cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Connection and creativity: generating relational depth in improvised music-making
Creators: name: Hunka, Boris
Publisher: name: University of Limerick
Year: 2023
Subjects: classificationCode: 3603
subject: Music

description: This research explores potential ways to improve musicians experience of improvised music by focusing on increased relational depth. The hypothesis being tested is whether borrowing tenets developed in the context of psychotherapy – specifically adherence to core conditions of empathy, congruence and unconditional positive regard – can have a positive impact on the music. the musician and the audience experience.The research is centred on a series of musical improvisation sessions that took place between 2019 and 2021 between the author and a panel of six selected musicians. The impact of the Covid pandemic meant that some of these sessions were live, and some online – an unanticipated variety of formats that added a layer of research data and insight. A mixed methodology of a Descriptive Phenomenological framework, supplemented by auto-ethnographical elements was utilised.In the course of the research thesis a number of paths to connection as well as obstacles are explored. These include various modes of musical communication, the role of idiom, the ubiquity of judgement and the improvisers’ relationship with the unknown. The research concludes that a conscious adherence to the core conditions of psychotherapy can have a positive impact on improvised music making, by increasing relational depth between the players. This has the potential to benefit the musicians and audiences by enhancing the experience. The research further posits a theoretical model in which rational, emotional and physical elements of communication combine and form an interdependent relationship with spontaneous creativity.
Obelia tenuis Fraser 1938
Creators: name: Mendoza-Becerril, María A.
name: Murillo-Torres, Paulina
name: Serviere-Zaragoza, Elisa
name: León-Cisneros, Karla
name: Mazariegos-Villarreal, Alejandra
name: López-Vivas, Juan Manuel
name: Agüero, José
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Cnidaria
Hydrozoa
Leptothecata
Campanulariidae
Obelia
Obelia tenuis

description: Obelia tenuis Fraser, 1938
Materials
Type status: Other material. Location: locality: La Concha; minimumDepthInMeters: 0.5; maximumDepthInMeters: 1.0; Event: year: 2022; month: 2; day: 11; habitat: middle macroalgae regions; Record Level: dataGeneralizations: 18 ° C; 36 PSU
Notes
Fig. 6 g
Type locality. Ecuador: Santa Elena Bay (Calder et al. 2009).
Detailed description in Mendoza-Becerril et al. (2020).
Taxonomic status. Accepted. AphiaID 832333.
Remarks. Recent morphological studies support the validity of species with sufficient support. Therefore, we follow the morphological evidence indicated in Mendoza-Becerril et al. (2020).
Diagnosis
Colonies erect, sympodial and branching. Stem monosiphonic, divided into nodes and internodes. Internodes with annulations at the base and distal apophysis alternately given off the hydrothecal pedicel or branches. Hydrothecal pedicels are short, with annulations throughout. Hydrothecae with a margin slightly waived or with fine longitudinal folds. Hydrothecal diaphragm straight to slightly oblique. Without gonothecae.
description: Published as part of Mendoza-Becerril, María A., Murillo-Torres, Paulina, Serviere-Zaragoza, Elisa, León-Cisneros, Karla, Mazariegos-Villarreal, Alejandra, López-Vivas, Juan Manuel & Agüero, José, 2024, First records of hydroid epibionts on the introduced macroalga Gracilaria parvispora in the Mexican Pacific, pp. e 130248 in Biodiversity Data Journal 12 on page e130248, DOI: 10.3897/BDJ.12.e130248
A Herschel Study of D/H in Water in the Jupiter-Family Comet 45P/Honda-Mrkos-Pajdusakova and Prospects for D/H Measurements with CCAT
Creators: name: Lis, D. C.
name: Biver, N.
name: Bockelee-Morvan, D.
name: Hartogh, P.
name: Bergin, E. A.
name: Blake, G. A.
name: Crovisier, J.
name: de Val-Borro, M.
name: Jehin, E.
name: Kuppers, M.
name: Manfroid, J.
name: Moreno, R.
name: Rengel, M.
name: Szutowicz, S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present Herschel observations of water isotopologues in the atmosphere of the Jupiter-family comet 45P/Honda-Mrkos-Pajdusakova. No HDO emission is detected, with a 3 sigma upper limit of 2.0 10-4 for the D/H ratio. This value is consistent with the earlier Herschel measurement in the Jupiter-family comet 103P/Hartley 2. The canonical value of 3 10-4 measured pre-Herschel in a sample of Oort-cloud comets can be excluded at a 4.5 sigma level. The observations presented here further confirm that a diversity of D/H ratios exists in the comet population and emphasize the need for additional measurements with future ground-based facilities, such as CCAT, in the post-Herschel era.
description: To appear in The Astrophysical Journal Letters, 8 pages, 4 figures, 1 table
title: Marie Himelfart; 1512
title: Uier schöner predige[n] von vnser liebe[n] Frawe[n]. Eine seit von irer himmelfart, wie sie gott der herr geeret hatt, mit sibe[n]erlei eren. Vnd inn der aller letsten ere, da würt vßgelegt ein frag, an welchem ort im himmelreich, gott ... sein wonu[n]g hatt. Vnd vff welchem stůl ... Maria sitz. Aber die and[er]n drei predigen, sagen von dreyerlei empfengnißen Marie ...
titleType: Subtitle
Creators: name: Geiler von Kaysersberg, Johannes
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2015

