cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Bothriogenys gorringei
Creators: name: Al-Kindi, Mohammed
name: Pickford, Martin
name: Al-Sinani, Yusouf
name: Al-Ismaili, Ibrahim
name: Hartman, Axel
name: Heward, Alan
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Artiodactyla
Anthracotheriidae
Bothriogenys
Bothriogenys gorringei

description: Bothriogenys gorringei (ANDREWS et BEADNELL, 1902)
M a t e r i a l. ONHM TN 2017-01, first phalanx.
 D e s c r i p t i o n. The Omanitherium type locality yielded a first phalanx of an anthracothere in situ in indurated marl (Text-fig. 20). The specimen, ONHM TN 2017-01, is complete. The distal end shows a moderate central valley between the two articular surfaces, a feature of artiodactyl phalanges, which distinguishes this fossil from proboscidean phalanges that have an almost obsolete central valley (Gheerbrant et al. 2005, Delmer et al. 2006). The specimen is 41.4 mm long, and the distal end is 15.3 mm broad by ca. 9 mm tall, and is thus compatible in dimensions with the species Bothriogenys gorringei, which has already been recorded from the Ashawq Formation on the basis of upper and lower molars (Pickford 2015c)
 D i s c u s s i o n. The anthracothere phalanx from the Omanitherium type locality proves the association of this family with fossils of the arsinoithere, Arsinoitherium andrewsi, and the numidotherioid, Omanitherium dhofarense. This association was already noted at the Thaytiniti locality excavated by the Thomas Expedition of 1992 (Pickford 2015c).
 Sileem et al. (2015, 2016) and Sallam et al. (2016) extended knowledge of Bothriogenys and other anthracotheres in the Fayum deposits of northern Egypt, in particular regarding stratigraphic distribution of various taxa, reporting specimens from the Late Eocene Qasr el Sagha Formation and the Jebel Qatrani Formation. The results of this work agree with the Omani record, which, it must be admitted, is still rather sparse. It suggests that the Ashawq Formation is close in age to Quarry L 41 in the Jebel Qatrani Formation (Rupelian) (Seiffert 2006), although a correlation to the earlier Qasr el Sagha Formation (Priabonian) cannot be discounted (Sileem et al. 2016).
 The fossil record of anthracotheres in the Arabian Peninsula is filling in, but there are still long gaps in the stratigraphic representation of the family. The next youngest anthracotheres following the Ashawq records (Pickford 2015c) and those from the Usfan and Shumaysi Formations, Western Saudi Arabia (Zalmout et al. 2012) of Early Oligocene age, are those from the Early Miocene deposits at Wadi Sabya, southwestern Saudi Arabia (Brachyodus DEPÉRET, 1895, at 17°12’46.3”N: 42°47’08.8”E 79 m a.s.l. – Madden et al. 1983) and Ghaba, Oman (Afromeryx zelteni PICKFORD, 1991 – Roger et al. 1994a).
description: Published as part of Al-Kindi, Mohammed, Pickford, Martin, Al-Sinani, Yusouf, Al-Ismaili, Ibrahim, Hartman, Axel & Heward, Alan, 2017, Large Mammals From The Rupelian Of Oman - Recent Finds, pp. 300-321 in Fossil Imprint 73 (3 - 4) on page 313, DOI: 10.2478/if-2017-0017, http://zenodo.org/record/5385120
Bashar H. Malkawi, Chinese State-Owned Enterprise Investment
Creators: name: Malkawi, Bashar H.
Publisher: name: figshare
Year: 2019
Subjects: subject: 180105 Commercial and Contract Law
subject: FOS: Law

description: China has overtaken Japan as the world's second-biggest economy. In a remarkably short span– less than fifteen years– the United States economy has experienced a relatively huge decline vis-à-vis China on a nominal GDP basis.
RXTE monitoring of Centaurus A
Creators: name: Benlloch, S.
name: Rothschild, R. E.
name: Wilms, J.
name: Reynolds, C. S.
name: Heindl, W. A.
name: Staubert, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the analysis from ~110 ks of X-ray observations of Centaurus A carried out with the Proportional Counter Array (PCA) and the High Energy X-ray Timing Experiment (HEXTE) instruments on Rossi X-ray Timing Explorer (RXTE) during three monitoring campaigns over the last 4 years (10 ks in 1996, 74 ks in 1998, and 25 ks in 2000). The joint PCA/HEXTE X-ray spectrum can be well described by a heavily absorbed power law with photon index 1.8 and a narrow iron line due to fluorescence of cold matter. The measured column depth decreased by about 30% between 1996 and 2000, while the detected 2-10 keV continuum flux remained constant between 1996 and 1998, but increased by 60% in 2000. Since in all three observations the iron line flux did not vary, a corresponding decrease in equivalent width was noted. No appreciable evidence for a reflection continuum in the spectrum was detected. We present the interpretation of the iron line strength through Monte Carlo computations of various geometries. No significant temporal variability was found in Cen A at time scales from days to tens of minutes.
description: 7 pages, 4 figures. Accepted for publication in A&A
Some remarks on the spectral functions of the Abelian Higgs Model
Creators: name: Dudal, D.
name: van Egmond, D. M.
name: Guimaraes, M. S.
name: Holanda, O.
name: Mintz, B. W.
name: Palhares, L. F.
name: Peruzzo, G.
name: Sorella, S. P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the unitary Abelian Higgs model and investigate its spectral functions at one-loop order. This analysis allows to disentangle what is physical and what is not at the level of the elementary particle propagators, in conjunction with the Nielsen identities. We highlight the role of the tadpole graphs and the gauge choices to get sensible results. We also introduce an Abelian Curci-Ferrari action coupled to a scalar field to model a massive photon which, like the non-Abelian Curci-Ferarri model, is left invariant by a modified non-nilpotent BRST symmetry. We clearly illustrate its non-unitary nature directly from the spectral function viewpoint. This provides a functional analogue of the Ojima observation in the canonical formalism: there are ghost states with nonzero norm in the BRST-invariant states of the Curci-Ferrari model.
description: 32 pages, 12 figures
The Clustering of Chicago - a Long Term Perspective
Creators: name: Lai, Yutian
Publisher: name: University of Chicago
Year: 2021
Subjects: subject: Cluster Analysis
subject: Geoda
subject: Python
subject: Spatio-temporal Change

