cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Bezzia (Bezzia) laciniastyla Dow and Turner
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Bezzia
Bezzia laciniastyla

description: Bezzia (Bezzia) laciniastyla Dow and Turner
 Bezzia (Pseudobezzia) laciniastyla Dow and Turner, 1976: 42 (Florida).
 Bezzia (Bezzia) laciniastyla: Wilkening et al. 1985: 529 (Florida records); Borkent and Grogan 2009: 26 (in Nearctic catalog; distribution).
 Discussion. All specimens in the type series were from Glades Co., Florida and Georgetown Co., South Carolina (Dow and Turner 1976). Wilkening et al. (1985) also recorded this species from Alachua and Wakulla counties. However, as noted by Dow and Turner (1976), the material they studied included a complex of at least two undescribed species and these will be addressed in a study in progress by WLG.
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on page 48, DOI: 10.5281/zenodo.5352908
13 Briefe an Unbekannte
Creators: name: Hirzel, Salomon
name: Hegner, U.
Publisher: name: [s.n.]
Year: 1760

description: von Sal[omon?] Hirzel und U. Hegner
description: Zusammengebunden mit weiteren Werken in Sammelband mit Rückentitel "Zürcher Biographien"
description: Öffentliche Bibliothek der Universität Basel
description: Deutsch
description: Verzeichnung=Description=Inventaire Januar 2025 HAN-Katalogisierungsregeln ben
Bezzia (Bezzia) mallochi Wirth
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Bezzia
Bezzia mallochi

description: Bezzia (Bezzia) mallochi Wirth
 Bezzia (Pseudobezzia) mallochi Wirth, 1951: 323 (Virginia); Dow and Turner 1976: 51 (revision of Nearctic Bezzia; distribution).
 Bezzia (Bezzia) mallochi: Borkent and Grogan 2009: 26 (in Nearctic catalog; distribution).
 Discussion. The following specimens from Liberty and Santa Rosa counties are apparently the first records of this species from Florida (Borkent and Grogan 2009).
 New records. Liberty Co., Torreya St. Park, 20-V-1966, H. V. Weems, 1 male (USNM). Santa Rosa Co., Jay, May 1962, T. W. Boyd, lt. trap, 1 female (USNM). New Florida state record.
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on page 48, DOI: 10.5281/zenodo.5352908
Electromechanical Effects in Carbon Nanotubes
Creators: name: Verissimo-Alves, M.
name: Koiller, Belita
name: Chacham, H.
name: Capaz, R. B.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We perform ab initio calculations of charged graphene and single-wall carbon nanotubes (CNTs). A wealth of electromechanical behaviors is obtained: (1) Both nanotubes and graphene expand upon electron injection. (2) Upon hole injection, metallic nanotubes and graphene display a non-monotonic behavior: Upon increasing hole densities, the lattice constant initially contracts, reaches a minimum, and then starts to expand. The hole densities at minimum lattice constants are 0.3 |e|/atom for graphene and between 0.1 and 0.3 |e|/atom for the metallic nanotubes studied. (3)Semiconducting CNTs with small diameters (d ~ 20 A) display a behavior intermediate between those of metallic and large-gap CNTs. (5) The strain versus extra charge displays a linear plus power-law behavior, with characteristic exponents for graphene, metallic, and semiconducting CNTs. All these features are physically understood within a simple tight-binding total-energy model.
description: Submitted to Physical Review Letters on May 23rd 2002
MOESM2 of Improving plant transient expression through the rational design of synthetic 5′ and 3′ untranslated regions
Creators: name: Peyret, Hadrien
name: Brown, James
name: Lomonossoff, George
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Additional file 2. Sequences of the cloning fragments of the synthetic 5′ and 3′UTRs. Restriction sites (BsmB1 for 5′UTRs and Sap1 for 3′UTRs) are in bold and italicized. The sequence of the UTR once cloned into the expression cassette is underlined. Yellow: simplified synthetic CITE component complementary sequences. Green: synthetic CIRE component sequence. Blue: simplified BTE sequence. Magenta: CPMV RNA-2 3′UTR Y-loop structure.
Letzte Vorlesung an seine Lernjünger
Creators: name: Füssli, Johann Heinrich
Publisher: name: [s.n.]
Year: 1770

description: von J[ohann] H[einrich?] Füssli
description: Zusammengebunden mit weiteren Werken in Sammelband mit Rückentitel "Zürcher Biographien"
description: Öffentliche Bibliothek der Universität Basel
description: Deutsch
description: Verzeichnung=Description=Inventaire Januar 2025 HAN-Katalogisierungsregeln ben
Bezzia (Bezzia) nobilis
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Bezzia
Bezzia nobilis

