cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
New perspectives on MASCARA-1b: A combined analysis of pre- and post-eclipse emission data using CRIRES+
Creators: name: Ramkumar, Swaetha
name: Gibson, Neale P.
name: Nugroho, Stevanus K.
name: Fortune, Mark
name: Maguire, Cathal
Publisher: name: arXiv
Year: 2025
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present high-resolution emission spectroscopy observations of the ultra-hot Jupiter MASCARA-1b with CRIRES+ in the K-band, covering the post-eclipse phases of its orbit. These observations complement previously published pre-eclipse data. The stellar and telluric features were removed using SysRem, and the planetary signal was analysed with the cross-correlation technique. After confirming the presence of chemical species in our atmospheric model, we combined the pre- and post-eclipse datasets for a joint analysis. By employing a Bayesian retrieval framework, this joint retrieval enabled us to constrain the spatially varying temperature-pressure (T-P) profile and atmospheric carbon-to-oxygen (C/O) ratio. We detected strong emission signatures of CO and H$_2$O in the post-eclipse and combined datasets. While a well-mixed retrieval model results in a super-solar C/O, allowing for vertically varying chemistry yields C/O values consistent with solar. The retrieved parameters are not only consistent across the datasets but also across different chemical regimes. We did not identify any significant velocity shifts between the detected species or across the datasets, which could otherwise serve as proxies for possible atmospheric dynamics. We also explored phase dependence through the model scaling factor and found no substantial changes in atmospheric properties throughout the observed phases. Due to strong degeneracies between the temperature gradient and chemical abundances, our retrieved temperatures are broadly consistent with either a full redistribution of heat or strong day-night contrasts. While this complicates direct comparisons with recent Spitzer phase curve analyses suggesting inefficient recirculation, we find no clear evidence of spatial variation in the chemical or temperature structure of MASCARA-1b from pre- to post-eclipse, nor temporal variation over $\approx$2 years.
description: Accepted for publication in Astronomy & Astrophysics. 29 pages, 31 figures and 3 tables (including appendix)
Additional file 7 of SINE-derived satellites in scaled reptiles
Creators: name: Vassetzky, Nikita S.
name: Kosushkin, Sergei A.
name: Ryskov, Alexey P.
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Ecology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology

description: Additional file 7. Distribution of nucleotide positions of sSat2Gja with 10 middle monomers along Squam2 consensus sequence. Each position of all monomers was compared against Squam2 sequence and assigned a weight of 10 for a match; 1, for mismatch, and 0 for a gap. The cumulative statistics is presented. Abscissa: Squam2 consensus position; ordinate: total position weight.
DS_10.1177_0094582X19857170 – Supplemental material for The Fall of the Alberto Fujimori Government: New Evidence and Interpretations
Creators: name: Joo, Carlos Ugo Santander
name: Avila, Carlos Federico Domínguez
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 160607 International Relations
subject: FOS: Political science
subject: 120505 Regional Analysis and Development
subject: FOS: Social and economic geography

description: Supplemental material, DS_10.1177_0094582X19857170 for The Fall of the Alberto Fujimori Government: New Evidence and Interpretations by Carlos Ugo Santander Joo and Carlos Federico Domínguez Avila in Latin American Perspectives
A very young tau-Herculid meteor cluster observed during a 2022 shower outburst
Creators: name: Koten, Pavel
name: Čapek, David
name: Tóth, Juraj
name: Shrbený, Lukáš
name: Borovička, Jiří
name: Vaubaillon, Jeremie
name: Zander, Fabian
name: Buttsworth, David
name: Loehle, Stefan
Publisher: name: arXiv
Year: 2025
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: To date only very few meteor clusters have been instrumentally recorded. This means that every new detection is an important contribution to the understanding of these phenomena, which are thought to be evidence of the meteoroid fragmentation in the Solar System. On 31 May 2022, at 6:48:55 UT, a cluster consisting of 52 meteors was detected within 8.5 seconds during a predicted outburst of the tau-Herculid meteor shower. The aim of this paper is to reconstruct the atmospheric trajectories of the meteors and use the collected information to deduce the origin of the cluster. The meteors were recorded by two video cameras during an airborne campaign. Due to only the single station observation, their trajectories were estimated under the assumption that they belonged to the meteor shower. The mutual positions of the fragments, together with their photometric masses, was used to model the processes leading to the formation of the cluster. The physical properties of the cluster meteors are very similar to the properties of the tau-Herculids. This finding confirms the assumption of the shower membership used for the computation of atmospheric trajectories. This was the third cluster that we have studied in detail, but the first one where we do not see the mass separation of the particles. The cluster is probably less than 2.5 days old, which is too short for such a complete mass separation. Such an age would imply disintegration due to thermal stress. However, we cannot rule out an age of only a few hours, which would allow for other fragmentation mechanisms.
description: 9 pages, 7 figures, 4 tables, accepted for publication in A&A
A population synthesis study of the Gaia 100 pc unresolved white dwarf-main sequence binary population
Creators: name: Santos-García, Alejandro
name: Torres, Santiago
name: Rebassa-Mansergas, Alberto
name: Brown, Alex J.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Binary stars consisting of a white dwarf and a main sequence star (WDMS) are valuable for studying key astrophysical questions. However, observational biases strongly affect the known population, particularly unresolved systems where the main sequence star outshines the white dwarf. This work aims to comprehensively simulate the population of unresolved WDMS binaries within 100 pc of the Sun and to compare the outcome with the currently most complete volume-limited sample available from Gaia data. We employ a population synthesis code, MRBIN, extensively developed by our group and based on Monte Carlo techniques, which uses a standard binary stellar evolutionary code adapted to cover a wide range of stars across all ages, masses, and metallicities. Selection criteria matching those of Gaia observations are applied to generate synthetic populations comparable to the observed WDMS sample. The synthetic data accurately populate the expected regions in the Gaia color-magnitude diagram. However, simulations predict a lower number of extremely low-mass white dwarfs, suggesting potential issues in observed mass derivations. Additionally, our analysis constrains the common envelope efficiency to 0.1-0.4, consistent with previous findings, and estimates a total completeness of about 25% for the observed sample, confirming the strong observational limitations for unresolved WDMS.
description: 17 pages, 11 figures, 2 tables; accepted for publication in A&A
Additional file 8 of SINE-derived satellites in scaled reptiles
Creators: name: Vassetzky, Nikita S.
name: Kosushkin, Sergei A.
name: Ryskov, Alexey P.
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Ecology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology

description: Additional file 8. Variation of orthologous sSat3SRP loci in two snakes, southwestern speckled rattlesnake Crotalus pyrrhus and prairie rattlesnake Crotalus viridis. A. Distribution of orthologous sSat3SRP loci by difference in the number of tandem repeat units. B. Examples of orthologous sSat3SRP loci in C. pyrrhus and C. viridis genomes. The red arrows indicate the repeat units, while the green and blue ones correspond to the 5′ and 3′ ends of Squam3 SINE. No flanking genomic sequences are shown. Genomic affiliations are given above diagrams.
Density fluctuation in the solar corona and solar wind: A comparative analysis of radio-occultation observations and magnetohydrodynamic simulation
Creators: name: Chiba, Shota
name: Shoda, Munehito
name: Imamura, Takeshi
Publisher: name: arXiv
Year: 2025
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Recent in-situ observations and numerical models indicated various types of magnetohydrodynamic (MHD) waves contributing to the solar wind acceleration. Among them is an MHD wave decomposition at distances closer than 50 $R_{\odot}$ using data taken by the first perihelion pass of Parker Solar Probe (PSP). However, the underlying physical processes responsible for the formation of the solar wind have not yet been observationally confirmed at distances closer than 10 $R_{\odot}$. We aim to infer the mode population of density fluctuations observed by radio occultation, which has all been attributed to slow magnetoacoustic waves. We compare the radio occultation observations conducted in 2016 using the JAXA's Venus orbiter Akatsuki with the MHD simulation. The time-frequency analysis was applied to the density fluctuations observed by the radio occultation and those reproduced in the MHD model. The time-spatial spectrum of the density fluctuation in the model exhibits two components that are considered to be fast and slow magnetoacoustic waves. The fast magnetoacoustic waves in the model tend to have periods shorter than the slow magnetoacoustic waves, and the superposition of these modes has a broadened spectrum extending in the range of approximately 20$-$1000 s, which resembles that of the observed waves. Based on this comparison, it is probable that the density oscillations observed by radio occultation include fast and slow magnetoacoustic waves, and that fast magnetoacoustic waves are predominant at short periods and slow magnetoacoustic waves are prevalent at long periods. This is qualitatively similar to the results of the mode decomposition obtained from the PSP's first perihelion at more distance regions.
The bulge globular cluster Terzan 6 as seen from multi-conjugate adaptive optics and HST
Creators: name: Loriga, Martina
name: Pallanca, Cristina
name: Ferraro, Francesco R.
name: Dalessandro, Emanuele
name: Lanzoni, Barbara
name: Cadelano, Mario
name: Origlia, Livia
name: Fanelli, Cristiano
name: Geisler, Douglas
name: Villanova, Sandro
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: This work consists of the first detailed photometric study of Terzan 6, one of the least known globular clusters in the Galactic bulge. Through the analysis of high angular resolution and multi-wavelength data obtained from adaptive optics corrected and space observations, we built deep, optical and near-infrared color-magnitude diagrams reaching $\approx 4$ magnitudes below the main-sequence turnoff. Taking advantage of 4 different epochs of observations, we measured precise relative proper motions for a large sample of stars, from which cluster members have been solidly distinguished from Galactic field interlopers. A non-canonical reddening law (with $R_V=2.85$) and high-resolution differential reddening map, with color excess variations up to $δE(B-V) \approx 0.8 $ mag, have been derived in the direction of the system. According to these findings, new values of the extinction and distance modulus have been obtained: respectively, $E(B-V)=2.36\pm0.05$ and $(m-M)_0=14.46 \pm 0.10$ (corresponding to $d=7.8 \pm 0.3$ kpc). We also provide the first determinations of the cluster center and projected density profile from resolved star counts. The center is offset by more than $7$ arcsec to the east from the literature value, and the structural parameters obtained from the King model fitting to the density profile indicate that Terzan 6 is in an advanced stage of its dynamical evolution. We also determined the absolute age of the system, finding $t=13\pm 1 $ Gyr, in agreement with the old ages found for the globular clusters in the Galactic bulge. From the re-determination of the absolute magnitude of the red giant branch bump and the recent estimate of the cluster global metallicity, we find that Terzan 6 nicely matches the tight relation between these two parameters drawn by the Galactic globular cluster population.
description: Accepted for publication in A&A
Additional file 9 of SINE-derived satellites in scaled reptiles
Creators: name: Vassetzky, Nikita S.
name: Kosushkin, Sergei A.
name: Ryskov, Alexey P.
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Ecology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology

description: Additional file 9. Sequence alignment of Squam1 SINE and sSat1Aca repeat unit from the green anole Anolis carolinensis.
Unveiling the warm molecular outflow component of type-2 quasars with SINFONI
Creators: name: Zanchettin, M. V.
name: Almeida, C. Ramos
name: Audibert, A.
name: Acosta-Pulido, J. A.
name: Cezar, P. H.
name: Hicks, E.
name: Lapi, A.
name: Mullaney, J.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present seeing-limited (0.8 arcsec) near-infrared integral field spectroscopy data of the type-2 quasars (QSO2s) SDSS J135646.10+102609.0 (J1356) and SDSS J143029.89+133912.1 (J1430, the Teacup), both belonging to the Quasar Feedback (QSOFEED) sample. The nuclear K-band spectra (1.95-2.45 \textmu m) of these radio-quiet QSO2s reveal several $H_2$ emission lines, indicative of the presence of a warm molecular gas reservoir (T$\geq$1000 K). We measure nuclear masses of 5.9, 4.1, and 1.5 $\times 10^3~M_{\odot}$ in the inner 0.8 arcsec diameter region of the Teacup, J1356 north (J1356N), and south nuclei, respectively. The total warm $H_2$ mass budget is $\sim 4.5$ and $\sim 1.3 \times 10^4~M_{\odot}$ for the Teacup and J1356N, implying warm-to-cold molecular gas ratios of $10^{-6}$. The warm molecular gas kinematics, traced with the $H_2$1-0S(1) and S(2) emission lines, is consistent with that of the cold molecular phase, traced by ALMA CO emission at higher angular resolution (0.2 and 0.6 arcsec). In J1430, we detect the blue- and red-shifted sides of a compact warm molecular outflow extending up to 1.9 kpc and with velocities of 450 km/s. In J1356 only the red-shifted side is detected, with a radius of up to 2.0 kpc and velocity of 370 km/s. The outflow masses are 2.6 and 1.5 $\times 10^3~M_{\odot}$ for the Teacup and J1356N, and the warm-to-cold gas ratios in the outflows are 0.8 and 1 $\times 10^{-4}$, implying that the cold molecular phase dominates the mass budget. We measure warm molecular mass outflow rates of 6.2 and 2.9 $\times 10^{-4}~M_{\odot}/yr$ for the Teacup and J1356N, approximately 0.001\% of the total mass outflow rate. We find an enhancement of velocity dispersion in the $H_2$1-0S(1) residual dispersion map of the Teacup, both along and perpendicular to the compact radio jet direction. This enhanced turbulence can be reproduced by simulations of jet-ISM interactions.
description: Accepted for publication on A&A
Robust machine learning model of inferring the ex-situ stellar fraction of galaxies from photometric data
Creators: name: Cai, Runsheng
name: Zhu, Ling
name: Shen, Shiyin
name: Wang, Wenting
name: Pillepich, Annalisa
name: Falcón-Barroso, Jesús
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We search for parameters defined from photometric images to quantify the ex situ stellar mass fraction of galaxies. We created mock images using galaxies in the cosmological hydrodynamical simulations TNG100, EAGLE, and TNG50 at redshift $z=0$. We define a series of parameters describing their structures. In particular, the inner and outer halo of a galaxy are defined by sectors ranging from $45-135$ degrees from the disk major axis, and with radii ranging from $3.5-10$ kpc and $10-30$ kpc, respectively, to avoid the contamination of disk and bulge. The surface brightness and colour gradients are defined by the same sectors along the minor axis and with similar radii ranges. We used the Random Forest method to create a model that predicts $f_{\rm exsitu}$ from morphological parameters. The model predicts $f_{\rm exsitu}$ well with a scatter smaller than 0.1 compared to the ground truth in all mass ranges. The models trained from TNG100 and EAGLE work similarly well and are cross-validated; they also work well in making predictions for TNG50 galaxies. The analysis using Random Forest reveals that $\nabla ρ_{\rm outer}$, $\nabla (g-r)_{\rm outer}$, $f_{\rm outerhalo}$ and $f_{\rm innerhalo}$ are the most influential parameters in predicting $f_{\rm exsitu}$, underscoring their significance in uncovering the merging history of galaxies. We further analyse how the quality of images will affect the results by using SDSS-like and HSC-like mock images for galaxies at different distances. Our results can be used to infer the ex situ stellar mass fractions for a large sample of galaxies from photometric surveys.
description: Accepted in A&A
Astrometry, orbit determination, and thermal inertia of the Tianwen-2 target asteroid (469219) Kamo`oalewa
Creators: name: Fenucci, Marco
name: Novaković, Bojan
name: Zhang, Pengfei
name: Carbognani, Albino
name: Micheli, Marco
name: Faggioli, Laura
name: Gianotto, Francesco
name: Ocaña, Francisco
name: Föhring, Dora
name: Cano, Juan Luis
name: Conversi, Luca
name: Moissl, Richard
Publisher: name: arXiv
Year: 2025
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Context. (469219) Kamo`oalewa is a small near-Earth asteroid, which is currently a quasi-satellite of the Earth. Lightcurve measurements also reveal a rotation period of only about 30 minutes. This asteroid has been selected as the target of the Tianwen-2 sample-return mission of the China National Space Administration.
 Aims. The first goal of this paper is to observe and improve the orbit determination of (469219) Kamo`oalewa, and better determine the Yarkovsky effect acting on it. The second goal is to estimate the thermal inertia of the asteroid, taking advantage of an improved Yarkovsky effect determination.
 Methods. Our observational campaign imaged the asteroid from the Loiano Astronomical Station and from the Calar Alto Observatory, in March 2024. We also accurately re-measured a precovery detection from the Sloan Digital Sky Survey from 2004. New astrometry was later used in a 7-dimensional orbit determination, aimed at estimating both the orbital elements and the Yarkovsky effect. Thermal inertia is later studied by using the ASTERIA, a new method that is suitable to estimate thermal inertia of small asteroids.
 Results. We detected a semi-major axis drift of $(-67.35 \pm 4.70) \times 10^{-4}$ au My$^{-1}$ due to the Yarkovsky effect, with a high signal-to-noise ratio of 14. The new orbit solution also significantly reduced the position uncertainty for the arrival of the Tianwen-2 spacecraft. By using different models for the physical parameters of Kamo`oalewa, the ASTERIA model estimated the thermal inertia at $Γ= 150^{+90}_{-45}$ J m$^{-2}$ K$^{-1}$ s$^{-1/2}$ or $Γ= 181^{+95}_{-60}$ J m$^{-2}$ K$^{-1}$ s$^{-1/2}$.
description: Accepted for publication in Astronomy & Astrophysics
Supplemental_Material – Supplemental material for An innovative SMS intervention to improve adherence to stimulants in children with ADHD: Preliminary findings
Creators: name: Fried, Ronna
name: DiSalvo, Maura
name: Kelberman, Caroline
name: Adler, Amos
name: McCafferty, Debra
name: K Yvonne Woodworth
name: Green, Allison
name: Biederman, Itai
name: Faraone, Stephen V
name: Biederman, Joseph
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 110904 Neurology and Neuromuscular Diseases
subject: FOS: Clinical medicine
subject: 111599 Pharmacology and Pharmaceutical Sciences not elsewhere classified
subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology
subject: 110319 Psychiatry (incl. Psychotherapy)

