bluuebunny/crossref_metadata_2025_split huggingface dataset:
Madde Bağımlılığı ve Aile
Authors: Çifci Tekinarslan İlknur , Taylan Hasan Hüseyin , Aksakal Kuc Hülya , Yıkmış Ahmet , Alsancak Fatmanur , Kara Hüseyin Zahid , Yıldız Hülya , Curaoğlu Orhan , Kutlu İhsan , Altıparmak İpek Beyza , Işıklar Abdullah , Şar Ali Haydar , Güner Ümit , Güner Neslihan , Karabulut Alparslan , Akyüz İsmail , Kot Mehtap , Akkuş Dilek , Sarı Tuğba , Terzioğlu Nesime Kübra , Günerigök Mustafa , İnce Abdullah , Keskin Yahya Mustafa , Atasayar Mehmet 
Published: February 2024

Madde Bağımlılığının Aile Üzerindeki Etkisi Aile Eğitim Yaklaşımları
İlknur Çifci Tekinarslan
Madde Bağımlılığı Sürecinde Ailenin Rolü
Hasan Hüseyin Taylan
Madde Bağımlılığının Tedavisi Sonrasında Ailenin Rolü
Hülya Aksakal Kuc
Davranışçı Terapi ve Aile
Ahmet Yıkmış
Anne Baba Eğitimi
Fatmanur Alsancak
Hüseyin Zahid Kara
Hülya Yıldız
İletişim ve Aile
Orhan Curaoğlu
Literatür Taraması (Yapılan Araştırmalar Özetleri)
İhsan Kutlu
Bağımlılık ve Bağımlı Bireylerin Özellikleri
Yusuf Genç
İpek Beyza Altıparmak
Ergenlik Dönemi ve Madde Bağımlılığı
Abdullah Işıklar
Ali Haydar Şar
Madde Bağımlılığının Ekonomik Etkileri ve Bağımlılık Tedavisi Sağlayan Kurumlar İçin Pazarlama Stratejileri
Ümit Güner
Neslihan Güner
Madde Kullanımının Hukuki Yönü
Alparslan Karabulut
Bağımlılıkla Mücadelede Sivil Toplum Kuruluşları
İsmail Akyüz
Müdahale Yaklaşımları Davranışçı Müdahale
Mehtap Kot
Pozitif Psikoterapi Yaklaşımı (Madde Bağımlılığı Olan Bir Ergenin Annesi İçin Olgu Sunumu)
Dilek Akkuş
Tuğba Sarı
Bilişsel Müdahale Yaklaşımı
Hüseyin Zahid Kara, Fatmanur Alsancak
Mesleki Terapisi
Nesime Kübra Terzioğlu
Bozuk İşlevsellik, Birey ve Bağımlılık
Mustafa Günerigök
Abdullah İnce
Denetimli Serbestlikten Yararlanan Madde Bağımlıları Alan Araştırması (Saha Çalışması)
Yahya Mustafa Keskin
Grup Akran Etkileşimi ve Sosyal Becerilerin Kazandırılması
Mehmet Atasayar
Earnings Management, Leverage, Good Corporate Governance, And Tax Avoidance
Authors: Indriani Sintiati , Ramli Abdul Haeba 
Published: February 2024

The purpose of this research is to analyze the influence of earnings management, leverage and good corporate governance against tax avoidance. The sample used in this research is raw materials sector companies listed on the Indonesia Stock Exchange (IDX) during the period 2019 until 2022. The population of this research is 97 companies in the raw materials sector. The sampling technique used is purposive sampling So the total sample used in this research was 16 companies in the raw materials sector. The design of this research is causality which looks for the influence of cause and effect relationships. The data analysis technique in this research uses multiple linear regression analysis. The results of the research indicate that partially the earnings management and good corporate governance has no effect on tax avoidance, while the variable leverage has a positive effect on tax avoidance. Earnings management variables, leverage, and good corporate governance simultaneously influences tax avoidance.

