cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
SUGAMMADEX AND HORMONAL CONTRACEPTIVES: IMPROVING EDUCATION AND DOCUMENTATION
Creators: name: Dong, Sydnie Nicole
name: Solis, Christa
name: Tung, Victor
Publisher: name: Zenodo
Year: 2021
Subjects: Sugammadex
hormonal contraceptives
discharge instructions
CDS tools

description: Purpose/Objective  The objective of this DNP project was to improve perioperative counseling for female patients of reproductive age about the decrease in efficacy of hormonal contraceptives with Sugammadex administration and make this education readily available in the discharge instructions. Sugammadex is a neuromuscular blocker reversal agent given perioperatively that encapsulates steroidal non-depolarizing neuromuscular blocking agents and renders them inactive. However, other drugs share a similar steroid-based structure and can result in Sugammadex binding to medications that contain estrogens and progestin, which are often found in hormonal contraceptives. Sugammadex can decrease the efficacy of hormonal contraceptives and potentially lead to unintended pregnancy if proper education is not provided to the patient. Methods  The Iowa Model helped systematically guide this project, and there were three deliverables. An intraoperative Clinical Decision Support Tool (CDS) tool, a Patient Instruction Note function with a “smart text” option, and an in-service to educate anesthesia staff and Post-Anesthesia Care Unit (PACU) nurses about the first two deliverables. Pre- and post-education questionnaires were used to gather baseline data and data after one month of intervention implementation. A statistical analysis of pre-and post-education data was conducted to determine the effectiveness of the intervention. Results A CDS tool was successfully developed and implemented with a “smart text” option to a pilot facility. The educational module did yield a significant change in anesthesia provider understanding that Sugammadex decreases the efficacy of hormonal contraceptive efficacy from the pre-and post-test responses (p < 0.05). Conclusion: These results demonstrated an increase in knowledge about the interaction between Sugammadex and hormonal contraceptives; however, more research is needed to determine if a significant change in practice occurred. 
Hexacentrus japonicus Karny 1907
Creators: name: Chen, Po-Wei
name: Xie, Hui-Cong
name: Wu, Xue
name: Shen, Chu-Ze
name: He, Zhu-Qing
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Orthoptera
Tettigoniidae
Hexacentrus
Hexacentrus japonicus

description: 2.2 Hexacentrus japonicus Karny, 190 7
Hexacentrus japonicus Karny, 1907; Guo et al., 2016; Kim, et al., 2020
Hexacentrus japonicus japonicus Wang & Shi, 2005
Material examined: 1 male, CHINA, Hainan Prov., Jianfengling, 9-viii-2018, coll. He Zhu-Qing; 1 female, CHINA, Hainan Prov., Changjiang, 18-iii-2019, coll. He Zhu-Qing; 1 male, CHINA, Guizhou Prov., Xingyi, 22-vii-2019, coll. He Zhu-Qing; 1 male, CHINA, Yunnan Prov., Mengla, 6-viii-2017, coll. He Zhu-Qing.
Measurements (in mm): Male: SZ 40.11–47.20, PR 7.17–8.04, FW 33.72–40.90, HF 19.17–23.70; Female: SZ 48.54, PR 7.19, FW 39.67, HF 26.26, OV 12.64.
description: Published as part of Chen, Po-Wei, Xie, Hui-Cong, Wu, Xue, Shen, Chu-Ze & He, Zhu-Qing, 2021, A new species of genus Hexacentrus Serville, 1831 from Taiwan (Orthoptera Tettigoniidae: Hexacentrinae), pp. 543-556 in Zootaxa 4933 (4) on page 553, DOI: 10.11646/zootaxa.4933.4.5, http://zenodo.org/record/4556696
Can we put the PUBLIC back into UTILITIES
Creators: name: Cashman, A.
Publisher: name: DTU Library, Technical University of Denmark (DTU)
Year: 2005
Subjects: subject: Stakeholders
subject: public participation
subject: civil society
subject: water management
subject: service provision

description: Since the later half of the 1990\342\200\231s there has been a growing concern to define the role and rights of the public vis-\303\240-vis access to and provision of water services. Implicated in this debate has been the question of the nature and extent of stakeholder involvement and public participation. The purpose of this paper is to explore the relationship between civil society and industry with respect to the management of water resources and services in the light of the re-representation of water as an economic good. In doing so it reconfigured the relationship between those that provided the service, its oversight and those that received the service, locating the relationships in the market and manifest through market relationships. However, there appears to be increasing importance attributed to participation but it is uncertain how far and in what forms public participation and civil society might reach into policy, management and practices. The paper examines some emerging examples of public participation and stakeholder involvement from Europe before considering the implications for water service providers.
Thematische Materialsammlung zu verschiedenen Gegenständen
Creators: name: Bachofen, Johann Jakob
Publisher: name: [s.n.]
Year: 1863

description: Johann Jakob Bachofen
description: Blatt mit den Seiten 169a/169b mit Stecknadel an Seite 169 befestigt
description: Öffentliche Bibliothek der Universität Basel
description: Deutsch
description: Französisch
description: Lateinisch
Quittung (Nr. [1147]) an General maior [Karl Christoph von] Liven
Creators: name: Russland
Publisher: name: [s.n.]
Year: 1798

