bluuebunny/crossref_metadata_2025_split huggingface dataset:
Analisis Ketepatan Kode Diagnosis Kasus Persalinan Secara Sectio Caesarea Di Rumah Sakit Pelabuhan Jakarta
Authors: Anggraini Adelia , Widjaja Lily , Indawati Laela , Rosmala Dewi Deasy 
Published: January 2023

Salah satu aspek terpenting dalam pelayanan rekam medis adalah kegiatan klasifikasi dan kodefikasi diagnosis serta tindakan. Dalam melakukan pemberian kode diagnosis pasien, petugas koding mengacu pada aturan ICD-10. Berdasarkan aturan ICD-10 kasus persalinan terdiri atas tiga komponen yaitu kondisi atau penyulit (O00-O99), metode persalinan (O80-O84), dan outcome of delivery (Z37.-) yang digunakan sebagai kode tambahan untuk mengetahui hasil persalinan. Tujuan dalam penelitian yaitu untuk mengetahui ketepatan kode diagnosis kasus persalinan secara sectio caeasrea di Rumah Sakit Pelabuhan Jakarta. Penelitian menggunakan analisis deskriptif dengan pendekatan kuantitatif. Dengan sampel sebanyak 70 rekam medis kasus persalinan secara sectio caesarea di Rumah Sakit Pelabuhan Jakarta. Pada penelitian ini didapati hasil komponen atau penyulit ibu dengan ketepatan 90% (63 RM), lalu metode persalinan dengan ketepatan 11,43% (8 RM). Serta outcome of delivery yang memiliki ketepatan 0% (70 RM). Berdasarkan hasil wawancara dan observasi terhadap kepala rekam medis dan koder bahwa ketepatan pengodean dapat dipengaruhi oleh faktor 5M (man, money, material, method, machine), yaitu ketelitian koder dalam melakukan pengodean, kejelasan pada tulisan dokter, serta tersedianya SPO yang memiliki catatan khusus mengenai pengodean kasus persalinan sehingga proses pengodean dapat terstruktur dengan baik.
Między egzaminem a widowiskiem: Uczniowskie popisy publiczne na przykładzie Gimnazjum/Liceum Wołyńskiego
Authors: Buczek Katarzyna 
Published: January 2023

Organizowane w Gimnazjum i Liceum Wołyńskim w Krzemieńcu egzaminy publiczne zwane popisami nawiązywały do wielowiekowej tradycji edukacyjnej. Organizowane na zakończenie roku szkolnego, po decydujących o promocji do następnej klasy egzaminach wewnętrznych, miały być z jednej strony promocją szkoły, z drugiej popularyzacją wiedzy. Jednak nie bez znaczenia była ich widowiskowość, zwłaszcza gdy gromadzący się widzowie – rodziny uczniów i mieszkańcy Krzemieńca nie mieli odpowiedniego wykształcenia, by ocenić i docenić walory czysto naukowe. Podczas popisów uczniowie zachowywali się jak artyści. W reprezentacyjnej sali szkoły wychodzili na podwyższenie – scenę i prezentowali wyuczone odpowiedzi na pytania, które wcześniej znali. Zachowane w pamiętnikach relacje świadczą o tym, że publiczne egzaminy były dla mieszkańców Krzemieńca i okolic rozrywką i atrakcją, na którą czekano cały rok.
Detección canina de anaplasma platys mediante PCR en tiempo real
Authors: Tintel A María José , Arze Selich Paola , Rolón Miriam Soledad , Vega Gómez Celeste 
Published: January 2023

