bluuebunny/crossref_metadata_2025_split huggingface dataset:
Subjective Well Being Wanita Terlantar Pada Era New Normal Pandemi Covid-19 di Panti Sosial Perlindungan Jakarta
Authors: Yani Devi Antap , Sovitriana Rilla 
Published: November 2022

Penelitian ini bertujuan untuk mengetahui ada hubungan dukungan sosial temansebaya dan optimisme dengan subjective well being pada wanita terlantar yang beradadi Panti Sosial Perlindungan Bhakti Kasih. Jumlah sampel yang digunakan padapenelitian ini adalah wanita terlantar di Panti Sosial Perlindungan Bhakti Kasih yangberjumlah 92 orang. Pengujian hipotesis menggunakan teknik analisa bivariatecorrelation dan multivariate correlation dengan menggunakan SPSS forwindows. Teknik pengambilan sampel mengggunakan metode sampel jenuhyaitu teknik penentuan sampel bila semua anggota populasi digunakan menjadisampel. Pengambilan data sampel dilakukan dengan menggunakan penyebarankuisioner mengenai dukungan sosial teman sebaya dan optimisme dengan subjectivewell being. Berdasarkan analisis data yang dilakukan dengan bivariate correlation,diketahui hasil koefisien korelasi antara dukungan sosial teman sebaya dengansubjective well being sebesar r = 0,469 dengan taraf signifikansi 0,000 (p<0,05)artinya terdapat hubungan positif antara dukungan sosial teman sebaya dengansubjective well being dan hasil korelasi antara hubungan optimisme dengansubjective well being sebesar r = 0,394 dengan taraf signifikansi 0,000 (p<0,05)artinya terdapat hubungan yang positif antara optimisme dengan subjective wellbeing, sedangkan hasil analisis yang dilakukan dengan multivariate correationhasil korelasi antara hubungan dukungan sosial dan optimisme dengan subjective wellbeing sebesar R = 0,507 dengan taraf signifikasi sebesar 0,000 (p<0,05) artinyaterdapat hubungan yang positif antara dukungan sosial teman sebaya dan optimismedengan subjective well being. Dimana berdasarkan hasil uji analisa regresi denganmetode enter diperoleh nilai R2 = 0,257 yang menunjukkan bahwa variabel dukungan sosial teman sebaya dan optimisme berkontribusi sebesar 25,7%terhadap varibel subjective well being.
NGC 6153: Reality is Complicated*
Authors: Richer Michael G. , Arrieta Anabel , Arias Lorena , Castañeda-Carlos Lesly , Torres-Peimbert Silvia , López José Alberto , Galindo Adolfo 
Published: November 2022

Abstract
We study the kinematics of emission lines that arise from many physical processes in NGC 6153 based upon deep, spatially resolved, high-resolution spectra acquired with the UVES spectrograph at the European Southern Observatory Very Large Telescope. Our most basic finding is that the plasma in NGC 6153 is complex, especially its temperature structure. The kinematics of most emission lines defines a classic expansion law, with the outer part expanding fastest (normal nebular plasma). However, the permitted lines of O i, C ii, N ii, O ii, and Ne ii present a constant expansion velocity that defines a second kinematic component (additional plasma component). The physical conditions imply two plasma components, with the additional plasma component having lower temperature and higher density. The [O ii] density and the [N ii] temperature are anomalous, but may be understood considering the contribution of recombination to these forbidden lines. The two plasma components have very different temperatures. The normal nebular plasma appears to have temperature fluctuations in part of its volume (main shell), but only small fluctuations elsewhere. The additional plasma component contains about half of the mass of the N2+ and O2+ ions, but only 3%–5% of the mass of H+ ions, so the two plasma components have very different chemical abundances. We estimate abundances of

12
+
log
(

O

2
+

/

H

+

)
∼
9.2

dex and He/H ∼ 0.13. Although they are all complications, multiple plasma components, temperature fluctuations, and the contributions of multiple physical processes to a given emission line are all part of the reality in NGC 6153, and should generally be taken into account.
Solar-cycle-related Variation of Differential Rotation of the Chromosphere
Authors: Wan Miao , Gao Peng-xin 
Published: November 2022

