cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A Study of Specific Energy Consumption in Reheating Furnace Using Regenerative Burners Combined with Recuperator
Creators: name: Kanit Manatura
name: Mingsak Tangtrakul
Publisher: name: Silpakorn University Research and Development Institute
Year: 2010
Subjects: Energy consumption, Reheating furnace, Regenerative burners, Recuperator, Energy balance

description: 2, 4, Silpakorn University Science and Technology Journal
Off diagonal charged scalar couplings with the Z boson: the Zee model as an example
Creators: name: Florentino, Ricardo R.
name: Romão, Jorge C.
name: Silva, João P.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Models with scalar doublets and charged scalar singlets have the interesting property that they have couplings between one $Z$ boson and two charged scalars of different masses. This property is often ignored in phenomenological analysis, as it is absent from models with only extra scalar doublets. We explore this issue in detail, considering $h \rightarrow Z γ$, $B \to X_s γ$, and the decay of a heavy charged scalar into a lighter one and a $Z$ boson. We propose that the latter be actively searched for at the LHC, using the scalar sector of the Zee model as a prototype and proposing benchmark points which obey all current experimental data and could be within reach of the LHC.
description: 40 pages, 28 Figures in PDF
Μορφές του Κωνσταντίνος(19ος αι.-1913)
Creators: name: Ταχινοσλής, Νικόλαος
Publisher: name: Aristotle University of Thessaloniki
Year: 2005
Subjects: Νεοελληνικά ονόματα
New-Greek names

description: Στην παρούσα εργασία ερευνώνται οι πηγές των νεοελληνικών ονομάτων. υποστηρίζεται η άποψη ότι τα νεοελληνικά επώνυμα είναι κυρίως εξελίξεις αγαπητών βαφτιστικών του χριστιανικού εορτολογίου, οι οποίες μετά την απομάκρυνσή τους από την αρχική πηγή συνέπεσαν φωνητικά με έννοιες γνωστές του εκάστοτε γλωσσικού περιβάλλοντος και ταυτίστηκαν. Στην ίδια διαδικασία αποδίδεται και ο σχηματισμός πολλών βαφτιστικών. Με βάση τα συγκριτικά στοιχεία 223.841 ανδρικών και γυναικείων ονομάτων του 19ου κυρίως αιώνα από ολόκληρο τον ελλαδικό χώρο, παρατίθενται μορφές βαφτιστικών και επωνύμων, στις οποίες θα πρέπει πρωτίστως να αναγνωρίσουμε το όνομα Κωνσταντίνος
description: In this paper we research about the sources of the new-Greek names. It is claimed that the new-Greek last names are mainly evolved from the most favourite Christian names of the Christian church calendar, which after they were removed from their original sourch, they phonetically coincided with familiar notions of the given linguistic environment and were identified with them. In the same process we attribute the formation of many Christian names. According to the comparative types of 223.841 male and female names of the 19th century from all over Greece, we indicate forms of Christian names and last names, among which we must first of all identity the name Konstantinos
Supplementary document for Dictionary-based compressive Fourier ptychography - 5765846.pdf
Creators: name: li, xianye
name: Li, Li
name: Liu, Xiaoli
name: He, Wenqi
name: Tang, Qijian
name: Han, Sen
name: Peng, Xiang
Publisher: name: Optica Publishing Group
Year: 2022
Subjects: Uncategorized

description: Supplemental Document
Gas-solid coexistence of adhesive spheres
Creators: name: Charbonneau, P.
name: Frenkel, D.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: In this note we investigate using basic free energy considerations the location of the gas-liquid critical point with respect to solidification for narrow attractive interactions down to the Baxter limit. Possible experimental and simulation realizations leading to a stable critical point are briefly discussed.
description: 2 pages, 2 figures, submitted
Constraining Spatial Densities of Early Ice Formation in Small Dense Molecular Cores from Extinction Maps
Creators: name: Chu, Laurie E. U.
name: Hodapp, Klaus W.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Tracing dust in small dense molecular cores is a powerful tool to study the conditions required for ices to form during the pre-stellar phase. To study these environments, five molecular cores were observed: three with ongoing low-mass star formation (B59, B335, and L483) and two starless collapsing cores (L63 and L694-2). Deep images were taken in the infrared JHK bands with the United Kingdom Infrared Telescope (UKIRT) WFCAM (Wide Field Camera) instrument and IRAC channels 1 and 2 on the Spitzer Space Telescope. These five photometric bands were used to calculate extinction along the line of sight toward background stars. After smoothing the data, we produced high spatial resolution extinction maps ($\sim$13-29") . The maps were then projected into the third dimension using the AVIATOR algorithm implementing the inverse Abel transform. The volume densities of the total hydrogen were measured along lines of sight where ices (H$_2$O, CO, and CH$_3$OH) have previously been detected. We find that lines of sight with pure CH$_3$OH or a mixture of CH$_3$OH with CO have maximum volume densities above 1.0$\times$10$^5$ cm$^{-3}$. These densities are only reached within a small fraction of each of the cores ($\sim$0.3-2.1%). CH$_3$OH presence may indicate the onset of complex organic molecule formation within dense cores and thus we can constrain the region where this onset can begin. The maximum volume densities toward star-forming cores in our sample ($\sim$1.2-1.7$\times$10$^6$ cm$^{-3}$) are higher than those toward starless cores ($\sim$3.5-9.5$\times$10$^5$ cm$^{-3}$).
