bluuebunny/crossref_metadata_2025_split huggingface dataset:
Detailed study of the Boötes field using 300–500 MHz uGMRT observations: source properties and radio–infrared correlations
Authors: Sinha Akriti , Datta Abhirup 
Published: September 2023

ABSTRACT
The dominant source of radio continuum emissions at low frequencies is synchrotron radiation, which originates from star-forming regions in disc galaxies and from powerful jets produced by active galactic nuclei (AGNs). We studied the Boötes field using the upgraded Giant Meterwave Radio Telescope at 400 MHz, achieving a central minimum off-source rms noise of 35 μJy beam−1 and a catalogue of 3782 sources in ∼6 deg2 of the sky. The resulting catalogue was compared to other radio frequency catalogues, and the corrected normalized differential source counts were derived. We use standard multiwavelength techniques to classify the sources in star-forming galaxies (SFGs), radio-loud AGNs, and radio-quiet (RQ) AGNs that confirm a boost in the SFG and RQ AGN populations at lower flux levels. For the first time, we investigated the properties of the radio–infrared (IR) relations at 400 MHz in this field. The $L_{\rm 400\, MHz}$–LTIR relations for SFGs were found to show a strong correlation with non-linear slope values of 1.10 ± 0.01, and variation of qTIR with z is given as qTIR = (2.19 ± 0.07) (1 + z)−0.15 ± 0.08. This indicates that the non-linearity of the radio–IR relations can be attributed to the mild variation of qTIR values with z. The derived relationships exhibit similar behaviour when applied to Low-Frequency Array at 150 MHz and also at 1.4 GHz. This emphasizes the fact that other parameters like magnetic field evolution with z or the number densities of cosmic ray electrons can play a vital role in the mild evolution of q values.
Impact of M-dwarf stellar wind and photoevaporation on the atmospheric evolution of small planets
Authors: Modi Ashini , Estrela Raissa , Valio Adriana 
Published: September 2023

ABSTRACT
The evolution of a planet’s atmosphere depends strongly on its host star’s properties. When their host stars are younger, planets can experience stronger winds and extreme ultraviolet radiation (EUV) emissions. This is particularly true for planets orbiting M dwarfs due to their close proximity to the host star. To determine if these planets retain an atmosphere, we consider the impacts from stellar wind and EUV fluxes in driving atmospheric escape throughout the planet’s lifetime. For this, we determined the atmospheric mass-loss due to stellar wind and photoevaporation on four planets in close orbit and 34 in their star’s habitable zone (HZ). The M-dwarf host stars’ wind velocity, density, and EUV flux were calculated through rotation period and X-ray flux scaling over time. The mass-loss rate due to stellar wind and photoevaporation was then computed as a function of time and accumulated throughout the planet’s age to determine the total atmospheric mass-loss of the planet’s initial H/He envelope. We find that for HZ planets at orbits &lt;0.1 au, stellar wind can only remove ${\le} 1~{{ \rm per\ cent}}$ of the H/He envelope, while photoevaporation is essential for completely removing the H/He envelope of most targets. Moreover, due to either mechanism, most planets orbiting at &gt;0.1 au do not have their primordial envelope stripped. Overall, out of the 38 planets studied, 13 were predicted to have lost the primordial envelope due to photoevaporation, while two planets lost the envelope due to both stellar wind and photoevaporation.
Fundamental parameters of 318 contact binaries from the TESS survey
Authors: Ding Xu , Ji KaiFan , Li XuZhi , Xiong JianPing , Cheng QiYuan , Wang JinLiang 
Published: September 2023

ABSTRACT
The TESS Survey has released a large number of high-precision light curves of contact binaries. However, using the Phoebe program and Markov chain Monte Carlo (MCMC) algorithm to obtain the posterior distribution of contact binary parameters is a time-consuming process. In order to obtain the contact binary parameters from the TESS survey, we build neural network (NN) models and combine them with the MCMC algorithm to obtain the contact binary parameters and parameter errors quickly. NN model is used in place of the physical model, which can generate a light curve with a precision of less than a millimagnitude. The NN model is capable of generating light curves at a speed that is four orders of magnitude faster than Phoebe running on the same computing platform. In this study, we have determined the parameters of 318 contact binary systems exhibiting relatively symmetric light curves. Subsequently, a statistical analysis was conducted on the derived parameters of these 318 targets. The coefficient of determination (R2) for 318 contact binaries between the light curves generated by Phoebe using these parameters obtained by the NN model and MCMC as inputs and the original light curves is greater than 0.99. Additionally, the distribution and correlation of the parameters for these 318 contact binary systems have been presented.
Constraining dark matter substructure with Gaia wide binaries
Authors: Ramirez Edward D , Buckley Matthew R 
Published: September 2023