description: Supplemental material, Supplemental_Material for An innovative SMS intervention to improve adherence to stimulants in children with ADHD: Preliminary findings by Ronna Fried, Maura DiSalvo, Caroline Kelberman, Amos Adler, Debra McCafferty, K Yvonne Woodworth, Allison Green, Itai Biederman, Stephen V Faraone and Joseph Biederman in Journal of Psychopharmacology
Catching the wisps: Stellar mass-loss limits from low-frequency radio observations
Creators: name: Bloot, Sanne
name: Vedantham, Harish K.
name: Kavanagh, Robert D.
name: Callingham, Joseph R.
name: Pope, Benjamin J. S.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The winds of low-mass stars carry away angular momentum and impact the atmospheres of surrounding planets. Determining the properties of these winds is necessary to understand the mass-loss history of the star and the evolution of exoplanetary atmospheres. Due to their tenuous nature, the winds of low-mass main-sequence stars are difficult to detect. The few existing techniques for measuring these winds are indirect, with the most common inference method for winds of low-mass stars being astrospheric Lyman-$α$ absorption combined with complex hydrodynamical modelling of the interaction between the stellar wind and the interstellar medium. Here, we employ a more direct method to place upper limits on the mass-loss rates of low-mass stars by combining observations of low-frequency coherent radio emission, the lack of free-free absorption, and a simple stellar wind model. We determine upper limits on the mass-loss rate for a sample of 19 M dwarf stars detected with the LOFAR telescope at 120--168 MHz, reaching a sensitivity within an order of magnitude of the solar mass-loss rate for cold stars with a surface magnetic field strength of $\sim$100 G. The sensitivity of our method does not depend on distance or spectral type, allowing us to find mass-loss rate constraints for stars up to spectral type M6 and out to a distance of 50 pc, later and farther than previous measurements. With upcoming low-frequency surveys with both LOFAR and the Square Kilometre Array, the number of stars with mass-loss rate upper limits determined with this method could reach $\sim$1000.
description: Accepted for publication in A&A
JTE_AppendixA_8_30_19_final – Supplemental material for Examining Certification Requirements in Early Math and Literacy: What Do States Expect Prekindergarten Teachers to Know?
Creators: name: Wright, Tanya S.
name: Parks, Amy Noelle
name: Wilinski, Bethany
name: Domke, Lisa M.
name: Hopkins, Laura J.
Publisher: name: SAGE Journals
Year: 2020
Subjects: Education

