cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Mirabilicoxa Hessler 1970
Creators: name: George, Robert Y.
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Desmosomatidae
Mirabilicoxa

description: Genus Mirabilicoxa Hessler, 1970
 Type species. Mirabilicoxa gracilipes (Hansen, 1916).
 Diagnosis. Desmosomatinae with sexual dimorphism pronounced, male with coxae on anterior four pereopods enormously produced. Coxae of anterior four pereopods of female moderately produced. Pleotelson anteriorly wide. First pereopod attenuated, propodus without setae, carpus slender, often with few setae.
description: Published as part of George, Robert Y., 2001, Desmosomatidae and Nannoniscidae (Crustacea, Isopoda, Asellota) from bathyal and abyssal depths oOE North Carolina and their evolution, pp. 1831-1859 in Journal of Natural History 35 (12) on page 1835, DOI: 10.1080/00222930152667131, http://zenodo.org/record/5275960
GR-MHD disk winds and jets from black holes and resistive accretion disks
Creators: name: Vourellis, Christos
name: Fendt, Christian
name: Qian, Qian
name: Noble, Scott
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We perform GR-MHD simulations of outflow launching from thin accretion disks. As in the non-relativistic case, resistivity is essential for the mass loading of the disk wind. We implemented resistivity in the ideal GR-MHD code HARM3D, extending previous works (Qian et al. 2017, 2018) for larger physical grids, higher spatial resolution, and longer simulation time. We consider an initially thin, resistive disk orbiting the black hole, threaded by a large-scale magnetic flux. As the system evolves, outflows are launched from the black hole magnetosphere and the disk surface. We mainly focus on disk outflows, investigating their MHD structure and energy output in comparison with the Poynting-dominated black hole jet. The disk wind encloses two components -- a fast component dominated by the toroidal magnetic field and a slower component dominated by the poloidal field. The disk wind transitions from sub to super-Alfvénic speed, reaching velocities $\simeq 0.1c$. We provide parameter studies varying spin parameter and resistivity level, and measure the respective mass and energy fluxes. A higher spin strengthens the $B_ϕ$-dominated disk wind along the inner jet. We disentangle a critical resistivity level that leads to a maximum matter and energy output for both, resulting from the interplay between re-connection and diffusion, which in combination govern the magnetic flux and the mass loading. For counter-rotating black holes the outflow structure shows a magnetic field reversal. We estimate the opacity of the inner-most accretion stream and the outflow structure around it. This stream may be critically opaque for a lensed signal, while the axial jet funnel remains optically thin.
description: 27 pages, 31 figures, accepted for publication in ApJ
The QMAP and MAT/TOCO Experiments for Measuring Anisotropy in the Cosmic Microwave Background
Creators: name: Miller, A.
name: Beach, J.
name: Bradley, S.
name: Devlin, M. J.
name: Caldwell, R.
name: Chapman, H.
name: Dorwart, W. B.
name: Herbig, T.
name: Jones, D.
name: Monnelly, G.
name: Netterfield, C. B.
name: Nolta, M.
name: Page, L. A.
name: Puchalla, J.
name: Robertson, T.
name: Torbet, E.
name: Tran, H. T.
name: Vinje, W. E.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe two related experiments that measured the anisotropy in the cosmic microwave background (CMB). QMAP was a balloon-borne telescope that flew twice in 1996, collecting data on degree angular scales with an array of six high electron mobility transistor-based amplifiers (HEMTs). QMAP was the first experiment to use an interlocking scan strategy to directly produce high signal-to-noise CMB maps. The QMAP gondola was then refit for ground based work as the MAT/TOCO experiment. Observations were made from 5200 m on Cerro Toco in Northern Chile in 1997 and 1998 using time-domain beam synthesis. MAT/TOCO was the first experiment to see both the rise and fall of the CMB angular spectrum, thereby localizing the position of the first peak to l_{peak}=216 +/- 14. In addition to describing the instruments, we discuss the data selection methods, checks for systematic errors, and we compare the MAT/TOCO results to those from recent experiments. We also correct the data to account for an updated calibration and a small contribution from foreground emission. We find the amplitude of the first peak for l between 160 and 240 to be T_{peak}=80.9 +/- 3.4 +/- 5.1 uK, where the first error is statistical and the second is from calibration.
description: 31 pages, 11 figures, Submitted to ApJ
Exoclimenella maldivensis Duris & Bruce 1995
Creators: name: Li, Xinzheng
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Palaemonidae
Exoclimenella
Exoclimenella maldivensis