description: The purpose of this research lies in two aspects. The first is to carry out an in-depth comparison of the clustering results obtained from different methods, so as to find the “optimal” clustering method. The second is to conduct cluster analysis of Chicago utilizing the census tracts data from three years 1950, 1980 and 2010, aiming to understand the spatio-temporal transitions of Chicago neighborhoods across the years. This study is both a theoretical investigation and a methodological investigation. The results indicates K-means clustering using principal components proved to be the optimal method in terms of the measures we chose, and the longitudinal change in spatial patterns of Chicago resembled the description of Chicago School theorists, while some brand-new trajectories were also detected.
Chromodoris tennentana
Creators: name: Yonow, Nathalie
name: Anderson, R. Charles
name: Buttress, Susan G.
Publisher: name: Zenodo
Year: 2002
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Nudibranchia
Chromodorididae
Chromodoris
Chromodoris tennentana

description: Chromodoris tennentana (Kelaart, 1859)
(®gure 13a)
 Chromodoris tennentana (Kelaart): Rudman, 1987: 364, ®gures 23, 32, 35, 36.
 Material. Chag96/61: 18 3 4 mm; coral bommie east of Ile Poule, Peros Banhos Atoll; 25 February 1996; at 7 m depth.
 Description. Mantle with irregular purple margin and broad cream submarginal band which contained raised orange patches. Central area of notum brown with numerous black spots, each ocellated with white. Rhinophore clubs brown with white tips; stalks translucent. Gills grey and white.
The preserved specimen is soft and well relaxed. It is translucent white and the dark gut is clearly visible through the body wall. The orange pigment spots around the mantle edge remain as patches and the mantle glands are extremely clear as evenly distributed groups around the edge, just in from the margin; they are absent in front of the rhinophores.
 Geographic distribution. Western Indian Ocean: recorded from Tanzania and Sri Lanka as C. cavae Eliot and C. vicina Eliot; this record from Chagos is a new locality. It is not uncommon in the Seychelles (photographs of several individuals and one specimen 83 5 mm alive; coll. P. Kemp, 1992).
 Remarks. Chromodoris tennentana is a large species, growing to more than 60 mm in length (preserved measurement, Eliot, 1904a). The orange spots in the white submarginal band of our specimen are slightly raised; this had not been noted in previous descriptions.
description: Published as part of Yonow, Nathalie, Anderson, R. Charles & Buttress, Susan G., 2002, Opisthobranch molluscs from the Chagos Archipelago, Central Indian Ocean, pp. 831-882 in Journal of Natural History 36 (7) on page 854, DOI: 10.1080/00222930110039161, http://zenodo.org/record/10100688
รูปแบบความสัมพันธ์เชิงสาเหตุความรักที่มีต่อแบรนด์ผ่านสื่อสังคมออนไลน์ ของผู้บริโภคในกรุงเทพมหานครและปริมณฑล
Creators: name: ไพโรจน์ บุตรชีวัน
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: ดิจิทัลแบรนดิ้ง
ความรักที่มีต่อแบรนด์
สื่อสังคมออนไลน์

description: วารสารเทคโนโลยีภาคใต้, 12, 1, 72-83
Glossodoris cincta
Creators: name: Yonow, Nathalie
name: Anderson, R. Charles
name: Buttress, Susan G.
Publisher: name: Zenodo
Year: 2002
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Nudibranchia
Chromodorididae
Glossodoris
Glossodoris cincta