description: Supplemental material, JTE_AppendixA_8_30_19_final for Examining Certification Requirements in Early Math and Literacy: What Do States Expect Prekindergarten Teachers to Know? by Tanya S. Wright, Amy Noelle Parks, Bethany Wilinski, Lisa M. Domke and Laura J. Hopkins in Journal of Teacher Education
Additional file 1 of Development and validation of chemometric-assisted spectrophotometric models for efficient quantitation of a binary mixture of supportive treatments in COVID-19 in the presence of its toxic impurities: a comparative study for eco-friendly assessment
Creators: name: Abd El-Hadi, Heidi R.
name: Eissa, Maya S.
name: Zaazaa, Hala E.
name: Eltanany, Basma M.
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified

description: Additional file 1. Fig. S1: Chemical structure of (a) paracetamol, (b) hyoscine butylbromide, (c) p-aminophenol, (d) p-nitrophenol, (e) p-chloractanilide and (f) tropic acid.
Additional file 2 of Efficient design of synthetic gene circuits under cell-to-cell variability
Creators: name: Turpin, Baptiste
name: Bijman, Eline Y.
name: Kaltenbach, Hans-Michael
name: Stelling, Jörg
Publisher: name: figshare
Year: 2024
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 2: Figure S1. Viable samples in the population parameter space, scalar covariance matrix, obtained with the naive method. Symbols as Fig. 4A.
MSJ851245_Supplementary_file_1 – Supplemental material for Reproductive history of the Danish multiple sclerosis population: A register-based study
Creators: name: Moberg, Julie Yoon
name: Laursen, Bjarne
name: Thygesen, Lau Caspar
name: Magyari, Melinda
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 110904 Neurology and Neuromuscular Diseases
subject: FOS: Clinical medicine
subject: 111702 Aged Health Care
subject: FOS: Health sciences

description: Supplemental material, MSJ851245_Supplementary_file_1 for Reproductive history of the Danish multiple sclerosis population: A register-based study by Julie Yoon Moberg, Bjarne Laursen, Lau Caspar Thygesen and Melinda Magyari in Multiple Sclerosis Journal
Additional file 3 of Efficient design of synthetic gene circuits under cell-to-cell variability
Creators: name: Turpin, Baptiste
name: Bijman, Eline Y.
name: Kaltenbach, Hans-Michael
name: Stelling, Jörg
Publisher: name: figshare
Year: 2024
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 3: Figure S2. Viable samples in the population parameter space, diagonal covariance matrix. Samples in all two-dimensional projections of the parameter space, obtained with the SLMCMC algorithm. Orange dots: viable samples for the threshold on the individual cost $$\varepsilon = 6\,\textrm{nM}$$ ε = 6 nM ; red dots: viable samples for $$\varepsilon = 3\,\textrm{nM}$$ ε = 3 nM ; black dots: populations with cost $$c(\gamma ) > 0.2$$ c ( γ ) > 0.2 , representing less than 4.5% of samples. All parameters are in $$\hbox {log}_{10}$$ log 10 -scale.
Supplemental_material_B – Supplemental material for Monuments and economies: What drove their variability in the middle-Holocene Neolithic?
Creators: name: Brozio, Jan Piet
name: Müller, Johannes
name: Furholt, Martin
name: Kirleis, Wiebke
name: Dreibrodt, Stefan
name: Feeser, Ingo
name: Dörfler, Walter
name: Weinelt, Mara
name: Raese, Hendrik
name: Bock, Annalena
Publisher: name: SAGE Journals
Year: 2019
Subjects: Geography
History

description: Supplemental material, Supplemental_material_B for Monuments and economies: What drove their variability in the middle-Holocene Neolithic? by Jan Piet Brozio, Johannes Müller, Martin Furholt, Wiebke Kirleis, Stefan Dreibrodt, Ingo Feeser, Walter Dörfler, Mara Weinelt, Hendrik Raese and Annalena Bock in The Holocene
Identification and characterisation of the gamma-ray counterpart of the transitional pulsar candidate CXOU J110926.4-650224
Creators: name: Manca, A.
name: Zelati, F. Coti
name: Li, J.
name: Torres, D. F.
name: Ballet, J.
name: Marino, A.
name: Sanna, A.
name: Rea, N.
name: Di Salvo, T.
name: Riggio, A.
name: Burderi, L.
name: Iaria, R.
Publisher: name: arXiv
Year: 2025
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Transitional millisecond pulsars (tMSPs) represent a crucial link between the rotation-powered and accretion-powered states of binary pulsars. During their active X-ray state, tMSPs are the only low-mass X-ray binary systems detected up to GeV energies by the Fermi Large Area Telescope (LAT). CXOU J110926.4-650224 is a newly discovered tMSP candidate in an active X-ray state, potentially spatially compatible with a faint gamma-ray source listed in the latest Fermi-LAT point-source catalogue as 4FGL J1110.3-6501. Confirming the association between CXOU J110926.4-650224 and the Fermi source is a key step toward validating its classification as a tMSP. In this study, we analyse Fermi-LAT data collected from August 2008 to June 2023 to achieve a more accurate localisation of the gamma-ray source, characterise its spectral properties, and investigate potential time variability. By thoroughly reconstructing the gamma-ray background around the source using a weighted likelihood model, we obtain a new localisation that aligns with the position of the X-ray source at the 95% confidence level, with a Test Statistic value of $\sim 42$. This establishes a spatial association between the gamma-ray source and CXOU J110926.4-650224. The gamma-ray emission is adequately described by a power-law model with a photon index of $Γ= 2.5 \pm 0.1$ and a corresponding flux of $(3.7\pm0.9) \times 10^{-12}$ erg cm$^{-2}$ s$^{-1}$ in the 0.1-300 GeV range.
description: 7 pages, 6 figures. Accepted for publication by Astronomy&Astrophysics
Supplemental Material, Supplemental_File - Tic Suppression in Children With Recent-Onset Tics Predicts 1-Year Tic Outcome
Creators: name: Soyoung Kim
name: Greene, Deanna J.
name: Robichaux-Viehoever, Amy
name: Bihun, Emily C.
name: Koller, Jonathan M.
name: Acevedo, Haley
name: Schlaggar, Bradley L.
name: Black, Kevin J.
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 110904 Neurology and Neuromuscular Diseases
subject: FOS: Clinical medicine
subject: 111403 Paediatrics
subject: Neuroscience

