bluuebunny/crossref_metadata_2025_split huggingface dataset:
Wprowadzenie do badań nad dzieciństwem w kulturze Zachodu
Authors: Mostowska Jadwiga 
Published: January 2025

Artykuł jest próbą zarysowania wybranych problemów i refleksji odnoszących się do kategorii dziecka i dzieciństwa, jak również wskazania kilku zmian, jakie zaszły w postrzeganiu najmłodszych i ich roli w zachodnich społeczeństwach na przestrzeni ostatnich kilku stuleci – zmian, które były kluczowe dla ukształtowania się dzisiejszego sposobu percepcji dzieciństwa. Artykuł jest zatem: po pierwsze, próbą doprecyzowania kategorii dziecka i dzieciństwa odnoszących się do nieco innych sfer pojęciowych; po drugie, wskazania kilku istotnych czynników, które wpływały na zmianę sposobu widzenia roli dziecka oraz rozumienia dzieciństwa w społeczeństwie i kulturze, doprowadzając do wykształcenia się współczesnej wizji dzieciństwa; po trzecie, zarysowania współczesnego wizerunku dziecka i dzieciństwa w oparciu o refleksje pojawiające się na gruncie interdyscyplinarnych badań nad dzieciństwem oraz wskazania na pewne sposoby obecności i rekonstruowania wizerunku dziecka i dzieciństwa w tekstach kultury.
Pengaruh Faktor Individu, Psikologis dan Organisasi Terhadap Kinerja Guru Pns dan Non Pns Di Taman Kanak-Kanak Se-Kecamatan Weru Sukoharjo
Authors: Warih Anggi Pratiwi  , Prehatiningsih Arip 
Published: January 2025

Penelitian ini bertujuan untuk mengetahui apakah faktor individu, psikologis dan organisasi berpengaruh terhadap kinerja guru PNS dan Non PNS di Taman Kanak-kanak se- Kabupaten Sukoharjo. Penelitian ini menggunakan penelitian kuantitatif. Dengan teknik pengumpulan data menggunakan kuesioner/angket dan dokumentasi. Teknik analisis data: (1) uji prasyarat analisis yaitu validitas instrument, reliabilitas instrument, (2) Uji Hipotesis, pengujian hipotesis dalam penelitian ini menggunakan regresi parametrik. Hasil penelitian menunjukkan (1) Bahwa faktor individu (X1) berpengaruh terhadap kinerja guru PNS (Y1). (2) Bahwa faktor psikologis (X2) berpengaruh terhadap kinerja guru PNS (Y1). (3) Bahwa faktor organisasi (X3) tidak berpengaruh terhadap kinerja guru PNS (Y1). (4) Faktor Individu (X1), Faktor Psikologi (X2) dan Faktor Organisasi (X3), berpengaruh secara signifikan bersama-sama terhadap Kinerja Guru PNS (Y1). (5) Bahwa faktor individu berpengaruh terhadap kinerja guru non-PNS (Y2). (6) Bahwa faktor psikologis berpengaruh terhadap kinerja guru non-PNS (Y2). (7) Bahwa faktor organisasi tidak berpengaruh terhadap kinerja guru non-PNS (Y2). (4) Faktor Individu (X1), Faktor Psikologi (X2) dan Faktor Organisasi (X3), berpengaruh secara signifikan bersama-sama terhadap Kinerja Guru non-PNS (Y2)
The Clear Sky Corridor: Insights Towards Aerosol Formation in Exoplanets Using an AI-based Survey of Exoplanet Atmospheres
Authors: Ashtari Reza , Stevenson Kevin B. , Sing David , López-Morales Mercedes , Alam Munazza K. , Nikolov Nikolay K. , Evans-Soma Thomas M. 
Published: January 2025

