bluuebunny/crossref_metadata_2025_split huggingface dataset:
Hyperkalemia and Risk of CKD Progression: A Propensity Score–Matched Analysis
Authors: Agiro Abiy , Cook Erin , Mu Fan , Greatsinger Alexandra , Chen Jingyi , Zhao Angela , Louden Elaine , Colman Ellen , Desai Pooja , Chertow Glenn M. 
Published: August 2024

Key Points

Hyperkalemia is a known complication of CKD; however, it is not known whether hyperkalemia directly contributes to CKD progression and risk of death.We found that patients with stages 3b/4 CKD and hyperkalemia had higher risk of CKD progression and death than matched patients without hyperkalemia.

Background
Hyperkalemia is a known complication of CKD; however, it is not known whether hyperkalemia directly contributes to CKD progression and the risk of death. Clarifying the extent to which hyperkalemia is associated with CKD progression and mortality can inform clinical practice and guide future research. The objective of this study was to quantify the risks of CKD progression and mortality associated with hyperkalemia in patients with stages 3b/4 CKD.

Methods
This was a real-world, exact and propensity score matched, observational cohort study using data (January 2016 to December 2021) from Optum's deidentified Market Clarity Data, a large US integrated insurance claims/electronic medical record database. The study included matched adult patients with stages 3b/4 CKD with and without hyperkalemia, not regularly treated with an intestinal potassium (K+) binder. Measured outcomes were CKD progression and all-cause mortality. CKD progression was defined as diagnosis of CKD stage 4 (if stage 3b at index), CKD stage 5 or kidney failure, or receipt of dialysis or kidney transplantation.

Results
After matching, there were 6619 patients in each of the hyperkalemia and nonhyperkalemia cohorts, with a mean follow-up time of 2.12 (SD, 1.42) years. Use of any renin-angiotensin-aldosterone system inhibitors during baseline was common (75.9%), and most patients had CKD stage 3b (71.2%). Patients with hyperkalemia had a 1.60-fold (95% confidence interval, 1.50 to 1.71) higher risk of CKD progression and a 1.09-fold (1.02 to 1.16) higher risk of all-cause mortality relative to patients without hyperkalemia. Relative risks of CKD progression associated with hyperkalemia were similar within the subset of patients receiving renin-angiotensin-aldosterone system inhibitor, across CKD stages, and when alternative definitions of CKD progression were used.

Conclusions
Patients with CKD stages 3b/4 and hyperkalemia experienced significantly higher risks of CKD progression and all-cause mortality than propensity score matched patients without hyperkalemia.
CHARACTERISTICS OF CAUSATIVE AGENTS OF SURGICAL WOUND INFECTIONS IN MEDICAL INSTITUTIONS
Authors: Atakişizadə S.A. , Cəfərova K.Ə. , Kərimova İ.A. , Qurbanova L.M. 
Published: August 2024