description: Glossodori s cincta (Bergh, 1888)
 (®gure 13c) Glossodoris cincta (Bergh): Rudman, 1986a: 149, numerous ®gures; Yonow, 1994a: 120, ®gure 10H.
 Material. Chag96/59: 27 mm; on rubble near bommie east of Ile Poule, inside Peros Banhos Atoll; 23 February 1996; at 7 m depth. Chag96/82: 25 mm; Three Brothers, Great Chagos Bank; 3 March 1996; at 5 m depth. Chag96/92a, b: 37 mm, 35 mm; Victory Bank; 3 March 1996; at 8 m depth.
 Description. The body is solid and the mantle edge undulated, with a noticeably enlarged permanent fold mid-laterally on both sides. The mantle edge appeared dark green from a distance, but comprised an outer royal blue margin and an olive green submarginal band (®gure 13c). The dorsal surface was pustular and mottled pinkish brown, speckled with white and yellow dots; there was a darker central ®eld extending from the rhinophores to the gills. The foot was dark pink, mottled with white-tipped pustules, with thin bright blue and olive green marginal bands. Rhinophores were dark brown speckled with white; white midline present anteriorly and (in one specimen) posteriorly. Gills pale brown, with ®ne dark edges.
The preserved specimens are all well relaxed; they retain the red marbling on the dorsum and the blue and green margins on the mantle and foot. The colour pattern on the gills and rhinophores also remains. All specimens have stained their formaldehyde preservative yellow to yellowish brown.
 Geographic distribution. Indo-West Paci®c: Red Sea (Yonow, 1989) and western Indian Ocean (Yonow and Hayward, 1991; Yonow, 1994a) to Christmas Island (Indian Ocean), north Australia and the Philippines (Rudman, 1986a).
 Remarks. This species is well known, occurring in several colour morphs: these specimens conform with the Red Sea and western Indian Ocean form which has a mottled red dorsum, an olive green submarginal and thin blue marginal line. In life the gills vibrated constantly in specimen 96/59, a feature also noted for the specimens from East Africa and the Philippines (Rudman, 1986a), and typical of numerous species of Glossodoris. Specimen 96/92 was photographed in situ on a black sponge (cf. specimen from Maldives on purple sponge in Yonow, 1994a: ®gure 10H).
description: Published as part of Yonow, Nathalie, Anderson, R. Charles & Buttress, Susan G., 2002, Opisthobranch molluscs from the Chagos Archipelago, Central Indian Ocean, pp. 831-882 in Journal of Natural History 36 (7) on pages 856-857, DOI: 10.1080/00222930110039161, http://zenodo.org/record/10100688
Evident black hole-bulge coevolution in the distant universe
Creators: name: Yang, Guang
name: Brandt, W. N.
name: Alexander, D. M.
name: Chen, C. -T. J.
name: Ni, Q.
name: Vito, F.
name: Zhu, F. -F.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Observations in the local universe show a tight correlation between the masses of supermassive black holes (SMBHs; $M_{\rm BH}$) and host-galaxy bulges ($M_{\rm bulge}$), suggesting a strong connection between SMBH and bulge growth. However, direct evidence for such a connection in the distant universe remains elusive. We have studied sample-averaged SMBH accretion rate ($\overline{\rm BHAR}$) for bulge-dominated galaxies at $z=0.5-3$. While previous observations found $\overline{\rm BHAR}$ is strongly related to host-galaxy stellar mass ($M_\star$) for the overall galaxy population, our analyses show that, for the bulge-dominated population, $\overline{\rm BHAR}$ is mainly related to SFR rather than $M_\star$. This ${\overline{\rm BHAR}}$-SFR relation is highly significant, e.g. $9.0σ$ (Pearson statistic) at $z=0.5-1.5$. Such a $\overline{\rm BHAR}$-SFR connection does not exist among our comparison sample of galaxies that are not bulge-dominated, for which $M_\star$ appears to be the main determinant of SMBH accretion. This difference between the bulge-dominated and comparison samples indicates that SMBHs only coevolve with bulges rather than the entire galaxies, explaining the tightness of the local $M_{\rm BH}$-$M_{\rm bulge}$ correlation. Our best-fit $\overline{\rm BHAR}$-SFR relation for the bulge-dominated sample is $\log\overline{\rm BHAR} = \log\mathrm{SFR} - (2.48\pm0.05)$ (solar units). The best-fit $\overline{\rm BHAR}/\mathrm{SFR}$ ratio ($10^{-2.48}$) for bulge-dominated galaxies is similar to the observed $M_{\rm BH}/M_{\rm bulge}$ values in the local universe. Our results reveal that SMBH and bulge growth are in lockstep, and thus non-causal scenarios of merger averaging are unlikely the origin of the $M_{\rm BH}$-$M_{\rm bulge}$ correlation. This lockstep growth also predicts that the $M_{\rm BH}$-$M_{\rm bulge}$ relation should not have strong redshift dependence.
description: 18 Pages, 11 figures, 4 tables; MNRAS accepted
An irradiated accretion disk in the narrow-line Seyfert 1 RE J1034+396?
Creators: name: Soria, R.
name: Puchnarewicz, E. M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We model the optical to X-ray continuum spectrum of the narrow-line Seyfert 1 galaxy RE J1034+396. We show that the flat optical spectrum is consistent with emission from an irradiated accretion disk. The X-ray emission can be modelled with a disk blackbody and a Comptonised component. The temperature at the inner edge of the disk T_{in} = (0.12 +/- 0.02) keV. Using this constraint, we show that the flat optical spectrum is consistent with emission from the irradiatively heated outer part of the accretion disk. We constrain the outer radius of the optically thick disk (R >~ 5 x 10^{16} cm) and the inner radius of the irradiation-dominated region (R >~ 5 x 10^{12} cm). Our optical and X-ray spectral fits indicate a mass 0.6
description: accepted for publication in MNRAS
Fryeria marindica
Creators: name: Yonow, Nathalie
name: Anderson, R. Charles
name: Buttress, Susan G.
Publisher: name: Zenodo
Year: 2002
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Nudibranchia
Phyllidiidae
Fryeria
Fryeria marindica

description: Fryeria marindica (Yonow and Hayward, 1991)
(®gure 16a)
 Reyfria marindica Yonow and Hayward, 1991: 23, ®gures 10C, D, 13E.
 Fryeria marindica: Brunckhorst, 1993: 45, pl. 5B, C; Yonow, 1996: 509, ®gure 13A±F.
 Material. Chag96/24a, b: 24 mm, 18 mm; outer reef between Ile Boddam and Ile Poule, Salomon Atoll; 13 February 1996; at 10 m depth. Chag96/27: 24 mm; coral bommie inside Salomon Atoll; 13 February 1996; at 12 m depth.
(a) (b)
(c) (d)
(e) (f)
 Description. Ground colour pale blue. Raised median ridge with orange tubercles; orange tubercles almost continuous in smallest specimen; interrupted in two places by the joining of the two longitudinal black stripes in specimen 96/27. Two black stripes, one on either side of median ridge, with ®ve to seven rays extended to the mantle edge; additional black streaks between these rays. Rhinophores yellow.
 Geographic distribution. Indian Ocean: from Mauritius to Western Australia (Yonow, 1996).
description: Published as part of Yonow, Nathalie, Anderson, R. Charles & Buttress, Susan G., 2002, Opisthobranch molluscs from the Chagos Archipelago, Central Indian Ocean, pp. 831-882 in Journal of Natural History 36 (7) on pages 860-861, DOI: 10.1080/00222930110039161, http://zenodo.org/record/10100688
Australosymmerus (Melosymmerus) bororo
Creators: name: Falaschi, Rafaela Lopes
name: Toczek, Fernanda Ceres
name: Lamas, Carlos José Einicker
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ditomyiidae
Australosymmerus
Australosymmerus bororo