description: Kolophon: Getruckt durch Johannes grüninger in ... Straßburg vnd vollendet vff den abent vnser lieben frauwe[n] der geburt, vnd inn dem iar von christi vnseres Herre[n] geburt Tusent fünffhund[er]t vn[n] zwölffe gezalt.
Marmota olympus Olympus (Merriam 1898
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
Marmota
Marmota olympus

description: Marmota olympus (Merriam, 1898). Proc. Acad. Nat. Sci. Phila., 50:352. TYPE LOCALITY: U.S.A., Washington, timberline at head of Soleduc River, Olympic Mtns. DISTRIBUTION: Olympic Mtns, of W. Washington (U.S.A.). COMMENT: Reviewed by Hoffmann et al., 1979, Occas. Pap. Mus. Nat. Hist. Univ. Kans., 83:1 -56. ISIS NUMBER: 5301410002016007001.
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 355, DOI: 10.5281/zenodo.7353023
description: {"references": ["Hoffmann, R. S., J. W. Koeppl, and C. F. Nadler. 1979. The relationships of the amphiberingian marmots (Mammalia: Sciuridae). Occasional Papers of the Museum of Natural History, University of Kansas, 83: 1 - 56."]}
Quantum pumping in helimagnet heterostructures
Creators: name: Zhu, Rui
name: Cui, Li-Juan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Spin-dependent diffraction occurs in helimagnet-related transport processes. In this work, we investigated quantum pumping properties in the normal-metal/helimagnet/normal-metal heterostructure driven by two out of phase time-dependent gate potentials. At the condition when one of the diffracted beams goes out of the horizon the pumped charge and spin currents demonstrate sharp dips and rises as a function of the helimagnet spiral wavevector $q$. At small and large $q$'s, the transmission and pumping properties approach the behaviors of a ferromagnet and an insulating barrier, respectively. For different helimagnet spiral periods, the diffracted angles are different. As a result, the pumped charge and spin currents demonstrate multiple maximal and minimal peaks as a function of $q$, hence, sensitively depend on the helimagnet spin configuration. All the pumping properties can be interpreted by the quantum gate-switching mechanisms.
description: 20 pages, 6 figures
BAmbergische halszgerichts vnd rechtlich Ordenung, jn Peinlichen sachen zů volnfare[n], allen Stetten, Communen Regimenten, Ampleüten, Vogkten Verwesern, Schulteysen Schöffen vnd Richtern Dienlich, fürderlich vnd behilfflich, Darnach zuhandeln vnd rechtsprechen gantz glich-formig gemeine[n] geschrieben rechten [et]c. Daruß auch diß büchlin getzogen vnd vleissig ge-meynem nůtz zugůtt, gesamelt vnd verordnet ist.; 1508.03.12
Creators: name: Georg III., Bamberg, Bischof
name: Schwarzenberg, Johann von
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2017

description: Vorlageform des Erscheinungsvermerks: Getruckt zů Mentz durch Johannem Schöffer vff Mitfasten Jm jar do man zalt nach Christi geburt fünfftzehenhundert vnd acht Jare.
Measuring the Hubble Constant with Double Gravitational Wave Sources in Pulsar Timing
Creators: name: McGrath, Casey
name: D'Orazio, Daniel J.
name: Creighton, Jolien
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Pulsar timing arrays (PTAs) are searching for gravitational waves from supermassive black hole binaries (SMBHBs). Here we show how future PTAs could use a detection of gravitational waves from individually resolved SMBHB sources to produce a purely gravitational wave-based measurement of the Hubble constant. This is achieved by measuring two separate distances to the same source from the gravitational wave signal in the timing residual: the luminosity distance $D_L$ through frequency evolution effects, and the parallax distance $D_\mathrm{par}$ through wavefront curvature (Fresnel) effects. We present a generalized timing residual model including these effects in an expanding universe. Of these two distances, $D_\mathrm{par}$ is challenging to measure due to the pulsar distance wrapping problem, a degeneracy in the Earth-pulsar distance and gravitational wave source parameters that requires highly precise, sub-parsec level, pulsar distance measurements to overcome. However, in this paper we demonstrate that combining the knowledge of two SMBHB sources in the timing residual largely removes the wrapping cycle degeneracy. Two sources simultaneously calibrate the PTA by identifying the distances to the pulsars, which is useful in its own right, and allow recovery of the source luminosity and parallax distances which results in a measurement of the Hubble constant. We find that, with optimistic PTAs in the era of the Square Kilometer Array, two SMBHB sources within a few hundred Mpc could be used to measure the Hubble constant with a relative uncertainty on the order of 10 per cent.
description: 23 pages, 11 figures. Published by the Monthly Notices of the Royal Astronomical Society. arXiv admin note: text overlap with arXiv:2109.07603
title: Erclärünng der landsfreyhait des Herczogthůmbs Baüren [et]c.; [ca. 1513]
title: [Geben vnd geschehen zů Landßhůt. an Montag nach Natiuitatis Marie. Als man zelet ... Fünffzehenhundert vnnd jm achten jare.]
titleType: Subtitle
Creators: name: Wilhelm IV., Bayern, Herzog
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Erscheinungsvermerk nach der Zuweisung des VD16
What is the nature of motor adaptation to dynamic perturbations?
Creators: name: Moullet, Etienne
name: Roby-Brami, Agnès
name: Guigon, Emmanuel
Publisher: name: arXiv
Year: 2022
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Biological sciences