Abstract
Solar-cycle-related variation of the solar chromospheric rotation is studied by analyzing the chromospheric rotation rate of 938 synoptic maps generated from the Ca ii K line at the Mount Wilson Observatory during the period of 1915 August 10 to 1985 July 7. The results obtained are as follows: (1) The parameters A (the equatorial rotation rate) and B (the latitudinal gradient of rotation) in the standard form of differential rotation both show a decreasing trend in the considered time frame, although A has weak statistical significance. (2) There is a significant negative correlation between the level of solar activity and parameter B, indicating that there seems to be a correlation between field strength and chromospheric differential rotation. (3) During solar cycles 15, 16, 19, 20, and 21, the southern hemisphere rotates faster, whereas in cycles 17 and 18, the northern hemisphere rotates faster. (4) There exists a significant negative correlation between the N–S asymmetry of the chromospheric rotation rate and that of solar activity, indicating that differential rotation of the chromosphere seems to be strengthened by stronger magnetic activity in a certain hemisphere. Possible explanations for the above results are given.
X-Ray Reverberation Mapping of Ark 564 Using Gaussian Process Regression
Authors: Lewin Collin , Kara Erin , Wilkins Dan , Mastroserio Guglielmo , García Javier A. , Zhang Rachel C. , Alston William N. , Connors Riley , Dauser Thomas , Fabian Andrew , Ingram Adam , Jiang Jiachen , Lohfink Anne , Lucchini Matteo , Reynolds Christopher S. , Tombesi Francesco , Klis Michiel van der , Wang Jingyi 
Published: November 2022

Abstract
Ark 564 is an extreme high-Eddington narrow-line Seyfert 1 galaxy, known for being one of the brightest, most rapidly variable soft X-ray active galactic nuclei (AGN), and for having one of the lowest temperature coronae. Here, we present a 410 ks NuSTAR observation and two 115 ks XMM-Newton observations of this unique source, which reveal a very strong, relativistically broadened iron line. We compute the Fourier-resolved time lags by first using Gaussian processes to interpolate the NuSTAR gaps, implementing the first employment of multitask learning for application in AGN timing. By simultaneously fitting the time lags and the flux spectra with the relativistic reverberation model reltrans, we constrain the mass at

2.3

−
1.3

+
2.6

×

10

6

M

⊙

, although additional components are required to describe the prominent soft excess in this source. These results motivate future combinations of machine learning, Fourier-resolved timing, and the development of reverberation models.
Optical Variability of Eight FRII-type Quasars with 13 yr Photometric Light Curves
Authors: Kuźmicz Agnieszka , Goyal Arti , Zola Stanisław , Jamrozy Marek , Dróżdż Marek , Ogłoza Waldemar , Siwak Michał , Reichart Daniel E. , Kouprianov Vladimir V. , Caton Daniel B. 
Published: November 2022

Abstract
We characterize the optical variability properties of eight lobe-dominated radio quasars (QSOs): B2 0709+37, FBQS J095206.3+235245, PG 1004+130, [HB89] 1156+631, [HB89] 1425+267, [HB89] 1503+691, [HB89] 1721+343, and 4C +74.26, systematically monitored for a duration of 13 yr since 2009. The quasars are radio-loud objects with extended radio lobes that indicate their orientation close to the sky plane. Five of the eight QSOs are classified as giant radio quasars. All quasars showed variability during our monitoring, with magnitude variations between 0.3 and 1 mag for the least variable and the most variable QSOs, respectively. We performed both structure function (SF) analysis and power spectral density (PSD) analysis for the variability characterization and search for characteristic timescales and periodicities. As a result of our analysis, we obtained relatively steep SF slopes (α ranging from 0.49 to 0.75) that are consistent with the derived PSD slopes (∼2–3). All the PSDs show a good fit to single power-law forms, indicating a red-noise character of variability between timescales of ∼13 yr and weeks. We did not measure reliable characteristic timescales of variability from the SF analysis, which indicates that the duration of the gathered data is too short to reveal them. The absence of bends in the PSDs (change of slope from ≥1 to ∼0) on longer timescales indicates that optical variations are most likely caused by thermal instabilities in the accretion disk.
Has JWST Already Falsified Dark-matter-driven Galaxy Formation?
Authors: Haslbauer Moritz , Kroupa Pavel , Zonoozi Akram Hasani , Haghi Hosein 
Published: November 2022