Abstract
Producing optimized and accurate transmission spectra of exoplanets from telescope data has traditionally been a manual and labor intensive procedure. Here we present the results of the first attempt to improve and standardize this procedure by using artificial-intelligence-based (AI-based) processing of light curves and spectroscopic data from transiting exoplanets observed with the Hubble Space Telescope's (HST) Wide Field Camera (WFC3) instrument. We implement an AI-based parameter optimizer that autonomously operates the Eureka! pipeline to produce homogeneous transmission spectra of publicly available HST WFC3 datasets, spanning exoplanet types from hot Jupiters to sub-Neptunes. Surveying 42 exoplanets with temperatures between 280 and 2580 K, we confirm modeled relationships between the amplitude of the water band at 1.4 μm of hot Jupiters and their equilibrium temperatures. We also identify a similar, novel trend in Neptune/sub-Neptune atmospheres, but shifted to cooler temperatures. Excitingly, a planet-mass versus equilibrium-temperature diagram reveals a “Clear Sky Corridor,” where planets between 700 and 1700 K (depending on the mass) show stronger 1.4 μm H2O band measurements. This novel trend points to metallicity as a potentially important driver of aerosol formation. With HST sculpting this foundational understanding for aerosol formation in various exoplanet types ranging from Jupiters to sub-Neptunes, we present a compelling platform for the James Webb Space Telescope to discover similar atmospheric trends for more planets across a broader wavelength range.
Atmospheric Mass Loss from TOI-1259 A b, a Gas Giant Planet with a White Dwarf Companion
Authors: Saidel Morgan , Vissapragada Shreyas , Spake Jessica , Knutson Heather A. , Linssen Dion , Zhang Michael , Greklek-McKeon Michael , Pérez-González Jorge , Oklopčić Antonija 
Published: January 2025

Abstract
The lack of close-in Neptune-mass exoplanets evident in transit surveys has largely been attributed to either photoevaporative mass loss or high-eccentricity migration. To distinguish between these two possibilities, we investigate the origins of TOI-1259 A b, a Saturn-mass (0.4M
J, 1.0R
J) exoplanet lying along the upper edge of the Neptune desert. TOI-1259 A b's close-in (P = 3.48 days) orbit and low bulk density make the planet particularly vulnerable to photoevaporation. We studied the upper atmosphere of TOI-1259 A b using metastable helium 1083 nm transits observed with Palomar/WIRC and Keck/NIRSPEC. We report a band-integrated excess absorption of 0.395% ± 0.072% with Palomar/WIRC and a spectroscopically resolved 5.5 ± 0.94 km s−1 blueshifted absorption of 2.4% ± 0.52% (T
1–T
4) and 3.5% ± 0.72% (T
2–T
3) with Keck/NIRSPEC. These measurements indicate the presence of an extended escaping atmosphere. Fitting these signals with a Parker wind model, we determine a corresponding atmospheric mass-loss rate of log(

M

̇

) = 10.2–10.65 g s−1 for thermosphere temperatures between 7900 and 8600 K. This relatively low rate suggests that this planet would not have been significantly altered by mass loss even if it formed in situ. However, the presence of a white dwarf companion, TOI-1259 B, hints that this planet may not have formed close-in, but rather migrated inward relatively late. Given the estimated parameters of the proto−white dwarf companion, we find that high-eccentricity migration is possible for the system.
A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): Spectroscopically Complete Census of Obscured Cosmic Star Formation Rate Density at z = 4–6
Authors: Sun Fengwu , Wang Feige , Yang Jinyi , Champagne Jaclyn B. , Decarli Roberto , Fan Xiaohui , Bañados Eduardo , Cai Zheng , Colina Luis , Egami Eiichi , Hennawi Joseph F. , Jin Xiangyu , Jun Hyunsung D. , Khusanova Yana , Li Mingyu , Li Zihao , Lin Xiaojing , Liu Weizhe , Meyer Romain A. , Pudoka Maria A. , Rieke George H. , Shen Yue , Tee Wei Leong , Venemans Bram , Walter Fabian , Wu Yunjing , Zhang Huanian , Zou Siwei 
Published: January 2025

Abstract
We present a stringent measurement of the dust-obscured star formation rate density (SFRD) at z = 4–6 from the ASPIRE JWST Cycle-1 medium and ALMA Cycle-9 large program. We obtained JWST/NIRCam grism spectroscopy and ALMA 1.2 mm continuum map along 25 independent quasar sightlines, covering a total survey area of ∼35 arcmin2 where we search for dusty star-forming galaxies (DSFGs) at z = 0–7. We identify eight DSFGs in seven fields at z = 4–6 through the detection of Hα or [O iii] λ5008 lines, including fainter lines such as Hβ, [O iii] λ4960, [N ii] λ6585, and [S ii] λλ6718,6733 for six sources. With this spectroscopically complete DSFG sample at z = 4–6 and negligible impact from cosmic variance (shot noise), we measure the infrared luminosity function (IRLF) down to L
IR ∼ 2 × 1011
L
⊙. We find flattening of IRLF at z = 4–6 towards the faint end (power-law slope