description: 21 pages, 4 figures, Accepted for publication by ApJ
Η διδασκαλία της νέας ελληνικής στο δημοτικό σχολείο σχολείο σήμερα: οργανωτικές και διδακτικές πρακτικές
Creators: name: Μούσιου-Μυλωνά, Ολγα
Publisher: name: Aristotle University of Thessaloniki
Year: 2005

description: Στην παρούσα εργασία περιγράφονται οι οργανωτικές και διδακτικές πρακτικές που εφαρμόζουν οι δάσκαλοι του δημοτικού σχολείου κατά την διδασκαλία της νέας ελληνικής γλώσσας. Τα δεδομένα της έρευνας προέρχονται α)από τη στατιστική ανάλυση(περιγραφική, ανάλυση παραγόντων) 1551 ερωτηματολογίων, β)απο την ανάλυση λόγου 112 κειμένων που έγραψαν δάσκαλοι και γ)από τη μελέτη 10 δίωρων διδασκαλιών γλωσσικού μαθήματος σε τάξεις του δημοτικού σχολείου(Γ'-Στ' τάξη)(μεθοδολογική τριγωνοποίηση). Από την έρευνα προκύπτει ότι κάτω από τη φαινομενική ομοιομορφία των διδακτικών τάσεων ενυπάρχει μια ποικιλία οργανωτικών και διδακτικών πρακτικών και μια δυναμική που μπορεί να λειτουργήσει στην κατεύθυνση της ανανέωσης του γλωσσικού μαθήματος. Επίσης, προκύπτουν χρήσιμα συμπεράσματα για την εκπαίδευση και την επιμόρφωση των δασκάλων σύμφωνα με τις διδακτικές τάσεις της εφαρμοσμένης γλωσσολογίας
description: This study presents the organisational and teaching practices that the teachers of primary school apply during the teaching process of modern greek. The researching data derive a)from the statisatic analysis(SPSS) of 1551 questionnaires, b)from the discourse analysis of 112 tests written by teachers and c)from the study of 19 two-hours lasting teaching classes of languages teaching in the primary school. According to the research under the phenomenical similarity of teaching trends there is a dynamic which can function in the direction of the renew of language teaching. In addition, useful conclusions are made about the teaching education and training of teachers according to the modern teaching of applied linguistics
[Elicitation session in pairs]
Creators: name: Palacio, Philip Tim
name: Cathcart, Chundra
name: Stickles, Elise
Publisher: name: California Language Archive, University of California, Berkeley
Year: 2020
Subjects: subject: cab

description: 5 WAV, 4 TextGrid, and 4 TXT files.
Garifuna subordinate clauses - purposives, 'because'/resultatives, conditionals (ems_01, ems_02).
Elicitation of causatives (cac_01, cac_02).
Additional file 1: of Screening of Streptococcus Suis serotype 2 resistance genes with GWAS and transcriptomic microarray analysis
Creators: name: Ma, Zhe
name: Zhu, Haodan
name: Su, Yiqi
name: Meng, Yu
name: Lin, Huixing
name: He, Kongwang
name: Fan, Hongjie
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology
subject: Computational Biology

description: Figure S1. Breeding scheme used to generate F2 mice. Since the fertility of C57BL/6 female mice is higher than A/J female mice, we chose C57BL/6 female mice and A/J male mice as parents to generate F1 progeny. To avoid inbreeding, F1 male mice were mated with F1 female mice from a different group to generate the F2 mice. Figure S2. Overall strategy for identifying genes associated with resistance to S. suis in swine. Flow chart of the strategy for identifying S. suis resistant genes in swine through gene expression profiling and SNP genotyping chip. Figure S3. Population structure analyzed from PCA values. Principal component values (C1, C2 and C3) were obtained through PLINK1.09 and used to correct population structure. Each point stands for a sample in the plots. Although points are concentrated in (A) and (B), and scattered in (C), none formed into several clusters in the three plots, showing the genetic background was consistent in F2 mice. Figure S4. Q-Q plot of F2 susceptible samples and F2 resistant samples. The plot showed deviation between expected P-values and observed P-values. Each point stands for a SNP. Points on the diagonal of coordinate were considered as non-influential to SS2 susceptibility, while points deviating from the diagonal might be associated with the trait. (PDF 594 kb)
Dark Energy and the Accelerating Universe
Creators: name: Frieman, Joshua
name: Turner, Michael
name: Huterer, Dragan
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The discovery ten years ago that the expansion of the Universe is accelerating put in place the last major building block of the present cosmological model, in which the Universe is composed of 4% baryons, 20% dark matter, and 76% dark energy. At the same time, it posed one of the most profound mysteries in all of science, with deep connections to both astrophysics and particle physics. Cosmic acceleration could arise from the repulsive gravity of dark energy -- for example, the quantum energy of the vacuum -- or it may signal that General Relativity breaks down on cosmological scales and must be replaced. We review the present observational evidence for cosmic acceleration and what it has revealed about dark energy, discuss the various theoretical ideas that have been proposed to explain acceleration, and describe the key observational probes that will shed light on this enigma in the coming years.
description: Invited review for Annual Reviews of Astronomy and Astrophysics; 53 pages, 18 figures
Evolution of entanglement after a local quench
Creators: name: Eisler, V.
name: Peschel, I.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study free electrons on an infinite half-filled chain, starting in the ground state with a bond defect. We find a logarithmic increase of the entanglement entropy after the defect is removed, followed by a slow relaxation towards the value of the homogeneous chain. The coefficients depend continuously on the defect strength.
description: 14 pages, 9 figures, final version
Low-luminosity galaxies in the early universe have observed sizes similar to star cluster complexes
Creators: name: Bouwens, R. J.
name: Illingworth, G. D.
name: van Dokkum, P. G.
name: Ribeiro, B.
name: Oesch, P. A.
