo; Lee, Sang-Sung; Park, Geumsook; Yoo, Hyunju; Chung, Eun Jung; Whitworth, Anthony; Mairs, Steve; Soam, Archana; Liu, Tie; Tang, Xindi; Coude, Simon; Andre, Philippe; Bourke, Tyler L.; Chen, Huei-Ru Vivien; Chen, Zhiwei; Chen, Wen Ping; Chen, Mike; Ching, Tao-Chung; Cho, Jungyeon; Choi, Minho; Choi, Yunhee; Chrysostomou, Antonio; Dai, Sophia; Dowell, C. Darren; Duan, Hao-Yuan; Duan, Yan; Eden, David; Eswaraiah, Chakali; Eyres, Stewart; Fiege, Jason; Fissel, Laura M.; Franzmann, Erica; Friberg, Per; Friesen, Rachel; Fuller, Gary; Gledhill, Tim; Graves, Sarah; Greaves, Jane; Griffin, Matt; Gu, Qilao; Han, Ilseung; Hatchell, Jannifer; Hayashi, Saeko; Houde, Martin; Inoue, Tsuyoshi; Inutsuka, Shu-ichiro; Iwasaki, Kazunari; Jeong, Il-Gyo; Kang, Miju; Kataoka, Akimasa; Kawabata, Koji; Kemper, Francisca; Kim, Gwanjeong; Kim, Mi-Ryang; Kim, Shinyoung; Kim, Kyoung Hee; Kirk, Jason; Kobayashi, Masato I. N.; Konyves, Vera; Kusune, Takayoshi; Kwon, Jungmi; Lacaille, Kevin; Lai, Shih-Ping; Law, Chi-Yan; Lee, Jeong-Eun; Lee, Yong-Hee; Lee, Hyeseung; Li, Dalei; Li, Di; Li, Hua-Bai; Liu, Hong-Li; Liu, Junhao; Liu, Sheng-Yuan; Lu, Xing; Matsumura, Masafumi; Matthews, Brenda; Moriarty-Schieven, Gerald; Nagata, Tetsuya; Nakamura, Fumitaka; Nakanishi, Hiroyuki; Ngoc, Nguyen Bich; Ohashi, Nagayoshi; Parsons, Harriet; Peretto, Nicolas; Priestley, Felix; Pyo, Tae-soo; Qian, Lei; Qiu, Keping; Rao, Ramprasad; Rawlings, Jonathan; Rawlings, Mark G.; Retter, Brendan; Richer, John; Rigby, Andrew; Saito, Hiro; Savini, Giorgio; Scaife, Anna; Seta, Masumichi; Shimajiri, Yoshito; Shinnaga, Hiroko; Tahani, Mehrnoosh; Tang, Ya-Wen; Tomisaka, Kohji; Le Ngoc Tram; Tsukamoto, Yusuke; Viti, Serena; Wang, Jia-Wei; Wang, Hongchi; Xie, Jinjin; Yen, Hsi-Wei; Yuan, Jinghua; Yun, Hyeong-Sik; Zenko, Tetsuya; Zhang, Guoyin; Zhang, Chuan-Peng; Zhang, Yapeng; Zhou, Jianjun; Zhu, Lei; de Looze, Ilse; Dowell, C. Darren; Falle, Sam; Robitaille, Jean-Francois; van Loo, Sven | Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea; Univ Sci & Technol Korea, 217 Gajeong Ro, Daejeon 34113, South Korea; Queens Univ, Dept Phys Engn Phys & Astrophys, Kingston, ON K7L 3N6, Canada; NRC Herzberg Astron & Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada; Univ Victoria, Dept Phys & Astron, Victoria, BC V8W 2Y2, Canada; East Asian Observ, 660 N Aohoku Pl, Hilo, HI 96720 USA; Natl Univ Ireland Galway, Ctr Astron, Sch Phys, Univ Rd, Galway, Ireland; Seoul Natl Univ, Dept Earth Sci Educ, 1 Gwanak Ro, Seoul 08826, South Korea; Seoul Natl Univ, SNU Astron Res Ctr, 1 Gwanak Ro, Seoul 08826, South Korea; Univ Montreal, Ctr Rech Astrophys Quebec, 1375 Ave Therese Lavoie Roux, Montreal, PQ H2V 0B3, Canada; Univ Montreal, Dept Phys, 1375 Ave Therese Lavoie Roux, Montreal, PQ H2V 0B3, Canada; Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan; Meisei Univ, Fac Sci & Engn, Dept Phys, 2-1-1 Hodokubo, Hino, Tokyo 11918506, Japan; Tokushima Univ, Minami Jousanajima Machi 1-1, Tokushima 7708502, Japan; Tokushima Univ, Inst Liberal Arts & Sci, Minami Jousanajima Machi 1-1, Tokushima 7708502, Japan; NAOJ Chile, Natl Astron Observ Japan, Alonso de Cordova 3788,Off 61B, Santiago 7630422, Chile; Joint ALMA Observ, Alonso de Cordova 3107, Santiago, Chile; Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan; Natl Inst Nat Sci, Astrobiol Ctr, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan; Acad Sinica, Inst Astron & Astrophys, 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan; Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England; Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, P-4150762 Porto, Portugal; Nagoya Univ, Grad Sch Sci, Dept Phys, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan; UCL, Dept Phys & Astron, London WC1E 6BT, England; Univ Tokyo, Grad Sch Arts & Sci, Dept Earth Sci & Astron, Meguro Ku, 3-8-1 Komaba, Tokyo 1538902, Japan; Vietnam Acad Sci & Technol, Vietnam Natl Space Ctr, 18 Hoang Quoc Viet, Hanoi, Vietnam; Chungnam Natl Univ, Dept Astron & Space Sci, 99 Daehak Ro, Daejeon 34134, South Korea; Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales; Univ Space Res Assoc, SOFIA Sci Ctr, NASA, Ames Res Ctr, Moffett