description: When human participants repeatedly encounter a velocity-dependent force field that distorts their movement trajectories, they adapt their motor behavior to recover straight trajectories. Computational models suggest that adaptation to a force field occurs at the action selection level through changes in the mapping between goals and actions. The quantitative prediction from these models indicates that early perturbed trajectories before adaptation and late unperturbed trajectories after adaptation should have opposite curvature, i.e. one being a mirror image of the other. We tested these predictions in a human adaptation experiment and we found that the expected mirror organization was either absent or much weaker than predicted by the models. These results are incompatible with adaptation occurring at the action selection level but compatible with adaptation occurring at the goal selection level, as if adaptation corresponds to aiming toward spatially remapped targets.
description: 72 pages, 8 figures, 10 supplementary figures. To appear in PLoS Computational Biology
Impact of disk demographics on the formation of Giant Planets through pebble accretion
Creators: name: Ronnet, Thomas
Publisher: name: Zenodo
Year: 2020

description: Recent observations suggest that disks around type II protostars do not contain enough dust to account for the observed exoplanet population. Younger disks appear to be more massive, hinting towards the onset of planet formation in the earliest stages of star formation and the rapid assembly of planetary cores. We investigate planet formation through pebble accretion in young disks and discuss the outcome in terms of the observed dust disk mass distribution around class 0 protostars. We find that giant planet formation is possible only within the 30% most massive disks. Giant planets can form at large orbital distances (>10 au) but should be rare, in qualitative agreement with observational inferences.
Marmota sibirica
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
Marmota
Marmota sibirica

description: Marmota sibirica (Radde, 1862). Reise Sud. Ost. Sibir., p. 159. TYPE LOCALITY: U.S. S. R., R.S.F.S. R., Chitinsk Obi., near Tarei-Nor (Lake). DISTRIBUTION: S.W. Siberia, Tuva, Transbaikalia (U.S. S. R.); N. and W. Mongolia; Heilungkiang and Inner Mongolia; formerly Manchuria (China). COMMENT: Placed (with baibacina and himalayana) by Ellerman and Morrison-Scott, 1951:515, and Corbet, 1978:81, in bobak. Gromov et al., 1965:337-415, and Zimina, ed., 1978, [Marmots. Distribution and Ecology], "Nauka," Moscow, provided evidence of specific distinctness and included caliginosus in this species; see comment under baibacina. Nikol'skii, 1974, Zool. Zh., 53:436-444, analyzed contact between baibacina and sibirica in Tuva; Sokolov and Orlov, 1980:329, also indicated sympatry in N.W. Mongolia.
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 356, DOI: 10.5281/zenodo.7353023
description: {"references": ["Ellerman, J. R., and T. C. S. Morrison-Scott. 1951. Checklist of Palaearctic and Indian mammals 1758 to 1946. Trustees of the British Museum (Natural History), London, 810 pp.", "Gromov, I. M., D. I. Bibikov, N. I. Kalabukhov, and M. N. N. Meier. 1965. Fauna SSSR, Mlekopitayushchie, tom. 3, vyp. 2 [Fauna of the U. S. S. R. Mammals. vol. 3, No. 2]. Nazemnye belich'e [Ground Squirrels]. Nauka, Moscow-Leningrad, 467 pp. (in Russian).", "Zimina, R. P. (ed.). 1978. Surki. Rasprostranenie i ekologiya [Marmots. distribution and ecology]. Nauka, Moscow, 222 pp. (in Russian).", "Nikol'skii, A. A. 1974. Geograficheskaya izmenchivost' ritmicheskoi organizatsii zvukovo signala surkov gruppy bobac (Rodentia, Sciuridae) [Geographic variation in rhythmic organization of sound signal in marmots of the bobac group ...]. Zoologicheskii Zhurnal, 53: 436 - 444 (in Russian).", "Sokolov, V. E., and V. N. Orlov. 1980. Opredelitel' mlekopitayushchickh Mongol'skoi Narodnoi Respubliki [Guide to the mammals of the Mongolian People's Republic]. Nauka, Moscow, 351 pp. (in Russian)."]}
title: Sabina von gottes genaden geborne Fürstin von Bairn hertzogin zu Wirttenberg vnd Degk Gräfin zu Münpelgart [et]c. nnsern [!] günstlichen gruss zuuor Ersamen fursichtigen vnnd weysen lieben getrewen ...; [1515]
title: [Datum Munchen an dem heiligen Christabend. Anno [et]c. decimoquinto.]
titleType: Subtitle
Creators: name: Sabina Herzogin Von Württemberg
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2010

