cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 3 of A near complete genome for goat genetic and genomic research
Creators: name: Li, Ran
name: Yang, Peng
name: Dai, Xuelei
name: Asadollahpour Nanaei, Hojjat
name: Fang, Wenwen
name: Yang, Zhirui
name: Cai, Yudong
name: Zheng, Zhuqing
name: Wang, Xihong
name: Jiang, Yu
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Table S1. The publicly available miRNA-seq data used for miRNA annotation. We downloaded publicly available miRNA-seq data to annotate miRNA genes. Table S2. Summary of raw reads from PacBio sequencing. The data summarized the reads counts and length of PacBio sequencing. Table S3. Comparison of the basic statistics of the Saanen_v1 and ARS1 assemblies. The assembly length and continuity were compared between Saanen_v1 and ARS1. Table S4. Comparison of the repeat content of Saanen_v1 with ARS1. The total repeat content of Saanen_v1 was slightly higher than ARS1. The unplaced scaffolds from each assembly were not included for comparison. Table S5. Telomere signals identified in each assembly. Telomeres were found on 27 chromosomes of Saanen_v1 compared with 7, 6 and 5 chromosomes of ARS1, sheep (Oar_rambouillet_v1.0) and cattle (ARS-UCD1.2), respectively. Table S6. Centromere signals identified in each assembly. Saanen_v1 harbors more and longer centromeric repeats per chromosome than the other three assemblies of the reference genome for goat (ARS1), sheep (Oar_rambouillet_v1.0) and cattle (ARS-UCD1.2). Table S7. Structural inconsistencies when comparing Saanen_v1 and ARS1 assemblies. Various categories of structural inconsistencies were compared between Saanen_v1 and ARS1 using the FRC_align tool. Table S8. Mapping ratio of whole-genome sequencing data. Four whole-genome sequencing data of domestic goats were aligned to Saanen_v1 and ARS1 to compare the mapping ratio. Table S9. Mapping ratio of RNA-seq data. Nine RNA-seq datasets were aligned to Saanen_v1 and ARS1 to compare the mapping ratio. Table S10. Mapping ratio of Iso-seq data. Four Iso-seq datasets were aligned to Saanen_v1 and ARS1 to compare the mapping ratio. Table S11. Summary of structural variations in Saanen_v1 as compared with ARS1. The data represented the count and total length of structural variations in Saaenen_v1 as compared with ARS1. Table S13. Blast alignment of previously reported goat Y chromosome amplicons to the Y chromosome assembly included in Saanen_v1. The previously reported goat Y chromosome amplicons could be aligned to our generated Y chromosome assembly, implying the validity of our sequence. Table S15. Information on the large gap regions (> 1 Mb) between two adjacent SNP probes. The data presented seven large gap regions which were not covered by SNP probes.
Magnetosphere of a spinning black hole and the role of the current sheet
Creators: name: East, William E.
name: Yang, Huan
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We revisit the problem of a spinning black hole immersed in a uniformly magnetized plasma within the context of force-free electrodynamics. Such configurations have been found to relax to stationary jetlike solutions that are powered by the rotational energy of the black hole. We write down an analytic description for the jet solutions in the low black hole spin limit, and demonstrate that it provides a good approximation to the configurations found dynamically. For characterizing the magnetospheres of rapidly spinning black holes, we find that the current sheet which forms in the black hole ergosphere plays an essential role. We study the properties of the current sheet, and its importance in determining the jet solution and the rate at which energy is extracted from the black hole.
description: 10 pages, 8 figures; revised to match PRD version
Reminiscences of Arthur C. Lundahl, 1981
Publisher: name: Columbia University
Year: 2021
Subjects: Photographers
Photography, Military
Photogrammetry
Photographic interpretation (Military science)

description: Childhood, education in Chicago; BS and graduate work at University of Chicago 1933-42; World War II service Navy: officer at Navy Radio Operators School, student Navy photointerpretation, assignments in Aleutians and Washington DC; civil service photointerpreter, Navy and Central Intelligence Agency from 1946 to retirement; U-2 incident; Open Skies for Peace program; Cuban missile crisis; improvements in photointerpretation: comparison of American and European equipment; National Photointerpretation Center: establishment, incentive program, equal opportunity application; future use of photointerpretation: natural disaster predictions, food source location, mapping, computers; American Society of Photogrammetry; stereo photography; philosophy of photography
Magnetic phases of skyrmion-hosting GaV$_4$S$_{8-y}$Se$_{y}$ ($y = 0, 2, 4, 8$) probed with muon spectroscopy
Creators: name: Franke, Kévin J. A.
name: Huddart, Benjamin M.
name: Hicken, Thomas J.
name: Xiao, Fan
name: Blundell, Stephen J.
name: Pratt, Francis L.
name: Crisanti, Marta
name: Barker, Joel
name: Clark, Stewart J.
