bluuebunny/crossref_metadata_2025_split huggingface dataset:
CLASS Data Pipeline and Maps for 40 GHz Observations through 2022
Authors: Li 李 Yunyang 云炀 , Eimer Joseph R. , Osumi Keisuke , Appel John W. , Brewer Michael K. , Ali Aamir , Bennett Charles L. , Bruno Sarah Marie , Bustos Ricardo , Chuss David T. , Cleary Joseph , Couto Jullianna Denes , Dahal Sumit , Datta Rahul , Denis Kevin L. , Dünner Rolando , Espinoza Francisco , Essinger-Hileman Thomas , Fluxá Rojas Pedro , Harrington Kathleen , Iuliano Jeffrey , Karakla John , Marriage Tobias A. , Miller Nathan J. , Novack Sasha , Núñez Carolina , Petroff Matthew A. , Reeves Rodrigo A. , Rostem Karwan , Shi 时 Rui 瑞 , Valle Deniz A. N. , Watts Duncan J. , Weiland Janet L. , Wollack Edward J. , Xu 徐 Zhilei 智磊 , Zeng Lingzhen ,   CLASS Collaboration
Published: October 2023

Abstract
The Cosmology Large Angular Scale Surveyor (CLASS) is a telescope array that observes the cosmic microwave background over 75% of the sky from the Atacama Desert, Chile, at frequency bands centered near 40, 90, 150, and 220 GHz. This paper describes the CLASS data pipeline and maps for 40 GHz observations conducted from 2016 August to 2022 May. We demonstrate how well the CLASS survey strategy, with rapid (∼10 Hz) front-end modulation, recovers the large-scale Galactic polarization signal from the ground: the mapping transfer function recovers ∼67% (85%) of EE and BB (VV) power at ℓ = 20 and ∼35% (47%) at ℓ = 10. We present linear and circular polarization maps over 75% of the sky. Simulations based on the data imply the maps have a white noise level of

110

μ
K

arcmin

and correlated noise component rising at low-ℓ as ℓ
−2.4. The transfer-function-corrected low-ℓ component is comparable to the white noise at the angular knee frequencies of ℓ ≈ 18 (linear polarization) and ℓ ≈ 12 (circular polarization). Finally, we present simulations of the level at which expected sources of systematic error bias the measurements, finding subpercent bias for the Λ cold dark matter EE power spectra. Bias from E-to-B leakage due to the data reduction pipeline and polarization angle uncertainty approaches the expected level for an r = 0.01 BB power spectrum. Improvements to the instrument calibration and the data pipeline will decrease this bias.
Constraining Inputs to Realistic Kilonova Simulations through Comparison to Observed r-process Abundances
Authors: Ristić Marko , Holmbeck Erika M. , Wollaeger Ryan T. , Korobkin Oleg , Champion Elizabeth , O’Shaughnessy Richard , Fryer Chris L. , Fontes Christopher J. , Mumpower Matthew R. , Sprouse Trevor M. 
Published: October 2023

Abstract
Kilonovae, one source of electromagnetic emission associated with neutron star mergers, are powered by the decay of radioactive isotopes in the neutron-rich merger ejecta. Models for kilonova emission consistent with the electromagnetic counterpart to GW170817 predict characteristic abundance patterns, determined by the relative balance of different types of material in the outflow. Assuming that the observed source is prototypical, this inferred abundance pattern in turn must match r-process abundances deduced by other means, such as what is observed in the solar system. We report on analysis comparing the input mass-weighted elemental compositions adopted in our radiative transfer simulations to the mass fractions of elements in the Sun, as a practical prototype for the potentially universal abundance signature from neutron star mergers. We characterize the extent to which our parameter inference results depend on our assumed composition for the dynamical and wind ejecta and examine how the new results compare to previous work. We find that a dynamical ejecta composition calculated using the FRDM2012 nuclear mass and FRLDM fission models with extremely neutron-rich ejecta (Y

e
= 0.035) along with moderately neutron-rich (Y

e
= 0.27) wind ejecta composition yields a wind-to-dynamical mass ratio of M

w
/M

d
= 0.47, which best matches the observed AT2017gfo kilonova light curves while also producing the best-matching abundance of neutron capture elements in the solar system, though, allowing for systematics, the ratio may be as high as of order unity.
On the Effectiveness of the Planetary Infrared Excess (PIE) Technique to Retrieve the Parameters of Multiplanet Systems around M Dwarfs: A Case Study on the TRAPPIST-1 System
Authors: Mayorga L. C. , Lustig-Yaeger J. , Stevenson K. B. ,   Consortium on Habitability and Atmospheres of M-dwarf Planets (CHAMPs)
Published: October 2023