description: Bibliogr. Nachweis: VD16 ZV 29100. - Variante zu VD16 S 48 und ZV 24698. Erkennungslesarten: "Degk ... M#[ue]npelgart", endet: "decimoquinto." - Erscheinungsort und Drucker nach der Zuweisung des VD16
Searching for gravitational-wave transients with a qualitative signal model: seedless clustering strategies
Creators: name: Thrane, Eric
name: Coughlin, Michael
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Gravitational-wave bursts are observable as bright clusters of pixels in spectrograms of strain power. Clustering algorithms can be used to identify candidate gravitational-wave events. Clusters are often identified by grouping together seed pixels in which the power exceeds some threshold. If the gravitational-wave signal is long-lived, however, the excess power may be spread out over many pixels, none of which are bright enough to become seeds. Without seeds, the problem of detection through clustering becomes more complicated. In this paper we investigate seedless clustering algorithms in searches for long-lived narrowband gravitational-wave bursts. Using four astrophysically motivated test waveforms, we compare a seedless clustering algorithm to two algorithms using seeds. We find that the seedless algorithm can detect gravitational-wave signals (at fixed false-alarm and false-dismissal rate) at distances between 150-200% greater than those achieved with the seed-based clustering algorithms, corresponding to significantly increased detection volumes: 420-740%. This improvement in sensitivity may extend the reach of second-generation detectors such as Advanced LIGO and Advanced Virgo deeper into astrophysically interesting distances.
description: 8 pages, 1 figure
The chemical abundance pattern of the extremely metal-poor thin disk star 2MASS J1808-5104 and its origins
Creators: name: Mardini, Mohammad K.
name: Frebel, Anna
name: Ezzeddine, Rana
name: Chiti, Anirudh
name: Meiron, Yohai
name: Ji, Alexander P.
name: Placco, Vinicius M.
name: Roederer, Ian U.
name: Meléndez, Jorge
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a high-resolution ($R\sim35,000$), high signal-to-noise ($S/N=350$) Magellan/MIKE spectrum of the bright extremely metal-poor star 2MASS~J1808$-$5104. We find [Fe/H] = $-$4.01 (spectroscopic LTE stellar parameters), [Fe/H] = $-$3.8 (photometric stellar parameters), [Fe/H] = $-$3.7 (spectroscopic NLTE stellar parameters). We measured a carbon-to-iron ratio of $\mbox{[C/Fe]}= 0.38$ from the CH G-band. J1808$-$5104 is thus not carbon-enhanced, contrary to many other stars with similarly low iron abundances. We also determine, for the first time, a barium abundance ($\mbox{[Ba/Fe]} =-0.78$), and obtain a significantly reduced upper limit for the nitrogen abundance ([N/Fe]$ < - 0.2$). J1808$-$5104 has low ratio of $\mbox{[Sr/Ba]}=-0.17$, which is consistent with that of stars in ultra-faint dwarf galaxies. We also fit the abundance pattern of J1808$-$5104 with nucleosynthesis yields from a grid of Population\,III supernova models. There is a good fit to the abundance pattern which suggests J1808$-$5104 originated from gas enriched by a single massive supernova with a high explosion energy of E $=10\times10^{51}$\,erg and a progenitor stellar mass of M$=29.5$\,M$_{\odot}$. Interestingly, J1808$-$5104 is a member of the Galactic thin disk, as confirmed by our detailed kinematic analysis and calculated stellar actions and velocities. Finally, we also established the orbital history of J1808$-$5104 using our time-dependent Galactic potential the \texttt{ORIENT}. J1808$-$5104 appears to have a stable quasi-circular orbit and been largely confined to the thin disk. This unique orbital history, the star's very old age ($\sim13.5$\,Gyr), and the low [C/Fe] and [Sr/Ba] ratios suggest that J1808$-$5104 may have formed at the earliest epoch of the hierarchical assembly of the Milky Way, and it is most likely associated with the primordial thin disk.
Marmota vancouverensis Swarth 1911
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
Marmota
Marmota vancouverensis

description: Marmota vancouverensis Swarth, 1911. Univ. Calif. Publ. Zool., 7: 201. TYPE LOCALITY: Canada, British Columbia, Vancouver Isl., Mt. Douglas. DISTRIBUTION: Mountains of Vancouver Isl. (British Columbia, Canada). COMMENT: Reviewed by Hoffmann et al., 1979, Occas. Pap. Mus. Nat. Hist. Univ. Kans., 83:1 -56. ISIS NUMBER: 5301410002016008001.
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 356, DOI: 10.5281/zenodo.7353023
description: {"references": ["Hoffmann, R. S., J. W. Koeppl, and C. F. Nadler. 1979. The relationships of the amphiberingian marmots (Mammalia: Sciuridae). Occasional Papers of the Museum of Natural History, University of Kansas, 83: 1 - 56."]}
WISDOM Project XII. Clump properties and turbulence regulated by clump-clump collisions in the dwarf galaxy NGC404
Creators: name: Liu, Lijie
name: Bureau, Martin
name: Li, Guang-Xing
name: Davis, Timothy A.
name: Nguyen, Dieu D.
name: Liang, Fu-Heng
name: Choi, Woorak
name: Smith, Mark R.
name: Iguchi, Satoru
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a study of molecular structures (clumps and clouds) in the dwarf galaxy NGC 404 using high-resolution (0.86x0.51 pc^2) Atacama Large Millimeter/sub-millimeter Array ^{12}CO(2-1) observations. We find two distinct regions in NGC 404: a gravitationally-stable central region (Toomre parameter Q=3-30) and a gravitationally-unstable molecular ring (Q<=1). The molecular structures in the central region have a steeper size -- linewidth relation and larger virial parameters than those in the molecular ring, suggesting gas is more turbulent in the former. In the molecular ring, clumps exhibit a shallower mass -- size relation and larger virial parameters than clouds, implying density structures and dynamics are regulated by different physical mechanisms at different spatial scales. We construct an analytical model of clump-clump collisions to explain the results in the molecular ring. We propose that clump-clump collisions are driven by gravitational instabilities coupled with galactic shear, that lead to a population of clumps whose accumulation lengths (i.e. average separations) are approximately equal to their tidal radii. Our model-predicted clump masses and sizes (and mass -- size relation) and turbulence energy injection rates (and size -- linewidth relation) match the observations in the molecular ring very well, suggesting clump-clump collisions is the main mechanism regulating clump properties and gas turbulence in that region. As expected, our collision model does not apply to the central region, where turbulence is likely driven by clump migration.
description: Accepted for publication on MNRAS
Measuring ligand-receptor binding kinetics and dynamics using k-space image correlation spectroscopy
Creators: name: Brandao, Hugo B.
name: Sangji, Hussain
name: Pandzic, Elvis
name: Bechstedt, Susanne
name: Brouhard, Gary J.
name: Wiseman, Paul W.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantitative Methods (q-bio.QM)
subject: FOS: Biological sciences