name: Štefančič, Aleš
name: Hatnean, Monica Ciomaga
name: Balakrishnan, Geetha
name: Lancaster, Tom
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present the results of a muon-spin spectroscopy investigation of GaV$_4$S$_{8-y}$Se$_{y}$ with $y=0, 2, 4$ and 8. Zero-field measurements suggest that GaV$_{4}$Se$_{8}$ and GaV$_{4}$S$_{8}$ have distinct magnetic ground states, with the latter material showing an anomalous temperature-dependence of the local magnetic field. It is not possible to evolve the magnetic state continuously between these two systems, with the intermediate $y=2$ and $4$ materials showing glassy magnetic behaviour at low temperature. The skyrmion lattice (SkL) phase is evident in the $y=0$ and 8 materials through an enhanced response of the muon-spin relaxation to the emergent dynamics that accompany the SkL. For our polycrystalline samples of GaV$_4$Se$_{8}$, this enhanced dynamic response is confined to a smaller region of the magnetic field-temperature phase diagram than the previous reports of the SkL in single crystals.
Quantum Cryptography
Creators: name: Hughes, Richard J.
name: Alde, D. M.
name: Dyer, P.
name: Luther, G. G.
name: Morgan, G. L.
name: Schauer, M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum cryptography is a new method for secret communications offering the ultimate security assurance of the inviolability of a Law of Nature. In this paper we shall describe the theory of quantum cryptography, its potential relevance and the development of a prototype system at Los Alamos, which utilises the phenomenon of single-photon interference to perform quantum cryptography over an optical fiber communications link.
description: 36 pages in compressed PostScript format, 10 PostScript figures compressed tar file
A Unifying View of the Spectral Energy Distributions of Blazars
Creators: name: Fossati, G.
name: Maraschi, L.
name: Celotti, A.
name: Comastri, A.
name: Ghisellini, G.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We collect data from the radio to the gamma-ray range for three complete samples of blazars: the Slew Survey and the 1Jy samples of BL Lacs and the 2Jy sample of Flat Spectrum Radio-Loud Quasars (FSRQs). The fraction of objects detected in gamma-rays (E > 100 MeV) is 17%, 26% and 40% in the three samples respectively. Except for the Slew Survey sample, gamma-ray detected sources do not differ either from other sources in each sample, nor from all the gamma-ray detected sources, in terms of the distributions of redshift, radio and X-ray luminosities and of the broad band spectral indices (radio to optical and radio to X-ray). We compute average Spectral Energy Distributions (SEDs) from radio to gamma rays for groups of blazars binned according to radio luminosity, irrespective of the original classification as BL Lac or FSRQ. The resulting SEDs show a remarkable continuity in that: i) the first peak occurs in different frequency ranges for different luminosity classes, with most luminous sources peaking at lower frequencies; ii) the peak frequency of the gamma-ray component correlates with the peak frequency of the lower energy one; iii) the luminosity ratio between the high and low frequency components increases with bolometric luminosity. The continuity of properties among different classes of blazars and the systematic trends of the SEDs as a function of luminosity favor a unified view of the blazar phenomenon: a single parameter, related to luminosity, seems to govern the physical properties and radiation mechanisms in the relativistic jets present in BL Lac objects as well as in FSRQ. The general implications of this unified scheme are discussed.
description: Revised version submitted to Monthly Notices of the R.A.S. 15 pages, 13 Postscript figures, 1 Postscript Table. Uses psfig.sty (included)
Predicted microlensing events from analysis of Gaia Data Release 2
Creators: name: Bramich, D. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Astrometric microlensing can be used to make precise measurements of the masses of lens stars that are independent of their assumed internal physics. Such direct mass measurements, obtained purely by observing the gravitational effects of the stars on external objects, are crucial for validating theoretical stellar models. Specifically, astrometric microlensing provides a channel to direct mass measurements of single stars for which so few measurements exist. To use the astrometric solutions and photometric measurements of ~1.7 billion stars from Gaia Data Release 2 to predict microlensing events during the nominal Gaia mission and beyond. This will enable astronomers to observe the entirety of each event with appropriate observing resources. The data will allow precise lens mass measurements for white dwarfs and low-mass main sequence stars helping to constrain stellar evolutionary models. I search for source-lens pairs in GDR2 that could lead to events between 25/07/2014 and 25/07/2026. I estimate lens masses using GDR2 photometry and parallaxes, and appropriate model isochrones. Combined with source and lens parallax measurements from GDR2, this allows the Einstein radius to be computed for each pair. By considering the paths on the sky, I calculate the microlensing signals that are to be expected. I present a list of 76 predicted microlensing events. 9 and 5 astrometric events will be caused by LAWD37 and Stein2051B. 9 events will exhibit detectable photometric and astrometric signatures. Of the remaining events, ten will exhibit astrometric signals with amplitudes above 0.5 mas, while the rest are low-amplitude astrometric events with amplitudes between 0.131 and 0.5 mas. 5 and 2 events will reach their peaks during 2018 and 2019. 5 of the photometric events have the potential to evolve into high-magnification events, which may also probe for planetary companions to the lenses.
description: Accepted A&A
Conus imperialis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Conidae
Conus
Conus imperialis

description: Conus imperialis [spec. nov.]