description: Exoclimenella maldivensis Duris & Bruce, 1995
 Exoclimenella maldivensis Duris & Bruce, 1995: 622, figs 1-5. — Li & Bruce 2006: 633.
 MATERIAL EXAMINED. — Austral Is. Rapa I., Pointe Teruametitoi, BENTHAUS, malacologist fieldwork, stn 33, 27°34.8’S, 144°18.6’W, 30 m, dead coral, 19.XI.2002, 1 ♂ (MNHN-Na 15448).
DISTRIBUTION. — Type locality: Maldives. Previously also known from Timor Sea, Loyalty Is; 2-60 m depth. Not previously recorded from French Polynesia.
REMARKS
The specimen has the following rostral formula 2+7/5, the subapical dorsal tooth is tiny.
description: Published as part of Li, Xinzheng, 2008, Report on some species of Palaemonidae (Crustacea, Decapoda) from French Polynesia, pp. 203-252 in Zoosystema 30 (1) on page 206, DOI: 10.5281/zenodo.5390379
SaaS CloudQual: A Quality Model for Evaluating Software as a Service on the Cloud Computing Environment
Creators: name: Jagli, Dhanamma
name: Purohit, Seema
name: Chandra, N. Subash
Publisher: name: arXiv
Year: 2019
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: Abstract The cloud computing is a key computing approach adopted by many organizations in order to share resources. It provides Everything As-A-Service (XaaS). Software-As-A-Service is an important resource on the cloud computing environment. Without installing any software locally, service user can use software as a utility. And enjoy the benefits of SaaS model. Hence SaaS usage is increased drastically, the demand for selecting quality is also increased. This paper presents a novel quality model intended for evaluating software as a service (SaaS), depending on the key features of Software as a service. Because SaaS key features are playing critical role in the quality and differentiating from conventional software quality.
description: 8 Pages
High-accuracy wavemeter based on a stabilized diode laser
Creators: name: Banerjee, Ayan
name: Rapol, Umakant D.
name: Wasan, Ajay
name: Natarajan, Vasant
Publisher: name: arXiv
Year: 2002
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: We have built a high-accuracy wavelength meter for tunable lasers using a scanning Michelson interferometer and a reference laser of known wavelength. The reference laser is a frequency stabilized diode laser locked to an atomic transition in Rb. The wavemeter has a statistical error per measurement of 5 parts in $10^7$ which can be reduced considerably by averaging. Using a second stabilized diode laser, we have verified that systematic errors are below 4 parts in $10^8$.
description: 3 pages, 2 figures
Simulating Low-cost Rotating Panel Designs for the Commercial Buildings Energy Consumption Survey
Creators: name: Sijuwade, Adebowale
name: Lent, Janice
name: Winkler, Michael
Publisher: name: Zenodo
Year: 2024
Subjects: rotating panel surveys
complex surveys
simulation

description: The U.S. Energy Information Administration's (EIA's) Commercial Buildings Energy Consumption Survey (CBECS) is the primary source of data on energy use in the U.S. commercial sector. The survey collects detailed information about commercial building characteristics, energy consuming equipment, and fuel use in commercial buildings. EIA has collected 11 cycles of CBECS data since 1979. Because CBECS data collection is complicated and increasingly expensive, EIA is researching options to potentially reduce costs for future CBECS cycles. Winkler et al, (2022) examined rotating panel designs recommended for CBECS by the National Academy of Sciences (NAS 2012). In this study, we consider low-cost panel designs involving fewer panels and smaller samples within the panels. Simulation results suggest that a longitudinal CBECS, involving dependent interviewing (Ridolfo et al. 2022), may provide useful time-series data despite increased standard errors.
การบริหารราชการส่วนภูมิภาคที่ก่อให้เกิดประสิทธิผลในการพัฒนาประเทศไทย
Creators: name: อธิภัทร สินทรโก
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: การบริหารราชการส่วนภูมิภาค
ประสิทธิผล
การพัฒนาประเทศไทย

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 122-130
Additional file 2 of Causal relationships between genetically determined metabolites and human intelligence: a Mendelian randomization study
Creators: name: Yang, Jian
name: Zhao, Binbin
name: Qian, Li
name: Gao, Fengjie
name: Fan, Yanjuan
name: He, Xiaoyan
name: Ma, Qingyan
name: Yang, Lihong
name: Yan, Bin
name: Wang, Wei
name: Ma, Xiancang
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified

description: Additional file 2: Fig. S2. Mendelian randomization associations of dihomo-linoleate(20:2n6) on other intelligence-related outcomes from other data sources.
การพัฒนาโมเดลเครื่องคำนวณหาค่ามวลน้ำหนักของไก่เนื้อ
Creators: name: ปุญฑรษา อุ่นเลิศ
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: โมเดล
เครื่องคำนวณน้ำหนัก
ไก่เนื้อ
โหลดเซลล์

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 131-140
การจัดการปัญหาราคาผลไม้ตกต่ำในพื้นที่ภาคตะวันออก
Creators: name: ชวโรจน์ แย้มกลิ่น
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: การจัดการปัญหา
ปัญหาราคาผลไม้ไทยตกต่ำ

