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2. OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf

Author

Iona Kondo, Jennifer C. Yee, David P. Bennett, Takahiro Sumi, Naoki Koshimoto, Ian A. Bond, Andrew Gould, Andrzej Udalski, Yossi Shvartzvald, Youn Kil Jung, Weicheng Zang, Valerio Bozza, Etienne Bachelet, Markus P. G. Hundertmark, Nicholas J. Rattenbury, F. Abe, R Barry, A. Bhattacharya, M. Donachie, A. Fukui, H. Fujii, Y. Hirao, S. Ishitani Silva, Y. Itow, R. Kirikawa, M. C. A. Li, Y. Matsubara, S. Miyazaki, Y. Muraki, G. Olmschenk, C. Ranc, Y. Satoh, H. Shoji, D. Suzuki, Y. Tanaka, K. Ulaczyk, P. J. Tristram, T. Yamawaki, A Yonehara, R. Poleski, J. Skowron, M. K. Szymański, K. A. Rybicki, I. Soszynski, S. Kozłowski, P. Pietrukowicz, P. Iwanek, M. Wrona, M. D. Albrow, J. Wambsganss, S. J. Chung, C. Han, K. H. Hwang, H. W. Kim, I. G. Shin, S. M. Cha, D. J. Kim, S. L. Kim, C. U. Lee, D. J. Lee, Y. Lee, B. G. Park, R. W. Pogge, Y.-H. Ryu, C. A. Beichman, G Bryden, S. Calchi Novati, S. Carey, B. S. Gaudi, C. B. Henderson, W. Zhu, D. Maoz, M. T. Penny, M. Dominik, U. G. Jorgensen, P. Longa-Pena, N. Peixinho, S. Sajadian, J. Skottfelt, C. Snodgrass, J. Tregloan-Reed, M. J. Burgdorf, J. Campbell-White, S. Dib, Y. I. Fujii, E. Khalouei, S. Rahvar, M. Rabus, J. Southworth, Y. Tsapras, R. A. Street, D. M. Bramich, A. Cassan, K. Horne, S. Mao, A. Saha, and P. Mroz

Subjects
Astronomy
Abstract

We report an analysis of the planetary microlensing event OGLE-2018-BLG-1185, which was observed by a large number of ground-based telescopes and by the Spitzer Space Telescope. The ground-based light curve indicates a low planet–host star mass ratio ofq=(6.9±0.2)×10−5, which is near the peak of the wide-orbit exoplanet mass-ratio distribution. We estimate the host star and planet masses with a Bayesian analysis using the measured angular Einstein radius under the assumption that stars of all masses have an equal probability of hosting the planet. The flux variation observed by Spitzer is marginal, but still places a constraint on the microlens parallax. Imposing a conservative constraint that this flux variation should beΔfSpz<4 instrumental flux units yields a host mass of=-+MM0.37 host 0.210.35 and a planet mass of =-+ÅmM8.4p4.77.9. A Bayesian analysis including the full parallax constraint from Spitzer suggests smaller host star and planet masses of =-+MM0.091 host 0.0180.064 and =-+ÅmM2.1p0.41.5, respectively. Future high-resolution imaging observations with the Hubble Space Telescope or Extremely Large Telescope could distinguish between these two scenarios and help reveal the planetary system properties in more detail.

Published
2021
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3. OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing

Author

S-S Li, W Zang, A Udalski, Y Shvartzvald, D Huber, C-U Lee, T Sumi, A Gould, S Mao, P Fouqué, T Wang, S Dong, U G Jørgensen, A Cole, P Mróz, M K Szymański, J Skowron, R Poleski, I Soszyński, P Pietrukowicz, S Kozłowski, K Ulaczyk, K A Rybicki, P Iwanek, J C Yee, S Calchi Novati, C A Beichman, G Bryden, S Carey, B S Gaudi, C B Henderson, W Zhu, M D Albrow, S-J Chung, C Han, K-H Hwang, Y K Jung, Y-H Ryu, I-G Shin, S-M Cha, D-J Kim, H-W Kim, S-L Kim, D-J Lee, Y Lee, B-G Park, R W Pogge, I A Bond, F Abe, R Barry, D P Bennett, A Bhattacharya, M Donachie, A Fukui, Y Hirao, Y Itow, I Kondo, N Koshimoto, M C A Li, Y Matsubara, Y Muraki, S Miyazaki, M Nagakane, C Ranc, N J Rattenbury, H Suematsu, D J Sullivan, D Suzuki, P J Tristram, A Yonehara, G Christie, J Drummond, J Green, S Hennerley, T Natusch, I Porritt, E Bachelet, D Maoz, R A Street, Y Tsapras, V Bozza, M Dominik, M Hundertmark, N Peixinho, S Sajadian, M J Burgdorf, D F Evans, R Figuera Jaimes, Y I Fujii, L K Haikala, C Helling, T Henning, T C Hinse, L Mancini, P Longa-Peña, S Rahvar, M Rabus, J Skottfelt, C Snodgrass, J Southworth, E Unda-Sanzana, C von Essen, J-P Beaulieu, J Blackman, and K Hill

Published
2019
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4. Comparative genomics of Eucalyptus and Corymbia reveals low rates of genome structural rearrangement

Author

J. B. Butler, R. E. Vaillancourt, B. M. Potts, D. J. Lee, G. J. King, A. Baten, M. Shepherd, and J. S. Freeman

Subjects
Chromosome rearrangement, Corymbia citriodora, DArTseq, Eucalyptus grandis, Genome structure, Linkage mapping, Biotechnology, TP248.13-248.65, Genetics, QH426-470
Abstract

Abstract Background Previous studies suggest genome structure is largely conserved between Eucalyptus species. However, it is unknown if this conservation extends to more divergent eucalypt taxa. We performed comparative genomics between the eucalypt genera Eucalyptus and Corymbia. Our results will facilitate transfer of genomic information between these important taxa and provide further insights into the rate of structural change in tree genomes. Results We constructed three high density linkage maps for two Corymbia species (Corymbia citriodora subsp. variegata and Corymbia torelliana) which were used to compare genome structure between both species and Eucalyptus grandis. Genome structure was highly conserved between the Corymbia species. However, the comparison of Corymbia and E. grandis suggests large (from 1–13 MB) intra-chromosomal rearrangements have occurred on seven of the 11 chromosomes. Most rearrangements were supported through comparisons of the three independent Corymbia maps to the E. grandis genome sequence, and to other independently constructed Eucalyptus linkage maps. Conclusions These are the first large scale chromosomal rearrangements discovered between eucalypts. Nonetheless, in the general context of plants, the genomic structure of the two genera was remarkably conserved; adding to a growing body of evidence that conservation of genome structure is common amongst woody angiosperms.

Published
2017
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8. The 2L1S/1L2S Degeneracy for Two Microlensing Planet Candidates Discovered by the KMTNet Survey in 2017

Author

I.-G. Shin, J. C. Yee, A. Gould, M. T. Penny, I. A. Bond, M. D. Albrow, S.-J. Chung, C. Han, K.-H. Hwang, Y. K. Jung, Y.-H. Ryu, Y. Shvartzvald, S.-M. Cha, D.-J. Kim, H.-W. Kim, S.-L. Kim, C.-U. Lee, D.-J. Lee, Y. Lee, B.-G. Park, R. W. Pogge, F. Abe, R Barry, D P Bennett, A Bhattacharya, M. Donachie, H. Fujii, A. Fukui, Y. Hirao, Y. Itow, Y. Kamei, Iona Kondo, N. Koshimoto, M. C. A. Li, Y. Matsubara, S. Miyazaki, Y. Muraki, M. Nagakane, C Ranc, N. J. Rattenbury, Harmon Suematsu, D. J. Sullivan, T. Sumi, Daisuke Suzuki, P. J. Tristram, T. Yamakawa, A. Yonehara, P. Fouqué, and W. Zang

Subjects
Astrophysics, Astronomy
Abstract

We report two microlensing planet candidates discovered by the Korea Microlensing Telescope Network (KMTNet) survey in 2017. However, both events have the 2L1S/1L2S degeneracy, which is an obstacle to claiming the discovery of the planets with certainty unless the degeneracy can be resolved. For KMT-2017-BLG-0962, the degeneracy cannot be resolved. If the 2L1S solution is correct, KMT-2017-BLG-0962 might be produced by a super Jupiter-mass planet orbiting a mid-M-dwarf host star. For KMT-2017-BLG-1119, the light-curve modeling favors the 2L1S solution but higher-resolution observations of the baseline object tend to support the 1L2S interpretation rather than the planetary interpretation. This degeneracy might be resolved by a future measurement of the lens-source relative proper motion. This study shows that the problem of resolving 2L1S/1L2S degeneracy exists over a much wider range of conditions than those considered by the theoretical study of Gaudi (1998).

Published
2019
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9. Spitzer Microlensing Parallax for OGLE-2016-BLG-1067: A Sub-Jupiter Orbiting an M Dwarf in the Disk

Author

S. Calchi Novati, D Suzuki, A. Udalski, A. Gould, Y. Shvartzvald, V. Bozza, D P Bennett, C. Beichman, G Bryden, S. Carey, B. S. Gaudi, C. B. Henderson, J. C. Yee, W. Zhu, F. Abe, Y. Asakura, R Barry, A Bhattacharya, I. A. Bond, M. Donachie, P. Evans, A. Fukui, Y. Hirao, Y. Itow, K. Kawasaki, N. Koshimoto, M. C. A. Li, C. H. Ling, Y. Matsubara, S. Miyazaki, Y. Muraki, M. Nagakane, K. Ohnishi, C Ranc, N. J. Rattenbury, To. Saito, A. Sharan, D. J. Sullivan, T. Sumi, P. J. Tristram, T. Yamada, A. Yonehara, P. Mroz, R. Poleski, J. Skowron, M. K. Szymanski, I. Soszynski, S. Kozłowski, P. Pietrukowicz, K. Ulaczyk, M. Pawlak, M. D. Albrow, S.-J. Chung, C. Han, K.-H. Hwang, Y. K. Jung, Y.-H. Ryu, I.-G. Shin, W. Zang, S.-M. Cha, D.-J. Kim, H.-W. Kim, S.-L. Kim, C.-U. Lee, D.-J. Lee, Y. Lee, B.-G. Park, and R. W. Pogge

Subjects
Astronomy
Abstract

We report the discovery of a sub-Jupiter-mass planet orbiting beyond the snow line of an M dwarf most likely in the Galactic disk as part of the joint Spitzer and ground-based monitoring of planetary microlensing anomalies toward the Galactic bulge. Most of the microlensing parameters are strongly constrained by the light-curve modeling, and in particular there is a Spitzer-based measurement of the microlens parallax, π(E). However, there are no caustic crossings, so the angular Einstein radius has only an upper limit based on the light-curve modeling alone. Additionally, the analysis leads us to identify eight degenerate configurations: the fourfold microlensing parallax degeneracy being doubled by a degeneracy in the caustic structure present at the level of the ground-based solutions. To calculate the physical parameters, and at the same time to break the parallax degeneracy, we make use of a series of arguments: the χ(exp 2) hierarchy, the Rich argument (stating that the small-parallax solution is more likely), and a prior Galactic model. The preferred configuration, favored by a likelihood ratio of at least 4000, is for a host at D(L)={3.73}(-0.67+0.66)kpc with mass M(L)=0.30(-0.12+0.15) M(☉) , orbited by a Saturn-like planet with M(planet) =0.43(-0.17+0.21) M(Jup) at projected separation a(⊥) =1.70(-0.39+0.38) au, about 2.1 times beyond the system snow line. Therefore, it adds to the growing population of sub-Jupiter planets orbiting beyond the snow line of M dwarfs discovered by microlensing. Based on the rules of the real-time protocol for the selection of events to be followed up with Spitzer, this planet will not enter the sample for measuring the Galactic distribution of planets.

Published
2019
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10. Broadband measurement of high permittivity at millimetre‐wave frequencies

Author

Y.‐P. Hong, M.J. Salter, and D.‐J. Lee

Subjects
broadband high permittivity measurement, millimetre‐wave frequencies, quasi‐optical technique, quasi‐optical system calibration, S‐parameters, vector network analyser, Electrical engineering. Electronics. Nuclear engineering, TK1-9971
Abstract

In this Letter, a method for the broadband measurement of complex permittivity using a quasi‐optical technique is presented. After calibration of the quasi‐optical system, the material under test is inserted into the system and S‐parameters are measured from 220 to 330 GHz using a vector network analyser. An extraction method is then applied to calculate the complex permittivity. The permittivity measurements are validated by comparing with a well‐established extraction method and the comparison shows good agreement.

Published
2016
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13. Elevating the charge separation of MgFe

Author

G Mohan, Kumar, H D, Cho, D J, Lee, J Ram, Kumar, C, Siva, P, Ilanchezhiyan, D Y, Kim, and T W, Kang

Subjects
Zinc, Light, Water, Catalysis, Nanostructures
Abstract

Magnesium ferrites (MgFe

Published
2021

14. Causation and the Problem of Inter-Disability Discrimination in Hong Kong

Author

Kevin D. J. Lee

Subjects
Plaintiff, State (polity), Order (business), media_common.quotation_subject, Law, Disability discrimination, Legislature, Ambiguity, Tort, Causation, Psychology, media_common
Abstract

An anomalous series of cases has held that the tort of direct disability discrimination is not made out where the plaintiff cannot compare her circumstances with those of a person who is not disabled. There are situations, however, where comparison of this sort is necessary in order to ascertain whether the treatment complained of was caused by the plaintiff’s disability. In these cases, relief has been denied where it may ought to have been granted, and at a doctrinal and theoretical level the law is in an unsatisfactory state. The legislative text in question, however, admits of an ambiguity, and recourse can be made to its objects and purposes – and if necessary the constitutional guarantee of equality – to construe the provisions so that ‘inter-disability discrimination’ as it has been called is prohibited, not permitted.

