cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
Creators: name: Dainotti, M. G.
name: Lenart, A. Ł.
name: Chraya, A.
name: Sarracino, G.
name: Nagataki, S.
name: Fraija, N.
name: Capozziello, S.
name: Bogdan, M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Cosmological models and their corresponding parameters are widely debated because of the current discrepancy between the results of the Hubble constant, $H_{0}$, obtained by SNe Ia, and the Planck data from the Cosmic Microwave Background Radiation. Thus, considering high redshift probes like Gamma-Ray Bursts (GRBs) is a necessary step. However, using GRB correlations between their physical features to infer cosmological parameters is difficult because GRB luminosities span several orders of magnitude. In our work, we use a 3-dimensional relation between the peak prompt luminosity, the rest-frame time at the end of the X-ray plateau, and its corresponding luminosity in X-rays: the so-called 3D Dainotti fundamental plane relation. We correct this relation by considering the selection and evolutionary effects with a reliable statistical method, obtaining a lower central value for the intrinsic scatter, $σ_{int}=0.18 \pm 0.07$ (47.1 \%) compared to previous results, when we adopt a particular set of GRBs with well-defined morphological features, called the platinum sample. We have used the GRB fundamental plane relation alone with both Gaussian and uniform priors on cosmological parameters and in combination with SNe Ia and BAO measurements to infer cosmological parameters like $H_{0}$, the matter density in the universe ($Ω_{M}$), and the dark energy parameter $w$ for a $w$CDM model. Our results are consistent with the parameters given by the $Λ$CDM model but with the advantage of using cosmological probes detected up to $z=5$, much larger than the one observed for the furthest SNe Ia.
description: 43 pages, 29 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society
Sciurus nayaritensis J. A. Allen 1890
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Sciurus
Sciurus nayaritensis

description: Sciurus nayaritensis J. A. Allen, 1890. Bull. Am. Mus. Nat. Hist., 2:7, footnote. TYPE LOCALITY: Mexico, Zacatecas, Sierra Valparaiso. DISTRIBUTION: Jalisco (Mexico) north to S.E. Arizona (U.S.A.). COMMENT: Subgenus Sciurus; see Hall, 1981:431. Includes chiricahuae and apache; see Lee and Hoffmeister, 1963, Proc. Biol. Soc. Wash., 76:188- 189, and Hall, 1981:431. ISIS NUMBER: 5301410002030014001 as S. nayaritensis. 5301410002030004001 as S. apache. 5301410002030008001 as S. chiricahuae.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 364, DOI: 10.5281/zenodo.7353023
description: {"references": ["Hall, E. R. 1981. The mammals of North America. Second ed. John Wiley and Sons, New York, 1: 1 - 600 + 90, 2: 601 - 1181 + 90."]}
Magnetic induction dependence of the dispersion of magnetoplasmon in a two-dimensional electron gas with finite layer thickness
Creators: name: Uchida, T.
name: Hiraiwa, N.
name: Yamada, K.
name: Fujita, M.
name: Toyoda, T.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Magnetic induction dependence of the dispersion of longitudinal magnetoplasmon in a two-dimensional electron gas with finite layer thickness under a static uniform magnetic field normal to the layer plane is calculated using the self-consistent linear response approximation. Two longitudinal magnetoplasmon modes are obtained. The calculated dispersion agrees with the experiment by Batke {\it et al.} [Phys. Rev. B {\bf 34}, 6951 (1986)].
[Fünfteilige Sammelhandschrift]. (1r) Bibelsummarium. (28r) [Notate zu Texten und Büchern]. (29r) [Quaestiones in Petri Lombardi sententiarum libros III-IV]. (40r) [Johannes Calderinus: Tabula auctoritatum et sententiarum bibliae cum concordantiis decretorum et decretalium]. (160r) [Michael de Bononia: Tabula de quattuor libris sententiarum]. (242r) [Heinrich Lur: De modo audiendi confessiones]. (266r) [Sermones quadragesimales S. Augustini, Caesarii aliorumque]. (282v) [Bonaventura: Soliloquium]. (311r) [Sermones quadragesimales; [1444-1461]
Creators: name: Johannes Calderinus
name: Michael Aiguani De Bononia
name: Lur, Henricus
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2017