ABSTRACT
We use a catalogue of stellar binaries with wide separations (up to 1 pc) identified by the Gaia satellite to constrain the presence of extended substructure within the Milky Way galaxy. Heating of the binaries through repeated encounters with substructure results in a characteristic distribution of binary separations, allowing constraints to be placed independent of the formation mechanism of wide binaries. Across a wide range of subhalo density profiles, we show that subhaloes with masses $\gtrsim 65\, \mathrm{ M}_\odot$ and characteristic length scales similar to the separation of these wide binaries cannot make up 100 per cent of the Galaxy’s dark matter. Constraints weaken for subhaloes with larger length scales and are dependent on their density profiles. For such large subhaloes, higher central densities lead to stronger constraints. Subhaloes with density profiles similar to those expected from cold dark matter must be at least ∼5000 times denser than predicted by simulation to be constrained by the wide binary catalogue.
Modelling the effect of 3D temperature and chemistry on the cross-correlation signal of transiting ultra-hot Jupiters: a study of five chemical species on WASP-76b
Authors: Wardenier Joost P , Parmentier Vivien , Line Michael R , Lee Elspeth K H 
Published: September 2023

ABSTRACT
Ultra-hot Jupiters are perfect targets for transmission spectroscopy. However, their atmospheres feature strong spatial variations in temperature, chemistry, dynamics, cloud coverage, and scale height. This makes transit observations at high spectral resolution challenging to interpret. In this work, we model the cross-correlation signal of five chemical species – Fe, CO, H2O, OH, and TiO – on WASP-76b, a benchmark ultra-hot Jupiter. We compute phase-dependent high-resolution transmission spectra of three-dimensional (3D) SPARC/MITgcm models. The spectra are obtained with gCMCRT, a 3D Monte-Carlo radiative-transfer code. We find that, on top of atmospheric dynamics, the phase-dependent Doppler shift of the absorption lines in the planetary rest frame is shaped by the combined effect of planetary rotation and the unique 3D spatial distribution of chemical species. For species probing the dayside (e.g. refractories or molecules like CO and OH), the two effects act in tandem, leading to increasing blueshifts with orbital phase. For species that are depleted on the dayside (e.g. H2O and TiO), the two effects act in an opposite manner, and could lead to increasing redshifts during the transit. This behaviour yields species-dependent offsets from a planet’s expected Kp value that can be much larger than planetary wind speeds. The offsets are usually negative for refractory species. We provide an analytical formula to estimate the size of a planet’s Kp offsets, which can serve as a prior for atmospheric retrievals. We conclude that observing the phase-resolved absorption signal of multiple species is key to constraining the 3D thermochemical structure and dynamics of ultra-hot Jupiters.
Variability, polarimetry, and timing properties of single pulses from PSR J2222−0137 using FAST
Authors: Miao X L , Zhu W W , Kramer M , Freire P C C , Shao L , Yuan M , Meng L Q , Wu Z W , Miao C C , Guo Y J , Champion D J , Fonseca E , Yao J M , Xue M Y , Niu J R , Hu H , Zhang C M 
Published: September 2023

ABSTRACT
In our work, we analyse 5 × 104 single pulses from the recycled pulsar PSR J2222−0137 in one of its scintillation maxima observed by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). PSR J2222−0137 is one of the nearest and best studies of binary pulsars and a unique laboratory for testing gravitational theories. We report single pulses’ energy distribution and polarization from the pulsar’s main-pulse region. The single-pulse energy follows the lognormal distribution. We resolve a steep polarization swing, but at the current time resolution ($64\ \mu {\rm s}$), we find no evidence for the orthogonal jump in the main-pulse region, as has been suspected. We find a potential sub-pulse drifting period of $P_{3} \sim 3.5 P$. We analyse the jitter noise from different integrated numbers of pulses and find that its σj is $270\pm {9}\ {\rm ns}$ for 1-h integration at 1.25 GHz. This result is useful for optimizing future timing campaigns with FAST or other radio telescopes.
Comparison of damping models for kink oscillations of coronal loops
Authors: Zhong Yu , Kolotkov Dmitrii Y , Zhong Sihui , Nakariakov Valery M 
Published: September 2023