description: Diese Quittung wurde an Generalmajor Karl Andreevič Liven ausgestellt und ist eine Bestätigung für den Entzug von Lievens Befugnissen als Chef des Musketier-Regiments von Rjažsk. Das Dokument besagt, dass Lieven das Regiment gemäss dem Befehl Seiner kaiserlichen Majestät (Paul I.) verlässt (Lieven war Chef des Musletier-Regiments von 27.07.1797 bis zum 11.08.1798) und zum Kommandeur Leibgarde-Grenadier-Regiment ernannt wird (Lieven war Kommandeur von Leibgarde-Grenadier-Regiment von 11.08.1798 bis zum 01.11.1798). Er übernimmt Personen und Eigentum des Musketier-Regiments von Rjažsk gemäss der Liste in der Rechtsordnung. Unterzeichnet vom Regimentskommandeur (Familienname nicht leserlich). Der Entstehungsort (Rjažsk) des Dokuments ist aufgrund des Inhaltes ermittelt
description: ausgestellt von Polkovoj komandir Rjažskij mušketesrkoj polkʺ [Unbekannt]
description: Mit Lacksiegel
description: Russisch
description: Verzeichnung=Description=Inventaire HAN-Katalogisierungsregeln
Modeling the Optical to Ultraviolet Polarimetric Variability from Thomson Scattering in Colliding Wind Binaries
Creators: name: Ignace, Richard
name: Fullard, Andrew
name: Shrestha, Manisha
name: Naze, Yael
name: Gayley, Kenneth
name: Hoffman, Jennifer L
name: Lomax, Jamie R
name: St-Louis, Nicole
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Massive star binaries are critical laboratories for measuring masses and stellar wind mass-loss rates. A major challenge is inferring viewing inclination and extracting information about the colliding wind interaction (CWI) region. Polarimetric variability from electron scattering in the highly ionized winds provides important diagnostic information about system geometry. We combine for the first time the well-known generalized treatment of \citet{brown_polarisation_1978} for variable polarization from binaries with the semi-analytic solution for the geometry and surface density CWI shock interface between the winds based on Canto et al 1996. Our calculations include some simplifications in the form of inverse square-law wind densities and the assumption of axisymmetry, but in so doing arrive at several robust conclusions. One is that when the winds are nearly equal (e.g., O\,+\,O binaries), the polarization has a relatively mild decline with binary separation. Another is that despite Thomson scattering being a gray opacity, the continuum polarization can show chromatic effects at ultraviolet wavelengths but will be mostly constant at longer wavelengths. Finally, when one wind dominates the other, as for example in WR+OB binaries, the polarization is expected to be larger at wavelengths where the OB component is more luminous, and generally smaller at wavelengths where the WR component is more luminous. This behavior arises because from the perspective of the WR star, the distortion of the scattering envelope from spherical is a minor perturbation situated far from the WR star. By contrast, the polarization contribution from the OB star is dominated by the geometry of the CWI shock.
description: accepted for publication in the Astrophysical Journal. arXiv admin note: text overlap with arXiv:2111.11552
Ukaz (Nr. 6181) an Graf [Karl Christoph von] Liven
Creators: name: Apraksin, Stepan Fedorovič
name: Tarutin, Nikifor Ivanovič
name: Paul
name: Voennaja kollegija
Publisher: name: [s.n.]
Year: 1800

description: Dieses Dokument ist der Befehl Nr. 6181 des Staatlichen Militärkollegiums an General-Leutnant Kavalier Graf Liven I. (Karl Christoph von Lieven, 1767-1844). Der Befehl entstand am 10. März 1800 (jul.) aufgrund eines Befehls von Pavel I. vom 4. März 1800 (jul.) und behandelt die Fusion der drei Garnisonsregimenter: Kireev-Regiment (Garnisonsregiment Archangelsk), Latyschev-Regiment (Garnisonsbataillon Vladimir) und Reichenberg-Regiment (Garnisonsbataillon Nischni Nowgorod). Alle Bataillone, aus denen das neue Regiment besteht, sollen in ihren derzeitigen Orten bleiben und die Uniformen des neu ernannten Chefs tragen. Lieven selbst solle auf weitere Befehlen warten. Das Dokument wurde von drei Personen unterschrieben: Generalleutnant Apraksin, Sekretär Nikifor Tarutin, Registrar Berezovskij.
description: von Generalʺ lejtenantʺ G. Apraksinʺ
description: Russisch
description: Verzeichnung=Description=Inventaire HAN-Katalogisierungsregeln
Diflunisal treatment is associated with improved survival for patients with early stage wild-type transthyretin (ATTR) amyloid cardiomyopathy: the Boston University Amyloidosis Center experience
Creators: name: Siddiqi, Omar K.
name: Mints, Yuliya Y.
name: Berk, John L.
name: Connors, Lawreen
name: Doros, Gheorghe
name: Gopal, Deepa M.
name: Kataria, Shivangi
name: Lohrmann, Graham
name: Pipilas, Alexandra R.
name: Ruberg, Frederick L.
Publisher: name: Taylor & Francis
Year: 2022
Subjects: Cell Biology
Marine Biology
Cancer
Science Policy