Published
2021

15. Executive Expropriation Under Hong Kong’s National Security Law

Author

Kevin D. J. Lee

Subjects
National security, Human rights, Constitution, business.industry, media_common.quotation_subject, Fundamental rights, Legislation, Rule of law, Expropriation, Law, Political science, Ultra vires, business, media_common
Abstract

Perhaps two of the less anticipated aspects of the National Security Law (NSL) were its commitments to respect human rights and the rule of law in the safeguarding of national security, and the Court of First Instance has now held that the NSL is to be construed in accordance with fundamental rights guarantees in the constitution, so far as is reasonably possible. Against this backdrop, the Chief Executive and National Security Committee have promulgated Implementation Rules for article 43 of the NSL, Schedule 3 of which provides police officers with powers to freeze, restrain, charge, confiscate and forfeit property, when handling national security cases. This article identifies four ways in which Schedule 3 may be ineffective for operating ultra vires its empowering provision, article 43 of the NSL. It goes on to suggest that primary legislation could have achieved the means sought to be achieved by the four provisions in question, notwithstanding what may be the Administration’s view to the contrary.

Published
2021

16. KMT-2018-BLG-1988Lb: microlensing super-Earth orbiting a low-mass disk dwarf

Author

C. Han, In-Gu Shin, Hyoun-Woo Kim, Yoon-Hyun Ryu, Byeong-Gon Park, Dong-Jin Kim, Jennifer C. Yee, K. H. Hwang, Shinyoung Kim, Andrew Gould, C.-U. Lee, Yongseok Lee, Michael D. Albrow, Sun-Ju Chung, Yossi Shvartzvald, Y. Kil Jung, Doeon Kim, D. J. Lee, R. W. Pogge, W. Zang, Shude Mao, Chun-Hwey Kim, and Sang-Mok Cha

Subjects
Physics, Earth and Planetary Astrophysics (astro-ph.EP), Super-Earth, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Gravitational microlensing, Astrophysics - Astrophysics of Galaxies, Astrophysics - Earth and Planetary Astrophysics
Abstract

We reexamine high-magnification microlensing events in the previous data collected by the KMTNet survey with the aim of finding planetary signals that were not noticed before. In this work, we report the planetary system KMT-2018-BLG-1988L that was found from this investigation. The planetary signal appears as a deviation with $\lesssim 0.2$~mag from a single-lens light curve and lasted for about 6 hours. The deviation exhibits a pattern of a dip surrounded by weak bumps on both sides of the dip. The analysis of the lensing light curve indicates that the signal is produced by a low mass-ratio ($q\sim 4\times 10^{-5}$) planetary companion located near the Einstein ring of the host star. The mass of the planet, $M_{\rm planet}=6.8^{+4.7}_{-3.5}~M_\oplus$ and $5.6^{+3.8}_{-2.8}~M_\oplus$ for the two possible solutions, estimated from the Bayesian analysis indicates that the planet is in the regime of a super-Earth. The host of the planet is a disk star with a mass of $M_{\rm host} = 0.47^{+0.33}_{-0.25}~M_\odot$ and a distance of $D_{\rm L}= 4.2^{+1.8}_{-.14}$~kpc. KMT-2018-BLG-1988Lb is the seventeenth microlensing planet with a mass below the upper limit of a super-Earth. The fact that 14 out of 17 microlensing planets with masses $\lesssim 10~M_\oplus$ were detected during the last 5 years since the full operation of the KMTNet survey indicates that the KMTNet database is an important reservoir of very low-mass planets., Comment: 8 pages, 7 figures

Published
2021
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17. Myxoedema in Hashimoto's thyroiditis

Author

S.-W. Wu and D J Lee

Subjects
medicine.medical_specialty, business.industry, MEDLINE, General Medicine, Hashimoto Disease, medicine.disease, Dermatology, Thyroiditis, Myxedema, medicine, Humans, Thyroid Neoplasms, business
Published
2020

18. The Legal Status of Unincorporated Treaties in Hong Kong – Constitutionally Unique?

Author

Kevin D. J. Lee

Subjects
Legal status, Human rights, media_common.quotation_subject, Law, Political science, Estoppel, Context (language use), Orthodoxy, International law, media_common, Adjudication
Abstract

This article questions the received orthodoxy from England and Wales that unincorporated treaties are ineffective (or not self-executing) on the domestic plane, and that municipal courts are incompetent to adjudicate the rights and liabilities arising from them. Anomalous gaps in protection have arisen from the application of this orthodoxy in the human rights context in Hong Kong. A close analysis, however, shows the orthodox positions in both Hong Kong and England and Wales to have been overstated, and there is room and good constitutional reason for an estoppel to be imposed against the executive in human rights cases, resulting, effectively, in the direct application of unincorporated human rights norms.

Published
2020

19. Dual linear polarized cavity-backed patch rectenna with DC power management network for optimized wireless RF power transfer

Author

S.-T. Khang, D.-J. Lee, Soo-Chang Chae, and J.-W. Yu

Subjects
Power management, Computer science, business.industry, 020208 electrical & electronic engineering, RF power amplifier, Electrical engineering, 020206 networking & telecommunications, 02 engineering and technology, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, Electronic, Optical and Magnetic Materials, Dual (category theory), Rectenna, Transfer (computing), 0202 electrical engineering, electronic engineering, information engineering, Wireless, Electrical and Electronic Engineering, business
Published
2018

20. Unsupervised Video Shot Detection Using Clustering Ensemble with a Color Global Scale-Invariant Feature Transform Descriptor

Author

Yuchou Chang, D. J. Lee, Yi Hong, and James Archibald

Subjects
Electronics, TK7800-8360
Abstract

Scale-invariant feature transform (SIFT) transforms a grayscale image into scale-invariant coordinates of local features that are invariant to image scale, rotation, and changing viewpoints. Because of its scale-invariant properties, SIFT has been successfully used for object recognition and content-based image retrieval. The biggest drawback of SIFT is that it uses only grayscale information and misses important visual information regarding color. In this paper, we present the development of a novel color feature extraction algorithm that addresses this problem, and we also propose a new clustering strategy using clustering ensembles for video shot detection. Based on Fibonacci lattice-quantization, we develop a novel color global scale-invariant feature transform (CGSIFT) for better description of color contents in video frames for video shot detection. CGSIFT first quantizes a color image, representing it with a small number of color indices, and then uses SIFT to extract features from the quantized color index image. We also develop a new space description method using small image regions to represent global color features as the second step of CGSIFT. Clustering ensembles focusing on knowledge reuse are then applied to obtain better clustering results than using single clustering methods for video shot detection. Evaluation of the proposed feature extraction algorithm and the new clustering strategy using clustering ensembles reveals very promising results for video shot detection.

Published
2008
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21. OGLE-2018-BLG-1011Lb,c: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star

Author

B. Scott Gaudi, Masayuki Nagakane, Andrzej Udalski, Man Cheung Alex Li, Michał K. Szymański, Radek Poleski, Charles Beichman, Jennifer C. Yee, Sun-Ju Chung, Kohei Kawasaki, Igor Soszyński, Matthew T. Penny, Paweł Pietrukowicz, Dong-Jin Kim, M. Hundertmark, Keivan G. Stassun, Etienne Bachelet, Chung-Uk Lee, Byeong-Gon Park, In-Gu Shin, Cheongho Han, Marcin Wrona, Richard Barry, Sebastiano Calchi Novati, Youn Kil Jung, Fumio Abe, Andrew Gould, Clément Ranc, Yasushi Muraki, Weicheng Zang, Yongseok Lee, Atsunori Yonehara, D. J. Lee, K. H. Hwang, Richard W. Pogge, Aparna Bhattacharya, Paul J. Tristram, Daisuke Suzuki, Yutaka Matsubara, Seung-Lee Kim, Michael D. Albrow, Haruno Suematsu, Arnaud Cassan, Yoon-Hyun Ryu, Kay-Sebastian Nikolaus, David P. Bennett, Hyoun-Woo Kim, K. A. Rybicki, Szymon Kozłowski, Krzysztof Ulaczyk, Pascal Fouqué, Valerio Bozza, Sang-Mok Cha, Kyeongsoo Hong, Yoshitaka Itow, Wei Zhu, Geoffery Bryden, Martin Donachie, Tianshu Wang, Shota Miyazaki, Denis J. Sullivan, Naoki Koshimoto, Calen B. Henderson, Savannah Jacklin, Shude Mao, Patryk Iwanek, Przemek Mróz, Nicholas J. Rattenbury, Jan Skowron, Ian A. Bond, Iona Kondo, Akihiko Fukui, Doeon Kim, Takahiro Sumi, Yuki Hirao, and Yossi Shvartzvald

Subjects
gravitational lensing: micro, planetary systems, Physics, Earth and Planetary Astrophysics (astro-ph.EP), 010504 meteorology & atmospheric sciences, Lens (geology), Binary number, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Planetary system, Gravitational microlensing, Light curve, 01 natural sciences, Space and Planetary Science, Planet, 0103 physical sciences, Anomaly (physics), Low Mass, 010303 astronomy & astrophysics, Astrophysics - Earth and Planetary Astrophysics, 0105 earth and related environmental sciences
Abstract

著者人数: Leading authors 13名, The KMTNet Collaboration 18名, The OGLE Collaboration 11名, The MOA Collaboration 22名, The CFHT Collaboration 5名, The UKIRT Microlensing Team 7名, 全66名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 鈴木, 大介), Number of authors: Leading authors 13, The KMTNet Collaboration 18, The OGLE Collaboration 11, The MOA Collaboration 22, The CFHT Collaboration 5, The UKIRT Microlensing Team 7, Total 66 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Suzuki, Daisuke), Accepted: 2019-07-02, 資料番号: SA1190106000

Published
2019

22. Bubble Column Reactors

Author

D. J. Lee and L.-S. Fan

Subjects
Physics::Fluid Dynamics, Pressure drop, Bubble column, Materials science, Bubble, Flow (psychology), Mixing (process engineering), Mechanics, Diffusion (business), Wake, Dispersion (water waves)
Abstract

This chapter introduces some fundamental bubble dynamics in liquid media. Understanding bubble dynamics is critical for bubble column design since the hydrodynamic behaviors are induced and dictated by the gas phase in the form of bubbles. Complex hydrodynamic behavior in bubble columns is closely related to the characteristics of rising bubbles and bubble wake structures. The interaction between a rising bubble and the surrounding liquid medium produces the bubble shape and determines the extent of the disturbance in the surrounding flow field. In gas-liquid contacting systems, the velocity distribution in the wake region controls the diffusion/dispersion of gas from bubbles into liquid media. For gas-liquid systems, the experimental results available in the literature indicate that an increase of pressure retards the bubble coalescence. In bubble column reactors, the hydrodynamics, transport, and mixing properties, such as pressure drop, holdup of various phases, gas-liquid interfacial areas, and mass and heat transfers, depend strongly on the prevailing flow regime.

Published
2019

23. $Spitzer$ Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M-dwarf

Author

C. Han, Richard Barry, Seung-Lee Kim, K. A. Rybicki, Chung-Uk Lee, Akihiko Fukui, Tianshu Wang, Fumio Abe, Shude Mao, Paul J. Tristram, Naoki Koshimoto, Takahiro Sumi, Sebastiano Calchi Novati, Masayuki Nagakane, Sang-Mok Cha, Igor Soszyński, Dong-Jin Kim, Richard W. Pogge, Yutaka Matsubara, Geoffery Bryden, Man Cheung Alex Li, W. Zang, Jennifer C. Yee, R. Poleski, Wei Zhu, S. Miyazaki, Haruno Suematsu, D. J. Lee, Yoon-Hyun Ryu, Andrzej Udalski, Clément Ranc, Michał K. Szymański, Calen B. Henderson, Keivan G. Stassun, Yasushi Muraki, Yuki Hirao, Yongseok Lee, Atsunori Yonehara, Yossi Shvartzvald, Aparna Bhattacharya, In-Gu Shin, Martin Donachie, Denis J. Sullivan, Pascal Fouqué, Spitzer Team, Przemek Mróz, Michael D. Albrow, Marcin Wrona, David P. Bennett, B. G. Park, Ian A. Bond, Sean Carey, B. Scott Gaudi, Szymon Kozłowski, Yoshitaka Itow, Youn Kil Jung, Iona Kondo, Matthew T. Penny, Charles A. Beichman, Andrew Gould, Paweł Pietrukowicz, Hyoun-Woo Kim, K. Ulaczyk, K. H. Hwang, Savannah Jacklin, Sun-Ju Chung, Daisuke Suzuki, Patryk Iwanek, Nicholas J. Rattenbury, and Jan Skowron

Subjects
Physics, Earth and Planetary Astrophysics (astro-ph.EP), Proper motion, 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Mass ratio, Planetary system, Light curve, Gravitational microlensing, 01 natural sciences, Space and Planetary Science, Planet, Bulge, 0103 physical sciences, Astrophysics::Earth and Planetary Astrophysics, Low Mass, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Astrophysics - Earth and Planetary Astrophysics
Abstract

We report the discovery of a $Spitzer$ microlensing planet OGLE-2018-BLG-0596Lb, with preferred planet-host mass ratio $q \sim 2\times10^{-4}$. The planetary signal, which is characterized by a short $(\sim 1~{\rm day})$ "bump" on the rising side of the lensing light curve, was densely covered by ground-based surveys. We find that the signal can be explained by a bright source that fully envelops the planetary caustic, i.e., a "Hollywood" geometry. Combined with the source proper motion measured from $Gaia$, the $Spitzer$ satellite parallax measurement makes it possible to precisely constrain the lens physical parameters. The preferred solution, in which the planet perturbs the minor image due to lensing by the host, yields a Uranus-mass planet with a mass of $M_{\rm p} = 13.9\pm1.6~M_{\oplus}$ orbiting a mid M-dwarf with a mass of $M_{\rm h} = 0.23\pm0.03~M_{\odot}$. There is also a second possible solution that is substantially disfavored but cannot be ruled out, for which the planet perturbs the major image. The latter solution yields $M_{\rm p} = 1.2\pm0.2~M_{\oplus}$ and $M_{\rm h} = 0.15\pm0.02~M_{\odot}$. By combining the microlensing and $Gaia$ data together with a Galactic model, we find in either case that the lens lies on the near side of the Galactic bulge at a distance $D_{\rm L} \sim 6\pm1~{\rm kpc}$. Future adaptive optics observations may decisively resolve the major image/minor image degeneracy., 34 pages, 8 figures, Submitted to AAS journal