Abstract
The James Webb Space Telescope (JWST) discovered several luminous high-redshift galaxy candidates with stellar masses of M
* ≳ 109
M
⊙ at photometric redshifts z
phot ≳ 10, which allows to constrain galaxy and structure formation models. For example, Adams et al. identified the candidate ID 1514 with

log

10

(

M

*

/

M

⊙

)
=

9.8

−
0.2

+
0.2

located at

z

phot

=

9.85

−
0.12

+
0.18

and Naidu et al. found even more distant candidates labeled as GL-z11 and GL-z13 with

log

10

(

M

*

/

M

⊙

)
=

9.4

−
0.3

+
0.3

at

z

phot

=

10.9

−
0.4

+
0.5

and

log

10

(

M

*

/

M

⊙

)
=

9.0

−
0.4

+
0.3

at

z

phot

=

13.1

−
0.7

+
0.8

, respectively. Assessing the computations of the IllustrisTNG (TNG50-1 and TNG100-1) and EAGLE projects, we investigate if the stellar mass buildup as predicted by the ΛCDM paradigm is consistent with these observations assuming that the early JWST calibration is correct and that the candidates are indeed located at z ≳ 10. Galaxies formed in the ΛCDM paradigm are by more than an order of magnitude less massive in stars than the observed galaxy candidates implying that the stellar mass buildup is more efficient in the early universe than predicted by the ΛCDM models. This in turn would suggest that structure formation is more enhanced at z ≳ 10 than predicted by the ΛCDM framework. We show that different star formation histories could reduce the stellar masses of the galaxy candidates alleviating the tension. Finally, we calculate the galaxy-wide initial mass function (gwIMF) of the galaxy candidates assuming the integrated galaxy IMF theory. The gwIMF becomes top-heavy for metal-poor star-forming galaxies decreasing therewith the stellar masses compared to an invariant canonical IMF.
Quick-look Pipeline Light Curves for 5.7 Million Stars Observed Over the Second Year of TESS’ First Extended Mission
Authors: Kunimoto Michelle , Tey Evan , Fong Willie , Hesse Katharine , Shporer Avi , Fausnaugh Michael , Vanderspek Roland , Ricker George 
Published: November 2022

Abstract
We present High-Level Science Products (HLSPs) containing light curves from MIT's Quick-Look Pipeline (QLP) from the second year of Transiting Exoplanet Survey Satellite (TESS’) first Extended Mission (Sectors 40–55; 2021 July–2022 September). In total, 12.2 million per-sector light curves for 5.7 million unique stars were extracted from 10 minutes cadence Full-Frame Images (FFIs) and are made available to the community. As in previous deliveries, QLP HLSPs include both raw and detrended flux time series for all observed stars brighter than TESS magnitude T = 13.5 mag. Starting in Sector 41, QLP also produces light curves for select fainter M dwarfs. QLP has provided the community with one of the largest sources of FFI-extracted light curves to date since the start of the TESS mission.
A Prospective Study to Determine the Incidence, Clinical Profile, and Outcomes of Patients with Ventilator-Associated Pneumonia
Authors: Bhattacharjee Sagnik , Khyriem Annie B. , Lyngdoh Clarissa Jane , Prasad Abhijit Kumar 
Published: November 2022

Objective:
The objective was to determine the incidence, etiological agents, and antibiotic susceptibility pattern of isolates causing ventilator-associated pneumonia (VAP).

Methods:
The prospective observational study was carried out on 146 adults admitted to the hospital, who were put on mechanical ventilation for a minimum period of 48 h at NEIGRIHMS, Shillong. The study was conducted for 1 year from December 2019 to December 2020. VAP was diagnosed as per the Clinical Pulmonary Infection Score. Demographic, clinical characteristics, culture reports, and antibiotic susceptibility of the patients were noted. Patients were followed up till discharge or death. Outcome measures were risk factors for VAP and mortality.

Results:
We report an incidence of VAP as 10.6/1000 ventilator days. The predominant organisms seen were Acinetobacter baumannii (62.33%), Klebsiella pneumoniae (47.26%), and Pseudomonas aeruginosa (19.18%). 33/146 (22.6%) patients expired, among which 17 patients had VAP (40.48% vs. 15.38%, P = 0.001). VAP patients had significantly higher odds of smoking (odds ratio [OR] = 2.412, P = 0.016), more polybacterial infections (OR = 2.271, P = 0.024), and more mortality (OR = 3.681, P = 0.001). Among the organisms, P. aeruginosa (OR = 0.115, P = 0.013) and K. pneumoniae (OR = 6.818, P = 0.003) were significantly associated with mortality in patients with VAP.

Conclusion:
We report an incidence of VAP as 10.6/1000 ventilator days among intensive care unit patients. Smoking was a significant risk factor for VAP. VAP patients had a significantly higher risk of mortality with K. pneumoniae and P. aeruginosa being significant organisms responsible for it.
Serological screening of celiac disease in children and adolescents with juvenile idiopathic arthritis
Authors: Abdelgalil Abobakr A. , Tarek Sara 
Published: November 2022

Background
Patients with juvenile idiopathic arthritis (JIA) seem to be at higher risk of developing immune-mediated diseases like celiac disease (CD) than general population.