description: Diflunisal is a non-steroidal anti-inflammatory drug that stabilises transthyretin (TTR) and reduces neurologic deterioration in patients with polyneuropathy caused by hereditary transthyretin amyloidosis (ATTRv). We conducted a retrospective cohort study of patients with wild-type transthyretin cardiac amyloidosis (ATTRwt-CM) treated with diflunisal for at least one year between 2009 and 2016 at the Boston University Amyloidosis Centre. Baseline and one year follow up characteristics were measured, including plasma chemistries and echocardiography. Cox proportional hazards analysis assessed the primary outcome of all-cause mortality. A total of 104 ATTRwt-CM patients were evaluated with 35 patients receiving diflunisal. Patients in the diflunisal group were younger (73.8 vs 76.8 years, p = 0.034), with lower B-type natriuretic peptide (BNP, 335 +/- 67 vs. 520 +/- 296 pg/mL, p = 0.006), similar troponin I (0.1 +/- 0.1 vs 0.2 +/- 0.3 ng/mL, p = 0.09), and better renal function (eGFR 67 +/- 17 vs 53 +/- 18 mL/min/1.73m2, p = 0.0002) at baseline. Over a median follow-up of 3.2 years, 52 deaths occurred. Diflunisal administration was associated with improved survival in unadjusted analysis (HR 0.13, 95% CI 0.05 − 0.36, p < 0.001) that persisted after adjustment for age, baseline BNP, eGFR, troponin I, interventricular septal thickness, and left ventricular ejection fraction (HR 0.18, 95% CI 0.06 − 0.51, p = 0.0006). Over the observation period, no significant changes in BNP, troponin I, interventricular septal thickness or left ventricular ejection fraction were observed with diflunisal treatment. A total of 14 patients (40%) discontinued diflunisal in this study, but only 3 within the first year. Mean eGFR in treated patients was 59 ml/min/1.73m2 at 1 year (change from baseline p = 0.03). Diflunisal administration in ATTRwt-CM was associated with improved survival and overall stability in clinical and echocardiographic markers of disease with decrement renal function.
Quittung (Nr. 527) an General maior [Karl Andreevič] Liven
Creators: name: Kuprejanov, Evdokim Fëdorovič
name: Russland
Publisher: name: [s.n.]
Year: 1798

description: Dieses Dokument ist die Quittung Nr. 527 an den ehemaligen Kommandeur des Leibgarde-Grenadier-Regiments, Herrn Generalmajor Karl Andreevič Liven (Karl Christoph von Lieven, 1767-1844), erstellt durch den aktuellen Kommandeur des Leibgarde-Grenadier-Regiments, Generalmajor Evdokim Fëdorovič Kuprejanov (1766-1816). Die Quittung bestätigt die rechtmässige Übergabe des Regiments an den neuen Kommandanten. Kuprejanov bestätigt, dass er das Regiment im ordentlichen Zustand übernommen und keine Beschwerden habe
description: von General maior [Evdokim Fëdorovič] Kuprejanovʺ
description: Mit rotem Lacksiegel
description: Russisch
description: Verzeichnung=Description=Inventaire HAN-Katalogisierungsregeln
Photosphere Recession and Luminosity of Homologous Explosions Revisited
Creators: name: Jiang, Hongxuan
name: Liu, Xuewen
name: You, Zhiyong
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: By assuming the photosphere located at the outmost edge of the ejecta, Arnett et al. (1980, 1982, 1989) presented the light curves of homologous explosions in supernovae analytically and numerically to include recombination effects. Actually as homologous expansion proceeds, the photosphere recedes deeper into the ejecta. In this situation, the photosphere radius increases at early times and decreases later on which can be described by a simple method proposed by Liu et al. (2018). To study how the photosphere recession effect the luminosity evolution, we impose a boundary condition on the photosphere to determine the spatial and time distribution of the temperature of the ejecta which is clarified to be reasonable. We find that the photosphere recession reduce the luminosity compared with the previous result without the recession, which can be tested with observations of Type-IIP supernovae.
description: 9 pages, 3 figures
The 3D Galactocentric velocities of Kepler stars: marginalizing over missing RVs
Creators: name: Angus, Ruth
name: Price-Whelan, Adrian M.
name: Zinn, Joel C.
name: Bedell, Megan
name: Yuxi
name: Lu
name: Foreman-Mackey, Daniel
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Precise Gaia measurements of positions, parallaxes, and proper motions provide an opportunity to calculate 3D positions and 2D velocities (i.e. 5D phase-space) of Milky Way stars. Where available, spectroscopic radial velocity (RV) measurements provide full 6D phase-space information, however there are now and will remain many stars without RV measurements. Without an RV it is not possible to directly calculate 3D stellar velocities, however one can infer 3D stellar velocities by marginalizing over the missing RV dimension. In this paper, we infer the 3D velocities of stars in the Kepler field in Cartesian Galactocentric coordinates (vx, vy, vz). We directly calculate velocities for around a quarter of all Kepler targets, using RV measurements available from the Gaia, LAMOST and APOGEE spectroscopic surveys. Using the velocity distributions of these stars as our prior, we infer velocities for the remaining three-quarters of the sample by marginalizing over the RV dimension. The median uncertainties on our inferred vx, vy, and vz velocities are around 4, 18, and 4 km/s, respectively. We provide 3D velocities for a total of 148,590 stars in the Kepler field. These 3D velocities could enable kinematic age-dating, Milky Way stellar population studies, and other scientific studies using the benchmark sample of well-studied Kepler stars. Although the methodology used here is broadly applicable to targets across the sky, our prior is specifically constructed from and for the Kepler field. Care should be taken to use a suitable prior when extending this method to other parts of the Galaxy.
description: Accepted for publication in AAS Journals
Accounting for uncertainty in urban drainage system performance assessment using safety factors applied to runoff
Creators: name: Hansen, A. C.
name: Liu, L.
name: Linde, J. J.
name: Mark, O.
name: Mikkelsen, P. S.
Publisher: name: DTU Library, Technical University of Denmark (DTU)
Year: 2005
Subjects: subject: Uncertainty
subject: statistics
subject: Monte Carlo simulations
subject: safety factor
subject: surcharge
subject: pluvial flooding