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 141-149
Additional file 3 of Genetically determined blood pressure, antihypertensive medications, and risk of Alzheimer’s disease: a Mendelian randomization study
Creators: name: Ou, Ya-Nan
name: Yang, Yu-Xiang
name: Shen, Xue-Ning
name: Ma, Ya-Hui
name: Chen, Shi-Dong
name: Dong, Qiang
name: Tan, Lan
name: Yu, Jin-Tai
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3. Genome-wide significant and independent SNPs that were used as instruments for SBP.
Searches for other vacua II: A new Higgstory at the cosmological collider
Creators: name: Hook, Anson
name: Huang, Junwu
name: Racco, Davide
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The detection of an oscillating pattern in the bispectrum of density perturbations could suggest the existence of a high-energy second minimum in the Higgs potential. If the Higgs field resided in this new minimum during inflation and was brought back to the electroweak vacuum by thermal corrections during reheating, the coupling of Standard Model particles to the inflaton would leave its imprint on the bispectrum. We focus on the fermions, whose dispersion relation can be modified by the coupling to the inflaton, leading to an enhanced particle production during inflation even if their mass during inflation is larger than the Hubble scale. This results in a large non-analytic contribution to non-Gaussianities, with an amplitude $f_{\rm NL}$ as large as $100$ in the squeezed limit, potentially detectable in future 21-cm surveys. Measuring the contributions from two fermions would allow us to compute the ratio of their masses, and to ascribe the origin of the signal to a new Higgs minimum. Such a discovery would be a tremendous step towards understanding the vacuum instability of the Higgs potential, and could have fascinating implications for anthropic considerations.
description: 38 pages, 8 figures and 2 tables
State of the Food Supply New Zealand 2019
Creators: name: Mackay, Sally
name: Cliona Ni Mhurchu
name: Swinburn, Boyd
name: Eyles, Helen
name: Young, Leanne
name: Castro, Teresa Gontijo De
Publisher: name: The University of Auckland
Year: 2019
Subjects: subject: 111199 Nutrition and Dietetics not elsewhere classified
subject: FOS: Health sciences

description: This State of the Food Supply report for New Zealand 2019 analyses all packaged food in Nutritrack for healthiness and focuses on the dominant packaged food and beverage companies by market share
Light Curves of Jetted Gamma-Ray Burst Afterglows in Circumstellar Clouds
Creators: name: Dai, Z. G.
name: Huang, Y. F.
name: Lu, T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The afterglow emission from a spreading jet expanding in a circumstellar cloud is discussed. Prompt X-ray radiation and a strong UV flash from the reverse shock produced by the interaction of the jet with the cloud may destroy and clear the dust out to about 30 pc within the initial solid angle of the jet. As the sideways expansion of the jet becomes significant, most of the optical radiation from the high-latitude part of the jet may be absorbed by the dust outside the initial solid angle of the jet, but only the radiation from the part within the initial solid angle can be observed. We analytically show that the flux of the observational radiation decays as $\propto t^{-(p+1)}$ (where $p$ is the power-law index of the electron distribution) in the relativistic phase. This preliminary result motivates us to perform numerical calculations. Our results show that one break in the optical afterglow ligh curve extends over a factor of $\sim 3$ in time rather than one decade in time in the previous jet model. These results may provide a way to judge whether GRBs locate in dense clouds or not. Finally, we carry out a detailed modelling for the R-band afterglow of GRB 000926.
description: 14 Pages, 3 eps figures, in press in MNRAS Lett
Towards lattice-assisted hadron physics calculations based on QCD n-point functions
Creators: name: Sternbeck, André
name: Leutnant, Milena
name: Eichmann, Gernot
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We present preliminary lattice results for the nonperturbative tensor structure of the vector and axial-vector quark-antiquark vertices in QCD. Our lattice calculations are for $N_f=2$ mass-degenerate Wilson fermion flavors whose quark mass values include an almost physical one. We compare our lattice results with the corresponding continuum solutions of the inhomogeneous Bethe-Salpeter equations in a rainbow-ladder truncation. We find similarities in the momentum dependencies of the form factors but also clear deviations at low momentum.
description: 7 pages, 3 figures, Proceedings of the 36th Annual International Symposium on Lattice Field Theory (Lattice 2018), 22-28 July 2018, Michigan State University, East Lansing, Michigan USA
Spectral Statistics for the Dirac Operator on Graphs
Creators: name: Bolte, Jens
name: Harrison, Jonathan
Publisher: name: arXiv
Year: 2002
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We determine conditions for the quantisation of graphs using the Dirac operator for both two and four component spinors. According to the Bohigas-Giannoni-Schmit conjecture for such systems with time-reversal symmetry the energy level statistics are expected, in the semiclassical limit, to correspond to those of random matrices from the Gaussian symplectic ensemble. This is confirmed by numerical investigation. The scattering matrix used to formulate the quantisation condition is found to be independent of the type of spinor. We derive an exact trace formula for the spectrum and use this to investigate the form factor in the diagonal approximation.
Direct measurement of the fine-structure interval in alkali atoms using diode lasers
Creators: name: Banerjee, Ayan
name: Rapol, Umakant D.
name: Natarajan, Vasant
Publisher: name: arXiv
Year: 2002
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We demonstrate a technique for directly measuring the fine-structure interval in alkali atoms using two frequency-stabilized diode lasers. Each laser has a linewidth of order 1 MHz and precise tunability: one laser is tuned to a hyperfine transition in the D_1 line, and the other laser to a hyperfine transition in the D_2 line. The outputs of the lasers are fed into a scanning Michelson interferometer that measures the ratio of their wavelengths accurately. To illustrate the technique, we measure the fine-structure interval in Rb, and obtain a value of 237.6000(3)(5) cm^-1 for the hyperfine-free 5P_{3/2} - 5P_{1/2} interval.
description: 3 pages, 2 figures, to be published in Applied Physics Letters, 20 May 2002 edition
Eugerda Meinert 1890
Creators: name: George, Robert Y.
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Desmosomatidae
Eugerda