description: Entstehungsort: [Teil I u. III Österreich; Teil II Westdeutschland; Teil IV-V Süddeutschland]. - Entstehungszeit: [1444-1461]
Semi-Supervised Classification and Clustering Analysis for Variable Stars
Creators: name: Pantoja, R.
name: Catelan, M.
name: Pichara, K.
name: Protopapas, P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The immense amount of time series data produced by astronomical surveys has called for the use of machine learning algorithms to discover and classify several million celestial sources. In the case of variable stars, supervised learning approaches have become commonplace. However, this needs a considerable collection of expert-labeled light curves to achieve adequate performance, which is costly to construct. To solve this problem, we introduce two approaches. First, a semi-supervised hierarchical method, which requires substantially less trained data than supervised methods. Second, a clustering analysis procedure that finds groups that may correspond to classes or sub-classes of variable stars. Both methods are primarily supported by dimensionality reduction of the data for visualization and to avoid the curse of dimensionality. We tested our methods with catalogs collected from OGLE, CSS, and Gaia surveys. The semi-supervised method reaches a performance of around 90\% for all of our three selected catalogs of variable stars using only $5\%$ of the data in the training. This method is suitable for classifying the main classes of variable stars when there is only a small amount of training data. Our clustering analysis confirms that most of the clusters found have a purity over 90\% with respect to classes and 80\% with respect to sub-classes, suggesting that this type of analysis can be used in large-scale variability surveys as an initial step to identify which classes or sub-classes of variable stars are present in the data and/or to build training sets, among many other possible applications.
description: 23 pages, 21 figures, 4 tables, submitted to MNRAS
Surface state evolution induced by magnetic order in axion insulator candidate EuIn2As2
Creators: name: Gong, Mingda
name: Sar, Divyanshi
name: Friedman, Joel
name: Kaczorowski, Dariusz
name: Razek, S. Abdel
name: Lee, Wei-Cheng
name: Aynajian, Pegor
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Gapping of Dirac surface states through time reversal symmetry breaking may realize the axion insulator state in condensed matter. Despite tremendous efforts, only a few material systems fall in this category of intrinsic magnetic topological insulators (TI). Recent theoretical calculations proposed the antiferromagnetic EuIn$_2$As$_2$ to be a topologically non-trivial magnetic insulator with gapped surface states. Here we use scanning tunneling microscopy and spectroscopy (STM/STS) complemented with density-functional theory (DFT) calculations and modelling to probe the surface electronic states in EuIn$_2$As$_2$. We find a spin-orbit induced bulk gap of ~120 meV located only a few meV above the Fermi energy, within which topological surface states reside. Temperature dependent measurements provide evidence of the partial gapping (~40 meV) of the surface states at low temperatures below the AFM order, which decreases with increasing temperature but remains finite above $T_N$
description: 8 pages, 8 figures, to be published in Physical Review B
Observing a topological phase transition with deep neural networks from experimental images of ultracold atoms
Creators: name: Zhao, Entong
name: Mak, Ting Hin
name: He, Chengdong
name: Ren, Zejian
name: Pak, Ka Kwan
name: Liu, Yu-Jun
name: Jo, Gyu-Boong
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Although classifying topological quantum phases have attracted great interests, the absence of local order parameter generically makes it challenging to detect a topological phase transition from experimental data. Recent advances in machine learning algorithms enable physicists to analyze experimental data with unprecedented high sensitivities, and identify quantum phases even in the presence of unavoidable noises. Here, we report a successful identification of topological phase transitions using a deep convolutional neural network trained with low signal-to-noise-ratio (SNR) experimental data obtained in a symmetry-protected topological system of spin-orbit-coupled fermions. We apply the trained network to unseen data to map out a whole phase diagram, which predicts the positions of the two topological phase transitions that are consistent with the results obtained by using the conventional method on higher SNR data. By visualizing the filters and post-convolutional results of the convolutional layer, we further find that the CNN uses the same information to make the classification in the system as the conventional analysis, namely spin imbalance, but with an advantage concerning SNR. Our work highlights the potential of machine learning techniques to be used in various quantum systems.
description: 7 pages, 5 figures
title: Almanach nova; [1500-1525]
title: [bei dem Wiegendruck mit vielen handschriftlichen, chronikartigen Einträgen handelt es sich um den Kalender mit den Tagbucheintragungen des Regensburger Weihbischofs Peter Krafft (1470-1530). Die Inkunabel wurde im Januar 1921 in den Handschriftenbestand umgestellt]
titleType: Subtitle
Creators: name: Krafft, Peter
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2015

description: Entstehungsort:[Regensburg]. - Entstehungszeit: erstes Viertel des 16. Jh.
Reconciling 56Ni Production in Type Ia Supernovae with Double Degenerate Scenarios
Creators: name: Piro, Anthony L.
name: Thompson, Todd A.
name: Kochanek, Christopher S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Binary white dwarf (WD) coalescences driven by gravitational waves or collisions in triple systems are potential progenitors of Type Ia supernovae (SNe Ia). We combine the distribution of 56Ni inferred from observations of SNe Ia with the results of both sub-Chandrasekhar detonation models and direct collision calculations to estimate what mass WDs should be exploding in each scenario to reproduce the observations. These WD mass distributions are then compared with the observed Galactic WD mass distribution and Monte Carlo simulations of WD-WD binary populations. For collisions, we find that the average mass of the individual components of the WD-WD binary must be peaked at ~0.75Msun, significantly higher than the average WD mass in binaries or in the field of ~0.55-0.60Msun. Thus, if collisions produce a large fraction of SNe Ia, then a mechanism must exist that favors large mass WDs. On the other hand, in an old stellar population, collisions would naturally result in a class of low luminosity SNe Ia, and we suggest these may be related to 1991bg-like events. For sub-Chandrasekhar detonations, we find that the average mass of the exploding WDs must be peaked at ~1.1Msun. This is interestingly similar to the average sum of the masses in WD-WD binaries, but it is not clear (and should be further explored) whether double degenerate mergers would be sufficiently efficient at synthesizing 56Ni to match the observed yields. If not, then actual ~1.1Msun WDs would be needed for sub-Chandrasekhar detonations. Since such high mass WDs are produced relatively quickly in comparison to the age of the environments where SNe Ia are found, this would require either accretion onto lower mass WDs prior to ignition or a long timescale between formation of the ~1.1Msun WD and ignition (such as set by gravitational wave emission or binary interactions).
description: 8 pages, 5 figures, submitted for publication in The Astrophysical Journal. Revised manuscript includes an updated 56Ni distribution, a new emphasis on subluminous 1991bg-like SNe Ia, and a different approach to binary population models. Updated acknowledgements
Logik u[nd] Enzcyclopaedie der Philosophie; 1862-1863
Creators: name: Prantl, Carl ¬von
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Entstehungsort: München. - Entstehungszeit: 1862/63 (dat. 1r)
Το έγκλημα της παρακώλυσης συναγωνισμού (άρθρο 395 ΠΚ)
Creators: name: Δωρής, Παναγιώτης Σωκράτη
Publisher: name: Aristotle University of Thessaloniki
Year: 2024
Subjects: Παρακώλυση συναγωνισμού
Δημόσιες Συμβάσεις
Καρτέλ
Οbstructing competition
Public contracts
Cartel