Abstract
The planetary infrared excess (PIE) technique has the potential to efficiently detect and characterize the thermal spectra of both transiting and non-transiting exoplanets. However, the technique has not been evaluated on multiplanet systems. We use the TRAPPIST-1 system as our test bed to evaluate PIE’s ability to resolve multiple planets. We follow the unfolding discoveries in the TRAPPIST-1 system and examine the results from the PIE technique at every stage. We test the information gained from observations with JWST and next-generation infrared observatories like the proposed MIRECLE mission concept. We find that even in the case where only the star is known, the PIE technique would infer the presence of multiple planets in the system. The precise number inferred is dependent on the wavelength range of the observation and the noise level of the data. We also find that in such a tightly packed, multiplanet system such as TRAPPIST-1, the PIE technique struggles to constrain the semimajor axis beyond prior knowledge. Despite these drawbacks and the fact that JWST is less sensitive to the fluxes from planets g and h, with strong priors in their orbital parameters we are able to constrain their equilibrium temperatures. We conclude that the PIE technique may enable the discovery of unknown exoplanets around solar-neighborhood M dwarfs and could characterize known planets around them.
A Fundamental Mechanism of Solar Eruption Initiation in a Multipolar Magnetic Field
Authors: Bian Xinkai , Jiang Chaowei , Feng Xueshang , Zuo Pingbing , Wang Yi 
Published: October 2023

Abstract
Recently, we established a fundamental mechanism of solar eruption initiation in which an eruption can be initiated from a bipolar field through magnetic reconnection in the current sheet (CS) that is formed slowly in the core field as driven by photospheric shearing motion. Here, using a series of fully 3D MHD simulations with a range of different photospheric magnetic flux distributions, we extended this fundamental mechanism to the quadrupolar magnetic field containing a null point above the core field, which is the basic configuration of the classical breakout model. As is commonly believed, in such a multipolar configuration, the reconnection triggered in the CS originated at the null point (namely, the breakout reconnection) plays the key role in eruption initiation by establishing a positive feedback loop between the breakout reconnection and the expansion of the core field. However, our simulation showed that the key to eruption initiation in such a multipolar configuration remains the slow formation of the CS in the sheared core, rather than the onset of fast breakout reconnection. The breakout reconnection only helps the formation of the core CS by letting the core field expand faster, but the eruption cannot occur when the bottom surface driving is stopped well before the core CS is formed, even though the fast reconnection has already been triggered in the breakout CS. This study clarified the role of breakout reconnection and confirmed formation of the core CS as the key to the eruption initiation in a multipolar magnetic field.
The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. I. Detection of a Rich Population of Dusty Objects in the IRS 13 Cluster
Authors: Peißker Florian , Zajaček Michal , Thomkins Lauritz , Eckart Andreas , Labadie Lucas , Karas Vladimír , Sabha Nadeen B. , Steiniger Lukas , Melamed Maria 
Published: October 2023

Abstract
A detailed analysis of the nuclear star cluster not only concedes the existence of the S cluster, with its fast-moving stars and the supermassive black hole Sgr A*. It also reveals an embedded region of gas and dust with an exceptionally high stellar density called IRS 13. The IRS 13 cluster can be divided into the northern and eastern counterparts, called IRS 13N and IRS 13E, respectively. This work will focus on both regions and study their most prominent members using rich infrared and radio/submillimeter data baselines. Applying a multiwavelength analysis enables us to determine a comprehensive photometric footprint of the investigated cluster sample. Using the ray-tracing-based radiative transfer model HYPERION, the spectral energy distribution of the IRS 13 members suggests a stellar nature of the dusty sources. These putative young stellar objects (YSOs) have a comparable spectroscopic identification to the D and G sources in or near the S cluster. Furthermore, we report the existence of a population of dusty sources in IRS 13 that can be mostly identified in the H, K, and L band. We propose that, together with the objects reported in the literature, this population is the outcome of a recent star formation process. Furthermore, we report that these presumably young objects are arranged in a disk structure. Although it cannot be excluded that the intrinsic arrangement of IRS 13 does show a disk structure, we find indications that the investigated cluster sample might be related to the counterclockwise disk.
Abundances and Transients from Neutron Star–White Dwarf Mergers
Authors: Kaltenborn M. Alexander R. , Fryer Chris L. , Wollaeger Ryan T. , Belczynski Krzysztof , Even Wesley , Kouveliotou Chryssa 
Published: October 2023

