cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
TactIcons: Designing 3D Printed Map Icons for People who are Blind or have Low Vision
Creators: name: Holloway, Leona
name: Butler, Matthew
name: Marriott, Kim
Publisher: name: arXiv
Year: 2024
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: Visual icons provide immediate recognition of features on print maps but do not translate well for touch reading by people who are blind or have low vision due to the low fidelity of tactile perception. We explored 3D printed icons as an equivalent to visual icons for tactile maps addressing these problems. We designed over 200 tactile icons (TactIcons) for street and park maps. These were touch tested by blind and sighted people, resulting in a corpus of 33 icons that can be recognised instantly and a further 34 icons that are easily learned. Importantly, this work has informed the creation of detailed guidelines for the design of TactIcons and a practical methodology for touch testing new TactIcons. It is hoped that this work will contribute to the creation of more inclusive, user-friendly tactile maps for people who are blind or have low vision.
description: Published in Proceedings of the 2023 CHI Conference on Human Factors in Computing Systems (CHI '23), April 23-28, 2023, Hamburg, Germany. ACM, New York, NY, USA
Realitas dan Ilusi dalam Sains: Kajian Filsafat Terhadap Realisme dan Antirealisme
Creators: name: Seena Az-Zahra, Asep Saefurohman
Publisher: name: Zenodo
Year: 2024

description: Penelitian ini mengkaji perdebatan filosofis antara realisme dan antirealisme dalam konteks sains, dengan fokus pada pemahaman tentang realitas dan ilusi. Realisme dalam filsafat sains berpendapat bahwa teori- teori ilmiah memberikan deskripsi yang benar tentang dunia nyata, termasuk entitas yang tidak dapat diamati. Sebaliknya, antirealisme menolak klaim tersebut, menekankan bahwa teori-teori ilmiah hanyalah alat untuk mengorganisir pengalaman manusia tanpa harus mengacu pada keberadaan entitas yang tidak teramati. Melalui analisis literatur dan studi kasus dalam sejarah sains, artikel ini mengeksplorasi argumen utama kedua posisi tersebut dan dampaknya terhadap perkembangan ilmu pengetahuan. Ditemukan bahwa baik realisme maupun antirealisme memiliki implikasi signifikan dalam metode ilmiah, penafsiran data, dan kepercayaan terhadap hasil ilmiah. Penelitian ini juga membahas kemungkinan pendekatan hibrida yang dapat mengakomodasi elemen- elemen dari kedua posisi tersebut untuk mencapai pemahaman yang lebih komprehensif tentang sifat realitas ilmiah.
Additional file 3 of The identification and treatment of alcohol problems in primary care (iTAPP) study: protocol for a stepped wedge cluster randomized control trial testing the 15-method in a primary care setting
Creators: name: Schøler, Peter Næsborg
name: Volke, Kristina Hasselbalch
name: Andréasson, Sven
name: Rasmussen, Sanne
name: Søndergaard, Jens
name: Nielsen, Anette Søgaard
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Cell Biology
Pharmacology
Biotechnology
Mental Health

description: Supplementary Material 3
Stellar Populations in the Transition Region of Nuclear Star Cluster and Nuclear Stellar Disc
Creators: name: Feldmeier-Krause, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Milky Way nuclear star cluster (NSC) is located within the nuclear stellar disc (NSD) in the Galactic centre. It is not fully understood if the formation and evolution of these two components are connected, and how they influence each other. We study the stellar populations in the transition region of NSC and NSD. We observed two $\sim$4.3 pc$^2$ fields with the integral-field spectrograph KMOS (VLT), located at r$\sim$20 pc (> 4 R$_e$) to the Galactic East and West of the NSC. We extract and analyse medium-resolution stellar spectra of >200 stars per field. The data contain in total nine young star candidates. We use stellar photometry to estimate the stellar masses, effective temperatures, and spectral types of the young stars. The stars are consistent with an age of 4-6 Myr, they may have formed inside the Quintuplet cluster, but were dispersed in dynamical interactions. Most stars in the two fields are red giant stars, and we measure their stellar metallicities [M/H] using full spectral fitting. We compare our [M/H] distributions to the NSC and NSD, using data from the literature, and find that the overall metallicity decreases from the central NSC, over the transition region, to the NSD. The steep decrease of [M/H] from the NSC to the region dominated by the NSD indicates that the two components have distinct stellar populations and formation histories.
description: 14 pages (16 pages incl. Appendix), 12 Figures (13), 6 Tables (7). Accepted for publication in MNRAS
NGC 5236's stars as tracers of arms and arm widths in spiral galaxies
Creators: name: Silva-Villa, E.
name: Cano-Gómez, X
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Generally, identifying the spiral arms of a spiral galaxy is not a hard task. However, defining the main characteristics, width and length of those structure is not a common task. Previous studies have used different tracers: Star clusters, Massers, H$α$. It was until recently that individual stars were used as tracers of spiral structures. The basic method of measuring the width of spiral arms assumes a Gaussian distribution around the mean concentration, either of gas or other tracer. In this work we use NGC 5236's stars as tracers. We estimated the surface stellar density of arms and inter-arm regions to measure the width of the arms. As a test case, this works focused on NGC 5236 (M83). We find that field stellar populations can trace the (two) main spiral arms of NGC 5236. We find a correlation between the arm width and the galactocentric radii, found using other tracers. The slope of the growth of the width of the arm correlates with the morphological types of spiral galaxies. A second finding of our study suggest the possible correlation between the width of the arms and the corrotation radius, result that will be presented in a follow up paper.
description: 5 pages, 4 figures. Accepted in MNRAS letter
title: Die Entwicklung des Kasussystems der Wortart Substantiv vom Urindogermanischen zum Neuschwedischen
Creators: name: Lackner, Harald
Year: 2010