description: Genus Eugerda Meinert 1890
 Type species. Eugerda tenuimana (G. O. Sars, 1868)
 Diagnosis. Desmosomatinae with biramous uropod, exopod always well developed. Pleotelson without posterolateral spines. First pereonite shorter than the second pereonite. First pereopod slightly or moderately reduced, carpus lacking major setae. Carpus of second pereopod broad, often with a comb of small spines distoventrally. Sexual dimorphism pronounced, in copulatory male posterior three pereonites and pleotelson with marginal ¯anges. Coxae of ®rst pereopod moderately produced.
 Remarks. The genus is closely related to the genus Desmosoma.
 Eugerda latipes (Hansen, 1916) (®gure 4A±D) Desmosoma latipes Hansen, 1916.
 Material examined. Identi®ed male, length 2.6 mm, width 1.0 mm.
 Locality. Carolina slope at 620 m, Eastward Sta. G-29 (4931).
 Diagnosis. Eugerda with ®rst pereonite strongly reduced. Copulatory male with anterior and posterior corner of ®fth pereonite and pleotelson all rounded. Antennula with a ¯agellum of four articles. First pereopod slender, merus short, carpus broader and longer than propodus, both bearing long setae. Coxae of ®rst pereopod not produced anteriorly. Uropod biramous, exopod much shorter than endopod.
 Remarks. The present record of this species oOE North Carolina is the southernmost location for this North Atlantic boreal, bathyal species. Originally this species was collected during the Danish Ingolf expedition at 1065 m at lat. 63ss30¾N and long. 54ss25¾W. Subsequently Russian carcinologist Professor O. Kussakin collected it from the Grand Banks at 850 m at lat. 44ss56.9¾N and long. 48ss53.3¾W (Hessler, 1970). This same species was collected at six diOEerent stations between 200 and 1102 m in the Gay Head± Bermuda transect (Hessler, 1970).
description: Published as part of George, Robert Y., 2001, Desmosomatidae and Nannoniscidae (Crustacea, Isopoda, Asellota) from bathyal and abyssal depths oOE North Carolina and their evolution, pp. 1831-1859 in Journal of Natural History 35 (12) on pages 1837-1840, DOI: 10.1080/00222930152667131, http://zenodo.org/record/5275960
กลยุทธ์การตลาดเพื่อส่งเสริมขนมไทยท้องถิ่นในจังหวัดนนทบุรี
Creators: name: เจณิภา คงอิ่ม
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: พฤติกรรมผู้บริโภค
ทัศนคติ
ปัจจัยดำเนินงาน
กลยุทธ์การตลาด
ขนมไทยท้องถิ่น

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 150-157
Tensions between the Early and the Late Universe
Creators: name: Verde, L.
name: Treu, T.
name: Riess, A. G.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The standard cosmological model successfully describes many observations from widely different epochs of the Universe, from primordial nucleosynthesis to the accelerating expansion of the present day. However, as the basic cosmological parameters of the model are being determined with increasing and unprecedented precision, it is not guaranteed that the same model will fit more precise observations from widely different cosmic epochs. Discrepancies developing between observations at early and late cosmological time may require an expansion of the standard model, and may lead to the discovery of new physics. The workshop "Tensions between the Early and the Late Universe" was held at the Kavli Institute for Theoretical Physics on July 15-17 2019 (More details of the workshop (including on-line presentations) are given at the website: https://www.kitp.ucsb.edu/activities/enervac-c19) to evaluate increasing evidence for these discrepancies, primarily in the value of the Hubble constant as well as ideas recently proposed to explain this tension. Multiple new observational results for the Hubble constant were presented in the time frame of the workshop using different probes: Cepheids, strong lensing time delays, tip of the red giant branch (TRGB), megamasers, Oxygen-rich Miras and surface brightness fluctuations (SBF) resulting in a set of six new ones in the last several months. Here we present the summary plot of the meeting that shows combining any three independent approaches to measure H$_0$ in the late universe yields tension with the early Universe values between 4.0$σ$ and 5.8$σ$. This shows that the discrepancy does not appear to be dependent on the use of any one method, team, or source. Theoretical ideas to explain the discrepancy focused on new physics in the decade of expansion preceding recombination as the most plausible. This is a brief summary of the workshop.
description: (10 pages 1 figure; summary of KITP conference described at this link https://www.kitp.ucsb.edu/activities/enervac-c19 )
The anomalous properties of Markarian 1460
Creators: name: Trentham, Neil
name: Tully, R. Brent
name: Verheijen, Marc A. W.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present and discuss optical, near-infrared and HI measurements of the galaxy Markarian 1460 at a distance of 19 Mpc in the Ursa Major Cluster. This low-luminosity (M_B = -14) galaxy is unusual because (i) it is blue (B-R=0.8) and has the spectrum of an HII galaxy, (ii) it has a light profile that is smooth and well fit by an r^{1/4} and not an exponential function at all radii larger than the seeing, and (iii) it has an observed central brightness of about mu_B = 20 mag arcsec^{-2}, intermediate between those of elliptical galaxies (on the bright mu_B side) and normal low-luminosity dwarf irregular (on the low mu_B side) galaxies. No other known galaxy exhibits all these properties in conjunction. On morphological grounds this galaxy looks like a normal distant luminous elliptical galaxy, since the fundamental plane tells us that higher luminosity normal elliptical galaxies tend to have lower surface-brightnesses. Markarian 1460 has 2 X 10^7 M_sun of HI and a ratio M(HI)/L_B of 0.2, which is low compared to typical values for star-forming dwarf galaxies. From the high surface brightness and r^{1/4} profile, we infer that the baryonic component of Markarian 1460 has become self-gravitating through dissipative processes. From the colours, radio continuum, HI and optical emission line properties, yet smooth texture, we infer that Markarian 1460 has had significant star formation as recently as about 1 Gyr ago but not today.
description: MNRAS in press
Eugerda svavarssoni George 2001, n. sp.
Creators: name: George, Robert Y.
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Desmosomatidae
Eugerda
Eugerda svavarssoni