Published
2019

24. OGLE-2018-BLG-0022: First Prediction of an Astrometric Microlensing Signal from a Photometric Microlensing Event

Author

B. Scott Gaudi, K. A. Rybicki, Valerio Bozza, Andrzej Udalski, Michał K. Szymański, Yasushi Muraki, Jennifer C. Yee, Yongseok Lee, Paweł Pietrukowicz, Atsunori Yonehara, Masayuki Nagakane, Aparna Bhattacharya, Marcin Wrona, Seung-Lee Kim, David P. Bennett, Radek Poleski, Calen B. Henderson, Yoshitaka Itow, Sean Carey, K. H. Hwang, Takahiro Sumi, Andrew Gould, Woong-Tae Kim, Clément Ranc, Paul J. Tristram, Youn Kil Jung, Weicheng Zang, Kohei Kawasaki, Szymon Kozłowski, Przemek Mróz, Byeong-Gon Park, Dong-Jin Kim, Charles Beichman, D. J. Lee, Sun-Ju Chung, Ian A. Bond, Yuki Hirao, Man Cheung Alex Li, Richard W. Pogge, Cheongho Han, Yutaka Matsubara, Yossi Shvartzvald, Michael D. Albrow, Akihiko Fukui, Yoon-Hyun Ryu, Hyoun-Woo Kim, Doeon Kim, Daisuke Suzuki, Geoffery Bryden, Iona Kondo, Richard Barry, Krzysztof Ulaczyk, Arnaud Cassan, Shota Miyazaki, Naoki Koshimoto, Martin Donachie, Denis J. Sullivan, Patryk Iwanek, Nicholas J. Rattenbury, Jan Skowron, Igor Soszyński, In-Gu Shin, Chung-Uk Lee, Fumio Abe, Haruno Suematsu, and Sang-Mok Cha

Subjects
Physics, Proper motion, binaries: general, gravitational lensing: micro, 010308 nuclear & particles physics, FOS: Physical sciences, Astronomy, Centroid, Astronomy and Astrophysics, Gravitational microlensing, 01 natural sciences, Photometry (optics), Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Bulge, 0103 physical sciences, Satellite, Parallax, 010303 astronomy & astrophysics, Event (particle physics), Solar and Stellar Astrophysics (astro-ph.SR)
Abstract

著者人数: Leading authors 7名, The KMTNet Collaboration 20名, The MOA Collaboration 23名, The OGLE Collaboration 11名, Spitzer Microlensing Team 5名, 全66名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 鈴木, 大介), Number of authors: Leading authors 7, The KMTNet Collaboration 20, The MOA Collaboration 23, The OGLE Collaboration 11, Spitzer Microlensing Team 5, Total 66 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Suzuki, Daisuke), Accepted: 2019-04-02, 資料番号: SA1190031000

Published
2019

25. Spitzer Microlensing Parallax for OGLE-2016-BLG-1067: A Sub-Jupiter Orbiting an M Dwarf in the Disk

Author

Charles A. Beichman, Radosław Poleski, Naoki Koshimoto, Yasushi Muraki, Yongseok Lee, Atsunori Yonehara, Clément Ranc, K. Kawasaki, David P. Bennett, Michał Pawlak, Yoshitaka Itow, Hyoun-Woo Kim, Takahiro Sumi, Richard Barry, Andrew Gould, K. H. Hwang, Paweł Pietrukowicz, Wei Zhu, Igor Soszyński, Nicholas J. Rattenbury, Jan Skowron, Sang-Mok Cha, Masayuki Nagakane, Yuki Hirao, K. Ulaczyk, W. Zang, Yossi Shvartzvald, Michael D. Albrow, Y. Asakura, Sean Carey, Spitzer Team, Ian A. Bond, Daisuke Suzuki, Geoffery Bryden, In-Gu Shin, Valerio Bozza, Paul J. Tristram, S. Miyazaki, C. H. Ling, P. Evans, Seung-Lee Kim, To. Saito, S. Calchi Novati, Chung-Uk Lee, C. Han, D. J. Lee, Dong-Jin Kim, Jennifer C. Yee, Fumio Abe, Andrzej Udalski, B. G. Park, Michał K. Szymański, Szymon Kozłowski, Man Cheung Alex Li, K. Ohnishi, S. J. Chung, Aparna Bhattacharya, Youn Kil Jung, Yoon-Hyun Ryu, Calen B. Henderson, Przemek Mróz, Martin Donachie, Denis J. Sullivan, B. S. Gaudi, Akihiko Fukui, Richard W. Pogge, Yutaka Matsubara, T. Yamada, and A. Sharan

Subjects
Earth and Planetary Astrophysics (astro-ph.EP), Physics, 010504 meteorology & atmospheric sciences, FOS: Physical sciences, Astronomy, Astronomy and Astrophysics, gravitational lensing: micro, planetary systems, Space and Planetary Science, Astrophysics::Cosmology and Extragalactic Astrophysics, Planetary system, Gravitational microlensing, 01 natural sciences, Jupiter, 0103 physical sciences, Astrophysics::Earth and Planetary Astrophysics, Parallax, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Astrophysics - Earth and Planetary Astrophysics, 0105 earth and related environmental sciences
Abstract

We report the discovery of a sub-Jupiter mass planet orbiting beyond the snow line of an M-dwarf most likely in the Galactic disk as part of the joint Spitzer and ground-based monitoring of microlensing planetary anomalies toward the Galactic bulge. The microlensing parameters are strongly constrained by the light curve modeling and in particular by the Spitzer-based measurement of the microlens parallax, $\pi_\mathrm{E}$. However, in contrast to many planetary microlensing events, there are no caustic crossings, so the angular Einstein radius, $\theta_\mathrm{E}$ has only an upper limit based on the light curve modeling alone. Additionally, the analysis leads us to identify 8 degenerate configurations: the four-fold microlensing parallax degeneracy being doubled by a degeneracy in the caustic structure present at the level of the ground-based solutions. To pinpoint the physical parameters, and at the same time to break the parallax degeneracy, we make use of a series of arguments: the $\chi^2$ hierarchy, the Rich argument, and a prior Galactic model. The preferred configuration is for a host at $D_L=3.73_{-0.67}^{+0.66}~\mathrm{kpc}$ with mass $M_\mathrm{L}=0.30_{-0.12}^{+0.15}~\mathrm{M_\odot}$, orbited by a Saturn-like planet with $M_\mathrm{planet}=0.43_{-0.17}^{+0.21}~\mathrm{M_\mathrm{Jup}}$ at projected separation $a_\perp = 1.70_{-0.39}^{+0.38}~\mathrm{au}$, about 2.1 times beyond the system snow line. Therefore, it adds to the growing population of sub-Jupiter planets orbiting near or beyond the snow line of M-dwarfs discovered by microlensing. Based on the rules of the real-time protocol for the selection of events to be followed up with Spitzer, this planet will not enter the sample for measuring the Galactic distribution of planets., Comment: Submitted to AAS Journals

Published
2019

26. OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing

Author

R. Figuera Jaimes, Man Cheung Alex Li, Daniel Huber, Andrew A. Cole, K. H. Hwang, Calen B. Henderson, Masayuki Nagakane, I.-G. Shin, Wei Zhu, Sohrab Rahvar, Yasushi Muraki, Nuno Peixinho, C.-U. Lee, Steve Hennerley, Yuri I. Fujii, M. Rabus, Paul J. Tristram, Yongseok Lee, Andrzej Udalski, G. Bryden, Michał K. Szymański, C. von Essen, Penélope Longa-Peña, Radek Poleski, Atsunori Yonehara, Eduardo Unda-Sanzana, D. J. Lee, Lauri K. Haikala, Szymon Kozłowski, Naoki Koshimoto, Patryk Iwanek, B. S. Gaudi, Julie Green, Przemek Mróz, P. Fouqué, Daniel F. Evans, Thomas Henning, Jennifer C. Yee, M. Hundertmark, J.-P. Beaulieu, Iona Kondo, Richard W. Pogge, Yutaka Matsubara, Martin Dominik, K. Hill, Akihiko Fukui, Nicholas J. Rattenbury, Etienne Bachelet, Jan Skowron, Richard Barry, Tobias C. Hinse, Tianshu Wang, Michael D. Albrow, Igor Soszyński, Krzysztof Ulaczyk, Fumio Abe, Shota Miyazaki, Yoon-Hyun Ryu, S. Calchi Novati, Rachel Street, Aparna Bhattacharya, K. A. Rybicki, Byeong-Gon Park, Martin Donachie, Denis J. Sullivan, J. W. Blackman, J. Drummond, Sedighe Sajadian, Tim Natusch, Sang-Mok Cha, Takahiro Sumi, Martin Burgdorf, Daisuke Suzuki, Andrew Gould, Clément Ranc, Yuki Hirao, Weicheng Zang, Jesper Skottfelt, Yossi Shvartzvald, G. W. Christie, Luigi Mancini, Haruno Suematsu, I. Porritt, Dong-Jin Kim, S. S. Li, Ian A. Bond, John Southworth, D. Maoz, Shude Mao, Sean Carey, David P. Bennett, Yoshitaka Itow, Y. K. Jung, Valerio Bozza, Charles A. Beichman, Hyoun-Woo Kim, Chang S. Han, Colin Snodgrass, Christiane Helling, Paweł Pietrukowicz, Subo Dong, U. G. Jørgensen, Yiannis Tsapras, Seung-Lee Kim, S. J. Chung, University of St Andrews. School of Physics and Astronomy, and University of St Andrews. St Andrews Centre for Exoplanet Science

Subjects
oscillations [stars], Red giant, fundamental parameters [stars], DWARF STARS, Astrophysics, gravitational lensing: micro, 01 natural sciences, STANDARD, Angular diameter, Bulge, QB460, PROGRAM, QB Astronomy, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, QB, Earth and Planetary Astrophysics (astro-ph.EP), Physics, PLANET PHOTOMETRY, 3rd-DAS, Astrophysics - Solar and Stellar Astrophysics, stars: fundamental parameters, stars: oscillations, Astrophysics::Earth and Planetary Astrophysics, astro-ph.SR, STELLAR OSCILLATIONS, Brown dwarf, FOS: Physical sciences, asteroseismology, Astrophysics::Cosmology and Extragalactic Astrophysics, SUBGIANTS, Gravitational microlensing, Asteroseismology, Settore FIS/05 - Astronomia e Astrofisica, ANGULAR SIZES, SYSTEMS, 0103 physical sciences, Solar and Stellar Astrophysics (astro-ph.SR), DISTANCES, Astrophysics::Galaxy Astrophysics, 010308 nuclear & particles physics, Astronomy and Astrophysics, Light curve, SURFACE BRIGHTNESS RELATIONS, Space and Planetary Science, astro-ph.EP, micro [gravitational lensing], Parallax, QB799, Astrophysics - Earth and Planetary Astrophysics
Abstract

著者人数: 105名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 鈴木, 大介), Number of authors: 105 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Suzuki, Daisuke), Accepted: 2019-07-03, 資料番号: SA1190108000

Published
2019

27. OGLE-2016-BLG-0156: Microlensing Event With Pronounced Microlens-Parallax Effects Yielding Precise Lens Mass Measurement

Author

Paweł Pietrukowicz, Naoki Koshimoto, Kohei Kawasaki, Seung-Lee Kim, K. H. Hwang, Yasushi Muraki, Dong-Jin Kim, Yongseok Lee, Atsunori Yonehara, Chung-Uk Lee, David P. Bennett, Nicholas J. Rattenbury, Ian A. Bond, Jan Skowron, Yoshitaka Itow, Hyoun-Woo Kim, Richard Barry, Sun-Ju Chung, Daisuke Suzuki, Masayuki Nagakane, Fumio Abe, Aparna Bhattacharya, Radek Poleski, Sang-Mok Cha, Byeong-Gon Park, Yuki Hirao, Yossi Shvartzvald, Akihiko Fukui, Paul J. Tristram, Cheongho Han, Igor Soszyński, Haruno Suematsu, Doeon Kim, Iona Kondo, D. J. Lee, In-Gu Shin, Youn Kil Jung, Szymon Kozłowski, Richard W. Pogge, Yutaka Matsubara, Krzysztof Ulaczyk, Martin Donachie, Denis J. Sullivan, Takahiro Sumi, Andrzej Udalski, Michał K. Szymański, Michał Pawlak, M. James Jee, Yoon-Hyun Ryu, Michael D. Albrow, Przemek Mróz, Andrew Gould, Clément Ranc, Man Cheung Alex Li, Shota Miyazaki, and Jennifer C. Yee

Subjects
010504 meteorology & atmospheric sciences, Flux, FOS: Physical sciences, gravitational lensing: micro, Astrophysics, Gravitational microlensing, 01 natural sciences, law.invention, Einstein radius, Gravitation, law, 0103 physical sciences, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), 0105 earth and related environmental sciences, Physics, Microlens, Earth and Planetary Astrophysics (astro-ph.EP), Astronomy and Astrophysics, Light curve, Lens (optics), Astrophysics - Solar and Stellar Astrophysics, binaries: general, Space and Planetary Science, Parallax, Astrophysics - Earth and Planetary Astrophysics
Abstract

We analyze the gravitational binary-lensing event OGLE-2016-BLG-0156, for which the lensing light curve displays pronounced deviations induced by microlens-parallax effects. The light curve exhibits 3 distinctive widely-separated peaks and we find that the multiple-peak feature provides a very tight constraint on the microlens-parallax effect, enabling us to precisely measure the microlens parallax $\pi_{\rm E}$. All the peaks are densely and continuously covered from high-cadence survey observations using globally located telescopes and the analysis of the peaks leads to the precise measurement of the angular Einstein radius $\theta_{\rm E}$. From the combination of the measured $\pi_{\rm E}$ and $\theta_{\rm E}$, we determine the physical parameters of the lens. It is found that the lens is a binary composed of two M dwarfs with masses $M_1=0.18\pm 0.01\ M_\odot$ and $M_2=0.16\pm 0.01\ M_\odot$ located at a distance $D_{\rm L}= 1.35\pm 0.09\ {\rm kpc}$. According to the estimated lens mass and distance, the flux from the lens comprises an important fraction, $\sim 25\%$, of the blended flux. The bright nature of the lens combined with the high relative lens-source motion, $\mu=6.94\pm 0.50\ {\rm mas}\ {\rm yr}^{-1}$, suggests that the lens can be directly observed from future high-resolution follow-up observations., Comment: 9 pages, 9 figures

Published
2019
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28. PSIII-42 Effects of non-genetically modified organism wheat on growth performance, nutrient digestibility, blood profile and meat quality in grower-finisher pigs

Author

D J Lee, Huan Wang, Hong Ik Jung, and I. H. Kim

Subjects
Nutrient digestibility, Abstracts, media_common.quotation_subject, Genetics, food and beverages, Animal Science and Zoology, Quality (business), General Medicine, Food science, Biology, Food Science, media_common, Genetically modified organism
Abstract

With the continuous development of animal husbandry, alternative low cost and safety feed ingredient such as non-genetically modified organism wheat (non-GMO) is being researched as a source of energy as well as other nutrients to replace certain amount of corn in the diet. This study was conducted to determine the effects of dietary non-GMO wheat-based diets on growth performance, nutrient digestibility, fecal score, blood profile and meat quality of grower-finisher pigs. A total of 70 [(Landrace × Yorkshire) × Duroc] growing pigs with an initial body weight of 26.15 ± 1.57 kg were used in a 112 days study. Dietary treatments were as follows: (I) CD, corn-based diet；(II) non-GMO WD, non-genetically modified organism wheat-based diet (completely wheat based diet). Each treatment consisted of 7 replicate pens with 5 pigs per pen. All data were statistically analyzed using the GLM procedure of the SAS program (SAS Inst. Inc., Cary, NC, USA). In the current study, pigs fed corn-based diet had higher body weight than pigs fed non-GMO wheat-based diet atday 21（38.93 kg，38.32 kg，respectively，p=0.042） and day77(81.54 kg，49.54 kg，respectively，p=0.036). There was a significant difference in average daily gain (ADG) during 0-21days(608 kg，580 kg，respectively，p=0.047), but there was no difference in overall ADG. In addition, non-GMO wheat-based diet were no effects on protein, blood urea nitrogen (BUN), creatinine, and glucose except for BUN at day 21 on blood profile. In conclusion, non-GMO wheat-based diet had no significant impact on the growth performance, nutrient digestibility, blood profile and meat quality of pigs during the grower-finisher period. Non-GMO wheat-based diet appears to be aviable possible alternative to basal diet in Grower-Finisher pigs.