description: Supplemental Material, Supplemental_File for Tic Suppression in Children With Recent-Onset Tics Predicts 1-Year Tic Outcome by Soyoung Kim, Deanna J. Greene, Amy Robichaux-Viehoever, Emily C. Bihun, Jonathan M. Koller, Haley Acevedo, Bradley L. Schlaggar and Kevin J. Black in Journal of Child Neurology
Additional file 1 of Using fuzzy logic to compare species distribution models developed on the basis of expert knowledge and sampling records
Creators: name: Romero, David
name: Maneyro, Raúl
name: Guerrero, José Carlos
name: Real, Raimundo
Publisher: name: figshare
Year: 2024
Subjects: subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Science Policy
subject: Plant Biology

description: Additional file 1: Table S1 shows the list of amphibian species analysed in Uruguay, including the IUCN threat category.
Mastering the growth of antimonene on Bi2Se3: strategies and insights
Creators: name: Flammini, Roberto
name: Hogan, Conor
name: Colonna, Stefano
name: Ronci, Fabio
name: Satta, Mauro
name: Papagno, Marco
name: Aliev, Ziya S.
name: Eremeev, Sergey V.
name: Chulkov, Evgueni V.
name: Benher, Zipporah R.
name: Gardonio, Sandra
name: Petaccia, Luca
name: Di Santo, Giovanni
name: Carbone, Carlo
name: Moras, Paolo
name: Sheverdyaeva, Polina M.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Antimonene, the two-dimensional phase of antimony, appears in two distinct allotropes when epitaxially grown on Bi2Se3: the puckered asymmetric washboard (α) and buckled honeycomb (β) bilayer structures. As-deposited antimony films exhibit varying proportions of single α and β structures. We identify the conditions necessary for ordered, pure-phase growth of single to triple β-antimonene bilayers. Additionally, we determine their electronic structure, work function, and characteristic core-level binding energies, offering an explanation for the relatively large chemical shifts observed among the different phases. This study not only establishes a protocol for achieving a single β phase of antimonene but also provides key signatures for distinguishing between the different allotropes using standard spectroscopic and microscopic techniques.
description: 9 pages, 4 figures, 77 references
Additional file 2 of Using fuzzy logic to compare species distribution models developed on the basis of expert knowledge and sampling records
Creators: name: Romero, David
name: Maneyro, Raúl
name: Guerrero, José Carlos
name: Real, Raimundo
Publisher: name: figshare
Year: 2024
Subjects: subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Science Policy
subject: Plant Biology

description: Additional file 2: Figure S1 shows the results of the Kruskal–Wallis test comparing the discrimination and classification abilities for threatened (T), non-threatened and non-ubiquitous (NtNu) and ubiquitous species (U) of the models based on expert knowledge and species records, respectively. Figure S2 compares the average number of factors, average number of variables and entropy values of the models based on expert knowledge and species records.
Supplementary_Information – Supplemental material for Synthesis, cytotoxicity evaluation, and molecular modeling studies of 2,N10-substituted acridones as DNA-intercalating agents
Creators: name: Nisachon Khunnawutmanotham
name: Watthanachai Jumpathong
name: Chatchakorn Eurtivong
name: Nitirat Chimnoi
name: Supanna Techasakul
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental material, Supplementary_Information for Synthesis, cytotoxicity evaluation, and molecular modeling studies of 2,N10-substituted acridones as DNA-intercalating agents by Nisachon Khunnawutmanotham, Watthanachai Jumpathong, Chatchakorn Eurtivong, Nitirat Chimnoi and Supanna Techasakul in Journal of Chemical Research
Strong constraints on self-interacting dark matter with light mediators
Creators: name: Bringmann, Torsten
name: Kahlhoefer, Felix
name: Schmidt-Hoberg, Kai
name: Walia, Parampreet
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2016
Subjects: dark matter: annihilation
dark matter: coupling
production: thermal
cosmic background radiation
velocity dependence
new particle
mediation
formation
structure