description: Die vorliegende Diplomarbeit befasst sich mit der Entwicklung, die das Kasussystem der Wortart Substantiv von der urindogermanischen Sprachstufe (bis ca. 3500 v. Chr.) bis zum Beginn der neuschwedischen Sprachstufe (ab ca. 1550 n. Chr.) durchläuft. Der Schwerpunkt der Darstellung liegt auf den Vorgängen, die nach der Ausgliederung des Schwedischen aus dem Altnordischen stattfinden.
description: This thesis describes the development of the case system of nouns from Proto-Indo-European to Early Modern Swedish.
Crambe kotschyana Boiss.
Creators: name: AL-Shehbaz, Ihsan A.
name: Barriera, Gabrielle
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Crambe
Crambe kotschyana

description: Crambe kotschyana Boiss., Diagn. Pl. Orient. 6: 19. 1846.
Type: “Hab. ad latera occidentalia montis Sabst Buschom prope Schiraz. Kotschy No. 380”.
Lectotypus (designated here): IRAN: “Ad latera occid. spectantia m. Sabst-Buschom pr. u. Schiras”, 14.V.1842, Kotschy 380 (G-BOIS [G00330471]; isolecto-: BM [BM000521176, BM000522982], E [E00042585], FI [FI 005712], G [G00389494, G00389495, G00389496], H [H1350881], HAL [HAL0080982], JE [JE00006108], K [K000653909], L [L1834828], LE [LE00012944, LE00012945], MO [MO 830199, MO3830200], MPU [MPU013479], P [P00741683, P00741684, P00741687, P00741688, P00741689], US [US00099990], W [W0051060, W18890029619], WAG [WAG0000793, WAG0000794, WAG0000795, WAG0000796], WU [WU0101805]).
Notes. – The name needs lectotypification because Boissier examined and annotated the duplicate at FI and based the species description on it and the duplicate in G-BOIS.
Although HEDGE (1968: 46) indicated that the type is at W, none of the two W duplicates of Kotschy 380 is acceptable because they were not examined or annotated by Boissier. Furthermore, W0051060 has the year of collection as 1841 instead of 1842 and lacks the locality data.
The lectotype in G-BOIS is a collection folder of three sheets all carrying the collection number but missing the date of gathering and two of which carrying locality data. The three isolectotypes at G each consists of two sheets in a collection folder.
description: Published as part of AL-Shehbaz, Ihsan A. & Barriera, Gabrielle, 2019, Typification of Edmond Boissier's Cruciferae (Brassicaceae) names enumerated in Flora Orientalis, pp. 1-193 in Boissiera 72 on page 171, DOI: 10.5281/zenodo.7630433
Constraints on cosmic rays in the Milky Way circumgalactic medium from OVIII observations
Creators: name: Roy, Manami
name: Nath, Biman B.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We constrain the cosmic ray (CR) population in the circumgalactic medium (CGM) of Milky Way by comparing the observations of absorption lines of OVIII ion with predictions from analytical models of CGM : precipitation (PP) and isothermal (IT) model. For a CGM in hydrostatic equilibrium, the introduction of CR suppresses thermal pressure, and affects the OVIII ion abundance. We explore the allowances given to the ratio of CR pressure to thermal pressure ($\rm{P}_{\rm{CR}}/\rm{P}_{\rm{th}}=η$), with varying boundary conditions, CGM mass content, photoionization by extragalactic ultraviolet background and temperature fluctuations. We find that the allowed maximum values of $η$ are : $η\lesssim10$ in the PP model and $η\lesssim6$ in the IT model. We also explore the spatial variation of $η$ : rising ($η=Ax$) or declining ($η=A/x$) with radius, where A is the normalization of the profiles. In particular, the models with declining ratio of CR to thermal pressure fare better than those with rising ratio with suitable temperature fluctuation (larger $σ_{\rm ln T}$ for PP and lower for IT). The declining profiles allow $A\lesssim8$ and $A\lesssim10$ in the case of IT and PP models, respectively, thereby accommodating a large value of $η\,(\simeq 200)$ in the central region, but not in the outer regions. These limits, combined with the limits derived from $γ$-ray and radio background, can be useful for building models of Milky Way CGM including CR population. However, the larger amount of CR can be packed in cold phase which may be one way to circumvent these constraints.
description: 11 pages, 5 figures, 1 table Accepted for publication in ApJ on Apr 22, 2022
A modeling method for the Earth's interior structure based on the principles of 2 n geometry and the resulting Earth's tectonic model
Creators: name: hu, jun
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 370699
subject: Geophysics not elsewhere classified
classificationCode: 379901
subject: Earth system sciences
classificationCode: 519901
subject: Complex physical systems