description: Bezzia (Bezzia) nobilis (Winnertz)
 Ceratopogon nobilis Winnertz, 1852: 79 (Europe).
 Bezzia nobilis: Kieffer 1901: 153 (combination).
 Bezzia (Bezzia) nobilis: Wirth 1983c: 673 (review of New World nobilis group); Wilkening et al. 1985: 530 (Florida records); Borkent and Grogan 2009: 26 (in Nearctic catalog; distribution).
 Ceratopogon setulosus Loew, 1861: 312 (Washington D.C.)
 Ceratopogon barberi Coquillett, 1901: 601 (Maryland).
 Bezzia atlantica Wirth and Williams, 1957: 13 (Bermuda).
 Discussion. This very common Holarctic and Neotropical species was listed by Wilkening et al. (1985) from 15 Florida counties including Wakulla Co. We provide additional records from that county.
 New records. Wakulla Co., Wakulla Springs State Park, Lodge Road, 25 May 2004, S. Murphree, CDC light trap with UV wand, 1 male, 2 females (BUTC).
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on pages 48-49, DOI: 10.5281/zenodo.5352908
Adaptive compressive tomography: a numerical study
Creators: name: Ahn, D.
name: Teo, Y. S.
name: Jeong, H.
name: Koutny, D.
name: Rehacek, J.
name: Hradil, Z.
name: Leuchs, G.
name: Sanchez-Soto, L. L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We perform several numerical studies for our recently published adaptive compressive tomography scheme [D. Ahn et al. Phys. Rev. Lett. 122, 100404 (2019)], which significantly reduces the number of measurement settings to unambiguously reconstruct any rank-deficient state without any a priori knowledge besides its dimension. We show that both entangled and product bases chosen by our adaptive scheme perform comparably well with recently-known compressed-sensing element-probing measurements, and also beat random measurement bases for low-rank quantum states. We also numerically conjecture asymptotic scaling behaviors for this number as a function of the state rank for our adaptive schemes. These scaling formulas appear to be independent of the Hilbert space dimension. As a natural development, we establish a faster hybrid compressive scheme that first chooses random bases, and later adaptive bases as the scheme progresses. As an epilogue, we reiterate important elements of informational completeness for our adaptive scheme.
description: 12 pages, 12 figures
Additional file 7: of Immunohistochemical validation of COL3A1, GPR158 and PITHD1 as prognostic biomarkers in early-stage ovarian carcinomas
Creators: name: Engqvist, Hanna
name: Toshima Parris
name: Anikรณ Kovรกcs
name: Szilรกrd Nemes
name: Rรถnnerman, Elisabeth Werner
name: Lara, Shahin De
name: Biermann, Jana
name: Sundfeldt, Karin
name: Karlsson, Per
name: Helou, Khalil
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Table S3.. KM plotter probe ID and P values for the study 647 genes. Twenty-six of the 29 study genes could be evaluated using KM plotter. The FRMPD2, SLC9A4 and TRIM71 genes could not be assessed since they are not included on the GeneChipโ ข Human Genome U133A 2.0 Array. Twenty one genes showed significant Kaplan-Meier plots for at least one Affymetrix ID probe (marked in bold). (DOCX 26 kb)
MOESM1 of Improving plant transient expression through the rational design of synthetic 5′ and 3′ untranslated regions
Creators: name: Peyret, Hadrien
name: Brown, James
name: Lomonossoff, George
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: Developmental Biology
subject: Computational Biology

description: Additional file 1. Sequence of the Synth expression cassette. The different elements follow the same colour scheme as in Fig. 1: blue for the 35S promoter and nos terminator, red for the 5S0 5′UTR, green for the cloning site, and yellow for the 3S0 3′UTR. Restriction sites indicated in Fig. 1 are underlined in the sequence: Pac1 at the 5′ end, BsmB1 in 5S0, Bsa1 in the cloning site, Sap1 in 3S0, and Asc1 at the 3′ end.
Gliese 569B: A young multiple brown dwarf system?
Creators: name: Kenworthy, M. A.
name: Hofmann, K-H.
name: Close, L.
name: Hinz, P.
name: Mamajek, E.
name: Schertl, D.
name: Weigelt, G.
name: Angel, R.
name: Balega, Y. Y.
name: Hinz, J.
name: Rieke, G.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The nearby late M star Gliese 569B was recently found by adaptive optics imaging to be a double with separation ~1 AU. To explore the orbital motion and masses, we have undertaken a high resolution (~0.05 arcsec) astrometric study. Images were obtained over 1.5 years with bispectrum speckle interferometry at the 6.5m MMT and 6m SAO telescopes. Our data show motion corresponding to more than half the orbital period, and constrain the total mass to be > 0.115 M_solar, with a most probable value of 0.145 M_solar. Higher masses cannot be excluded without more extended observations, but from statistical analysis we find an 80% probability that the total mass is less than 0.21 M_solar. An infrared spectrum of the blended B double obtained with the MMT has been modeled as a blend of two different spectral types, chosen to be consistent with the measured J and K band brightness difference of a factor ~2. The blended fit is not nearly as good as that to a pure M8.5+ template. Therefore we hypothesize that the brighter component likely has two unresolved components with near equal masses, each the same as the fainter component. If Gl 569B is a triple our dynamical limits suggest each component has a mass of 50 (+23/-4) M_jupiter. We infer an age for the system of 300 Myr, from its kinematic motion which places its as a member of the Ursa Major moving group. All the above parameters are consistent with the latest DUSTY evolutiuon models for brown dwarfs.
description: 17 pages, 3 figures, 2 tables, accepted by ApJ Letters. Version with high-res fig. 1 available at http://focus.as.arizona.edu/~mak/gl569b/
Fortcart-de Speyr, Ch
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1835