description: Coupling dark matter to light new particles is an attractive way to combine thermal production with strong velocity-dependent self-interactions. Here we point out that in such models the dark matter annihilation rate is generically enhanced by the Sommerfeld effect, and we derive the resulting constraints from the Cosmic Microwave Background and other indirect detection probes. For the frequently studied case of s-wave annihilation these constraints exclude the entire parameter space where the self-interactions are large enough to address the small-scale problems of structure formation.
DS_10.1177_0022034520901709 – Supplemental material for Socioeconomic Life Course Models and Oral Health: A Longitudinal Analysis
Creators: name: R.K. Celeste
name: H.S. Eyjólfsdóttir
name: C. Lennartsson
name: J. Fritzell
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 110599 Dentistry not elsewhere classified
subject: FOS: Clinical medicine
subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental material, DS_10.1177_0022034520901709 for Socioeconomic Life Course Models and Oral Health: A Longitudinal Analysis by R.K. Celeste, H.S. Eyjólfsdóttir, C. Lennartsson and J. Fritzell in Journal of Dental Research
JuSER – Volltextrepositorium und mehr
Creators: name: Mittermaier, B.
name: Wagner, A.
name: Barake, L.
name: Diallo, A. S.
name: Hesselbach, S.
name: Pazera, Tomasz
name: Plott, Cornelia
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2013

description: Open Access Tage 2013, OAT 2013, Hamburg, Staats- und Universitätsbibliothek Hamburg, Germany, 1 Oct 2013 - 2 Oct 2013
description: 1.5 minutes of madness: Kurzvorstellung des Posters zu JuSER
IMPLEMENTATION OF THE SPACED LEARNING METHOD INTO TEACHING PROCESS
Creators: name: Ismailova, Dildora
Publisher: name: Zenodo
Year: 2024

description: This article highlights the importance of strengthening memory which is the main factor in effective learning process. The language learning is both sophisticated and interesting process that helps learners obtain new knowledge, broaden a horizon, boost language acquisition and gift new opportunities for their future career. The article gives information about challenges that occur while learning L2 language that can be overcome owing to innovative methods including “Spaced learning”.
STROBE_checklist_ – Supplemental material for Improving Hashimoto’s thyroiditis by eradicating Blastocystis hominis: Relation to IL-177
Creators: name: El-Zawawy, Hanaa Tarek
name: Farag, Huda Fahmy
name: Tolba, Mona Mohamed
name: Abdalsamea, Hanaa Abdalbasit
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 110306 Endocrinology
subject: FOS: Clinical medicine
subject: 111403 Paediatrics
subject: 111599 Pharmacology and Pharmaceutical Sciences not elsewhere classified

description: Supplemental material, STROBE_checklist_ for Improving Hashimoto’s thyroiditis by eradicating Blastocystis hominis: Relation to IL-177 by Hanaa Tarek El-Zawawy, Huda Fahmy Farag, Mona Mohamed Tolba and Hanaa Abdalbasit Abdalsamea in Therapeutic Advances in Endocrinology and Metabolism
Phantom RN-AdS black holes in noncommutative space
Creators: name: Hamil, B.
name: Lütfüoğlu, B. C.
Publisher: name: arXiv
Year: 2025
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We analyze the effects of noncommutativity on phantom Reissner-Nordström-Anti-de Sitter black holes by modeling mass and charge distributions with Lorentzian profiles. The modified metric function exhibits significant deviations from the classical case, leading to changes in the horizon structure and the suppression of singularities. Through a comparative thermodynamic analysis, we derive expressions for the mass, Hawking temperature, entropy, and heat capacity, identifying stability conditions and phase transitions induced by noncommutative corrections. The efficiency of the black hole as a heat engine is evaluated, showing that noncommutativity influences the thermodynamic cycle differently in the presence of phantom fields. Furthermore, we investigate the orbital motion of test particles and photons, deriving the effective potential, innermost stable circular orbits, and the shadow profile. Finally, we compute quasinormal modes to assess dynamical stability, revealing that noncommutativity modifies the damping behavior and introduces a new branch of non-oscillatory modes, absent in the classical case. Our findings provide a deeper understanding of the interplay between phantom fields, noncommutative geometry, and black hole thermodynamics, offering potential observational signatures for exotic compact
description: Submitted to EPJC, 30 pages, 14 Figures, 4 Tables
JuSER – Volltextrepositorium und mehr
Creators: name: Mittermaier, B.
name: Wagner, A.
name: Barake, L.
name: Diallo, A. S.
name: Hesselbach, S.
name: Pazera, Tomasz
name: Plott, Cornelia
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2013

description: Open Access Tage 2013, OAT 2013, Hamburg, Staats- und Universitätsbibliothek Hamburg, Germany, 1 Oct 2013 - 2 Oct 2013
description: JuSER ist die Jülicher Instanz der gemeinsam mit dem Deutschen Elektronensyncrotron (DESY, Hamburg), der Gesellschaft für Schwerionenforschung (GSI, Darmstadt), der RWTH Aachen und der Maier-Leibnitz-Zentrum (MLZ, München) entwickelten Publikationsdatenbank.
IPS809106_French_Spanish – Supplemental material for Majoritarian systems, rural groups, and (arrested) welfare state development
Creators: name: Knutsen, Carl Henrik
name: Rasmussen, Magnus Bergli
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 160607 International Relations
subject: FOS: Political science