Field, CA 94035 USA; Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China; Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China; Univ Paris Diderot, Lab AIM CEA DSM CNRS, CEA Saclay, IRFU,Serv Astrophys, F-91191 Gif Sur Yvette, France; SKA Org, Jodrell Bank, Macclesfield SK11 9FT, Cheshire, England; Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Oxford Rd, Manchester M13 9PL, Lancs, England; Natl Tsing Hua Univ, Inst Astron, Hsinchu 30013, Taiwan; Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan; Chinese Acad Sci, Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Peoples R China; Natl Cent Univ, Inst Astron, Zhongli 32001, Taiwan; Chinese Acad Sci, Natl Astron Observ, CAS Key Lab FAST, Beijing, Peoples R China; Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China; Jet Prop Lab, M-S 169-506,4800 Oak Grove Dr, Pasadena, CA 91109 USA; Liverpool John Moores Univ, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England; Univ South Wales, Pontypridd CF37 1DL, M Glam, Wales; Univ Manitoba, Dept Phys & Astron, Winnipeg, MB R3T 2N2, Canada; Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA; Univ Hertfordshire, Sch Phys Astron & Math, Coll Lane, Hatfield AL10 9AB, Herts, England; Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China; Univ Exeter, Phys & Astron, Stocker Rd, Exeter EX4 4QL, Devon, England; Natl Astron Observ Japan, Subaru Telescope, 650 N Aohoku Pl, Hilo, HI 96720 USA; Univ Western Ontario, Dept Phys & Astron, 1151 Richmond St, London, ON N6A 3K7, Canada; Doshisha Univ, Dept Environm Syst Sci, Miyakodani 1-3, Kyoto 6100394, Japan; Kyungpook Natl Univ, Coll Nat Sci, Dept Astron & Atmospher Sci, 80 Daehakro, Daegu 41566, South Korea; Natl Inst Nat Sci, Natl Astron Observ Japan, Div Theoret Astron, Mitaka, Tokyo 1818588, Japan; Hiroshima Univ, Hiroshima Astrophys Sci Ctr, Kagamiyama 1-3-1, Higashihiroshima, Hiroshima 7398526, Japan; Hiroshima Univ, Dept Phys, Kagamiyama 1-3-1, Higashihiroshima, Hiroshima 7398526, Japan; Hiroshima Univ, Core Res Energet Universe CORE U, Kagamiyama 1-3-1, Higashihiroshima, Hiroshima 7398526, Japan; European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany; Natl Inst Nat Sci, Nobeyama Radio Observ, Natl Astron Observ Japan, Minamisa Ku, Minamimaki, Nagano 3841305, Japan; Tohoku Univ, Grad Sch Sci, Astron Inst, Aoba Ku, Sendai, Miyagi 9808578, Japan; McMaster Univ, Dept Phys & Astron, Hamilton, ON L8S 4M1, Canada; Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS B3H 4R2, Canada; Chalmers Univ Technol, Dept Space Earth & Environm, SE-41296 Gothenburg, Sweden; Kyung Hee Univ, Sch Space Res, 1732 Deogyeong Daero, Yongin 17104, Gyeonggi Do, South Korea; Yunnan Univ, Dept Astron, Kunming 650091, Yunnan, Peoples R China; Nanjing Univ, Sch Astron & Space Sci, 163 Xianlin Ave, Nanjing 210023, Peoples R China; Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Peoples R China; Kagawa Univ, Fac Educ, Saiwai Cho 1-1, Takamatsu, Kagawa 7608522, Japan; Kagawa Univ, Ctr Educ Dev & Support, Saiwai Cho 1-1, Takamatsu, Kagawa 7608522, Japan; Kyoto Univ, Grad Sch Sci, Dept Astron, Sakyo Ku, Kyoto 6068502, Japan; Natl Astron Observ Japan, Div Theoret Astron, Mitaka, Tokyo 1818588, Japan; SOKENDAI Grad Univ Adv Studies, Hayama, Kanagawa 2400193, Japan; Kagoshima Univ, Grad Sch Sci & Engn, Dept Phys & Astron, 1-21-35 Korimoto, Kagoshima, Kagoshima 8900065, Japan; Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England; Univ Cambridge, Kavli Inst Cosmol, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England; Univ Tsukuba, Fac Pure & Appl Sci, 1-1-1 Tennodai, Tsukuba, Ibaraki 3058577, Japan; UCL, Phys & Astron Dept, OSL, London WC1E 6BT, England; Kwansei Gakuin Univ, Sch Sci & Technol, Dept Phys, 2-1 Gakuen, Sanda, Hyogo 6691337, Japan; Natl Res Council Canada, Herzberg Astron & Astrophys Res Ctr, Dominion Radio Astrophys Observ, POB 248, Penticton, BC V2A 6J9, Canada; Univ Sci & Technol Hanoi, Vietnam Acad Sci & Technol, 18 Hoang Quoc Viet, Hanoi, Vietnam; UCL, Phys & Astron Dept, London WC1E 6BT, England; Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China; Univ Leeds, Dept Appl