C. testa albida: fasciis lividis cingulisque linearibus albo fuscoque articulatis.
Rumph. mus. t. 34. f. H. I.
Gvalt. test. t. 22. f. A.
Argenv. conch. t. 15. f. F.
Kratzenst. Regenf. 12. t. 3. f. 35.
Habitat ..
Testa saepius coronata, albida maculis confluentibus caesiis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 712, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Global effects of climate change on animal population dynamics
Creators: name: Garcia-Carreras, Bernardo
Publisher: name: Imperial College London
Year: 2012

description: Climate change affects many statistical descriptions of the environment. The impact of changes in mean environmental conditions on animal populations has been widely reported. The variability and autocorrelation of environmental variables are also changing over time, yet less research has focussed on what impact these changes may have on populations. Is the research focus on changes in mean conditions justified? How do changes in different statistical descriptions of climate change affect populations, and how do the impacts compare? To answer these questions, we developed a simple stochastic population model, explicitly linked to the environment, and compared the impacts of changes in environmental mean and variability. We found, using both the long-term stochastic growth rate and extinction risk as proxies for population fitness, that changes in variability have a significant impact on population dynamics. The main gradient along which the relative importance of changes in environmental mean and variability varied was the population's distance from its ideal environment. We also re-analysed existing population models to yield the sensitivity of the population to changes in environmental mean and variability. Results support the findings from our model, and confirm the importance of changes in variability for population dynamics. Previous theoretical and laboratory studies concluded that the autocorrelation in the environment in part affects the autocorrelation in population time series. So far, this hypothesis has not been tested using empirical data. We used a database of population time series to find that the autocorrelation in mean summer temperature is significantly correlated with the autocorrelation in population time series. Results also show that environmental variables have become less autocorrelated in most geographical regions, suggesting that populations' autocorrelation may also be changing. Autocorrelation in population time series has been linked to extinction; these results may therefore have important implications for animal populations.
The image separation-source redshift relation for gravitational lenses as a cosmological test
Creators: name: Helbig, Phillip
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recently, Park & Gott claimed that there is a statistically significant, strong, negative correlation between the image separation and source redshift for gravitational lenses. This is somewhat puzzling if one believes in a flat (k = 0) universe, since in this case the typical image separation is expected to be independent of the source redshift, while one expects a negative correlation in a k = -1 universe and a positive one in a k = +1 universe. Park & Gott explored several effects which could cause the observed correlation, but no combination of these can explain the observations with a realistic scenario. Here, I explore this test further in three ways. First, I show that in an inhomogeneous universe a negative correlation is expected regardless of the value of k. Second, I test whether the image separation-source redshift relation can be used as a test to determine lambda and Omega, rather than just the sign of k. Third, I compare the results of the test from the Park & Gott sample to those using other samples of gravitational lenses, which can illuminate (unknown) selection effects and probe the usefulness of the image separation-source redshift relation as a cosmological test.
description: 5 pages, 3 included figures, accepted for publication in MNRAS
Gregory-Laflamme instability of black hole in Einstein-scalar-Gauss-Bonnet theories
Creators: name: Myung, Yun Soo
name: Zou, De-Cheng
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We investigate the stability analysis of Schwarzschild black hole in Einstein-scalar-Gauss-Bonnet (ESGB) theory because the instability of Schwarzschild black hole without scalar hair implies the Gauss-Bonnet black hole with scalar hair. The linearized scalar equation is compared to the Lichnerowicz-Ricci tensor equation in the Einstein-Weyl gravity. It turns out that the instability of Schwarzschild black hole in ESGB theory is interpreted as not the tachyonic instability, but the Gregory-Laflamme instability of black string. In the small mass regime of $1/λ<1.174/r_+$, the Schwarzschild solution becomes unstable and a new branch of solution with scalar hair bifurcates from the Schwarzschild one. This is very similar to finding a newly non-Schwarzschild black hole in Einstein-Weyl gravity.
description: 14 pages, 4 figures, version to appear in Physical Review D
Gravity in a warped 6D world with an extra 2D sphere
Creators: name: Kokado, Akira
name: Saito, Takesi
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Corrections to Newton's inverse law have been so far considered, but not clear in warped higher dimensional worlds, because of complexity of the Einstein equation. Here we give a model of a warped 6D world with an extra 2D sphere. We take a general energy-momentum tensor, which does not depend on a special choice of bulk matter fields. The 6D Einstein equation reduces to the spheroidal differential equation, which can be easily solved. The gravitational potential in our 4D universe is calculated to be composed of infinite series of massive Yukawa potentials coming from the KK mode, together with Newton's inverse law. The series of Yukawa type potentials converges well to behave as $1/r^3$ near $r=0$.