description: We propose a vertical model of the Earth based on 2n geometry and compare it with the PREM model. It is found the results of the two models are similar. The 2n model can be used to obtain and predict some new discoveries, for example, in May 2020, the 2n geometry theory was used to deduce a possible boundary in the core of the Earth near 5574 km, and it was later confirmed there is a boundary in the core with a radius of 650 km. The 2n models can predict some Earth structures that have not yet been discovered. Or explain the current controversy over seismic wave models; Explain why the main discontinuities are "Gutenberg discontinuity" and"Lehman discontinuity". Explain the causes of various discontinuities with new physical geometric ideas, and understand the causes of the earth's circle and the internal logical laws of the earth's sphere from a new theoretical perspective.
Ultracool Dwarfs Observed with the Spitzer Infrared Spectrograph. II. Emergence and Sedimentation of Silicate Clouds in L Dwarfs, and Analysis of the Full M5--T9 Field Dwarf Spectroscopic Sample
Creators: name: Suárez, Genaro
name: Metchev, Stanimir
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: We present a uniform analysis of all mid-infrared $R\approx90$ spectra of field M5--T9 dwarfs obtained with the Spitzer Infrared Spectrograph (IRS). The sample contains 113 spectra out of which 12 belong to late-M dwarfs, 69 to L dwarfs, and 32 to T dwarfs. Sixty-eight of these spectra are presented for the first time. We measure strengths of the main absorption bands in the IRS spectra, namely H$_2$O at 6.25 $μ$m, CH$_4$ at 7.65 $μ$m, NH$_3$ at 10.5 $μ$m, and silicates over 8--11 $μ$m. Water absorption is present in all spectra and strengthens with spectral type. The onset of methane and ammonia occurs at the L8 and T2.5 types, respectively, although ammonia can be detectable as early as T1.5. Silicate absorption sets in at spectral type L2, is on average the strongest in L4--L6 dwarfs, and disappears past L8. However, silicate absorption can also be absent from the spectra at any L subtype. We find a positive correlation between the silicate absorption strength and the excess (deviation from median) near-infrared colour at a given L subtype, which supports the idea that variations of silicate cloud thickness produce the observed colour scatter in L dwarfs. We also find that variable L3--L7 dwarfs are twice more likely to have above-average silicate absorption than non-variables. The ensemble of results solidifies the evidence for silicate condensate clouds in the atmospheres of L dwarfs, and for the first time observationally establishes their emergence and sedimentation between effective temperatures of $\approx$2000 K and $\approx$1300 K, respectively.
description: Accepted for publication in MNRAS
Relationship between Gamma-ray loudness and X-ray spectra of Radio Galaxies
Creators: name: Kayanoki, Taishu
name: Fukazawa, Yasushi
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The {\it Fermi} satellite has detected $\sim$60 radio galaxies (RGs). In this study, we investigate the difference in the properties of X-ray spectra between GeV-loud RGs and GeV-quiet RGs. Our sample comprises 68 objects: 36 RGs detected with {\it Fermi} and 32 RGs not detected with gamma rays. We analyzed the X-ray spectra of these 68 objects using data from the {\it XMM-Newton}, {\it Chandra}, {\it NuSTAR}, and {\it Swift} satellites. Our results show that most GeV-loud RGs do not exhibit significant absorption, while $\sim$50\% of the GeV-quiet RGs exhibit significant absorption. This suggests that the jet of GeV-loud RGs is viewed from a small angle, and thus the emission is not easily blocked by the torus. Moreover, we reported that RGs with a heavy absorption are mostly in the X-ray luminosity range of $10^{43}-10^{45}$erg s$^{-1}$; however, few RGs with lower and higher luminosity suffer from heavy absorption. This is the same trend as that of Seyfert galaxies.
description: 23 pages, 7 figures, 4 tables, PASJ accepted (2022/04/27)
Crambe quadricostata Boiss.
Creators: name: AL-Shehbaz, Ihsan A.
name: Barriera, Gabrielle
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Crambe
Crambe quadricostata

description: Crambe quadricostata Boiss. in Ann. Sci. Nat., Bot. ser. 2, 17: 388. 1842.
Type: “[Aucher-Eloy] N. 179, Mesopotamia ”.
Holotypus: SINE PATRIA: “ Mesopotamia ”, s.d., AucherEloy 179 (G-BOIS [G00330472]; iso-: G [G00446310, G00446311], K [K000653911], P [P05408797, P05408804]).
= Crambe orientalis L., Sp. Pl.: 671. 1753.
Notes. – It is not possible to determine the country of origin of the type collection, and it could be Iraq, Syria, or Turkey.
Boissier in Flora Orientalis reduced the species to synonymy of C. orientalis.
description: Published as part of AL-Shehbaz, Ihsan A. & Barriera, Gabrielle, 2019, Typification of Edmond Boissier's Cruciferae (Brassicaceae) names enumerated in Flora Orientalis, pp. 1-193 in Boissiera 72 on page 172, DOI: 10.5281/zenodo.7630433
Additional file 1 of Using machine learning to develop preoperative model for lymph node metastasis in patients with bladder urothelial carcinoma
Creators: name: Ji, Junjie
name: Zhang, Tianwei
name: Zhu, Ling
name: Yao, Yu
name: Mei, Jingchang
name: Sun, Lijiang
name: Zhang, Guiming
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer

description: Supplementary Material 1
Hybrid Equations of State for Neutron Stars with Hyperons and Deltas
Creators: name: Clevinger, A.
name: Corkish, J.
name: Aryal, K.
name: Dexheimer, V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In this contribution, we describe new chemically-equilibrated charge-neutral hybrid equations of state for neutron stars. They present a first-order phase transition to quark matter and differentiate by the particle population considered and how these particles interact. While some equations of state contain just nucleons and up, down-quarks, others also contain hyperons, Delta baryons, and strange quarks. The hybrid equations of state, together with corresponding hadronic ones, are available on the CompOSE repository and can be used for different astrophysical applications.
description: Invited contribution to Special Issue on "CompOSE: a repository for Neutron Star Equations of State and Transport Properties"
ผลของระยะปลูกต่อการเจริญเติบโตและผลผลิตของมันจาวมะพร้าว
Creators: name: รัตนาภรณ์  กุลชาติ
Publisher: name: คณะเทคโนโลยีการเกษตร มหาวิทยาลัยราชภัฏมหาสารคาม
Year: 2024
Subjects: มันจาวมะพร้าว
ระยะปลูก
การเจริญเติบโต
ผลผลิต
ผลตอบแทน