Math, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England; Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France; Univ Leeds, Sch Phys & Astron, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England | ; Ohashi, Nagayoshi/ABA-9767-2020; Shimajiri, Yoshito/B-1445-2013; Priestley, Felix/KYP-3257-2024; ONAKA, TAKASHI/G-5058-2014; Kemper, Francisca/AAZ-8274-2020; Yen, Hsi-Wei/C-8307-2011; Savini, Gianluca/C-1188-2009; Lee, Jeong-Eun/E-2387-2013; Liu, Hong-Li/AAR-1998-2020; Gu, Qilao/LTZ-1282-2024; Tang湯雅雯, Ya-Wen/AAZ-7382-2020; Liu, Junhao/GNH-4246-2022; Han, Ilseung/MBG-4273-2025; Kim, Shinyoung/JEO-8879-2023; Koch, Patrick/AAV-3373-2021; Kataoka, Akimasa/AAU-5038-2020; Soam, Archana/AAG-4250-2021; Lee, Chang/HME-1129-2023; Chakali, Eswaraiah/L-5146-2018; 顏士韋, Hsi-Wei/C-8307-2011; Yuan, Jinghua/W-4699-2017; Lee, Chin-Fei/AAZ-3391-2020; Hwang, Jihye/JXW-6363-2024; WANG, Qiuhong/L-9577-2016; Li, Hua-bai/AEU-0239-2022; chen, zhiwei/AAP-5465-2020; Liu, Sheng-Yuan/AAZ-4303-2020; , Le Ngoc Tram/AAH-2951-2019; Van Loo, Sven/JRX-9178-2023; NGOC, NGUYEN/JQJ-4239-2023; Tomisaka, Kohji/E-6508-2013; Li, Di/HLH-4146-2023; LI, DI/HLH-4146-2023; Doi, Yasuo/A-3395-2013; Arzoumanian, Doris/JQT-3284-2023; Inutsuka, Shu-ichiro/I-7024-2014; Nanayakkara, Themiya/AAT-6271-2020; Tsukamoto, Yusuke/AAU-3453-2020; Li, Dalei/ABF-2406-2021; Lee, Sang-Sung/AFS-2722-2022 | 6508022172; 7601365384; 35238413800; 57215516631; 8355600600; 56512202800; 15822192800; 7005805931; 57203067199; 6603570734; 57201082771; 7005566228; 7103332462; 7403258846; 7202929125; 7004002583; 7404174499; 16549809400; 36237885400; 59684797600; 35330124000; 57203026080; 55633098300; 7401662157; 7409321582; 57202952564; 24170690100; 55874635700; 37056945900; 18936782900; 55441261000; 57206389610; 7006011851; 55750223500; 55757586800; 55727743600; 55320822200; 56568251300; 59821849300; 35499669400; 12790268500; 55705656800; 35242015200; 56566873100; 56342326600; 55231989000; 57218669464; 7005084542; 57218489062; 49865000200; 55210722100; 57217586664; 7403536449; 55170000100; 8318213100; 7004237751; 6602882601; 22834355900; 55673595500; 7005672565; 8547622700; 9234005200; 7003509373; 22834101100; 7101632548; 7403310385; 57194592820; 57194798843; 6603664735; 7404169517; 35237077900; 55226383000; 35377433200; 24074312000; 35330159300; 25627568300; 55750138400; 7201640315; 36571804600; 55671720700; 57194595458; 34770134800; 35773361100; 57189663358; 7005283695; 36238131700; 56455301400; 55370384000; 57194605392; 7402935899; 35748985900; 57209285153; 57190230987; 56252021400; 7405326474; 35185338100; 56436978700; 57209260420; 57194603379; 7409459358; 56179884700; 7402157762; 35569334500; 7003401658; 13310130800; 7201941871; 36714093500; 57216925030; 7202558313; 35096693300; 16070455300; 57194941451; 6602816367; 36976168000; 38862759600; 7403068909; 7101942174; 7004265198; 57194586988; 7006586973; 56800212700; 7407452361; 15844178300; 6603887796; 6604032293; 23061889500; 35482578500; 57202847250; 27868095600; 6701467496; 57201731842; 36971326200; 7003564783; 57194606597; 56084174100; 57219690533; 43361931100; 55170380200; 57209281402; 57199325064; 56493265600; 57207478624; 56183368700; 36955785700; 36238023800; 35308644100; 7004415016; 36908360800; 14042952700 | ASTROPHYSICAL JOURNAL | ASTROPHYS J | 0004-637X | 1538-4357 | 918 | 2 | SCIE | ASTRONOMY & ASTROPHYSICS | 2021 | 5.521 | 19.6 | 1.19 | 2025-07-30 | 17 | 18 | FAR-INFRARED POLARIZATION; FORMING MOLECULAR CLOUDS; GOULD BELT SURVEY; MAGNETIC-FIELDS; SUBMILLIMETER POLARIZATION; IMAGING POLARIMETRY; BIPOLAR OUTFLOW; STAR-FORMATION; SCUBA-2; CORES | English | 2021 | 2021-09 | 10.3847/1538-4357/ac0ce9 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |||||