description: Accurate measurements of kinetic rate constants for interacting biomolecules is crucial for understanding the mechanisms underlying intracellular signalling pathways. The magnitude of binding rates plays a very important molecular regulatory role which can lead to very different cellular physiological responses under different conditions. Here, we extend the k-space image correlation spectroscopy (kICS) technique to study the kinetic binding rates of systems wherein: (a) fluorescently labelled, free ligands in solution interact with unlabelled, diffusing receptors in the plasma membrane and (b) systems where labelled, diffusing receptors are allowed to bind/unbind and interconvert between two different diffusing states on the plasma membrane. We develop the necessary mathematical framework for the kICS analysis and demonstrate how to extract the elevant kinetic binding parameters of the underlying molecular system from fluorescence video-microscopy image time-series. Finally, by examining real data for two model experimental systems, we demonstrate how kICS can be a powerful tool to measure molecular transport coefficients and binding kinetics.
description: 14 pages, 5 figures
Von gottes genaden Wilhelm vnd Ludwig gebruerder Paltzgrauen [!] bey Rein. Hertzogen in Obern vnd Nidern Bairn [et]c. nnserñ [!] guenstlichen grues/ mit sonderm geneigtem vnd gnedigem willen zuuor Wirdigen vñ Ersamen in got/ auch Fuersichtigẽ weisen/ besonder liebñ/ Wie wol der Allerdurchleuechtigist vnd grosmechtigist furst vñ herr/ herr Maximilian Roemischer kayser ... mit weyland ... herrn Albrechten pfaltzgrauen bey Rein Hertzogen in Oberñ vnd Niderñ Bairn [et]c. vnserm ... vatterñ ... vmb merung willen sondrer freuntschaft frid vñ ainigkheit/ zwischen beder Fuerstnthuemb Bairn vñ Wirttenberg ... souil gehandelt/ das zwüschen ... hertzog Vlrichen/ vnd ... vnser ... Schwester/ Frawen Sabina/ ain ... verainigung khunfftiger vermaehlung abgeredt ist worden/ Hat sich doch ... hertzog Vlrich von Wirttenberg nach absterben vnsers ... vatterñ ... gegen ... vnser ... Schwester ... dermassen empaert ... dadurch nit klaine sorg ... eingefalen ist ...; [1515]
Creators: name: Wilhelm IV., Bayern, Herzog
name: Ludwig Philipp Pfalz, Pfalzgraf
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Schreiben in betreff der Ehetrennung ihrer Schwester Sabina vermählt mit Herzog Ulrich von Würtenberg. - Bibliogr. Nachweis: VD16 B 1014. - Variante von VD16 B 1013: Erkennungslesart Zeile 1 und 2 "gebruerder Paltzgrauen" (VD16 B 1014) bzw. "gebrueder Pfaltzgrauen" (VD16 B 1013). - Erscheinungsort und Drucker nach der Zuweisung des VD16
Qvesto Sie Vno Libro Vtilissimo A Chi Se Dileta De Intendere Todescho dechiarando in lingua Taliana[!]; [ca. 1555]
Creators: name: Rotweil, Adam von
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2010

description: Verf. ermittelt. - Text ital. u. dt.
title: Spiegel der Haußucht, Jesus Syrach genand; 1556
title: Sampt einer kurtzen Außlegung. Für die armen Haußuaetter, vnd jhr Gesinde, Wie sie ein Gottselig leben, gegen menigklich sollen erzeygen. ...
titleType: Subtitle
Creators: name: Huberinus, Caspar
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2017