description: A crucial step in looking for causes of flooding is a thorough understanding of the uncertainty related to model-based performance assessment of urban drainage systems. This study introduces a methodology for design and analysis of urban drainage systems that takes into account the uncertainties related to the model inputs and parameters. The methodology has the advantage that it can be applied in different stages of the design process irrespective of the complexity of the calculations. For less complex situations the first order analysis of uncertainty is used, while the Monte Carlo method is used for more complex situations. In both cases the uncertainty analysis leads to a safety factor, which can be multiplied by the storm water runoff as part of the design procedure. The safety factor can be calculated for any desired confidence level. The method considers only statistical uncertainties and therefore needs to be further developed.
Disks in Nearby Young Stellar Associations Found Via Virtual Reality
Creators: name: Higashio, Susan
name: Kuchner, Marc J.
name: Silverberg, Steven M.
name: Brandt, Matthew A.
name: Grubb, Thomas G.
name: Gagné, Jonathan
name: Debes, John H.
name: Schlieder, Joshua
name: Wisniewski, John P.
name: Slocum, Stewart
name: Bans, Alissa S.
name: Bhattacharjee, Shambo
name: Biggs, Joseph R.
name: Bosch, Milton K. D.
name: Cernohous, Tadeas
name: Doll, Katharina
name: Luca, Hugo A. Durantini
name: Enachioaie, Alexandru
name: Griffith, Phillip
name: Hamilton, Joshua
name: Holden, Jonathan
name: Hyogo, Michiharu
name: Jung, Dawoon
name: Lau, Lily
name: Piipuu, Fernanda Piñiero Art
name: Stiller, Lisa
name: Collaboration, Disk Detective
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: The Disk Detective citizen science project recently released a new catalog of disk candidates found by visual inspection of images from NASA's Wide-Field Infrared Survey Explorer (WISE) mission and other surveys. We applied this new catalog of well-vetted disk candidates to search for new members of nearby young stellar associations (YSAs) using a novel technique based on Gaia data and virtual reality (VR). We examined AB Doradus, Argus, $β$ Pictoris, Carina, Columba, Octans-Near, Tucana-Horologium, and TW Hya by displaying them in VR together with other nearby stars, color-coded to show infrared excesses found via Disk Detective. Using this method allows us to find new association members in mass regimes where isochrones are degenerate. We propose ten new YSA members with infrared excesses: three of AB Doradus (HD 44775, HD 40540 and HD 44510), one of $β$ Pictoris (HD 198472), two of Octans-Near (HD 157165 and BD+35 2953), and four disk-hosting members of a combined population of Carina, Columba and Tucana-Horologium: CPD-57 937, HD 274311, HD 41992, and WISEA J092521.90-673224.8. This last object (J0925) appears to be an extreme debris disk with a fractional infrared luminosity of $3.7 \times 10^{-2}$. We also propose two new members of AB Doradus that do not show infrared excesses: TYC 6518-1857-1 and CPD-25 1292. We find HD 15115 appears to be a member of Tucana-Horologium rather than $β$ Pictoris. We advocate for membership in Columba-Carina of HD 30447, CPD-35 525, and HD 35841. Finally, we propose that three M dwarfs, previously considered members of Tuc-Hor are better considered a separate association, tentatively called ``Smethells 165''.
description: 26 pages; 17 figures, 3 tables. Accepted for publication in AAS Journals
Estimation of water level in the trunk sewer during drainage pump operation support (RTC) in wet weather
Creators: name: Matsumoto, R.
name: Nishiyama, T.
name: Mushika, S.
name: Morita, S.
Publisher: name: DTU Library, Technical University of Denmark (DTU)
Year: 2005
Subjects: subject: Pump operation support(including RTC)
subject: hydraulic model test
subject: integrated management software
subject: estimation of water level

description: The water levels in wet weather were compared in the Tosabori/Tsumori trunk sewer and at the Tsumori pumping station, which were being constructed in Osaka, a big city in Japan. The comparison was made through simulations using integrated management software systems such as MOUSE, SWMM and Info-Works and hydraulic model tests. As a result, the water level of open channel flow estimated in simulation was higher than that obtained in the test. The variance was less than 6.3% of the diameter of the trunk sewer. Thus, it was shown that the accuracy and reliability of water level estimation could be nearly ensured. It was also indicated that estimating the water level at a given point by simulation was difficult where open channel flow changed into pipe flow in the trunk sewer, where the pumping station was of special shape or where flow was greatly blocked in the trunk sewer by a high head manhole receiving large discharge of inflow.
On the Kalman smoother approach to the stochastic inverse problem of groundwater hydrology
Creators: name: Konecny, Franz
name: Konecny, Franz
Publisher: name: XVI International Conference on Computational Methods in Water Resources
Year: 2006

description: Key words: Inverse problems, distributed parameter systems, infinite dimensional
Kalman smoother, EM algorihm.

In this presentation we are concerned with the estimation of the hydraulic
conductivity profile on the basis of noisy observations of hydraulic heads. An
augmented Kalman smoother is applied to the stochastic flow equation. The
implementation of the smoother requires the solution of a Riccati type partial
differential equation for the smoother covariance and a stochastic partial
differential equation to obtain the optimal estimate of the augmented state. We
discuss finite dimensional approximations of the smoothing problem and propose an
EM algorithm for the estimation of the conductivity parameters.
Plasmid maps_CRISPR donors for Rab11 knock in
Creators: name: Gemperle, Jakub
Publisher: name: University of Manchester
Year: 2021
Subjects: Medical biotechnology not elsewhere classified
Biochemistry and cell biology not elsewhere classified
Bioinformatic methods development
Bioinformatics and computational biology not elsewhere classified
Other biological sciences not elsewhere classified
Agricultural biotechnology not elsewhere classified

description: Plasmid maps_donors for CRISPR mediated knock ins to Rab11 family (Rab11a/Rab11b/Rab25). The synthesized sequences coding fluorophores were codon-optimized for humans.
Olive Cake-Based Growing Diet For Montanera Iberian Pigs: Effects On Meat Quality Traits
Creators: name: López-García, Adrián
name: Fernández-Barroso, Miguel
name: García-Casco, Juan M
name: Caraballo, Carmen
name: Muñoz, María
name: González-Sánchez, Elena
Publisher: name: Zenodo
Year: 2017
Subjects: Iberian pig
olive by-products
growing period
meat quality

description: The traditional production system of Iberian pig includes a particular finish-fattening period called montanera. This semi-extensive system is based on ad libitum intake of grass and acorn, which has a positive effect on meat quality and favors animal wellbeing. However, the restricted diet supplied during the growing period to prevent a nondesirable fatness percentage in final pig products could cause feeding stress. The use of olive by-products during the growing phase diet of