Published
2018

29. Development of a collective scattering system and its application to the measurement of multiscale fluctuations in KSTAR plasmas

Author

W Lee, D J Lee, H K Park, Y U Nam, T-G Lee, M J Choi, H-J Ahn, H-K Park, Y-S Na, and M S Park

Subjects
Physics, Nuclear Energy and Engineering, Scattering, KSTAR, Plasma, Condensed Matter Physics, Computational physics
Abstract

A four-channel collective scattering system (CSS) has been developed to extend the current turbulence measurement capability (poloidal wavenumber < 3 cm−1) beyond the ion gyroscale in the KSTAR tokamak. By utilizing a 300 GHz probe beam and four-channel detector array, the CSS can measure electron density fluctuations of four distinct poloidal wavenumbers from 14 to 26 cm−1 at a high sampling rate (typically 10 MS s−1). In between discharges the radial measurement location can be varied from the plasma center to the outer edge with the remote control of the optical system. In this paper, the details of the major components and laboratory evaluation of the optical system are described. Several initial measurements such as (1) the broadband turbulence reduction during L–H transition, (2) the broadband turbulence increase in H-mode when the amplitude of edge-localized mode crashes is reduced by increased density, (3) the amplification of a quasi-coherent mode by additional heating in high-performance H-mode, and (4) the appearance of high-frequency magnetohydro-dynamical modes during slow L–H transition, are briefly presented. The possibility of the CSS as a hybrid system (of a scattering system and fluctuation interferometer), which complicates the interpretation of the CSS data, is also discussed.

Published
2021

30. Effect of chemical doping on the visible emission in Cu ions doped perovskite zirconates

Author

Y. S. Lee and D. J. Lee

Subjects
Materials science, Ionic radius, Doping, Analytical chemistry, General Physics and Astronomy, 02 engineering and technology, Chemical disorder, 010402 general chemistry, 021001 nanoscience & nanotechnology, 0210 nano-technology, 01 natural sciences, 0104 chemical sciences, Electronic properties
Abstract

We investigated the effect of the chemical doping on the visible emission of the Cu-ion-doped perovskite zirconates. We synthesized the Cu-ion-doped Sr1−x Ca x ZrO3 (SCZO:Cu) compounds (x = 0 − 1), where the structural distortion and the chemical disorder were tuned due to the ionic size difference between Sr2+ and Ca2+. The nominal doping concentration of Cu ion was chosen to be 1%. We found that the visible emission in SCZO:Cu was suppressed dramatically with the substitution of Ca2+ for Sr2+ (x > 0). The violet emission was more susceptible to the structural distortion than the orange and the green emissions. These experimental findings were discussed in relation to the electronic properties of SCZO:Cu.

Published
2016

31. Gender and laterality in semicircular canal dehiscence syndrome

Author

S Lookabaugh, K Karimnejad, Anthony A. Mikulec, D J Lee, and M S Czerny

Subjects
Adult, Male, medicine.medical_specialty, Adolescent, Hearing Loss, Conductive, Dentistry, Dehiscence, Medical care, Functional Laterality, Young Adult, 03 medical and health sciences, Sex Factors, 0302 clinical medicine, Chart review, otorhinolaryngologic diseases, medicine, Humans, Statistical analysis, In patient, Child, 030223 otorhinolaryngology, Aged, Aged, 80 and over, Semicircular canal, business.industry, General Medicine, Middle Aged, Semicircular Canals, Surgery, medicine.anatomical_structure, Otorhinolaryngology, Child, Preschool, Cerebral hemisphere, Laterality, Vertigo, Female, sense organs, business, 030217 neurology & neurosurgery
Abstract

Objective:To determine if there is gender or laterality predilection in patients with semicircular canal dehiscence syndrome.Methods:A multi-institutional chart review was performed to identify patients diagnosed with semicircular canal dehiscence between 2000 and 2015. A systematic literature search was conducted using PubMed to further identify patients with semicircular canal dehiscence. Age, gender and laterality data were collected. Statistical analysis was performed to evaluate for gender or laterality preponderance.Results:A total of 682 patients with semicircular canal dehiscence were identified by literature and chart review. Mean age of diagnosis was 49.75 years (standard deviation = 15.33). Semicircular canal dehiscence was associated with a statistically significant female predominance (chi-square = 7.185, p = 0.007); the female-to-male ratio was 1.2 to 1. Left-sided semicircular canal dehiscence was most common, followed by right-sided then bilateral (chi-square = 23.457, p < 0.001).Conclusion:Semicircular canal dehiscence syndrome is most commonly left-sided and exhibits a female predominance. This may be secondary to morphological cerebral hemisphere asymmetries in both sexes and a predilection of women to seek more medical care than men.

Published
2016

32. One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953

Author

Martin Donachie, Clément Ranc, Naoki Koshimoto, Weicheng Zang, In-Gu Shin, Yoon-Hyun Ryu, Michael D. Albrow, Sun-Ju Chung, Shota Miyazaki, Akihiko Fukui, Daisuke Suzuki, Cheongho Han, Doeon Kim, Ian A. Bond, Tsubasa Yamawaki, Seung-Lee Kim, Jennifer C. Yee, Richard K. Barry, Richard W. Pogge, Yutaka Matsubara, Haruno Suematsu, Man Cheung Alex Li, Woong-Tae Kim, Masayuki Nagakane, Sang-Mok Cha, Hikaru Shoji, Andrew Gould, Rintaro Kirikawa, Yuzuru Tanaka, Dong-Jin Kim, Byeong-Gon Park, Paul J. Tristram, Nicholas J. Rattenbury, Fumio Abe, Hirosane Fujii, D. J. Lee, Kyu-Ha Hwang, Yuki Satoh, Takahiro Sumi, Chung-Uk Lee, Yuki Hirao, Aparna Bhattacharya, Iona Kondo, David P. Bennett, Yoshitaka Itow, Youn Kil Jung, Hyoun-Woo Kim, Yasushi Muraki, Yongseok Lee, Atsunori Yonehara, and Yossi Shvartzvald

Subjects
Earth and Planetary Astrophysics (astro-ph.EP), Physics, 010504 meteorology & atmospheric sciences, Event (relativity), FOS: Physical sciences, Magnification, Astronomy, Astronomy and Astrophysics, Gravitational microlensing, Astrophysics - Astrophysics of Galaxies, 01 natural sciences, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Planet, Astrophysics of Galaxies (astro-ph.GA), 0103 physical sciences, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics - Earth and Planetary Astrophysics, 0105 earth and related environmental sciences, Ultra sensitive
Abstract

We present the analysis of a very high-magnification ($A\sim 900$) microlensing event KMT-2019-BLG-1953. A single-lens single-source (1L1S) model appears to approximately delineate the observed light curve, but the residuals from the model exhibit small but obvious deviations in the peak region. A binary lens (2L1S) model with a mass ratio $q\sim 2\times 10^{-3}$ improves the fits by $\Delta\chi^2=181.8$, indicating that the lens possesses a planetary companion. From additional modeling by introducing an extra planetary lens component (3L1S model) and an extra source companion (2L2S model), it is found that the residuals from the 2L1S model further diminish, but claiming these interpretations is difficult due to the weak signals with $\Delta\chi^2=16.0$ and $13.5$ for the 3L1S and 2L2L models, respectively. From a Bayesian analysis, we estimate that the host of the planets has a mass of $M_{\rm host}=0.31^{+0.37}_{-0.17}~M_\odot$ and that the planetary system is located at a distance of $D_{\rm L}=7.04^{+1.10}_{-1.33}~{\rm kpc}$ toward the Galactic center. The mass of the securely detected planet is $M_{\rm p}=0.64^{+0.76}_{-0.35}~M_{\rm J}$. The signal of the potential second planet could have been confirmed if the peak of the light curve had been more densely observed by followup observations, and thus the event illustrates the need for intensive followup observations for very high-magnification events even in the current generation of high-cadence surveys., Comment: 10 pages, 9 figures

Published
2020

33. OGLE-2017-BLG-0329L: A Microlensing Binary Characterized with Dramatically Enhanced Precision Using Data from Space-based Observations

Author

Christiane Helling, Jennifer C. Yee, Sedighe Sajadian, D. J. Lee, Richard W. Pogge, Stephen C. Lowry, Byeong-Gon Park, Yoon-Hyun Ryu, Shinyoung Kim, Patryk Iwanek, Tobias C. Hinse, B. S. Gaudi, Krzysztof Ulaczyk, Igor Soszyński, Andrew Gould, Weicheng Zang, Sohrab Rahvar, Dong-Jin Kim, Geoffrey Bryden, Charles A. Beichman, Radosław Poleski, Kyu-Ha Hwang, Jan Skowron, In-Gu Shin, S. Kozłowski, Paweł Pietrukowicz, S. Calchi Novati, Sang-Mok Cha, Calen B. Henderson, Chang S. Han, Michael D. Albrow, U. G. Jørgensen, Daniel F. Evans, Yossi Shvartzvald, Martin Dominik, Colin Snodgrass, Przemek Mróz, J. Campbell-White, Woong-Tae Kim, M. Hundertmark, C.-U. Lee, Hyo-Ryoung Kim, Martin Burgdorf, Krzysztof A. Rybicki, Valerio Bozza, Wei Zhu, Markus Rabus, Sean Carey, S. J. Chung, Andrzej Udalski, Michał K. Szymański, Yongseok Lee, Youn Kil Jung, Simona Ciceri, Lauri K. Haikala, M. Pawlak, Penélope Longa-Peña, University of St Andrews. School of Physics and Astronomy, and University of St Andrews. St Andrews Centre for Exoplanet Science

Subjects
010504 meteorology & atmospheric sciences, FOS: Physical sciences, Binary number, Astrophysics, gravitational lensing: micro, Space (mathematics), Gravitational microlensing, 01 natural sciences, micro [Gravitational lensing], Einstein radius, Gravitation, 0103 physical sciences, QB460, QB Astronomy, 010303 astronomy & astrophysics, QC, Solar and Stellar Astrophysics (astro-ph.SR), QB, 0105 earth and related environmental sciences, Physics, general [Binaries], DAS, Astronomy and Astrophysics, binaries: general, Space and Planetary Science, QC Physics, Astrophysics - Solar and Stellar Astrophysics, Caustic (optics), Degeneracy (mathematics), Parallax
Abstract

Mass measurements of gravitational microlenses require one to determine the microlens parallax $\pie$, but precise $\pie$ measurement, in many cases, is hampered due to the subtlety of the microlens-parallax signal combined with the difficulty of distinguishing the signal from those induced by other higher-order effects. In this work, we present the analysis of the binary-lens event OGLE-2017-BLG-0329, for which $\pie$ is measured with a dramatically improved precision using additional data from space-based $Spitzer$ observations. We find that while the parallax model based on the ground-based data cannot be distinguished from a zero-$\pie$ model at 2$\sigma$ level, the addition of the $Spitzer$ data enables us to identify 2 classes of solutions, each composed of a pair of solutions according to the well-known ecliptic degeneracy. It is found that the space-based data reduce the measurement uncertainties of the north and east components of the microlens-parallax vector $\pivec_{\rm E}$ by factors $\sim 18$ and $\sim 4$, respectively. With the measured microlens parallax combined with the angular Einstein radius measured from the resolved caustic crossings, we find that the lens is composed of a binary with components masses of either $(M_1,M_2)\sim (1.1,0.8)\ M_\odot$ or $\sim (0.4,0.3)\ M_\odot$ according to the two solution classes. The first solution is significantly favored but the second cannot be securely ruled out based on the microlensing data alone. However, the degeneracy can be resolved from adaptive optics observations taken $\sim 10$ years after the event., Comment: 9 pages, 4 tables, 6 figures

Published
2018

34. Towards nano-patterned perovskite layers for enhanced absorption in solar cells

Author

A. Assadillayev, D. J. Lee, Uli Lemmer, Somayeh Moghadamzadeh, Bryce S. Richards, Raphael Schmager, Philipp Brenner, Ulrich W. Paetzold, Tobias Abzieher, and Ihteaz M. Hossain

Subjects
Materials science, business.industry, 02 engineering and technology, 010402 general chemistry, 021001 nanoscience & nanotechnology, 01 natural sciences, 0104 chemical sciences, Active layer, Photovoltaics, Nano, Optoelectronics, Thin film, 0210 nano-technology, business, Absorption (electromagnetic radiation), Layer (electronics), Lithography, Perovskite (structure)
Abstract

Organo-metal halide perovskites have revolutionized thin film photovoltaics by their outstanding performance improvements over the last years. Modifying the active layer by thermal nano-imprint lithography enables a great opportunity to modify and further enhance the optical properties. During the imprint, the perovskite layer changes tremendously. Crystal sizes and structure can be controlled by different molds, pressure and heat. Most importantly, the ability to transfer two-dimensional photonic structures inside the active layer enables enhanced photon absorption in the weakly absorbing wavelength region of thin perovskites.