description: Supplemental material, IPS809106_French_Spanish for Majoritarian systems, rural groups, and (arrested) welfare state development by Carl Henrik Knutsen and Magnus Bergli Rasmussen in International Political Science Review
The Helmholtz INVENIO Repository Project: Between Organizational Tasks, Needs of Scientists, and Constraints
Creators: name: Große, Katrin
name: Wagner, Alexander
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2014

description: International Semiar on Applications of Communication and Information Technology in Library, SACITiL-2014, Kolkata, Variable Energy Cyclotron Center, India, 28 Jan 2014 - 30 Jan 2014
description: To accomodate the growing needs for publication databases stemming from scientific evaluation requirements as well as the growing requirements for open access repositories, the libraries of the Helmholtz centres DESY (Hamburg), Froschungszentrum Jülich, GSI (Darmstadt) together with the university library of RWTH Aachen decided to join forces and to migrate their existing solutions to Invenio. With the flexiblity of Marc21 in mind, the choosen apporach tries to accomodate various, at first sight diverging, needs reusing the host of fuctionalities already existing within Invenio. One main goal of the project was to ease up "cataloguing" to a level where it can easily be handled by non-library staff (e.g. secretaries) while still maintaining a high standard of metadata quality. This is accomplished by introducing Marc Authority throughout the system and using these records extensively during input as well as later on for statistical purposes. Additionally, the unification of publication databases as well as the open access repository tries to increase the visibility of research and ease up access to its results. To this end interfaces to content management systems were created.
Additional file 3 of Using fuzzy logic to compare species distribution models developed on the basis of expert knowledge and sampling records
Creators: name: Romero, David
name: Maneyro, Raúl
name: Guerrero, José Carlos
name: Real, Raimundo
Publisher: name: figshare
Year: 2024
Subjects: subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Science Policy
subject: Plant Biology

description: Additional file 3: Figure S3 represents cartographically the occurrences and favourability model values for all amphibian species analyzed in Uruguay according to expert criteria and to species records.
IPS808610_supplemetary_note – Supplemental material for Too big to fault? Effects of the 2010 Nobel Peace Prize on Norwegian exports to China and foreign policy
Creators: name: Kolstad, Ivar
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 160607 International Relations
subject: FOS: Political science

description: Supplemental material, IPS808610_supplemetary_note for Too big to fault? Effects of the 2010 Nobel Peace Prize on Norwegian exports to China and foreign policy by Ivar Kolstad in International Political Science Review
DS_10.1177_0022034520906384 – Supplemental material for Topical Fluoride to Prevent Root Caries: Systematic Review with Network Meta-analysis
Creators: name: J. Zhang
name: D. Sardana
name: K.Y. Li
name: K.C.M. Leung
name: E.C.M. Lo
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 110599 Dentistry not elsewhere classified
subject: FOS: Clinical medicine
subject: 91299 Materials Engineering not elsewhere classified
subject: FOS: Materials engineering

description: Supplemental material, DS_10.1177_0022034520906384 for Topical Fluoride to Prevent Root Caries: Systematic Review with Network Meta-analysis by J. Zhang, D. Sardana, K.Y. Li, K.C.M. Leung and E.C.M. Lo in Journal of Dental Research
Online_supplement_Values_trust_education_-_revised3 – Supplemental material for Democratic values, education, and political trust
Creators: name: Kołczyńska, Marta
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: Sociology
subject: FOS: Sociology

description: Supplemental material, Online_supplement_Values_trust_education_-_revised3 for Democratic values, education, and political trust by Marta Kołczyńska in International Journal of Comparative Sociology
Online_Appendix_2 – Supplemental material for Gaming alone: Videogaming and sociopolitical attitudes
Creators: name: Bacovsky, Pavel
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 200199 Communication and Media Studies not elsewhere classified
subject: FOS: Media and communications

description: Supplemental material, Online_Appendix_2 for Gaming alone: Videogaming and sociopolitical attitudes by Pavel Bacovsky in New Media & Society
Interpretable High-order Knowledge Graph Neural Network for Predicting Synthetic Lethality in Human Cancers
Creators: name: Chen, Xuexin
name: Cai, Ruichu
name: Huang, Zhengting
name: Li, Zijian
name: Zheng, Jie
name: Wu, Min
Publisher: name: arXiv
Year: 2025
Subjects: subject: Machine Learning (cs.LG)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: Synthetic lethality (SL) is a promising gene interaction for cancer therapy. Recent SL prediction methods integrate knowledge graphs (KGs) into graph neural networks (GNNs) and employ attention mechanisms to extract local subgraphs as explanations for target gene pairs. However, attention mechanisms often lack fidelity, typically generate a single explanation per gene pair, and fail to ensure trustworthy high-order structures in their explanations. To overcome these limitations, we propose Diverse Graph Information Bottleneck for Synthetic Lethality (DGIB4SL), a KG-based GNN that generates multiple faithful explanations for the same gene pair and effectively encodes high-order structures. Specifically, we introduce a novel DGIB objective, integrating a Determinant Point Process (DPP) constraint into the standard IB objective, and employ 13 motif-based adjacency matrices to capture high-order structures in gene representations. Experimental results show that DGIB4SL outperforms state-of-the-art baselines and provides multiple explanations for SL prediction, revealing diverse biological mechanisms underlying SL inference.
description: 15 pages. Accepted by Briefings in Bioinformatics