Abstract
We systematically investigate the mergers of neutron star–white dwarf binaries from beginning to end, with a focus on the properties of the inflows and outflows in accretion disks and their electromagnetic emissions. Using population synthesis models, we determine a subset of these binaries in which the white dwarf companion undergoes unstable mass transfer and complete tidal disruption, forming a large accretion disk around the neutron star. The material evolves according to a one-dimensional advection-dominated accretion-disk model with nuclear burning, neutrino emissions, and disk-surface wind ejection. The extreme dynamics of the entire process have proven difficult to analyze, and thus currently, the properties are poorly understood. The outflows from the mergers are iron- and nickel-rich, giving rise to optical and infrared emissions powered by the decay of the radioactive iron-type isotopes, calculated via the SuperNu light-curve code. We find these systems capable of powering bright, yet short-lived, optical transients with the potential to power gamma-ray bursts.
A new record of the genus Froggattiella Leonardi (Hemiptera, Coccomorpha, Diaspididae) in South Korea
Authors: Kim Hyeong Su , Kim Jaeyun , Lee Wonhoon 
Published: October 2023

The genus Froggattiella Leonardi, 1900 belongs to the family Diaspididae, and five species of Froggattiella have been recorded worldwide. In this study, Froggattiella penicillata (Green, 1905), which attacks bamboos, is newly recorded in South Korea. The colonies of F. penicillata were collected on a bamboo forest located in Gajwa-dong, Jinju-si, Gyeongsangnam-do, South Korea (35.1599, 128.1029). Description of the adult female, host plant, adult female illustrations, and global distribution of this species are provided.
Froggattiella penicillata (Green, 1905) is reported for the first time in South Korea. This species occurrs under sheathing bases of the leaves and is observed attached on the stem and not on the leaf.
De la fascisation
Authors: Zaoui Pierre 
Published: October 2023

Nous ne sommes pas tous fascistes, mais nous sommes tous fascisés : nous acceptons les signifiants de l’extermination et nous nous habituons à jouir de ce que nous ne voulons pas voir (les camps, les morts). Face à ces flux, plus que de barrages, nous avons besoin de lutter contre nous-mêmes.
Loin de toute orthodoxie, de la passion au divan
Authors: Lecoq Arlette 
Published: October 2023

Guidé par ses exigences de sincérité et par la turbulence de ses passions, Sándor Ferenczi ébranlera les limites de la psychanalyse naissante. Homme du XIX e siècle mais moderniste avant la lettre, il va tracer un chemin d’ouverture tant sur le plan clinique que sur le plan théorique. Un pas de deux prometteur l’entraîne avec Freud vers des découvertes fécondes : l’introjection, Thalassa , etc. mais il s’écartera de son maître pour glisser vers l’étiologie traumatique des névroses que Freud avait abandonnée au profit de la voie fantasmatique. Ce tournant lui valut la mise au ban de la communauté analytique mais ouvrit la voie à travers de multiples douleurs, découvertes et échecs à la psychanalyse contemporaine.
Le journal clinique de Sándor Ferenczi. La psychanalyse du traumatisme
Authors: Hebbrecht Marc 
Published: October 2023

L’article s’ouvre sur une discussion relative à la façon dont le journal a trouvé accès auprès du grand public. Il décrit ensuite les trois thèmes principaux du journal de Ferenczi : la relation de Ferenczi avec Freud, l’analyse mutuelle avec Elisabeth Severn (RN), enfin des considérations sur la thérapie de patients traumatisés ou victimes d’inceste, partie la plus importante du journal. Le traumatisme entraîne une fragmentation de la psyché en plusieurs parties. Ferenczi mentionne l’hypocrisie des parents, des éducateurs et des enseignants comme une cause importante du masochisme. En fin d’article, les implications thérapeutiques du traitement des victimes d’abus sexuels et d’inceste sont débattus.
La théorie du réel comme « ontologie négative »
Authors: Espinosa Santiago 
Published: October 2023