description: Σκοπός της παρούσας εργασίας είναι η εις βάθος ανάλυση του άρθρου 395 ΠΚ, του εγκλήματος της παρακώλυσης συναγωνισμού, με ιδιαίτερη προσοχή στην παράγραφο 1, και υπό το πρίσμα των δικαιϊκών διατάξεων που το σχηματίζουν, ήτοι των εμπορικών, των διοικητικών και των ουσιαστικών ποινικών. Το έγκλημα της παρακώλυσης συναγωνισμού κατά τη διενέργεια δημοσίων συμβάσεων αποτελεί τρανό παράδειγμα της σύγχρονης οικονομικής εγκληματικότητας και ως μέρος αυτής είναι σε μεγάλο βαθμό δυσαπόδεικτο, γεγονός που εμποδίζει κάθε προσπάθεια αντεγκληματικής πολιτικής. Η Ευρωπαϊκή Ένωση έχει καταβάλλει προσπάθεια στον μετριασμό της δημιουργίας καρτελικών συμπράξεων στις δημόσιες συμβάσεις, όπως αποδεικνύεται και από τις κατά καιρούς αποφάσεις της Επιτροπής. Αποτελεί, επιπρόσθετα, ένα έγκλημα που δύναται να διαπραχθεί από ιδιώτες, αλλά και αξιωματούχους επιχειρήσεων, ενώ ο τόπος γένεσης των αποτελεσμάτων διαδραματίζει σημαίνοντα ρόλο. Ακόμη, στην παρούσα μελέτη διενεργήθηκε, μεταξύ άλλων, εκτενής παρουσίαση των επιχειρημάτων περί συν-εφαρμογής ή μη της απάτης. Στο τελευταίο μέρος της παρούσας εξετάζεται η 2η παράγραφος του οικείου άρθρου, σχετικά με την παρακώλυση των δημόσιων πλειστηριασμών και τη σχέση του άρθρου αυτού με το παλαιό 396 ΠΚ, αλλά και με το έγκλημα της παρ. 1.
description: The purpose of this paper is the in-depth analysis of article 395 of the Greek Penal Code, the crime of obstructing competition, with particular attention to paragraph 1, and in the light of the legal provisions that form it, namely the commercial, administrative and substantive criminal provisions. The crime of obstructing competition in the award of public contracts is a striking example of modern economic crime and, as part of it, is largely unproven, which hinders any attempt at counter-criminal policy. The European Union has made efforts to mitigate the creation of cartels in public procurement, as demonstrated by the Commission's decisions from time to time. It is, moreover, a crime that can be committed by private individuals, but also by company officials, and the place where the results are generated plays an important role. Furthermore, this study has, inter alia, made an extensive presentation of the arguments concerning the co-existence or otherwise of fraud. In the last part of this paper, the second paragraph of the relevant article is examined, concerning the obstruction of public auctions and the relationship of this article with the old 396 Greek Penal Code, but also with the crime of the first paragraph.
description: Τμήμα Νομικής, Συνεργαζόμενα Τμήματα Νομικής (Δημοκρίτειο Πανεπιστήμιο Θράκης)
Sciurus niger Linnaeus 1758
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Sciurus
Sciurus niger