Məqalədə cərrahi yara infeksiyalarının etioloji agentlərinin və onların antimikrob preparatlara həssaslıq və rezistentliyinin araşdırılması məqsədilə aparılmış tədqiqat işi haqqında məlumat verilmişdir. Tədqiqat 2019-2022-ci illərdə Azərbaycan Tibb Universitetinin Tədris Cərrahiyyə klinikasında müalicə almış xəstələr üzərində aparılmışdır. Cərrahi əməliyyatlardan sonra baş verən yara infeksiyaları zamanı yara, drenaj və abses möhtəviyyatların mikrobioloji müayinəsi nəticəsində cərrahi yara infeksiyalarının əsas törədicilərinin S.aureus, P.aeruginosa, E.coli, Klebsiella cinsli bakteriyalar, eləcə də Candida cinsli göbələklər olduğu müəyyən edilmişdir. P.aeruginosa, E.coli vəKlebsiella cinsli bakteriyalar əksər antibiotiklərə davamlı olması ilə fərqlənmişlər. E.coli və Klebsiella cinsli bakteriya ştammlarının əksəriyyətində genişlənmiş spektrli betalaktamaza (GSBL), P.aeruginosa ştammlarının təqribən yarısında induksiya olunan beta-laktamaza (İsBL) produksiyası aşkar edilmişdir.
The article presents the results of a study conducted to investigate the etiological agents of surgical wound infections, their sensitivity, and resistance to antimicrobial agents. The study was carried out on patients who received surgical treatment at the clinic of Azerbaijan Medical University from 2019 to 2022. Microbiological examination of the contents of wounds, drains, and abscesses in wound infections that occurred after surgical operations was conducted. The study found that the main causative agents of surgical wound infections are S. aureus, P. aeruginosa, E. coli, Klebsiella, as well as Candida fungi. P. aeruginosa, E. coli, and Klebsiella are resistant to most antibiotics. Extended-spectrum beta-lactamase production was identified in most bacterial strains of E. coli and Klebsiella, while inducible beta-lactamase production was determined in approximately half of the P. aeruginosa strains.
В статье представлена результаты исследования, проведённого с целью изучения этиологических агентов хирургических раневых инфекций, их чувствительности и резистентности к антимикробным препаратам. Исследование было проведено у больных, получавших хирургическое лечение в клинике Азербайджанского медицинского университета в 2019-2022 гг. Проводили микробиологическое исследование содержимого ран, дренажей и абсцессов при раневых инфекциях, возникших после хирургических операций. В результате исследования установлено, что основными возбудителями хирургических раневых инфекций являются S.aureus, P.aeruginosa, E.coli, Klebsiella, а также грибы Candida. P.aeruginosa, E.coli и Klebsiella устойчивы к большинству антибиотиков. Продукция бета-лактамаз расширенного спектра была определена у большинства бактериальных штаммов E.coli и Klebsiella, а продукция индуцибельной бета-лактамазы (ИБЛ) была определена примерно у половины штаммов P.aeruginosa.
Diagnóstico e tratamento do câncer de mama: uma revisão de literatura
Authors: Briguenti Ramalho Rafaela , De Luca Castro Giovanna , Santana Sakamoto Gustavo , Romana Correia Sales Ana Karoline , Nicole Lino do Nascimento Whanela , Gomes Lourencini Yasmin , Oliveira de Lima Layla , Weiler Prado Letícia , Oliveira Freire do Nascimento Lucas , De Almeida Andrade Pereira Lucca , Camila Lira de Menezes Tatiana , Perinazzo da Rosa Felipe 
Published: August 2024

Este artigo tem por objetivo avaliar os aspectos clínicos do diagnóstico e do tratamento do câncer de mama realizada nos últimos cinco anos. Revisão integrativa no banco de dados da BVS, LILACS, SciELO, PubMed de trabalhos publicados entre 2020 e 2024, combinando os descritores "câncer de mama", "diagnóstico" e "tratamento" ao descritor booleano "AND". O câncer de mama é uma doença multifatorial. O avançar da idade é o principal fator de risco e se relaciona ao acúmulo de exposições ao longo da vida e às próprias alterações biológicas com o envelhecimento. Conclui-se que o diagnóstico do câncer de mama deve estar ancorado em um tripé: exame clínico, exame de imagem e análise histopatológica. O tratamento varia de acordo com o estadiamento da doença, suas características biológicas, bem como as condições da paciente (idade, status menopausal, comorbidades e preferências).
Proses Penegakan Putusan Pengadilan Tata Usaha Negara yang Berkekuatan Hukum Tetap
Authors: Mulyana Momon 
Published: August 2024