description: 12 pages, No figures
Reminiscences of Arthur Goldschmidt, 1995
Publisher: name: Columbia University
Year: 2021
Subjects: Civil service
Dams--Design and construction
Germans--Texas
Immigrants--Texas
New Deal, 1933-1939
Power resources--United States
Public service employment--United States
Public works
Reclamation of land--United States
Water resources development--United States

description: Childhood: reminiscences of Fredericksburg, southern politics; education: Brackenridge High School (1927), AB Columbia University (1928-1932); thoughts about depression-era political issues in New York: Social Problems Club at Columbia, Roosevelt and La Guardia campaigns; creation of work relief programs during the Great Depression: National Recovery Administration, Civil Works Administration, Civilian Conservation Corps, Historic American Buildings Survey, Writer Project; other work: railroad investigation, United Federal Workers Union (1930s); impressions of Lyndon B. Johnson; career at Public Works Administration, Power Division (1938-1947): distribution of power, dam construction, river management, Southern Report, Federal Power Act, Tennessee Valley Authority Act, Flood Control and Harbors Act; ideas about atomic power, aluminum production during World War II; development National Rural Electrification Co-ops Association; work in the United Nations (1950-1970s): African river basin development, East Asian work, Australian Snow River Project, Mu River work, Mekong River Project, development of Middle East Technical Institute, Latin American economic training; United States Ambassador to ECOSOC (1967-1969); post-United Nations consulting; thoughts about Desert Storm
Higher order Schmidt decompositions
Creators: name: Peres, Asher
Publisher: name: arXiv
Year: 1995
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Necessary and sufficient conditions are given for the existence of extended Schmidt decompositions, with more than two subspaces.
description: LaTeX 3 pages
Additional file 1 of Evaluation of the theranostic potential of [64Cu]CuCl2 in glioblastoma spheroids
Creators: name: Pinto, Catarina I. G.
name: Branco, André D. M.
name: Bucar, Sara
name: Fonseca, Alexandra
name: Abrunhosa, Antero J.
name: da Silva, Cláudia L.
name: Guerreiro, Joana F.
name: Mendes, Filipa
Publisher: name: figshare
Year: 2024
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1. Additional figures and analyses.
Investigating the physiological role of hypothalamic glucokinase in appetite and glucose homeostasis
Creators: name: Hussain, Syed Sufyan
Publisher: name: Imperial College London
Year: 2013

description: The brain relies on glucose as a source of energy. Mechanisms that promote the taste-independent intake of glucose have been proposed but not demonstrated. The arcuate nucleus (ARC) of the hypothalamus plays a critical role in regulating energy homoeostasis. It acts as a metabolic sensing unit responding to diverse signals, including glucose, to regulate appetite. Glucokinase is a glucose-sensing enzyme expressed in the ARC. The work in this thesis aims to investigate the physiological role of ARC glucokinase in energy homoeostasis. Recombinant adeno-associated virus (rAAV) expressing the pancreatic form of rat glucokinase mRNA (rAAV-GKS) was stereotactically delivered to the ARC of male Wistar rats (iARC-GKS). This approach specifically increased glucokinase activity in the ARC as compared to control rats (iARC-GFP). Pharmacological and genetic increase in ARC glucokinase activity resulted in a significant increase in food intake. Longitudinal experiments demonstrated that this food intake resulted in a significant increase in body weight and adiposity on normal chow and high-energy diets. Further work demonstrated that ARC glucokinase specifically promotes the intake of glucose, but not of fructose, and that the orexigenic effect of ARC glucokinase is driven by specific increase in appetite for glucose. Similar changes in glucose appetite and food intake were demonstrated to occur with alterations in ARC ATP-sensitive potassium (KATP) channel activation. Glucose-stimulated NPY release was increased with increased ARC glucokinase activity. This suggests that ARC glucokinase mediates its orexigenic glucose appetite promoting effects in part via altered KATP channel activation and NPY release, which is consistent with previous work. This work identifies ARC glucokinase as a regulator of glucose appetite and glucose appetite as an important driver of food intake. ARC glucokinase may represent the brain mechanism regulating the taste-independent intake of glucose and may underlie the phenomena of ‘sweet tooth’ and ‘carbohydrate craving’.
