cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
In vitro αξιολόγηση της ανοχής του ισχιακού νεύρου του επίμνος σε συνθήκες υποξίας και ανοξίας
Creators: name: Καγιαβά, Αλεξία Στέλιου
Publisher: name: Aristotle University of Thessaloniki
Year: 2007
Subjects: Ισχιακό νεύρο
Υποξία
Ανοξία
Ανοχή στην ανοξία
Θερμοκρασία
N-acetyl-d-cysteine (NAC)
Sciatic nerve
Hypoxia
Anoxia
Tolerance under conditions of anoxia
Temperature

description: Στην παρούσα εργασία έγινε αξιολόγηση της ανοχής του ισχιακού νεύρου του επίμυος σε συνθήκες υποξίας και ανοξίας. Μελετήθηκε η βιωσιμότητα του ισχυακού νεύρου στις διαφορετικές συνθήκες οξυγόνωσης-συνεχής οξυγόνωση, μερική οξυγόνωση, υποξία, ανοξία, πλήρης ανοξία-καθώ και οι επιπτώσεις των συνθηκών αυτών στις ηλεκτροφυσιολογικές ιδιότητες του νεύρου. Επιπλέον, ελέγχθηκε η ανοχή του ισχιακού νεύρου σε συνθήκες πλήρους ανοξίας. Μελετήθηκε επίσης η πιθανή νευροπροστατευτική δράση της μείωσης της θερμοκρασίας-από τους 37oC στους 25oC-καθώς και της αντιοξειδωτικής ένωσης N-acetyl-L-cysteine(NAC) που εξουδετερώνει ρίζες οξυγόνου
description: The aim of this study was the evaluation of tolerance of the rat sciatic nerve under conditions of hypoxia and anoxia. The viability of the nerve was studied under different conditions of oxygenation-continuous oxygenation, oxygenation after 4 hours, hypoxia, anoxia, complete conditions of hypoxia and anoxia-and the changes of the electrophysiological properties of the nerve. The tolerance of the rat sciatic nerve under conditions of complete anoxia was also studied as well as the possible neuroprotective effect of the reduction of the temperature-37oC to 25oC-and the neuroprotective effect of the antioxidant N-acetyl-L-cysteine(NAC)
Disparities in Nursing Home Quality Selected Measures - United States 2011
Creators: name: UNSPECIFIED
Publisher: name: Digital Repository at the University of Maryland
Year: 2014
Subjects: Access To Healthcare
Disparities
US Department of Health and Human Services

description: While the health care quality improvement community has prioritized health disparities in acute care settings, such as hospital inpatient and ambulatory care, less attention was given to disparities in long-term care. This is despite the fact that a growing body of evidence documents pervasive racial, ethnic, and class disparities in long-term care in the United States.5-10 Furthermore, in the past decade, nursing homes have instituted various quality improvement programs and collaboratives, but it is unclear what effect they might have had on disparities. To determine what effect quality improvement efforts have had on disparities, we conducted analyses of the prevalence of selected nursing home clinical measures among long-stay nursing home residents.
Thirty Years of Composite Fermions and Beyond
Creators: name: Jain, J. K.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: This chapter appears in "Fractional Quantum Hall Effects: New Development," edited by B. I. Halperin and J. K. Jain (World Scientific, 2020). The chapter begins with a primer on composite fermions, and then reviews three directions that have recently been pursued. It reports on theoretical calculations making detailed quantitative predictions for two sets of phenomena, namely spin polarization transitions and the phase diagram of the crystal. This is followed by the Kohn-Sham density functional theory of the fractional quantum Hall effect. The chapter concludes with recent applications of the parton theory of the fractional quantum Hall effect to certain delicate states.
description: Review with 79 pages, 19 figures
THE PERMIAN KULING GROUP (SPITI, LAHAUL AND ZANSKAR; NW HIMALAYA): SEDIMENTARY EVOLUTION DURING RIFT/DRIFT TRANSITION AND INITIAL OPENING OF NEO-TETHYS
Creators: name: GARZANTI, EDUARDO
name: ANGIOLINI, LUCIA
name: SCIUNNACH, DARIO
Publisher: name: Università degli Studi di Milano
Year: 1996

description: Rivista italiana di Paleontologia e Stratigrafia, Vol 102, No 2
Gravitational Lensing of Supernova Neutrinos
Creators: name: Mena, Olga
name: Mocioiu, Irina
name: Quigg, Chris
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The black hole at the center of the galaxy is a powerful lens for supernova neutrinos. In the very special circumstance of a supernova near the extended line of sight from Earth to the galactic center, lensing could dramatically enhance the neutrino flux at Earth and stretch the neutrino pulse.
description: 10 pages, 4 figures, uses RevTeX
Reading the Poetry of António Ramos Rosa from a Distance: Bird's-Eye View, Kingdoms of Nature, The Four Elements (SCRIPTS for generating datasets-bundle-2)
Creators: name: Ministro, Bruno
name: Reina, Patrícia Esteves
Publisher: name: Zenodo
Year: 2024

description: Scripts created by Patrícia Esteves Reina with contributions from Bruno Ministro

 

Corpus: António Ramos Rosa's complete poetryLanguage: Portuguese (Portugal)Language of annotation: English

 

Scripts for text analysis in R language

Visão Panorâmica (Bird’s-Eye View)

Reinos Animal, Vegetal e Mineral (Kingdoms of Nature)

Quatro Elementos (The Four Elements)

 

Development and annotation

Timeframe: October 2023 - June 2024

Work Package 2

Scripts used for generating datasets-bundle-2

Annotated version produced in September 2024

Timestamps of the .csv files attached here: 09-10-2024

 