Published
2018

35. The KMTNet/K2-C9 (Kepler) Data Release

Author

C. Han, Hyoun-Woo Kim, Sang-Mok Cha, Andrew Gould, Yongseok Lee, W. Zang, K. H. Hwang, Seung-Lee Kim, Michael D. Albrow, Yossi Shvartzvald, Dong-Jin Kim, D. J. Lee, Chung-Uk Lee, In-Gu Shin, Wei Zhu, Richard W. Pogge, Yoon-Hyun Ryu, Jennifer C. Yee, Youn Kil Jung, B. G. Park, and S. J. Chung

Subjects
Physics, Earth and Planetary Astrophysics (astro-ph.EP), 010504 meteorology & atmospheric sciences, Astronomy, FOS: Physical sciences, Astronomy and Astrophysics, 01 natural sciences, Kepler, Space and Planetary Science, 0103 physical sciences, 010303 astronomy & astrophysics, Data release, 0105 earth and related environmental sciences, Astrophysics - Earth and Planetary Astrophysics
Abstract

We present Korea Microlensing Telescope Network (KMTNet) light curves for microlensing-event candidates in the Kepler K2 C9 field having peaks within 3 effective timescales of the Kepler observations. These include 181 "clear microlensing" and 84 "possible microlensing" events found by the KMTNet event finder, plus 56 other events found by OGLE and/or MOA that were not found by KMTNet. All data for the first two classes are immediately available for public use without restriction., Submitted AAS Journals, 10 pages, 1 Figure. Lightcurves are available at http://kmtnet.kasi.re.kr/ulens/

Published
2018

36. Two Jupiter-Mass Planets Discovered by the KMTNet Survey in 2017

Author

Hyoun-Woo Kim, Kyu-Ha Hwang, Cheongho Han, Seung-Lee Kim, Jennifer C. Yee, D.-J. Kim, Yossi Shvartzvald, Yongseok Lee, Byeong-Gon Park, Michael D. Albrow, In-Gu Shin, C.-U. Lee, Youn Kil Jung, Andrew Gould, Weicheng Zang, D. J. Lee, S. J. Chung, Sang-Mok Cha, Richard W. Pogge, and Yoon-Hyun Ryu

Subjects
Physics, Earth and Planetary Astrophysics (astro-ph.EP), 010504 meteorology & atmospheric sciences, Gas giant, Star (game theory), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Planetary system, Gravitational microlensing, 01 natural sciences, Stars, 13. Climate action, Space and Planetary Science, Planet, Bulge, 0103 physical sciences, 010303 astronomy & astrophysics, Jupiter mass, Astrophysics - Earth and Planetary Astrophysics, 0105 earth and related environmental sciences
Abstract

We report two microlensing events, KMT-2017-BLG-1038 and KMT-2017-BLG-1146 that are caused by planetary systems. These events were discovered by KMTNet survey observations from the $2017$ bulge season. The discovered systems consist of a planet and host star with mass ratios, $5.3_{-0.4}^{+0.2} \times 10^{-3}$ and $2.0_{-0.1}^{+0.6} \times 10^{-3}$, respectively. Based on a Bayesian analysis assuming a Galactic model without stellar remnant hosts, we find that the planet, KMT-2017-BLG-1038Lb, is a super Jupiter-mass planet ($M_{\rm p}= 2.04_{-1.15}^{+2.02}\,M_{\rm J}$) orbiting a mid-M dwarf host ($M_{\rm h}= 0.37_{-0.20}^{+0.36}\, M_{\odot}$) that is located at $6.01_{-1.72}^{+1.27}$ kpc toward the Galactic bulge. The other planet, KMT-2017-BLG-1146Lb, is a sub Jupiter-mass planet ($M_{\rm p}= 0.71_{-0.42}^{+0.80}\,M_{\rm J}$) orbiting a mid-M dwarf host ($M_{\rm h}= 0.33_{-0.20}^{+0.36}\,M_{\odot}$) at a distance toward the Galactic bulge of $6.50_{-2.00}^{+1.38}$ kpc. Both are potentially gaseous planets that are beyond their hosts' snow lines. These typical microlensing planets will be routinely discovered by second-generation microlensing surveys, rapidly increasing the number of detections., Comment: 8 pages, 10 figures, 2 tables, accepted for publication in AJ

Published
2018
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37. Characterizations of dissimilar friction welding of ST37 and CK60 steels

Author

E. Y. Yoon, H. S. Kim, M. Azizieh, M. Khamisi, and D. J. Lee

Subjects
010302 applied physics, Toughness, Materials science, Mechanical Engineering, Metallurgy, Charpy impact test, 02 engineering and technology, Welding, 021001 nanoscience & nanotechnology, Microstructure, 01 natural sciences, Industrial and Manufacturing Engineering, Computer Science Applications, law.invention, Control and Systems Engineering, law, 0103 physical sciences, Ultimate tensile strength, Fracture (geology), Friction welding, 0210 nano-technology, Joint (geology), Software
Abstract

The aim of the current work is to study the effect of friction welding parameters such as joint design and rotational speed on the microstructure and mechanical properties of ST37 steel to CK60 steel joints. The tensile strength of the joints was determined using notch tensile tests. The hardness was measured across and perpendicular to the interface. Weld toughness was measured using Charpy impact tests. The results of notch tensile tests indicate that the strength of the weld zone is between those of the two components. The toughness of the weld zone was lower than both base materials. The fracture surface showed cleavage features. The round head samples had better results than for the flat ones.

Published
2015

39. OGLE-2015-BLG-1459L: The Challenges of Exo-Moon Microlensing

Author

Yoon-Hyun Ryu, Richard W. Pogge, Yutaka Matsubara, K. H. Hwang, Wei Zhu, Youn Kil Jung, Szymon Kozłowski, T. Yamada, Sang-Mok Cha, David P. Bennett, Shinyoung Kim, Takahiro Sumi, Kohei Kawasaki, Paweł Pietrukowicz, Dong-Jin Kim, Ian A. Bond, Paul J. Tristram, Byeong-Gon Park, Yoshitaka Itow, Phil Evans, Masayuki Nagakane, Martin Donachie, Denis J. Sullivan, Richard Barry, Aparna Bhattacharya, Igor Soszyński, Hyoun-Woo Kim, Yasushi Muraki, Fumio Abe, Nicholas J. Rattenbury, Jan Skowron, Yongseok Lee, Atsunori Yonehara, In-Gu Shin, Yuki Hirao, Radek Poleski, Shota Miyazaki, Akihiko Fukui, C. H. Ling, Kimiaki Masuda, Daisuke Suzuki, D. J. Lee, Michał Pawlak, Michael D. Albrow, Przemek Mróz, S. J. Chung, Andrew Gould, Clément Ranc, Yuichiro Asakura, Andrzej Udalski, Michał K. Szymański, A. Sharan, C. Han, Jennifer C. Yee, Krzysztof Ulaczyk, To. Saito, C.-U. Lee, Man Cheung Alex Li, K. Ohnishi, and Naoki Koshimoto

Subjects
Earth and Planetary Astrophysics (astro-ph.EP), Physics, 010504 meteorology & atmospheric sciences, FOS: Physical sciences, Library science, Astronomy and Astrophysics, gravitational lensing: micro, Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational microlensing, 01 natural sciences, Space and Planetary Science, 0103 physical sciences, Astrophysics::Earth and Planetary Astrophysics, Space Science, planetary systems, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, Astrophysics - Earth and Planetary Astrophysics
Abstract

著者人数: 61名ほか (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 鈴木, 大介), Accepted: 2018-05-02, 資料番号: SA1180047000

Published
2017

40. List of Contributors

Author

A. Asghar, N. Balagurusamy, E.R. Bandala, A. Buthiyappan, P. Champagne, C.-C. Chen, W.M.A.W. Daud, A. Daverey, C. Fu, V. Gadhamshetty, M. García Lozano, B.D. Gebrewold, B. Giri, J.-D. Gu, W. Guo, F.I. Hai, B.S. Herath, M. Howell, S. Hu, G. Kastl, S.K. Khanal, M. Kumar, C.-H. Lay, D.-J. Lee, C.-Y. Lin, J.-G. Lin, J.C. Liu, L. Liu, S.L. Low, Y. Lu, L.E. Montañez Hernandez, P. Mullai, H.Y. Ng, K.K. Ng, L.D. Nghiem, H.H. Ngo, S. Nitayavardhana, R. Oropeza Navarro, K. Pakshirajan, Y. Peña Garcia, W.E. Price, G. Qiu, A.A.A. Raman, M.E. Raynal Gutierrez, E.R. Rene, J.L. Sanchez-Salas, A. Sathasivan, S.T.M.L.D. Senevirathna, X. Shi, K.-Y. Show, Y. Song, D.S. Srinivasa Raghavan, S. Su, M.M. Tejas Namboodiri, R. Thiruvenkatachari, Y.-P. Ting, T.P. Tram Vo, J. Virkutyte, S. Vishali, R. Wickham, and M.K. Yogeswari

Published
2017

41. Measurement of the transverse momentum spectra of weak vector bosons produced in proton-proton collisions at root s=8TeV