Anaplasma platys es una bacteria pleomórfica intracelular, gramnegativa obligada que afecta especialmente a las plaquetas del perro, transmitida principalmente por garrapatas. Patógeno de importancia relevante en medicina veterinaria y reconocido mundialmente por su potencial zoonótico. El objetivo del trabajo fue determinar por PCR a tiempo real la presencia de A. platys en un canino de Asunción. Destacamos que es la primera evidencia molecular de A. platys en el país utilizando el método de qPCR, cuya secuenciación del producto obtenido confirmó la infección por CP046391.1 Anaplasma Platys con homología 100%. El desarrollo del método qPCR contribuye al avance de la investigación con A. platys, constituyendo una herramienta más sensible y específica para situaciones que indiquen una posible enfermedad clínica, pero con métodos diagnósticos tradicionales como citología sanguínea o serología negativa.
Correlations in Chromospheric and Coronal Activity Indicators of Giant Stars
Authors: Crandall Sara , Smith Graeme H. 
Published: January 2023

Abstract
The main goal of this paper is to use ultraviolet photometry from the Galaxy Evolution Explorer (GALEX) satellite to study chromospheric activity among red giant and core-helium-burning (CHeB) stars. Correlations are sought between several chromospheric and coronal activity indicators for giants that were detected in soft X-rays by the ROentgen SATellite. There is an evident correlation between

log
(

L

X

/

L

bol

)

and

log
(

F

Mg

II

/

F

bol

)

, where L
X is the X-ray luminosity and F
Mg II
is the flux from Mg ii
h and k emission lines, although there is substantial scatter. Using GALEX far-ultraviolet (FUV) magnitudes, the relationship between an FUV-excess parameter (a proxy for chromospheric and transition-region emission lines) and X-ray luminosity is documented. Correlations found herein are not strong, and may be linked to binarity. There is a varied range of FUV emission among CHeB stars, indicating that giants in this phase may be exhibiting differences or cycles in outer atmospheric activity. Additionally, efforts were made to constrain a relationship between excess FUV and near-ultraviolet emission and the projected surface rotation velocity,

v
sin
i

, of giants. No clear relationship was found. Obscurities in this relationship may result from a spread in

sin
i

inclinations, and/or too few stars with

v
sin
i
>
7

km s−1.
The Pan-STARRS1 z > 5.6 Quasar Survey. III. The z ≈ 6 Quasar Luminosity Function
Authors: Schindler Jan-Torge , Bañados Eduardo , Connor Thomas , Decarli Roberto , Fan Xiaohui , Farina Emanuele Paolo , Mazzucchelli Chiara , Nanni Riccardo , Rix Hans-Walter , Stern Daniel , Venemans Bram P. , Walter Fabian 
Published: January 2023

Abstract
We present the z ≈ 6 type-1 quasar luminosity function (QLF), based on the Pan-STARRS1 (PS1) quasar survey. The PS1 sample includes 125 quasars at z ≈ 5.7–6.2, with −28 ≲ M
1450 ≲ −25. With the addition of 48 fainter quasars from the SHELLQs survey, we evaluate the z ≈ 6 QLF over −28 ≲ M
1450 ≲ −22. Adopting a double power law with an exponential evolution of the quasar density (Φ(z) ∝ 10
k(z−6); k = −0.7), we use a maximum likelihood method to model our data. We find a break magnitude of

M

*

=
−

26.38

−
0.60

+
0.79

mag

, a faint-end slope of

α
=
−

1.70

−
0.19

+
0.29

, and a steep bright-end slope of

β
=
−

3.84

−
1.21

+
0.63

. Based on our new QLF model, we determine the quasar comoving spatial density at z ≈ 6 to be

n
(

M

1450

<
−
26
)
=

1.16

−
0.12

+
0.13

cGpc

−
3

. In comparison with the literature, we find the quasar density to evolve with a constant value of k ≈ −0.7, from z ≈ 7 to z ≈ 4. Additionally, we derive an ionizing emissivity of

ϵ

912

(
z
=
6
)
=

7.23

−
1.02

+
1.65

×

10

22

erg

s

−
1

Hz

−
1

cMpc

−
3

, based on the QLF measurement. Given standard assumptions, and the recent measurement of the mean free path by Becker et al. at z ≈ 6, we calculate an H i photoionizing rate of ΓH I(z = 6) ≈ 6 × 10−16 s−1, strongly disfavoring a dominant role of quasars in hydrogen reionization.
The Ionizing Spectra of Extremely Metal-poor O Stars: Constraints from the Only H ii Region in Leo P
Authors: Telford O. Grace , McQuinn Kristen B. W. , Chisholm John , Berg Danielle A. 
Published: January 2023