Optical Observations of the 2002cx-like Supernova 2014ek, and Characterizations of SNe Iax
Creators: name: Li, Linyi
name: Wang, Xiaofeng
name: Zhang, Jujia
name: Arcavi, Iair
name: Zhang, Tianmeng
name: Rui, Liming
name: Hosseinzadeh, Griffin
name: Howell, D. Andrew
name: McCully, Curtis
name: Zhang, Kaicheng
name: Valenti, Stefano
name: Mo, Jun
name: Li, Wenxiong
name: Huang, Fang
name: Xiang, Danfeng
name: Wang, Lifan
name: Zhou, Xu
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present optical observations of supernova (SN) 2014ek discovered during the Tsinghua-NAOC Transient Survey (TNTS), which shows properties that are consistent with those of SN 2002cx-like events (dubbed as SNe Iax). The photometry indicates that it is underluminous compared to normal SNe Ia, with the absolute $V$-band peak magnitude being as $-17.66\pm0.20$ mag. The spectra are characterized by highly ionized Fe III and intermediate-mass elements (IMEs). The expansion velocity of the ejecta is found to be $\sim$5000 km s$^{-1}$ near the maximum light, only half of that measured for normal SNe Ia. The overall spectral evolution is quite similar to SN 2002cx and SN 2005hk, while the absorption features of the main IMEs seem to be relatively weaker. The ${}^{56}$Ni mass synthesized in the explosion is estimated to be about 0.08 M$_{\odot}$ from the pseudo bolometric light curve. Based on a large sample of SNe Iax, we examined the relations between peak luminosity, ejecta velocity, decline rate, and peak $V - R$ color but did not find noticeable correlations between these observables, in particular when a few extreme events like SN 2008ha are excluded in the analysis. For this sample, we also studied the birthplace environments and confirm that they still hold the trend of occurring preferentially in late-type spiral galaxies. Moreover, SNe Iax tend to occur in large star-forming regions of their host galaxies, more similar to SNe Ibc than SNe II, favoring that their progenitors should be associated with very young stellar populations.
description: 15 pages, 14 figures, published on Monthly Notices of the Royal Astronomical Society
Conus marmoreus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Conidae
Conus
Conus marmoreus

description: Conus marmoreus [spec. nov.]
C. testa conica fusca, maculis ovatis albis, spirae anfractibus canaliculatis.
Bonan. recr. 3. f. 123.
Rumph. mus. t. 32. f. N. 1.
Gvalt. test. t. 22. f. D.
Argenv. conch. t. 15. f. O.
Pet. gaz t. 47. f. 11.
Kratzenst. Regenf. 20. t. 5. f. 53.
Habitat in Asia.
Testa saepe coronata atra maculis trigono-ovatis albis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 712, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 4: of Healthy diets ASAP â Australian Standardised Affordability and Pricing methods protocol
Creators: name: Lee, Amanda
name: Kane, Sarah
name: Meron Lewis
name: Good, Elizabeth
name: Pollard, Christina
name: Landrigan, Timothy
name: Dick, Mathew
Publisher: name: figshare
Year: 2018
Subjects: subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified

description: Energy and nutrient analysis of individual current and healthy diet baskets compared to results of the AHS and Foundation Diet modelling. (DOCX 36 kb)
A Possible Bias Model for Quasars
Creators: name: Fang, Li-Zhi
name: Jing, Y. P.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose that the majority of quasars at redshift $z\sim 1 - 5$ formed in the environment of new born collapsed halos with 1-D velocity dispersion $σ_v^{1d} \sim 400 \kms$. The harboring coefficient $f$ of quasars per halo and the lifetime of quasars depend only on local process, not modulated by the density inhomogeneities on scales larger than the size of the halos. Thus, the bias of quasars on scale larger than the size of these halos is mainly determined by the parameter $σ_v$ used for quasar environment identification. With this model, the popular structure formation models, like SCDM and LCDM, can be fairly well reconciled with the data of quasars, including a. observed feature of the environment for quasars; b. redshift evolution of quasar abundance; c. the two-point correlation functions of quasars. This bias model predicts that the correlation function of quasars doesn't significantly evolve, or only slightly increases with redshift.