Keywords: Earnings Management, Leverage, Good Corporate Governance, Tax Avoidance
On the Interpretation of XSPEC Abundances and Emission Measures
Authors: Leahy D. A. , Foster A. , Seitenzahl I. 
Published: February 2024

Abstract
The purpose of this work is to describe the assumptions built into the X-ray spectrum fitting software XSPEC for the calculation of element abundances and emission measure of a plasma and to describe the effects when those assumptions are not accurate. The ratio of electron density to hydrogen density in XSPEC is fixed at a constant. The correct ratio can be calculated from the ionization states of the elements. We show the constant value used in XSPEC is valid to within ≃3.5% for a solar-abundance plasma. For a plasma that deviates from solar abundance, e.g., hydrogen-poor or heavy-element-rich plasmas such as those found in the ejecta of supernova remnants, this ratio can be smaller by factors of 0.1–0.001. The hydrogen emission measure, defined by integral of electron density times hydrogen density over plasma volume, is derived from the norm in XSPEC, but one needs to include the hydrogen abundance factor. For other elements, the emission measures are the XSPEC values multiplied by the element abundance factors. Using the correct electron-to-hydrogen ratio and emission measures, we show the correct electron density is smaller by the square root of the correct electron density ratio divided by the XSPEC value. Element densities and total masses (for given distance and volume) are larger by the abundance factors divided by the above square root. Because hydrogen-poor plasmas occur in the ejecta of Type Ia supernova remnants, previously estimated element masses from X-ray spectra are likely to be significantly underestimated.
A Large Jet Narrow-line Seyfert 1 Galaxy: Observations from Parsec to 100 kpc Scales
Authors: Chen Sina , Kharb Preeti , Sasikumar Silpa , Nandi Sumana , Berton Marco , Järvelä Emilia , Laor Ari , Behar Ehud , Foschini Luigi , Vietri Amelia , Gu Minfeng , La Mura Giovanni , Crepaldi Luca , Zhou Minhua 
Published: February 2024

Abstract
We present new 1.5–8.5 GHz Very Long Baseline Array (VLBA) observations and 0.32–1.26 GHz Giant Meterwave Radio Telescope (GMRT) observations of J0354−1340, which is the only known radio-quiet (RQ) or radio-intermediate (RI) narrow-line Seyfert 1 galaxy with a 100 kpc, two-sided radio jet. A parsec-scale, one-sided jet in the southeastern direction from the core emission is found in the VLBA observations, while the kiloparsec-scale jet observed with the Karl G. Jansky Very Large Array (VLA) and GMRT is in the south–north direction. Core spectra on parsec and kiloparsec scales are presented in combination with archival VLA Sky Survey observations at 3.0 GHz and VLA C-configuration observations at 5.5 GHz. The parsec-scale emission dominates the kiloparsec-scale emission above ∼5 GHz, and the spectrum is inverted due to synchrotron self-absorption. This indicates a compact synchrotron source with a size of ∼0.04 pc, which is associated with either the jet base or the corona. A subkiloparsec-scale jet, which is unresolved on scales of ∼3″, probably dominates the emission below ∼5 GHz. Future radio observations can explore the jet structure between the parsec and 100 kpc scales, the origin of their direction mismatch, and the parsec-scale jet proper motion. It remains to be explored how common such large-scale jets are in RQ or RI active galactic nuclei.
Probing the Anisotropy and Non-Gaussianity in the Redshift Space through the Conditional Moments of the First Derivative
Authors: Kanafi M. H. Jalali , Movahed S. M. S. 
Published: February 2024

Abstract
Focusing on the redshift space observations with plane-parallel approximation and relying on the rotational dependency of the general definition of excursion sets, we introduce the so-called conditional moments of the first derivative (cmd) measures for the smoothed matter density field in three dimensions. We derive the perturbative expansion of cmd for the real space and redshift space where peculiar velocity disturbs the galaxies’ observed locations. Our criteria can successfully recognize the contribution of linear Kaiser and Finger-of-God effects. Our results demonstrate that the cmd measure has significant sensitivity for pristine constraining the redshift space distortion parameter β = f/b and interestingly, the associated normalized quantity in the Gaussian linear Kaiser limit has only β dependency. Implementation of the synthetic anisotropic Gaussian field approves the consistency between the theoretical and numerical results. Including the first-order contribution of non-Gaussianity perturbatively in the cmd criterion implies that the N-body simulations for the Quijote suite in the redshift space have been mildly skewed with a higher value for the threshold greater than zero. The non-Gaussianity for the perpendicular direction to the line of sight in the redshift space for smoothing scales R ≳ 20 Mpc h
−1 is almost the same as in the real space. In contrast, the non-Gaussianity along the line-of-sight direction in the redshift space is magnified. The Fisher forecasts indicate a significant enhancement in constraining the cosmological parameters Ω
m
, σ
8, and n

s
when using cmd + cr jointly.
Earth as an Exoplanet. III. Using Empirical Thermal Emission Spectra as an Input for Atmospheric Retrieval of an Earth-twin Exoplanet
Authors: Mettler Jean-Noël , Konrad Björn S. , Quanz Sascha P. , Helled Ravit 
Published: February 2024