description: Sciurus niger Linnaeus, 1758. Syst. Nat., 10th ed., 1:64. TYPE LOCALITY: U.S.A., S. South Carolina (probably). DISTRIBUTION: Texas (U.S.A.) and adjacent Mexico, north to Manitoba (Canada) east to the Atlantic Coast. COMMENT: Subgenus Sciurus; see Hall, 1981:427. PROTECTED STATUS: U.S. ESA - Endangered as S. n. cinereus subspecies only. ISIS NUMBER: 5301410002030016001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 365, DOI: 10.5281/zenodo.7353023
description: {"references": ["Hall, E. R. 1981. The mammals of North America. Second ed. John Wiley and Sons, New York, 1: 1 - 600 + 90, 2: 601 - 1181 + 90."]}
The VMC Survey - X. Cepheids, RR Lyrae stars and binaries as probes of the Magellanic System's structure
Creators: name: Moretti, M. I.
name: Clementini, G.
name: Muraveva, T.
name: Ripepi, V.
name: Marquette, J. B.
name: Cioni, M. -R. L.
name: Marconi, M.
name: Girardi, L.
name: Rubele, S.
name: Tisserand, P.
name: de Grijs, R.
name: Groenewegen, M. A. T.
name: Guandalini, R.
name: Ivanov, V. D.
name: van Loon, J. Th.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The VMC survey is obtaining multi-epoch photometry in the Ks band of the Magellanic System down to a limiting magnitude of Ks ~ 19.3 for individual epoch data. The observations are spaced in time such as to provide optimal sampling of the light curves for RR Lyrae stars and for Cepheids with periods up to 20-30 days. We present examples of the Ks-band light curves of Classical Cepheids and RR Lyrae stars we are obtaining from the VMC data and outline the strategy we put in place to measure distances and infer the System three-dimensional geometry from the variable stars. For this purpose the near-infrared Period-Luminosity, Period-Wesenheit, and Period-Luminosity-Colour relations of the system RR Lyrae stars and Cepheids are used. We extensively exploit the catalogues of the Magellanic Clouds' variable stars provided by the EROS-2 and OGLE III/IV microlensing surveys. By combining these surveys we present the currently widest-area view of the Large Magellanic Cloud as captured by the galaxy Cepheids, RR Lyrae stars and binaries. This reveals the full extent of the main structures (bar/s - spiral arms) that have only been vaguely guessed before. Our work strengthens the case for a detailed study of the Large Magellanic Cloud three-dimensional geometry.
description: 20 pages, 18 figures. Accepted for publication in MNRAS
Total Solar Irradiance during the Last Five Centuries
Creators: name: Penza, V.
name: Berrilli, F.
name: Bertello, L.
name: Cantoresi, M.
name: Criscuoli, S.
name: Giobbi, P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The total solar irradiance (TSI) varies on timescales of minute to centuries. On short timescales it varies due to the superposition of intensity fluctuations produced by turbulent convection and acoustic oscillations. On longer scale times, it changes due to photospheric magnetic activity, mainly because of the facular brightenings and dimmings caused by sunspots. While modern TSI variations have been monitored from space since 1970s, TSI variations over much longer periods can only be estimated using either historical observations of magnetic features, possibly supported by flux transport models, or from the measurements of the cosmogenic isotope (e.g., \textsuperscript{14}C or \textsuperscript{10}Be) concentrations in tree rings and ice cores. The reconstruction of the TSI in the last few centuries, particularly in the 17th/18th centuries during the Maunder minimum, is of primary importance for studying climatic effects. To separate the temporal components of the irradiance variations, specifically the magnetic cycle from secular variability, we decomposed the signals associated with historical observations of magnetic features and the solar modulation potential $Φ$ by applying an Empirical Mode Decomposition algorithm. Thus, the reconstruction is empirical and does not require any feature contrast or field transport model. The assessed difference between the mean value during the Maunder minimum and the present value is $\simeq2.5 Wm^{-2}$. Moreover it shows, in the first half of the last century, a growth of $\simeq 1.5 W m^{-2}$ which stops around the middle of the century to remain constant for the next 50 years, apart from the modulation due to the solar cycle.
Report on the development and promotion of services to industry
Creators: name: I.FAST WP13 members
Publisher: name: Zenodo
Year: 2023

description: This report is the final report on the development and promotion of services to industry in AMICI Technical Facilities (TFs). It corresponds to the final report of task 13.2.
The report outlines the achievements and activities within task 13.2 in establishing a central information and contact point to streamline the access for external partners (sub-task 13.2.1), proposing standardized rules to simplify and expedite access for external partners across different TFs (sub-task 13.2.2), and in summarizing the results of 4 workshops to facilitate collaboration between laboratories and external stakeholders, with a particular focus on specific types of Test Platforms (sub-task (13.2.3). The report therefore underscores the collective commitment to promote collaboration, innovation, and the advancement of technological infrastructure within the AMICI Test Facilities.
Task Leader: DESY, with the active participation of partners including CEA, CIEMAT, CNRS, IFJ-PAN, INFN, KIT, UKRI, and UU.
MENSTRUAL HYGIENE MANAGEMENT PRACTICE AND ITS DETERMINANTS AMONG ADOLESCENT GIRLS IN SECOND CYCLE STUDENTS OF SEBETA TOWN, OROMIA, ETHIOPIA
Creators: name: Abera Degefu
Publisher: name: Zenodo
Year: 2017