description: Eugerda svavarssoni n. sp.
(®gure 4E, F)
 Material examined. Holotype female, length 3.0 mm, width 0.55 mm. USNM Cat. No. 1387333.
 Type locality. Carolina slope at 620 m. Eastward Sta. G-29 (4931).
 Etymology. This species is named in honour of the isopodologist Dr JoÈrundur Svavarsson of the Institute of Biology, University of Iceland, Reykjavik, Iceland.
 Diagnosis of the female. Body six times longer than the tergal width of the third pereonite. First pereonite shorter than the second pereonite, about as long as the fourth pereonite. Third pereonite more than twice the length of the fourth pereonite. Fifth and sixth pereonites subequal, long and cylindrical in shape, each longer than the seventh pereonite. Pleotelson elliptical in shape. Coxal plates of the ®rst pereopod not dorsally visible and that of the second, third and fourth pereopods rounded and not well developed.
 Description. Cephalon as long as the ®rst and second pereonites combined. Frontal margin of cephalon somewhat truncated. Antennula composed of six articles, basal peduncular article broad, twice as wide as the second article and with a long distal seta. Flagellum of four articles, terminal article with long apical setae.
 Remarks. The pereopod morphology is not given since the type specimen was found to lack all the pereopods. This new species resembles both E. setifera Hessler, 1970 and E. pannosa Hessler, 1970 in having the ®fth and sixth pereonites long and cylindrical in shape. However, these two species are distinguished from the new species by the presence of small setae on the body surface. In E. svavarssoni the body surface is smooth and also the coxal plates are poorly developed in this new species (female).
description: Published as part of George, Robert Y., 2001, Desmosomatidae and Nannoniscidae (Crustacea, Isopoda, Asellota) from bathyal and abyssal depths oOE North Carolina and their evolution, pp. 1831-1859 in Journal of Natural History 35 (12) on page 1840, DOI: 10.1080/00222930152667131, http://zenodo.org/record/5275960
Magnetic Structure of Nano-Graphite Moebius Ribbon
Creators: name: Wakabayashi, Katsunori
name: Harigaya, Kikuo
Publisher: name: arXiv
Year: 2002
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Mathematical Physics (math-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We consider the electronic and magnetic properties of nanographite ribbon with zigzag edges under the periodic or Moebius boundary conditions. The zigzag nano-graphite ribbons possess edge localized states at the Fermi level which cause a ferrimagnetic spin polarization localized at the edge sites even in the very weak Coulomb interaction. The imposition of the Moebius boundary condition makes the system non-AB-bipartite lattice, and depress the spin polarization, resulting in the formation of a magnetic domain wall. The width of the magnetic domain depends on the Coulomb interaction and narrows with increasing U/t.
description: 4 pages; 6 figures; published at J. Phys. Soc. Jpn. Vol. 72 No. 5 pp. 998-1001 (2003)
Observation of sub-natural linewidths for cold atoms in a magneto-optic trap
Creators: name: Rapol, Umakant D.
name: Wasan, Ajay
name: Natarajan, Vasant
Publisher: name: arXiv
Year: 2002
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We have studied the absorption of a weak probe beam through cold rubidium atoms in a magneto-optic trap. The absorption spectrum shows two peaks with the smaller peak having linewidth as small as 28% of the natural linewidth. The modification happens because the laser beams used for trapping also drive the atoms coherently between the ground and excited states. This creates ``dressed'' states whose energies are shifted depending on the strength of the drive. Linewidth narrowing occurs due to quantum coherence between the dressed states. The separation of the states increases with laser intensity and detuning, as expected from this model.
description: 8 pages, 4 figures
เศรษฐศาสตร์การเมืองว่าด้วยความขัดแย้งทางวาทกรรมของการแพทย์แผนปัจจุบัน การแพทย์แผนไทย การแพทย์ทางเลือกเกี่ยวกับการปฏิรูปทางการแพทย์
Creators: name: จรัสศรี รูปขำดี
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: วาทกรรมการแพทย์แผนปัจจุบัน
วาทกรรมการแพทย์แผนไทย
วาทกรรมการแพทย์ทางเลือก
การปฏิรูปทางการแพทย์