description: Bibliogr. Nachweis: VD16 B 4091. - Titelbl. in Rot- und Schwarzdr. - Vorlageform des Erscheinungsvermerks: Nürnberg/ M.D.LVI. - Kolophon: Gedruckt zu Nürnberg durch Johan[n] vom Berg, vnd Vlrich Newber
The LSST era of supermassive black holes accretion-disk reverberation mapping
Creators: name: Kovacevic, Andjelka B.
name: Radovic, Viktor
name: Ilic, Dragana
name: Popovic, Luka C.
name: Assef, Roberto J.
name: Sanchez-Saez, Paula
name: Nikutta, Robert
name: Raiteri, Claudia M.
name: Yoon, Ilsang
name: Homayouni, Yasaman
name: Li, Yan-Rong
name: Caplar, Neven
name: Czerny, Bozena
name: Panda, Swayamtrupta
name: Ricci, Claudio
name: Jankov, Isidora
name: Landt, Hermine
name: Wolf, Christian
name: Kovacevic-Dojcinovic, Jelena
name: Lakicevic, Masa
name: Savic, Djorđe
name: Vince, Oliver
name: Simic, Sasa
name: Cvorovic-Hajdinjak, Iva
name: Marceta-Mandic, Sladjana
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will detect an unprecedentedly large sample of actively accreting supermassive black holes with typical accretion disk (AD) sizes of a few light days. This brings us to face challenges in the reverberation mapping (RM) measurement of AD sizes in active galactic nuclei (AGNs) using interband continuum delays. We examine the effect of LSST cadence strategies on AD RM using our metric AGNTimeLagMetric. It accounts for redshift, cadence, the magnitude limit, and magnitude corrections for dust extinction. Running our metric on different LSST cadence strategies, we produce an atlas of the performance estimations for LSST photometric RM measurements. We provide an upper limit on the estimated number of quasars for which the AD time lag can be computed within 01000 sources in each Deep Drilling field (DDF, 10 sq. deg) in any filter, with the redshift distribution of these sources peaking at z~1. We find the LSST observation strategies with a good cadence (~ 5 days) and a long cumulative season (~9 yr), as proposed for LSST DDF, are favored for the AD size measurement. We create synthetic LSST light curves for the most suitable DDF cadences and determine RM time lags to demonstrate the impact of the best cadences based on the proposed metric.
description: accepted for publication in the Astrophysical Journal Focus Issue on Rubin LSST cadence and survey strategy
Metamaking and Me - Ceramics Reader
Creators: name: Murphy, Ingrid
Publisher: name: figshare
Year: 2020
Subjects: subject: 190501 Crafts
subject: FOS: Arts (arts, history of arts, performing arts, music)
subject: 190502 Fine Arts (incl. Sculpture and Painting)

description: Metamaking and me is a essay outlining the practice based research of Ingrid Murphy in how new technologies and technological constructs can be applied to traditionally crafted ceramic objects. The essay was published in the Ceramics Reader. Eds Livinstone A, Pertrie, K. Bllomsbury Academic 2017 ISBN 9781472584427
The relativity of space-time-property
Creators: name: Delbourgo, Robert
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We describe a geometrical way to unify gravity with the other natural forces by adding fermionic Lorentz scalar variables, characterising attribute, or property, to space-time location. [With five such properties one can accommodate all known leptons and quarks.] Using just one property, viz. electricity, the general relativity of such a scheme and its superscalar curvature automatically produces the Einstein-Maxwell Lagrangian and a cosmological term. By adding more properties we envisage the geometrical unification of the standard model with gravitation.
description: 11 pages, conference proceedings
N-Band Photonic Hopf Insulators Based on 2D Microring Lattices
Creators: name: Leng, Bo
name: Van, Vien
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Hopf insulators are topological insulators whose topological behavior arises from the nontrivial mapping from a 3D sphere to a 2D sphere, known as the Hopf map. The Hopf map, typically encountered in the study of spinor and skyrmion systems, is classified topologically by an integer invariant called the Hopf index. Here we show that due to the periodic circulation of light inside each microring, a 2D lattice of microring resonators can emulate an $N$-band photonic Hopf insulator with nontrivial Hopf index. In particular, we show by numerical computation and direct analytical proof that the $N$-band Hopf index of the microring lattice is identical to its winding number. The result shows that the Hopf index is an alternative topological invariant for classifying 2D microring photonic lattices and establishes a correspondence between the Hopf insulator phase and the anomalous Floquet insulator phase of the lattice. More generally, our work shows that 2D microring lattices can provide a versatile nanophotonic platform for studying non-Abelian topological photonic systems.
description: 10 pages, 3 figures
title: Melosine geschicht; 1491
title: Mit den figuren
titleType: Subtitle
Creators: name: Thüring Von Ringoltingen
name: Thüring Von Ringoltingen
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2019

description: Weiterer Titel (Textanfang): Von einer frowe[n] gena[n]t Melusina
Menetes Thomas 1908
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
Menetes

description: Menetes Thomas, 1908. J. Bombay Nat. Hist. Soc., 18: 244. ISIS NUMBER: 5301410002017000000.
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 356, DOI: 10.5281/zenodo.7353023
Super prima parte Digesti veteris; [um 1471-72]
Creators: name: Bartolus De Saxoferrato
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2017

description: Bibliografischer Nachweis: H 2579; Fav e Bres 16; Pell 1925; CIBN B-144; IBE 6211; GW 3581
IMPROVINGCOMPLETENESS OFINPATIENT MEDICALRECORDSIN AMDEWORK PRIMARY HOSPITAL, AMHARA, NORTH ETHIOPIA
Creators: name: BAY NAKACHEW ASMAMAW
Publisher: name: Zenodo
Year: 2019

description: Back ground: Globally, Medical recording service is a component of all health care system,

as it is the entry point of the health service and one of the key areas to have quality service in

the health facilities. Clinical record documentation is one of the most basic professional

responsibilities even if it is often poorly practiced. Record keeping and information

management are the requirement for the provision of quality patient service. They are

essential for the patient’s present and future healthcare decision making. The information

contained in the record is essential, but the process of documenting it is often considered a

lesser priority by many health institutions.