Tujuan penelitian ini adalah untuk meneliti dan mnganalisa bagaimana kekuatan hukum putusan Peradilan Tata Usaha Negara ( PTUN ) yang telah mempunyaI kekuatan hukum tetap, serta bagaimana sanksi bagi pejabat Tata Usaha Negara yang tidak mrlaksanakan Purtusan Peradilan Tata Usaha Negara tersebut. Metode penelitian yang digunakan adalah metode penelitian normatif yakni penelitian hukum yang dilakukan dengan cara mengkaji peraturan perundang-undangan yang diterapkan terhadap suatu permasalahan hukum tertentu.hasil penelitian adalah bahwa Putusan pengadilan tata usaha negara bersifat mengikat umum (erga omnes), maka kekuatan putusan pengadilan tata usaha negara tersebut sama dengan kekuatan peraturan perundang-undangan. Dengan demikian, suatu putusan pengadilan tata usaha negara yang berkekuatan hukum tetap mempunyai kekuatan sebagai berikut: 1) kekuatan mengikat; 2) kekuatan pembuktian; dan 3) kekuatan eksekutorial. Dan bagaimana sanksi Bagi pejabat pemerintahan yang tidak melaksanakan putusan tata usaha negara yang berkekuatan hukum tetap (in kracht van gewijsde) menurut Pasal 116 Undang-undang Nomor 51 Tahun 2009 tentang Perubahan Kedua Atas Undangundang Nomor 5 Tahun 1986 tentang Peradilan Tata Usaha Negara, dapat dikenai sanksi.
Blood microcirculation under conditions of a translational model of alcohol cardiomyopathy in rats
Authors: Kryzhanovskii S. A. , Tsorin I. B. , Ionova E. O. , Simonenko S. A. , Vititnova M. B. 
Published: August 2024

Purpose of the study. Studying the blood microcirculation characteristics in the brain and heart of rats with ACM.Materials and methods. The study was carried out on white outbred male rats. The animals were randomized into 2 groups: 1st (n = 7) — control (intact) rats that received a normal diet and free access to water; 2nd (n = 6) — animals that received a normal diet and a 10 % ethanol solution as the only source of liquid. After 24 weeks of alcoholization in animals, the size and inotropic function of the heart were assessed using echocardiography. The next day, in anesthetized rats (urethane 1300 mg/kg i.p.), blood microcirculation in the heart and brain was recorded using a computerized laser analyzer “LAZMA-D” (manufactured by NPP “Lazma”, Russia) using the LDF 3.0.2.396 program. Using spectral wavelet analysis, the amplitudes of endothelial, neurogenic, myogenic, pulse and respiratory oscillations of microblood flow and the shunting index were determined.Results. According to echocardiography data, in rats that consumed a 10 % ethanol solution for 24 weeks, ACM is formed, which is accompanied by a decrease in blood microcirculation in the brain and myocardium. Thus, if in control animals the indicator of blood microcirculation in the myocardium was 36.60±2.19 perf. u., then in rats with ACM it was equal to 26.88±1.50 perf. u. units (p = 0.004). In the myocardium of rats with ACM, compared with control animals, the amplitude of both active and passive oscillations of microblood flow was significantly greater.Conclusion. In rats with ACM, the level of blood microcirculation in the heart muscle is significantly reduced, which, according to the results of spectral wavelet analysis, is prognostically unfavorable.
Analysis Impact Application SFAS 72 On Financial Performance
Authors: Irfani Cahaya Fajrina Putri , Efrianti Desi 
Published: August 2024

The property, real estate and building construction sectors play an important role in the economy and development in Indonesia. The property, real estate and building construction sectors are currently facing budget problems. This is caused by limited APBN funds, which hinder the achievement of development goals. Real Estate refers to assets that include land, buildings, and other fixed resources, which include ownership rights to property. Meanwhile, building construction refers to the construction of facilities and infrastructure in a certain area, such as the construction of buildings, roads, etc. This research is included in the mixed type of research because it uses quantitative and qualitative methods. The data used comes from officially registered sources, namely the financial reports of Property Companies listed on the Indonesia Stock Exchange in 2018 and 2021. The object of this research is financial performance variables. The research subject is what and who is used as the research unit. In this research, the research subjects are property companies listed on the Indonesia Stock Exchange in 2018 and 2021. The research results refer to the output of the paired samples test table shows that the Sig. (2-tailed) there is no difference before and after the implementation of the PSAK. Referring to the output of the test statistics table, it is known that the value of Asymp.Sig. (2-tailed) 0.117 which is 0.05. Thus, at a real level of 5% it can be concluded that the implementation of PSAK 72 (currently PSAK 115) does not provide significant changes to the financial statements.