description: Background: Menstruation and menstrual practices are still clouded by socio-cultural restrictions resulting in adolescent girls remaining ignorant of the scientific facts and hygienic health practices. Objective: The objective of this study was to assess menstrual hygiene management practice among adolescent girls and its determinants in second cycle schools of Sebeta Town, Oromia Regional State. Materials and Methods: A school based cross-sectional study design was conducted among 466 in-school adolescent girls of grade 7 & 8 in Sebeta Town in December 2016. A single-stage cluster sampling was used to select the students for the present study. The outcome variable for the present study was menstrual hygiene management practice among in-school adolescents. Data management task was undertaken on EpiData 3.1 and analysis was done using SPSS for windows version 21. Bivariate and multivariable logistic regressions analysis were conducted to identify the determinant factors of menstrual hygiene practice of adolescent female in-school students. A p-value of 5% was used as a cut off value to declare statistical significance in this study
A refined dynamical mass for the black hole in the X-ray transient XTE J1859+226
Creators: name: Rizo, I. V. Yanes
name: Torres, M. A. P.
name: Casares, J.
name: Motta, S. E.
name: Muñoz-Darias, T.
name: Rodríguez-Gil, P.
name: Padilla, M. Armas
name: Jiménez-Ibarra, F.
name: Jonker, P. G.
name: Corral-Santana, J.
name: Fender, R.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present two contiguous nights of simultaneous time-resolved GTC spectroscopy and WHT photometry of the black hole X-ray transient XTE J1859+226, obtained in 2017 July during quiescence. Cross-correlation of the individual spectra against a late K-type spectral template enabled us to constrain the orbital period to $0.276 \pm 0.003$ d and the radial velocity semi-amplitude of the donor star to $K_2 = 550 \pm 59$ km s$^{-1}$. An ellipsoidal modulation is detected in the photometric $r$- and $i$-band light curves, although it is strongly contaminated by flickering activity. By exploiting correlations between the properties of the double-peaked H$α$ emission-line profile and the binary parameters, we derived an orbital inclination of $66.6 \pm 4.3$ deg, a refined $K_2 = 562 \pm 40$ km s$^{-1}$ and mass ratio $q = M_2/M_1 = 0.07 \pm 0.01$. From these values we obtained an updated black hole mass of $M_1 = 7.8 \pm 1.9$ M$_\odot$. An independent mass estimate based on X-ray timing agrees well with our value, which gives further support for the outburst QPO triplet being explained by the relativistic precession model. We also obtained a companion star mass $M_2 = 0.55 \pm 0.16$ M$_\odot$, which is consistent with its K5-K7 V spectral type.
description: 7 pages, 5 figures
title: Laijen Spiegel.; 1511
title: Uon rechtmässigen ordnungen in Burgerlichen vnd peinlichen regimenten. mit allegation[en] vn[d] bewerunge[n] ausz geschribnen rechten vnnd gesatzen.
titleType: Subtitle
Creators: name: Tengler, Ulrich
name: Brant, Sebastian
name: Locher, Jakob
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Verfasser nicht auf der Haupttitelseite genannt. - Beiträger: Brant, Sebastian; Locher, Jakob
title: Glosa notabilis prime partis Alexandri; 1492
title: cum interlinearib[us] ex positionibus textus eiusdem in planissimis sententijs. cum vocabulorum lucida exposit[i]o[n]e. subiunctis perpulcre ordinatis questionibus atq[ue] argume[n]tis. cum replicis contra eorundu[m] solut[i]ones. omnibus qui scire desiderant summe necessaria
titleType: Subtitle
Creators: name: Alexander De Villa Dei
name: Gerardus Zutphaniensis
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Alexander de Villa Dei: Doctrinale. P. 1. Mit Komm. von Gerardus Zutphaniensis. - Kolophon: Impressura Magistri Johannis Omar in Reüttling[e]n Anno M.cccc.xcij. Temp[or]e quo c[on]federator[um] populus sueuie cu[m] rege romanor[um] Maximiliano et margrauio de Prandenburg occupaueru[n]t p[ar]tes Bauarie contra ducem Albertu[m de munaco qui ratispanam ciuitatem imperiale[m] contra cesaris volu[n]tatem sibi vsurpauerat. - Bogensignatur: a–f8, gh6, ik8, lm6, no8, pq6, r8, st6, v8
"truthcode_SUSY-2016-25.cxx" of "Search for electroweak production of supersymmetric states in scenarios with compressed mass spectra at $\sqrt{s}=13$ TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2018

description: Truth code to compute acceptance
description: A search for electroweak production of supersymmetric particles in scenarios with compressed mass spectra in final states with two low-momentum leptons and missing transverse momentum is presented. This search uses proton--proton collision data recorded by the ATLAS detector at the Large Hadron Collider in 2015--2016, corresponding to 36.1 fb$^{-1}$ of integrated luminosity at $\sqrt{s}=13$ TeV. Events with same-flavor pairs of electrons or muons with opposite electric charge are selected. The data are found to be consistent with the Standard Model prediction. Results are interpreted using simplified models of R-parity-conserving supersymmetry in which there is a small mass difference between the masses of the produced supersymmetric particles and the lightest neutralino. Exclusion limits at 95% confidence level are set on next-to-lightest neutralino masses of up to 130 GeV for Higgsino production and 170 GeV for wino production, and sleptons masses of up to 180 GeV for pair production of sleptons. In the compressed mass regime, the exclusion limits extend down to mass splittings of 3 GeV for Higgsino production, 2.5 GeV for wino production, and 1 GeV for slepton production. The results are also interpreted in the context of a radiatively-driven natural supersymmetry model with non-universal Higgs boson masses.
"higgsino_110_100.slha" of "Search for electroweak production of supersymmetric states in scenarios with compressed mass spectra at $\sqrt{s}=13$ TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2018