Author

Khachatryan, V. Sirunyan, A. M. Tumasyan, A. Adam, W. and Asilar, E. Bergauer, T. Brandstetter, J. Brondolin, E. and Dragicevic, M. Eroe, J. Flechl, M. Friedl, M. and Fruehwirth, R. Ghete, V. M. Hartl, C. Hoermann, N. and Hrubec, J. Jeitler, M. Koenig, A. Krammer, M. and Kraetschmer, I. Liko, D. Matsushita, T. Mikulec, I. and Rabady, D. Rad, N. Rahbaran, B. Rohringer, H. Schieck, J. Schoefbeck, R. Strauss, J. Treberer-Treberspurg, W. and Waltenberger, W. Wulz, C. -E. Mossolov, V. Shumeiko, N. and Gonzalez, J. Suarez Alderweireldt, S. Cornelis, T. De Wolf, E. A. Janssen, X. Knutsson, A. Lauwers, J. Luyckx, S. and Van De Klundert, M. Van Haevermaet, H. Van Mechelen, P. and Van Remortel, N. Van Spilbeeck, A. Abu Zeid, S. Blekman, F. and D'Hondt, J. Daci, N. De Bruyn, I. Deroover, K. and Heracleous, N. Keaveney, J. Lowette, S. Moortgat, S. and Moreels, L. Olbrechts, A. Python, Q. Strom, D. and Tavernier, S. Van Doninck, W. Van Mulders, P. Van Parijs, I. and Brun, H. Caillol, C. Clerbaux, B. De Lentdecker, G. and Fasanella, G. Favart, L. Goldouzian, R. Grebenyuk, A. and Karapostoli, G. Lenzi, T. Leonard, A. Maerschalk, T. and Marinov, A. Randle-conde, A. Seva, T. Vander Velde, C. and Vanlaer, P. Yonamine, R. Zenoni, F. Zhang, F. Benucci, L. Cimmino, A. Crucy, S. Dobur, D. Fagot, A. Garcia, G. Gul, M. Mccartin, J. Rios, A. A. Ocampo Poyraz, D. and Ryckbosch, D. Salva, S. Sigamani, M. Tytgat, M. Van Driessche, W. Yazgan, E. Zaganidis, N. Basegmez, S. and Beluffi, C. Bondu, O. Brochet, S. Bruno, G. Caudron, A. and Ceard, L. De Visscher, S. Delaere, C. Delcourt, M. and Favart, D. Forthomme, L. Giammanco, A. Jafari, A. Jez, P. Komm, M. Lemaitre, V. Mertens, A. Musich, M. and Nuttens, C. Piotrzkowski, K. Quertenmont, L. Selvaggi, M. and Marono, M. Vidal Beliy, N. Hammad, G. H. Alda Junior, W. L. Alves, F. L. Alves, G. A. Brito, L. Correa Martins Junior, M. Hamer, M. Hensel, C. Moraes, A. Pol, M. E. and Rebello Teles, P. Belchior Batista Das Chagas, E. Carvalho, W. Chinellato, J. Custodio, A. Da Costa, E. M. De Jesus Damiao, D. De Oliveira Martins, C. Fonseca De Souza, S. and Huertas Guativa, L. M. Malbouisson, H. Matos Figueiredo, D. and Mora Herrera, C. Mundim, L. Nogima, H. Prado Da Silva, W. L. and Santoro, A. Sznajder, A. Tonelli Manganote, E. J. Vilela Pereira, A. Ahuja, S. Bernardes, C. A. Santos, A. De Souza and Dogra, S. Fernandez Perez Tomei, T. R. Gregores, E. M. and Mercadante, P. G. Moon, C. S. Novaes, S. F. Padula, Sandra S. Romero Abad, D. Ruiz Vargas, J. C. Aleksandrov, A. and Hadjiiska, R. Iaydjiev, P. Rodozov, M. Stoykova, S. and Sultanov, G. Vu-tova, M. Dimitrov, A. Glushkov, I. and Litov, L. Pavlov, B. Petkov, P. Fang, W. Ahmad, M. and Bian, J. G. Chen, G. M. Chen, H. S. Chen, M. Cheng, T. and Du, R. Jiang, C. H. Leggat, D. Plestina, R. Romeo, F. Shaheen, S. M. Spiezia, A. Tao, J. Wang, C. Wang, Z. Zhang, H. Asawatangtrakuldee, C. Ban, Y. Li, Q. and Liu, S. Mao, Y. Qian, S. J. Wang, D. Xu, Z. Avila, C. Cabrera, A. Chaparro Sierra, L. F. Florez, C. Gomez, J. P. Gomez Moreno, B. Sanabria, J. C. Godinovic, N. and Lelas, D. Puljak, I. Ribeiro Cipriano, P. M. Antunovic, Z. and Kovac, M. Brigljevic, V. Ferencek, D. Kadija, K. and Luetic, J. Micanovic, S. Sudic, L. Attikis, A. and Mavromanolakis, G. Mousa, J. Nicolaou, C. Ptochos, F. and Razis, P. A. Rykaczewski, H. Finger, M. Finger, Jr., M. and Carrera Jarrin, E. Awad, A. Elgammal, S. Mohamed, A. and Salama, E. Calpas, B. Kadastik, M. Murumaa, M. Perrini, L. Raidal, M. Tiko, A. Veelken, C. Eerola, P. and Pekkanen, J. Voutilainen, M. Harkonen, J. Karimaki, V. and Kinnunen, R. Lampen, T. Lassila-Perini, K. Lehti, S. and Linden, T. Luukka, P. Peltola, T. Tuominiemi, J. and Tuovinen, E. Wendland, L. Talvitie, J. Tuuva, T. and Besancon, M. Couderc, F. Dejardin, M. Denegri, D. and Fabbro, B. Faure, J. L. Favaro, C. Ferri, F. Ganjour, S. and Givernaud, A. Gras, P. de Monchenault, G. Hamel Jarry, P. Locci, E. Machet, M. Malcles, J. Rander, J. and Rosowsky, A. Titov, M. Zghiche, A. Abdulsalam, A. and Antropov, I. Baffioni, S. Beaudette, F. Busson, P. and Cadamuro, L. Chapon, E. Charlot, C. Davignon, O. de Cassagnac, R. Granier Jo, M. Lisniak, S. Mine, P. and Naranjo, I. N. Nguyen, M. Ochando, C. Ortona, G. and Paganini, P. Pigard, P. Regnard, S. Salerno, R. Sirois, Y. Strebler, T. Yilmaz, Y. Zabi, A. Agram, J. -L. and Andrea, J. Aubin, A. Bloch, D. Brom, J. -M. Buttignol, M. Chabert, E. C. Chanon, N. Collard, C. Conte, E. and Coubez, X. Fontaine, J. -C. Gele, D. Goerlach, U. and Goetzmann, C. Le Bihan, A. -C. Merlin, J. A. Skovpen, K. and Van Hove, P. Gadrat, S. Beauceron, S. Bernet, C. and Boudoul, G. Bouvier, E. Montoya, C. A. Carrillo Chierici, R. and Contardo, D. Courbon, B. Depasse, P. El Mamouni, H. and Fan, J. Fay, J. Gascon, S. Gouze-vitch, M. Ille, B. and Lagarde, F. Laktineh, I. B. Lethuillier, M. Mirabito, L. and Pequegnot, A. L. Perries, S. Popov, A. Alvarez, J. D. Ruiz and Sabes, D. Sordini, V. Vander Donckt, M. Verdier, P. and Viret, S. Khvedelidze, A. Tsamalaidze, Z. Autermann, C. and Beranek, S. Feld, L. Heister, A. Kiesel, M. K. Klein, K. and Lipinski, M. Ostapchuk, A. Preuten, M. Raupach, F. and Schael, S. Schulte, J. F. Verlage, T. Weber, H. Zhukov, V. Ata, M. Brodski, M. Dietz-Laursonn, E. Duchardt, D. and Endres, M. Erdmann, M. Erdweg, S. Esch, T. Fischer, R. Gueth, A. Hebbeker, T. Heidemann, C. Hoepfner, K. and Knutzen, S. Merschmeyer, M. Meyer, A. Millet, P. and Mukherjee, S. Olschewski, M. Padeken, K. Papacz, P. and Pook, T. Radziej, M. Reithler, H. Rieger, M. Scheuch, F. and Sonnenschein, L. Teyssier, D. Thueer, S. Cherepanov, V. and Erdogan, Y. Fluegge, G. Geenen, H. Geisler, M. and Hoehle, F. Kargoll, B. Kress, T. Kuensken, A. Lingemann, J. Nehrkorn, A. Nowack, A. Nugent, I. M. Pistone, C. and Pooth, O. Stahl, A. Martin, M. Aldaya Asin, I. and Beernaert, K. Behnke, O. Behrens, U. Borras, K. and Burgmeier, A. Campbell, A. Contreras-Campana, C. Costanza, F. Pardos, C. Diez Dolinska, G. Dooling, S. Eckerlin, G. and Eckstein, D. Eichhorn, T. Gallo, E. Garcia, J. Garay and Geiser, A. Gizhko, A. Gunnellini, P. Harb, A. Hauk, J. and Hempel, M. Jung, H. Kalogeropoulos, A. Karacheban, O. and Kasemann, M. Katsas, P. Kieseler, J. Kleinwort, C. and Korol, I. Lange, W. Leonard, J. Lipka, K. Lobanov, A. and Lohmann, W. Mankel, R. Melzer-Pellmann, I. -A. Meyer, A. B. Mittag, G. Mnich, J. Mussgiller, A. Ntomari, E. and Pitzl, D. Placakyte, R. Raspereza, A. Roland, B. Sahin, M. Oe. Saxena, P. Schoerner-Sadenius, T. Seitz, C. and Spannagel, S. Stefaniuk, N. Trippkewitz, K. D. Van Onsem, G. P. Walsh, R. Wissing, C. Blobel, V. Vignali, M. Centis and Draeger, A. R. Dreyer, T. Erfle, J. Garutti, E. and Goebel, K. Gonzalez, D. Goerner, M. Haller, J. Hoffmann, M. Hoeing, R. S. Junkes, A. Klanner, R. Kogler, R. and Kovalchuk, N. Lapsien, T. Lenz, T. Marchesini, I. and Marconi, D. Meyer, M. Niedziela, M. Nowatschin, D. Ott, J. Pantaleo, F. Peiffer, T. Perieanu, A. Pietsch, N. and Poehlsen, J. Sander, C. Scharf, C. Schleper, P. and Schlieckau, E. Schmidt, A. Schumann, S. Schwandt, J. and Stadie, H. Steinbrueck, G. Stober, F. M. Tholen, H. and Troendle, D. Usai, E. Vanelderen, L. Vanhoefer, A. and Vormwald, B. Barth, C. Baus, C. Berger, J. Boeser, C. and Butz, E. Chwalek, T. Colombo, F. De Boer, W. and Descroix, A. Dierlamm, A. Fink, S. Frensch, F. Friese, R. Giffels, M. Gilbert, A. Haitz, D. Hartmann, F. and Heindl, S. M. Husemann, U. Katkov, I. Kornmayer, A. and Pardo, P. Lobelle Maier, B. Mildner, H. Mozer, M. U. and Mueller, T. Mueller, Th. Plagge, M. Quast, G. Rabbertz, K. Roecker, S. Roscher, F. Schroeder, M. Sieber, G. and Simonis, H. J. Ulrich, R. Wagner-Kuhr, J. Wayand, S. and Weber, M. Weiler, T. Williamson, S. Woehrmann, C. Wolf, R. Anagnostou, G. Daskalakis, G. Geralis, T. and Giakoumopoulou, V. A. Kyriakis, A. Loukas, D. Psallidas, A. and Topsis-Giotis, I. Agapitos, A. Kesisoglou, S. and Panagiotou, A. Saoulidou, N. Tziaferi, E. Evangelou, I. and Flouris, G. Foudas, C. Kokkas, P. Loukas, N. Manthos, N. and Papadopoulos, I. Paradas, E. Strologas, J. Filipovic, N. and Bencze, G. Hajdu, C. Hidas, P. Horvath, D. Sikler, F. Veszpremi, V. Vesztergombi, G. Zsigmond, A. J. Beni, N. Czellar, S. Karancsi, J. Molnar, J. Szillasi, Z. and Bartok, M. Makovec, A. Raics, P. Trocsanyi, Z. L. and Ujvari, B. Choudhury, S. Mal, P. Mandal, K. Nayak, A. and Sahoo, D. K. Sahoo, N. Swain, S. K. Bansal, S. Beri, S. B. Bhatnagar, V. Chawla, R. Dhingra, N. Gupta, R. and Bhawandeep, U. Kalsi, A. K. Kaur, A. Kaur, M. Kumar, R. and Mehta, A. Mittal, M. Singh, J. B. Walia, G. Kumar, Ashok Bhardwaj, A. Choudhary, B. C. Garg, R. B. Keshri, S. Kumar, A. Malhotra, S. Naimuddin, M. Nishu, N. and Ranjan, K. Sharma, R. Sharma, V. Bhattacharya, R. and Bhattacharya, S. Chatterjee, K. Dey, S. Dutta, S. Ghosh, S. Majum-dar, N. Modak, A. Mondal, K. Mukhopadhyay, S. and Nandan, S. Purohit, A. Roy, A. Roy, D. Chowdhury, S. Roy Sarkar, S. Sharan, M. Chudasama, R. Dutta, D. and Jha, V. Kumar, V. Mohanty, A. K. Pant, L. M. Shukla, P. and Topkar, A. Aziz, T. Banerjee, S. Bhowmik, S. and Chatterjee, R. M. Dewanjee, R. K. Dugad, S. Gan-guly, S. and Ghosh, S. Guchait, M. Gurtu, A. Jain, Sa. Kole, G. and Kumar, S. Mahakud, B. Maity, M. Majumder, G. Mazumdar, K. Mitra, S. Mohanty, G. B. Parida, B. Sarkar, T. and Sur, N. Sutar, B. Wickramage, N. Chauhan, S. Dube, S. and Kapoor, A. Kothekar, K. Rane, A. Sharma, S. and Bakhshiansohi, H. Behnamian, H. Etesami, S. M. Fahim, A. and Khakzad, M. Najafabadi, M. Mo-hammadi Naseri, M. Mehdiabadi, S. Paktinat Hosseinabadi, F. Rezaei Safarzadeh, B. Zeinali, M. Felcini, M. Grunewald, M. Abbrescia, M. Calabria, C. and Caputo, C. Colaleo, A. Creanza, D. Cristella, L. De Filippis, N. De Palma, M. Fiore, L. Iaselli, G. Maggi, G. Maggi, M. Miniello, G. My, S. Nuzzo, S. Pompili, A. Pugliese, G. Radogna, R. Ranieri, A. Selvaggi, G. and Silvestris, L. Venditti, R. Abbiendi, G. 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Evans, A. Finkel, A. Gude, A. Hansen, P. and Kalafut, S. Kao, S. C. Klapoetke, K. Kubota, Y. and Lesko, Z. Mans, J. Nourbakhsh, S. Ruckstuhl, N. Rusack, R. Tambe, N. Turkewitz, J. Acosta, J. G. Oliveros, S. and Avdeeva, E. Bartek, R. Bloom, K. Bose, S. Claes, D. R. Dominguez, A. Fangmeier, C. Suarez, R. Gonzalez and Kamalieddin, R. Knowlton, D. Kravchenko, I. Meier, F. and Monroy, J. Ratnikov, F. Siado, J. E. Snow, G. R. and Stieger, B. Alyari, M. Dolen, J. George, J. Godshalk, A. and Harrington, C. Iashvili, I. Kaisen, J. Kharchilava, A. and Kumar, A. Parker, A. Rappoccio, S. Roozbahani, B. and Alverson, G. Barberis, E. Baumgartel, D. Chasco, M. and Hortiangtham, A. Massironi, A. Morse, D. M. Nash, D. and Orimoto, T. De Lima, R. Teixeira Trocino, D. Wang, R. -J. and Wood, D. Zhang, J. Bhattacharya, S. Hahn, K. A. and Kubik, A. Low, J. F. Mucia, N. Odell, N. Pollack, B. and Schmitt, M. H. Sung, K. Trovato, M. Velasco, M. Dev, N. and Hildreth, M. Jessop, C. Karmgard, D. J. Kellams, N. and Lannon, K. Marinelli, N. Meng, F. Mueller, C. Musienko, Y. Planer, M. Reinsvold, A. Ruchti, R. Rupprecht, N. and Smith, G. Taroni, S. Valls, N. Wayne, M. Wolf, M. and Woodard, A. Antonelli, L. Brinson, J. Bylsma, B. Durkin, L. S. Flowers, S. Hart, A. Hill, C. Hughes, R. Ji, W. Ling, T. Y. Liu, B. Luo, W. Puigh, D. Rodenburg, M. Winer, B. L. Wulsin, H. W. Driga, O. Elmer, P. and Hardenbrook, J. Hebda, P. Koay, S. A. Lujan, P. Marlow, D. Medvedeva, T. Mooney, M. Olsen, J. Palmer, C. and Piroue, P. Stickland, D. Tully, C. Zuranski, A. Malik, S. Barker, A. Barnes, V. E. Benedetti, D. Bortoletto, D. and Gutay, L. Jha, M. K. Jones, M. Jung, A. W. Jung, K. and Miller, D. H. Neumeister, N. Radburn-Smith, B. C. Shi, X. Shipsey, I. Silvers, D. Sun, J. Svyatkovskiy, A. and Wang, F. Xie, W. Xu, L. Parashar, N. Stupak, J. and Adair, A. Akgun, B. Chen, Z. Ecklund, K. M. Geurts, F. J. M. Guilbaud, M. Li, W. Michlin, B. Northup, M. and Padley, B. P. Redjimi, R. Roberts, J. Rorie, J. Tu, Z. and Zabel, J. Betchart, B. Bodek, A. de Barbaro, P. and Demina, R. Duh, Y. T. Eshaq, Y. Ferbel, T. Galanti, M. and Garcia-Bellido, A. Han, J. Hindrichs, O. and Khukhunaishvili, A. Lo, K. H. Tan, P. Verzetti, M. Chou, J. P. Contreras-Campana, E. Gershtein, Y. Halkiadakis, E. and Heindl, M. Hidas, D. Hughes, E. Kaplan, S. and Elayavalli, R. Kunnawalkam Lath, A. Nash, K. Saka, H. and Salur, S. Schnetzer, S. Sheffield, D. Somalwar, S. and Stone, R. Thomas, S. Thomassen, P. Walker, M. Foerster, M. Heideman, J. Riley, G. Rose, K. Spanier, S. and Thapa, K. Bouhali, O. Hernandez, A. Castaneda Celik, A. and Dalchenko, M. De Mattia, M. Del-gado, A. Dildick, S. and Eusebi, R. Gilmore, J. Huang, T. Kamon, T. Krutelyov, V. and Mueller, R. Osipenkov, I. Pakhotin, Y. Patel, R. and Perloff, A. Pernie, L. Rathjens, D. Rose, A. Safonov, A. and Tatarinov, A. Ulmer, K. A. Akchurin, N. Cowden, C. and Damgov, J. Dragoiu, C. Dudero, P. R. Faulkner, J. and Kunori, S. Lamichhane, K. Lee, S. W. Libeiro, T. and Undleeb, S. Volobouev, I. Wang, Z. Appelt, E. Delannoy, A. G. Greene, S. Gurrola, A. Janjam, R. Johns, W. and Maguire, C. Mao, Y. Melo, A. Ni, H. Sheldon, P. Tuo, S. Velkovska, J. Xu, Q. Arenton, M. W. Barria, P. and Cox, B. Francis, B. Goodell, J. Hirosky, R. Ledovskoy, A. Li, H. Neu, C. Sinthuprasith, T. Sun, X. Wang, Y. and Wolfe, E. Xia, F. Clarke, C. Harr, R. Karchin, P. E. and Don, C. Kottachchi Kankanamge Lamichhane, P. Sturdy, J. and Belknap, D. A. Carlsmith, D. Dasu, S. Dodd, L. Duric, S. and Gomber, B. Grothe, M. Herndon, M. Herve, A. and Klabbers, P. Lanaro, A. Levine, A. Long, K. Loveless, R. and Mohapatra, A. Ojalvo, I. Perry, T. Pierro, G. A. and Polese, G. Ruggles, T. Sarangi, T. Savin, A. Sharma, A. and Smith, N. Smith, W. H. Taylor, D. Verwilligen, P. and Woods, N. Burns, D CMS Collaboration