Dans cet article il s’agit de jeter quelque lumière sur les concepts de réel et de double dans l’œuvre de Clément Rosset. Il y est montré que ces deux concepts, fondamentaux pour sa pensée, ont toujours été clairement définis et déterminés, qu’ils n’ont pas prêté à confusion dans son œuvre, qu’ils ont toujours désigné chacun le même objet philosophique : ce qui existe et ce qui n’existe pas, respectivement. Le réel est l’ensemble de ce qui existe, qui peut être perçu ; le double est ce qui n’existe pas, qui ne peut donc être perçu ni pensé, mais qui n’en produit pas moins l’illusion d’une perception ou d’une pensée. À ce titre, l’article signale quelques malentendus ou contresens auxquels ces concepts ont pu prêter, non pas, encore une fois, en raison d’une définition faible ou vague, mais plutôt en raison d’une lecture orientée ou partielle de l’œuvre de Rosset.
Management of autofluorescence in formaldehyde-fixed myocardium: choosing the right treatment
Authors: Zhang Zhao , Fan Hongming , Richardson William , Gao Bruce Z. , Ye Tong 
Published: October 2023

Autofluorescence (AF) poses challenges for detecting proteins of interest in situ when employing immunofluorescence (IF) microscopy. This interference is particularly pronounced in strongly autofluorescent tissues such as myocardium, where tissue AF can be comparable to IF. Although various histochemical methods have been developed to achieve effective AF suppression in different types of tissue, their applications on myocardial samples have not been well validated. Due to inconsistency across different autofluorescent structures in sometypes of tissue, it is unclear if these methods can effectively suppress AF across all autofluorescent structures within the myocardium. Here, we quantitatively evaluated the performance of several commonly used quenching treatments on formaldehyde-fixed myocardial samples, including 0.3 M glycine, 0.3% Sudan Black B (SBB), 0.1% and 1% sodium borohydride (NaBH4), TrueVIEW® and TrueBlack®. We further assessed their quenching performance by employing the pre-treatment and post-treatment protocols, designed to cover two common IF staining scenarios where buffers contained detergents or not. The results suggest that SBB and TrueBlack® outperform other reagents in AF suppression on formaldehyde-fixed myocardial samples in both protocols. Furthermore, we inspected the quenching performance of SBB and TrueBlack® on major autofluorescent myocardial structures and evaluated their influence on IF imaging. The results suggest that SBB outperforms TrueBlack® in quenching major autofluorescent structures, while TrueBlack® excels in preserving IF labeling signal. Surprisingly, we found the treatment of NaBH4 increased AF signal and enhanced the AF contrast of major autofluorescent structures. This finding suggests that NaBH4 has the potential to act as an AF enhancer and may facilitate the interpretation of myocardial structures without the need for counterstaining.
Awareness, Knowledge, and Attitudes Regarding Cardiopulmonary Resuscitation in Case of Cardiac Arrest among the Population in the Jazan Region, Saudi Arabia
Authors: Sayed Ahmed I. , Mobarki Sarah J. , Hakami Abdulaziz Ahmed , Saabi Somaya M. , Oraibi Manaf M. , Darraj Bushra H. , Alshamakhi Atheer H. , Abuhadi Hamzah M. , Abdulwali Hany M. , Hakami Abdulrahman M. 
Published: October 2023

Introduction:
For cardiac arrest victims, providing high-quality cardiopulmonary resuscitation (CPR) is a fundamental component of initial care, especially in out-of-hospital settings. We sought to assess the knowledge of nonmedically trained individuals about CPR in case of cardiac arrest in the population of Jazan, Saudi Arabia.

Materials and Methods:
A cross-sectional survey containing 22 questions was administered to individuals aged ≥ 18 years who were not health-care providers. The sample comprised residents of Jazan, Saudi Arabia. The survey included knowledge about the signs of cardiac arrest, previous experiences with CPR, knowledge of basic life support (BLS), and concerns related to CPR.