description: SLHA file for Higgsino signal benchmark
description: A search for electroweak production of supersymmetric particles in scenarios with compressed mass spectra in final states with two low-momentum leptons and missing transverse momentum is presented. This search uses proton--proton collision data recorded by the ATLAS detector at the Large Hadron Collider in 2015--2016, corresponding to 36.1 fb$^{-1}$ of integrated luminosity at $\sqrt{s}=13$ TeV. Events with same-flavor pairs of electrons or muons with opposite electric charge are selected. The data are found to be consistent with the Standard Model prediction. Results are interpreted using simplified models of R-parity-conserving supersymmetry in which there is a small mass difference between the masses of the produced supersymmetric particles and the lightest neutralino. Exclusion limits at 95% confidence level are set on next-to-lightest neutralino masses of up to 130 GeV for Higgsino production and 170 GeV for wino production, and sleptons masses of up to 180 GeV for pair production of sleptons. In the compressed mass regime, the exclusion limits extend down to mass splittings of 3 GeV for Higgsino production, 2.5 GeV for wino production, and 1 GeV for slepton production. The results are also interpreted in the context of a radiatively-driven natural supersymmetry model with non-universal Higgs boson masses.
Logik und Enzcyclopaedie der Philos[ophie]. (1r) [Korrekturfassung]. (75r) [Reinschrift]; 1851-1852
Creators: name: Prantl, Carl ¬von
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Entstehungsort: München. - Entstehungszeit: 1851/52 (dat. 1r u. 73r)
Remarks on double Higgs boson production by gluon fusion at threshold
Creators: name: Li, Xin
name: Voloshin, M. B.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The amplitude of double Higgs boson production by the gluon fusion, $gg \to hh$, is known to be small due to cancellation between the graphs with the boson trilinear coupling and those with the coupling to the top quark. For this reason a study of this process was suggested as a sensitive probe of the Higgs sector nonlinearity. We calculate in a closed analytical form this amplitude at the threshold of the two bosons, where the cancellation is the strongest, and discuss the origin of the small value of the amplitude. We also note that the cancellation in the double boson production is in fact a part of a more general phenomenon of suppression of similar threshold amplitudes for multiple boson production, which, although not directly relevant to the actual top quark and the Higgs boson, can be useful in other studies.
description: 9 pages, 3 figures
MT: a Mathematica package to compute convolutions
Creators: name: Hoeschele, Maik
name: Hoff, Jens
name: Pak, Alexey
name: Steinhauser, Matthias
name: Ueda, Takahiro
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We introduce the \prog{Mathematica} package \prog{MT} which can be used to compute, both analytically and numerically, convolutions involving harmonic polylogarithms, polynomials or generalized functions. As applications contributions to next-to-next-to-next-to leading order Higgs boson production and the Drell-Yan process are discussed.
description: 18 pages
"slepton_110_100.slha" of "Search for electroweak production of supersymmetric states in scenarios with compressed mass spectra at $\sqrt{s}=13$ TeV with the ATLAS detector"
Creators: name: ATLAS Collaboration
Publisher: name: HEPData
Year: 2018

description: SLHA file for slepton signal benchmark
description: A search for electroweak production of supersymmetric particles in scenarios with compressed mass spectra in final states with two low-momentum leptons and missing transverse momentum is presented. This search uses proton--proton collision data recorded by the ATLAS detector at the Large Hadron Collider in 2015--2016, corresponding to 36.1 fb$^{-1}$ of integrated luminosity at $\sqrt{s}=13$ TeV. Events with same-flavor pairs of electrons or muons with opposite electric charge are selected. The data are found to be consistent with the Standard Model prediction. Results are interpreted using simplified models of R-parity-conserving supersymmetry in which there is a small mass difference between the masses of the produced supersymmetric particles and the lightest neutralino. Exclusion limits at 95% confidence level are set on next-to-lightest neutralino masses of up to 130 GeV for Higgsino production and 170 GeV for wino production, and sleptons masses of up to 180 GeV for pair production of sleptons. In the compressed mass regime, the exclusion limits extend down to mass splittings of 3 GeV for Higgsino production, 2.5 GeV for wino production, and 1 GeV for slepton production. The results are also interpreted in the context of a radiatively-driven natural supersymmetry model with non-universal Higgs boson masses.
Sciurus oculatus Peters 1863
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Sciurus
Sciurus oculatus

description: Sciurus oculatus Peters, 1863. Monatsb. Preuss. Akad. Wiss. Berlin, p. 653. TYPE LOCALITY: Mexico, Veracruz, probably near Las Vigas. DISTRIBUTION: San Luis Potosi, Hidalgo, Veracruz, Puebla, Mexico, Queretaro and Guanajuato (Mexico). COMMENT: Subgenus Sciurus; see Hall, 1981:430. ISIS NUMBER: 5301410002030017001.
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 365, DOI: 10.5281/zenodo.7353023
description: {"references": ["Hall, E. R. 1981. The mammals of North America. Second ed. John Wiley and Sons, New York, 1: 1 - 600 + 90, 2: 601 - 1181 + 90."]}
[Sammelhandschrift]. (1r) Iulianus Toletanus: Liber prognosticorum futuri saeculi. (63r) [Isidorus Hispalensis: Etymologiarum libri]. (66r) [Ps. Cyprianus]: De duodecim abusivis saeculi. (79r) Origenes: Homilia XXVII in numeros interprete Rufino; [nach 1150]
Creators: name: Iulianus Toletanus
name: Isidorus Hispalensis
name: Cyprianus, Thascius Caecilius
name: Origenes
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2017

description: Entstehungsort: Süddeutschland. - Entstehungszeit: nach 1150
Sciurus pucheranii
Creators: name: Honacki, James H.
name: Kinman, Kenneth E.
name: Koeppl, James W.
Publisher: name: Zenodo
Year: 1982
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Rodentia
Sciuridae
Sciurus
Sciurus pucheranii