ABSTRACT
Kink oscillations of solar coronal loops are of intense interest due to their potential for diagnosing plasma parameters in the corona. The accurate measurement of the kink oscillation damping time is crucial for precise seismological diagnostics, such as the transverse density profile, and for the determination of the damping mechanism. Previous studies of large-amplitude rapidly decaying kink oscillations have shown that both an exponential damping model and a generalized model (consisting of Gaussian and exponential damping patterns) fit observed damping profiles sufficiently well. However, it has recently been shown theoretically that the transition from the decaying regime to the decayless regime could be characterized by a superexponential damping model. In this work, we reanalyse a sample of decaying kink oscillation events, and utilize the Markov chain Monte Carlo Bayesian approach to compare the exponential, Gaussian–exponential, and superexponential damping models. It is found that in 7 out of 10 analysed oscillations, the preferential damping model is the superexponential one. In two events, the preferential damping is exponential, and in one it is Gaussian–exponential. This finding indicates the plausibility of the superexponential damping model. The possibility of a non-exponential damping pattern needs to be taken into account in the analysis of a larger number of events, especially in the estimation of the damping time and its associated empirical scalings with the oscillation period and amplitude, and in seismological inversions.
Detailed asteroseismic modelling of RR Lyrae stars with non-radial modes
Authors: Netzel H , Molnár L , Joyce M 
Published: September 2023

ABSTRACT
Photometric observations from the last decade have revealed additional low-amplitude periodicities in many classical pulsators that are likely due to pulsations in non-radial modes. One group of multimode RR Lyrae stars, the so-called 0.61 stars, is particularly interesting. In these stars, the radial first overtone is accompanied by additional signals with period ratios around 0.61. The most promising explanation for these signals is pulsation in non-radial modes of degrees 8 and 9. If the theory behind the additional signals in the 0.61 stars is substantiated, it would allow us to use non-radial modes to study classical pulsators. We aim to perform asteroseismic modelling of selected 0.61 stars with independently determined physical parameters to test whether this assumption behind the modelling leads to correct results. Namely, we test whether the additional signals are indeed due to non-radial modes of the proposed moderate degrees. We selected a number of RR Lyrae stars that are also 0.61 stars and have good observational constraints on their other physical parameters. We assume that the nature of those modes is correctly explained with non-radial modes of degrees 8 or 9. Using this assumption and observational constraints on physical parameters, we performed asteroseismic modelling to test whether the observed periods and period ratios can be reproduced. For the majority of selected targets, we obtained a good match between observed and calculated periods and period ratios. For a few targets however, the results obtained are ambiguous and not straightforward to interpret.
First detection of the BAO signal from early DESI data
Authors: Moon Jeongin , Valcin David , Rashkovetskyi Michael , Saulder Christoph , Aguilar Jessica Nicole , Ahlen Steven , Alam Shadab , Bailey Stephen , Baltay Charles , Blum Robert , Brooks David , Burtin Etienne , Chaussidon Edmond , Dawson Kyle , de la Macorra Axel , de M attia Arnaud , Dhungana Govinda , Eisenstein Daniel , Flaugher Brenna , Font-Ribera Andreu , Forero-Romero Jaime E , Garcia-Quintero Cristhian , Gontcho A Gontcho Satya , Guy Julien , Hanif Malik Muhammad Sikandar , Honscheid Klaus , Ishak Mustapha , Kehoe Robert , Kim Sumi , Kisner Theodore , Kremin Anthony , Landriau Martin , Le Guillou Laurent , Levi Michael , Manera Marc , Martini Paul , McDonald Patrick , Meisner Aaron , Miquel Ramon , Moustakas John , Myers Adam , Nadathur Seshadri , Neveux Richard , Newman Jeffrey A , Nie Jundan , Padmanabhan Nikhil , Palanque-Delabrouille Nathalie , Percival Will , Pérez Fernández Alejandro , Poppett Claire , Prada Francisco , Raichoor Anand , Ross Ashley J , Rossi Graziano , Samushia Lado , Schlegel David , Seo Hee-Jong , Tarlé Gregory , Vargas Magana Mariana , Variu Andrei , Weaver Benjamin Alan , White Martin J , Yèche Christophe , Yuan Sihan , Zhao Cheng , Zhou Rongpu , Zhou Zhimin , Zou Hu 
Published: September 2023