Results:
This study examined responses from 480 people to assess their knowledge of CPR. More than one-half were female, and only 33% were male. Only 36.04% reported having received CPR training. In the event of a family member’s cardiac arrest, more than 90% state that they would perform CPR. If a family member suffered a sudden cardiac arrest, more than 70% would call an ambulance immediately, whereas only 48% would call an ambulance if the same thing happened to a stranger. Fear of making a mistake was the most common reason for not performing CPR (70.63%). The media was the most common source of CPR training. Women were more aware of the warning signs of sudden cardiac arrest than men. Women were also more likely than men to perform CPR or call for assistance. Furthermore, women were significantly more likely than men to discontinue CPR on a sudden cardiac arrest patient for fear of stopping a working heart or being contaminated by blood or vomit. Few respondents were willing to undergo CPR training; students, homemakers, and retired people were more willing to be trained in CPR than others.

Conclusion:
In the Saudi Arabian province of Jazan, nonmedically trained people demonstrated a low level of CPR training and knowledge. We believe that making BLS courses available to the general public will increase CPR awareness and understanding among adults and increase survival rates in cases of sudden cardiac arrest.
Dose-dependent Reduction of Blood Pressure by Angiotensin Receptor-neprilysin Inhibitor: A Network Meta-analysis
Authors: Kao Ting-Wei , Lee Yi-Chih 
Published: October 2023

Context:
Angiotensin receptor-neprilysin inhibitor (ARNi) has been established as the standard medication for heart failure. However, the blood pressure (BP)-lowering effect circumvented its administration and titration in patients with borderline hypotension.

Aim:
This study aimed to determine the correlation between ARNi dosage and hemodynamic impacts.

Subjects and Methods:
A network meta-analysis was conducted to interrogate the BP impact of ARNi (sacubitril/valsartan 100 mg/d, 200 mg/d, 400 mg/d) and angiotensin receptor blocker (ARB) counterparts. Individuals with mild-to-moderate systolic hypertension were enrolled in respective studies. The outcomes were set as the change from baseline systolic and diastolic BP.

Statistical Analysis Used:
Network meta-analysis, node-splitting, and inconsistency model methods in Bayesian approach were employed.

Results:
A total of 14 manuscripts with 7705 subjects were included for pooled analysis. Compared with ARB, sacubitril/valsartan 400 mg/d and 200 mg/d, but not 100 mg/d, were associated with significantly greater reduction effect of systolic and diastolic BP, either by office documentation or 24-h ambulatory monitoring. The BP-lowering effect of sacubitril/valsartan 400 mg/d and 200 mg/d was nevertheless equivalent.

Conclusions:
ARNi exerts a dose-dependent effect on BP reduction. Such hemodynamic impact exceeds ARB at higher doses.
Evaluation of Response to Thrombolytic Therapy versus Surgery in Patients with Aortic Prosthetic Valve Thrombosis in a Tertiary Heart Center in Tehran, Iran, during 2007–2019
Authors: Shojaeifard Maryam , Koochari Iman , Zarei Keyvan , Mohammadabadi Hossein Dehghani , Erami Sajad , Khoshtinat Vadood , Bahadori Mohammad Javad , Rezazadeh Parisa , Parhizgar Seyed Ehsan 
Published: October 2023

Background:
Prosthetic valve thrombosis is of the serious long-term complications of heart valve replacement that its treatment particularly in left-sided valves is controversial. Both surgery and thrombolysis are associated with their own merits and drawbacks. Hence, the aim of the present study is the evaluation of response to surgery and thrombolytic therapy in patients with aortic prosthetic valve thrombosis in a tertiary heart center in Tehran, Iran, during 2007–2019.

Materials and Methods:
In this retrospective study, 85 patients with aortic prosthetic valve thrombosis (including 63 case of surgery and 22 case of thrombolytic therapy) were evaluated. Response to clinical and hemodynamic treatment and frequency of complications and mortality were determined in each group.

Results:
Clinical complete response in surgery group (84.13%) was significantly more than patients with thrombolytic therapy (64.63%). The frequency of complications in surgery and the thrombolytic group was 12.7% and 9.09%, respectively, which show no significant difference. Mortality was seen in 1.58% and 4.53% of patients with surgery and thrombolytic therapy respectively that was not statistically significant. Complete failure of treatment was seen in 18.18% of patients with thrombolytic therapy and re-surgery was done for them. The surgery success rate was significantly more than thrombolytic success rate in patients with a therapeutic range of international normalized ratio (INR) level.

Conclusion:
Surgery versus thrombolytic therapy has more efficacy and similar safety in patients with aortic prosthetic valve thrombosis and may be preferable treatment for these patients. However, thrombolytic therapy also can be used as a suitable alternative, particularly in patients with a high risk of surgery.