description: วารสารเกษตรพระวรุณ, 21, 2, 53-62
WIYN Open Cluster Study: The Old Open Cluster, NGC 188, and a Re-evaluation of Lithium-Richness Among Red Giants
Creators: name: Sun, Qinghui
name: Deliyannis, Constantine P.
name: Twarog, Bruce A.
name: Anthony-Twarog, Barbara J.
name: Cummings, Jeffrey D.
name: Steinhauer, Aaron
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present WIYN/Hydra spectra of 34 red giant candidate members of NGC 188, which, together with WOCS and Gaia data yield 23 single members, 6 binary members, 4 single nonmembers, and 1 binary nonmember. We report [Fe/H] for 29 members and derive [Fe/H]$_{\rm{NGC188}}$ = +0.064 $\pm$ 0.018 dex ($σ_μ$) (sky spectra yield A(Fe)$_{\odot}$ = 7.520 $\pm$ 0.015 dex ($σ_μ$)). We discuss effects on the derived parameters of varying Yale-Yonsei isochrones to fit the turnoff. We take advantage of the coolest, lowest-gravity giants to refine the line list near Li 6707.8 Å. Using synthesis we derive detections of A(Li) = 1.17, 1.65, 2.04, and 0.60 dex for stars 4346, 4705, 5027, and 6353, respectively, and 3$σ$ upper-limits for the other members. Whereas only two of the detections meet the traditional criterion for "Li-richness" of A(Li) > 1.5 dex, we argue that since the cluster A(Li) vanish as subgiants evolve to the base of the RGB, all four stars are Li-rich in this cluster's context. An incidence of even a few Li-rich stars in a sample of 29 stars is far higher than what recent large surveys have found in the field. All four stars lie either slightly or substantially away from the cluster fiducial sequence, possibly providing clues about their Li-richness. We discuss a number of possibilities for the origin for the Li in each star, and suggest potentially discriminating future observations.
description: 20 pages, 16 figures, 7 tables, accepted for publication in MNRAS
Crambe orientalis var. aucheri Boiss.
Creators: name: AL-Shehbaz, Ihsan A.
name: Barriera, Gabrielle
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Crambe
Crambe orientalis
Crambe orientalis var. aucheri (boiss.) boiss., fl.

description: Crambe orientalis var. aucheri (Boiss.) Boiss., Fl. Orient. 1: 407. 1867.
 Crambe aucheri Boiss. in Ann. Sci. Nat., Bot. ser. 2, 17: 388. 1842.
Type: “[Aucher-Eloy] N. 180, Syria ”.
Lectotypus (designated here): SYRIA: sine loco, s.d., AucherEloy 180 (G-BOIS [G00330473]; isolecto-: G [G00441286, G00441553], K [K000653916, K000653917], P [P00741691, P00741692, P00741693]).
= Crambe orientalis L., Sp. Pl.: 671. 1753.
Note. – Boissier examined both G00441286 and the G-BOIS specimens, but none of the other duplicates, in drafting the species description and therefore the name needed lectotypification. The specimen in G-BOIS is a fruiting material without leaves, and the original description provides a good description of leaves that was most likely taken from the former duplicate.
description: Published as part of AL-Shehbaz, Ihsan A. & Barriera, Gabrielle, 2019, Typification of Edmond Boissier's Cruciferae (Brassicaceae) names enumerated in Flora Orientalis, pp. 1-193 in Boissiera 72 on page 172, DOI: 10.5281/zenodo.7630433
Arichlidon Watson Russell 1998
Creators: name: Watson, Charlotte
name: Chivers, Adam J.
name: Narayanaswamy, Bhavani E.
name: Lamont, Peter
name: Turnewitsch, Robert
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Annelida
Polychaeta
Phyllodocida
Chrysopetalidae
Arichlidon

description: Arichlidon Watson Russell, 1998
 Arichlidon hanneloreae Watson Russell, 1998: 160, Figs 1–4 [type species]
description: Published as part of Watson, Charlotte, Chivers, Adam J., Narayanaswamy, Bhavani E., Lamont, Peter & Turnewitsch, Robert, 2014, Chrysopetalidae (Annelida: Phyllodocida) from the Senghor Seamount, north-east Atlantic: taxa with deep-sea affinities and morphological adaptations, pp. 311-325 in Memoirs of Museum Victoria 71 on page 317, DOI: 10.24199/j.mmv.2014.71.24, http://zenodo.org/record/12212666
Additional file 2 of Using machine learning to develop preoperative model for lymph node metastasis in patients with bladder urothelial carcinoma
Creators: name: Ji, Junjie
name: Zhang, Tianwei
name: Zhu, Ling
name: Yao, Yu
name: Mei, Jingchang
name: Sun, Lijiang
name: Zhang, Guiming
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer

description: Supplementary Material 2
Investigating Compensatory Brain Activity in Older Adults with Subjective Cognitive Decline
Creators: name: Krebs, Christine
name: Brill, Esther
name: Minkova, Lora
name: Federspiel, Andrea
name: Kellner-Weldon, Frauke
name: Wyss, Patric
name: Teuniessen, Charlotte
name: Van Harten, Argonde
name: Seydell-Greenwald, Anna
name: Klink, Katharina
name: Züst, Marc
name: Brem, Anna-Katharina
name: Kloeppel, Stefan
Publisher: name: Zenodo
Year: 2023