description: Australosymmerus (Melosymmerus) bororo (Lane, 1946)
 Lane, 1946a: 342 (original description), fig. 8 (male genitalia). Ref. – Papavero, 1977b: 19 B.2 (catalogue). Type locality: Brazil, Rio de Janeiro, Itatiaia. Distr. – Neotropical: Brazil (Rio de Janeiro, São Paulo). Holotype ♂, MZUSP.
 Holotype ♂ with labels: (1) printed on pink paper: “HOLOTIPO”; (2) handwritten on white paper: “IX.46 [ix.1946] | R. Janeiro [Rio de Janeiro] | Itatiaia | Barretto col.”; (3) printed with handwritten inscriptions on white paper: “ Centrocnemis | bororo | det. John Lane 194 6 ”; (4) printed on white paper:“MZSP”; (5) printed on white paper:“ MZ004490 ”.
Slide with labels:(1) printed on white paper:“ MZ004490 ”; (2) printed on red paper: “ HOLOTYPE ”; (3) printed on white paper:“ BRASIL, Rio de Janeiro | Itatiaia | ix.1946 | Barreto col.”.
description: Published as part of Falaschi, Rafaela Lopes, Toczek, Fernanda Ceres & Lamas, Carlos José Einicker, 2019, Catalogue of Ditomyiidae and Diadocidiidae (Diptera: Bibionomorpha) types housed in the collection of the Museu de Zoologia da Universidade de São Paulo, Brazil, pp. 1-7 in Papéis Avulsos de Zoologia 59 on page 3, DOI: 10.11606/1807-0205/2019.59.56, http://zenodo.org/record/5385190
A database of saturated hydraulic conductivity of fine-grained soils: probability density functions
Creators: name: Shuyin Feng
name: Vardanega, Paul J.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 20199 Astronomical and Space Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Hematology
subject: Plant Biology

description: Saturated hydraulic conductivity is a key soil mechanics parameter which has widespread use in many geotechnical applications. In order to set up stochastic analyses, geotechnical modellers require databases to calibrate the parameter ranges and distributions employed. This letter uses a recently compiled database of saturated hydraulic conductivity measurements called FG/KSAT-1358 and reports on the fitting of various probability density functions to the data of void ratio, liquid limit, water content ratio and the negative natural logarithm of ksat. It is shown that the best fit distribution is the lognormal for void ratio, while the loglogistic distribution is most favoured for liquid limit and water content ratio, and the best fit distribution for -ln[ksat(m/s)] is the logistic function. The data of -ln[ksat(m/s)] is then subdivided according to liquid limit level, silt or clay classification, type of hydraulic conductivity test used and sample preparation/condition. When some subdivisions of the database are analysed, the best fit distribution is more variable with GEV and logistic being the most favoured for most of the studied subsets.
The Column Density, Kinematics, and Thermal State of Metal-Bearing Gas within the Virial Radius of z~2 Star-Forming Galaxies in the Keck Baryonic Structure Survey
Creators: name: Rudie, Gwen C.
name: Steidel, Charles C.
name: Pettini, Max
name: Trainor, Ryan F.
name: Strom, Allison L.
name: Hummels, Cameron B.
name: Reddy, Naveen A.
name: Shapley, Alice E.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present results from the Keck Baryonic Structure Survey (KBSS) including the first detailed measurements of the column densities, kinematics, and internal energy of metal-bearing gas within the virial radius (35-100 physical kpc) of eight ~$L^*$ galaxies at $z\sim2$. From our full sample of 130 metal-bearing absorbers, we infer that halo gas is kinematically complex when viewed in singly, doubly, and triply ionized species. Broad OVI and CIV absorbers are detected at similar velocities to the lower-ionization gas but with very different kinematic structure indicating that the circumgalactic medium (CGM) is multi-phase. There is a high covering fraction of metal-bearing gas within 100 kpc including highly ionized gas such as OVI; however, observations of a single galaxy probed by a lensed background QSO suggest the size of metal-bearing clouds is small (<400 pc for all but the OVI-bearing gas). The mass in metals found within the halo is substantial, equivalent to $\gtrsim$ 25% of the metal mass within the interstellar medium. The gas kinematics unambiguously show that 70% of galaxies with detected metal absorption have some unbound metal-enriched gas, suggesting galactic winds may commonly eject gas from halos at $z\sim2$. Significant thermal broadening is detected in CGM absorbers which dominates the internal energy of the gas. 40% of the detected gas has temperatures in the range $10^{4.5-5.5}$ K where cooling times are short, suggesting the CGM is dynamic, with constant heating and/or cooling to produce this short-lived thermal phase.
description: submitted to ApJ
An Average Case NP-Complete Graph Coloring Problem
Creators: name: Levin, Leonid A.
name: Venkatesan, Ramarathnam
Publisher: name: arXiv
Year: 2001
Subjects: subject: Computational Complexity (cs.CC)
subject: FOS: Computer and information sciences
subject: F.2.2
subject: 60C-05, 68Q-17, 25, 87, 05C-15, 20, 80

description: NP-complete problems should be hard on some instances but those may be extremely rare. On generic instances many such problems, especially related to random graphs, have been proven easy. We show the intractability of random instances of a graph coloring problem: this graph problem is hard on average unless all NP problem under all samplable (i.e., generatable in polynomial time) distributions are easy. Worst case reductions use special gadgets and typically map instances into a negligible fraction of possible outputs. Ours must output nearly random graphs and avoid any super-polynomial distortion of probabilities.
description: 15 pages
The High-Frequency QPOs in GRS 1915+105
Creators: name: Belloni, T.
name: Mendez, Mariano
name: Sanchez-Fernandez, Celia
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyzed two 1996 observations of the Galactic Microquasar GRS 1915+105 taken with the Proportional Counter Array on board the Rossi X-ray Timing Explorer. We focus on the properties of the high-frequency QPO as a function of the `dip' oscillations, a factor of 1000 slower. In one observation, 1996 May 5th, we find that the energy spectrum of the QPO at ~65 Hz changes drastically between the high-intervals and the dips, hardening during the dips to the point that the QPO peak is no longer detected at low energies. In the second observation, 1996 May 14th, although it has similar overall characteristics, the 65 Hz QPO is not seen, but another broader QPO peak appears at 27 Hz, only during the dips. This peak is too weak to obtain reliable information about its spectrum. Our results indicate that the presence/absence of high-frequency features in this enigmatic source are intimately linked to the slower oscillations and variations that happen on longer time scales.
description: Accepted for publication in Astronomy & Astrophysics, April 2001
ความสัมพันธ์ของปัจจัยเชิงสาเหตุที่มีต่อการสร้างความได้เปรียบทางการแข่งขัน ของธุรกิจโรงแรมกลุ่มที่พักขนาดกลางและขนาดเล็กในประเทศไทย
Creators: name: ประวิทย์ สระแก้ว
name: พงษ์เทพ ศรีโสภาจิต
name: ณัชชา กริ่มใจ
name: ชนิดาภา ดีสุขอนันต์
Publisher: name: สมาคมปรัชญาดุษฎีบัณฑิตทางสังคมศาสตร์ มหาวิทยาลัยรามคำแหง
Year: 2562
Subjects: ปัจจัยเชิงสาเหตุ
การสร้างความได้เปรียบทางการแข่งขัน
ธุรกิจโรงแรมกลุ่มที่พัก
Causal Factors
Competitive Advantage
Hotel Business Group