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 158-167
Constraining the scalar-tensor gravity theories with and without screening mechanisms by combined observations
Creators: name: Zhang, Xing
name: Niu, Rui
name: Zhao, Wen
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Screened modified gravity (SMG) and Brans-Dicke (BD) gravity are typical examples of scalar-tensor theories with and without screening mechanisms, which can suppress the scalar field in dense regions. In this paper, we investigate the tests of time-varying gravitational constant $G$, gravitational dipole radiation, and Nordtvedt effect in BD and SMG theories, respectively. We place new constraints on these theories by combining Cassini experiment, lunar laser ranging (LLR) measurements, and pulsar observations from PSRs J1738$+$0333 and J0348$+$0432. We find that screening mechanism has important influence on theoretical constraints. The strongest, second, and weakest constraints on BD are from Cassini, pulsar, and LLR tests, respectively. The most stringent constraint on SMG comes from LLR measurements and improves the previous best constraint by more than seven orders of magnitude. We derive the bounds on the cosmological evolution of the scalar background in these theories using the time variation of $G$. The results of all tests agree well with general relativity (GR) and give more stringent constraints on the deviations from GR. Finally, as an example, we consider the chameleon model and derive the constraints on the model parameters.
description: 6 pages, 2 figures, 1 table, Phys. Rev. D accepted
Eugerdellatinae Hessler 1970
Creators: name: George, Robert Y.
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Desmosomatidae

description: SUBFAMILYEUGERDELLATINAE Hessler, 1970    Diagnosis. Desmosomatidae with ®rst pereopod chelate or raptorial, more strongly developed than the second pereopod, its distal articles forming the robust grasping structure. First pereonite as large as or larger than the second pereonite.
description: Published as part of George, Robert Y., 2001, Desmosomatidae and Nannoniscidae (Crustacea, Isopoda, Asellota) from bathyal and abyssal depths oOE North Carolina and their evolution, pp. 1831-1859 in Journal of Natural History 35 (12) on page 1840, DOI: 10.1080/00222930152667131, http://zenodo.org/record/5275960
Kemponia ensifrons
Creators: name: Li, Xinzheng
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Palaemonidae
Kemponia
Kemponia ensifrons

description: Kemponia ensifrons (Dana, 1852)
 Anchistia ensifrons Dana, 1852: 25.
 Periclimenes ensifrons – Nobili 1907: 359.— Chace & Bruce 1993: 111. — Poupin 1998: 16. — Li 2000: 180.
 Kemponia ensifrons – Bruce 2004b: 15. — Li & Bruce 2006: 644, figs 4, 5.
 MATERIAL EXAMINED. — Austral Is. Rapa I., Mei Point, BENTHAUS, malacologist fieldwork, stn 30, 27°38.2’S, 144°18.2’W, 16-20 m, dead coral, above barrier, 16- 18.XI.2002, 2 ♀♀ (1 ovig.) (MNHN-Na 15468). —Teruametitoi Point, BENTHAUS, malacologist fieldwork, stn 33, 27°34.8’S, 144°18.6’W, 30 m, dead coral, 19.XI.2002, 1 ovig. ♀ (MNHN-Na 15469).
DISTRIBUTION. — Type locality: Balabac Strait, North Borneo. Previously also reported from Egyptian Red Sea, Zanzibar, Comoro Is, Seychelles, Burma, China, Papua New Guinea, New Caledonia, Marshall Is and French Polynesia (Tuamotu Is); 0-35 m depth. Not reported previously from Austral Is.
REMARKS
The present specimens have the carpus of second pereiopod long, about 1.3 times the merus length, subequal or distinctly longer than the palm, unarmed distally; rostral dentition is 1+6-8/2.
description: Published as part of Li, Xinzheng, 2008, Report on some species of Palaemonidae (Crustacea, Decapoda) from French Polynesia, pp. 203-252 in Zoosystema 30 (1) on page 215, DOI: 10.5281/zenodo.5390379
Additional file 9 of The lungs were on fire: a pilot study of 18F-FDG PET/CT in idiopathic-inflammatory-myopathy-related interstitial lung disease
Creators: name: Liang, Junyu
name: Cao, Heng
name: Liu, Yinuo
name: Ye, Bingjue
name: Sun, Yiduo
name: Ke, Yini
name: He, Ye
name: Xu, Bei
name: Lin, Jin
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 9. Comparisons of bilateral lung SUVmean and spleen SUVmean in RP-ILD patients with different survival
ความน่าเชื่อถือของพยานหลักฐานทางนิติวิทยาศาสตร์: ปัญหา สาเหตุ และแนวทางการพัฒนาสำหรับประเทศไทย
Creators: name: วราภรณ์ พรหมวิกร
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: ความน่าเชื่อถือ
พยานหลักฐาน
นิติวิทยาศาสตร์

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 168-180
The Antecedent Effects of Human Resource Development Capability of Auto Parts Businesses in Thailand
Creators: name: Aphi Khamphroh
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: Human Resource Development
Transformational Leadership Orientation
Human Capital Policy
Organizational Resource Readiness
IT Capability
Environmental Complexity Force

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 181-192
The Effect of Servicescape on Customer Satisfaction
Creators: name: Chatchai Inthasang
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: Servicescape
Place Attachment
Customer Satisfaction

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 193-204
Exact solutions of domain wall and spiral ground states in Hubbard models
Creators: name: Homma, Makoto
name: Itoi, Chigak
Publisher: name: arXiv
Year: 2002
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Lattice (hep-lat)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We construct a set of exact ground states with a localized ferromagnetic domain wall and an extended spiral structure in a deformed flat-band Hubbard model. In the case of quarter filling, we show the uniqueness of the ground state with a fixed magnetization. We discuss more realistic situation given by a band-bending perturbation, which can stabilize these curious structures. We study the scattering of a conduction electron by the domain wall and the spiral spins.
description: 4 pages, 2 figures. To be published in J. Phys. Soc. Jpn. 73 (2004)
East Versus West: Eastern Man and Western Man in the Novel of Shanghai Baby
Creators: name: Aphiradi Suphap
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: Chinese Patriarchy
Masculinity
Chinese Men
Shanghai Baby