Objective: The overall objective of the project is to improve completeness of inpatient

medical records from 65 % to 90% in Amdework primary hospital by the end of June,30,

2019
Co[n]tra monachos proprietarios plurimi egregio[rum] viro[rum] tractatus; [um 1503]
Creators: name: Currifex, Johannes
name: Johannes De Bomalia
name: Petrus Damiani
name: Petrus Cantor
name: Tinctor, Johannes
name: Currifex, Johannes
name: Tinctor, Johannes
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Kopftitel Bl. a2r: Tractatus de vicio proprietatis editus per Iohannem currificis ... - Kolophon: Exaratu[m] Parisius summacu[m] diligentia sumptibus [et] expensis honestorum virorum Gilberti [et] Gaufridi de marnef fratrum bibliopolarum alme vniuersitatis Parisiensis commorantium in vico sancti Jacobi sub Pelicano
The Turing Way: Una guía asertiva para la ciencia de datos reproducible
Creators: name: Santero, Marilina
Publisher: name: Zenodo
Year: 2020

description: Abstract TBA. Información Adicional: Mira el video de presentación en YouTube Leer el documento "README" en español. Contribuir a traducir el libro The Turing Way al español. Gracias Martina G. Vilas, Laura Ación, Malvika Sharan y Kirstie Whitaker por los comentarios sobre esta presentación.
Interpolation between Hilbert spaces
Creators: name: Ameur, Yacin
Publisher: name: arXiv
Year: 2014
Subjects: subject: Functional Analysis (math.FA)
subject: Complex Variables (math.CV)
subject: Operator Algebras (math.OA)
subject: FOS: Mathematics
subject: 46B70, 47A57

description: This note comprises a synthesis of certain results in the theory of exact interpolation between Hilbert spaces. In particular, we examine various characterizations of interpolation spaces and their relations to a number of results in operator-theory and in function-theory.
description: This last update is to conform with what was published
Evolution of the Hub-filament Structures in IC 5146 in the Context of the Energy Balance of Gravity, Turbulence, and Magnetic Field
Creators: name: Chung, Eun Jung
name: Lee, Chang Won
name: Kwon, Woojin
name: Yoo, Hyunju
name: Soam, Archana
name: Cho, Jungyeon
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the results of 850 $μ$m polarization and C$^{18}$O (3-2) line observations toward the western hub-filament structure (W-HFS) of the dark Streamer in IC 5146 using the James Clerk Maxwell Telescope (JCMT) SCUBA-2/POL-2 and HARP instruments. We aim to investigate how the relative importance of the magnetic field, gravity, and turbulence affects core formation in HFS by comparing the energy budget of this region. We identified four 850 $μ$m cores and estimated the magnetic field strengths ($B_{\rm pos}$) of the cores and the hub and filament using the Davis-Chandrasekhar-Fermi method. The estimated $B_{\rm pos}$ is $\sim$80 to 1200 $μ$G. From Wang et al., $B_{\rm pos}$ of E-47, a core in the eastern hub (E-hub), and E-hub were re-estimated to be 500 and 320 $μ$G, respectively, with the same method. We measured the gravitational ($E_{\rm G}$), kinematic ($E_{\rm K}$), and magnetic energies ($E_{\rm B}$) in the filament and hubs and compared the relative importance among them. We found that an $E_{\rm B}$-dominant filament has $aligned$ fragmentation type, while $E_{\rm G}$-dominant hubs show $no$ and $clustered$ fragmentation types. In the $E_{\rm G}$ dominant hubs, it seems that the portion of $E_{\rm K}$ determines whether the hub becomes to have $clustered$ (the portion of $E_{\rm K}\sim20\%$) or $no$ fragmentation type ($\sim10\%$). We propose an evolutionary scenario for the E- and W-HFSs, where the HFS forms first by the collision of turbulent flows, and then the hubs and filaments can go into various types of fragmentation depending on their energy balance of gravity, turbulence, and magnetic field.
description: 19 pages, 10 figures, accepted for publication in AJ
Prognosticon; 1496
Creators: name: Grünpeck, Joseph
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliographischer Nachweis: BSB-Ink G-383.025. Goff G514. Hain 8087. Klebs 478.1. Kotvan 574. Schr 4125. Langer II,2 15a. 15b. Ce³ G-514. CIH 1525. IBS 574. Oates 4033. Šimáková-Vrchotka 873. GW 11567. ISTC ig00514000
Menetes berdmorei
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
Menetes
Menetes berdmorei

description: Menetes berdmorei (Blyth, 1849). J. Asiat. Soc. Bengal, 18(30):600 -603. TYPE LOCALITY: Burma, Tenasserim, Thougyeen Dist. DISTRIBUTION: Indochina; Thailand; Burma; Yunnan (China). ISIS NUMBER: 5301410002017001001.
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 356, DOI: 10.5281/zenodo.7353023
Generalized multifractality in the spin quantum Hall symmetry class with interaction
Creators: name: Babkin, S. S.
name: Burmistrov, I. S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Scaling of various local observables with a system size at Anderson transition criticality is characterized by a generalized multifractality. We study the generalized multifractality in the spin quantum Hall symmetry class (class C) in the presence of interaction. We employ Finkel'stein nonlinear sigma model and construct the pure scaling derivativeless operators for class C in the presence of interaction. Within the two-loop renormalization group analysis we compute the anomalous dimensions of the pure scaling operators and demonstrate that they are affected by the interaction. We find that the interaction breaks exact symmetry relations between generalized multifractal exponents known for a noninteracting problem.
description: 20 LaTex pages
Breviarium Romanum (Francisca usus); 10.07.1481
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2014