Keywords: Property and PSAK 72 (now PSAK 115)
Conditions under which the convergence of a sequence or its certain subsequences follows from the summability by deferred weighted means
Authors: Sezer Sefa Anıl , Çanak İbrahim 
Published: August 2024

UDC 517.5
Let

(

u
k

)

be a sequence of real or complex numbers. First, we consider a real sequence

(

u
k

)

and formulate one-sided Tauberian conditions, which are necessary and sufficient for the convergence of certain subsequences of

(

u
k

)

to follow from its deferred weighted summability. These conditions are satisfied if

(

u
k

)

is deferred slowly decreasing or if

(

u
k

)

obeys a Landau-type Tauberian condition. Second, we consider a complex sequence

(

u
k

)

and present a two-sided Tauberian condition which is necessary and sufficient in order that the convergence of certain subsequences of

(

u
k

)

follow from its deferred weighted summability. This condition is satisfied either if

(

u
k

)

is deferred slowly oscillating or if

(

u
k

)

obeys a Hardy-type Tauberian condition. Finally, we extend these results to sequences in ordered linear spaces over the real numbers.
Поводження субгармонічних функцій повільного зростання зовні виняткових множин
Authors: Zabolotskyy M. , Zabolotskyy T. 
Published: August 2024

УДК 517.53
Нехай

v

– повільно зростаюча, необмежена на

[
0
,

+
∞
)

функція,

u

–субгармонічна в площині функція нульового порядку,

μ

– її міра Рісса,

n

(
t
,
u
)

=
μ

(

{
x
:
|
x
|
≤
t
}

)

,

N

(
t
,
u
)

=

∫
1
t

n

(
τ
,
u
)

/
τ
ⅆ
τ
,

n

(
r
,
u
)

=
O

(
v
(
r
)
)

,

r
→
+
∞
.

Множину

E
∈
ℂ

назвемо

C
0
β

-множиною,

0
<
β
≤
1
,

якщо її можна покрити системою кругів

K

(

a
n

,

r
n

)

=

{
z
:
|
z
-

a
n

|
<

r
n

}

таких, що

∑

|

a
n

|
≤
r

r
n
β

=
o

(

r
β

)

,

r
→
+
∞
.

Тоді для довільної неспадної необмеженої на

[
0
,

+
∞
)

функції

ϕ

існує

C
0
β

-множина

E

така, що

u

(
z
)

=
N

(
r
,
u
)

+
o

(
ϕ
(
r
)
v
(
r
)
)

,

r
=
|
z
|
→
+
∞
,

z
∉
E
.

Показано також, що у цій асимптотичній формулі залишковий член

o

(
ϕ
(
r
)
v
(
r
)
)

не можна замінити на

O

(
v
(
r
)
)

.
JWST COMPASS: A NIRSpec/G395H Transmission Spectrum of the Sub-Neptune TOI-836c
Authors: Wallack Nicole L. , Batalha Natasha E. , Alderson Lili , Scarsdale Nicholas , Adams Redai Jea I. , Aguichine Artyom , Alam Munazza K. , Gao Peter , Wolfgang Angie , Batalha Natalie M. , Kirk James , López-Morales Mercedes , Moran Sarah E. , Teske Johanna , Wakeford Hannah R. , Wogan Nicholas F. 
Published: August 2024