ABSTRACT
We present the first detection of the baryon acoustic oscillations (BAOs) signal obtained using unblinded data collected during the initial 2 months of operations of the Stage-IV ground-based Dark Energy Spectroscopic Instrument (DESI). From a selected sample of 261 291 luminous red galaxies spanning the redshift interval 0.4 &lt; z &lt; 1.1 and covering 1651 square degrees with a 57.9 per cent completeness level, we report a ∼5σ level BAO detection and the measurement of the BAO location at a precision of 1.7 per cent. Using a bright galaxy sample of 109 523 galaxies in the redshift range 0.1 &lt; z &lt; 0.5, over 3677 square degrees with a 50.0 per cent completeness, we also detect the BAO feature at ∼3σ significance with a 2.6 per cent precision. These first BAO measurements represent an important milestone, acting as a quality control on the optimal performance of the complex robotically actuated, fibre-fed DESI spectrograph, as well as an early validation of the DESI spectroscopic pipeline and data management system. Based on these first promising results, we forecast that DESI is on target to achieve a high-significance BAO detection at sub-per cent precision with the completed 5-yr survey data, meeting the top-level science requirements on BAO measurements. This exquisite level of precision will set new standards in cosmology and confirm DESI as the most competitive BAO experiment for the remainder of this decade.
Cool and gusty, with a chance of rain: dynamics of multiphase CGM around massive galaxies in the Romulus simulations
Authors: Saeedzadeh Vida , Jung S Lyla , Rennehan Douglas , Babul Arif , Tremmel Michael , Quinn Thomas R , Shao Zhiwei , Sharma Prateek , Mayer Lucio , O’Sullivan E , Loubser S Ilani 
Published: September 2023

ABSTRACT
Using high-resolution Romulus simulations, we explore the origin and evolution of the circumgalactic medium (CGM) in the region 0.1 ≤ R/R500 ≤ 1 around massive central galaxies in group-scale halos. We find that the CGM is multiphase and highly dynamic. Investigating the dynamics, we identify seven patterns of evolution. We show that these are robust and detected consistently across various conditions. The gas cools via two pathways: (1) filamentary cooling inflows and (2) condensations forming from rapidly cooling density perturbations. In our cosmological simulations, the perturbations are mainly seeded by orbiting substructures. The condensations can form even when the median tcool/tff of the X-ray emitting gas is above 10 or 20. Strong amplitude perturbations can provoke runaway cooling regardless of the state of the background gas. We also find perturbations whose local tcool/tff ratios drop below the threshold but which do not condense. Rather, the ratios fall to some minimum value and then bounce. These are weak perturbations that are temporarily swept up in satellite wakes and carried to larger radii. Their tcool/tff ratios decrease because tff is increasing, not because tcool is decreasing. For structures forming hierarchically, our study highlights the challenge of using a simple threshold argument to infer the CGM’s evolution. It also highlights that the median hot gas properties are suboptimal determinants of the CGM’s state and dynamics. Realistic CGM models must incorporate the impact of mergers and orbiting satellites, along with the CGM’s heating and cooling cycles.
Call to Improve the Quality of Prediction Tools for Intrahepatic Cholangiocarcinoma Resection: A Critical Appraisal, Systematic Review, and External Validation Study
Authors: Choi Woo Jin , Walker Richard , Rajendran Luckshi , Jones Owen , Gravely Annie , Englesakis Marina , Gallinger Steven , Hirschfield Gideon , Hansen Bettina , Sapisochin Gonzalo 
Published: September 2023

Objective:
To conduct a systematic review, critical appraisal, and external validation of survival prediction tools for patients undergoing intrahepatic cholangiocarcinoma (iCCA) resection.

Summary background data:
Despite the development of several survival prediction tools in recent years for patients undergoing iCCA resections, there is a lack of critical appraisal and external validation of these models.

Methods:
We conducted a systematic review and critical appraisal of survival and recurrence prediction models for patients undergoing curative-intent iCCA resections. Studies were evaluated based on their model design, risk of bias, reporting, performance, and validation results. We identified the best model and externally validated it using our institution’s data.

Results:
This review included a total of 31 studies, consisting of 26 studies with original prediction tools and 5 studies that only conducted external validations. Among the 26, 54% of the studies conducted internal validations, 46% conducted external validations, and only 1 study scored a low risk of bias. Harrell’s C-statistics ranged from 0.67 to 0.76 for internal validation and from 0.64 to 0.75 for external validation. Only 81% of the studies reported model calibration. Our external validation of the best model (Intrahepatic Cholangiocarcinoma [ICC]-Metroticket) estimated Harrell’s and Uno’s C-statistics of 0.67 (95% CI: 0.56–0.77) and Uno’s time-dependent area under the receiver operating characteristic curve (AUC) of 0.71 (95% CI: 0.53–0.88), with a Brier score of 0.20 (95% CI: 0.15–0.26) and good calibration plots.