α
=
0.5

9

−
0.45

+
0.39

). We determine the dust-obscured cosmic SFRD at this epoch to be

log
[

ρ

SFR
,
IR

/
(

M
⊙

yr

−
1

Mpc

−
3

)
]
=
−
1.5

2

−
0.13

+
0.14

. This is significantly higher than previous determinations using ALMA data in the Hubble Ultra Deep Field, which is void of DSFGs at z = 4–6 because of strong cosmic variance (shot noise). We conclude that the majority (66% ± 7%) of cosmic star formation at z ∼ 5 is still obscured by dust. We also discuss the uncertainty of SFRD propagated from far-IR spectral energy distribution and IRLF at the bright end, which will need to be resolved with future ALMA and JWST observations.
The DiskMass Survey. XI. Disk Geometries and Star Formation Surface Densities from Ionized Gas Kinematics and Line Intensities for the Full Hα Sample
Authors: Swaters Robert A. , Andersen David R. , Bershady Matthew A. , Martinsson Thomas P. K. , Scholz Paul , Verheijen Marc A.W. , Westfall Kyle B. 
Published: January 2025

Abstract
We present Hα-region integral-field spectroscopy for 137 low-inclination, intermediate to late-type galaxies. Spectroscopic data, obtained with SparsePak and the Bench Spectrograph on the WIYN 3.5 m telescope, span 6475–6880 Å with an instrumental resolution of 13 km s−1 (σ). The spectral range includes Hα and [N ii]λλ6548, 6584 for every source, and in most cases includes [S ii]λλ6717, 6731. We present and publicly release 18,288 calibrated spectra and visually inspected Gaussian line fits to the Hα emission. Most measurements yield a signal-to-noise ratio above 5 in integrated Hα line flux, adequate to derive reliable line centroids and widths. Second kinematic components are required to adequately describe the emission-line profile in 15% of reliable data. The Hα velocity dispersion distribution peaks at 18 km s−1, modestly increasing with Hα surface brightness, reaching 20 km s−1 at ΣHα
= 1040 erg s−1 kpc−2. Lower-flux secondary components, when present, have widths of ~50 km s−1. These results agree well with previous echelle measurements of nearby galaxies. Velocity-field analysis yields kinematic inclinations, with a sample mean of 26°. Large kinematic asymmetries systematically affect kinematic inclination estimates in a small fraction of our sample. When deviations from circular motion are below 10% of the projected velocity, kinematic inclinations are consistent, within errors, to estimates from inverting the Tully–Fisher relation. This confirms previous disk-submaximality estimates for galaxies with regular kinematics based on inclinations derived from inverting the Tully–Fisher relation.
Production, Transport, and Destruction of Dust in the Kuiper Belt: The Effects of Refractory and Volatile Grain Compositions
Authors: Corbett Thomas , Doner Alex , Horányi Mihály , Brandt Pontus , Grundy Will , Lisse Carey M. , Parker Joel , Peltier Lowell , Poppe Andrew R. , Singer Kelsi N. , Stern S. Alan , Verbiscer Anne J. 
Published: January 2025

Abstract
The Venetia Burney Student Dust Counter (SDC) on board the New Horizons spacecraft measures the spatial and size distributions of dust along its trajectory. Models based on early SDC measurements predicted a peak dust number density at a heliocentric distance of ∼40 au, followed by a rapid decline. Instead, SDC observed dust fluxes 2–3 times higher than predicted between 40 and 60 au. One potential explanation for this discrepancy is that SDC may be encountering icy grains with different dynamical behavior than previously modeled silicate grains. Due to ultraviolet photosputtering, water–ice grains rapidly erode and migrate outward, significantly contributing to the measured dust number densities only at distances ≳40 au. We present a model of silicate and ice grain dynamics in the outer solar system, considering gravitational and radiation forces and grain erosion. Using SDC data, we estimate that the mass production rate of ice grains between 0.1 and 10 μm in the Kuiper Belt (KB) would need to be 20–70 times higher than that of silicate grains. However, KB grains are expected to be refractory/volatile mixtures rather than pure silicate or ice. Thus, we briefly explore simple models of more realistic mixed-grain cases to further gauge the effects of grain composition on the equilibrium dust distribution. Future SDC measurements at greater distances will test the model predictions and further constrain silicate and ice grain production rates in the KB.
History and Habitability of the LP 890-9 Planetary System
Authors: Barnes Rory , do Amaral Laura N. R. , Birky Jessica , Carone Ludmila , Driscoll Peter , Livesey Joseph R. , Graham David , Becker Juliette , Cui Kaiming , Schlecker Martin , Garcia Rodolfo , Gialluca Megan , Adams Arthur , Ahmed MD Redyan , Bonney Paul , Broussard Wynter , Chawla Chetan , Damasso Mario , Danchi William C. , Deitrick Russell , Ducrot Elsa , Fromont Emeline F. , Gaches Brandt A. L. , Gupta Sakshi , Hill Michelle L. , Jackman James A. G. , Janin Estelle M. , Karawacki Mikołaj , Koren Matheus Daniel , La Greca Roberto , Leung Michaela , Miranda-Rosete Arturo , Olohoy Michael Kent A. , Ngo Cecelia , Paul Daria , Sahu Chandan Kumar , Sarkar Debajyoti Basu , Shadab Mohammad Afzal , Schwieterman Edward W. , Sedler Melissa , Texeira Katie , Vazan Allona , Delgado Vega Karen N. , Vijayakumar Rohit , Wojack Jonathan T. 
Published: January 2025