description: Ort: Basel
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Comments on the Final Orbital Separation in Common Envelope Evolution
Creators: name: Soker, Noam
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I study some aspects of common envelope evolution, where a compact star enters the envelope of a giant star. I show that in some binary systems under a narrow range of parameters, a substantial fraction of the giant stellar envelope is lost before the onset of the common envelope. The reduced envelope mass at the onset of the common envelope implies that the binary system emerges from the common envelope with a relatively large orbital separation. I therefore caution against a simple treatment, which omits this process, in the study of systems that evolved through a common envelope phase and ended with a relatively large orbital separation, e.g., PG1115+166. A fraction of the envelope that is lost while the companion is still outside the giant stellar envelope is accreted by the companion. The companion may form an accretion disk and blow two jets. I propose this scenario for the formation of the bipolar planetary nebula NGC 2346, which has a binary nucleus with an orbital period longer than that of any other known binary system in planetary nebulae. Because this scenario, of a late common envelope phase, occurs for a narrow range of parameters, I expect it to be applicable to a small, but non-negligible, number of systems.
description: MNRAS, submitted; 8 pages
Franke, Runge & Co
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1835

description: Ort: Tampico
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Bezzia (Bezzia) perplexa Dow and Turner
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Bezzia
Bezzia perplexa

description: Bezzia (Bezzia) perplexa Dow and Turner
 Bezzia (Pseudobezzi a) perplexa Dow and Turner, 1976: 57 (Florida).
 Bezzia (Bezzia) perplexa: Wilkening et al. 1985: 529 (Florida records); Borkent and Grogan 2009: 26 (in Nearctic catalog; distribution).
 Discussion. Dow and Turner (1976) designated the holotype and paratypes from Alachua Co. and additional Florida paratypes from Hillsborough, Indian River and Liberty counties as well as three paratypes from Drew Co., Arkansas. We provide the first records from Glades, Gulf, Manatee, Marion, Orange and Wakulla counties.
 New records. Glades Co., Palmdale, 14 July 1970, E. Irons, light trap, 1 male (USNM). Gulf Co., Wewahitchka, Aug. 1967, Blanton & Boike, light trap, 1 female; same data except Sept. 1967, 1 female (USNM). Manatee Co., Oneco, 23 March 1954, G. E. Ball, 1 male (USNM). Marion Co., Juniper Springs, 28 April 1970, W. W. Wirth, light trap, 1 female (USNM). Orange Co., Rock Springs, 21 April 1970, W. W. Wirth, light trap, 1 female (USNM). Wakulla Co., Ochlockonee Riv. St. Park, 29-IV-1970, W. W. Wirth, light trap, 1 male (USNM); Wakulla Springs State Park, Lodge Road, 25 May 2004, S. Murphree, CDC light trap with UV wand, 1 female (WLGC).
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on page 49, DOI: 10.5281/zenodo.5352908
Additional file 12 of Integrated multi-omics analysis and microbial recombinant protein system reveal hydroxylation and glycosylation involving nevadensin biosynthesis in Lysionotus pauciflorus
Creators: name: Wu, Tianze
name: Xiang, Li
name: Gao, Ranran
name: Wu, Lan
name: Deng, Gang
name: Wang, Wenting
name: Zhang, Yongping
name: Wang, Bo
name: Shen, Liang
name: Chen, Shilin
name: Liu, Xia
name: Yin, Qinggang
Publisher: name: figshare
Year: 2022
Subjects: subject: Microbiology
subject: FOS: Biological sciences