Iberian pigs could be the solution to avoid this stress, but it might have an influence on meat quality. Here, we studied the effect of three different dietary regimens given to Iberian pigs during the growing period (42 kg to 95 kg) on several meat quality traits. A control standard diet group (CD) was compared with two diets based on olive byproducts, one incorporating dry olive pulp in the feed (DD) and the other one incorporating olive cake in wet form (WD). The last one

consisted of olive cake in a silage presentation offered ad libitum and supplemented with a specific feed given once a day in a restricted regimen as the CD and DD diets. We performed meat quality analysis on several traits related with water-holding capacity (thaw loss, (TL); cook loss, (CL); and centrifuge force loss, (CFL)), tenderness (Warner-Bratzler

shear force (Sf)), marbling (Vet) and color (CIELab coordinates for luminosity (L), redness (a), and yellowness (b); color indexes Hue (H) and Chroma (C); and myoglobin concentration, (Mb)). ANOVA was made in order to compare growing diets. We found significant differences in several measured traits. CFL was higher in CD than in WD, meaning that meat from pigs fed with standard diet may have lower water-holding capacity than with olive-based diets. According to color, DD samples were paler and less red-colored than CD and WD ones, and myoglobin concentration was also lower in DD. No differences were observed in visual marbling measures, nor in shear force. We conclude that ad libitum supplementary silage should be a good choice to decrease stress due to pre-montanera restriction, but dry olive pulp-based diet may

have a negative effect on meat quality, since color is important for the consumer.
Energetic Particle Perpendicular Diffusion: Simulations and Theory in Noisy Reduced Magnetohydrodynamic Turbulence
Creators: name: Snodin, A. P.
name: Jitsuk, T.
name: Ruffolo, D.
name: Matthaeus, W. H.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: The transport of energetic charged particles (e.g., cosmic rays) in turbulent magnetic fields is usually characterized in terms of the diffusion parallel and perpendicular to a large-scale (or mean) magnetic field. The nonlinear guiding center theory (NLGC) has been a prominent perpendicular diffusion theory. A recent version of this theory, based on random ballistic spreading of magnetic field lines and a backtracking correction (RBD/BC), has shown good agreement with test particle simulations for a two-component magnetic turbulence model. The aim of the present study is to test the generality of the improved theory by applying it to the noisy reduced magnetohydrodynamic (NRMHD) turbulence model, determining perpendicular diffusion coefficients that are compared with those from the field line random walk (FLRW) and unified nonlinear (UNLT) theories and our test particle simulations. The synthetic NRMHD turbulence model creates special conditions for energetic particle transport, with no magnetic fluctuations at higher parallel wavenumbers so there is no resonant parallel scattering if the particle Larmor radius $R_{\rm L}$ is even slightly smaller than the minimum resonant scale. This leads to non-monotonic variation in the parallel mean free path $λ_\parallel$ with $R_{\rm L}$. Among the theories considered, only RBD/BC matches simulations within a factor of two over the range of parameters considered. This accuracy is obtained even though the theory depends on $λ_\parallel$ and has no explicit dependence on $R_{\rm L}$. In addition, the UNLT theory often provides accurate results and even the FLRW limit provides a very simple and reasonable approximation in many cases.
description: 13 pages, 9 figures, accepted for publication in ApJ
Shock recovery with decaying compressive pulses: Shock effects in calcite (CaCO$_3$) around the Hugoniot elastic limit
Creators: name: Kurosawa, Kosuke
name: Ono, Haruka
name: Niihara, Takafumi
name: Sakaiya, Tatsuhiro
name: Kondo, Tadashi
name: Tomioka, Naotaka
name: Mikouchi, Takashi
name: Genda, Hidenori
name: Matsuzaki, Takuya
name: Kayama, Masahiro
name: Koike, Mizuho
name: Sano, Yuji
name: Murayama, Masafumi
name: Satake, Wataru
name: Matsui, Takafumi
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: Shock metamorphism of minerals in meteorites provides insights into the ancient Solar System. Calcite is an abundant aqueous alteration mineral in carbonaceous chondrites. Return samples from the asteroids Ryugu and Bennu are expected to contain calcite-group minerals. Although shock metamorphism in silicates has been well studied, such data for aqueous alteration minerals are limited. Here, we investigated the shock effects in calcite with marble using impact experiments at the Planetary Exploration Research Center of Chiba Institute of Technology. We produced decaying compressive pulses with a smaller projectile than the target. A metal container facilitates recovery of a sample that retains its pre-impact stratigraphy. We estimated the peak pressure distributions in the samples with the iSALE shock physics code. The capability of this method to produce shocked grains that have experienced different degrees of metamorphism from a single experiment is an advantage over conventional uniaxial shock recovery experiments. The shocked samples were investigated by polarizing microscopy and X-ray diffraction analysis. We found that more than half of calcite grains exhibit undulatory extinction when peak pressure exceeds 3 GPa. This shock pressure is one order of magnitude higher than the Hugoniot elastic limit (HEL) of marble, but it is close to the HEL of a calcite crystal, suggesting that the undulatory extinction records dislocation-induced plastic deformation in the crystal. Finally, we propose a strategy to re-construct the maximum depth of calcite grains in a meteorite parent body, if shocked calcite grains are identified in chondrites and/or return samples from Ryugu and Bennu.
description: 25 pages, 9 figures, 1 table, 1 supporting information, accepted for publication in Journal of Geophysical Research Planets
Taking into account air pressure variations in subsoil air-water
Creators: name: Jaffre, Jerome
name: Marchand, Estelle
name: Clement, François
name: Roberts, Jean
name: Jaffre, Jerome
Publisher: name: XVI International Conference on Computational Methods in Water Resources
Year: 2006

description: The Richards equation is widely used in hydrogeology for modelling flow in an
unsaturated porous media. It is a simplified version of the general two-phase
model, which assumes that air pressure is invariant. To fully take into
account the presence of air which may be trapped in the subsoil, it will be
necessary to consider the non simplified two-phase flow. The aim of this work
is to examine different numerical methods for trading these two models and to
compare the results obtained using 3-dimensional experiments.