description: accepted for publication in ApJ Letters; 11 pages with 3 figures included
Additional file 1: of Global, regional, and national prevalence of hepatitis B infection in the general and key populations living with HIV: a systematic review and meta-analysis protocol
Creators: name: Leumi, Steve
name: Bigna, Jean
name: Amougou, Marie
name: Aminde, Leopold
name: Nyaga, Ulrich
name: Noubiap, Jean
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Preferred Reporting Items for Systematic Review and Meta-Analysis for protocol checklist. (DOCX 32Â kb)
MOESM5 of CRISPR-Cas genome engineering of esterase activity in Saccharomyces cerevisiae steers aroma formation
Creators: name: Dank, Alexander
name: Smid, Eddy
name: Notebaart, Richard
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 5. Protocol used to transform linear repair fragment DNA and plasmids into S. cerevisiae
Homodyne-detector-blinding attack in continuous-variable quantum key distribution
Creators: name: Qin, Hao
name: Kumar, Rupesh
name: Makarov, Vadim
name: Alléaume, Romain
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Cryptography and Security (cs.CR)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We propose an efficient strategy to attack a continuous-variable quantum key distribution (CV-QKD) system, that we call homodyne detector blinding. This attack strategy takes advantage of a generic vulnerability of homodyne receivers: a bright light pulse sent on the signal port can lead to a saturation of the detector electronics. While detector saturation has already been proposed to attack CV-QKD, the attack we study in this paper has the additional advantage of not requiring an eavesdropper to be phase locked with the homodyne receiver. We show that under certain conditions, an attacker can use a simple laser, incoherent with the homodyne receiver, to generate bright pulses and bias the excess noise to arbitrary small values, fully comprising CV-QKD security. These results highlight the feasibility and the impact of the detector blinding attack. We finally discuss how to design countermeasures in order to protect against this attack.
Additional file 3 of Non-contrast cardiovascular magnetic resonance detection of myocardial fibrosis in Duchenne muscular dystrophy
Creators: name: Raucci, Frank J.
name: Xu, Meng
name: George-Durrett, Kristen
name: Crum, Kimberly
name: Slaughter, James C.
name: Parra, David A.
name: Markham, Larry W.
name: Soslow, Jonathan H.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 3: Table S1. Models for prediction of presence and severity of LGE (myocardial tagging).
Photon states associated with Holstein-Primakoff realization of SU(1,1) Lie algebra
Creators: name: Brif, C.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Statistical and phase properties and number-phase uncertainty relations are systematically investigated for photon states associated with the Holstein-Primakoff realization of the SU(1,1) Lie algebra. Perelomov's SU(1,1) coherent states and the eigenstates of the SU(1,1) lowering generator (the Barut-Girardello states) are discussed. A recently developed formalism, based on the antinormal ordering of exponential phase operators, is used for studying phase properties and number-phase uncertainty relations. This study shows essential differences between properties of the Barut-Girardello states and the SU(1,1) coherent states. The philophase states, defined as states with simple phase-state representations, relate the quantum description of the optical phase to the properties of the SU(1,1) Lie group. A modified Holstein-Primakoff realization is derived, and eigenstates of the corresponding lowering generator are discussed. These states are shown to contract, in a proper limit, to the familiar Glauber coherent states.
description: 32 pages, no figures, REVTeX with amssymb, to be published in Quantum and Semiclassical Optics
Reminiscences of Arthur Kaminsky 1991
Publisher: name: Columbia University
Year: 2020
Subjects: Lawyers
Presidents--Election--1968.--United States
Military campaigns--New York (State)
Campaign management

description: Recollections of Allard K. Lowenstein [Lowenstein]; introduction to Lowenstein, Cornell University student government, 1967, Dump Johnson movement; involvement with Robert F. Kennedy presidential campaign: response to assasination, deepening commitment to Lowenstein; Lowenstein's New York congressional campaigns; campaign techniques, mistakes made in bids for office; ambivalence toward official endorsements of presidential candidates; Kaminsky's use of Lowenstein techniques in John Lindsay presidential bid, other campaigns; Lowenstein's death
Characterization of the Novel Saccharomyces cerevisiae Protein, Sdm1
Creators: name: Minuzzi, Florencia
Publisher: name: Imperial College London
Year: 2014

description: Yir016w (named Sdm1 for deficient in Separation of Daughter and Mother cells) was found in a screen for Saccharomyces cerevisiae cell separation-defective mutants, where yir016w cells were clumped together in groups of three or four. This gene was of special interest due to its ability to interact with Ace2 and members of the RAM (Regulation of Ace2 and Morphogeneis) network, which exert control over cell separation. This study aimed to elucidate the function of this previously uncharacterized gene YIR016W. The cell separation defect of sdm1 cells was found to be milder than that of RAM mutants, although still of statistical significance. Also, sdm1 cells neither showed the lack of polarization of the RAM mutants, nor any defects in the localization of Cts1, a key chitinase required for cell separation controlled by the transcription factor Ace2. Instead of a role in the RAM network, Sdm1 may play a role in protein trafficking, as sdm1 cells have vacuolar defects. This study also aimed to localize Sdm1. The protein responsible for Sdm1 expression is Ume6, a key transcriptional regulator of meiosis. While an Sdm1-GFP fusion was not visible under normal growth conditions, under meiosis-inducing conditions the signal was strong enough to be visualized. Using co-localization, Sdm1-GFP was found to be present in the Golgi body, and analysis of sdm1 cells show that they contained defects in the division of their vacuoles. These results point at additional functions of Sdm1, such as the control of mitosis-meiosis switching and protein processing and export. In addition, a second protein, Yol036w (termed Sdm2) was investigated, as it interacted with both the RAM network and Sdm1. yol036w cells showed no significant phenotypes in our screens, however, its interactions support the idea that it might also be involved in protein trafficking, or in cell wall biogenesis.