description: Additional file 12: Figure S6. Identification of UGTs in L. pauciflorus. (a) Phylogenetic analysis of L. pauciflorus and Arabidopsis UGTs. The sequences were aligned using the ClustalW algorithm, based on the neighbor-joining method. The size of light blue represents the bootstrap value. (b) L. pauciflorus expression profiles. Hierarchical clustering for 187 LpUGTs was conducted based on transcript data.
A Bayesian interpretation of inconsistency measures in cosmology
Creators: name: Lin, Weikang
name: Ishak, Mustapha
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Measures of discordance between datasets have become an essential part of cosmological analyses. It is important to accurately evaluate the significance of such discordances when present. We propose here a Bayesian interpretation of inconsistency measures that can extract information about physical inconsistencies in the presence of data scatter. The new framework is based on the conditional probability distribution of the level of physical inconsistency given the obtained value of the measure. We use the index of inconsistency as a case study to illustrate the new interpretation framework, but this can be generalized to other metrics. Importantly, there are two aspects in the quantification of inconsistency that behave differently as the number of model parameters increases. The first is the probability for the level of physical inconsistency to reach a threshold which drops with the increase of the number of parameters under consideration. Then the second is the actual level of physical inconsistency which remains rather insensitive to such an increase in parameters. This often-overlooked ambiguity leads to an underestimation of the physical inconsistency by the commonly adopted significance level when used, but is resolved by the Bayesian interpretation because the conditional probability distribution includes all the statistical information of the level of physical inconsistency. Finally, we apply the Bayesian interpretation to examine the (in)consistency between Planck versus the Cepheid-based local measurement, the Dark Energy Survey (DES), the Atacama Cosmology Telescope (ACT) and WMAP. We confirm and revisit the degrees of previous physical inconsistencies and show the stability of the new interpretation to the number of cosmological parameters compared to the commonly used n-$σ$ interpretation when applied to cosmological tensions in multi-parameter spaces.
description: Matches JCAP published version. This paper proposes a novel Bayesian method to interpret the significance of inconsistency measures and resolves a long-standing ambiguity in the field
The role of cattle genetically efficient in feed utilisation in an Australian carbon trading environment
Creators: name: Arthur, Paul F.
name: Herd, Robert M.
name: Basarab, John A.
name: Arthur, Paul F.
name: Herd, Robert M.
name: Basarab, John A.
Publisher: name: Unknown
Year: 2011
Subjects: subject: Farm Management
subject: feed efficiency
subject: residual feed intake
subject: methane
subject: greenhouse gas
subject: emission
subject: beef cattle

description: Residual feed intake (RFI) is a measure of feed efficiency in beef cattle. It is a moderately heritable trait, and cattle with low RFI consume less feed than expected at the same level of growth relative to their high RFI contemporaries. Selection for RFI is a relatively new genetic improvement tool in beef cattle to reduce the cost of production, and currently has a low level of adoption in the industry. Selection for low RFI is associated with reduction in greenhouse gas (GHG) emissions, hence could play a role in any carbon trading scheme implemented in Australia. For any GHG reduction protocol to be acceptable in a carbon trading/offset environment, it needs to follow United Nations IPCC guidelines, be based on science, be quantifiable and be auditable. The beef industry already has quality assurance systems in place for RFI that can be fine-tuned to meet these criteria. Scientific information currently available is adequate for the development of GHG emission reduction protocols for cattle raised for slaughter. Selection for RFI also has an impact on GHG emissions from the breeding herd. However, information currently available lacks the degree of accuracy needed for protocol development. It is therefore recommended that funding be provided to continue the research on the relationships among RFI, cow feed intake and maternal productivity traits.
description: Special Edition Sheep and Cattle Production in New South Wales
Recovering the unsigned photospheric magnetic field from Ca II K observations
Creators: name: Chatzistergos, Theodosios
name: Ermolli, Ilaria
name: Solanki, Sami K.
name: Krivova, Natalie A.
name: Giorgi, Fabrizio
name: Yeo, Kok Leng
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We reassess the relationship between the photospheric magnetic field strength and the Ca II K intensity for a variety of surface features as a function of the position on the disc and the solar activity level. This relationship can be used to recover the unsigned photospheric magnetic field from images recorded in the core of Ca II K line. We have analysed 131 pairs of high-quality, full-disc, near-co-temporal observations from SDO/HMI and Rome/PSPT spanning half a solar cycle. To analytically describe the observationally-determined relation, we considered three different functions: a power law with an offset, a logarithmic function, and a power law function of the logarithm of the magnetic flux density. We used the obtained relations to reconstruct maps of the line-of-sight component of the unsigned magnetic field (unsigned magnetograms) from Ca II K observations, which were then compared to the original magnetograms. We find that both power-law functions represent the data well, while the logarithmic function is good only for quiet periods. We see no significant variation over the solar cycle or over the disc in the derived fit parameters, independently of the function used. We find that errors in the independent variable, usually not accounted for, introduce attenuation bias. To address this, we binned the data with respect to the magnetic field strength and Ca II K contrast separately and derived the relation for the bisector of the two binned curves. The reconstructed unsigned magnetograms show good agreement with the original ones. RMS differences are less than 90 G. The results were unaffected by the stray-light correction of the SDO/HMI and Rome/PSPT data. Our results imply that Ca~II~K observations, accurately processed and calibrated, can be used to reconstruct unsigned magnetograms by using the relations derived in our study.
description: 18 pages, 22 figures, accepted in A&A
Gex & Decosterd
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1835