In our study we assume that water is incompressible and that air is slightly
compressible. We model both air and water flows using generalized Darcy's law together
with mass conservation. Under the hypothesis that the capillary
pressure depends only on water saturation, the
two-phase flow is described by a system of two nonlinear equations, the
saturation equation and the pressure equation, whose unknows are water
saturation and air pressure.  Richards's equation is obtained, up to a change
of variable, by supposing that air pressure is uniformly equal to atmospheric
pressure. Thus the flow is described by the saturation equation alone, as for
a single-phase flow.  Without this hypothesis, the coupling between the air
equation and the pressure equation is strong: the pressure equation contains
indeed a saturation diffusion term, and because of air compressibility the
pressure equation is not stationary.

A formulation for two-phase flow using the global pressure (a device introduced for
petroleum engineering, generally for incompressible flows) is discussed. The
idea is to eliminate the saturation diffusion term in the pressure equation by
introducing a new artificial variable, homogeneous to a pressure, using the
assumption that the capillary pressure remains low. The mathematical
properties of the new system are interesting, but we will see that it is not
valid for low saturations and so we turn our attention to a standard two-phase
model.

For time discretization of the two-phase equations we use a variation of the
IMPES method (implicit pressure explicit saturation): we decouple the air and
pressure equations. For the spatial discretization, we use finite volumes for
convection, and mixte finite elements of lowest order for diffusion.
Convection terms are upwinded with a Godunov scheme. The treating of the diffusion
term is difficult because it varies rapidly in space. We will compare two
different methods for handling this term. One is the classical method using
harmonic averages of the diffusion coefficients, the other uses implicit
upwinding to evaluate these coefficients.

We use a Newton method to solve the nonlinear systems.

Numerical 3-D simulation of infiltration under rainfalls will illustrate the
presentation.
Tidal disruption of solitons in self-interacting ultralight axion dark matter
Creators: name: Glennon, Noah
name: Nadler, Ethan O.
name: Musoke, Nathan
name: Banerjee, Arka
name: Prescod-Weinstein, Chanda
name: Wechsler, Risa H.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Ultralight axions (ULAs) are promising dark matter candidates that can have a distinct impact on the formation and evolution of structure on nonlinear scales relative to the cold, collisionless dark matter (CDM) paradigm. However, most studies of structure formation in ULA models do not include the effects of self-interactions, which are expected to arise generically. Here, we study how the tidal evolution of solitons is affected by ULA self-interaction strength and sign. Specifically, using the pseudospectral solver UltraDark.jl, we simulate the tidal disruption of self-interacting solitonic cores as they orbit a $10^{11}~M_{\mathrm{\odot}}$ Navarro-Frenk-White CDM host halo potential for a range of orbital parameters, assuming a fiducial ULA particle mass of $10^{-22}\mathrm{eV}$. We find that repulsive (attractive) self-interactions significantly accelerate (decelerate) soliton tidal disruption. We also identify a degeneracy between the self-interaction strength and soliton mass that determines the efficiency of tidal disruption, such that disruption timescales are affected at the $\sim 50\%$ level for variations in the dimensionless ULA self-coupling from $λ=-10^{-92}$ to $λ=10^{-92}$.
description: 15 pages, 10 figures. This paper was made to be as similar to the PRD version as possible
Apparent spot areas in millionths of the solar disk 1973; Scheinbare Flecken-Flächen in Millionsteln der Sonnenscheibe 1973, erhoben von Osservatorio di Roma Monte Mario.
Tabellenblatt (unnum.) mit Daten, eingetragen unter Max Waldmeier, Eidgenössische Sternwarte Zürich
Creators: name: Eidgenössische Sternwarte in Zürich (ETH Zürich bzw. vor 1911 Polytechnikum)
Publisher: name: [s.n.]
Year: 1973

description: Handschriftlich ausgefüllte Tabelle (Vordruck), verwendet für tägliche Werte.
Von unbekannter Hand geführt und als unnum. Blatt ins Jahresregister 1973 eingeordnet, vorgefunden 2019 als letztes Blatt
description: ETH-Bibliothek
Provisional daily Zurich Relative Sunspot Numbers (Rprov.; Rz [prov.]) 1973; Provisorische Relativzahlen der Sonnenflecken 1973.
Tabellenblatt (1) mit Häufigkeitszahlen der täglichen Sonnenfleckenaktivität 1973, erstellt und ergänzt als provisorische Übersicht u.a. durch Max Waldmeier, Eidgenössische Sternwarte Zürich
Creators: name: Eidgenössische Sternwarte in Zürich (ETH Zürich bzw. vor 1911 Polytechnikum)
Publisher: name: [s.n.]
Year: 1973