Exploratory research project (2022.08122.PTDC)To See the Tree and the Forest. Reading the Poetry of António Ramos Rosa from a Distancehttps://doi.org/10.54499/2022.08122.PTDCFunding: Fundação para a Ciência e a Tecnologia, PortugalPI: Bruno MinistroHost: Institute for Comparative Literature - Faculty of Arts and Humanities of the University of Portohttps://arvore.ilcml.com/en/home-en/
FIRST REPORT OF CLARAIA (BIVALVIA) IN THE SERVINO FORMATION (LOWER TRIASSIC) OF THE WESTERN OROBIC ALPS, ITALY
Creators: name: POSENATO, RENATO
name: SCIUNNACH, DARIO
name: GARZANTI, EDUARDO
Publisher: name: Università degli Studi di Milano
Year: 1996

description: Rivista italiana di Paleontologia e Stratigrafia, Vol 102, No 2
Neoperlops obscuripennis Banks 1939
Creators: name: Mo, Raorao
name: Wang, Guoquan
name: Li, Weihai
name: Murányi, Dávid
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperlops
Neoperlops obscuripennis

description: Neoperlops obscuripennis species group
This morphological species group is characterized by the short hemitergal apex of the male, and smooth chorion of the eggs. Contains three species:
description: Published as part of Mo, Raorao, Wang, Guoquan, Li, Weihai & Murányi, Dávid, 2020, Review of the Oriental genus Neoperlops Banks, 1939 (Plecoptera: Perlidae), pp. 405-418 in Zootaxa 4763 (3) on page 409, DOI: 10.11646/zootaxa.4763.3.5, http://zenodo.org/record/3759537
Nonmonotonic Pressure Dependence of the Lattice Parameter $a$ in the Quasi-one-dimensional Superconductor Pr$_2$Ba$_4$Cu$_7$O$_{15-δ}$
Creators: name: Taniguchi, Haruka
name: Nakarokkaku, Yuya
name: Takahashi, Riku
name: Murakami, Masatoshi
name: Nakayama, Atsuko
name: Matsukawa, Michiaki
name: Nakano, Satoshi
name: Hagiwara, Makoto
name: Sasaki, Takahiko
Publisher: name: arXiv
Year: 2020
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: In the quasi-one-dimensional superconductor, Pr$_2$Ba$_4$Cu$_7$O$_{15-δ}$, we found that the lattice parameter, $a$ increased against pressure, starting at 2.0 GPa at approximately 300 K. This result suggests that the two-dimensional inter-conducting-chain interaction along the $a$ axis is most enhanced at approximately 2.0 GPa. To discuss the dimensionality, we also measured the resistance under magnetic fields up to 14 T, because magneto-resistance is induced when a system changes from one-dimensional to two-dimensional.
Evolution of Close White Dwarf Binaries
Creators: name: Gokhale, Vayujeet
name: Peng, Xiao Meng
name: Frank, Juhan
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe the evolution of double degenerate binary systems, consisting of components obeying the zero temperature mass radius relationship for white dwarf stars, from the onset of mass transfer to one of several possible outcomes including merger, tidal disruption of the donor, or survival as a semi-detached AM CVn system. We use a combination of analytic solutions and numerical integrations of the standard orbit-averaged first-order evolution equations, including direct impact accretion and the evolution of the components due to mass exchange. We include also the effects of mass-loss during super-critical (super-Eddington) mass transfer and the tidal and advective exchanges of angular momentum between the binary components. We cover much the same ground as Marsh et al.(2004) with the additional effects of the advective or consequential angular momentum from the donor and its tidal coupling to the orbit which is expected to be stronger than that of the accretor. With the caveat that our formalism does not include an explicit treatment of common envelope phases, our results suggest that a larger fraction of detached double white dwarfs than what has been hitherto assumed, survive the onset of mass transfer, even if this mass transfer is initially unstable and rises to super-Eddington levels. In addition, as a consequence of the tidal coupling, systems that come into contact near the mass transfer instability boundary undergo a phase of oscillation cycles in their orbital period (and other system parameters). Much of the formalism developed here would also apply to other mass-transferring binaries, and in particular to cataclysmic variables and Algol systems.
description: Accepted for publication in ApJ
Tracking Down a Critical Halo Mass for Killing Galaxies through the Growth of the Red-Sequence
Creators: name: Gilbank, David G.
name: Balogh, Michael L.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Red-sequence galaxies record the history of terminated star-formation in the Universe and can thus provide important clues to the mechanisms responsible for this termination. We construct composite samples of published cluster and field galaxy photometry in order to study the build-up of galaxies on the red-sequence, as parameterised by the dwarf-to-giant ratio (DGR). We find that the DGR in clusters is higher than that of the field at all redshifts, implying that the faint end of the red-sequence was established first in clusters. We find that the DGR evolves with redshift for both samples, consistent with the ``down-sizing'' picture of star formation. We examine the predictions of semi-analytic models for the DGR and find that neither the magnitude of its environmental dependence nor its evolution is correctly predicted in the models. Red-sequence DGRs are consistently too high in the models, the most likely explanation being that the strangulation mechanism used to remove hot gas from satellite galaxies is too efficient. Finally we present a simple toy model including a threshold mass, below which galaxies are not strangled, and show that this can predict the observed evolution of the field DGR.
description: MNRAS letters accepted. 5 pages, 1 figure
Mito sobre Yompor Yompuer, Nuestro Padre Yompuer
Creators: name: Huayol, Domingo
name: Santos Granero, Fernando
Publisher: name: California Language Archive, University of California, Berkeley
Year: 2021
Subjects: subject: ame

description: Hermano de la divinidad solar Yompor Ror. Transcrito, traducido, mecanografiado y digitalizado.
Neoperlops obscuripennis Banks 1939
Creators: name: Mo, Raorao
name: Wang, Guoquan
name: Li, Weihai
name: Murányi, Dávid
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperlops
Neoperlops obscuripennis