name: Stefanon, M.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We compare the sizes and luminosities of faint $z=6$-8 galaxies magnified by the Hubble Frontier Fields (HFF) clusters with star-forming regions, as well as more evolved objects, in the nearby universe. Our high-redshift comparison sample includes 333 z=6-8 galaxies, for which size measurements were made as part of a companion study where lensing magnifications were estimated from various public models. Accurate size measurements for these sources are complicated by the lens model uncertainties, but other results and arguments suggest that faint galaxies are small, as discussed in a companion study. The measured sizes for sources in our comparison sample range from <50 pc to ~500 pc. For many of the lowest luminosity sources, extremely small sizes are inferred, reaching individual sizes as small as 10-30 pc, with several sources in the 10-15 pc range with our conservative magnification limits. The sizes and luminosities are similar to those of single star cluster complexes like 30 Doradus in the lower-redshift universe and -- in a few cases -- super star clusters. The identification of these compact, faint star-forming sources in the z~6-8 universe also allows us to set upper limits on the proto-globular cluster LF at z~6. By comparisons of the counts and sizes with recent models, we rule out (with some caveats) proto-globular cluster formation scenarios favoring substantial (xi=10) post-formation mass loss and set useful upper limits on others. Our size results suggest we may be very close to discovering a bona-fide population of forming globular clusters at high redshift.
description: 14 pages, 5 figures, AJ, in press. arXiv admin note: substantial text overlap with arXiv:1711.02090
Sammelhandschrift (Theologie)
Creators: name: Nikolaus
name: Gerson, Jean
name: Albertus
Publisher: name: [s.n.]
Year: 1453

description: Öffentliche Bibliothek der Universität Basel
description: Lateinisch
description: Aus dem Predigerkloster Basel gemäss Eintrag auf Bl. av: "Liber fratrum predicatorum Basiliensium", von dort auch das Titelschild mit der alten Signatur "R 1". Geschrieben wurde der Band von Albertus Löffler im Dominikanerinnenkloster Himmelskron in Hohenheim bei Worms, vgl. Einträge auf Bll. 66r, 75v, 129r, 212r, 248r, 284v, 329r und 354v.
description: Neidiger, Bernhard. - Selbstverständnis und Erfolgschancen der Dominikanerobservanten. In: Rottenburger Jahrbuch für Kirchengeschichte ; 17 (1998), S. 67-122, hier S. 105 Anm. 200
description: Brînzei, Monica; Schabel, Chris. - The past, present, and future of late medieval theology : the commentary on the Sentences by Nicholas of Dinkelsbühl, Vienna, ca. 1400. - In: Mediaeval commentaries on the Sentences of Peter Lombard. - Leiden : Brill, 2015. - Volume 3, S. 174-266, hier S. 264 127a
description: Verzeichnung=Description=Inventaire Dez. 2009 Titel, Jahr und Signatur nach: Schmidt, unpublizierte Beschreibung
description: Verzeichnung=Description=Inventaire Sept. 2014 HAN-Katalogisierungsregeln Minimalbescheibung nach: Schmidt, unpublizierte Beschreibung
description: Verzeichnung=Description=Inventaire November 2023 HAN-Katalogisierungsregeln Ergänzung des Minimalkatalogisats nach Autopsie und Schmidt, ungedruckte Beschreibung
description: Digitalisierung=Digitization=Numérisation Dezember 2023 TIFF
description: Erschliessungsniveau Minimalniveau
description: Die zehn nicht einzeln beschrifteten/gezählten Beilagen sind alles Lesezeichen: 8 wahrscheinlich zeitgenössische, sehr kleine Papierstreifen, gefunden auf Bll. 252, 288, 334, 338, 340, 345, 346 und 347; 1 Stück Faden, ca. 3,5 cm, gefunden auf Bl. 175; und ein moderner Papierstreifen (Stück eines Kalenderblatts), gefunden auf Bl. 43.
Conductance of a quantum point contact based on spin-density-functional theory
Creators: name: Ihnatsenka, S.
name: Zozoulenko, I. V.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We present full quantum mechanical conductance calculations of a quantum point contact (QPC) performed in the framework of the density functional theory (DFT) in the local spin-density approximation (LDA). We show that a spin-degeneracy of the conductance channels is lifted and the total conductance exhibits a broad plateau-like feature at 0.5*2e^{2}/h. The lifting of the spin-degeneracy is a generic feature of all studied QPC structures (both very short and very long ones; with the lengths in the range 40
description: 9 pages, 5 figures
All-electron full-potential implementation of real-time TDDFT in exciting
Creators: name: Pela, Ronaldo Rodrigues
name: Draxl, Claudia
Publisher: name: arXiv
Year: 2021
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Linearized augmented planewaves combined with local-orbitals (LAPW+lo) are arguably the most precise basis set to represent Kohn-Sham states. When employed within real-time time-dependent density functional theory (RT-TDDFT), they promise ultimate precision achievable for exploring the evolution of electronic excitations. In this work, we present an implementation of RT-TDDFT in the full-potential LAPW+lo code exciting. We benchmark our results against those obtained by linear-response TDDFT with exciting and by RT-TDDFT calculations with the Octopus code, finding a satisfactory level of agreement. To illustrate possible applications of our implementation, we have chosen three examples: the dynamic behavior of excitations in MoS$_2$ induced by a laser pulse, the third harmonic generation in silicon, and a pump-probe experiment in diamond.