Abstract
Metal-poor, star-forming dwarf galaxies produce extreme nebular emission and likely played a major role in cosmic reionization. Yet, determining their contribution to the high-redshift ionizing photon budget is hampered by the lack of observations constraining the ionizing spectra of individual massive stars more metal-poor than the Magellanic Clouds (20%–50% Z
⊙). We present new Keck Cosmic Web Imager (KCWI) optical integral field unit spectroscopy of the only H ii region in Leo P (3% Z
⊙), which is powered by a single O star. We calculate the required production rate of photons capable of ionizing hydrogen and helium from the observed Hβ and He i
λ4471 emission-line fluxes. Remarkably, we find that the ionizing photon production rate and spectral hardness predicted by a tlusty model fit to the stellar spectral energy distribution agrees with our observational measurements within the uncertainties. We then fit Cloudy photoionization models to the full suite of optical emission lines in the KCWI data and show that the shape of the same tlusty ionizing continuum simultaneously matches lines across a wide range of ionization energies. Finally, we detect O iii] and N iii] nebular emission in the Hubble Space Telescope far-ultraviolet spectrum of the Leo P H ii region, and highlight that the rarely observed N iii] emission cannot be explained by our Cloudy models. These results provide the first observational evidence that widely used, yet purely theoretical, model spectra accurately predict the ionizing photon production rate from late-O stars at very low metallicity, validating their use to model metal-poor galaxies both locally and at high redshift.
Quijote-PNG: Simulations of Primordial Non-Gaussianity and the Information Content of the Matter Field Power Spectrum and Bispectrum
Authors: Coulton William R , Villaescusa-Navarro Francisco , Jamieson Drew , Baldi Marco , Jung Gabriel , Karagiannis Dionysios , Liguori Michele , Verde Licia , Wandelt Benjamin D. 
Published: January 2023

Abstract
Primordial non-Gaussianity (PNG) is one of the most powerful probes of the early universe, and measurements of the large-scale structure of the universe have the potential to transform our understanding of this area. However, relating measurements of the late-time universe to the primordial perturbations is challenging due to the nonlinear processes that govern the evolution of the universe. To help address this issue, we release a large suite of N-body simulations containing four types of PNG: quijote-png. These simulations were designed to augment the quijote suite of simulations that explored the impact of various cosmological parameters on large-scale structure observables. Using these simulations, we investigate how much information on PNG can be extracted by extending power spectrum and bispectrum measurements beyond the perturbative regime at z = 0.0. This is the first joint analysis of the PNG and cosmological information content accessible with power spectrum and bispectrum measurements of the nonlinear scales. We find that the constraining power improves significantly up to

k

max

≈
0.3
h

Mpc

−
1

, with diminishing returns beyond as the statistical probes signal-to-noise ratios saturate. This saturation emphasizes the importance of accurately modeling all the contributions to the covariance matrix. Further, we find that combining the two probes is a powerful method of breaking the degeneracies with the ΛCDM parameters.
Narrow Fe–Kα Reverberation Mapping Unveils the Deactivated Broad-line Region in a Changing-look Active Galactic Nucleus
Authors: Noda Hirofumi , Mineta Taisei , Minezaki Takeo , Sameshima Hiroaki , Kokubo Mitsuru , Kawamuro Taiki , Yamada Satoshi , Horiuchi Takashi , Matsumoto Hironori , Watanabe Makoto , Morihana Kumiko , Itoh Yoichi , Kawabata Koji S. , Fukazawa Yasushi 
Published: January 2023