description: วารสารดุษฎีบัณฑิตทางสังคมศาสตร์, 9, 2, 420-437
การวิเคราะห์เส้นทางความสัมพันธ์ปัจจัยที่มีอิทธิพลต่อประสิทธิภาพการจัดเก็บภาษีเงินได้นิติบุคคล
Creators: name: วชิรธร คงสุข
name: กฤษฎาภรณ์ รุจิธำรงกุล
name: บุรพร กำบุญ
Publisher: name: สมาคมปรัชญาดุษฎีบัณฑิตทางสังคมศาสตร์ มหาวิทยาลัยรามคำแหง
Year: 2562
Subjects: ภาษีเงินได้นิติบุคคล
ประสิทธิภาพ
ระบบภาษี
การจัดเก็บภาษีเงินได้นิติบุคคล
Corporate Income Tax
Efficiency
Tax System
Income Tax Collection

description: วารสารดุษฎีบัณฑิตทางสังคมศาสตร์, 9, 2, 307-321
Australosymmerus (Melosymmerus) guayanasi
Creators: name: Falaschi, Rafaela Lopes
name: Toczek, Fernanda Ceres
name: Lamas, Carlos José Einicker
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ditomyiidae
Australosymmerus
Australosymmerus guayanasi

description: Australosymmerus (Melosymmerus) guayanasi (Lane, 1946)
 Lane, 1946a: 340 (original description), fig. 2 (male genitalia). Ref. – Papavero, 1977b: 19 B.2 (catalogue). Type locality: Brazil, São Paulo, Campos do Jordão. Distr. – Neotropical: Brazil (São Paulo). Holotype ♂, MZUSP.
 Holotype ♂ with labels: (1) printed on pink paper: “HOLOTIPO”; (2) printed with handwritten inscriptions on white paper: “ São Paulo XII 45 [xii.1945] | C. Jordão [Campos do Jordão] | det. J. Lane coll”; (3) printed with handwritten inscriptions on white paper:“ Centrocnemis guayanasi | det. John Lane 194”; (4) printed on white paper: “MZSP [MZUSP]”; (5) printed on white paper:“ MZ004496 ”.
 Slide with labels: (1) printed on white paper:“ MZ004496 ”; (2) printed with handwritten inscriptions on white paper: “ BRASIL, São Paulo | Campos do Jordão | xii.1945 | J. Lane col. | M. guayanasi ”; (3) printed on red paper: “ HOLOTYPE ”.
description: Published as part of Falaschi, Rafaela Lopes, Toczek, Fernanda Ceres & Lamas, Carlos José Einicker, 2019, Catalogue of Ditomyiidae and Diadocidiidae (Diptera: Bibionomorpha) types housed in the collection of the Museu de Zoologia da Universidade de São Paulo, Brazil, pp. 1-7 in Papéis Avulsos de Zoologia 59 on page 4, DOI: 10.11606/1807-0205/2019.59.56, http://zenodo.org/record/5385190
True and fake Lax pairs: how to distinguish them
Creators: name: Sakovich, Sergei
Publisher: name: arXiv
Year: 2001
Subjects: subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: Mathematical Physics (math-ph)
subject: Analysis of PDEs (math.AP)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: The gauge-invariant description of zero-curvature representations of evolution equations is applied to the problem of how to distinguish the fake Lax pairs from the true Lax pairs. The main difference between the true Lax pairs and the fake ones is found in the structure of their cyclic bases.
description: 5 pages; v2: sections, discussion, references added
Hydrodynamics at RHIC
Creators: name: Huovinen, Pasi
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The hydrodynamical models used to describe the evolution of heavy-ion collisions are briefly reviewed and their results compared with recent RHIC data.
description: Contribution to the proceedigns of the Cracow Epiphany Conference on quarks and gluons in extreme conditions. 16 pages, 9 figures, uses appolb.cls
Australosymmerus (Melosymmerus) lenkoi Lane 1959
Creators: name: Falaschi, Rafaela Lopes
name: Toczek, Fernanda Ceres
name: Lamas, Carlos José Einicker
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ditomyiidae
Australosymmerus
Australosymmerus lenkoi

description: Australosymmerus (Melosymmerus) lenkoi Lane, 1959
 Lane, 1959: 105 (original description), fig. 12 (male genitalia). Ref. – Papavero, 1977b: 19 B.2 (catalogue). Type locality: Brazil, Amapá, Serra do Navio. Distr. – Neotropical: Brazil (Amapá). Holotype ♂, MZUSP.
 Holotype ♂ with labels: (1) printed on pink paper: “HOLOTIPO”; (2) printed with handwritten inscriptions on white paper: “ Serra do Navio | Terr. Amapá BRASIL | 20.I X-1957 [20.ix.1957] | J. Lane [John Lane] leg.”; (3) printed with handwritten inscriptions on white paper: “ Australosymmerus | lenkoi | det. John Lane 195 9 ”; (4) printed on white paper: “MZSP [MZUSP]”; (5) printed on white paper:“ MZ004495 ”.
Slide with labels:(1) printed on white paper:“ MZ004495 ”; (2) printed on white paper:“ BRASIL, Amapá | Serra do Navio | 20.ix.1957 | J. Lane [John Lane] col.”; | (3) handwritten on white paper:“ M. lenkoi.”; (4) printed on red paper:“ HOLOTYPE ”.
 Condition of holotype: Pinned. Left wing and male terminalia on the permanent slide. Left antenna broken. Missing parts: none.
description: Published as part of Falaschi, Rafaela Lopes, Toczek, Fernanda Ceres & Lamas, Carlos José Einicker, 2019, Catalogue of Ditomyiidae and Diadocidiidae (Diptera: Bibionomorpha) types housed in the collection of the Museu de Zoologia da Universidade de São Paulo, Brazil, pp. 1-7 in Papéis Avulsos de Zoologia 59 on pages 4-5, DOI: 10.11606/1807-0205/2019.59.56, http://zenodo.org/record/5385190
Additional file 1: of Effect of Ultraviolet-Ozone Treatment on MoS2 Monolayers: Comparison of Chemical-Vapor-Deposited Polycrystalline Thin Films and Mechanically Exfoliated Single Crystal Flakes
Creators: name: Changki Jung
name: Yang, Hae
name: Choi, Woong
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Developmental Biology
subject: Marine Biology