title: ADCO, Cartulaire de Fontenay, second fragment (XIIIe siècle), Cart. 201 (15 H 9), folios 47-142, f. 016r
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2009
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de Fontenay, second fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), folios 47-142. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Fontenay, second fragment (XIIIe siècle), Archives départementales de la Côte-d'Or, Cart. 201 (15 H 9), folios 47-142, f. 016r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Fontenay
description: Provenance: http://www.wikidata.org/entity/Q464918
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb119679755
description: Provenance: https://www.geonames.org/7874015
description: Provenance: http://www.idref.fr/027691802/id
Town Hall for Planetary Science Research Programs_Oct24
Creators: name: Vander Kaaden
Publisher: name: Zenodo
Year: 2024
Subjects: NASA
PSD
R&A

description: On October 15, 2024 at 3 PM Eastern, NASA’s Planetary Science Division (PSD) hosted a webinar to discuss changes made to select upcoming Research Opportunities in Space and Earth Science (ROSES)-24 programs and anticipated program changes for ROSES-25. The following topics were included in this discussion: 1) General overview for broad scale changes, 2) Future Investigators in NASA Earth and Space Science and Technology (FINESST) including requirements for ROSES-24 and implementation of Dual Anonymous Peer Review (DAPR), 3) Merging of Emerging Worlds (EW), Solar System Workings (SSW), Solar System Observations (SSO) into a single program for ROSES-25, 4) Changes to Astrobiology Programs including scope modification of Habitable Worlds (HW), Exobiology (Exo), and Exoplanet Research Programs (XRP).
The Orbital Evolution and Proper Motion of PSR J2051-0827
Creators: name: Stappers, B. W.
name: Bailes, M.
name: Manchester, R. N.
name: Sandhu, J. S.
name: Toscano, M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have carried out high-precision timing observations of the eclipsing binary PSR J2051-0827 in the 3.3 years since its discovery. These data indicate that the orbital period is decreasing at a rate of dPb/dt = (-11+-1)X10^-12. If secular, this orbital period derivative implies a decay time for the orbit of only 25 Myr which is much shorter than the expected timescale for ablation of the companion. We have also measured the proper motion of the pulsar to be 5+-3 mas/yr. Assuming the pulsar is at the dispersion-measure distance this implies a very slow transverse velocity vt=(30+-20) km/s. This combination of low velocity and short orbital period argue against formation of the system in the standard manner and we discuss the implications for its evolutionary history.
description: 7 pages, 1 figure, accepted for publication in Astrophysical Journal Letters
Conus capitaneus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Conidae
Conus
Conus capitaneus

description: Conus capitaneus [spec. nov.]
C. testa conica glabra basi fusca, spira convexiuscula.
Gvalt. test. t. 20. f. I.
Rumph. mus. t. 33. f. X.
Gvalt. test. t. 22. f. M.
Bonan. recr. 3. t. 139.
Argenv. conch. t. 15. f. K.
Pet. gaz. t. 27. f. 11.
Kratzenst. Regenf. t. 7. f. 7.
Rumph. mus. t. 33. f. Y.
Kratz. Regenf. 26. t. 6. f. 65.
Gvalt. test. t. 20. f. G.
Bonan. recr. 3. t. 361.
Habitat in Asia.
Testa caesia fasciis 2 s. 3 albis fusco-maculatis.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 713, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1 of Post-recovery health domain scores among outpatients by SARS-CoV-2 testing status during the pre-Delta period
Creators: name: King, Jennifer P.
name: Chung, Jessie R.
name: Donahue, James G.
name: Martin, Emily T.
name: Leis, Aleda M.
name: Monto, Arnold S.
name: Gaglani, Manjusha
name: Dunnigan, Kayan
name: Raiyani, Chandni
name: Saydah, Sharon
name: Flannery, Brendan
name: Belongia, Edward A.
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Mental Health
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Supplemental Table 1. First follow-up questionnaire questions common to all sites. Supplemental Table 2. PROMIS questions administered on second follow-up survey. Supplemental Table 3. Unadjusted raw PROMIS mean T-scores1 and mean T-score ratios2 by SARS-CoV-2 test-positive or SARS-CoV-2 test-negative groups and participant characteristics. Supplemental Table 4. Multivariable Gamma regression mean T-score ratios and 95% confidence intervals from subgroup and sensitivity analyses. Models adjusted for base factors and health factors. Supplemental Figure 1. Survey completion and participant exclusions. Supplemental Figure 2. Adjusted Global Health, Physical Function, Fatigue, and Dyspnea domain mean T-score ratios from multivariable1-3 Gamma regression models.