description: Neoperlops obscuripennis Banks, 1939
 Neoperlops obscuripennis Banks, 1939 — Banks 1939: 445. (original description of the female from Guangdong); Illies 1966: 493. (species inquirenda, catalog); Zwick 1984: 174. (redescription of female based on types); Sivec et al. 1988: 40. (synopsis); Du et al. 1999: 61 (checklist); Stark & Sivec 2008: (description of putative male and larva from Vietnam (partim?)); Yang & Li 2018: 32. (catalog); DeWalt et al. 2020 (catalog).
 Distribution. China, described from Guangdong Province, Yim Na San, based on four females (Banks 1939). Stark & Sivec (2008) reported several specimens from Vietnam, including males, females and larvae (Lào Cai, Nghệ An and Vĭnh Phúc provinces).
 Remarks. The female types of N. obscuripennis are distinctive by having elongated oval eggs, contrary to nearly globular eggs of the congeners (Zwick 1984). The putative male and larva from Vietnam were associated with this species based on the female and eggs similar to the redescription of the types (Stark & Sivec 2008). However, the illustrated Vietnamese eggs are nearly globular (Stark & Sivec 2008, fig. 7), so conspecificity can be questioned. In addition, Stark & Sivec (2008) mention one male specimen that lacked spines on the apex of male hemiterga, a character that is characteristic for N. vietnamellus and the proposed new species. Molecular studies of topotypes are needed to clear identity of the species.
description: Published as part of Mo, Raorao, Wang, Guoquan, Li, Weihai & Murányi, Dávid, 2020, Review of the Oriental genus Neoperlops Banks, 1939 (Plecoptera: Perlidae), pp. 405-418 in Zootaxa 4763 (3) on page 409, DOI: 10.11646/zootaxa.4763.3.5, http://zenodo.org/record/3759537
Structured, relativistic jets driven by radiation
Creators: name: Coughlin, Eric R.
name: Begelman, Mitchell C.
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Relativistic jets, or highly collimated and fast-moving outflows, are endemic to many astrophysical phenomena. The jets produced by gamma-ray bursts and tidal disruption events are accompanied by the accretion of material onto a black hole or neutron star, with the accretion rate exceeding the Eddington limit of the compact object by orders of magnitude. In such systems, radiation dominates the energy-momentum budget of the outflow, and the dynamical evolution of the jet is governed by the equations of radiation hydrodynamics. Here we show that there are analytic solutions to the equations of radiation hydrodynamics in the viscous (i.e., diffusive) regime that describe structured, relativistic jets, which consist of a fast-moving, highly relativistic core surrounded by a slower-moving, less relativistic sheath. In these solutions, the slower-moving, outer sheath contains most of the mass, and the jet structure is mediated by local anisotropies in the radiation field. We show that, depending on the pressure and density profile of the ambient medium, the angular profile of the jet Lorentz factor is Gaussian or falls off even more steeply with angle. These solutions have implications for the nature of jet production and evolution in hyperaccreting systems, and demonstrate that such jets -- and the corresponding jet structure -- can be sustained entirely by radiative processes. We discuss the implications of these findings in the context of jetted tidal disruption events and short and long gamma-ray bursts.
description: MNRAS Accepted
Neoperlops cheni
Creators: name: Mo, Raorao
name: Wang, Guoquan
name: Li, Weihai
name: Murányi, Dávid
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperlops
Neoperlops cheni

description: Neoperlops cheni (Wu, 1938)
 Tetropina cheni Wu, 1938 — Wu 1938: 206. (original description of the male from Guangxi); Claassen 1940: 170. (catalog); Illies 1966: 300. (catalog).
 Neoperlops cheni (Wu, 1938) — Zwick 1984: 173. (comb. n., note on the similarity with N. gressitti); Sivec et al. 1988: 40. (synopsis); Du et al. 1999: 61 (checklist); Stark & Sivec 2008: 94. (note on possible conspecific with N. gressitti); Yang & Li 2018: 32. (catalog); DeWalt et al. 2020. (catalog).
 Distribution. China, Guangxi Zhuang Autonomous Region, Lo Ch’eng. Previously known only from the holotype male, which is lost (Wu 1938a, Zwick 1984).
 Remarks. Zwick (1984) noted that only on the basis of the original description, this species is indistinguishable from N. gressitti. Despite that this is the only species hitherto known from Guangxi, below we report our gressitti group specimen as N. gressitti. Wu (1938, figs. 308–309) originally illustrated an undivided sensilla basiconica patch on tergum 9, probably a species specific character of Neoperlops. Our specimen has a divided sensilla patch, similar to the redescription of N. gressitti (Zwick 1984: fig. 2d). However, topotypes need to be examined from Luocheng City (Lo Ch’eng) to clarify this the status of this species.
description: Published as part of Mo, Raorao, Wang, Guoquan, Li, Weihai & Murányi, Dávid, 2020, Review of the Oriental genus Neoperlops Banks, 1939 (Plecoptera: Perlidae), pp. 405-418 in Zootaxa 4763 (3) on page 406, DOI: 10.11646/zootaxa.4763.3.5, http://zenodo.org/record/3759537
Ιερά και λατρεία της Αθηνάς στην Ιωνία κατά την αρχαϊκή περίοδο
Creators: name: Μπέτσιου, Αταλάντη Χρήστου
Publisher: name: Aristotle University of Thessaloniki
Year: 2007
Subjects: Ασπιδίσκες
Αγαλμα
Ιερό
Πομπή
Πόρπες
Statue
Sanctuary
Fibula
Shields
Procession