Abstract
“Changing-look active galactic nuclei” (CLAGNs) are known to change their apparent types between types 1 and 2, usually accompanied by a drastic change in their luminosity on timescales of years. However, it is still unclear whether materials in broad-line regions (BLRs) in CLAGNs appear and disappear during the type-transition or remain at the same location while the line production is simply activated or deactivated. Here we present our X-ray–optical monitoring results of a CLAGN, NGC 3516, by Suzaku, Swift, and ground telescopes, with our primary focus on the narrow Fe–Kα emission line, which is an effective probe of the BLR materials. We detected significant variations of the narrow Fe–Kα line on a timescale of tens of days during the type-2 (faint) phase in 2013–2014, and conducted “narrow Fe–Kα reverberation mapping,” comparing its flux variation with those of the X-ray continuum from a corona and B-band continuum from an accretion disk. We derived, as a result, a time lag of

10.1

−
5.6

+
5.8

days (1σ errors) for the Fe–Kα line behind the continuum, which is consistent with the location of the BLR determined in optical spectroscopic reverberation mapping during the type-1 (bright) phase. This finding shows that the BLR materials remained at the same location without emitting optical broad lines during the type-2 phase. Considering the drastic decrease of the radiation during the type-transition, our result is possibly inconsistent with the hotly discussed formation models of the BLR, which propose that the radiative pressure from an accretion disk should be the main driving force.
The Orion OB Association as a Generator for the Hot Circumgalactic Medium
Authors: Fuller Chase A. , Kaaret Philip , Bluem Jesse , Kuntz K. D. , Hodges-Kluck Edmund , Jahoda Keith M. 
Published: January 2023

Abstract
Feedback from star formation may play a key role in energizing the hot, diffuse, X-ray emitting circumgalactic medium (CGM). We observed the diffuse hot gas on the interior of the Orion–Eridanus Superbubble (OES) produced by feedback from the Orion OB association. Using HaloSat, a CubeSat X-ray observatory, we cover the majority of the OES using 11 HaloSat fields, each with a 10° diameter. We find the gas is well described by two thermal plasma components. There are regions of enhanced emission measure (EM) that coincide with the Eridanus X-ray Enhancement and the Orion OB association. Individual field temperatures are statistically consistent with the weighted average of all of the OES fields: a warm temperature kT

w
= 0.17 ± 0.02 keV and a hot temperature kT

h
= 0.79 ± 0.12 keV. The gas is overpressured in comparison with typical interstellar medium pressures, and the rate of energy injected by Orion OB1 can sufficiently power growth of the superbubble. The gas’s radiative cooling timescale (∼30 Myr) is long in comparison with the rate of hot gas production. The temperatures and EMs of the gas agree with properties of the bulk CGM elsewhere in the Milky Way. If we take the OES as a typical superbubble, these factors together suggest that the hot CGM is energized by star formation activity.
The Contribution of Evolved Stars to Polycyclic Aromatic Hydrocarbon Heating and Implications for Estimating Star Formation Rates
Authors: Zhang Lulu , Ho Luis C. 
Published: January 2023

Abstract
Emission from polycyclic aromatic hydrocarbons (PAHs) is a promising tool for estimating star formation rate (SFR) in galaxies, but the origin of its sources of excitation, which include not only young but possibly also old stars, remains uncertain. We analyze Spitzer mid-infrared mapping-mode spectroscopic observations of the nuclear and extranuclear regions of 33 nearby galaxies to study the contribution of evolved stars to PAH emission. In combination with photometric measurements derived from ultraviolet, Hα, and infrared images, the spatially resolved spectral decomposition enables us to characterize the PAH emission, SFR, and stellar mass of the sample galaxies on subkiloparsec scales. We demonstrate that the traditional empirical correlation between PAH luminosity and SFR has a secondary dependence on specific SFR, or, equivalently, stellar mass. Ultraviolet-faint regions with lower specific SFRs and hence a greater fraction of evolved stars emit stronger PAH emission at fixed SFR than ultraviolet-bright regions. We reformulate the PAH-based SFR estimator by explicitly introducing stellar mass as a second parameter to account for the contribution of evolved stars to PAH excitation. The influence of evolved stars can explain the sublinear correlation between PAH emission and SFR, and it can partly account for the PAH deficit in dwarf galaxies and low-metallicity environments.
NEOWISE Variability of the New Gaia Herbig Ae/Be and Classical Be Stars—Variability Sample and Statistical Analysis
Authors: Mei Ying , Song Shi-Ming , Liu Jun-Ting , Hyland Lucas J. , Chen Xi 
Published: January 2023