description: Handschriftlich ausgefüllte Tabelle (Vordruck) für die täglichen Gruppenzahlen g und für die täglichen Fleckenzahlen f 1973 sowie bearbeitet für die provisorische Jahresübersicht 1973 mit täglichen Sonnenfleckenrelativzahlen R.
Tabelle, die Waldmeiers Beobachtungen für Arosa und für Zürich (8cm, 64fache Vergrösserung) ausweist (inkl. tiefgestellt Wert für Bildqualität), die Beobachtungen in Locarno (L) einbezieht, Werte in Klammern setzt, die damit früher als interpolierte Werte ausgewiesen waren und neu keine A (früher für auswärtige Beobachtung) mehr setzt. Die üblicherweise notierte Legende fehlt.
Von Max Waldmeier geführt und als Blatt Nr. 1 ins Jahresregister 1973 eingeordnet.
Die Herausgabe der provisorischen Werte erfolgte zeitgenössisch in maschinenschriftlichen, monatlichen Ausgaben als "Sunspot-Bulletin" (im Bestand nicht überliefert). Die Daten sind ab 1969 dank ESSA Research Laboratories monthly series, IER-FB Solar-Geophysical Data, greifbar, denn die Publikation der Daten in Journal pf Geophysical Research, Space Physics. wurde in jenem Jahr gestoppt. Siehe Vol. 74, Nr. 3, S. 928 https://doi.org/10.1029/JA074i003p00928
description: ETH-Bibliothek
Hexacentrus mundus
Creators: name: Chen, Po-Wei
name: Xie, Hui-Cong
name: Wu, Xue
name: Shen, Chu-Ze
name: He, Zhu-Qing
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Orthoptera
Tettigoniidae
Hexacentrus
Hexacentrus mundus

description: 2.3 Hexacentrus mundus (Walker, 1869)
Piura munda Walker, 1869
Hexacentrus munda Kirby, 1906
Hexacentrus mundus Hebard, 1922; Wang & Shi, 2005; Guo et al., 2016
Material examined: 1 male, CHINA, Yunnan Prov., Gengma, 9-viii-2017, coll. He Zhu-Qing. 1 male, CHINA, Yunnan Prov., Mengla, 6-viii-2017, coll. He Zhu-Qing; 1 male, CHINA, Yunnan Prov., Baihualing, 11-viii-2017, coll. He Zhu-Qing; 1 male, CHINA, Yunnan Prov., Longyang, 11-viii-2017, coll. He Zhu-Qing; 1 male, CHINA, Yunnan Prov., Nabang, 24-iv-2018, coll. He Zhu-Qing.
Measurements (in mm): Male: SZ 39.03–48.15, PR 6.89–8.12, FW 34.45–40.35, HF 19.04–23.53.
description: Published as part of Chen, Po-Wei, Xie, Hui-Cong, Wu, Xue, Shen, Chu-Ze & He, Zhu-Qing, 2021, A new species of genus Hexacentrus Serville, 1831 from Taiwan (Orthoptera Tettigoniidae: Hexacentrinae), pp. 543-556 in Zootaxa 4933 (4) on pages 553-554, DOI: 10.11646/zootaxa.4933.4.5, http://zenodo.org/record/4556696
Epidemiology of hereditary transthyretin amyloidosis in the northernmost region of Sweden: a retrospective cohort study
Creators: name: Baranda, Jorge Mejia
name: Ljungberg, Jenny
name: Wixner, Jonas
name: Anan, Intissar
name: Oskarsson, Viktor
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Epidemiological data on hereditary transthyretin (ATTRv) amyloidosis from the northernmost region of Sweden (Norrbotten) are sparse. We reviewed the medical records of all incident cases of ATTRv amyloidosis in Norrbotten between 2006 and 2018. Official population and mortality statistics were used to estimate incidence rates and standardised mortality ratios (SMRs). Ninety-three patients were diagnosed with ATTRv amyloidosis between 2006 and 2018 (median age, 72.8 years; 68.8% men; 95.7% Val30Met [p.Val50Met] mutation). The incidence rate per 100,000 persons and year increased from 1.50 (95% confidence interval [CI], 0.84–2.47) cases in 2006–2009 to 4.92 (95%CI, 3.46–6.78) cases in 2016–2018. The SMR in the ATTRv amyloidosis cohort was 2.64 times higher than in the general population in 2006–2018 (95%CI, 1.78–3.77). However, there were indications of lower SMRs over time (2006–2012, 2.96 [95%CI, 1.73–4.74]; 2013–2018, 2.32 [95%CI, 1.23–3.96]) and by use of disease-modifying drugs (no, 3.21 [95%CI, 1.87–5.13]; yes, 2.09 [95%CI, 1.08–3.64]). The incidence of ATTRv amyloidosis increased 3-fold in Norrbotten between 2006 and 2018, most likely due to a previous underdiagnosis – with suggestions of lowered mortality during later years, possibly due to the introduction of disease-modifying drugs.
Behaviour of mixed finite element and multipoint point flux approximations for flow with discontinuous coefficients
Creators: name: FONTAINE, Vincent
name: YOUNES, Anis
name: FONTAINE, Vincent
Publisher: name: XVI International Conference on Computational Methods in Water Resources
Year: 2006

description: We study the numerical behaviour and the relationships between some numerical
methods derived from the Mixed Finite Element (MFE) formulation and from the
Control Volume formulation using the Multi-Point Flux Approximation (MPFA) of
Aavatsmark et al. (1996).

All methods are locally mass conservative and are well suited to solve the flow
problem for both steady state (elliptic case) an transient (parabolic case) on a
general irregular grid with anisotropic and heterogeneous discontinuous
coefficients.

Hybridization of the standard MFE method allows to obtain a symmetric positive
definite system which is not, in general, an M-matrix. Moreover, the mixed hybrid
finite element method uses more unknowns (one per edge or face) than the finite
volume formulation (one per element). On the other hand, for a general element
grid, the MPFA method does not give a symmetric matrix of coefficients and
monotonicity issues are known to arise for high aspect ratios combined with skewed
of computational grids.