Aim
The aim of this study was to detect the prevalence of CD among children and adolescents with JIA.

Patients and methods
We carried out a cross-sectional study that included 42 JIA patients under the age of 16 years. In addition to demographic, clinical, and laboratory data, anti-tissue transglutaminase immunoglobulin A (anti-TTG IgA) antibodies were measured using a novel chemiluminescent immunoassay.

Results
Only one (2.4%) patient had positive anti-TTG IgA. There was no significant correlation between anti-TTG IgA and terms of growth parameters, JIA subtype, or medications.

Conclusion
JIA patients seem to be at higher risk to develop CD. Being mostly asymptomatic, they should be candidates for periodic screening. Methodologically standardized larger studies are recommended to reach a cost-effective protocol for monitoring JIA patients regarding the development of CD, adding to early diagnosis and control of the disease.
Effect of Prana vidya Practices on Intelligence Quotient and Performance Quotient of Adolescents
Authors: Prabhu Prem , Gowda Paran , Chandra Girish 
Published: November 2022

Background:
Intelligence is one of the most important aspects of one's consciousness. Various practices have been given in yogic texts to develop human consciousness in its entirety. The present study assesses whether Prana vidya practices (PVPs) are effective for the enhancement of intelligence in adolescents. Various studies have established that prana-related practices such as pranayama and pranic healing have played an important role in the prevention and treatment of various aspects of human health.

Aim:
To study the effect of PVPs on the intelligence quotient (IQ) and performance quotient (PQ) of adolescents.

Materials and Methods:
The present study was a randomized control trial, conducted to find the effect of 5-week Prana vidya intervention on IQ and PQ of adolescents where five different PVPs were given every day for 35 min. Thirty six adolescents aged between 11 and 16 years were selected for this study and assessed by Bhatia's Battery of Performance Tests of Intelligence before and after the intervention.

Data Analysis:
The data were analyzed for the variables IQ and PQ under the descriptive statistics, correlation, and the paired t-test.

Results:
The results show a significant increase (P < 0.01) in the IQ and PQ scores of the experimental group after the given intervention. The mean ± standard error values of IQ and PQ were found as be IQ (pre = 109.44 ± 3.46, post = 123.40 ± 2.43) and PQ (pre = 111.66 ± 3.48, post = 124.27 ± 2.53). The correlation coefficient was found to be significantly positive between pre- and post-tests of both IQ and PQ.

Conclusions:
The study findings suggest that PVPs increase IQ and PQ in adolescents.
Parenting Styles and Dimensions of Emerging Adulthood in Yoga and Nonyoga Practitioners
Authors: Venkatesan Raji , Ilavarasu Judu 
Published: November 2022

Background:
Career choice in engineering, especially in India, is determined by many factors such as parental influence and other inherent traits of students. Understanding the factors that are associated with self-regulated, choiceful decision-making in a career choice is essential to build better human resources. Early yoga practice may influence certain inherent traits, which can enable autonomous decision-making. Hence, exploration of those psychological factors is attempted in this study.

Aim:
This study aims to explore the parenting styles and dimensions of emerging adulthood among yoga and nonyoga practitioners.

Methods:
From an engineering college in South India, 311 first-semester students were recruited for the study. The Free will and Determinism Scale, the General Health Questionnaire, the Inventory of the Dimensions of Emerging Adulthood, the 13-item short form of the Marlowe–Crowne Social Desirability Scale, and the Perceived Parental Autonomy Support Scale were administered.

Results:
The students were divided into two categories, yoga practitioners and nonyoga practitioners. We performed Pearson's partial correlation between various variables across these two groups, controlling for social desirability scores. Overall, the magnitude of the correlations was low to moderate.

Conclusion:
There are a few dimensions of emerging adulthood that have desirable outcome trends, both in yoga and nonyoga practitioners. Distinct features of yoga practitioners are students who exercise inner free will, and with autonomy-supportive parenting style tend to have a positive outlook. Therefore, yoga may promote self-regulated ways of inner growth and learning in emerging adults.
Evaluation Process of Rasa in the Context of Nonlyrical Nonpercussive Indian Pure Music for Possible Application as Music Therapy
Authors: Gangopadhyay Abirlal , R. Prasad J. S. , Shamanna B. R. 
Published: November 2022

Background:
The famous rasa theory, with its three complete components, has been widely discussed in the doctrines of poetics and dramaturgy but not in the context of pure music. This study tries to find out the application of three rasa components in the context of Nonlyrical Nonpercussive Indian Pure Music (NNIPM). This would help the field of Indian music therapy to explore its application as a rendition according to desirable emotions relevant to needful subjects after customizing it to the individual need.