description: Η λατρεία της Αθηνάς στον χώρο της Ιωνίας έχει αστικό χαρακτήρα, όπως άλλωστε υποδηλώνεται με την επίκληση της θεάς ως Πολιάδα ή Πολιούχος. Σύμφωνα με τα πρωιμότερα ευρήματα της Μιλήτου, η χρονική αφετηρία της ανάγεται στο α΄ μισό του 8ου αι.π.Χ., ενώ στην ύστερη αρχαϊκή περίοδο εντοπίζεται στις περισσότερες ιωνικές πόλεις. Με την εξέταση των αναθημάτων, ο μελετητής επικεντρώνει το ενδιαφέρον του στη διερεύνηση επαφών μεταξύ των ιερών της Ιωνίας με τους λαούς της Ανατολής, αλλά και με την μητρόπολη, την Αθήνα.
description: The cult of Athena in Ionia is engrelated to the city and for this reason the goddess is called as Polias or Poliouchos. In the first half of 8th B.C. the cult of Athena appears in Miletus but later, in the late archaic period, it is located in most of the cities. By studying the votive offerings, the researcher is interested to detect the contacts between the sanctuaries of Ionia with the peoples of Asia, and with the mother city Athena
Large mass expansion in two-loop QCD corrections of para-charmonium decay
Creators: name: Hasegawa, K.
name: Pak, Alexey
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate the two-loop QCD corrections to paracharmonium decays $eta_{c} rightarrow gamma gamma$ and $eta_{c} rightarrow g g$ involving light-by-light scattering diagrams with light quark loops. Artificial large mass expansion and convergence improvement techniques are used to evaluate these corrections. The obtained corrections to the decays $eta_{c} rightarrow gamma gamma$ and $eta_{c} rightarrow g g$ account for $-1.25 %$ and $ -0.73 %$ of the leading order contribution, respectively.
description: 24 pages, 10 figures; REVTeX version; Version to appear in Phys. Rev. D, 9 pages, 4 figures
Διερεύνηση απόψεων και προθέσεων χρηστών σταθμών αυτοκινήτων σύγχρονης τεχνολογίας. Η περίπτωση του σταθμού της ΧΑΝΘ
Creators: name: Τσαπικίδης, Ιωάννης Σταύρος
Publisher: name: Aristotle University of Thessaloniki
Year: 2007
Subjects: Στάθμευση
Μηχανικά συστήματα στάθμευσης
Αυτοματοποιημένοι σταθμοί αυτοκινήτων
Απόψεις και προθέσεις χρηστών
Parking places
Automated parking systems
Automated car stations
Opinions and intentions of the users

description: Τα μηχανικά συστήματα στάθμευσης αποτελούν τη σύγχρονη λύση για τη βέλτιστη χρησιμοποίηση του διαθέσιμου χώρου στους σταθμούς αυτοκινήτων, προκειμένου να καλυφθεί η συνεχώς αυξανόμενη ζήτηση για στάθμευση στα κέντρα των πόλεων. Κατέχουν μια σειρά από συγκριτικά πλεονεκτήματα έναντι των συμβατικών τρόπων στάθμευσης που τα καθιστούν άκρως ανταγωνιστικά.Διεθνώς καταγράφονται πλήθος σταθμών που κάνουν χρήση της σύγχρονης τεχνολογίας, ενώ στην πόλη της Θεσσαλονίκης υπάρχει ο μεγαλύτερος αυτοματοποιημένος σταθμός αυτοκινήτων στην Ευρώπη, αυτός που βρίσκεται επί του οικοπέδου της Χ.Α.Ν.Θ.Στην παρούσα Μεταπτυχιακή Διατριβή, έχοντας ως δείγμα τους χρήστες του σταθμού της Χ.Α.Ν.Θ., επιχειρείται διερεύνηση των απόψεων και προθέσεων των χρηστών σταθμών αυτοκινήτων σύγχρονης τεχνολογίας σχετικά με τη συγκεκριμένη τεχνολογία.
description: Automated Parking Systems constitute the modern solution for the most optimal utilisation of available space in the car-stations, in order to supply the continuously increasing demand for parking places in the city-centres. They are characterized by comparative advantages against the conventional ways of parking that make them extremely competitive.A big number of stations that use modern technology are recorded worldwide, while in the city of Thessaloniki the largest automated car-station in Europe is the one which is founded in the area of Y.M.C.A. This specific Thesis attempts - having the users of the Y.M.C.A.-station as sample - to investigate the opinions and intentions of modern technology car-station users regarding this particular technology.
Neoperlops vietnamellus Cao & Bae 2008
Creators: name: Mo, Raorao
name: Wang, Guoquan
name: Li, Weihai
name: Murányi, Dávid
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperlops
Neoperlops vietnamellus