description: Sciurus pucheranii (Fitzinger, 1867). Sitzb. Math. Naturw. CL, 55, Abth., 1:487. TYPE LOCALITY: Colombia, near Bogota. DISTRIBUTION: Colombia in the W., C., and E. ranges of the Andes. COMMENT: Subgenus Guerlinguetus; see Cabrera, 1961:372. Moore, 1959, Bull. Am. Mus. Nat. Hist., 118:203, placed pucheranii in the genus Microsciurus. Includes medellinensis; see Cabrera, 1961:372. ISIS NUMBER: 5301410002018006001 as Microsciurus pucherani (sic). 5301410002018005001 as Microsciurus medellineusis (sic).
description: Published as part of James H. Honacki, Kenneth E. Kinman & James W. Koeppl, 1982, Order Rodentia (Part 1), pp. 345-382 in Mammal Species of the World (1 st Edition), Lawrence, Kansas, USA :Alien Press, Inc. & The Association of Systematics Collections on page 365, DOI: 10.5281/zenodo.7353023
description: {"references": ["Moore, J. C. 1959. Relationships among the living squirrels of the Sciurinae. Bulletin of the American Museum of Natural History, 118 (4): 157 - 206."]}
A study of fundamental limitations to statistical detection of redshifted HI from the epoch of reionization
Creators: name: Thyagarajan, Nithyanandan
name: Shankar, N. Udaya
name: Subrahmanyan, Ravi
name: Arcus, Wayne
name: Bernardi, Gianni
name: Bowman, Judd D.
name: Briggs, Frank
name: Bunton, John D.
name: Cappallo, Roger J.
name: Corey, Brian E.
name: deSouza, Ludi
name: Emrich, David
name: Gaensler, Bryan M.
name: Goeke, Robert F.
name: Greenhill, Lincoln J.
name: Hazelton, Bryna J.
name: Herne, David
name: Hewitt, Jacqueline N.
name: Johnston-Hollitt, Melanie
name: Kaplan, David L.
name: Kasper, Justin C.
name: Kincaid, Barton B.
name: Koenig, Ronald
name: Kratzenberg, Eric
name: Lonsdale, Colin J.
name: Lynch, Mervyn J.
name: McWhirter, S. Russell
name: Mitchell, Daniel A.
name: Morales, Miguel F.
name: Morgan, Edward H.
name: Oberoi, Divya
name: Ord, Stephen M.
name: Pathikulangara, Joseph
name: Remillard, Ronald A.
name: Rogers, Alan E. E.
name: Roshi, Anish A.
name: Salah, Joseph E.
name: Sault, Robert J.
name: Srivani, K. S.
name: Stevens, Jamie B.
name: Thiagaraj, Prabu
name: Tingay, Steven J.
name: Wayth, Randall B.
name: Waterson, Mark
name: Webster, Rachel L.
name: Whitney, Alan R.
name: Williams, Andrew J.
name: Williams, Christopher L.
name: Wyithe, J. Stuart B.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In this paper we explore for the first time the relative magnitudes of three fundamental sources of uncertainty, namely, foreground contamination, thermal noise and sample variance in detecting the HI power spectrum from the Epoch of Reionization (EoR). We derive limits on the sensitivity of a Fourier synthesis telescope to detect EoR based on its array configuration and a statistical representation of images made by the instrument. We use the Murchison Widefield Array (MWA) configuration for our studies. Using a unified framework for estimating signal and noise components in the HI power spectrum, we derive an expression for and estimate the contamination from extragalactic point-like sources in three-dimensional k-space. Sensitivity for EoR HI power spectrum detection is estimated for different observing modes with MWA. With 1000 hours of observing on a single field using the 128-tile MWA, EoR detection is feasible (S/N > 1 for $k\lesssim 0.8$ Mpc$^{-1}$). Bandpass shaping and refinements to the EoR window are found to be effective in containing foreground contamination, which makes the instrument tolerant to imaging errors. We find that for a given observing time, observing many independent fields of view does not offer an advantage over a single field observation when thermal noise dominates over other uncertainties in the derived power spectrum.
description: 19 pages, 14 figures (19 figures in total including subfigures), 2 appendices, in press for publication in ApJ
Re-examining the Bayesian colour excess estimation for the local star-forming galaxies observed in the HETDEX Pilot Survey
Creators: name: Shinn, Jong-Ho
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In my previous reanalysis of the local star-forming galaxies observed in the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) pilot survey, I reported that the overestimation of E(B - V), hence the star formation rate (SFR), undermined the claim of new galaxy population discovery in the original study. Herein, I re-examine whether the E(B - V) overestimation problem can be alleviated in the Bayesian parameter estimation framework by adopting scientifically motivated new priors. I modelled the emission-line fluxes of galaxies using the strong-line method and four model parameters-metallicity 12 + log (O/H), nebula emission-line colour excess E(B - V), intrinsic [O III] $λ$5007 line flux and intrinsic [N II] $λ$6584 line flux. Based on mock-data tests, I found that all input values can be recovered within and around the 1-$σ$ credible interval by adopting suitable priors for the intrinsic [O III] $λ$5007 and [N II] $λ$6584 line fluxes: the inverse gamma distribution reflecting the logical constraint that an intrinsic emission-line flux must exceed the observed (reddened) emission-line flux. The mock-data tests were performed for two metallicity calibrations, three colour excess input values [E(B - V) = 0.1, 0.3 and 0.5] and two metallicity input values [12 + log (O/H) = 8.0 and 8.5]. I also found that the new prior can diminish the SFR overestimation eightfold. This study demonstrates how the Bayesian parameter estimation can achieve more accurate estimates with no further observations when the likelihood does not constrain the model parameters correctly.
description: 10 pages, 6 figures, MNRAS in press, online supplementary data are included in the source file
title: Erlaeuterungen und Zusaetze zu Hugo’s Lehrbuch der Geschichte des römischen Rechtes. 3. Auflage. Berlin. Mylius 1806.; [1809]
title: aufgezeichnet in den Vorlesungen des Herrn Professors von Savigny, vormals in Landshut, jetzt in Berlin, während dem Wintersemester im Jahre 1808/1809
titleType: Subtitle
Creators: name: Savigny, Friedrich Carl ¬von
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: [Landshut]. - Entstehungszeit: 1809
[Sammelhandschrift mit mathematischen Abhandlungen]. (1r) Mathematicae scientiae Tractatus [prim]us de Circulis sphaerae mundi. (9v) Mathematicae scientiae Tractatus s[ecundus] de Geographia. (69v) Mathematicaru[m] sci[enti]arum Tract[atus] tertius de Perspectiva. (127r) Mathematicarum sci[enti]arum Tractatus [de] Horologiographia. (150r) [Trigonometrie]. (163r) Astrorum apparentes diametri et distantiae a terra mediocres eorundam, a Tyhone [Brahe] observatae. (nach 163v) 1. Druck: Christoph Scheiner, Ocvlvs Hoc Est: Fvndamentvm Opticvm, In Qvo Ex Accvrata Ocvli Anatome, Abstrvsarvm Experientiarvm Sedvla Pervestigatione, ex inuisis specierum visibilium tam euerso quam erecto situ spectaculis, necnon solidis rationum momentis Radivs Visvalis Ervitvr ... [Innsbruck] 1619. 2. Druck: Cysat, Johann Baptist: Mathemata Astronomica De Loco, Motv, Magnitvdine, Et Cavsis Cometae, Qvi Svb Finem Anni 1618 Et Initivm Anni 1619 In Coelo Fvlsit. Ingolstadii, 1619; 1600-1699
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2016