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 205-215
Loading of a Rb magneto-optic trap from a getter source
Creators: name: Rapol, Umakant D.
name: Wasan, Ajay
name: Natarajan, Vasant
Publisher: name: arXiv
Year: 2002
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We study the properties of a Rb magneto-optic trap loaded from a commercial getter source which provides a large flux of atoms for the trap along with the capability of rapid turn-off necessary for obtaining long trap lifetimes. We have studied the trap loading at two different values of background pressure to determine the cross-section for Rb--N$_2$ collisions to be 3.5(4)x10^{-14} cm^2 and that for Rb--Rb collisions to be of order 3x10^{-13} cm^2. At a background pressure of 1.3x10^{-9} torr, we load more than 10^8 atoms into the trap with a time constant of 3.3 s. The 1/e lifetime of trapped atoms is 13 s limited only by background collisions.
description: 5 pages, 5 figures
การท่องเที่ยวเพื่อ (คุณภาพ) ชีวิต
Creators: name: สรรค์นันธ์ ตันติอุโฆษกุล อัครวงศ์
Publisher: name: วิทยาลัยเทคโนโลยีภาคใต้
Year: 2562
Subjects: การท่องเที่ยว
คุณภาพชีวิต
ชีวิต

description: วารสารเทคโนโลยีภาคใต้, 12, 2, 216-227
Palaemonella lata Kemp 1922
Creators: name: Li, Xinzheng
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Decapoda
Palaemonidae
Palaemonella
Palaemonella lata

description: Palaemonella lata Kemp, 1922
 Palaemonella lata Kemp, 1922: 127-129, figs 3- 6. — Odinetz 1983: 207. — Chace & Bruce 1993: 89. — Poupin 1998: 15. — Li 2000: 103, fig. 112.
 MATERIAL EXAMINED. — Society Is. Tahiti, coll. Odinetz, 1 ♀ (MNHN-Na 6622).
DISTRIBUTION. — Type locality: Port Blair, Andaman Is. Previously reported also from Zanzibar, la Réunion, Indonesia, Hawaii, and French Polynesia (Society Is); littoral. Previously recorded from the Society Islands by Odinetz (1983) and Poupin (1998).
REMARKS
The only specimen examined (cl 3.58 mm) has a rostral dentition of 3+5/3. There is no trace of any supraorbital ridge or tubercle, but a postorbital ridge is distinct. The second pereiopods are subequal and similar, the carpus with upper and lower distomedial teeth and the merus without a lateral distoventral tooth. The third ambulatory pereiopod has the dactyl relatively long and slender in comparison with the type specimen described by Kemp (1922), about 0.3 times the propod length, opposed to 0.26 in the type, and about 6.0 times longer than its proximal depth, instead of about 4.0 times in the type.
description: Published as part of Li, Xinzheng, 2008, Report on some species of Palaemonidae (Crustacea, Decapoda) from French Polynesia, pp. 203-252 in Zoosystema 30 (1) on page 217, DOI: 10.5281/zenodo.5390379
The Nature of the Nuclear H2O Masers of NGC 1068: Reverberation and Evidence for a Rotating Disk Geometry
Creators: name: Gallimore, J. F.
name: Henkel, C.
name: Baum, S. A.
name: Glass, I. S.
name: Claussen, M. J.
name: Prieto, M. A.
name: von Kap-Herr, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report new (1995) Very Large Array observations and (1984 - 1999) Effelsberg 100m monitoring observations of the 22 GHz H2O maser spectrum of the Seyfert 2 galaxy NGC 1068. The sensitive VLA observations provide a registration of the 22 GHz continuum emission and the location of the maser spots with an accuracy of ~ 5 mas. Within the monitoring data, we find evidence that the nuclear masers vary coherently on time-scales of months to years, much more rapidly than the dynamical time-scale. We argue that the nuclear masers are responding in reverberation to a central power source, presumably the central engine. Between October and November 1997, we detected a simultaneous flare of the blue-shifted and red-shifted satellite maser lines. Reverberation in a rotating disk naturally explains the simultaneous flaring. There is also evidence that near-infrared emission from dust grains associated with the maser disk also responds to the central engine. We present a model in which an X-ray flare results in both the loss of maser signal in 1990 and the peak of the near-infrared light curve in 1994. In support of a rotating disk geometry for the nuclear masers, we find no evidence for centripetal accelerations of the redshifted nuclear masers; the limits are +/- 0.006 km/s/year, implying that the masers are located within 2 degrees of the kinematic line-of-nodes. We also searched for high velocity maser emission like that observed in NGC 4258. In both VLA and Effelsberg spectra, we detect no high velocity lines between +/- 350 km/s to +/- 850 km/s relative to systemic, arguing that masers only lie outside a radius of ~ 0.6 pc (1.9 light years) from the central engine (assuming a distance of 14.4 Mpc).
description: 62 pages, 19 figures
Prochelator Hessler 1970
Creators: name: George, Robert Y.
Publisher: name: Zenodo
Year: 2001
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Desmosomatidae
Prochelator