Environmental issues in British Columbia : an historical-geographical perspective
Creators: name: Qureshi, Yasmeen
Publisher: name: University of British Columbia
Year: 2011

description: Concern for the state of the natural environment has been growing throughout the world in recent years as it becomes clear that the world is in the midst of an environmental crisis. In B.C., this has led to widespread public controversy over issues such as pollution, logging, and the preservation of wilderness areas. This thesis seeks to bring present conflicts into perspective by examining the historical roots of the various discourses on the environment in B.C. Present environmental controversies take place within a legislative framework, therefore some understanding of the historical development of that legislation and the predominant attitudes that helped shape it is necessary. The first two chapters of this thesis provide this background, focusing on forest policy and parks and wilderness policy. The third chapter addresses the outdoor recreationists, the sport hunters and anglers of B.C., who, although often contributing to the depletion of wildlife populations, also helped shape wildlife policy and worked for the preservation of wildlife habitats. With the foundations for the environmental movement set, the fourth chapter deals with the rise of the environmental movement and environmental interest groups during the 1960's and 70's. This includes a discussion of the counter culture, general social changes of the period, the rise of ecology, and protests in Strathcona Park during the late 1980's. The final chapter considers the reactions of the forest industry to the environmental movement. The forest industry has never had to be so aware of public opinion and so cautious about the image it projects as it is now. The focus is on one major company, MacMillan Bloedel, and the evolution of its public relations policies during the 1960's and 70's.
Pentacerotidae
Creators: name: Golani, Daniel
name: Fricke, Ronald
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Perciformes
Pentacerotidae

description: PENTACEROTIDAE   Histiopterus typus Temminck & Schlegel 1844
 Gulf of Suez: ¯
 Gulf of Aqaba: Israel (Baranes & Golani 1993), Jordan (Khalaf 2004).
 Red Sea main basin: Saudi Arabia (Klausewitz 1980, as Histiopterus spinifer).
 General distribution: Red Sea, Indo-West Pacific: East Africa east to Philippines.
description: Published as part of Golani, Daniel & Fricke, Ronald, 2018, Checklist of the Red Sea Fishes with delineation of the Gulf of Suez, Gulf of Aqaba, endemism and Lessepsian migrants, pp. 1-215 in Zootaxa 4509 (1) on page 112, DOI: 10.11646/zootaxa.4509.1.1, http://zenodo.org/record/2607566
Nucleon matrix elements and baryon masses in the Dirac orbital model
Creators: name: Simonov, Yu. A.
name: Trusov, M. A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Using the expansion of the baryon wave function in a series of products of single quark bispinors (Dirac orbitals), the nonsinglet axial and tensor charges of a nucleon are calculated. The leading term yields $g_A = 1.27$ in good agreement with experiment. Calculation is essentially parameter-free and depends only on the strong coupling constant value $α_s$. The importance of lower Dirac bispinor component, yielding 18% to the wave function normalization is stressed. As a check, the baryon decuplet masses in the formalism of this model are also computed using standard values of the string tension $σ$ and the strange quark mass $m_s$; the results being in a good agreement with experiment.
description: 8 pages, 2 tables; LaTeX2e
A Spatially-Resolved Survey of Distant Quasar Host Galaxies: I. Dynamics of galactic outflows
Creators: name: Vayner, Andrey
name: Wright, Shelley A.
name: Murray, Norman
name: Armus, Lee
name: Boehle, Anna
name: Cosens, Maren
name: Larkin, James E.
name: Mieda, Etsuko
name: Walth, Gregory
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present observations of ionized gas outflows in eleven z$ =1.39-2.59$ radio-loud quasar host galaxies. Data was taken with the integral field spectrograph (IFS) OSIRIS and the adaptive optics system at the W.M. Keck Observatory targeting nebular emission lines (H$β$, [OIII], H$α$, [NII] and [SII]) redshifted into the near-infrared (1-2.4 \micron). Outflows with velocities of 500 - 1700 km\,s$^{-1}$ are detected in 10 systems on scales ranging from $<1$ kpc to 10 kpc with outflow rates from 8-2400 M$_\odot$yr$^{-1}$. For five sources, the outflow momentum rates are 4-80 times $L_{AGN}$/c, consistent with outflows being driven by an energy conserving shock. The five other outflows are either driven by radiation pressure or an isothermal shock. The outflows are the dominant source of gas depletion, and we find no evidence for star formation along the outflow paths. For eight objects, the outflow paths are consistent with the orientation of the jets. Yet, given the calculated pressures, we find no evidence of the jets currently doing work on these galactic-scale ionized outflows. We find that galactic-scale feedback occurs well before galaxies establish a substantial fraction of their stellar mass, as expected from local scaling relationships.
description: 39 pages, 18 figures, 7 tables, accepted for publication in ApJ
An exquisitely deep view of quenching galaxies through the gravitational lens: Stellar population, morphology, and ionized gas
Creators: name: Man, Allison W. S.
name: Zabl, Johannes
name: Brammer, Gabriel B.
name: Richard, Johan
name: Toft, Sune
name: Stockmann, Mikkel
name: Gallazzi, Anna R.