description: Crystallinity and AFM analysis. (DOCX 13198 kb)
Prospects for Star Formation Studies with Mid-Infrared Instruments on Large Telescopes
Creators: name: Jayawardhana, Ray
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Imaging and spectroscopic observations in the mid-infrared wavelength range (5$μ$m--30$μ$m) offer valuable insight into the origins of stars and planets. Sensitive new array detectors on 8-meter class telescopes make it possible to study a wide range of phenomena, from protoplanetary disks to starburst galaxies, in unprecedented detail. I review the capablities of ground-based mid-infrared instruments (e.g., high spatial resolution) and their limitations (e.g., poor sensitivity, small field of view) using several examples in the field of star formation, and discuss prospects for the near future.
description: 6 pages, 3 PostScript figures, to appear in proceedings of "Origins of Stars and Planets: The VLT View", Garching, April 24-27 2001
Phyllidia coelestis Bergh 1905
Creators: name: Yonow, Nathalie
name: Anderson, R. Charles
name: Buttress, Susan G.
Publisher: name: Zenodo
Year: 2002
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Nudibranchia
Phyllidiidae
Phyllidia
Phyllidia coelestis

description: Phyllidia coelestis Bergh, 1905
(®gure 16b)
 Phyllidia coelestis Bergh, 1905: 182, pl. 3, ®gure 16; Lin, 1983: 152, pl. 1, ®gure 3; Brunckhorst, 1989: 37, numerous ®gures; Brunckhorst, 1993: 30, pl. 1F, H.
 Phyllidia nobilis: Farran, 1905: 345, pl. 3, ®gures 16, 17.
 Phyllidia elegans: Edmunds, 1972: 82, ®gure 4B.
 Phyllidia alia Yonow, 1984: 224, ®gures 6C, D, 7A, 8F, G.
 NOT Phyllidia picta Pruvot-Fol, 1957: 110, ®gures 5±12 (as per Brunckhorst, 1993) (5 Fryeria picta; see Yonow, 1996).
 Material. Chag96/32: 12 mm; outer reef, Ile de la Passe, Salomon Atoll; 14 February 1996; at 15 m depth. Chag96/43a, b: 32 mm, 28 mm; inner reef, Ile Diamant, Peros Banhos Atoll; 19 February 1996; at 3 m depth. Chag96/46: 16 mm; outer reef, Ile Diamant, Peros Banhos Atoll; 20 February 1996; depth not recorded; no photographs taken. Chag96/53a, b: 25 mm, 22 mm; inner reef, Ile Mapou, Peros Banhos Atoll; 21 February 1996; at 9 m depth; no photographs taken. Chag96/67: 353 15 mm; coral bommie, east of Ile Poule, Peros Banhos Atoll; 25 February 1996; at 9 m depth; no photographs taken.
 Description. Ground colour pale granular blue. Three longitudinal black stripes, one on the midline interrupted by yellow tubercles; the two laterals were continuous but did not meet anteriorly between the rhinophores. Variable number of rounded, yellow tubercles arranged longitudinally; fewest in smallest specimen but otherwise no obvious correlation with size. Small black ¯ecks peripherally. Rhinophores slightly deeper yellow than tubercles.
 Geographic distribution. Indo-West Paci®c: Sri Lanka (Yonow, 1984 as P. alia), the Seychelles (Edmunds, 1972 as P. elegans) and South Africa (Gosliner, 1987 as P. varicosa) to Fiji (Brunckhorst, 1993).
 Remarks. Brunckhorst (1989, 1993) redescribed and illustrated this species; the majority of his material was from the Paci®c, where it also appears to be relatively common.
description: Published as part of Yonow, Nathalie, Anderson, R. Charles & Buttress, Susan G., 2002, Opisthobranch molluscs from the Chagos Archipelago, Central Indian Ocean, pp. 831-882 in Journal of Natural History 36 (7) on page 862, DOI: 10.1080/00222930110039161, http://zenodo.org/record/10100688
Additional file 3: of Identification and potential mechanisms of a 4-lncRNA signature that predicts prognosis in patients with laryngeal cancer
Creators: name: Guihai Zhang
name: Erxi Fan
name: Qiuyue Zhong
name: Guangyong Feng
name: Shuai, Yu
name: Mingna Wu
name: Qiying Chen
name: Xiaoxia Gou
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology

description: lncRNA-related genes. Top 200 lncRNA-related genes predicted by MEM. (PDF 7558 kb)
Blockchain-based Bidirectional Updates on Fine-grained Medical Data
Creators: name: Li, Chunmiao
name: Cao, Yang
name: Hu, Zhenjiang
name: Yoshikawa, Masatoshi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Software Engineering (cs.SE)
subject: Databases (cs.DB)
subject: FOS: Computer and information sciences
subject: H.2; D.2; K.6.5