Aim:
This pilot study aims to know the pragmatic approach of rasa theory regarding NNIPM, coupled with rasa-centric rendering method to evoke śānta rasa (related to calmness, satisfaction, pleasantness, and other related emotions).

Materials and Methods:
Five music clips were recorded on Rudra Vīā, which are the stimuli to get emotional responses from fifty participants. A questionnaire was developed to elicit psychophysical responses and transitory emotions to get emotional reactions from them. Based on rasa theory, a Rasa-Matrix (RM) was designed. Based on RM, a Rasa Equation formula was further designed to get the rasa values of each response.

Results:
Fifty people participated from India and Bangladesh (n = 50). There were 210 (84%) rasa responses, and 40 (16%) were null as the rasa outcomes overlapped. According to Cronbach's alpha for reliability and internal consistency, the questionnaire was highly reliable for all five tunes (α was always 0.86-0.89). Accuracy of desirable śāntarasa (0.98, P < 0.001) was satisfactory.

Conclusion:
This study shows that the application of rasa theory regarding NNIPM is a reliable approach for emotion-centric music therapy. With the help of the rasa-centric rendering method, there is a considerable potential to create tunes that will be more helpful for inclusion as part of Indian music therapy in specific mental health conditions.
Human Being as a Self-Responsible and Connected Being
Authors: Singh Arun Pratap 
Published: November 2022

Background:
In contemporary scenario, we can notice a significant drop in self-responsibility and social connectedness among modern intellectuals and youth. As a result, several irresponsible and denigrating comments against cultural tools and practices continue to surface in the media and on the social networking sites. Psychological studies have identified co-occurrence between loss of reliance on cultural practices and emergence of physical and mental health issues.

Objectives:
Against this backdrop, current study has sought to analyzes integrative and comprehensive perspective of human nature found in Gandhian literature to expand the paradigms of self-nurturance and psychological counseling.

Materials and Method:
The data were analyzed by using thematic analysis.

Results:
Gandhian view goes beyond the prevalent notions of individualism and identifies over-indulgence in sensory pleasures, lack of self-investigation, utilitarianism, and lack of faith in God as causal pathways for mental health concerns. Addressing these challenges requires attending to the functioning of body, mind, spirit /soul, and nature (svabhav).

Conclusion:
Inculcating spirituality, love, non-violence, truth, theism, service, and celibacy in the process of psychological counseling is important. The Gandhian perspective especially acknowledges the relevance of self-expansion, sensory restraint, prayer, and inculcation of peace as techniques for Psychological counseling to restore physical and mental health.
Radiobiological modelling of radiation-induced acute skin toxicity (dermatitis): A single institutional study of breast carcinoma
Authors: Singh Balbir , Singh Gaganpreet , Oinam Arun Singh , Singh Maninder , Katake Ajay , Kumar Vivek , Vashistha Rajesh , Singh Pankaj Kumar , Mahajan Rohit 
Published: November 2022

ABSTRACT

Purpose:
The purpose of the study was to estimate the fitting parameters of the sigmoidal dose response (SDR) curve of radiation-induced acute dermatitis in breast cancer patients treated with intensity-modulated radiation therapy for calculation of normal tissue complication probability (NTCP).

Materials and Methods:
Twenty-five breast cancer patients were enrolled to model the SDR curve for acute dermatitis. The acute radiation-induced (ARI) dermatitis toxicity was assessed weekly for all the patients, and their scores were determined using the common terminology criterion adverse events version 5.0. The radiobiological parameters n, m, TD50, and γ50 were derived using the fitted SDR curve obtained from breast cancer Patient’s clinical data.

Results:
ARI dermatitis toxicity in carcinoma of breast patients was calculated for the end point of acute dermatitis. The n, m, TD50, and γ50 parameters from the SDR curve of Grade-1 dermatitis are found to be 0.03, 0.04, 28.65 ± 1.43 (confidence interval [CI] 95%) and 1.02 and for Grade-2 dermatitis are found to be 0.026, 0.028, 38.65 ± 1.93 (CI. 95%) and 1.01 respectively.

Conclusion:
This research presents the fitting parameters for NTCP calculation of Grade-1 and Grade-2 acute radiation-induced skin toxicity in breast cancer for the dermatitis end point. The presented nomograms of volume versus complication probability and dose versus complication probability assist radiation oncologists in establishing the limiting dose to reduce acute toxicities for different grades of acute dermatitis in breast cancer patients.