description: Genus Prochelator Hessler, 1970
 Type species. Prochelator lateralis (G. O. Sars, 1899).
 Diagnosis. First pereopod large, chelate. Dactylus and enlarged propodus together forming a movable ®nger which acts in opposition to immovable claw formed by large stout spine on the distal inner margin of enlarged carpus. Inner margin of carpus with two accessory setae and long slender seta, located at the base of the ®xed claw. First pereonite as large as or larger than second pereonite. Pleotelson with posterolateral spines that are sometimes obscure or absent. Uropod biramous. Coxae of anterior four pereopods not produced.
description: Published as part of George, Robert Y., 2001, Desmosomatidae and Nannoniscidae (Crustacea, Isopoda, Asellota) from bathyal and abyssal depths oOE North Carolina and their evolution, pp. 1831-1859 in Journal of Natural History 35 (12) on page 1840, DOI: 10.1080/00222930152667131, http://zenodo.org/record/5275960
Crystal field splitting, local anisotropy, and low energy excitations in the quantum magnet YbCl$_3$
Creators: name: Sala, G.
name: Stone, M. B.
name: Rai, Binod K.
name: May, A. F.
name: Parker, D. S.
name: Halász, Gábor B.
name: Cheng, Y. Q.
name: Ehlers, G.
name: Garlea, V. O.
name: Zhang, Q.
name: Lumsden, M. D.
name: Christianson, A. D.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study the correlated quantum magnet, YbCl$_3$, with neutron scattering, magnetic susceptibility, and heat capacity measurements. The crystal field Hamiltonian is determined through simultaneous refinements of the inelastic neutron scattering and magnetization data. The ground state doublet is well isolated from the other crystal field levels and results in an effective spin-1/2 system with local easy plane anisotropy at low temperature. Cold neutron spectroscopy shows low energy excitations that are consistent with nearest neighbor antiferromagnetic correlations of reduced dimensionality.
description: main paper plus supplemental information
An integrative approach unveils speciation within the threatened spider Calathotarsus simoni (Araneae: Mygalomorphae: Migidae)
Creators: name: Ferretti, Nelson E.
name: Soresi, Daniela S.
name: González, Alda
name: Arnedo, Miquel
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified

description: The mygalomorph trapdoor spider family Migidae displays a quintessential Gondwanan distribution, including species in Australia, Africa, Madagascar, New Zealand, New Caledonia, and the southern cone of South America. The Argentinean fauna consists of a single species, Calathotarsus simoni Schiapelli & Gerschman, 1975, with a highly localized distribution range restricted to two mountain ranges in the southern Buenos Aires province, central Argentina. The recent discovery of specimens from new localities including adult males and females revealed morphological differences. Similarly, a molecular phylogenetic analysis using mitochondrial and nuclear markers distinguished two main lineages within C. simoni, showing genetic divergence in the levels reported for other species within the family. The two lineages corresponded to each of the two main ranges inhabited by the species and matched the morphological differences observed. Finally, an ecological niche modelling analysis revealed significant ecological differences between the lineages inhabiting the two mountain ranges. Based on integration of all the evidence, the new species Calathotarsus fangioi sp. nov. is described. The new species is circumscribed to the easternmost mountain range of Tandilia, while the distribution C. simoni is re-delimited to include only the western range of Ventania. Both species are diagnosed, described, and illustrated. This new species description and the conservation status for these remarkable spiders are further discussed.
Additional file 7 of The lungs were on fire: a pilot study of 18F-FDG PET/CT in idiopathic-inflammatory-myopathy-related interstitial lung disease
Creators: name: Liang, Junyu
name: Cao, Heng
name: Liu, Yinuo
name: Ye, Bingjue
name: Sun, Yiduo
name: Ke, Yini
name: He, Ye
name: Xu, Bei
name: Lin, Jin
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 7. Univariate Cox proportional hazards regression analyses of survival in IIM-ILD patients
Unveiling molecular clouds toward bipolar HII region G8.14+0.23
Creators: name: Dewangan, L. K.
name: Sano, H.
name: Enokiya, R.
name: Tachihara, K.
name: Fukui, Y.
name: Ojha, D. K.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Most recent numerical simulations suggest that bipolar HII regions, powered by O-type stars, can be formed at the interface of two colliding clouds. To observationally understand the birth of O-type stars, we present a detailed multi-wavelength analysis of an area of 1 deg x 1 deg hosting G8.14+0.23 HII region associated with an infrared bipolar nebula (BPN). Based on the radio continuum map, the HII region is excited by at least an O-type star, which is located toward the waist of the BPN. The NANTEN2 13CO line data reveal the existence of two extended clouds at [9, 14.3] and [15.3, 23.3] km/s toward the site G8.14+0.23, which are connected in the position-velocity space through a broad-bridge feature at the intermediate velocity range. A "cavity/intensity-depression" feature is evident in the blueshifted cloud, and is spatially matched by the "elongated redshifted cloud". The spatial and velocity connections of the clouds suggest their interaction in the site G8.14+0.23. The analysis of deep near-infrared photometric data reveals the presence of clusters of infrared-excess sources, illustrating ongoing star formation activities in both the clouds. The O-type star is part of the embedded cluster seen in the waist of the BPN, which is observed toward the spatial matching zone of the cavity and the redshifted cloud. The observational results appear to be in reasonable agreement with the numerical simulations of cloud-cloud collision (CCC), suggesting that the CCC process seems to be responsible for the birth of the O-type star in G8.14+0.23.
description: 16 pages, 9 figures, Accepted for publication in The Astrophysical Journal