description: Electronic medical data sharing between stakeholders, such as patients, doctors, and researchers, can promote more effective medical treatment collaboratively. These sensitive and private data should only be accessed by authorized users. Given a total medical data, users may care about parts of them and other unrelated information might interfere with the user interested data search and increase the risk of exposure. Besides accessing these data, users may want to update them and propagate to other sharing peers so that all peers keep identical data after each update. To satisfy these requirements, in this paper we propose a medical data sharing architecture that addresses the permission control using smart contracts on the blockchain and splits data into fined grained pieces shared with different peers then synchronize full data and these pieces with bidirectional transformations. Medical data reside on each userś local database and permission related data are stored on smart contracts. Only all peers have gained the newest shared data after updates can they start to do next operations on it, which are enforced by smart contracts. Blockchain based immutable shared ledge enables users to trace data updates history. This paper can provide a new perspective to view full medical data as different slices to be shared with various peers but consistency after updates between them are still promised, which can protect the privacy and improve data search efficiency.
อิทธิพลของการดูแลเชิงจิตวิญญาณและสิ่งแวดล้อมทางกายภาพบนพื้นฐานวัฒนธรรมอิสลามต่อการเป็นแบรนด์แอดโวเคซี่
Creators: name: วิทยา มุงอินทร์
name: ระพีพรรณ พิริยะกุล
name: วงศ์ธีรา สุวรรณิน
Publisher: name: สมาคมปรัชญาดุษฎีบัณฑิตทางสังคมศาสตร์ มหาวิทยาลัยรามคำแหง
Year: 2562
Subjects: การดูแลเชิงจิตวิญญาณ
สิ่งแวดล้อมทางกายภาพ
ความเชื่อมั่น
แบรนด์แอดโวเคซี่
Spiritual Care
Physical Environment
Trust
Brand Advocacy

description: วารสารดุษฎีบัณฑิตทางสังคมศาสตร์, 9, 2, 438-451
Simulating the X-ray Forest
Creators: name: Fang, T.
name: Bryan, G. L.
name: Canizares, C. R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Numerical simulations predict that a large number of baryons reside in intergalactic space at temperatures between 10^5-10^7 K. Highly-ionized metals, such as O VII and O VIII, are good tracers of this ``warm-hot intergalactic medium'', or WHIM. For collisionally-ionized gas, the ionization fraction of each ion peaks at some particular temperature (``peak temperatures''), so different ions can therefore trace the IGM at different temperatures. We performed a hydrodynamic simulation to study the metal distributions in the IGM. We then draw random lines-of-sight across the simulated region and synthesize resonance absorption line spectra in a similar way to simulating the Ly-alpha forest. By studying the distribution functions of H- and He-like O, Si and Fe in a collisionally-ionized IGM and comparing with semi-analytic results based on the Press-Schechter formalism, we find: (1) ions with higher peak temperatures (for instance, Fe XXVI) tend to concentrate around virialized halos, which can be well described by the Press-Schechter distribution, ions with lower peak temperatures are found both in small halos (such as groups of galaxies) and in filaments; (2) lower peak temperature ions are more abundant and should be easily observed; (3) peculiar velocities contribute a significant part to the broadening of the resonant absorption lines.
description: 43 pages, 18 figures. Accepted for publication in the Astrophysical Journal. For high resolution figures, see http://space.mit.edu/~fangt/www/x-ray
แนวทางการใช้ประโยชน์จากเปลือกทุเรียนและเปลือกมังคุดเป็นเชื้อเพลิงเขียวอัดแท่งและปุ๋ย: กรณีศึกษาอำเภอแก่งหางแมว จังหวัดจันทบุรี
Creators: name: วิลาสินี หอมระรื่น
name: วิสาขา ภู่จินดา
Publisher: name: สมาคมปรัชญาดุษฎีบัณฑิตทางสังคมศาสตร์ มหาวิทยาลัยรามคำแหง
Year: 2562
Subjects: เชื้อเพลิงเขียวอัดแท่ง
ปุ๋ย
เปลือกทุเรียนและเปลือกมังคุด
อำเภอแก่งหางแมว จังหวัดจันทบุรี
Fuel Briquettes
Fertilizers
Durian Shells and Mangosteen Shells
Kaeng Hang Maeo District, Chanthaburi Province

description: วารสารดุษฎีบัณฑิตทางสังคมศาสตร์, 9, 2, 452-466
Optical IFU spectroscopy of a bipolar microquasar jet in NGC 300
Creators: name: McLeod, A. F.
name: Scaringi, S.
name: Soria, R.
name: Pakull, M. W.
name: Urquhart, R.
name: Maccarone, T. J.
name: Knigge, C.
name: Miller-Jones, J. C. A.
name: Plotkin, R. M.
name: Motch, C.
name: Kruijssen, J. M. D.
name: Schruba, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We recently reported the discovery of a candidate jet-driving microquasar (S10) in the nearby spiral galaxy NGC 300. However, in the absence of kinematic information, we could not reliably determine the jet power or the dynamical age of the jet cavity. Here, we present optical MUSE integral field unit (IFU) observations of S10, which reveal a bipolar line-emitting jet structure surrounding a continuum-emitting central source. The optical jet lobes of S10 have a total extent of $\sim$ 40 pc and a shock velocity of $\sim$ 150 km s$^{-1}$. Together with the jet kinematics, we exploit the MUSE coverage of the Balmer H$β$ line to estimate the density of the surrounding matter and therefore compute the jet power to be $P_{jet}\approx$ 6.3 $\times$ 10$^{38}$ erg s$^{-1}$. An optical analysis of a microquasar jet bubble and a consequent robust derivation of the jet power have been possible only in a handful of similar sources. This study therefore adds valuable insight into microquasar jets, and demonstrates the power of optical integral field spectroscopy in identifying and analysing these objects.
description: Accepted for publication in MNRAS
Is Cinema a Vessel for Empathy: An Assessment of Audiences' Active Inaction
Creators: name: Boyle, Aislinn (Author)
Publisher: name: Capilano University
Year: 2020