Abstract
Planets between the sizes of Earth and Neptune are the most common in the Galaxy, bridging the gap between the terrestrial and giant planets in our solar system. Now that we are firmly in the era of JWST, we can begin to measure, in more detail, the atmospheres of these ubiquitous planets to better understand their evolutionary trajectories. The two planets in the TOI-836 system are ideal candidates for such a study, as they fall on either side of the radius valley, allowing for direct comparisons of the present-day atmospheres of planets that formed in the same environment but had different ultimate end states. We present results from the JWST NIRSpec G395H transit observation of the larger and outer of the planets in this system, TOI-836c (2.587 R
⊕, 9.6 M
⊕, T
eq ∼ 665 K). While we measure average 30-pixel binned precisions of ∼24 ppm for NRS1 and ∼43 ppm for NRS2 per spectral bin, we do find residual correlated noise in the data, which we attempt to correct using the JWST Engineering Database. We find a featureless transmission spectrum for this sub-Neptune planet and are able to rule out atmospheric metallicities <175× solar in the absence of aerosols at ≲1 mbar. We leverage microphysical models to determine that aerosols at such low pressures are physically plausible. The results presented herein represent the first observation from the COMPASS (Compositions of Mini-Planet Atmospheres for Statistical Study) JWST program, which also includes TOI-836b and will ultimately compare the presence and compositions of atmospheres for 12 super-Earths/sub-Neptunes.
SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 μm and Data Release for the COSMOS Field
Authors: Gao 高 Zhen-Kai 振凱 , Lim 林 Chen-Fatt 征發 , Wang 王 Wei-Hao 為豪 , Chen 陳 Chian-Chou 建州 , Smail Ian , Chapman Scott C. , Zheng Xian Zhong , Shim Hyunjin , Kodama Tadayuki , Ao Yiping , Chang 張 Siou-Yu 修瑜 , Clements David L. , Dunlop James S. , Ho Luis C. , Hsu 徐 Yun-Hsin 允心 , Hwang Chorng-Yuan , Hwang Ho Seong , Koprowski M. P. , Scott Douglas , Serjeant Stephen , Toba Yoshiki , Urquhart Sheona A. 
Published: August 2024

Abstract
We present confusion-limited SCUBA-2 450 μm observations in the COSMOS-CANDELS region as part of the James Clerk Maxwell Telescope Large Program SCUBA-2 Ultra Deep Imaging EAO Survey. Our maps at 450 and 850 μm cover an area of 450 arcmin2. We achieved instrumental noise levels of σ
450 = 0.59 mJy beam−1 and σ
850 = 0.09 mJy beam−1 in the deepest area of each map. The corresponding confusion noise levels are estimated to be 0.65 and 0.36 mJy beam−1. Above the 4σ (3.5σ) threshold, we detected 360 (479) sources at 450 μm and 237 (314) sources at 850 μm. We derive the deepest blank-field number counts at 450 μm, covering the flux-density range of 2–43 mJy. These are in agreement with other SCUBA-2 blank-field and lensing-cluster observations but are lower than various model counts. We compare the counts with those in other fields and find that the field-to-field variance observed at 450 μm at the

R
=
6
′

scale is consistent with Poisson noise, so there is no evidence of strong 2D clustering at this scale. Additionally, we derive the integrated surface brightness at 450 μm down to 2.1 mJy to be

57.3

−
6.2

+
1.0

Jy deg−2, contributing to 41% ± 4% of the 450 μm extragalactic background light (EBL) measured by Cosmic Background Explorer and Planck. Our results suggest that the 450 μm EBL may be fully resolved at

0.08

−
0.08

+
0.09

mJy, which extremely deep lensing-cluster observations and next-generation submillimeter instruments with large aperture sizes may be able to achieve.
Feedback in Emerging Extragalactic Star Clusters, FEAST: The Relation between 3.3 μm Polycyclic Aromatic Hydrocarbon Emission and Star Formation Rate Traced by Ionized Gas in NGC 628
Authors: Gregg Benjamin , Calzetti Daniela , Adamo Angela , Bajaj Varun , Ryon Jenna E. , Linden Sean T. , Correnti Matteo , Cignoni Michele , Messa Matteo , Sabbi Elena , Gallagher John S. , Grasha Kathryn , Pedrini Alex , Gutermuth Robert A. , Melinder Jens , Kotulla Ralf , Pérez Gustavo , Krumholz Mark R. , Bik Arjan , Östlin Göran , Johnson Kelsey E. , Bortolini Giacomo , Smith Linda J. , Tosi Monica , Maji Subhransu , Faustino Vieira Helena 
Published: August 2024