Subjects
High Energy Physics::Experiment, Nuclear Experiment
Abstract

The transverse momentum spectra of weak vector bosons are measured in the CMS experiment at the LHC. The measurement uses a sample of proton-proton collisions at root s = 8TeV, collected during a special low-luminosity running that corresponds to an integrated luminosity of 18: 4 +/- 0: 5 pb(-1). The production of W bosons is studied in both electron and muon decay modes, while the production of Z bosons is studied using only the dimuon decay channel. The ratios of W- to W+ and Z to W di ff erential cross sections are also measured. The measured di ff erential cross sections and ratios are compared with theoretical predictions up to next-to-next leading order in QCD.

Published
2017

42. A Neptune-mass Free-floating Planet Candidate Discovered by Microlensing Surveys

Author

Chung-Uk Lee, Richard W. Pogge, Sang-Mok Cha, Michał Pawlak, Hyoun-Woo Kim, K. H. Hwang, Jan Skowron, Andrew Gould, Igor Soszyński, Szymon Kozłowski, In-Gu Shin, Seung-Lee Kim, Youn Kil Jung, Yongseok Lee, Przemek Mróz, D. J. Lee, Paweł Pietrukowicz, K. Ulaczyk, Michael D. Albrow, Yoon-Hyun Ryu, Andrzej Udalski, Michał K. Szymański, S. J. Chung, B. G. Park, Dong-Jin Kim, C. Han, Jennifer C. Yee, Wei Zhu, and Radosław Poleski

Subjects
Physics, Earth and Planetary Astrophysics (astro-ph.EP), 010504 meteorology & atmospheric sciences, Astronomy, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational microlensing, 01 natural sciences, Space and Planetary Science, Planet, Neptune, 0103 physical sciences, Astrophysics::Earth and Planetary Astrophysics, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Astrophysics - Earth and Planetary Astrophysics, 0105 earth and related environmental sciences
Abstract

Current microlensing surveys are sensitive to free-floating planets down to Earth-mass objects. All published microlensing events attributed to unbound planets were identified based on their short timescale (below two days), but lacked an angular Einstein radius measurement (and hence lacked a significant constraint on the lens mass). Here, we present the discovery of a Neptune-mass free-floating planet candidate in the ultrashort ($t_{\rm E}=0.320\pm0.003$ days) microlensing event OGLE-2016-BLG-1540. The event exhibited strong finite-source effects, which allowed us to measure its angular Einstein radius of $\theta_{\rm E}=9.2\pm0.5\,\mu$as. There remains, however, a degeneracy between the lens mass and distance. The combination of the source proper motion and source-lens relative proper motion measurements favors a Neptune-mass lens located in the Galactic disk. However, we cannot rule out that the lens is a Saturn-mass object belonging to the bulge population. We exclude stellar companions up to 15 au., Comment: accepted to AJ

Published
2017
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43. Measurements of the t(t)over-bar production cross section in lepton plus jets final states in pp collisions at 8 and ratio of 8 to 7 cross sections

Author

Khachatryan, V. Sirunyan, A. M. Tumasyan, A. Adam, W. and Asilar, E. Bergauer, T. Brandstetter, J. Brondolin, E. and Dragicevic, M. Ero, J. Flechl, M. Friedl, M. Fruhwirth, R. Ghete, V. M. Hartl, C. Hormann, N. Hrubec, J. and Jeitler, M. Knunz, V. Konig, A. Krammer, M. Kratschmer, I. Liko, D. Matsushita, T. Mikulec, I. Rabady, D. and Rahbaran, B. Rohringer, H. Schieck, J. Schofbeck, R. and Strauss, J. Treberer-Treberspurg, W. Waltenberger, W. Wulz, C. -E. Mossolov, V. Shumeiko, N. Suarez Gonzalez, J. and Alderweireldt, S. Cornelis, T. De Wolf, E. A. Janssen, X. and Knutsson, A. Lauwers, J. Luyckx, S. Van De Klundert, M. and Van Haevermaet, H. Van Mechelen, P. Van Remortel, N. Van Spilbeeck, A. Abu Zeid, S. Blekman, F. D'Hondt, J. Daci, N. Bruyn, I. De Deroover, K. Heracleous, N. Keaveney, J. and Lowette, S. Maes, M. Moreels, L. Olbrechts, A. and Python, Q. Strom, D. Tavernier, S. Van Doninck, W. Van Mulders, P. Van Onsem, G. P. Van Parijs, I. Barria, P. and Brun, H. Caillol, C. Clerbaux, B. De Lentdecker, G. and Fasanella, G. Favart, L. Grebenyuk, A. Karapostoli, G. and Lenzi, T. Leonard, A. Maerschalk, T. Marinov, A. Pernie, L. Randle-conde, A. Reis, T. Seva, T. Vander Velde, C. and Vanlaer, P. Yonamine, R. Zenoni, F. Zhang, F. and Beernaert, K. Benucci, L. Cimmino, A. Costantini, S. and Crucy, S. Dobur, D. Fagot, A. Garcia, G. Gul, M. and Mccartin, J. Ocampo Rios, A. A. Poyraz, D. Ryckbosch, D. and Salva, S. Sigamani, M. Strobbe, N. Tytgat, M. Van Driessche, W. Yazgan, E. Zaganidis, N. Basegmez, S. and Beluffi, C. Bondu, O. Brochet, S. Bruno, G. Caudron, A. and Ceard, L. Da Silveira, G. G. Delaere, C. Favart, D. and Forthomme, L. Giammanco, A. Hollar, J. Jafari, A. Jez, P. Komm, M. Lemaitre, V. Mertens, A. Musich, M. and Nuttens, C. Perrini, L. Pin, A. Piotrzkowski, K. Popov, A. Quertenmont, L. Selvaggi, M. Vidal Marono, M. Beliy, N. Hammad, G. H. Alda Junior, W. L. Alves, F. L. Alves, G. A. Brito, L. Correa Martins Junior, M. Hamer, M. and Hensel, C. Mora Herrera, C. Moraes, A. Pol, M. E. and Rebello Teles, P. Belchior Batista Das Chagas, E. Carvalho, W. and Chinellato, J. Custodio, A. Da Costa, E. M. De Jesus Damiao, D. De Oliveira Martins, C. Fonseca De Souza, S. and Huertas Guativa, L. M. Malbouisson, H. Matos Figueiredo, D. and Mundim, L. Nogima, H. Prado Da Silva, W. L. Santoro, A. and Sznajder, A. Tonelli Manganote, E. J. Vilela Pereira, A. and Ahuja, S. Bernardes, C. A. De Souza Santos, A. Dogra, S. and Fernandez Perez Tomei, T. R. Gregores, E. M. Mercadante, P. G. and Moon, C. S. Novaes, S. F. Padula, Sandra S. Romero Abad, D. Ruiz Vargas, J. C. Aleksandrov, A. Hadjiiska, R. and Iaydjiev, P. Rodozov, M. Stoykova, S. Sultanov, G. and Vutova, M. Dimitrov, A. Glushkov, I. Litov, L. Pavlov, B. Petkov, P. Ahmad, M. Bian, J. G. Chen, G. M. and Chen, H. S. Chen, M. Cheng, T. Du, R. Jiang, C. H. and Plestina, R. Romeo, F. Shaheen, S. M. Spiezia, A. Tao, J. Wang, C. Wang, Z. Zhang, H. Asawatangtrakuldee, C. and Ban, Y. Li, Q. Liu, S. Mao, Y. Qian, S. J. Wang, D. Xu, Z. Avila, C. Cabrera, A. Chaparro Sierra, L. F. and Florez, C. Gomez, J. P. Gomez Moreno, B. Sanabria, J. C. and Godinovic, N. Lelas, D. Puljak, I. Ribeiro Cipriano, P. M. Antunovic, Z. Kovac, M. Brigljevic, V. Kadija, K. and Luetic, J. Micanovic, S. Sudic, L. Attikis, A. and Mavromanolakis, G. Mousa, J. Nicolaou, C. Ptochos, F. and Razis, P. A. Rykaczewski, H. Bodlak, M. Finger, M. and Finger, Jr., M. Abdelalim, A. A. Awad, A. El Sawy, M. and Mahrous, A. Radi, A. Calpas, B. Kadastik, M. Murumaa, M. and Raidal, M. Tiko, A. Veelken, C. Eerola, P. Pekkanen, J. Voutilainen, M. Harkonen, J. Karimaki, V. Kinnunen, R. Lampen, T. Lassila-Perini, K. Lehti, S. Linden, T. and Luukka, P. Maenpaa, T. Peltola, T. Tuominen, E. and Tuominiemi, J. Tuovinen, E. Wendland, L. Talvitie, J. and Tuuva, T. Besancon, M. Couderc, F. Dejardin, M. Denegri, D. Fabbro, B. Faure, J. L. Favaro, C. Ferri, F. and Ganjour, S. Givernaud, A. Gras, P. 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Pistone, C. Pooth, O. Stahl, A. Aldaya Martin, M. Asin, I. Bartosik, N. and Behnke, O. Behrens, U. Bell, A. J. Borras, K. Burgmeier, A. Campbell, A. Choudhury, S. Costanza, F. Diez Pardos, C. Dolinska, G. Dooling, S. Dorland, T. Eckerlin, G. and Eckstein, D. Eichhorn, T. Flucke, G. Gallo, E. Garay Garcia, J. Geiser, A. Gizhko, A. Gunnellini, P. Hauk, J. and Hempel, M. Jung, H. Kalogeropoulos, A. Karacheban, O. and Kasemann, M. Katsas, P. Kieseler, J. Kleinwort, C. and Korol, I. Lange, W. Leonard, J. Lipka, K. Lobanov, A. and Lohmann, W. Mankel, R. Marfin, I. Melzer-Pellmann, I. -A. Meyer, A. B. Mittag, G. Mnich, J. Mussgiller, A. and Naumann-Emme, S. Nayak, A. Ntomari, E. Perrey, H. Pitzl, D. Placakyte, R. Raspereza, A. Roland, B. Sahin, M. O-. and Saxena, P. Schoerner-Sadenius, T. Schroder, M. Seitz, C. and Spannagel, S. Trippkewitz, K. D. Walsh, R. Wissing, C. and Blobel, V. Centis Vignali, M. Draeger, A. R. Erfle, J. and Garutti, E. Goebel, K. Gonzalez, D. Gorner, M. and Haller, J. 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Yelton, J. Hewamanage, S. Linn, S. and Markowitz, P. Martinez, G. Rodriguez, J. L. Ackert, A. and Adams, J. R. Adams, T. Askew, A. Bochenek, J. Diamond, B. Haas, J. Hagopian, S. Hagopian, V. Johnson, K. F. and Khatiwada, A. Prosper, H. Weinberg, M. Baarmand, M. M. and Bhopatkar, V. Colafranceschi, S. Hohlmann, M. Kalakhety, H. and Noonan, D. Roy, T. Yumiceva, F. Adams, M. R. and Apanasevich, L. Berry, D. Betts, R. R. Bucinskaite, I. and Cavanaugh, R. Evdokimov, O. Gauthier, L. Gerber, C. E. and Hofman, D. J. Kurt, P. O'Brien, C. Sandoval Gonzalez, I. D. and Silkworth, C. Turner, P. Varelas, N. Wu, Z. Zakaria, M. Bilki, B. Clarida, W. Dilsiz, K. Durgut, S. and Gandrajula, R. P. Haytmyradov, M. Khristenko, V. Merlo, J. -P. Mermerkaya, H. Mestvirishvili, A. Moeller, A. and Nachtman, J. Ogul, H. Onel, Y. Ozok, F. Penzo, A. and Snyder, C. Tiras, E. Wetzel, J. Yi, K. Anderson, I. and Barnett, B. A. Blumenfeld, B. Eminizer, N. Fehling, D. and Feng, L. Gritsan, A. V. Maksimovic, P. Martin, C. and Osherson, M. Roskes, J. Sady, A. Sarica, U. Swartz, M. and Xiao, M. Xin, Y. You, C. Baringer, P. Bean, A. and Benelli, G. Bruner, C. Kenny, III, R. P. Majumder, D. and Malek, M. Murray, M. Sanders, S. Stringer, R. Wang, Q. and Ivanov, A. Kaadze, K. Khalil, S. Makouski, M. and Maravin, Y. Mohammadi, A. Saini, L. K. Skhirtladze, N. and Toda, S. Lange, D. Rebassoo, F. Wright, D. Anelli, C. and Baden, A. Baron, O. Belloni, A. Calvert, B. Eno, S. C. Ferraioli, C. Gomez, J. A. Hadley, N. J. Jabeen, S. and Kellogg, R. G. Kolberg, T. Kunkle, J. Lu, Y. and Mignerey, A. C. Shin, Y. H. Skuja, A. Tonjes, M. B. and Tonwar, S. C. Apyan, A. Barbieri, R. Baty, A. Bierwagen, K. Brandt, S. Busza, W. Cali, I. A. Demiragli, Z. Di Matteo, L. Gomez Ceballos, G. Goncharov, M. Gulhan, D. and Iiyama, Y. Innocenti, G. M. Klute, M. Kovalskyi, D. Lai, Y. S. Lee, Y. -J. Levin, A. Luckey, P. D. Marini, A. C. and Mcginn, C. Mironov, C. Narayanan, S. Niu, X. Paus, C. Ralph, D. Roland, C. Roland, G. Salfeld-Nebgen, J. and Stephans, G. S. F. Sumorok, K. Varma, M. Velicanu, D. and Veverka, J. Wang, J. Wang, T. W. Wyslouch, B. Yang, M. Zhukova, V. Dahmes, B. Evans, A. Finkel, A. Gude, A. Hansen, P. Kalafut, S. Kao, S. C. Klapoetke, K. and Kubota, Y. Lesko, Z. Mans, J. Nourbakhsh, S. Ruckstuhl, N. Rusack, R. Tambe, N. Turkewitz, J. Acosta, J. G. and Oliveros, S. Avdeeva, E. Bloom, K. Bose, S. Claes, D. R. and Dominguez, A. Fangmeier, C. Gonzalez Suarez, R. and Kamalieddin, R. Keller, J. Knowlton, D. Kravchenko, I. and Meier, F. Monroy, J. Ratnikov, F. Siado, J. E. Snow, G. R. Alyari, M. Dolen, J. George, J. Godshalk, A. and Harrington, C. Iashvili, I. Kaisen, J. Kharchilava, A. and Kumar, A. Rappoccio, S. Roozbahani, B. Alverson, G. and Barberis, E. Baumgartel, D. Chasco, M. Hortiangtham, A. and Massironi, A. Morse, D. M. Nash, D. Orimoto, T. Teixeira De Lima, R. Trocino, D. Wang, R. -J. Wood, D. Zhang, J. and Hahn, K. A. Kubik, A. Mucia, N. Odell, N. Pollack, B. Pozdnyakov, A. Schmitt, M. Stoynev, S. Sung, K. and Trovato, M. Velasco, M. Brinkerhoff, A. Dev, N. and Hildreth, M. Jessop, C. Karmgard, D. J. Kellams, N. and Lannon, K. Lynch, S. Marinelli, N. Meng, F. Mueller, C. and Musienko, Y. Pearson, T. Planer, M. Reinsvold, A. and Ruchti, R. Smith, G. Taroni, S. Valls, N. Wayne, M. and Wolf, M. Woodard, A. Antonelli, L. Brinson, J. Bylsma, B. Durkin, L. S. Flowers, S. Hart, A. Hill, C. and Hughes, R. Ji, W. Kotov, K. Ling, T. Y. Liu, B. Luo, W. Puigh, D. Rodenburg, M. Winer, B. L. Wulsin, H. W. and Driga, O. Elmer, P. Hardenbrook, J. Hebda, P. Koay, S. A. Lujan, P. Marlow, D. Medvedeva, T. Mooney, M. and Olsen, J. Palmer, C. Piroue, P. Saka, H. Stickland, D. and Tully, C. Zuranski, A. Malik, S. Barnes, V. E. and Benedetti, D. Bortoletto, D. Gutay, L. Jha, M. K. Jones, M. Jung, K. Miller, D. H. Neumeister, N. Radburn-Smith, B. C. Shi, X. Shipsey, I. Silvers, D. Sun, J. and Svyatkovskiy, A. Wang, F. Xie, W. Xu, L. Parashar, N. and Stupak, J. Adair, A. Akgun, B. Chen, Z. Ecklund, K. M. Geurts, F. J. M. Guilbaud, M. Li, W. Michlin, B. and Northup, M. Padley, B. P. Redjimi, R. Roberts, J. Rorie, J. Tu, Z. Zabel, J. Betchart, B. Bodek, A. de Barbaro, P. Demina, R. Eshaq, Y. Ferbel, T. Galanti, M. and Garcia-Bellido, A. Han, J. Harel, A. Hindrichs, O. and Khukhunaishvili, A. Petrillo, G. Tan, P. Verzetti, M. and Arora, S. Barker, A. Chou, J. P. Contreras-Campana, C. and Contreras-Campana, E. Duggan, D. Ferencek, D. Gershtein, Y. and Gray, R. Halkiadakis, E. Hidas, D. Hughes, E. and Kaplan, S. Kunnawalkam Elayavalli, R. Lath, A. Nash, K. and Panwalkar, S. Park, M. Salur, S. Schnetzer, S. and Sheffield, D. Somalwar, S. Stone, R. Thomas, S. and Thomassen, P. Walker, M. Foerster, M. Riley, G. Rose, K. and Spanier, S. York, A. Bouhali, O. Castaneda Hernandez, A. and Dalchenko, M. De Mattia, M. Delgado, A. Dildick, S. and Eusebi, R. Gilmore, J. Kamon, T. Krutelyov, V. Mueller, R. Osipenkov, I. Pakhotin, Y. Patel, R. Perloff, A. and Rose, A. Safonov, A. Tatarinov, A. Ulmer, K. A. and Akchurin, N. Cowden, C. Damgov, J. Dragoiu, C. Dudero, P. R. Faulkner, J. Kunori, S. Lamichhane, K. Lee, S. W. and Libeiro, T. Undleeb, S. Volobouev, I. Appelt, E. and Delannoy, A. G. Greene, S. Gurrola, A. Janjam, R. Johns, W. Maguire, C. Mao, Y. Melo, A. Ni, H. Sheldon, P. and Snook, B. Tuo, S. Velkovska, J. Xu, Q. Arenton, M. W. Cox, B. Francis, B. Goodell, J. Hirosky, R. and Ledovskoy, A. Li, H. Lin, C. Neu, C. Sinthuprasith, T. and Sun, X. Wang, Y. Wolfe, E. Wood, J. Xia, F. and Clarke, C. Harr, R. Karchin, P. E. Don, C. Kottachchi Kankanamge Lamichhane, P. Sturdy, J. Belknap, D. A. and Carlsmith, D. Cepeda, M. Dasu, S. Dodd, L. Duric, S. and Gomber, B. Grothe, M. Hall-Wilton, R. Herndon, M. Herve, A. Klabbers, P. Lanaro, A. Levine, A. Long, K. and Loveless, R. Mohapatra, A. Ojalvo, I. Perry, T. Pierro, G. A. Polese, G. Ruggles, T. Sarangi, T. Savin, A. and Sharma, A. Smith, N. Smith, W. H. Taylor, D. Woods, N. and CMS Collaboration