description: Neoperlops vietnamellus Cao & Bae, 2008
 Neoperlops vietnamellus Cao & Bae, 2008 — Cao & Bae 2008: 34. (original description of the male, female and larva from Vietnam); DeWalt et al. 2020 (catalog).
 Distribution. Vietnam, described from Hà Tĭnh, Lào Cai, Phú Thọ and Vĭnh Phúc provinces on the basis of several specimens including males, females and larvae (Cao & Bae 2008).
 Remarks. Affinities of the species were discussed above. Some specimens reported as N. obscuripennis by Stark & Sivec (2008) may refer to this species.
description: Published as part of Mo, Raorao, Wang, Guoquan, Li, Weihai & Murányi, Dávid, 2020, Review of the Oriental genus Neoperlops Banks, 1939 (Plecoptera: Perlidae), pp. 405-418 in Zootaxa 4763 (3) on page 417, DOI: 10.11646/zootaxa.4763.3.5, http://zenodo.org/record/3759537
Stellar populations in the Canis Major over-density
Creators: name: Carraro, Giovanni
name: Moitinho, Andre'
name: Vazquez, Ruben A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We performed a photometric multicolor survey of the core of the Canis Major over-density at l 244, -8.0, reaching V = 22 and covering 0.3 x 1 degree. The main aim is to unravel the complex mixture of stellar populations toward this Galactic direction, where in the recent past important signatures of an accretion event have been claimed to be detected. While our previous investigations were based on disjointed pointings aimed at revealing the large scale structure of the third Galactic Quadrant, we now focus on a complete coverage of a smaller field centered on the Canis Major over-density. A large wave-length baseline, in the UBVRI bands, allows us to build up a suite of colour colour and colour magnitude diagrams, providing a much better diagnostic tool to disentangle the stellar populations of the region. In fact, the simple use of one colour magnitude diagram, widely employed in all the previous studies defending the existence of the Canis Major galaxy, does not allow one to separate the effects of the different parameters (reddening, age, metallicity, and distance) involved in the interpretation of data, forcing to rely on heavy modeling. In agreement with our previous studies in the same general region of the Milky Way, we recognize a young stellar population compatible with the expected structure and extension of the Local (Orion) and Outer (Norma-Cygnus) spiral arms in the Third Galactic Quadrant. Moreover we interpret the conspicuous intermediate-age metal poor population as belonging to the Galactic thick disk, distorted by the effect of strong disk warping at this latitude, and to the Galactic halo.
description: 9 pages, 12 eps figures (some of them somewhat degraded in resolution), accepted for publication in MNRAS
Muon absorption tomography of a lead structure through the use of iterative algorithms
Creators: name: Baccani, Guglielmo
Publisher: name: arXiv
Year: 2020
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The muon radiography technique is part of the straight-ray scanning imaging methods and it is usually employed to produce two-dimensional images of the integrated density in the radial direction from the detector position. However, in the literature there are already some examples of muon tomographies made by combining several measurements from different observation points. The work presented in this article fits into this line of research: a tomography of a target composed of lead blocks arranged in a non-trivial geometry was carried out by means of muon absorption radiography measurements. To solve the inversion problem, an iterative algorithm called SART was employed, obtaining better results than using a Chi-squared minimization.
description: 10 pages, 7 figures
Διάταξη αποτύπωσης σιδηροδρομικής γραμμής με φωτογραμμετρικές μεθόδους: αρχές λειτουργίας, γεωμετρικό μοντέλο και πειραματικά δεδομένα
Creators: name: Σαββουλίδης, Γεώργιος Κωνσταντίνου
Publisher: name: Aristotle University of Thessaloniki
Year: 2007
Subjects: σιδηρόδρομος
Φωτογραμμετρία
Βαθμονόμηση
Μετασχηματισμός ομοιότητας
Railroad
Photogrammetry
Calibration
3d similarity transformation

description: Η συγκεκριμένη εργασία αφορά στην ανάπτυξη ενός συστήματος αποτύπωσης σιδηροδρομικής γραμμής με φωτογραμμετρικές μεθόδους. Στόχος του συστήματος αυτού είναι η αποτύπωση τουλάχιστον 10 μέτρων του αντικειμένου, με επιθυμητή ακρίβεια μικρότερη των 10 χιλιοστών.Θα γίνουν αναφορές στις αρχές της επιστήμης της Φωτογραμμετρίας και στις μαθηματικές εξισώσεις που περιγράφουν τις αρχές αυτές, αφού οι συγκεκριμένες εξισώσεις θα αποτελέσουν το μαθηματικό μοντέλο του συστήματος. Ακολουθεί μία ενδεικτική γεωμετρία του συστήματος αποτύπωσης με κάποια υποχρεωτικά χαρακτηριστικά που διέπουν τη γεωμετρία αυτή.Τέλος παρουσιάζονται πειραματικά αποτελέσματα του συγκεκριμένου συστήματος αποτύπωσης το οποίο προσομοιώθηκε με κατάλληλες διατάξεις.Διάταξη αποτύπωσης σιδηροδρομικής γραμμής με φωτογραμμετρικές μεθόδους : Αρχές λειτουργίας,
description: The particular work concerns the development of a railway surveying system utilising photogrammetric methods. The objective of this system is the imprinting of at least 10 metres of the object, with desirable precision smaller than 10 millimetres. We will refer to the principles of Photogrammetry science plus the mathematic equations that describe these principles, because the specific equations will constitute the mathematical model of the system. It follows an indicative geometry of the surveying system with certain obligatory characteristics that condition this geometry.Finally experimental results of the particular system are presented as a simulation was formed with suitable provisions.
THE LADINIAN AMMONOIDS FROM THE CALCARE DI ESINO OF VAL PARINA (BERGAMASC ALPS, NORTHERN ITALY). PT. 2
Creators: name: FANTINI SESTINI, NERINA
Publisher: name: Università degli Studi di Milano
Year: 1996

description: Rivista italiana di Paleontologia e Stratigrafia, Vol 102, No 2
Cosmology of the Tachyon in Brane Inflation
Creators: name: Leblond, Louis
name: Shandera, Sarah
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In certain implementations of the brane inflationary paradigm, the exit from inflation occurs when the branes annihilate through tachyon condensation. We investigate various cosmological effects produced by this tachyonic era. We find that only a very small region of the parameter space (corresponding to slow-roll with tiny inflaton mass) allows for the tachyon to contribute some e-folds to inflation. In addition, non-adiabatic density perturbations are generated at the end of inflation. When the brane is moving relativistically this contribution can be of the same order as fluctuations produced 55 e-folds before the end of inflation. The additional contribution is very nearly scale-invariant and enhances the tensor/scalar ratio. Additional non-gaussianities will also be generated, sharpening current constraints on DBI-type models which already predict a significantly non-gaussian signal.
description: 30 pages, 2 figures; v3, minor revision, JCAP version
GABANELLIA AGILIS GEN. N. SP. N., (ACTINOPTERYGII, PERLEIDIFORMES) FROM THE CALCARE DI ZORZINO OF LOMBARDY (NORTH ITALY)
Creators: name: TINTORI, ANDREA
name: LOMBARDO, CRISTINA
Publisher: name: Università degli Studi di Milano
Year: 1996