A Survey on Bohmian Mechanics
Creators: name: Berndl, K.
name: Daumer, M.
name: Dürr, D.
name: Goldstein, S.
name: Zanghi, N.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Bohmian mechanics is the most naively obvious embedding imaginable of Schrödinger's equation into a completely coherent physical theory. It describes a world in which particles move in a highly non-Newtonian sort of way, one which may at first appear to have little to do with the spectrum of predictions of quantum mechanics. It turns out, however, that as a consequence of the defining dynamical equations of Bohmian mechanics, when a system has wave function $ψ$ its configuration is typically random, with probability density $ρ$ given by $|ψ|^2$, the quantum equilibrium distribution. It also turns out that the entire quantum formalism, operators as observables and all the rest, is a consequence of Bohmian mechanics.
description: 9 pages, Revtex, To appear in Il Nuovo Cimento
Additional file 4 of Non-contrast cardiovascular magnetic resonance detection of myocardial fibrosis in Duchenne muscular dystrophy
Creators: name: Raucci, Frank J.
name: Xu, Meng
name: George-Durrett, Kristen
name: Crum, Kimberly
name: Slaughter, James C.
name: Parra, David A.
name: Markham, Larry W.
name: Soslow, Jonathan H.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 4: Table S2. Models for prediction of presence/absence LGE and FWHM by segment (myocardial tagging).
The attractive behaviour of ultra-slow-roll inflation
Creators: name: Pattison, Chris
name: Vennin, Vincent
name: Assadullahi, Hooshyar
name: Wands, David
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: It is often claimed that the ultra-slow-roll regime of inflation, where the dynamics of the inflaton field are friction dominated, is a non-attractor and/or transient. In this work we carry out a phase-space analysis of ultra-slow roll in an arbitrary potential, $V(ϕ)$. We show that while standard slow roll is always a dynamical attractor whenever it is a self-consistent approximation, ultra-slow roll is stable for an inflaton field rolling down a convex potential with $M_{\scriptscriptstyle{\mathrm{Pl}}} V''>|V'|$ (or for a field rolling up a concave potential with $M_{\scriptscriptstyle{\mathrm{Pl}}} V''
description: 23 pages, 6 figures, matches version published in JCAP
Conus miles Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Gastropoda
Neogastropoda
Conidae
Conus
Conus miles

description: Conus miles [spec. nov.]
C. testa conica rudi basi fusca, spira convexa.
Rumph. mus. t. 33. f. W.
Habitat in India.
Testa ignobilis pallido testacea fasciis fusco-ferrugineis.
* * Pyriformes basi rotundata, sub-cylindrica quam spira sesquilongiore.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 713, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Age, Metallicity, and the Distance to the Magellanic Clouds From Red Clump Stars
Creators: name: Cole, Andrew A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that the luminosity dependence of the red clump stars on age and metallicity can cause a difference of up to < ~0.6 mag in the mean absolute I magnitude of the red clump between different stellar populations. We show that this effect may resolve the apparent ~0.4 mag discrepancy between red clump-derived distance moduli to the Magellanic Clouds and those from, e.g., Cepheid variables. Taking into account the population effects on red clump luminosity, we determine a distance modulus to the LMC of 18.36 +/- 0.17 mag, and to the SMC of 18.82 +/- 0.20 mag. Our alternate red clump LMC distance is consistent with the value (m-M){LMC} = 18.50 +/- 0.10 adopted by the HST Cepheid Key Project. We briefly examine model predictions of red clump luminosity, and find that variations in helium abundance and core mass could bring the Clouds closer by some 0.10--0.15 mag, but not by the ~0.4 mag that would result from setting the mean absolute I-magnitude of the Cloud red clumps equal to the that of the Solar neighborhood red clump.
description: Accepted for publication in The Astrophysical Journal Letters, AASTeX 4.0, 10 pages, 1 postscript figure
The Generation of Vorticity in Cosmological N-body Simulations
Creators: name: Jelic-Cizmek, Goran
name: Lepori, Francesca
name: Adamek, Julian
name: Durrer, Ruth
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Clustering of a perfect fluid does not lead to the generation of vorticity. It is the collisionless nature of dark matter, inducing velocity dispersion and shell crossing, which is at the origin of cosmological vorticity generation. In this paper we investigate the generation of vorticity during the formation of cosmological large scale structure using the public relativistic N-body code $\textit{gevolution}$. We test several methods to compute the vorticity power spectrum and we study its convergence with respect to the mass and grid resolution of our simulations. We determine the power spectrum, the spectral index on large-scales, the amplitude of the peak position and their time evolution. We also compare the vorticity extracted from our simulations with the vector perturbations of the metric. Our results are accompanied by resolution studies and compared with previous studies in the literature.
description: 26 pages, 13 figures