description: Entstehungsort: Unbekannt. - Entstehungszeit: 17. Jh.
An extended Petviashvili method for the numerical generation of traveling and localized waves
Creators: name: Alvarez, J.
name: Duran, A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: A family of fixed-point iterations is proposed for the numerical computation of traveling waves and localized ground states. The methods are extended versions of Petviashvili type, and they are applicable when the nonlinear term of the system contains homogeneous functions of different degree. The methods are described and applied to several examples of interest, that calibrate their efficiency.
Missing metals in DQ stars: A simple explanation
Creators: name: Blouin, Simon
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Classical DQ stars are white dwarfs whose atmospheres contain detectable traces of carbon brought up to the surface by a convective dredge-up process. Intriguingly, unlike other white dwarf spectral classes, DQ stars virtually never show signs of external pollution by elements heavier than carbon. In this Letter, we solve this long-standing problem by showing that the absence of detectable external pollution in DQ stars is naturally explained by the impact of metal accretion on the atmospheric structure of the white dwarf. A DQ star that accretes heavy elements sees its atmospheric density decrease, which leads to a sharp drop in the molecular carbon abundance and a strong suppression of the C$_2$ Swan bands. We show that a typical DQ star that accretes heavy elements from planetary material generally transforms directly into a DZ star.
description: 5 pages, 5 figures (+12 pages of supplementary figures). Accepted for publication as a Letter in A&A
Determination of Common Hematological Parameters Reference Intervals among Apparently Healthy Pregnant and Non-Pregnant women of South Wollo Zone, Amhara region, Northeast Ethiopia.
Creators: name: Mesfin Fiseha
Publisher: name: Zenodo
Year: 2019

description: Background: The physiology of a normal pregnancy involves major alterations in the

hematological parameters. However, hematological parameters reference intervals currently

being used in Ethiopia is derived from western populations, even though significant variations

are reported previously.

Objective: To determine hematological parameters reference intervals among apparently healthy

pregnant and non-pregnant women of South wollo zone, Amhara region, Northeast Ethiopia.

Method: A community based cross-sectional study was conducted among 600 pregnant and nonpregnant

women in South Wollo Zone, Amhara Region, Northeast Ethiopia from June to August

2019. Medical history, physical examination and laboratory screening were performed for each

study participant. Socio-demographic and other important data were collected using a structured

questionnaire. 4ml of Whole blood was collected and Mindary BC-3000 plus hematology

analyzer was used to measure hematological parameters following standard procedures. Data

were entered and analyzed using SPSS version 23. The mean, median, and 2.5th percentile and

97.5th reference intervals limits with 90% CI were determined for the hematological parameters.

P-value <0.05 was considered statistically significant
[Chronik von Scheyern – Vom Aderlassen und von der Pest] – Jakob Engelin. (1r) Chronik von Scheyern. (5r) Von Nutzen und Zeit des Aderlasses. (5v) Vorbeugendes Pestregiment. (6r) Jakob Engelin: Pesttraktat. (7r) Von den Blattern. (8r) Vom Aderlassen bei Pest. (8v) Mittel gegen Fieber, von den Speisen bei Pest. (8v) Von der Zeit des Aderlassens. (9r) Lasstellentraktat (33 Paragraphen); 1400-1499
Creators: name: Engelin, Jakob
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Entstehungsort: süddeutscher Raum (mittelbairische Mundart). - Entstehungszeit: 15. Jahrhundert