description: Ort: Bahia
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Gross margins for NSW beef enterprises from 1999-2010
Creators: name: Andrews, Todd
name: Llewelyn, David
name: Davies, Lloyd
name: Andrews, Todd
name: Llewelyn, David
name: Davies, Lloyd
Publisher: name: Unknown
Year: 2011
Subjects: subject: Farm Management
subject: beef production
subject: NSW
subject: enterprise choices
subject: profitability
subject: market trends

description: Erratic rainfall and rapidly changing world markets have led to volatile stock prices and variable returns to beef producers in recent years. Many producers have subsequently reviewed their choice of enterprise or management system and so an examination of long-term markets is useful when contemplating or advising on possible changes. A comparison of selected beef enterprise gross margins from 1999-2010 indicates that producers supplying markets with tighter supply specifications were generally rewarded with higher returns. For example, EU producers are obliged to maintain rigorous records, subjected to audits, and need improved pastures in order to produce heavy, finished, young cattle. Accordingly, returns in that enterprise have often been among the highest. Conversely, returns from weaner production were, on average, the lowest of those presented. There are no specifications for weaners; they can be produced from all classes of land and many producers revert to this production system during droughts or to realise quick returns. Note that rising input costs and variable market premiums have recently impacted most enterprises.
description: Special Edition Sheep and Cattle Production in New South Wales
On the saturation of acoustic mode frequencies at high solar activity
Creators: name: Soares, M. Cristina Rabello
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Acoustic mode frequencies obtained by applying spherical harmonic decomposition to HMI, MDI and GONG observations were analysed throughout the solar cycle. Evidence of a deviation from a linear relation with solar radio flux was found indicating a saturation effect at high solar activity. The Gompertz model, which is one of the most frequently used sigmoid functions to fit growth data, is used. It is shown that its fitting to MDI and GONG data are statistically significant and a median saturation of four-hundred sfu is estimated. This saturation level is 50% larger than any obtained in the last century, hence the small effect observed in the minimum-to-maximum frequency shift. However, as shown here, it should not be disregarded.
description: Accepted on 2019 April 02 for publication MNRAS
Two New Low Redshift 21cm Absorbers
Creators: name: Lane, W. M.
name: Briggs, F. H.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: As part of a larger program to identify low redshift radio analogues of the damped Lyman-alpha (DLA) absorbers seen in the spectra of high redshift quasars, Westerbork Synthesis Radio Telescope (WSRT) observations have discovered two new HI 21cm absorption lines at z=0.394 and z=0.437 in the spectra of the radio sources B 0248+430 and B 1243-072 respectively. These sightlines and redshifts were selected for study on the basis of the previously known low ionization absorption lines of MgII, and neither has been observed in the Lyman-alpha line. The 21cm line observations provide information on column densities, temperatures and kinematics of the thickest cold neutral clouds in the absorbers.
description: 6 pages incl. 2 figures, accepted for publication in the Astrophysical Journal Letters, missing reference added
Additional file 1 of “I am not really into the government telling me what I need to eat”: exploring dietary beliefs, knowledge, and practices among ethnically diverse communities in England
Creators: name: Ojo, Abimbola S.
name: Nnyanzi, Lawrence A.
name: Giles, Emma L.
name: Ells, Louisa
name: Okeke, Sylvester R.
name: Ajayi, Kobi V.
name: Bolarinwa, Obasanjo Afolabi
Publisher: name: figshare
Year: 2023
Subjects: subject: Sociology
subject: FOS: Sociology

description: Supplementary Material 1
Workshop: Praktické využití umělé inteligence v praxi knihovníků
Creators: name: Švidrnochová, Kateřina
Publisher: name: AKVŠ ČR
Year: 2024
Subjects: BA2024