| ○ | ○ | Article | Aqueous Nd³⁺ capture using a carboxyl-functionalized porous carbon derived from ZIF-8 | A porous graphitic carbon was obtained via the pyrolysis of a zeolite imidazolate framework (ZIF-8) under Ar atmosphere. Then, the carbon was functionalized with carboxylic groups and applied for separation of neodymium ions (Nd3+) from water. The adsorbent (denoted as C-ZDC) was characterized by X-ray diffraction, N-2 adsorption-desorption isotherms, infrared spectroscopy, X-ray photoelectron spectroscopy, scanning and transition electron microscopies, thermogravimetric analysis, and Boehm titration. A practical adsorption equilibrium was attained within 4 h, and the adsorption isotherm at 25 degrees C revealed a maximum adsorption capacity of 175 mg/g, which is one of the highest values reported for different kinds of adsorbents. The adsorption kinetics and equilibrium isotherms were modeled, and the selectivity for Nd3+ over other metal ions was examined. From the effect of solution pH on the adsorption and material characterization results before and after adsorption, the high adsorption capacity of C-ZDC was ascribed to the formation of coordination bonds between Nd3+ ions and the -COOH groups. Further, the material was reusable for at least four adsorption-desorption cycles after a simple step of acid washing. (C) 2021 Elsevier Inc. All rights reserved. | Ahmed, Imteaz; Bhattacharjee, Samiran; Lee, Chang-Soo; Kang, Kyoung-Ku; Ahn, Ji-Whan; Ahn, Wha-Seung | Inha Univ, Dept Chem & Chem Engn, Incheon 402751, South Korea; Kyungpook Natl Univ, Dept Chem, Daegu 41566, South Korea; Univ Dhaka, Ctr Adv Res Sci CARS, Dhaka 1000, Bangladesh; Chungnam Natl Univ, Dept Chem Engn & Appl Chem, Daejeon 305764, South Korea; Korea Inst Geosci & Mineral Resources KIGAM, Daejeon 305350, South Korea | Lee, Chang/HME-1129-2023; Kang, Kyoung-Ku/HLX-0854-2023 | 55377179600; 7102306254; 7410150229; 55667087900; 8332940200; 55665260500 | rhadum@cnu.ac.kr;whasahn@inha.ac.kr; | JOURNAL OF COLLOID AND INTERFACE SCIENCE | J COLLOID INTERF SCI | 0021-9797 | 1095-7103 | 594 | SCIE | CHEMISTRY, PHYSICAL | 2021 | 9.965 | 19.7 | 1.26 | 2025-07-30 | 28 | 29 | ZIF-8; ZIF-derived carbon; Carboxylic acid functionalization; Rare-earth elements; Adsorption | RARE-EARTH-ELEMENTS; ADSORPTION; RECOVERY; SEPARATION; NANOPARTICLES; ADSORBENTS; MECHANISM; IONS | Adsorption; Carboxylic acid functionalization; Rare-earth elements; ZIF-8; ZIF-derived carbon | Adsorption isotherms; Carbon; Desorption; Infrared spectroscopy; Metal ions; Metals; Porous materials; Thermogravimetric analysis; X ray photoelectron spectroscopy; Zeolites; carbon; carboxylic acid; lanthanide; metal ion; neodymium; unclassified drug; zeolite; zeolite imidazolate framework; Adsorption capacities; Adsorption equilibria; Carboxyl-functionalized; Desorption isotherms; Equilibrium isotherms; High adsorption capacity; Material characterizations; Porous graphitic carbon; adsorption kinetics; Article; desorption; infrared spectroscopy; isotherm; priority journal; temperature measurement; Adsorption | English | 2021 | 2021-07-15 | 10.1016/j.jcis.2021.03.036 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||
| ○ | ○ | Article | Understanding the high performance of an iron-antimony binary metal oxide catalyst in selective catalytic reduction of nitric oxide with ammonia and its tolerance of water/sulfur dioxide | YIn recent years, Fe-based catalysts for the selective catalytic reduction of NO with NH3 (NH3-SCR) have been attracting more attention. In this work, a novel Fe-Sb binary metal oxide catalyst was synthesized using the ethylene glycol assisted co-precipitation method and was characterized using a series of tech-niques. It was found that the catalyst with a molar ratio of 7:3 (Fe:Sb) displayed the best NH3-SCR activity with 100% conversion of NOx (nitrogen oxides) over a wide temperature window and with good resistance to H2O + SO2 at 250 degrees C. The X-ray photoelectron spectroscopy (XPS) and in situ diffused reflectance infrared Fourier transform spectroscopy (in situ DRIFTS) of NOx adsorption results suggested that strong electron interactions between Fe and Sb in Fe-O-Sb species existed and electrons of Sb could be transferred to Fe through the 2Fe(3+) + Sb3+ 2Fe(2+) + Sb5+ redox cycle. The introduction of Sb significantly improved the adsorption behaviour of NOx species on the Fe0.7Sb0.3Ox surface, which benefitted the adsorption/transformation of NOx, thereby facilitating the NH3-SCR reaction. In addition, the Fe0.7Sb0.3Ox catalyst demonstrated a good tolerance of H2O and SO2, since the decomposition of NH4HSO4 on the catalyst