Subjects
High Energy Physics::Experiment
Abstract

A measurement of the top quark pair production () cross section in proton-proton collisions at the centre-of-mass energy of 8 is presented using data collected with the CMS detector at the LHC, corresponding to an integrated luminosity of 19.6. This analysis is performed in the decay channels with one isolated, high transverse momentum electron or muon and at least four jets, at least one of which is required to be identified as originating from hadronization of a b quark. The calibration of the jet energy scale and the efficiency of b jet identification are determined from data. The measured cross section is . This measurement is compared with an analysis of 7 data, corresponding to an integrated luminosity of 5.0, to determine the ratio of 8 to 7 cross sections, which is found to be . The measurements are in agreement with QCD predictions up to next-to-next-to-leading order.

Published
2017

47. 87 Effect of Nucleotides Supplementation to Corn Soybean Meal-Based Diet on Growth Performance, Fecal Microflora, and Blood Profiles in Sows and Their Piglets

Author

Jong-Gyu Kim, Yang Jiao, D J Lee, J Y Zhang, X X Liang, and I. H. Kim

Subjects
0301 basic medicine, chemistry.chemical_classification, 030109 nutrition & dietetics, Soybean meal, 0402 animal and dairy science, 04 agricultural and veterinary sciences, General Medicine, Biology, 040201 dairy & animal science, 03 medical and health sciences, Animal science, chemistry, Genetics, Animal Science and Zoology, Nucleotide, Feces, Food Science
Published
2018

48. 93 Effects of Yeast Culture (Saccharomyces cerevisiae) Supplementation on Growth Performance, Fecal Score, and Nutrient Digestibility of Weaning Pigs

Author

X Liu, D J Lee, H Y Sun, Jin Wan Park, and I. H. Kim

Subjects
0301 basic medicine, Nutrient digestibility, Saccharomyces cerevisiae, 0402 animal and dairy science, 04 agricultural and veterinary sciences, General Medicine, Biology, biology.organism_classification, 040201 dairy & animal science, Yeast, 03 medical and health sciences, 030104 developmental biology, Genetics, Weaning, Animal Science and Zoology, Food science, Feces, Food Science
Published
2018

49. Spectroscopic Mass and Host-star Metallicity Measurements for Newly Discovered Microlensing Planet OGLE-2018-BLG-0740Lb

Author

Akihiko Fukui, Doeon Kim, Aparna Bhattacharya, K. H. Hwang, Masayuki Nagakane, Paweł Pietrukowicz, Radek Poleski, K. A. Rybicki, Subo Dong, D. J. Lee, Martin Donachie, Denis J. Sullivan, Patryk Iwanek, Youn Kil Jung, Michael D. Albrow, Sun-Ju Chung, Byeong-Gon Park, Yuki Hirao, Seung-Lee Kim, Chung-Uk Lee, Igor Soszyński, Yossi Shvartzvald, Nicholas J. Rattenbury, Jan Skowron, Jennifer C. Yee, Cheongho Han, K. Boutsia, In-Gu Shin, Woong-Tae Kim, Richard W. Pogge, Yutaka Matsubara, Kohei Kawasaki, Fumio Abe, Nidia Morrell, Juna A. Kollmeier, Marcin Wrona, David P. Bennett, Krzysztof Ulaczyk, Dong-Jin Kim, Daisuke Suzuki, Arnaud Cassan, Yoshitaka Itow, Przemek Mróz, Takahiro Sumi, Richard Barry, Shota Miyazaki, Iona Kondo, Kyeongsoo Hong, Paul J. Tristram, Yoon-Hyun Ryu, Naoki Koshimoto, Hyoun-Woo Kim, Ian A. Bond, Andrzej Udalski, Michał K. Szymański, Yasushi Muraki, Man Cheung Alex Li, Yongseok Lee, Atsunori Yonehara, Andrew Gould, Clément Ranc, Weicheng Zang, Valerio Bozza, Sang-Mok Cha, Szymon Kozłowski, and Haruno Suematsu

Subjects
gravitational lensing: micro, planetary systems, 010504 meteorology & atmospheric sciences, Metallicity, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Gravitational microlensing, 01 natural sciences, Planet, 0103 physical sciences, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Earth and Planetary Astrophysics (astro-ph.EP), Physics, Very Large Telescope, Spectrometer, Astronomy and Astrophysics, Planetary system, Amplitude, 13. Climate action, Space and Planetary Science, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - Earth and Planetary Astrophysics
Abstract

著者人数: Leading authors 11名, The KMTNet Collaboration 21名, The OGLE Collaboration 11名, The MOA Collaboration 23名, 全66名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 鈴木, 大介), Number of authors: Leading authors 11, The KMTNet Collaboration 21, The OGLE Collaboration 11, The MOA Collaboration 23, Total 66 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Suzuki, Daisuke), Accepted: 2019-06-27, 資料番号: SA1190105000

Published
2019

50. KMT-2017-BLG-0165Lb: A Super-Neptune-mass Planet Orbiting a Sun-like Host Star

Author

Sang-Mok Cha, Jennifer C. Yee, Sun-Ju Chung, Dong-Jin Kim, W. Zang, D. J. Lee, Chung-Uk Lee, Matthew T. Penny, Andrew Gould, Yossi Shvartzvald, Seung-Lee Kim, Shude Mao, K. H. Hwang, Tianshu Wang, B. G. Park, Yoon-Hyun Ryu, Richard W. Pogge, Youn Kil Jung, In-Gu Shin, Wei Zhu, Yongseok Lee, Hyoun-Woo Kim, Pascal Fouqué, Michael D. Albrow, and C. Han

Subjects
Earth and Planetary Astrophysics (astro-ph.EP), Physics, 010504 meteorology & atmospheric sciences, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Mass ratio, Planetary system, Light curve, Gravitational microlensing, 01 natural sciences, Stars, 13. Climate action, Space and Planetary Science, Neptune, Planet, 0103 physical sciences, Parallax, 010303 astronomy & astrophysics, Astrophysics - Earth and Planetary Astrophysics, 0105 earth and related environmental sciences
Abstract

We report the discovery of a low mass-ratio planet $(q = 1.3\times10^{-4})$, i.e., 2.5 times higher than the Neptune/Sun ratio. The planetary system was discovered from the analysis of the KMT-2017-BLG-0165 microlensing event, which has an obvious short-term deviation from the underlying light curve produced by the host of the planet. Although the fit improvement with the microlens parallax effect is relatively low, one component of the parallax vector is strongly constrained from the light curve, making it possible to narrow down the uncertainties of the lens physical properties. A Bayesian analysis yields that the planet has a super-Neptune mass $(M_{2}=34_{-12}^{+15}~M_{\oplus})$ orbiting a Sun-like star $(M_{1}=0.76_{-0.27}^{+0.34}~M_{\odot})$ located at $4.5~{\rm kpc}$. The blended light is consistent with these host properties. The projected planet-host separation is $a_{\bot}={3.45_{-0.95}^{+0.98}}~{\rm AU}$, implying that the planet is located outside the snowline of the host, i.e., $a_{sl}\sim2.1~{\rm AU}$. KMT-2017-BLG-0165Lb is the sixteenth microlensing planet with mass ratio $q3.3$ is quite severe. Alternatively, the distribution is also suggestive of a "pile-up" of planets at Neptune-like mass ratios, below which there is a dramatic drop in frequency., 27 pages, 3 tables, 9 figures, accepted for publication in AJ

Published
2019

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