description: Prezentováno na konferenci Bibliotheca academica 2024.
description: Jak si z umělé inteligence udělat praktického pomocníka pro každodenní práci? Společně prozkoumáme praktické aplikace umělé inteligence, které nám ušetří čas a zjednoduší složité procesy tak, aby nám práce dělala radost. Ukážeme si práci s chatboty, základy promptování – tedy umění kladení otázek tak, aby vám AI poskytla přesně ty informace, které potřebujete. Dále se podíváme na to, jak využít nástroj Canva pro generování vizuálních a video materiálů, které zaujmou návštěvníky knihovny. Praktické ukázky a cvičení vám umožní si vše vyzkoušet na vlastní kůži a odnést si konkrétní dovednosti, které můžete okamžitě aplikovat ve své práci.
MGP-AttTCN: An Interpretable Machine Learning Model for the Prediction of Sepsis
Creators: name: Rosnati, Margherita
name: Fortuin, Vincent
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: With a mortality rate of 5.4 million lives worldwide every year and a healthcare cost of more than 16 billion dollars in the USA alone, sepsis is one of the leading causes of hospital mortality and an increasing concern in the ageing western world. Recently, medical and technological advances have helped re-define the illness criteria of this disease, which is otherwise poorly understood by the medical society. Together with the rise of widely accessible Electronic Health Records, the advances in data mining and complex nonlinear algorithms are a promising avenue for the early detection of sepsis. This work contributes to the research effort in the field of automated sepsis detection with an open-access labelling of the medical MIMIC-III data set. Moreover, we propose MGP-AttTCN: a joint multitask Gaussian Process and attention-based deep learning model to early predict the occurrence of sepsis in an interpretable manner. We show that our model outperforms the current state-of-the-art and present evidence that different labelling heuristics lead to discrepancies in task difficulty. For instance, when predicting sepsis five hours prior to onset on our new realistic labels, our proposed model achieves an area under the ROC curve of 0.660 and an area under the PR curve of 0.483, whereas the (less interpretable) previous state-of-the-art model (MGP-TCN) achieves 0.635 AUROC and 0.460 AUPR and the popular commercial InSight model achieves 0.490 AUROC and 0.359 AUPR.
description: Published at PLOS ONE
BUSINESS SUMMARY NEW YORK STATE 2004
Creators: name: Knoblauch, Wayne A.
name: Putnam, Linda D.
name: Karszes, Jason
name: Knoblauch, Wayne A.
name: Putnam, Linda D.
name: Karszes, Jason
Publisher: name: Unknown
Year: 2005
Subjects: subject: Livestock Production/Industries
subject: BUSINESS ANALYSIS
subject: DAIRY MANAGEMENT
subject: FARM BUSINESS SUMMARY
subject: NEW YORK FARMS

description: Business and financial records for 2004 from 200 New York dairy farm businesses are summarized and analyzed. This analysis demonstrates the use of cash accounting with accrual adjustments to measure farm profitability, financial performance, and costs of producing milk. Traditional methods of analyzing dairy farm businesses are combined with evaluation techniques that show the relationship between good management performance and financial success. The farms in the project averaged 334 cows per farm and 22,070 pounds of milk sold per cow, which represent above average size and management level for New York dairy farms. Net farm income excluding appreciation, which is the return to the operator's labor, management, capital, and other unpaid family labor, averaged $200,863 per farm. The rate of return to all capital invested in the farm business including appreciation averaged 11.3 percent. Differences in profitability between farms continue to widen. Average net farm income excluding appreciation of the top 10 percent of farms was $838,746, while the lowest 10 percent was a negative $11,854. Rates of return on equity with appreciation ranged from 46 percent to negative 11 percent for the highest 10 percent and the lowest 10 percent of farms, respectively. Large freestall farms averaged the highest milk output per cow and per worker, the lowest total cost of production and investment per cow, and the greatest returns to labor, management and capital. Farms milking three times a day (3X) were larger, produced more milk per cow and had higher net incomes than herds milking two times per day (2X). Operating costs per hundredweight of milk were $0.08 per hundredweight higher for 3X than 2X milking herds, while output per cow was 3,950 pounds higher. In 2004, farms supplementing the herd with bovine somatotropin (bST) attained higher rates of milk production per cow, had larger herds and were more profitable than farms not supplementing with bST for all measures of profitability. Farms adopting rotational grazing generally produced less milk per cow than non-grazing farms but had lower costs of production and higher profitability. One should not conclude that adoption of these technologies alone were responsible for differences in performance.
The Universal Mass Accretion History of CDM Haloes
Creators: name: Bosch, Frank C. van den
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use the extended Press-Schechter formalism to investigate the rate at which cold dark matter haloes accrete mass. We discuss the shortcomings of previous methods that have been used to compute the mass accretion histories of dark matter haloes, and present an improved method based on the N-branch merger tree algorithm of Somerville & Kolatt. We show that this method no longer suffers from inconsistencies in halo formation times, and compare its predictions with high resolution N-body simulations. Although the overall agreement is reasonable, there are slight inconsistencies which are most easily interpreted as a reflection of ellipsoidal collapse (as opposed to spherical collapse assumed in the Press-Schechter formalism). We show that the average mass accretion histories follow a simple, universal profile, and we present a recipe for computing the two scale-parameters which is applicable to a wide range of halo masses and cosmologies. Together with the universal profiles for the density and angular momentum distributions of CDM haloes, these universal mass accretion histories provide a simple but accurate framework for modeling the structure and formation of dark matter haloes. In particular, they can be used as a backbone for modeling various aspects of galaxy formation where one is not interested in the detailed effects of merging. As an example we use the universal mass accretion history to compute the rate at which haloes accrete mass, which we compare to the cosmic star formation history of the Universe.
description: Replaced with accepted version. Small changes to text and some figures. In addition, new appendix added presenting a detailed comparison with the work of Wechsler et al
Bezzia (Bezzia) punctipennis
Creators: name: William L. Grogan, Jr.
name: Hribar, Lawrence J.
name: Murphree, C. Steven
name: Cilek, James E.
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Ceratopogonidae
Bezzia
Bezzia punctipennis