description: Rivista italiana di Paleontologia e Stratigrafia, Vol 102, No 2
Μελέτη της σχέσης μεταξύ της διαχείρισης γνώσης και της ηλεκτρονικής τραπεζικής
Creators: name: Χρυσοπούλου, Σοφία Κωνσταντίνου
Publisher: name: Aristotle University of Thessaloniki
Year: 2007
Subjects: Ηλεκτρονικό εμπόριο
Διαχείριση γνώσης
Ηλεκτρονική τραπεζική
E-commerce
Knowledge management
E-banking

description: Σκοπός της εργασίας είναι να τονιστεί η σημασία της διαχείρισης γνώσης στον τομέα της ηλεκτρονικής τραπεζικής. Οι επιχειρήσεις και οι τράπεζες πρέπει να διαμορφώσουν στρατηγικές διαχείρισης γνώσης που να είναι συνεπείς με τους στόχους ανάπτυξης των προϊόντων και υπηρεσιών τους, τους επιθυμητούς στόχους διείσδυσης σε νέες αγορές και τις χρηματοοικονομικές τους επιδιώξεις. Το διαδίκτυο καθώς και ο ρόλος των νέων τεχνολογιών πληροφορικής και επικοινωνιών είναι καταλυτικά στοιχεία για τη διαχείριση της γνώσης. Ολο και περισσότερες τράπεζες εισάγουν τη διαχείριση γνώσης με σκοπό να καταλάβουν τα χαρακτηριστικά των εργασιών τους αλλά και τους πελάτες τους, είτε πρόκειται για λόγους σχεδίασης εκστρατειών μάρκετινγκ είτε για την επίτευξη ανταγωνιστικού πλεονεκτήματος. Αρκετές τράπεζες χρησιμοποιούν την πληροφόρηση που προσφέρουν τα συστήματα διαχείρισης γνώσης για να εφαρμόσουν πιο επιθετικές στρατηγικές πώλησης και να προσφέρουν υπηρεσίες που προσθέτουν αξία στον τελικό πελάτη.
description: The aim of this work is to stress the importance of knowledge management in the sector of electronic banking. The enterprises and the banks sould shape strategies of knowledge management that would be reliable with the objectives of growth of products and their services, the desirable objectives of infiltration in the new markets and their financing objectives. Internet as well as the role of information technology and communications are catalytic elements for the knowledge management. More banks import the knowledge management with a view to understand the characteristics of their work but also their customers, their reason is the planning of marketing expeditions or the achievement of competitive advantage. Many banks use the information that they acquire from knowledge management systems in order to apply more agressine sale strategies and also offer services that add value for the final customer.
RELATIONSHIPS BETWEEN FORAMINIFERAL ASSEMBLAGES AND DEPOSITIONAL SEQUENCES IN THE MERLI EST SECTION (FIGOLS ALLOGROUP – SOUTH-CENTRAL PYRENEES – LOWER EOCENE)
Creators: name: GABOARDI, SANDRA
Publisher: name: Università degli Studi di Milano
Year: 1996

description: Rivista italiana di Paleontologia e Stratigrafia, Vol 102, No 2
Pfaffian pairing and backflow wave functions for electronic structure quantum Monte Carlo methods
Creators: name: Bajdich, M.
name: Mitas, L.
name: Wagner, L. K.
name: Schmidt, K. E.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We investigate pfaffian trial wave functions with singlet and triplet pair orbitals by quantum Monte Carlo methods. We present mathematical identities and the key algebraic properties necessary for efficient evaluation of pfaffians. Following upon our previous study \cite{pfaffianprl}, we explore the possibilities of expanding the wave function in linear combinations of pfaffians. We observe that molecular systems require much larger expansions than atomic systems and linear combinations of a few pfaffians lead to rather small gains in correlation energy. We also test the wave function based on fully-antisymmetrized product of independent pair orbitals. Despite its seemingly large variational potential, we do not observe additional gains in correlation energy. We find that pfaffians lead to substantial improvements in fermion nodes when compared to Hartree-Fock wave functions and exhibit the minimal number of two nodal domains in agreement with recent results on fermion nodes topology. We analyze the nodal structure differences of Hartree-Fock, pfaffian and essentially exact large-scale configuration interaction wave functions. Finally, we combine the recently proposed form of backflow correlations \cite{drummond_bf,rios_bf} with both determinantal and pfaffian based wave functions.
description: 13 pages, 4 tables, 3 figure, submitted to PRB
Searching for gravitational wave bursts from cosmic string cusps with the Parkes Pulsar Timing Array
Creators: name: Yonemaru, N.
name: Kuroyanagi, S.
name: Hobbs, G.
name: Takahashi, K.
name: Zhu, X. -J.
name: Coles, W. A.
name: Dai, S.
name: Howard, E.
name: Manchester, R.
name: Reardon, D.
name: Russell, C.
name: Shannon, R.
name: Thyagarajan, N.
name: Spiewak, R.
name: Wang, J. -B.
Publisher: name: arXiv
Year: 2020
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Cosmic strings are potential gravitational wave (GW) sources that can be probed by pulsar timing arrays (PTAs). In this work we develop a detection algorithm for a GW burst from a cusp on a cosmic string, and apply it to Parkes PTA data. We find four events with a false alarm probability less than 1%. However further investigation shows that all of these are likely to be spurious. As there are no convincing detections we place upper limits on the GW amplitude for different event durations. From these bounds we place limits on the cosmic string tension of G mu ~ 10^{-5}, and highlight that this bound is independent from those obtained using other techniques. We discuss the physical implications of our results and the prospect of probing cosmic strings in the era of Square Kilometre Array (SKA).
description: Accepted for publication by MNRAS
СОВЕРШЕНСТВОВАНИЕ МЕХАНИЗМА РАБОТЫ С ПРОБЛЕМНЫМИ КРЕДИТАМИ В КОММЕРЧЕСКИХ БАНКАХ
Creators: name: Махмудов, Рахимжан
Publisher: name: Zenodo
Year: 2024