description: Investigating Compensatory Brain Activity in Older Adults with Subjective Cognitive Decline
Using EAGLE simulations to study the effect of observational constraints on the determination of HI asymmetries in galaxies
Creators: name: Bilimogga, P. V.
name: Oman, K. A.
name: Verheijen, M. A. W.
name: van der Hulst, J. M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the effect of observational constraints such as signal-to-noise, resolution and column density level on the HI morphological asymmetry ($\mathrm{A}_\mathrm{mod}$) and the effect of noise on the HI global profile ($\mathrm{A}_\mathrm{flux}$) asymmetry indices. Using mock galaxies from the EAGLE simulations we find an optimal combination of the observational constraints that are required for robust measurement of the $\mathrm{A}_\mathrm{mod}$ value of a galaxy: a column density threshold of $5\times10^{19}cm^{-2}$ or lower at a minimal signal-to-noise of 3 and a galaxy resolved with at least 11 beams. We also use mock galaxies to investigate the effect of noise on the $\mathrm{A}_\mathrm{flux}$ values and conclude that a global profile with signal-to-noise ratio greater than 5.5 is required to achieve a robust measurement of asymmetry. We investigate the relation between $\mathrm{A}_\mathrm{mod}$ and $\mathrm{A}_\mathrm{flux}$ indices and find them to be uncorrelated which implies that $\mathrm{A}_\mathrm{flux}$ values cannot be used to predict morphological asymmetries in galaxies.
description: 19 pages, 12 figures and 2 appendices. Accepted for publication in the Monthly Notices of the Royal Astronomical Soceity
Crambe persica Boiss.
Creators: name: AL-Shehbaz, Ihsan A.
name: Barriera, Gabrielle
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Crambe
Crambe persica

description: Crambe persica Boiss. in Ann. Sci. Nat., Bot. ser. 2, 17: 389. 1842.
Type: “[Aucher-Eloy] N. 4131, Demavend”.
Lectotypus (designated here): IRAN: “Demavend”, s.d., AucherEloy 4131 (G-BOIS [G00332129]; isolecto-: G [G00441285], K [K000653918], P [P00741694, P00741695]).
= Crambe orientalis L., Sp. Pl.: 671. 1753.
Note. – BOISSIER (1842c) based the species description on the material in his herbarium and on P00741695 that he annotated.
description: Published as part of AL-Shehbaz, Ihsan A. & Barriera, Gabrielle, 2019, Typification of Edmond Boissier's Cruciferae (Brassicaceae) names enumerated in Flora Orientalis, pp. 1-193 in Boissiera 72 on page 172, DOI: 10.5281/zenodo.7630433
Switching of the information backflow between a helical spin system and non-Markovian bath
Creators: name: Kaczor, Michał
name: Tralle, Igor
name: Jakubczyk, Paweł
name: Stagraczyński, Stefan
name: Chotorlishvili, Levan
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The dissipative dynamics of the spin chain coupled to the non-Markovian magnonic reservoir was studied. The chirality of the chain is formed due to the magnetoelectric coupling. We explored the sign of the trace distance derivative and found the alternating positive/negative periods in system's time evolution. The negative sign is associated with the flow of information from the system to the bath and decrease in states distinguishability, while the positive sign is related to the flow of the information in the opposite direction and increase in distinguishability. We found the distinct effect of the applied electric and magnetic fields. While the Dzyaloshinskii-Moriya interaction and external electric field lead to reshuffling of the periods, the applied magnetic field leads to the swift positive-negative transitions. Thus, in the helical quantum rings coupled to the non-Markovian magnonic baths, it is possible to control the directions of information flow through the external fields.
description: 17 pages, 3 figures
Additional file 3 of Using machine learning to develop preoperative model for lymph node metastasis in patients with bladder urothelial carcinoma
Creators: name: Ji, Junjie
name: Zhang, Tianwei
name: Zhu, Ling
name: Yao, Yu
name: Mei, Jingchang
name: Sun, Lijiang
name: Zhang, Guiming
Publisher: name: figshare
Year: 2024
Subjects: Medicine
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Mathematical Sciences not elsewhere classified
Cancer

description: Supplementary Material 3
Bunias L.
Creators: name: AL-Shehbaz, Ihsan A.
name: Barriera, Gabrielle
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Brassicales
Brassicaceae
Bunias

description: Bunias L., Sp. Pl.: 669. 1753.
Tribe: Buniadeae DC.
Note. – Bunias includes only two Eurasian species.
description: Published as part of AL-Shehbaz, Ihsan A. & Barriera, Gabrielle, 2019, Typification of Edmond Boissier's Cruciferae (Brassicaceae) names enumerated in Flora Orientalis, pp. 1-193 in Boissiera 72 on page 172, DOI: 10.5281/zenodo.7630433
title: Die neuen Beginen
Creators: name: Kastenhofer, Maria-Regina
Year: 2010