name: Zibetti, Stefano
name: Ebeling, Harald
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: This work presents an in-depth analysis of four gravitationally lensed red galaxies at z = 1.6-3.2. The sources are magnified by factors of 2.7-30 by foreground clusters, enabling spectral and morphological measurements that are otherwise challenging. Our sample extends below the characteristic mass of the stellar mass function and is thus more representative of the quiescent galaxy population at z > 1 than previous spectroscopic studies. We analyze deep VLT/X-SHOOTER spectra and multi-band Hubble Space Telescope photometry that cover the rest-frame UV-to-optical regime. The entire sample resembles stellar disks as inferred from lensing-reconstructed images. Through stellar population synthesis analysis we infer that the targets are young (median age = 0.1-1.2 Gyr) and formed 80% of their stellar masses within 0.07-0.47 Gyr. Mg II $λλ2796,2803$ absorption is detected across the sample. Blue-shifted absorption and/or redshifted emission of Mg II is found in the two youngest sources, indicative of a galactic-scale outflow of warm ($T\sim10^{4}$ K) gas. The [O III] $\lambda5007$ luminosity is higher for the two young sources (median age less than 0.4 Gyr) than the two older ones, perhaps suggesting a decline in nuclear activity as quenching proceeds. Despite high-velocity ($v\approx1500$ km s$^{-1}$) galactic-scale outflows seen in the most recently quenched galaxies, warm gas is still present to some extent long after quenching. Altogether our results indicate that star formation quenching at high redshift must have been a rapid process (< 1 Gyr) that does not synchronize with bulge formation or complete gas removal. Substantial bulge growth is required if they are to evolve into the metal-rich cores of present-day slow-rotators.
description: Accepted for publication in the Astrophysical Journal. 37 pages, 20 figures, 10 tables
Half-life and spin of 60Mn^g
Creators: name: Liddick, S. N.
name: Mantica, P. F.
name: Brown, B. A.
name: Carpenter, M. P.
name: Davies, A. D.
name: Horoi, M.
name: Janssens, R. V. F.
name: Morton, A. C.
name: Mueller, W. F.
name: Pavan, J.
name: Schatz, H.
name: Stolz, A.
name: Tabor, S. L.
name: Tomlin, B. E.
name: Wiedeking, M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: A value of 0.28 +/- 0.02 s has been deduced for the half-life of the ground state of 60Mn, in sharp contrast to the previously adopted value of 51 +/- 6 s. Access to the low-spin 60Mn ground state was accomplished via beta decay of the 0+ 60Cr parent nuclide. New, low-energy states in 60Mn have been identified from beta-delayed gamma-ray spectroscopy. The new, shorter half-life of 60Mn^g is not suggestive of isospin forbidden beta decay, and new spin and parity assignments of 1+ and 4+ have been adopted for the ground and isomeric beta-decaying states, respectively, of 60Mn.
description: 13 pages, 5 figures, Accepted for publication in Phys. Rev. C
TESS Data for Asteroseismology: Photometry
Creators: name: Handberg, Rasmus
name: Lund, Mikkel N.
name: White, Timothy R.
name: Hall, Oliver J.
name: Buzasi, Derek L.
name: Pope, Benjamin J. S.
name: Hansen, Jonas S.
name: von Essen, Carolina
name: Carboneau, Lindsey
name: Huber, Daniel
name: Vanderspek, Roland K.
name: Fausnaug, Michael M.
name: Tenenbaum, Peter
name: Jenkins, Jon M.
name: Collaboration, the T'DA
Publisher: name: arXiv
Year: 2021
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Over the last two decades, asteroseismology has increasingly proven to be the observational tool of choice for the study of stellar physics, aided by the high quality of data available from space-based missions such as CoRoT, Kepler, K2 and TESS. TESS in particular will produce more than an order of magnitude more such data than has ever been available before. While the standard TESS mission products include light curves from 120-sec observations suitable for both exoplanet and asteroseismic studies, they do not include light curves for the vastly larger number of targets observed by the mission at a longer 1800-sec cadence in Full Frame Images (FFIs). To address this lack, the TESS Data for Asteroseismology (T'DA) group under the TESS Asteroseismic Science Consortium (TASC), has constructed an open-source pipeline focused on producing light curves for all stars observed by TESS at all cadences, currently including stars down to a TESS magnitude of 15. The pipeline includes target identification, background estimation and removal, correction of FFI timestamps, and a range of potential photometric extraction methodologies, though aperture photometry is currently the default approach. For the brightest targets, we transparently apply a halo photometry algorithm to construct a calibrated light curve from unsaturated pixels in the image. In this paper, we describe in detail the algorithms, functionality, and products of this pipeline, and summarize the noise metrics for the light curves. Companion papers will address the removal of systematic noise sources from our light curves, and a stellar variability classification from these.
description: 27 pages, 14 figures, Accepted for publication in The Astronomical Journal
Cichlidae
Creators: name: Golani, Daniel
name: Fricke, Ronald
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Perciformes
Cichlidae

description: CICHLIDAE   Coptodon zillii (Gervais 1848)
 Gulf of Suez: Egypt (Bayoumi, 1969).
 Gulf of Aqaba: ¯
Red Sea main: ¯
 General distribution: Jordan River system and rivers of North and West Africa; introduced elsewhere.
 Oreochromis mossambicus (Peters 1852)
 Gulf of Suez: ¯
 Gulf of Aqaba: Israel (Golani & Lerner 2007).
 Red Sea main basin: ¯
Remark. Originally distributed in freshwater and transitional water of southeastern Africa; introduced into marine water of the Red Sea.