description: В данном тезисе исследованы такие вопросы, как передовой зарубежный опыт работы с проблемными кредитами в коммерческих банках, проблемы в практике работы с проблемными кредитами в коммерческих банках и пути их устранения, пути эффективного управления кредитными рисками банков, а также прогнозирования и планирования проблемных кредитов в коммерческих банках на основе модели ARIMA и по данным проблемам в конце главы сформулированы научные выводы.
Ποιοτικά χαρακτηριστικά προϊόντων με την επωνυμία "Πάστα ελιάς"
Creators: name: Αννίβα, Χριστίνα Πραξιτέλη
Publisher: name: Aristotle University of Thessaloniki
Year: 2007
Subjects: Πάστα ελιάς
Ποιοτικά χαρακτηριστικά
Χλωροφύλλες
Τοκοφερόλες
Σκουαλένιο
Καροτενοειδή
Olive paste
Quality characteristics
Chlorophylls
Tocopherols
Carotenoids
Squalene

description: Τα κύρια συστατικά του προϊόντος με την επωνυμία πάστα ελιάς, είναι η επιτραπέζια ελιά και το ελαιόλαδο. Η πάστα ελιάς ως εδώδιμο προϊόν μπορεί να καταναλωθεί ως έχει ή ενσωματωμένη σε άλλα προϊόντα(π.χ. ενσωματωμένη σε αλλαντικό, αντικαθιστώντας μέρος του ζωϊκού ιστού). Καθώς η ποιότητα της πάστας ελιάς εξαρτάται από τα επίπεδα και τις μεταβολές στα κύτια συστατικά της, στο πλαίσιο της εργασίας εξετάσθηκαν τα ποιοτικά χαρακτηριστικά της λιπαρής φάσης(Π.Φ.), ιδιαίτερα εκείνα που μπορεί να έχουν άμεση σχέση με διατροφικές συστάσεις ή απαιτήσεις. Συγκεκριμένα, η μελέτη επικεντρώθηκε στην εξέταση του περιεχομένου σε σκοναλένιο, τοκοφερόλες, καροτενοειδή και χλωροφύλλες με τη βοήθεια υγροχρωματογραφικών τεχνικών. Επιπλέον, εξετάσθηκε η οξειδωτική κατάσταση της Π.Φ. που παραλήφθηκε και έγιναν παρατηρήσεις σε σχέση με τα επίπεδα προοξειδωτικών/αντιοξειδωτικών ενώσεων και άλλων προσθέτων και βοηθητικών υλών που αναγράφονται στη συσκευασία των τελικών προϊόντων
description: The main components of the product under the name olive paste are table olives and olive oil. As an edible product olive paste can be consumed as such or as a part of other products(e.g. as a part of sausages, replacing part of the animal tishue. As the quality of the olive paste depends on the levels and the changes in its main components, the quality characteristics of the lipid fraction of the product were examined, especially the ones that may be directly related with nutritional value or needs. More specific, the study was focused on the examination of the content in squalene, tocophetols, carotenoids and chlorophylls with the aid of liquid chromatographic techniques. Moreover, the oxidative quality of the extracted lipid fraction was examined, and observation were made related with the levels of prooxidants/ontioxidants and other additives inscribed on the products labels
Gravitational wave stochastic background from cosmic (super)strings
Creators: name: Siemens, Xavier
name: Mandic, Vuk
name: Creighton, Jolien
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the stochastic background of gravitational waves produced by a network of cosmic strings and assess their accessibility to current and planned gravitational wave detectors, as well as to big bang nucleosynthesis (BBN), cosmic microwave background (CMB), and pulsar timing constraints. We find that current data from interferometric gravitational wave detectors, such as LIGO, are sensitive to areas of parameter space of cosmic string models complementary to those accessible to pulsar, BBN, and CMB bounds. Future more sensitive LIGO runs and interferometers such as Advanced LIGO and LISA will be able to explore substantial parts of the parameter space.
description: Replaced with version accepted for publication in Physical Review Letters. 4 pages, 2 figures
Additional file 1 of What is the impact of the Rashomon approach in primary care education?: An educational case report of implementing dialogue and improvisation into medical education
Creators: name: Takamura, Akiteru
name: Imafuku, Rintaro
Publisher: name: figshare
Year: 2021
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1. The questions in the survey questionnaire.
LATE VENDIAN (NEOPROTEROZOIC III) MICROBIAL AND ALGAL COMMUNITIES OF THE RUSSIAN PLATFORM: MODELS OF FACIES-DEPENDENT DISTRIBUTION, EVOLUTION AND REFLECTION OF BASIN DEVELOPMENT
Creators: name: B. BURZIN, MIKHAIL
Publisher: name: Università degli Studi di Milano
Year: 1996

description: Rivista italiana di Paleontologia e Stratigrafia, Vol 102, No 3
Mito sobre el origen de los blancos
Creators: name: Francisco Huayol, Espíritu
name: Santos Granero, Fernando
Publisher: name: California Language Archive, University of California, Berkeley
Year: 2021
Subjects: subject: ame

description: Se trata de un fragmento muy rico del mito de Enc, personaje mítico que se relaciona a la figura histórica del Inca. Transcrito, traducido, mecanografiado y digitalizado.
Participation and meaning in community : from the standpoint of consumers who reside in supported housing
Creators: name: Huston, Chris
Publisher: name: University of British Columbia
Year: 2009