Abstract
We present maps of ionized gas (traced by Paα and Brα) and 3.3 μm polycyclic aromatic hydrocarbon (PAH) emission in the nearby spiral galaxy NGC 628, derived from new JWST/NIRCam data from the Feedback in Emerging extrAgalactic Star clusTers (FEAST) survey. With this data, we investigate and calibrate the relation between 3.3 μm PAH emission and star formation rate (SFR) in and around emerging young star clusters (eYSCs) on a scale of ∼40 pc. We find a tight (correlation coefficient ρ ∼ 0.9) sublinear (power-law exponent α ∼ 0.75) relation between the 3.3 μm PAH luminosity surface density and SFR traced by Brα for compact, cospatial (within 0.″16 or ∼7 pc) peaks in Paα, Brα, and 3.3 μm (eYSC–I). The scatter in the relationship does not correlate well with variations in local interstellar medium metallicity, due to a radial metallicity gradient, but rather is likely due to stochastic sampling of the stellar initial mass function (IMF) and variations in the PAH heating and age of our sources. The deviation from a linear relation may be explained by PAH destruction in more intense ionizing environments, variations in age, and IMF stochasticity at intermediate to low luminosities. We test our results with various continuum subtraction techniques using combinations of NIRCam bands and find that they remain robust with only minor differences in the derived slope and intercept. An unexpected discrepancy is identified between the relations of hydrogen recombination lines (Paα versus Brα; Hα versus Brα).
OO Leo: An Active Contact Binary with Possible Solar-like Differential Rotation
Authors: Meng Zi-Bin , Wu Pei-Ru , Yu Yun-Xia , Hu Ke , Xiang Fu-Yuan 
Published: August 2024

Abstract
With Transiting Exoplanet Survey Satellite (TESS) high-precision photometry and Large Sky Area Multi-object Fiber Spectroscopic Telescope medium-resolution spectra, we present the first light and radial velocity curve analyses for the eclipsing binary OO Leo. The simultaneous solution suggests that OO Leo is a W-subtype contact binary with a relatively low mass ratio (1/q = 0.173) and a moderate degree of contact (f = 28.1%). The asymmetry and continuous changes observed in the TESS light curve were properly modeled by one retrograde cool spot on its secondary surface. A detailed investigation of the Hα line also confirmed that the secondary star had a high level of magnetic activity. The retrograde longitudinal motion of the spot can be explained by a solar-like differential rotation in the secondary component. The orbital period investigation revealed that OO Leo is undergoing a secular decrease and a cyclic variation in its orbital period. The secular decrease may be mainly caused by mass transfer from the more massive secondary star to the less massive primary star. The cyclic period variation can be explained by the light–time effect of an invisible third body or the cyclic magnetic activity of the secondary star. The long-lived spot migration in the longitudinal direction makes OO Leo an excellent target for investigating the differential rotations of contact binaries.
Toward a Live Homogeneous Database of Solar Active Regions Based on SOHO/MDI and SDO/HMI Synoptic Magnetograms. II. Parameters for Solar Cycle Variability
Authors: Wang Ruihui , Jiang Jie , Luo Yukun 
Published: August 2024

Abstract
Solar active regions (ARs) determine solar polar fields and cause solar cycle variability within the framework of the Babcock–Leighton dynamo. The contribution of an AR to the polar field is measured by its dipole field, which results from flux emergence and subsequent flux transport over the solar surface. The dipole fields contributed by an AR before and after the flux transport are referred to as the initial and final dipole fields, respectively. For a better understanding and prediction of solar cycles, in this paper, we provide a database including AR's initial and final dipole fields and the corresponding results of their bipolar magnetic region (BMR) approximation from 1996 onward. We also identify the repeated ARs and provide the optimized transport parameters. Based on our database, we find that although the commonly used BMR approximation performs well for the initial dipole field, it exhibits a significant deviation for the final dipole field. To accurately assess an AR’s contribution to the polar field, the final dipole field with its real configuration should be applied. Despite the notable contributions of a few rogue ARs, approximately the top 500 ARs ordered by their final dipole fields are necessary to derive the polar field at the cycle minimum. While flux transport may increase or decrease the dipole field for an individual AR, its collective impact over all ARs in a cycle is a reduction in their total dipole field.