Conclusions:
Many prediction models have been published in recent years, but their quality remains poor, and minimal methodological quality improvement has been observed. The ICC-Metroticket was selected as the best model (Uno’s time-dependent AUC of 0.71) for 5-year overall survival prediction in patients undergoing curative-intent iCCA resection.
Male Hypogonadism Does Not Affect Surgical Outcomes After Primary Artificial Urinary Sphincter Placement
Authors: Gabrielson Andrew T. , Galansky Logan B. , Choi Una , Cohen Andrew 
Published: September 2023

Purpose:
Studies suggest a link between hypogonadism and complications after artificial urinary sphincter (AUS) placement. We investigated this association and evaluated whether testosterone replacement therapy (TRT) before AUS placement attenuates this risk in hypogonadal patients.

Materials and Methods:
A retrospective cohort study was conducted using the TriNetX network between 2008 and 2022. We defined 2 groups undergoing primary AUS: (1) eugonadal and (2) hypogonadal patients. We further assessed the hypogonadal cohort by comparing TRT recipients with TRT-naïve patients before AUS. Propensity score matching was used to account for differences in covariates between eugonadal and hypogonadal cohorts. Outcomes included 5-year all-cause revision, erosion, mechanical failure, or device infection.

Results:
A total of 4308 eugonadal and 514 hypogonadal patients (95 with TRT, 409 TRT-naïve) were included. After matching, the eugonadal and hypogonadal cohorts each contained 504 patients. The median follow-up times for the eugonadal and hypogonadal cohorts were 6 and 5 years, respectively. We found no difference in 5-year all-cause revision (25% vs 28%, P = .35), erosion (1.2% vs 2.2%, P = .22), device infection (3.6% vs 4.0%, P = .74), or mechanical failure (16% vs 17%, P = .67) between eugonadal and hypogonadal patients. In the hypogonadal subanalysis, we found no difference in 5-year device outcomes between TRT recipients and TRT-naïve patients. Post-AUS, only 22 (5%) patients in the TRT-naïve arm received new TRT, suggesting minimal crossover.

Conclusions:
In matched cohorts of eugonadal and hypogonadal patients undergoing primary AUS placement, we observed no difference in 5-year device outcomes. TRT does not appear to affect surgical outcomes in hypogonadal patients undergoing AUS placement. These hypothesis-generating findings warrant further evaluation.
Efficacy, safety, and economy of shensongyangxin capsules for the treatment of coronary heart disease arrhythmia: a meta-analysis of randomized controlled trials
Authors: Ma Luyao , Li Libing , Ma Fujin , Ma Fuyun , Ma Shujia 
Published: September 2023

Background:
Shensong Yangxin Capsules (SSYX) is a proprietary Chinese medicine commonly, used in the treatment of arrhythmia. In recent years, a flurry of randomized controlled trials of SSYX was reported in the treatment of Coronary heart disease arrhythmia in China. However, these experiments have not been systematically evaluated by economics. The purpose of this study was to assess the efficacy, safety, and economy of the SSYX in the treatment of arrhythmia in patients with coronary heart disease.

Methods:
With “Shensong Yangxin Capsules” “Coronary Heart Disease” “Coronary Atherosclerotic Heart Disease”and “Arrhythmia” as the subject words, the relevant journals and conference papers were searched manually in China National Knowledge Infrastructure (CNKI), Wanfang Database, VIP, PubMed, Web Of Science, CBM, Embase and The Cochrane Library. The literature of randomized controlled trials of SSYX in the treatment of coronary heart disease arrhythmia was searched until November 2022. All data were analyzed using RevMan 5.3 Sotware and combined with cost-effectiveness for economic evaluation.

Results:
Twenty randomized controlled trials were included in this study, with a total of 2011 cases. The meta-analysis showed that the therapeutic effect of SSYX-metoprolol is superior to that of metoprolol alone. SSYX is superior to amiodarone in improving the total clinical effective rate, reducing the incidence of adverse reactions, and reducing the junction premature beats. There was no significant difference between the SSYX and amiodarone in the curative effect of ECG, ventricular premature complexes, and atrial premature beats. The results of pharmacoeconomics show that SSYX has a cost-effectiveness advantage in treating coronary heart disease arrhythmia. Single-factor sensitivity analysis also confirmed the stability of the results. In summary, SSYX has a curative effect, safety, and economy in treating coronary heart disease arrhythmia.