In this work, we propose two variants of the MFE method: (i) the lumped-MFE method,
based on the equivalence between MHFE method and the P1-nonconforming Galerkin
method for the Laplace equation  and (ii) the multipoint-MFE method based on
Multipoint finite volume discretization using the framework of the modified mixed
finite element space.

We discuss connections between the different approaches and perform numerical
experiments for both steady state and transient cases to compare (number of
unknowns, matrix properties, condition number) and study the numerical behaviour of
these methods (unphysical oscillations, CPU time).
Numerical evaluation of diffusive and dispersive transport in periodic porous media
Creators: name: Ern, Alexandre
name: Dormieux, Luc
name: Tardif D'Hamonville, Pierre
name: Tardif D'Hamonville, Pierre
Publisher: name: XVI International Conference on Computational Methods in Water Resources
Year: 2006

description: At the macroscopic scale, the transport of a fluid component
in a porous medium is governed by advective, diffusive, and dispersive
fluxes. The two latter fluxes are formulated using a
diffusion tensor and a dispersion tensor. The actual value of these
tensors depends on the pore geometry and on the magnitude of the
advection velocity.

Using the double scale expansion technique
and provided
the problem is homogeneizable, it is well-known that the
the diffusion and
dispersion tensors can be evaluated from the following procedure.
First, a velocity field at the pore scale is obtained
by solving a Stokes-like problem. Then, this
velocity field is used in a vector-valued
advection-diffusion equation,
still posed at the pore scale, and from which solution the
the diffusion and
dispersion tensors are evaluated.

Since we are interested in 3D pore geometries for which
analytical solutions are not available,
we use the finite element method to approximate the pore scale velocity
field and to solve the vector-valued
advection-diffusion equation. Three strategies for approximating
the pore scale velocity field are proposed and analyzed. The first uses
nodal Lagrange finite elements with Galerkin/Least Squares
stabilization. The second uses mixed Crouzeix-Raviart/P_0 finite
elements. The third uses the previous mixed finite elements and then
projects the velocity field onto a vector space of divergence-free
fields using Brezzi-Douglas-Marini finite elements.

We perform numerical simulations for cubic and centered cubic networks
of spheres, with several values of the porosity. We also vary the
velocity magnitude to study its effect on the diffusion and dispersion
tensors.
MUSUBI (MegaCam Ultra-deep Survey: $u^\ast$-Band Imaging)-Data for the COSMOS and SXDS Fields
Creators: name: Wang, Wei-Hao
name: Foucaud, Sebastien
name: Hsieh, Bau-Ching
name: Jian, Hung-Yu
name: Lin, Lihwai
name: Lin, Yen-Ting
name: Coupon, Jean
name: Hashimoto, Yasuhiro
name: Ouchi, Masami
name: Shimasaku, Kazuhiro
name: Ohyama, Youichi
name: Umetsu, Keiichi
name: Wang, Shiang-Yu
name: Chang, Tzu-Ching
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Subaru Hyper Suprime-Cam (HSC) Strategic Survey is the latest-generation multi-band optical imaging survey for galaxy evolution and structure formation. The "Ultra-Deep" component of the HSC survey provides $grizy$ broad-band images over $\sim3.4$ deg$^2$ to detection limits of $\sim26$-28 AB, along with narrow-band images, in the COSMOS and the SXDS fields. These images provide an unprecedented combination of depths and area coverage, for the studies galaxies up to $z\sim7$. However, the lack of coverage at $<4000$ Ang implies incomplete sampling of the rest-frame UV at $z\lesssim 3$, which is critically needed for understanding the buildup of stellar mass in the later cosmic time. We conducted a multi-year CFHT $u^\ast$-band imaging campaign in the two HSC Ultra-Deep fields with CFHT MegaCam. By including shallower archival data, we reach 5-$σ$ depths of $u^\ast=28.1$ and 28.4 (AB) at the centers of the COSMOS and SXDS fields, respectively, and $u^\ast=27.7$ and 27.8 in the central 1 deg$^2$ fields. The image quality is $\gtrsim0.90$ arcsec, fairly good for the $u^\ast$ band. Both the photometric and astrometric quality of our data are excellent. We show that the combination of our $u^\ast$-band and HSC data can lead to high-quality photometric redshifts at $z=0$-3, and robust measurements of rest-frame UV on galaxies at $0.4
description: 24 pages, 12 figures, accepted for publication on ApJS
Hexacentrus yunnaneus Bey-Bienko 1962
Creators: name: Chen, Po-Wei
name: Xie, Hui-Cong
name: Wu, Xue
name: Shen, Chu-Ze
name: He, Zhu-Qing
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Orthoptera
Tettigoniidae
Hexacentrus
Hexacentrus yunnaneus

description: 2.4 Hexacentrus yunnaneus Bey-Bienko, 1962
Hexacentrus yunnaneus Bey-Bienko, 1962
Hexacentrus yunnaeus Wang & Shi, 2005
Hexacentrus sp. Guo et al., 2016
description: Published as part of Chen, Po-Wei, Xie, Hui-Cong, Wu, Xue, Shen, Chu-Ze & He, Zhu-Qing, 2021, A new species of genus Hexacentrus Serville, 1831 from Taiwan (Orthoptera Tettigoniidae: Hexacentrinae), pp. 543-556 in Zootaxa 4933 (4) on page 554, DOI: 10.11646/zootaxa.4933.4.5, http://zenodo.org/record/4556696
Animal welfare: a survey of the opinion of farmers and consumers in Sardinia
Creators: name: Giuseppe, Pulina
name: Carta Simona
name: Daniele, Pulino
name: Sara, Spanu
name: Romina, Deriu
name: Antonietta, Mazzette
Publisher: name: Zenodo
Year: 2022

description: Survey texts regarding the opinion on animal welfare of farmers and consumers in Sardinia - Italian version