description: In Österreich und vor allem in Deutschland gibt es vermehrt Frauen, die versuchen an die Lebensform der mittelalterlichen Beginen anzuschließen. Sie leben in Beginenhöfen oder schließen sich zu Gemeinschaften zusammen (Notburga-Gemeinschaft, Beginen heute e.V.) und übersetzen dabei zentrale Momente der historischen Beginenbewegung in die heutige gesellschaftliche und kirchliche Situation. Anhand des pastoraltheologischen Dreischritts Sehen-Urteilen-Handeln wird in der vorliegenden Arbeit überprüft, inwiefern die neuen Beginen eine Anregung für zeitgenössische kirchliche Lebensformen sein können. Als erster Schritt wird eine empirische Darstellung der historischen und dann der neuen Beginen vorgenommen. Die historische und die gegenwärtige Bewegungen werden hernach anhand von neun Kriterien, die aus den Grundvollzügen kirchlicher Praxis, aus der Diskussion um Lebensformen und aus der Literatur über die alten Beginen abgeleitet werden, einzeln auf ihre Kirchlichkeit hin überprüft und bewertet. Dabei zeigt sich bei beiden Bewegungen ihre konstitutiv diakonische Ausrichtung, ihr Versuch neue Formen von Frauenleben zu etablieren, ihre Sensibilität für die Zeichen der Zeit und ihr kreativer Umgang mit der Tradition. Schließlich werden vom Zugang der Beginen zu ihrer Lebensform und von ihrem Handeln, Anregungen und Provokationen für Lebensformen in der Kirche von heute aufgestellt.
description: Currently in Austria and in Germany an increasing number of women try to connect to the medieval forms of Beguine life. They live in beguinages or form communities (e.g. the Notburga-Gemeinschaft or the association Beginen heute e.V.). Thereby they transfer essential characteristics of the historical Beguine movement into modern social and ecclesiastical contexts. According to the three steps of See-Judge-Act in Pastoral Theology the analysis in this thesis follows the aim to find out which suggestions for contemporary forms of ecclesial life can be drawn from the new Beguines. The first step is an empirical portray of the historical and later the new Beguines. After that, the historical as well as the contemporary Beguine movement are analysed according to nine criteria. Those criteria derive from the previous discussion of the functions of ecclesiastical practice, of different ways of living through a Pastoral Theological perspective and the literature on the historical Beguines. Findings in this process are: the constituent charitable orientation of the Beguines, their effort to establish new forms of female life, their sensitivity in reading the sings of time and their creative handling of tradition. Finally, suggestions and provocations for contemporary ecclesiastical ways of life are drawn from the Beguine’s approach to living and their social and ecclesial practice.
The Potential of Detecting Radio-flaring Ultracool Dwarfs at L band in the FAST Drift-scan Survey
Creators: name: Tang, Jing
name: Tsai, Chao-Wei
name: Li, Di
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The Five-hundred-meter Aperture Spherical radio Telescope (FAST) completed its commissioning and began the Commensal Radio Astronomy FasT Survey (CRAFTS), a multi-year survey to cover 60% of the sky, in 2020. We present predictions for the number of radio-flaring ultracool dwarfs (UCDs) that are likely to be detected by CRAFTS. Based on the observed flaring UCDs from a number of unbiased, targeted radio surveys in the literature, we derive a detection rate of $\ge$3%. Assuming a flat radio spectrum $νL _ν\propto ν^{β+1} $ with $β$ = -1.0 for UCD flares, we construct a flare luminosity function $d N/d L \propto L^{-1.96 \pm 0.45}$ (here $L=νL_ν$). CRAFTS is found to be sensitive enough for flares from UCDs up to $\sim$180 pc. Considering the Galactic thin disk, we carry out a 3D Monte Carlo simulation of the UCD population, which is then fed to mock CRAFTS observations. We estimate that $\sim$170 flaring UCDs would be detected through transient searches in circular polarization. Though only marginally sensitive to the scale height of UCDs, the results are very sensitive to the assumed spectral index $β$. For $β$ from 0 to -2.5, the number of expected detections increases dramatically from $\sim$20 to $\sim$3460. We also contemplate the strategies for following up candidates of flaring UCDs, and discuss the implications of survey results for improving our knowledge of UCD behavior at $L$ band and dynamos.
description: 22 pages, 8 figures, 1 table
Enhancing the R Dev Guide: A GSoD 2022 Journey and Ongoing Progress
Creators: name: Bhogal, Saranjeet Kaur
name: Sancho, Lluís Revilla
Publisher: name: Zenodo
Year: 2024

description: A talk on "Enhancing the R Dev Guide: A GSoD 2022 Journey and Ongoing Progress" presented at useR! 2024 virtual on 2nd July 2024.
THE ROLE OF OXIDATIVE STRESS IN AMPA RECEPTOR TRAFFICKING FOLLOWING ISCHEMIC STROKE
Creators: name: Achzet, Lindsay
Publisher: name: Washington State University
Year: 2024