 General distribution: Rivers of southeastern Africa; introduced elsewhere.
description: Published as part of Golani, Daniel & Fricke, Ronald, 2018, Checklist of the Red Sea Fishes with delineation of the Gulf of Suez, Gulf of Aqaba, endemism and Lessepsian migrants, pp. 1-215 in Zootaxa 4509 (1) on page 112, DOI: 10.11646/zootaxa.4509.1.1, http://zenodo.org/record/2607566
Exascale Laser Plasma Physics - From Computational Speed to Predictions
Creators: name: Huebl, Axel
name: Widera, René
name: Garten, Marco
name: Pausch, Richard
name: Steiniger, Klaus
name: Bastrakov, Sergei
name: Meyer, Felix
name: Bastrakova, Ksenia
name: Debus, Alexander
name: Ehrig, Simeon
name: Werner, Matthias
name: Worpitz, Benjamin
name: Matthes, Alexander
name: Rudat, Sophie
name: Starke, Sebastian
name: Kluge, Thomas
name: Cowan, Thomas E.
name: Schramm, Ulrich
name: Bussmann, Michael
Publisher: name: Zenodo
Year: 2019
Subjects: PIC
HPC
Plasma
Laser
Simulation
BigData
Open Science

description: Invited presentation given by Axel Huebl (HZDR, Germany) at the EPS 2019 conference in Milano (Italy) on July 11th, 2019.
description: This project has been enabled by many people in open-source and open-science communities. Great thanks to the communities and developers of: PIConGPU, PMacc, Alpaka, ROOT/Cling, Jupyter, the SciPy ecosystem, ADIOS, HDF5, Boost, CMake, openPMD, Spack, ...This research used resources of the Oak Ridge Leadership Computing Facility located in the Oak Ridge National Laboratory, which is supported by the Office of Science of the Department of Energy under Contract DE-AC05-00OR22725. This project received funding within the MEPHISTO project (BMBF-Förderkennzeichen 01IH16006C). This project has received funding from the European Unions Horizon 2020 research and innovation programme under grant agreement No 654220.
description: {"references": ["Huebl, Axel (2019). PIConGPU: Predictive Simulations of Laser-Particle Accelerators with Manycore Hardware. DOI:10.5281/zenodo.3266820", "Bussmann, Michael and Burau, Heiko and Cowan, Thomas E. and Debus, Alexander and Huebl, Aaxel and Juckeland, Guido and Kluge, Thomas and Nagel, Wolfgang E. and Pausch, Richard and Schmitt, Felix and Schramm, Ulrich and Schuchart, Joseph and Widera, Ren\u00e9 (2013). Radiative Signatures of the Relativistic Kelvin-Helmholtz Instability. DOI:10.1145/2503210.2504564"]}
The role of SPICA-like missions and the Origins Space Telescope in the quest for heavily obscured AGN and synergies with Athena
Creators: name: Barchiesi, L.
name: Pozzi, F.
name: Vignali, C.
name: Carrera, F. J.
name: Vito, F.
name: Calura, F.
name: Bisigello, L.
name: Lanzuisi, G.
name: Gruppioni, C.
name: Lusso, E.
name: Delvecchio, I.
name: Negrello, M.
name: Cooray, A.
name: Feltre, A.
name: Fernández-Ontiveros, J. A.
name: Gallerani, S.
name: Kaneda, H.
name: Oyabu, S.
name: Pereira-Santaella, M.
name: Piconcelli, E.
name: Ricci, C.
name: Rodighiero, G.
name: Spinoglio, L.
name: Tombesi, F.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In the BH-galaxy co-evolution framework, most of the star-formation (SF) and the black hole (BH) accretion is expected to take place in highly obscured conditions. Thus, obscured AGN are difficult to identify in optical or X-ray bands, but shine bright in the IR. Moreover, X-ray background (XRB) synthesis models predict that a large fraction of the yet-unresolved XRB is due to the most obscured (Compton thick, CT) of these AGN. In this work, we investigate the synergies between putative IR missions (using SPICA, proposed for ESA/M5 but withdrawn in October 2020, and Origins Space Telescope, OST, as `templates') and the X-ray mission Athena, which should fly in early 2030s, in detecting and characterizing AGN, with a particular focus on the most obscured ones. Using an XRB synthesis model, we estimated the number of AGN and the number of those which will be detected in the X-rays. For each AGN we associated an optical-to-FIR SED from observed AGN with both X-ray data and SED decomposition, and used these SEDs to check if the AGN will be detected by SPICA-like or OST at IR wavelengths. We expect that, with the deepest Athena and SPICA-like (or OST) surveys, we will be able to detect in the IR more than $90\,\%$ of all the AGN (down to L$_{2-10\text{keV}} \sim 10^{42}\,$erg/s and up to $z \sim 10$) predicted by XRB synthesis modeling, and we will detect at least half of them in the X-rays. Athena will be extremely powerful in detecting and discerning moderate- and high-luminosity AGN. We find that the most obscured and elusive CT-AGN will be exquisitely sampled by SPICA-like mission or OST and that Athena will allow a fine characterization of the most-luminous ones. This will provide a significant step forward in the process of placing stronger constraints on the yet-unresolved XRB and investigating the BH accretion rate evolution up to very high redshift ($z \ge 4$).
description: Accepted for publication in PASA
The Victorian ear: gendered acoustics in science and poetry
Creators: name: Παπαλεωνίδα, Παρασκευή Λ.