Abstract
We present numerous aspects of the evolution of the LP 890-9 (SPECULOOS-2/TOI-4306) planetary system, focusing on the likelihood that planet c can support life. We find that the host star reaches the main sequence in 1 Gyr and that planet c lies close to the inner boundary of the habitable zone. We find the magma ocean stage can last up to 50 Myr, remove eight Earth oceans of water, and leave up to 2000 bars of oxygen in the atmosphere. However, if the planet forms with a hydrogen envelope as small as 0.1 Earth masses, no water will be lost during the star's pre-main-sequence phase from thermal escape processes. We find that the planets are unlikely to be in a 3:1 mean motion resonance and that both planets tidally circularize within 0.5 Gyr when tidal dissipation is held constant. However, if tidal dissipation is a function of mantle temperature and rheology, then we find that planet c's orbit may require more than 7 Gyr to circularize, during which time tidal heating may reach hundreds of terawatts. We thus conclude that the habitability of planet c depends most strongly on the initial volatile content and internal properties, but no data yet preclude the viability of an active biosphere on the planet.
Cross Validation of Albedo Determination for 1627 Ivar from Three Different Techniques
Authors: Selmi Elena , Devogèle M. , Masiero J. R. , Santiago N. Vega , Wright E. L. , Ferrais M. , Fernández-Valenzuela E. , Borisov G. , Bendjoya Ph. , Rivet J.-P. , Abe L. , Vernet D. , Cellino A. 
Published: January 2025

Abstract
Near-Earth asteroids are of great interest to the scientific community due to their proximity to Earth, making them both potential hazards and possible targets for future missions, as they are relatively easy to reach by spacecraft. A number of techniques and models can be used to constrain their physical parameters and build a comprehensive assessment of these objects. In this work, we compare physical property results obtained from improved H

V
absolute magnitude values, thermophysical modeling, and polarimetry data for the well-known Amor-class NEO 1627 Ivar. We show that our fits for albedo are consistent with each other, thus demonstrating the validity of this cross-referencing approach, and propose a value for Ivar's albedo of

0.2

4

−
0.02

+
0.04

. Future observations will extend this work to a larger sample size, increasing the reliability of polarimetry for rapid asteroid property characterization as a technique independent of previously established methods and requiring significantly fewer observations.
Relationship between milk stability and physico-chemical characteristics of raw milk of different breeds during storage at ambient temperature
Authors: Pasan A. J. R. P. , Prasantha B. D. R. , Amarathunga K. S. P. 
Published: January 2025

This study investigated the relationship between milk stability and physico-chemical characteristics of raw milk of four cow breeds in Sri Lanka: Sahiwal, Friesian Cross, Jersey Cross, and Australian Friesian Sahiwal. This study examined the changes in electrical conductivity (EC), pH, turbidity, and total soluble solids (TSS%) during an 8 h storage period at ambient temperature (28±1 oC) and their correlation with the alcohol test results as a platform test. Results indicated that EC did not significantly change in the raw milk samples of Sahiwal, Friesian cross, or Australian Friesian Sahiwal breeds. Milk pH of all samples decreased with the storage period; however, significant (P<0.05) reductions of pH were observed in the Jersey cross and Australian Friesian Sahiwal breeds, compared to their initial pH of the raw milk samples 6.10±0.2 and 6.36±0.2, respectively. The turbidity of raw milk samples of the four cow breeds was significantly increased with the storage period (P<0.05). Australian Friesian Sahiwal breeds showed the highest turbidity development (241.0±3.7 NTU) while Jersey Crossbreeds showed the significantly (P<0.05) lowest turbidity development of 191.2±11.3 NTU. Both Sahiwal and Jersey Cross breeds significantly decreased (P<0.05) TSS content from 9.35 to 7.10% and 9.25 to 7.25% respectively with the storage period. The chi-square results indicated that there is no significant association (P>0.05) between alcohol test and the milk samples obtained from the different breeds. The significant negative correlation of turbidity (ρ>-0.8; P<0.05) and TSS% (ρ>-0.4; P<0.05) showed with the alcohol test in all cow breeds. Binary logistic regression results showed that the significant correlation between alcohol test and milk turbidity (Wald X2 = 4.44, P<0.05). These findings highlight measuring the turbidity of raw milk would be a critical parameter for assessing milk stability and development of an in-situ instrument to quantitatively detect raw milk turbidity instead of the qualitative alcohol test.
Removal of Expression of Concern for ‘Lipid-lowering therapy in patients with coronary heart disease: an Italian real-life survey. Results from the Survey on Risk FactOrs and CardiovascuLar secondary prevention and drug strategieS (SOFOCLES) in Italy’
Authors: Monaldi Archives for Chest Disease Editors The 
Published: January 2025