description: Bezzia (Bezzia) punctipennis (Williston)
 Ceratopogon punctipennis Williston, 1896: 278 (St. Vincent, West Indies).
 Bezzia punctipennis: Kieffer 1906: 58 (combination); Wirth 1952a: 235 (California; distribution).
 Bezzia (Pseudobezzia) punctipennis: Dow and Turner 1976: 68 (in revision of Nearctic Bezzia; distribution).
 Bezzia (Bezzia) punctipennis: Wilkening et al. 1985: 529 (Florida records); Borkent and Grogan 2009: 26 (in Nearctic catalog; distribution).
 Probezzia punctipennis: Johannsen 1943: 785 (combination).
 Discussion. This primarily Neotropical species is also known from California, Florida, Nevada and Texas and is unusual among New World Bezzia in that its wing has large, distinct, dark gray maculations. Wilkening et al. (1985) listed it in Florida from Dade and Palm Beach counties. We provide the first record from Alachua Co.
 New records. Alachua Co., Gainesville, Oakcrest, 10-IX-1992, W. W. Wirth, Blacklight trap, 1 female (FSCA).
description: Published as part of William L. Grogan, Jr., Hribar, Lawrence J., Murphree, C. Steven & Cilek, James E., 2010, New records of biting and predaceous midges from Florida, including species new to the fauna of the United States (Diptera: Ceratopogonidae), pp. 1-59 in Insecta Mundi 2010 (147) on pages 49-50, DOI: 10.5281/zenodo.5352908
Escape-rate formalism, decay to steady states, and divergences in the entropy-production rate
Creators: name: Vollmer, Juergen
name: Matyas, Laszlo
name: Tel, Tamas
Publisher: name: arXiv
Year: 2001
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: In summer 1997 we were sitting with Bob Dorfman and a few other friends interested in chaotic systems and transport theory on a terrace close to Oktogon in Budapest. While taking our (decaf) coffee after a very nice Italian meal, we discussed about logarithmic divergences in the entropy production of systems with absorbing boundary conditions and their consequences for the escape-rate formalism. It was guessed at that time that the problem could be resolved by a careful discussion of the physical content of the absorbing boundary conditions. To our knowledge a thorough analysis of this long-standing question is still missing. We dedicate it hereby to Bob on occasion of his 65th birthday.
description: 16 pages; RevTex 4 with graphicx package; eps-figures
Determination of cosmology and evolution from K-band magnitude-redshift and number count observations
Creators: name: Jackson, J. C.
name: Dodgson, Marina
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We determine cosmological and evolutionary parameters from the 3CR K-band Hubble diagram and K-band number counts, assuming that the galaxies in question undergo pure luminosity evolution. Separately the two data sets are highly degenerate with respect to choice of cosmological and evolutionary parameters, but in combination the degeneracy is resolved. Of models which are either flat or have $Ω_Λ=0$, the preferred ones are close to the canonical case $Ω_\CdM=1$, $Ω_Λ=0$, with luminosity evolution amounting to one magnitude brighter at z=1.
Energy Balance Climate Models, Damage Reservoirs and the Time Profile of Climate Change Policy
Creators: name: Brock, William A.
name: Engstrom, Gustav
name: Xepapadeas, Anastasios
name: Brock, William A.
name: Engstrom, Gustav
name: Xepapadeas, Anastasios
Publisher: name: Unknown
Year: 2012
Subjects: subject: Environmental Economics and Policy
subject: Energy Balance Climate Models
subject: Damage Reservoir
subject: Ice Line
subject: Permafrost
subject: Heat Diffusion
subject: Policy Ramp
subject: Skiba Points

description: A simplified energy balance climate model is considered with the global mean temperature as the state variable, and an endogenous ice line. The movements of the ice line towards the Poles are associated with damage reservoirs where initial damages are high and then eventually vanish as the ice caps vanish and the damage reservoir is exhausted. We couple this climate model with a simple economic growth model and we show that the endogenous ice line induces a nonlinearity. This nonlinearity when combined with two sources of damages - the conventional damages due to temperature increase and the reservoir damages - generates multiple steady states and Skiba points. It is shown that the policy ramp implied by this model calls for high mitigation now. Simulation results suggest that the policy ramp could be U-shaped instead of the monotonically increasing with low starting mitigation gradualist policy ramp.
Gonzenbach, V
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1835

description: Ort: Messina
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Guenet, C. F
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1835