surface was promoted by the introduction of Sb. (C) 2020 Elsevier Inc. All rights reserved. | Jia, Xuanxuan; Liu, Hao; Zhang, Yu; Chen, Wei; Tong, Qing; Piao, Guangxia; Sun, Chuanzhi; Dong, Lin | Shandong Normal Univ, Inst Mat & Clean Energy, Coll Chem Chem Engn & Mat Sci, Shandong Prov Key Lab Clean Prod Fine Chem, Jinan 250014, Peoples R China; Nanjing Univ, Sch Environm, Ctr Modern Anal, Jiangsu Key Lab Vehicle Emiss Control, Nanjing 210093, Peoples R China; Kyungpook Natl Univ, Sch Energy Engn, Daegu 41566, South Korea | Gao, Fei/F-9557-2015; Zhang, Yu-Yang/F-2078-2011; chen, wei/G-2032-2018; Dong, Lin/N-6988-2014 | 57209750368; 58607766700; 57225165987; 57202097729; 56389269600; 57193277010; 36993538500; 7402561333 | suncz@sdnu.edu.cn; | JOURNAL OF COLLOID AND INTERFACE SCIENCE | J COLLOID INTERF SCI | 0021-9797 | 1095-7103 | 581 | SCIE | CHEMISTRY, PHYSICAL | 2021 | 9.965 | 19.7 | 1.77 | 2025-07-30 | 39 | 37 | NH3-SCR; Fe-Sb binary metal oxide; Redox cycle; H2O+SO2 tolerance | SO2 TOLERANCE; REACTION-MECHANISM; ACTIVE-SITES; SCR REACTION; NH3; NO; OXIDATION; NH3-SCR; INSIGHT; CERIA | Fe-Sb binary metal oxide; H<sub>2</sub>O+SO<sub>2</sub> tolerance; NH<sub>3</sub>-SCR; Redox cycle | Adsorption; Ammonia; Antimony compounds; Catalysts; Ethylene; Ethylene glycol; Fourier transform infrared spectroscopy; Iron metallography; Metals; Molar ratio; Nitric oxide; Nitrogen oxides; Precipitation (chemical); Redox reactions; X ray photoelectron spectroscopy; ammonia; antimony; iron; nitric oxide; sulfur dioxide; Adsorption behaviour; Binary metal oxides; Coprecipitation method; Diffused reflectance; Electron interaction; Fe-based catalysts; Fourier transform spectroscopy; Selective catalytic reduction of NO; adsorption; Article; catalyst; comparative study; controlled study; Fourier transform infrared spectroscopy; physical chemistry; precipitation; priority journal; reaction analysis; room temperature; steady state; surface property; thermogravimetry; transmission electron microscopy; X ray photoemission spectroscopy; X ray powder diffraction; Selective catalytic reduction | English | 2021 | 2021-01-01 | 10.1016/j.jcis.2020.07.089 | 바로가기 | 바로가기 | 바로가기 | 바로가기 | ||
| ○ | ○ | Article | Clinical outcomes of endoscopic resection for undifferentiated intramucosal early gastric cancer larger than 2 cm | Background This study investigated the long-term clinical outcomes of endoscopic resection (ER) for undifferentiated-type (UD) early gastric cancer (EGC), with tumor size > 2 cm as the only non-curative factor. Methods From among 1123 patients who underwent ER for UD EGC at 18 tertiary hospitals in Korea between 2005 and 2014, we identified 216 patients with UD intramucosal EGC > 2 cm, which was completely resected, with negative resection margins, and absence of ulceration and lymphovascular invasion. The patients were divided into the additional surgery (n = 40) or observation (n = 176) groups, according to post-ER management and were followed up for a median duration of 59 months for recurrence and 90 months for overall survival. Results Lymph node (LN) or distant metastasis or cancer-related mortality was not observed in the surgery group. In the observation group, two (1.1%) patients developed LN or distant metastasis with a 5-year cumulative risk of 0.7%, and one (0.6%) patient died of gastric cancer. The 5- and 8-year overall survival rates were 94.1% and 89.9%, respectively, in the observation group and 100.0% and 95.2%, respectively, in the surgery group (log-rankP = 0.159). Cox regression analysis did not reveal an association between the observation group and increased mortality. Conclusion The risk of LN or distant metastasis was not negligible, but as low as 1% for patients undergoing non-curative ER for UD EGC, with tumor size > 2 cm as the only non-curative factor. Close observation may be an alternative to surgery, especially for older patients or those with poor physical status. | Yang, Hyo-Joon; Nam, Su Youn; Min, Byung-Hoon; Ahn, Ji Yong; Jang, Jae-Young; Kim, Jung; Kim, Jie-Hyun; Lee, Wan-Sik; Lee, Bong Eun; Joo, Moon Kyung; Park, Jae Myung; Shin, Woon Geon; Lee, Hang Lak; Gweon, Tae-Geun; Park, Moo