description: Stroke is a leading cause of disability and results in 140,000 deaths in the United States each year. Ischemic stroke occurs when blood flow to brain tissue is decreased or absent due to vessel occlusion, leading to infarction. While it is necessary to reintroduce blood flow to the infarcted area, this act also results in further damage to surrounding brain tissue by inflammation and oxidative stress, leading to delayed neuronal death within vulnerable neuronal populations, including hippocampal pyramidal neurons. During ischemia, the lack of energy available disrupts ATP-dependent processes that maintain ionic gradients, which are critical to cellular survival. Disrupting the ionic balance leads to excessive release of neurotransmitters, like glutamate, which are unable to effectively cleared from the synapses. Excessive stimulation of N-methyl-D-aspartate receptors (NMDARs) by glutamate is a contributing factor to delayed neuronal death, and multiple studies report that α-amino-3-hydroxy-5-methyl-4-isoxazolepropionic acid receptors (AMPARs) also contribute to delayed neuronal death. As a result of ischemia/reperfusion, AMPARs undergo a subunit composition switch from calcium-impermeable, GluA2-containing AMPARs, to calcium-permeable, GluA2-lacking AMPARs. This allows the AMPAR to conduct calcium which, in combination with excessive NMDAR stimulation, exacerbates cell death. We determined that there is a sex difference in the trafficking of AMPARs following oxygen glucose deprivation/reperfusion (OGD/R), an in vitro model for ischemia/reperfusion. GluA2-containing AMPARs are degraded by the lysosome in a calcium-dependent manner following OGD/R in male hippocampal slices, but AMPARs are not degraded in female hippocampal slices with OGD/R. Pharmacological inhibition of NADPH oxidase 1 rescues the OGD/R-induced degradation of GluA1 and GluA2 AMPAR subunits in males. Preventing the degradation of GluA2-containing AMPARs following ischemia/reperfusion has therapeutic implications in the treatment of stroke patients, so understanding the mechanisms at play are of utmost importance. In this dissertation I will discuss how OGD/R affects AMPARs in an ex vivo aged rodent acute hippocampal slice model and the role oxidative stress plays in the trafficking of these receptors.
An Interferometric View of H-MM1. I. Direct Observation of NH3 Depletion
Creators: name: Pineda, Jaime E.
name: Harju, Jorma
name: Caselli, Paola
name: Sipilä, Olli
name: Juvela, Mika
name: Vastel, Charlotte
name: Rosolowsky, Erik
name: Burkert, Andreas
name: Friesen, Rachel K.
name: Shirley, Yancy
name: Maureira, María José
name: Choudhury, Spandan
name: Segura-Cox, Dominique M.
name: Güsten, Rolf
name: Punanova, Anna
name: Bizzocchi, Luca
name: Goodman, Alyssa A.
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: Spectral lines of ammonia, NH$_3$, are useful probes of the physical conditions in dense molecular cloud cores. In addition to advantages in spectroscopy, ammonia has also been suggested to be resistant to freezing onto grain surfaces, which should make it a superior tool for studying the interior parts of cold, dense cores. Here we present high-resolution NH$_3$ observations with the Very Large Array (VLA) and Green Bank Telescope (GBT) towards a prestellar core. These observations show an outer region with a fractional NH$_3$ abundance of X(NH$_3$) = (1.975$\pm$0.005)$\times 10^{-8}$ ($\pm 10\%$ systematic), but it also reveals that after all, the X(NH$_3$) starts to decrease above a H$_2$ column density of $\approx 2.6 \times 10^{22}$ cm$^{-2}$. We derive a density model for the core and find that the break-point in the fractional abundance occurs at the density n(H$_2$) $\sim 2\times10^5$ cm$^{-3}$, and beyond this point the fractional abundance decreases with increasing density, following the power law $n^{-1.1}$. This power-law behavior is well reproduced by chemical models where adsorption onto grains dominates the removal of ammonia and related species from the gas at high densities. We suggest that the break-point density changes from core to core depending on the temperature and the grain properties, but that the depletion power law is anyway likely to be close to $n^{-1}$ owing to the dominance of accretion in the central parts of starless cores.
description: Accepted for publication in AJ. 18 Pages, 16 Figures, 3 Tables
Compatibility of muon $g-2$, $W$ mass anomaly in type-X 2HDM
Creators: name: Kim, Jongkuk
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recently CDF II Collaboration reported that they measured W boson mass precisely. The measurement is deviated from the Standard Model (SM) Prediction at 7$σ$. Also, the recent FNAL measurement of the muon magnetic moment shows a $4.2σ$ deviation. To resolve the W boson as well as the muon $(g-2)$ anomalies, we explore the type-X two Higgs doublet model (2HDM). We analyze the $(m_A, \tanβ)$ parameter space of the type-X 2HDM consistent with the muon $(g-2)$, lepton universality test and recent $W$ boson mass measurments from the CDF II collaboration. We find that the measurement of the $h\to AA$ branching ratio gives a strong lower mass bound on $m_H$.
description: 8 pages, 4figures
title: Sprachdynamik in Brasilien unter dem Einfluss afrikanischer Sprachen
Creators: name: Brückl, Christoph
Year: 2010

description: Mit der Ankunft der Portugiesen in Brasilien um 1500 war auch deren Sprache vielen linguistischen Einflüssen ausgesetzt. Durch diese Einflüsse entwickelte sie sich dort zu dem, was heute brasilianisches Portugiesisch, lingua brasileira (brasilianische Sprache) oder Brasilianisch genannt wird. In seiner neuen Umgebung wurde das Portugiesisch besonders von endogenen Tupí-Guaraní-Sprachen und von afrikanischen Sprachen beeinflusst. Der Einfluss der afrikanischen Sprachen auf das Portugiesisch lässt sich sowohl anhand lexikalischer als auch anhand grammatikalischer Vergleiche nachweisen. In den Bereichen Religion, Kultur und Nahrung, die für die Stiftung und Erhaltung einer kollektiven Identität eine zentrale Rolle spielen, ist dieser Einfluss in erhöhtem Ausmaß zu erwarten. Durch Analysieren und Vergleichen von Wortlisten brasilianischer Lexeme afrikanischen Ursprungs wird dieser Erwartung nachgegangen und überprüft, ob sie den Gegebenheiten entspricht. Einerseits sind im brasilianischen Lexikon afrikanische Präfixe – mit und ohne ihrer ursprünglich Bedeutung – zu finden, andererseits legen auch viele morphologische Prozesse im Brasilianisch einen afrikanischen Stimulus als Ursache für diese Prozesse nahe. Die afrikanischen Präfixe, die in den brasilianischen Wortschatz Eingang gefunden haben, sind anhand von Wortlisten leicht identifizierbar. Bei genauerer Betrachtung grammatikalischer Prozesse und Neuerungen wie der Bildung des Plurals oder der verbalen Flexion sind auch hier Parallelen zu afrikanischen Sprachen zu erkennen. Auch in der Phonologie und in der Phonetik können im Brasilianisch Eigenheiten aufgezeigt werden, die auch in afrikanischen Sprachen oder in Kreolsprachen in Afrika anzutreffen sind. Aus der Fülle dieser Informationen gilt es, den afrikanischen Stimulus auf die sprachliche Landschaft in Brasilien herauszufiltern und Raum für weitere linguistische Forschungen zu schaffen.
TOI-2046b, TOI-1181b and TOI-1516b, three new hot Jupiters from \textit{TESS}: planets orbiting a young star, a subgiant and a normal star
Creators: name: Kabáth, Petr
name: Chaturvedi, Priyanka
name: MacQueen, Phillip J.
name: Skarka, Marek
name: Šubjak, Ján
name: Esposito, Massimilliano
name: Cochran, William D.
name: Bellomo, Salvatore E.
name: Karjalainen, Raine
name: Guenther, Eike W.
name: Endl, Michael
name: Csizmadia, Szilárd
name: Karjalainen, Marie
name: Hatzes, Artie
name: Žák, Jiří
name: Gandolfi, Davide
name: Boffin, Henri M. J.
name: Vines, Jose I.
name: Livingston, John H.
name: García, Rafael A.
name: Mathur, Savita
name: González-Cuesta, Lucía
name: Blažek, Martin
name: Caldwell, Douglas A.
name: Colón, Knicole D.
name: Deeg, Hans
name: Erikson, Anders
name: Van Eylen, Vincent
name: Fong, William
name: Fridlund, Malcolm
name: Fukui, Akihiko
name: Fűrész, Gábor
name: Goeke, Robert F.
name: Goffo, Elisa
name: Howell, Steve
name: Jenkins, Jon M.
name: Klagyivik, Peter
name: Korth, Judith
name: Latham, David W.
name: Luque, Rafael
name: Moldovan, Dan
name: Murgas, Felipe
name: Narita, Norio
name: Orell-Miquel, Jaume
name: Palle, Enric
name: Parviainen, Hannu
name: Persson, Carina M.
name: Reed, Phillip A.
name: Redfield, Seth
name: Ricker, George R.
name: Seager, Sara
name: Serrano, Luisa Maria
name: Shporer, Avi
name: Smith, Alexis M. S.
name: Watanabe, Noriharu
name: Winn, Joshua N.
name: team, the KESPRINT
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the confirmation and characterization of three hot Jupiters, TOI-1181b, TOI-1516b, and TOI-2046b, discovered by the TESS space mission. The reported hot Jupiters have orbital periods between 1.4 and 2.05 days. The masses of the three planets are $1.18\pm0.14$ M$_{\mathrm{J}}$, $3.16\pm0.12$\, M$_{\mathrm{J}}$, and 2.30 $\pm 0.28$ M$_{\mathrm{J}}$, for TOI-1181b, TOI-1516b, and TOI-2046b, respectively. The stellar host of TOI-1181b is a F9IV star, whereas TOI-1516b and TOI-2046b orbit F main sequence host stars. The ages of the first two systems are in the range of 2-5 Gyrs. However, TOI-2046 is among the few youngest known planetary systems hosting a hot Jupiter, with an age estimate of 100-400 Myrs. The main instruments used for the radial velocity follow-up of these three planets are located at Ondřejov, Tautenburg and McDonald Observatory, and all three are mounted on 2-3 meter aperture telescopes, demonstrating that mid-aperture telescope networks can play a substantial role in the follow-up of gas giants discovered by \textit{TESS} and in the future by \textit{PLATO}.
description: MNRAS accepted
Tunneling Fundamentals, Practice And Innovations Annual Short Course - Special Session On University Transportation Infrastructure
Creators: name: Gutierrez, Marte
Publisher: name: Zenodo
Year: 2018
Subjects: Underground Transportation Infrastructure, Tunneling Sustainability Durability and lifetime Safety and reliability Resilience Technology transfer Education and outreach