Abstract
Light variability is an essential attribute of young stellar objects (YSOs) at the pre-main-sequence (PMS) stage, which can be treated as an indicator to trace star formation. We present a statistical study on the infrared NEOWISE variability of new and large-sized PMS stars as well as Herbig Ae/Be (HAeBe) and classical Be (CBe) stars identified from Gaia Data Release 2. A total of 3792 (including 714 HAeBe), 417, and 473 NEOWISE variable sources were detected from the catalog of 8470 PMS (including 1361 HAeBe), 693 CBe, and 1309 uncertain (possibly belonging to either HAeBe or CBe) stars, respectively. We found that 80% of the PMS variables are dominated by irregular infrared variability, whereas variables in the CBe and uncertain categories exhibit comparable contributions from secular (linear, curved, and periodic) and stochastic (burst, drop, and irregular) variables. This, in combination with infrared W1–W2 colors, W4 luminosities, and the spectral energy distribution slope at near- and mid-infrared wavelengths, suggests different evolutionary stages of the PMS (including HAeBe), uncertain, and CBe stars, from less to more evolved. A statistical analysis of variable source properties (e.g., period and fractional amplitude) further reveals a potential sequence possibly associated with disk evolution for different types of light curves (from linear, to curved, periodic, stochastic, and nonvariable stars). Possible mechanisms for the variable sources are suggested to be related to either extinction via circumstellar matter, or contribution of multiple systems surrounding the YSOs, as opposed to variable accretion (e.g., episodic accretion or accretion burst).
TESS Timings of 31 Hot Jupiters with Ephemeris Uncertainties
Authors: Shan Su-Su , Yang Fan , Lu You-Jun , Wei Xing , Tian Wen-Wu , Zhang Hai-Yan , Guo Rui , Cui Xiao-Hong , Yang Ai-Yuan , Zhang Bo , Liu Ji-Feng 
Published: January 2023

Abstract
A precise transit ephemeris serves as the premise for follow-up exoplanet observations. We compare TESS Object of Interest (TOI) transit timings of 262 hot Jupiters with the archival ephemeris and find 31 of them having TOI timing offsets, among which WASP-161b shows the most significant offset of −203.7 ± 4.1 minutes. The median value of these offsets is 17.8 minutes, equivalent to 3.6σ. We generate TESS timings in each sector for these 31 hot Jupiters, using a self-generated pipeline. The pipeline performs photometric measurements to TESS images and produces transit timings by fitting the light curves. We refine and update the previous ephemeris, based on these TESS timings (uncertainty ∼1 minute) and a long timing baseline (∼10 yr). Our refined ephemeris gives the transit timing at a median precision of 0.82 minutes until 2025 and 1.21 minutes until 2030. We regard the timing offsets to mainly originate from the underestimated ephemeris uncertainty. All the targets with timing offset larger than 10σ present earlier timings than the prediction, which cannot be due to underestimated ephemeris uncertainty, apsidal precision, or Rømer effect as those effects should be unsigned. For some particular targets, timing offsets are likely due to tidal dissipation. Our sample leads to the detection of period-decaying candidates of WASP-161b and XO-3b reported previously.
A Data-constrained Scheme for the Reconstruction of Solar Wind Parameters in the Inner Heliosphere
Authors: Zhang Man , Feng Xueshang , Yang Liping , Liu Xiaojing 
Published: January 2023