description: This study was carried out within a qualitative research framework. A purposeful sample was utilised with eight individuals in a focus group format, to gather information about their experiences. All eight individuals in the study experienced some form of a psychiatric disability, and lived in supported housing. The purpose of the study was to explore how people with psychiatric disabilities who live in supported housing define, and participate in community. A constant comparative analysis was used during the research, based on structuralist and standpoint theory. This resulted in six major issues/themes: The benefits and importance of the consumer/mental health community; ideas pertaining to community change; positives of support and subsidies; changes needed to support; barriers to involvement in the geographic community; losses. The study provided opportunities for consumers to explore their perceptions of community, and dialogue as a group. Some insight with respect to altering social work practice was developed through the findings. Social workers and other mental health professionals are required to acknowledge the strengths and resources of consumers, and cannot neglect a focus on community change to provide holistic support to individuals who reside in supported housing.
INTEGRAL SPI All-Sky View in Soft Gamma Rays: Study of Point Source and Galactic Diffuse Emissions
Creators: name: Bouchet, L.
name: Jourdain, E.
name: Roques, J. P.
name: Strong, A.
name: Diehl, R.
name: Lebrun, F.
name: Terrier, R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have processed the data accumulated with INTEGRAL SPI during 4 years (~ 51 Ms) to study the Galactic ``diffuse'' emission morphology in the 20 keV to 8 MeV energy range. To achieve this objective, we have derived simultaneously an all-sky census of emitting sources and images of the Galactic Ridge (GR) emission. In the central radian, the resolved point source emission amounts to 88%, 91% and 68% of the total emission in the 25-50, 50-100 and 100-300 keV domains respectively. We have compared the GR emission spatial distribution to those obtained from CO and NIR maps, and quantified our results through latitude and longitude profiles. Below 50 keV, the SPI data are better traced by the latter, supporting a stellar origin for this emission. Furthermore, we found that the GR emission spectrum follows a power law with a photon index ~ 1.55 above 50 keV while an additional component is required below this energy. This component shows a cutoff around 30 keV, reinforcing a stellar origin, as proposed by Krivonos et al. (2007). The annihilation diffuse emission component is extracted simultaneously, leading to the determination of the related parameters (positronium flux and fraction). A specific discussion is devoted to the annihilation line distribution since a significant emission is detected over a region as large as ~80 degrees by ~10 degrees potentially associated with the disk or halo surrounding the central regions of our Galaxy.
description: 28 pages, 10 figures. Astrophysical journal (accepted for publication)
The GUAPOS project: G31.41+0.31 Unbiased ALMA sPectral Observational Survey -- I. Isomers of C$_{2}$H$_{4}$O$_{2}$
Creators: name: Mininni, C.
name: Beltrán, M. T.
name: Rivilla, V. M.
name: Sánchez-Monge, A.
name: Fontani, F.
name: Möller, T.
name: Cesaroni, R.
name: Schilke, P.
name: Viti, S.
name: Jiménez-Serra, I.
name: Colzi, L.
name: Lorenzani, A.
name: Testi, L.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Understanding the degree of chemical complexity that can be reached in star-forming regions, together with the identification of precursors of the building blocks of life in the interstellar medium, is one of the goals of astrochemistry. Unbiased spectral surveys with large bandwidth and high spectral resolution are thus needed, to resolve line blending in chemically rich sources and identify complex organic molecules. This kind of observations has been successfully carried out, mainly towards the Galactic Center, a region that shows peculiar environmental conditions. We present an unbiased spectral survey at 3mm of one of the most chemically rich hot molecular cores located outside the Galactic Center, in the high-mass star-forming region G31.41+0.31. In this first paper, we present the survey and discuss the detection of the 3 isomers of C$_{2}$H$_{4}$O$_{2}$: methyl formate, glycolaldehyde and acetic acid. Observations were carried out with ALMA and cover the entire Band 3 from 84 to 116 GHz with an angular resolution of $1.2^{''}$x$1.2^{''}$ and a spectral resolution of $\sim0.488$ MHz. The transitions of the 3 molecules have been analyzed with the software XCLASS. All three isomers were detected and methyl formate and acetic acid abundances in G31 are the highest detected up to now, if compared to sources in literature. The size of the emission varies among the three isomers with acetic acid showing the most compact emission while methyl formate the most extended. The comparison with chemical models suggests the necessity of grain-surface routes for the formation of methyl formate in G31, while for glycolaldehyde both scenarios could be feasible. Proposed grain-surface reaction for acetic acid is not able to reproduce the observed abundance in this work, while gas-phase scenario should be further tested due to large uncertainties.
description: 49 pages, 29 figures, accepted for publication in A&A
Anisotropic Susceptibility of La_2-xSr_xCoO_4 related to the Spin States of Cobalt
Creators: name: Hollmann, N.
name: Haverkort, M. W.
name: Cwik, M.
name: Benomar, M.
name: Reuther, M.
name: Tanaka, A.
name: Lorenz, T.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present a study of the magnetic susceptibility of La_2-xSr_xCoO_4 single crystals in a doping range 0.3<=x<=0.8. Our data shows a pronounced magnetic anisotropy for all compounds. This anisotropy is in agreement with a low-spin ground state (S=0) of Co^3+ for x>=0.4 and a high-spin ground state (S=3/2) of Co^2+. We compare our data with a crystal-field model calculation assuming local moments and find a good description of the magnetic behavior for x>=0.5. This includes the pronounced kinks observed in the inverse magnetic susceptibility, which result from the anisotropy and low-energy excited states of Co^2+ and are not related to magnetic ordering or temperature-dependent spin-state transitions.