Removal of Expression of Concern for ‘Lipid-lowering therapy in patients with coronary heart disease: an Italian real-life survey. Results from the Survey on Risk FactOrs and CardiovascuLar secondary prevention and drug strategieS (SOFOCLES) in Italy’ by Caterina Oriana Aragona et al., Monaldi Arch Chest Dis, 2024, Accepted Manuscript, https://doi.org/10.4081/monaldi.2024.2972 IF: 1.1 Q4 NA

The Editors and Publisher of the Monaldi Archives for Chest Disease are publishing this removal of expression of concern to inform readers that the investigation is complete and all earlier issues have been addressed.This notice supersedes the information provided in the Expression of Concern related to this article (https://www.monaldi-archives.org/macd/article/view/3259).
Empowering church leaders for service in Africa: Situational Holistic Pastoral Ministry paradigm
Authors: Hove Rabson 
Published: January 2025

Empowering church leaders globally is a contested terrain, particularly in Africa. This article explores the challenges and pitfalls of church leadership on the continent. It not only examines the complexities of contemporary African church leadership but also proposes strategies for modelling its transformative development. The focus is on critically assessing how church leaders can be empowered to transform both the church and communities in Africa through the Situational Holistic Pastoral Ministry (SHPM) paradigm. The article argues that numerous challenges in Africa can be mitigated by equipping church leaders for transformative roles. A key issue identified is the tendency to idolise clergy, placing them at the centre of ministry, rather than fostering their role as models who empower others. Drawing on insights from SHPM theory, this article evaluates the empowerment of church leaders for transformative action within the African context. It concludes by emphasising the need to empower church leaders to facilitate the transformation of both the church and its surrounding communities.Contribution: This article contributes to the discourse on ethical Christian leadership by advocating role-modelling servant leadership as opposed to idolisation. It posits that empowering church leaders is essential for addressing the myriad challenges confronting churches and communities in sub-Saharan Africa.
Mia Couto and the enchantment of rain
Authors: Hooper Myrtle J. , Rawlins Isabel B. 
Published: January 2025

In his preface to Rain and Other Stories, Mia Couto refers to the remaking of the world following the Mozambican civil war: ‘we soak our faces in this rain of hope, this water of benedreamtion’. Pluvial rain, as Nuttall terms it, can bring huge destruction, as can drought, its absence. Scholars have insisted on the agency of water, including African ecocritics who argue for an ‘animist conception of the world’ which transposes and transgresses boundaries and identities. Garuba specifically refers to the ‘persistent re-enchantment of the world’ whereby the ‘rational and scientific are appropriated and transformed into the mystical and magical’. This article explores the range of roles, agentic and enchanted, which Couto accords rain in his stories. Although he rejected the label ‘magic realist’, his translator Chabal argues that in his stories the fantastic ‘transmutes the fictitious into the factual’ so that ‘all boundaries are put into question’: between past and present, far and near, material and spiritual. And he seeks to regain the ‘brotherhood’, the ‘relation’, the ‘link between nature and humanity’. Ashcroft says Couto’s vision as a writer is to ‘give back to the word its divine power … the power to enchant things, be these trees, birds, or landscapes’. Samuelson too claims that Couto’s stories ‘invoke an enlivening ecocritical method’ that draws readers into a ‘sacred web’, an ‘indivisible body, an ‘interconnected world’. While the notion of enchantment is not unproblematic, the interconnections it entails between human and environment, material and spiritual, generate a receptive matrix in which to understand and recognise the agency of rain.Contribution: This article engages with ecocritical readings of the stories of Mia Couto by examining his treatment of rain and his approach to the issue of enchantment. It thus contributes to criticism of his work as well as to the growing field of ecocriticism in this country.