In; Choi, Jeongmin; Tae, Chung Hyun; Kim, Young-Il; Choi, Il Ju | Sungkyunkwan Univ, Kangbuk Samsung Hosp, Sch Med, Div Gastroenterol,Dept Internal Med, Seoul, South Korea; Sungkyunkwan Univ, Kangbuk Samsung Hosp, Sch Med, Gastrointestinal Canc Ctr, Seoul, South Korea; Kyungpook Natl Univ, Kyungpook Natl Univ Hosp, Sch Med, Div Gastroenterol,Dept Internal Med, 807 Hoguk Ro, Daegu, South Korea; Sungkyunkwan Univ, Samsung Med Ctr, Dept Med, Sch Med, 81 Irwon Ro, Seoul 06351, South Korea; Univ Ulsan, Asan Med Ctr, Dept Internal Med, Div Gastroenterol,Coll Med, Seoul, South Korea; Kyung Hee Univ, Coll Med, Dept Internal Med, Seoul, South Korea; Seoul Natl Univ, Dept Internal Med, Div Gastroenterol, Coll Med, Seoul, South Korea; Seoul Natl Univ, Liver Res Inst, Coll Med, Seoul, South Korea; Yonsei Univ, Gangnam Severance Hosp, Dept Internal Med, Div Gastroenterol,Coll Med, Seoul, South Korea; Chonnam Natl Univ, Dept Internal Med, Med Sch, Gwangju, South Korea; Pusan Natl Univ, Dept Internal Med, Sch Med, Busan, South Korea; Korea Univ, Guro Hosp, Dept Internal Med, Coll Med, Seoul, South Korea; Catholic Univ Korea, Dept Internal Med, Seoul St Marys Hosp, Seoul, South Korea; Hallym Univ, Dept Internal Med, Coll Med, Seoul, South Korea; Hanyang Univ, Dept Internal Med, Div Gastroenterol, Coll Med, Seoul, South Korea; Catholic Univ Korea, Coll Med, Dept Internal Med, Div Gastroenterol,Incheon St Marys Hosp, Incheon, South Korea; Kosin Univ, Dept Internal Med, Coll Med, Busan, South Korea; Inje Univ, Sanggye Paik Hosp, Dept Internal Med, Coll Med, Seoul, South Korea; Ewha Womans Univ, Dept Internal Med, Coll Med, Seoul, South Korea; Natl Canc Ctr, Ctr Gastr Canc, Goyang, South Korea | Lee, In/J-9324-2013; Ahn, Ji Yong/AGO-1695-2022; Kim, Yuriy/ABD-7016-2020; Kim, Jie-Hyun/Q-9061-2019; Park, Jae Myung/AGK-6655-2022; Kim, Jung/L-9791-2019 | 57188930761; 55617028500; 7202932034; 36809017800; 57215881098; 57218359704; 49461401400; 57208140974; 36461131900; 35313509000; 8548758100; 13606883400; 7501478057; 55365094900; 8666034000; 55646404000; 35211966400; 57203809495; 7401471464 | nam20131114@gmail.com;bhmin@skku.edu; | GASTRIC CANCER | GASTRIC CANCER | 1436-3291 | 1436-3305 | 24 | 2 | SCIE | GASTROENTEROLOGY & HEPATOLOGY;ONCOLOGY | 2021 | 7.701 | 19.8 | 0.39 | 2025-07-30 | 6 | 7 | Stomach neoplasms; Undifferentiated-type histology; Endoscopic mucosal resection; Treatment outcome; Lymph node metastasis | LYMPH-NODE METASTASIS; LONG-TERM OUTCOMES; SUBMUCOSAL DISSECTION; RISK-FACTORS; HISTOLOGY; CRITERIA; SURGERY | Endoscopic mucosal resection; Lymph node metastasis; Stomach neoplasms; Treatment outcome; Undifferentiated-type histology | Aged; Carcinoma; Endoscopic Mucosal Resection; Female; Gastrectomy; Gastric Mucosa; Humans; Lymph Nodes; Lymphatic Metastasis; Male; Margins of Excision; Middle Aged; Neoplasm Metastasis; Proportional Hazards Models; Republic of Korea; Retrospective Studies; Stomach Neoplasms; Survival Rate; Treatment Outcome; Tumor Burden; adult; Article; cancer mortality; cancer recurrence; controlled study; early cancer; endoscopic mucosal resection; female; follow up; histopathology; human; lymph vessel metastasis; major clinical study; male; overall survival; preoperative period; South Korea; stomach cancer; surgical risk; tertiary care center; tumor volume; undifferentiated intramucosal early gastric cancer; aged; carcinoma; clinical trial; endoscopic mucosal resection; gastrectomy; lymph node; lymph node metastasis; metastasis; middle aged; mortality; multicenter study; pathology; procedures; proportional hazards model; retrospective study; stomach mucosa; stomach tumor; surgical margin; survival rate; treatment outcome | English | 2021 | 2021-03 | 10.1007/s10120-020-01115-y | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |
| ○ | ○ | Article | Comparison between endoscopic submucosal resection and surgery for the curative resection of undifferentiated-type early gastric cancer within expanded indications: a nationwide multi-center study | Background and aims Endoscopic submucosal dissection (ESD) for undifferentiated early gastric cancer (UD EGC) has debate due to the risk of lymph node metastasis. We investigated the outcomes of ESD compared to those of surgery for the UD EGC within expanded indication. Methods We reviewed 971 UD EGC patients performed ESD across 18 hospitals in Korea and 1812 patients who underwent surgical resection in two hospitals between February 2005 and May 2015. Of these cases, we enrolled a curative resected ESD group of 328 patients and surgery group of 383 cases within an expanded indication. Overall outcomes and one-to-one propensity score-matched (218 ESD group vs 218 surgery group cases) outcomes for these two groups were analyzed. Results Over the 75.6 month median follow-up period for the 711 enrolled cases, recurrences occurred in 22 patients (6.7%) in the ESD group but not in the surgery group. Overall survival (OS) was higher in the surgery group (p = 0.0316) in all cases, but there was no significant difference after propensity score matching (p = 0.069). According to the histologic type in propensity score matching, the OS of signet ring cell carcinoma and poorly differentiated carcinoma patients did not differ between the ESD and surgery groups (p = 0.1189 and p = 0.3087, respectively). In the surgery group involving expanded criteria, lymph node metastasis was found in six cases (1.56%). Conclusions Although ESD shows comparable outcomes to surgery for the UD EGC within expanded indications, appropriate patient selection is needed for the ESD due to the possibility of lymph node metastasis. | Ahn, Ji Yong; Kim, Young-, II; Shin, Woon Geon; Yang, Hyo-Joon; Nam, Su Youn; Min, Byung-Hoon; Jang, Jae-Young; Lim, Joo Hyun; Kim, Jie-Hyun; Lee, Wan Sik; Lee, Bong Eun; Joo, Moon Kyung; Park, Jae Myung; Lee, Hang Lak; Gweon, Tae- Geun; Park, Moo In; Choi, Jeongmin; Tae, Chung Hyun; Kim, Young-Woo; Park, Boram; Choi, I. I. Ju | Univ Ulsan, Coll Med, Asan Med Ctr, Div Gastroenterol,Dept Internal Med, Seoul, South Korea; Natl Canc Ctr, Res Inst & Hosp, Ctr Gastr Canc, Goyang, South Korea; Hallym Univ, Coll Med, Dept Internal Med, Inst Liver & Digest Dis, Chunchon, South Korea; Sungkyunkwan Univ, Sch Med, Div Gastroenterol, Dept Internal Med,Kangbuk Samsung Hosp, Seoul, South Korea; Sungkyunkwan Univ, Sch Med, Gastrointestinal Canc Ctr, Kangbuk Samsung Hosp, Seoul, South Korea; Kyungpook Natl Univ, Gastroenterol, Kyungpook Natl Univ Hosp, Sch Med, Daegu, South Korea; Sungkyunkwan Univ, Sch Med, Dept Med, Samsung Med Ctr, Seoul, South Korea; Kyung Hee Univ, Dept Internal Med, Coll Med, Seoul, South Korea; Seoul Natl Univ Hosp, Dept Internal Med, Inst Healthcare Res, Healthcare Syst Gangnam Ctr, Seoul, South Korea; Yonsei Univ, Coll Med, Div Gastroenterol, Dept Internal Med,Gangnam Severance Hosp, Seoul, South Korea; Chonnam Natl Univ, Sch Med, Dept Internal Med, Gwangju, South Korea; Pusan Natl Univ, Sch Med, Dept Internal Med, Busan, South Korea; Korea Univ, Coll Med, Dept Internal Med, Guro Hosp, Seoul, South Korea; Catholic Univ Korea, Dept Internal Med, Seoul St Marys Hosp, Seoul, South Korea; Hanyang Univ, Coll Med, Div Gastroenterol, Dept Internal Med, Seoul, South Korea; Catholic Univ Korea, Coll Med, Div Gastroenterol, Dept Internal Med,Incheon St Marys Hosp, Incheon, South Korea; Kosin Univ, Dept Internal Med, Coll Med, Busan, South Korea; Inje Univ, Coll Med, Dept Internal Med, Sanggye Paik Hosp, Seoul, South Korea; Ewha Womans Univ, Coll Med, Dept Internal Med, Seoul, South Korea; Natl Canc Ctr, Biostat Collaborat Team, Res Core Ctr, Res Inst, Goyang, South Korea; Kangdong Sacred Heart Hosp, Div Gastroenterol, Dept Internal Med, 445 Gil Dong, Seoul 05355, South Korea | Kim, Seong Cheol/ABD-1493-2022; Kim, Jie-Hyun/Q-9061-2019; Kim, Yuriy/ABD-7016-2020; Ahn, Ji Yong/AGO-1695-2022; Park, Jae Myung/AGK-6655-2022; Lee, In/J-9324-2013 | 36809017800; 57203809495; 13606883400; 57188930761; 55617028500; 7202932034; 57215881098; 55774506200; 49461401400; 57208140974; 36461131900; 35313509000; 8548758100; 7501478057; 55365094900; 8666034000; 55646404000; 35211966400; 57215377843; 55629622000; 59642100000 | sgun9139@gmail.com; | GASTRIC CANCER | GASTRIC CANCER | 1436-3291 | 1436-3305 | 24 | 3 | SCIE | GASTROENTEROLOGY & HEPATOLOGY;ONCOLOGY | 2021 | 7.701 | 19.8 | 1.57 | 2025-07-30 | 27 | 22 | Endoscopic submucosal dissection; Surgery; Undifferentiated histology; Stomach; Treatment outcome | LYMPH-NODE METASTASIS; RING CELL-CARCINOMA; LONG-TERM OUTCOMES; RISK-FACTORS; MUCOSAL RESECTION; DISSECTION; ADENOCARCINOMA; FEASIBILITY; RECURRENCE; ABSOLUTE | Endoscopic submucosal dissection; Stomach; Surgery; Treatment outcome; Undifferentiated histology | Adenocarcinoma; Carcinoma, Signet Ring Cell; Disease-Free Survival; Endoscopic Mucosal Resection; Female; Gastrectomy; Humans; Lymphatic Metastasis; Male; Middle Aged; Neoplasm Recurrence, Local; Propensity Score; Republic of Korea; Retrospective Studies; Stomach Neoplasms; Treatment Outcome; adult; Article; cancer recurrence; cancer survival; cohort analysis; early cancer; endoscopic submucosal dissection; female; follow up; histology; human; human tissue; Korea; lymph node metastasis; major clinical study; male; middle aged; overall survival; priority journal; propensity score; recurrence free survival; retrospective study; stomach cancer; stomach surgery; treatment indication; treatment outcome; adenocarcinoma; clinical trial; comparative study; disease free survival; endoscopic mucosal resection; gastrectomy; lymph node metastasis; multicenter study; pathology; signet ring carcinoma; South Korea; stomach tumor; tumor recurrence | English | 2021 | 2021-05 | 10.1007/s10120-020-01140-x | 바로가기 | 바로가기 | 바로가기 | 바로가기 | |
| ○ | ○ | Article | Development of a post-processing method to reduce the unique off-flavor of Allomyrina dichotoma: Yeast fermentation | Allomyrina dichotoma larva is an edible insect that has been consumed in East Asia for centuries. A. dichotoma is suitable for insect farming due to its numerous health benefits and advantages in industrial production. However, its market share is very poor due to their unique off-flavor, which negatively affects consumer preferences. So far, only one study has reported an effective method for reducing the unique off-flavor of A. dichotoma larvae. In this study, to reduce the off-flavor without increasing larval mortality, we inoculated Saccharomyces cerevisiae W-3, which is a wine fermentation yeast strain, in processed larva powder and investigated changes in volatiles. In the fermented larva powder, the intensity of indole, which has a strong fecal odor, decreased to 1/12. In addition, fruit-flavored volatiles such as ethyl acetate, isopentyl acetate, and 2-butanone increased by 17, 13, and 4 times, respectively. To provide clues for understanding the mechanisms by which volatiles change, we performed network analyses. Our yeast fermentation method can be used as a post process to reduce the off-flavor and improve the overall flavor of A. dichotoma larvae. | Kim, Jungyeon; Lee, Ha Eun; Kim, Yeojin; Yang, Jungwoo; Lee, Sung-Joon; Jung, Young Hoon | Univ Illinois, Carl R Woese Inst Genom Biol, Urbana, IL 61801 USA; Kyungpook Natl Univ, Sch Food Sci & Biotechnol, Daegu 41566, South Korea; Korea Univ, Dept Biotechnol, Coll Life Sci & Biotechnol, Seoul 02841, South Korea; Ildong Biosci, 17 Poseunggongdan Ro, Pyeongtaek Si 17957, Gyeonggi Do, South Korea | ; Jung, Young Hoon/F-1703-2013; Jung, Young/F-1703-2013; Kim, Jinkwon/AAR-6729-2021; Lee, Ha-Eun/HWQ-6568-2023 | 57214338692; 58601955500; 56045514100; 56076383700; 23065729100; 55550063700 | younghoonjung@knu.ac.kr; | LWT-FOOD SCIENCE AND TECHNOLOGY | LWT-FOOD SCI TECHNOL | 0023-6438 | 1096-1127 | 150 | SCIE | FOOD SCIENCE & TECHNOLOGY | 2021 | 6.056 | 19.8 | 0.91 | 2025-07-30 | 14 | 16 | Edible insects; Allomyrina dichotoma; Off-flavor; HS-SPME; GC-MS; Yeast fermentation | EDIBLE INSECTS; ALCOHOL ACETYLTRANSFERASE; ISOAMYL ACETATE; ETHYL-ACETATE; GRAPE; ODOR; WINE | Allomyrina dichotoma; Edible insects; HS-SPME/GC-MS; Off-flavor; Yeast fermentation | Competition; Fermentation; Allomyrina dichotoma; Dichotoma; East Asia; Edible insect; Health benefits; HS-SPME/GC-MS; Industrial production; Off-flavours; Postprocessing methods; Yeast fermentation; Yeast | English | 2021 | 2021-10 | 10.1016/j.lwt.2021.111940 | 바로가기 | 바로가기 | 바로가기 | 바로가기 |
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