description: Not peer reviewed
description: The purpose of this essay was to discover whether or not cinema has the power to garner true empathy and motivate audiences to enact it upon the real world. From what we have learned over four years, and especially during this course, it made sense to begin the essay by explaining the potential power film holds on a macro-level from a socio-political angle. Then, I delved into the psychoanalytical for a perspective on how media affects the individual. With that context, I lastly expanded into real-world studies, some pop culture, and other fields. I anticipated for this piece to end in a polemic. Our world is lacking in empathy, and that bleakness is seeping into my schoolwork; however, I found through further analysis that if the methodology of spurring empathy in audiences was modified to shock, compel, create vulnerability, and teach of a new side to life through film, then empathy en masse may not be lost just yet.
Australosymmerus (Melosymmerus) tupi
Creators: name: Falaschi, Rafaela Lopes
name: Toczek, Fernanda Ceres
name: Lamas, Carlos José Einicker
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ditomyiidae
Australosymmerus
Australosymmerus tupi

description: Australosymmerus (Melosymmerus) tupi (Lane, 1946)
 Lane, 1946a: 341 (original description), fig. 3 (male genitalia). Ref. – Papavero, 1977b: 19 B.3 (catalogue). Type locality: Brazil, Goiás, Corumbá de Goiás. Distr. – Neotropical: Brazil (Goiás, São Paulo), Argentina (Misiones). Holotype ♂, MZUSP.
 Holotype ♂ with labels: (1) printed pink paper: “HOLOTIPO”; (2) handwritten on white paper: “Goiáz [Goiás] | Corumbá [Corumbá de Goiás] | Barretto-col.”; (3) printed with handwritten inscriptions on white paper “ Centrocnemis | tupi | det. John Lane 194”; (4) printed on white paper:“MZSP”; (5) printed on white paper:“ MZ004498 ”.
Slide with labels:(1) printed on white paper:“ MZ004498 ”; (2) printed on white paper: “ BRASIL, GO, Corumbá [Corumbá de Goiás] | xi.1945 | Barreto col.”; (3) handwritten on white paper: “ M. tupi ”; (4) printed on red paper:“ Holotype ”.
Microvial with labels: (1) printed on white paper: “ MZ004498 ”.
description: Published as part of Falaschi, Rafaela Lopes, Toczek, Fernanda Ceres & Lamas, Carlos José Einicker, 2019, Catalogue of Ditomyiidae and Diadocidiidae (Diptera: Bibionomorpha) types housed in the collection of the Museu de Zoologia da Universidade de São Paulo, Brazil, pp. 1-7 in Papéis Avulsos de Zoologia 59 on page 5, DOI: 10.11606/1807-0205/2019.59.56, http://zenodo.org/record/5385190
Instabilities of infinite matter with effective Skyrme-type interactions
Creators: name: Margueron, Jerome
name: Navarro, Jesus
name: Nguyen, Van Giai
Publisher: name: arXiv
Year: 2002
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The stability of the equation of state predicted by Skyrme-type interactions is examined. We consider simultaneously symmetric nuclear matter and pure neutron matter. The stability is defined by the inequalities that the Landau parameters must satisfy simultaneously. A systematic study is carried out to define interaction parameter domains where the inequalities are fulfilled. It is found that there is always a critical density $ρ_{cr}$ beyond which the system becomes unstable. The results indicate in which parameter regions one can find effective forces to describe correctly finite nuclei and give at the same time a stable equation of state up to densities of 3-4 times the saturation density of symmetric nuclear matter.
description: 20 pages, 5 figures, submitted to Phys.Rev.C
Metalens With Artificial Focus Pattern
Creators: name: Ye, Mao
name: Ray, Vishva
name: Wu, Dachuan
name: Yi, Yasha
Publisher: name: arXiv
Year: 2019
Subjects: subject: Image and Video Processing (eess.IV)
subject: Optics (physics.optics)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Physical sciences

description: Metalens as one of the most popular applications of emmerging optical metasurfaces has raised widspread interest recently. With nano structures fully controlling phase, polarization and transmission, metalens has achieved comparable performance of commercial objective lenses. While recent studies seeking for the accomplishment of traditional focusing behaviors through metalens are successful, inthis work, we have discovered that instead of focusing light to a point, metasurface further enables shaping the focus into a flexibly designed pattern, with more promises and potentials. New mechanism and generalizations of conventional point-focused metalens guiding principles have been proposed with metalens concentrating light to artificial focus pattern. As proving examples, we have demonstrated the engineering of metalens with artificial focus pattern by creating line and ring-shaped focus as 'drawing tools'. The metalens with 'U' and 'M' shaped focus are characterized for the proof of concepts. These metalens are fabricated through a single layer of silicon-based material through CMOS compatible nano fabrication process. The mechanism to generate artificial focus pattern can be applied to a plethora of future on-chip optical devices with applications ranging from beam engineering to next generation nano lithography.
description: 9 pages, 6 figures
Additional file 1: of Identification and potential mechanisms of a 4-lncRNA signature that predicts prognosis in patients with laryngeal cancer
Creators: name: Guihai Zhang
name: Erxi Fan
name: Qiuyue Zhong
name: Guangyong Feng
name: Shuai, Yu
name: Mingna Wu
name: Qiying Chen
name: Xiaoxia Gou
Publisher: name: figshare
Year: 2019
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Cell Biology
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: ceRNA network. Competitive endogenous RNA (ceRNA) regulation network of differentially expressed lncRNAs in laryngeal cancer. (PDF 7834 kb)
ผลกระทบภาวะผู้นำเชิงเปลี่ยนแปลงต่อทีมที่ทรงประสิทธิผลของธนาคารพาณิชย์ไทย
Creators: name: สมฉวี ศิริโสภณา
name: ประยงค์ มีใจซื่อ
name: ชาคริต สกุลอิสริยาภรณ์
name: วิรัช สงวนวงศ์วาน
Publisher: name: สมาคมปรัชญาดุษฎีบัณฑิตทางสังคมศาสตร์ มหาวิทยาลัยรามคำแหง
Year: 2562
Subjects: ภาวะผู้นำเชิงเปลี่ยนแปลง
วัฒนธรรมองค์การแห่งการเรียนรู้
ความยึดมั่นผูกพันของบุคลากร
ทีมที่ทรงประสิทธิผล
Transformational Leadership
Learning Organization Culture
Employee Engagement
Effective Teams

description: วารสารดุษฎีบัณฑิตทางสังคมศาสตร์, 9, 2, 322-336