Abstract
With the development of our industrial society, the reconstruction of solar wind parameters in the inner heliosphere becomes very important to understanding the interplanetary propagation of various types of space weather disturbance. However, the situ observations of solar wind parameters are only applicable to several points where spacecraft are located. Therefore, we have to rely on the numerical technologies to reconstruct the solar wind parameters. The scheme for the reconstruction of solar wind parameters can be classified into two categories: one is based on the remote-sensing data at the Sun, and the other is based on the in situ data at 1 au. In this paper, the solar wind parameters in the inner heliosphere are reconstructed with magnetohydrodynamic simulations from 20 R

s
to 1 au. The inner boundary conditions are constrained by Wind observations at 1 au. The modeled results are compared with data from multispacecraft observations, such as those by Parker Solar Probe, Solar Orbiter, and the Solar Terrestrial Relations Observatory A and B. The results show that the solar wind parameters obtained with this new scheme agree with the in situ observations much better, which will provide a more realistic configuration for the study of various types of space weather disturbance in future.
Transitions chez des personnes transgenres et dimensions surmoïques, entre seconde peau et moi-peau corsets
Authors: Guichard Agathe , Jean-Dit-Pannel Romuald 
Published: January 2023

Selon différentes conceptions du genre et des parcours de transition, toujours singulières mais empreintes d’attentes sociales, l’enveloppe corporelle du sujet transgenre se métamorphose. Lors d’entretiens de recherche et d’épreuves projectives (Rorschach et tat ), deux jeunes adultes transgenres aux profils psychopathologiques névrotiques présentaient une sensibilité marquée aux normes, à la morale et aux attentes sociétales. La légitimité, la culpabilité et la honte étaient des problématiques redondantes. Différents temps de transitions subjectives, familiales, sociales et corporelles se sont trouvés en jeu : le passage à l’âge adulte, une vie étudiante hors du giron familial. Ces deux situations illustrent une discussion sur les transitions du corps et des enveloppes chez des sujets transgenres, entre seconde peau et moi-peau corsets.
Une écriture du déchirement : le polyhandicap sévère
Authors: Louise-Julie Marie-Line 
Published: January 2023

Au polyhandicap sévère, la société a réagi de trois manières différentes : par une « hémiplégie » visuelle d’abord, en l’ignorant, par une atteinte de son narcissisme, liée à sa culpabilité de le rejeter, et par une effraction enfin des enveloppes familiales. Pour les familles et les équipes éducatives, c’est la rencontre pérenne avec la différence, le traumatisme, mais aussi avec le déni. Même si historiquement cette prise en compte évolue, un travail de lien est à réaliser, ce que l’auteure illustre par diverses situations issues de sa pratique.
L’« Accordanse » mère-bébé dans un bain sensoriel et émotionnel en dépression
Authors: Stella Lucia 
Published: January 2023

La dépression hante notre contemporanéité. « Mal du siècle », elle envahit notamment les lieux de consultation et services hospitaliers accueillant les bébés et leurs parents. Les recherches montrent les impacts de la dépression maternelle sur le développement de l’enfant et la nécessité d’accompagner le processus de parentalité dans ce cas de figure. Après quelques repères théoriques autour de la dépression maternelle et/ou conjointe, l’article propose une thérapeutique qui s’est révélée efficace. Il s’agit d’Accordanse : un dispositif de soin et de recherche accueillant des mères et leurs bébés en souffrance psychique centré sur la danse. Quelques séquences cliniques permettront de mieux mesurer dans quelle mesure la danse soutient la construction d’une chorégraphie des interactions harmonieusement accordée lorsque celle-ci est « empêchée » par la lourdeur de la dépression.
L’enfant sur le pont. Figures du handicap
Authors: Ben Soussan Patrick 
Published: January 2023

À partir d’une rencontre singulière avec un enfant handicapé sur un pont, l’auteur, vieux briscard de la pédopsychiatrie, ayant exercé des années en périnatalité et dans le champ du handicap, rappelle avec force les représentations qui nous assaillent face aux figures de l’altérité et nous rappelle que toute clinique du handicap dialogue avec des parts bien sépulcrales et parfois insoupçonnées de notre Moi.