description: Bibliografischer Nachweis: Goff B1120; CR 1295; Boh(LB) 387; GW 5133
Goal oriented adaptivity in the IRGNM for parameter identification in PDEs I:\\ reduced formulation
Creators: name: Kaltenbacher, Barbara
name: Kirchner, Alana
name: c, Slobodan Veljovi\'
Publisher: name: arXiv
Year: 2013
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 65J20

description: In this paper we study adaptive discretization of the iteratively regularized Gauss-Newton method IRGNM with an a posteriori (discrepancy principle) choice of the regularization parameter in each Newton step and of the stopping index. We first of all prove convergence and convergence rates under some accuracy requirements formulated in terms of four quantities of interest. Then computation of error estimators for these quantities based on a weighted dual residual method is discussed, which results in an algorithm for adaptive refinement. Finally we extend the results from the Hilbert space setting with quadratic penalty to Banach spaces and general Tikhonov functionals for the regularization of each Newton step.
Shape of the outer stellar warp in the Large Magellanic Cloud disk
Creators: name: Saroon, S.
name: Subramanian, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Warps are vertical distortions of the stellar or gaseous disks of galaxies. One of the proposed scenarios for the formation of warps involves tidal interactions among galaxies. A recent study identified a stellar warp in the outer regions of the south-western (SW) disk of the Large Magellanic Cloud (LMC) and suggested that it might have originated due to the tidal interaction between the LMC and the Small Magellanic Cloud (SMC). Due to the limited spatial coverage of the data, the authors could not investigate the counterpart of this warp in the north-eastern (NE) region, which is essential to understanding the global shape, nature, and origin of the outer LMC warp. In this work, we study the structure of the LMC disk using data on red clump stars from the Gaia Early Data Release 3 (EDR3), which cover the entire Magellanic system. We detected a warp in the NE outer LMC disk which is deviated from the disk plane in the same direction as that of the SW outer warp, but with a lower amplitude. This suggests that the outer LMC disk has an asymmetric stellar warp, which is likely to be a U-shaped warp. Our result provides an observational constraint to the theoretical models of the Magellanic system aimed at improving the understanding the LMC-SMC interaction history.
description: 9 pages, 6 figures. Accepted for publication in A&A and in press
Scaling asymptotics of spectral Wigner functions
Creators: name: Hanin, Boris
name: Zelditch, Steve
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mathematical Physics (math-ph)
subject: Spectral Theory (math.SP)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We prove that smooth Wigner-Weyl spectral sums at an energy level $E$ exhibit Airy scaling asymptotics across the classical energy surface $Σ_E$. This was proved earlier by the authors for the isotropic harmonic oscillator and the proof is extended in this article to all quantum Hamiltonians $-\hbar^2 Δ+ V$ where $V$ is a confining potential with at most quadratic growth at infinity. The main tools are the Herman-Kluk initial value parametrix for the propagator and the Chester-Friedman-Ursell normal form for complex phases with a one-dimensional cubic degeneracy. This gives a rigorous account of Airy scaling asymptotics of spectral Wigner distributions of M.V. Berry, A. Ozorio de Almeida and other physicists.
Reference-star differential imaging on SPHERE/IRDIS
Creators: name: Xie, Chen
name: Choquet, Elodie
name: Vigan, Arthur
name: Cantalloube, Faustine
name: Benisty, Myriam
name: Boccaletti, Anthony
name: Bonnefoy, Mickael
name: Desgrange, Celia
name: Garufi, Antonio
name: Girard, Julien
name: Hagelberg, Janis
name: Janson, Markus
name: Kenworthy, Matthew
name: Lagrange, Anne-Marie
name: Langlois, Maud
name: Menard, François
name: Zurlo, Alice
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Reference-star differential imaging (RDI) is a promising technique in high-contrast imaging that is thought to be more sensitive to exoplanets and disks than angular differential imaging (ADI) at short angular separations (i.e., <0.3"). However, it is unknown whether the performance of RDI on ground-based instruments can be improved by using all the archival data to optimize the subtraction of stellar contributions. We characterize the performance of RDI on SPHERE/IRDIS data in direct imaging of exoplanets and disks. We made use of all the archival data in H23 obtained by SPHERE/IRDIS in the past five years to build a master reference library and perform RDI. In the point-source detection, RDI can outperform ADI at small angular separations (<0.4") if the observing conditions are around the median conditions of our master reference library. On average, RDI has a gain of ~0.8 mag over ADI at 0.15" separation for observations under median conditions. We demonstrate that including more reference targets in the master reference library can indeed help to improve the performance of RDI. In disk imaging, RDI can reveal more disk features and provide a more robust recovery of the disk morphology. We resolve 33 disks in total intensity (19 planet-forming disks and 14 debris disks), and 4 of them can only be detected with RDI. Two disks are resolved in scattered light for the first time. Three disks are detected in total intensity for the first time. The master reference library we built in this work can be easily implemented into legacy or future SPHERE surveys to perform RDI, achieving better performance than that of ADI. To obtain optimal RDI gains over ADI, we recommend future observations be carried out under seeing conditions of 0.6"-0.8".
description: Accepted for publication in Astronomy and Astrophysics; 19 pages, 14 figures, 3 tables
Stimulus amoris; [um 1495]
Creators: name: Bonaventura Heiliger
name: Quentin, Johannes
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2013

description: Bibliografischer Nachweis: Goff B966; GfT 2392; Pell 2658; CIBN B-683; Arnoult 344; Coq 115; Polain (B) 811; IDL 977; IBE 1271; GW 4825 (Pseudo-Bonaventura)