description: Presentations from the Tunneling Fundamentals, Practice and Innovations Annual Short Course

- Special Session on University Transportation Infrastructure
A Generic Solution to Register-bounded Synthesis with an Application to Discrete Orders
Creators: name: Exibard, Léo
name: Filiot, Emmanuel
name: Khalimov, Ayrat
Publisher: name: arXiv
Year: 2022
Subjects: subject: Formal Languages and Automata Theory (cs.FL)
subject: FOS: Computer and information sciences

description: We study synthesis of reactive systems interacting with environments using an infinite data domain. A popular formalism for specifying and modelling such systems is register automata and transducers. They extend finite-state automata by adding registers to store data values and to compare the incoming data values against stored ones. Synthesis from nondeterministic or universal register automata is undecidable in general. However, its register-bounded variant, where additionally a bound on the number of registers in a sought transducer is given, is known to be decidable for universal register automata which can compare data for equality, i.e., for data domain $(N,=)$. This paper extends the decidability border to the domain $(N,<)$ of natural numbers with linear order. Our solution is generic: we define a sufficient condition on data domains (regular approximability) for decidability of register-bounded synthesis. The condition is satisfied by natural data domains like $(N,<)$. It allows one to use simple language-theoretic arguments and avoid technical game-theoretic reasoning. Further, by defining a generic notion of reducibility between data domains, we show the decidability of synthesis in the domain $(N^d,<^d)$ of tuples of numbers equipped with the component-wise partial order and in the domain $(Σ^*,\prec)$ of finite strings with the prefix relation.
description: submitted by accident; was intended as an update of arXiv:2105.09978
The VVV Open Cluster Project II. Near-infrared sequences of 37 open clusters on eight-dimensional parameter space
Creators: name: Ramírez, K. Peña
name: Smith, L. C.
name: Alegría, S. Ramírez
name: Chené, A. -N.
name: González-Fernández, C.
name: Lucas, P. W.
name: Minniti, D.
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: Open clusters are key coeval structures that help us understand star formation, stellar evolution and trace the physical properties of our Galaxy. In the past years, the isolation of open clusters from the field has been heavily alleviated by the access to accurate large-scale stellar parallaxes and proper motions along a determined line of sight. Still, there are limitations regarding their completeness since large-scale studies rely on optical wavelengths. Here we extend the open clusters sequences towards fainter magnitudes complementing the Gaia photometric and astrometric information with near-infrared data from the VVV survey. We performed a homogeneous analysis on 37 open clusters implementing two coarse-to-fine characterization methods: extreme deconvolution Gaussian mixture models coupled with an unsupervised machine learning method on 8-dimensional parameter space. The process allowed us to separate the clusters from the field at near-infrared wavelengths. We report an increase of $\sim$47\% new member candidates on average in our sample (considering only sources with high membership probability p$\geqq$0.9). This study is the second in a series intended to reveal open cluster near-infrared sequences homogeneously.
description: 16 pages. 5 figures. MNRAS accepted. v2: language edits and references updated at the proof stage; arXiv admin note: text overlap with arXiv:2102.04303