Publisher: name: Aristotle University of Thessaloniki
Year: 2005
Subjects: Βικτωριανές ποιήτριες
Ακουστική επιστήμη
Φωνογράφος
Σειρήνες
Victorian women poets
Phonograph
19th century physiological acoustics
Siren

description: Στόχος της διατριβής είναι να παρέχει ένα πολιτισμικό πλαίσιο για το φαινόμενο του ομιλώντα ακροατή στη Βικτωριανή γυναικεία ποίηση. Αντιμετωπίζοντας την ακοή ως κατασκεύασμα του ποιητικού νεωτερισμού και του επιστημονικού λόγου, η διατριβή ακολουθεί μια διεπιστημονική μεθοδολογία, δίνοντας έμφαση στην φυσική, την φυσιολογία και την τεχνολογία ως τους χώρους όπου αναδείχθηκε ο προβληματισμός περί ακοής κατά το 2ο μισό του 19 αιώνα. Το συμπέρασμα είναι ότι το φαινόμενο του ακροατή επηρεάστηκε από την ακουστική επιστήμη. Ιδέες που λειτουργούν παράλληλα στην επιστήμη και ποίηση της εποχής 1860-1890(όπως η συμπαθητική δόνηση, η οπτική απεικόνιση του ήχου, ο αυτοματισμός στην αίσθηση της ακοής, η σειρήνα) αναλύονται στο έργο φυσικών όπως ο John Tyndall καιφυσιολόγων όπως ο William Carpenter και ποιητριών όπως οι Augusta Webster, Christina Rossetti, Mary Coleridge καθώς και στους δραματικούς μονολόγους των Jean Ingelaw, Amy Lery, Violet Fane, Mathilde Blind. Ο επιστημονικός λόγος σκιαγραφεί το αυτί ως αναπαραγωγικό και ταυτόχρονα αυτόφωνο όργανο που επεξεργάζεται τον ήχο. Στην γυναικεία ποίηση η επιστημονική σκιαγράφηση της ακοής αλληλεπιδρά με το ιδεολογικό κατασκεύασμα του θηλυκού αυτιού, και η μεταφορά της ακουστικής σύλληψης μεταβάλλεται σε μοτίβο έκφρασης
description: Women poets' introduction of an autonomous speaking auditor in dramatifc monologue, as well lyric and narrative poetry, was informed by developments in acoustic science in the period between the 1860s-1890s. An interdisciplinary approach focusing on physics and physiological psychology can help elucidate the importance of aurality in late-Victorian literature : the dramaticity of women's poetry. I believe the listening self manifest in poetic innovation is saturated by the scintific delineation of audition. I trace acoustic metaphors and motifs, shared by science and poetry, such as sympathetic vibration, the siren, the visual representation of sound, automatism in aural perception, in the work of scientists like John Tyndall and William Carpenter and poets such as Augusta Webster, Christina Rossetti and Mary Coleridge and the dramatic monologues of Jean Ingelaw, Amy Lery, Violet Fane(Mary M. Lamb) and Mathilde Blind. Having become in scintific discourse something other than the receptor of voice, the ear oscillated between being a reproducing and an autophonous instrument that processed sound_women poets allowed the implications of the scientific construction of audition to interact with the ideological construct of the receptive feminine ear, transforming the metaphor of the feminine ear into a trope of receptive expression
Deep Autoencoder-based Fuzzy C-Means for Topic Detection
Creators: name: Murfi, Hendri
name: Rosaline, Natasha
name: Hariadi, Nora
Publisher: name: arXiv
Year: 2021
Subjects: subject: Information Retrieval (cs.IR)
subject: Computation and Language (cs.CL)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: Topic detection is a process for determining topics from a collection of textual data. One of the topic detection methods is a clustering-based method, which assumes that the centroids are topics. The clustering method has the advantage that it can process data with negative representations. Therefore, the clustering method allows a combination with a broader representation learning method. In this paper, we adopt deep learning for topic detection by using a deep autoencoder and fuzzy c-means called deep autoencoder-based fuzzy c-means (DFCM). The encoder of the autoencoder performs a lower-dimensional representation learning. Fuzzy c-means groups the lower-dimensional representation to identify the centroids. The autoencoder's decoder transforms back the centroids into the original representation to be interpreted as the topics. Our simulation shows that DFCM improves the coherence score of eigenspace-based fuzzy c-means (EFCM) and is comparable to the leading standard methods, i.e., nonnegative matrix factorization (NMF) or latent Dirichlet allocation (LDA).
description: 18 pages
Short wavelength electromagnetic propagation in magnetized quantum plasmas
Creators: name: Lundin, J.
name: Zamanian, J.
name: Marklund, M.
name: Brodin, G.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The quantum electrodynamical (QED) short wavelength correction on plasma wave propagation for a non-relativistic quantum plasma is investigated. A general dispersion relation for a thermal multi-component quantum plasma is derived. It is found that the classical dispersion relation for any wave mode can be modified to include quantum and short wavelength QED effects by simple substitutions of the thermal velocity and the plasma frequency. Furthermore, the dispersion relation has been modified to include QED effects of strong magnetic fields. It is found that strong magnetic fields together with the short wavelength QED correction will induce dispersion both in vacuum and in otherwise non-dispersive plasma modes. Applications to laboratory and astrophysical systems are discussed.
description: 13 pages, 2 figures
Ανάπτυξη και επικύρωση καταστρεπτικών και μη καταστρεπτικών μεθόδων πολυστοιχειακής ανάλυσης κεραμικών με τις τεχνικές της φασματοσκοπικής ατομικής εκπομπής επαγωγικά συζευγμένου πλάσματος(ICP-AES) και της φασματοσκοπίας φθορισμού ακτίνων X(μ-XRF): εφαρμογή στην κεραμική των αρχαίων Αβδήρων
Creators: name: Παπαδοπούλου, Δέσποινα Ν.