description: Ort: Paris
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Additional file 5: of Immunohistochemical validation of COL3A1, GPR158 and PITHD1 as prognostic biomarkers in early-stage ovarian carcinomas
Creators: name: Engqvist, Hanna
name: Toshima Parris
name: Anikรณ Kovรกcs
name: Szilรกrd Nemes
name: Rรถnnerman, Elisabeth Werner
name: Lara, Shahin De
name: Biermann, Jana
name: Sundfeldt, Karin
name: Karlsson, Per
name: Helou, Khalil
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Cell Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer

description: Table S1. Reporting recommendations for tumor marker prognostic 642 studies (REMARK) guidelines. (DOCX 22 kb)
The BL Lac heart of Centaurus A
Creators: name: Chiaberge, Marco
name: Capetti, Alessandro
name: Celotti, Annalisa
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Emission from the nucleus of the closest radio galaxy, Centaurus A, is observed from the radio to the gamma ray band. We build, for the first time, its overall Spectral Energy Distribution (SED) that appears to be intriguingly similar to those of blazars, showing two broad peaks located in the far-infrared band and at ~0.1 MeV respectively. The whole nuclear emission of Centaurus A is successfully reproduced with a synchrotron self-Compton model. The estimated physical parameters of the emitting source are similar to those of BL Lacs, except for a much smaller beaming factor, as qualitatively expected when a relativistic jet is orientated at a large angle to the line of sight. These results represent strong evidence that Centaurus A is indeed a misoriented BL Lac and provide strong support in favour of the unification scheme for low luminosity radio-loud AGNs. Modeling of the SED of Centaurus A also provides further and independent indications of the presence of velocity structures in sub-pc scale jets.
description: 5 pages, 2 figures, accepted for publication in MNRAS, pink pages
Forcart-Bachofen
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1835

description: Ort: Basel
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Additional file 6: of Immunohistochemical validation of COL3A1, GPR158 and PITHD1 as prognostic biomarkers in early-stage ovarian carcinomas
Creators: name: Engqvist, Hanna
name: Toshima Parris
name: Anikรณ Kovรกcs
name: Szilรกrd Nemes
name: Rรถnnerman, Elisabeth Werner
name: Lara, Shahin De
name: Biermann, Jana
name: Sundfeldt, Karin
name: Karlsson, Per
name: Helou, Khalil
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: Inorganic Chemistry

description: Table S2. Distribution of clinicopathological characteristics 645 in relation to COL3A1, GPR158 and PITHD1 protein expression. (DOCX 22 kb)
Small-Worlds, Mazes and Random Walks
Creators: name: Luque, Bartolo
name: Octavio, Miramontes
Publisher: name: arXiv
Year: 2002
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We establish a relationship between the Small-World behavior found in complex networks and a family of Random Walks trajectories using, as a linking bridge, a maze iconography. Simple methods to generate mazes using Random Walks are discussed along with related issues and it is explained how to interpret mazes as graphs and loops as shortcuts. Small-World behavior was found to be non-logarithmic but power-law in this model, we discuss the reason for this peculiar scaling
description: article, 7 figures
DATS-6401 Amazon Rainforest Fire
Creators: name: Jiachen Li
Publisher: name: Zenodo
Year: 2021

description: The Amazon rainforest is approximately eight million square kilometers in size and is home to an incredible amount of biodiversity. It contributes to the global carbon budget by absorbing carbon dioxide from the atmosphere. It also plays a vital role in the worldwide water cycle, helping to stabilize global climate and rainfall. However, the rainforest began to experience the worst fires in a decade in 2020. This page will go through an overview of the Amazon rainforest fire.
Frey, Thurneysen & Christ
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1835

description: Ort: Basel
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Stochastic Dynamic Games in Belief Space
Creators: name: Schwarting, Wilko
name: Pierson, Alyssa
name: Karaman, Sertac
name: Rus, Daniela
Publisher: name: arXiv
Year: 2019
Subjects: subject: Robotics (cs.RO)
subject: Computer Science and Game Theory (cs.GT)
subject: Multiagent Systems (cs.MA)
subject: FOS: Computer and information sciences

description: Information gathering while interacting with other agents under sensing and motion uncertainty is critical in domains such as driving, service robots, racing, or surveillance. The interests of agents may be at odds with others, resulting in a stochastic non-cooperative dynamic game. Agents must predict others' future actions without communication, incorporate their actions into these predictions, account for uncertainty and noise in information gathering, and consider what information their actions reveal. Our solution uses local iterative dynamic programming in Gaussian belief space to solve a game-theoretic continuous POMDP. Solving a quadratic game in the backward pass of a game-theoretic belief-space variant of iLQG achieves a runtime polynomial in the number of agents and linear in the planning horizon. Our algorithm yields linear feedback policies for our robot, and predicted feedback policies for other agents. We present three applications: active surveillance, guiding eyes for a blind agent, and autonomous racing. Agents with game-theoretic belief-space planning win 44% more races than without game theory and 34% more than without belief-space planning.
description: Accepted in IEEE Transactions on Robotics (T-RO) 2021