Publisher: name: Aristotle University of Thessaloniki
Year: 2005
Subjects: Καταστρεπτική ανάλυση
Μη καταστρεπτική ανάλυση
Μικροφασματοσκοπία φθορισμού ακτίνων Χ
Destructive analysis
Non-destructive analysis
Micro fluorescwncw X-ray spectroscopy

description: Αντικείμενο της παρούσας διδακτορικής διατριβής είναι η μελέτη της κεραμικής των αρχαίων Αβδήρων με διάφορες φασματοσκοπικές μεθόδους ανάλυσης, όπως η φασματοσκοπία ατομικής εκπομπής με συζευγμένο πλάσμα(ICP-XRF), καθώς και με διάφορες άλλες φυσικοχημικές δοκιμές όπως η μέτρηση του πορώδους, της σκληρότητας και του χρώματος. Οι στόχοι της έρευνας περιελάμβαναν τη βελτιστοποίηση ενός πρωτοκόλλου προετοιμασίας των αρχαίων κεραμικών που πρόκειται να αναλυθούν με τη φασματοσκοπία ατομικής εκπομπής με συζευγμένο πλάσμα, τη βελτιστοποίηση της μικρο-φασματοσκοπίας φθορισμού ακτίνων Χ με σκοπό την ποιοτική και ποσοτική ανάλυση των αρχαίων κεραμικών, τη σύγκριση των δύο παραπάνω ενόργανων μεθόδων ανάλυσης, το χαρακτηριστικό ενός πληθυσμού από 115 κεραμικά ως προς τη στοιχειακή σύστασή τους και τη στατιστική επεξεργασία των αναλυτικών δεδομένων με τις μεθόδους της χημειομετρίας(ανάλυση κατά ομάδες, ανάλυση κύριων συνιστωσών)
description: The main subject of the scientific research is the study of the ancient ceramics from Abdera with different spectroscopy methods of analysis such as the Ibductively Coupled Plasma Atomic Emission Spectroscopy(ICP_AES), the Micro X-ray. Fluorescence Spectroscopy(μ-XRF) as well as with other physicochemical techniques as the porosity, hardness and color measurements. The research objectives include the introduction of a preparation procedure that can be successfully applied to the analysis of ancient ceramics with the inductively coupled plasma atomic emission spectroscopy the improvement of the micro X-ray fluorescence spectroscopy for the qualitative and quantitative analysis of ancient ceramics, the comparison of the above two analytical methods, the elemental and shysicochemical characterisation of a group of 115 ancient ceramic sherds and the statistical processing of the analytical data by chemometrical methods(cluster analysis, principal component analysis)
Broken axisymmetry phase of a spin-1 ferromagnetic Bose-Einstein condensate
Creators: name: Murata, Keiji
name: Saito, Hiroki
name: Ueda, Masahito
Publisher: name: arXiv
Year: 2006
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: A spin-1 ferromagnetic Bose-Einstein condensate subject to a certain magnetic field exhibits a broken-axisymmetry phase in which the magnetization tilts against the applied magnetic field due to the competition between ferromagnetism and linear and quadratic Zeeman effects. The Bogoliubov analysis shows that in this phase two Goldstone modes associated with U(1) and SO(2) symmetry breakings exist, in which phonons and magnons are coupled to restore the two broken symmetries.
description: 11 pages, 6 figures
Real-Time Feedback Control of Charge Sensing for Quantum Dot Qubits
Creators: name: Nakajima, Takashi
name: Kojima, Yohei
name: Uehara, Yoshihiro
name: Noiri, Akito
name: Takeda, Kenta
name: Kobayashi, Takashi
name: Tarucha, Seigo
Publisher: name: arXiv
Year: 2021
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Measurement of charge configurations in few-electron quantum dots is a vital technique for spin-based quantum information processing. While fast and high-fidelity measurement is possible by using proximal quantum dot charge sensors, their operating range is limited and prone to electrical disturbances. Here we demonstrate realtime operation of a charge sensor in a feedback loop to maintain its sensitivity suitable for fast charge sensing in a Si/SiGe double quantum dot. Disturbances to the charge sensitivity, due to variation of gate voltages for operating the quantum dot and $1/f$ charge fluctuation, are compensated by a digital PID controller with the bandwidth of $\approx 100\,{\rm kHz}$. The rapid automated tuning of a charge sensor enables unobstructed charge stability diagram measurement facilitating realtime quantum dot tuning and submicrosecond single-shot spin readout without compromising the performance of a charge sensor in time-consuming experiments for quantum information processing.
description: 6 pages, 4 figures
Weak localization correction to the density of transmission eigenvalues in the presence of magnetic field and spin-orbit coupling for a chaotic quantum dot
Creators: name: Béri, Benjamin
name: Cserti, József
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We calculated the weak localization correction to the density of the transmission eigenvalues in the case of chaotic quantum dots in the framework of Random Matrix Theory including the parametric dependence on the magnetic field and spin-orbit coupling. The result is interpreted in terms of spin singlet and triplet Cooperon modes of conventional diagrammatic perturbation theory. As simple applications, we obtained the weak localization correction to the conductance, the shot noise power and the third cumulant of the distribution of the transmitted charge.
description: 7 pages, 2 figures
Supplementary Figures and Tables from Genotype by environment interactions in the coral bleaching response
Creators: name: Drury, Crawford
name: Lirman, Diego
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: 60408 Genomics

description: Climate-driven reef decline has prompted the development of next-generation coral conservation strategies, many of which hinge on the movement of adaptive variation across genetic and environmental gradients. This process is limited by our understanding of how genetic and genotypic drivers of coral bleaching will manifest in different environmental conditions. We reciprocally transplanted 10 genotypes of Acropora cervicornis across eight sites along a 60 km span of the Florida Reef Tract and documented significant genotype × environment interactions in bleaching response during the severe 2015 bleaching event. Performance relative to site mean was significantly different between genotypes and can be mostly explained by ensemble models of correlations with genetic markers. The high explanatory power was driven by significant enrichment of loci associated DNA repair, cell signalling and apoptosis. No genotypes performed above (or below) bleaching average at all sites, so genomic predictors can provide practitioners with ‘confidence intervals' about the chance of success in novel habitats. These data have important implications for assisted gene flow and managed relocation and their integration with traditional active restoration.