Abstract
In this study, we treat Earth as an exoplanet and investigate our home planet by means of a potential future mid-infrared space mission called the Large Interferometer For Exoplanets (LIFE). We combine thermal spectra from an empirical data set of disk-integrated Earth observations with a noise model for LIFE to create mock observations. We apply a state-of-the-art atmospheric retrieval framework to characterize the planet, assess the potential for detecting the known bioindicators, and investigate the impact of viewing geometry and seasonality on the characterization. Our key findings reveal that we are observing a temperate habitable planet with significant abundances of CO2, H2O, O3, and CH4. Seasonal variations in the surface and equilibrium temperature, as well as in the Bond albedo, are detectable. Furthermore, the viewing geometry and the spatially and temporally unresolved nature of our observations only have a minor impact on the characterization. Additionally, Earth’s variable abundance profiles and patchy cloud coverage can bias retrieval results for the atmospheric structure and trace-gas abundances. Lastly, the limited extent of Earth’s seasonal variations in biosignature abundances makes the direct detection of its biosphere through atmospheric seasonality unlikely. Our results suggest that LIFE could correctly identify Earth as a planet where life could thrive, with detectable levels of bioindicators, a temperate climate, and surface conditions allowing liquid surface water. Even if atmospheric seasonality is not easily observed, our study demonstrates that next generation space missions can assess whether nearby temperate terrestrial exoplanets are habitable or even inhabited.
Measuring the Virial Factor in SDSS DR7 Active Galactic Nuclei with Redshifted Hβ and Hα Broad Emission Lines
Authors: Liu H. T. , Feng Hai-Cheng , Li Sha-Sha , Bai J. M. , Li H. Z. 
Published: February 2024

Abstract
Under the hypothesis of gravitational redshift induced by the central supermassive black hole and based on line widths and shifts of redward-shifted Hβ and Hα broad emission lines for more than 8000 Sloan Digital Sky Survey DR7 active galactic nuclei (AGNs), we measure the virial factor in determining supermassive black hole masses. The virial factor had been believed to be independent of accretion radiation pressure on gas clouds in broad-line regions (BLRs) and only dependent on the inclination effects of BLRs. The virial factor measured spans a very large range. For the vast majority of AGNs (>96%) in our samples, the virial factor is larger than the f = 1 usually used in the literature. The f-correction makes the percent of high-accreting AGNs decrease by about 100 times. There are positive correlations of f with the dimensionless accretion rate and Eddington ratio. The redward shifts of Hβ and Hα are mainly of gravitational origin, confirmed by a negative correlation between the redward shift and the dimensionless radius of the BLR. Our results show that radiation pressure force is a significant contributor to the measured virial factor, containing the inclination effects of the BLR. The usually used values of f should be corrected for high-accreting AGNs, especially high-redshift quasars. The f-correction increases their masses by 1–2 orders of magnitude, which will make it more challenging to explain the formation and growth of supermassive black holes at high redshifts.
EIGER IV. The Cool 104 K Circumgalactic Environment of High-redshift Galaxies Reveals Remarkably Efficient Intergalactic Medium Enrichment
Authors: Bordoloi Rongmon , Simcoe Robert A. , Matthee Jorryt , Kashino Daichi , Mackenzie Ruari , Lilly Simon J. , Eilers Anna-Christina , Liu Bin , DePalma David , Yue Minghao , P. Naidu Rohan 
Published: February 2024

Abstract
We report new observations of the cool diffuse gas around 29, 2.3 < z < 6.3 galaxies using deep JWST/NIRCam slitless grism spectroscopy around the sight line to the quasar J0100+2802. The galaxies span a stellar mass range of

7.1
≤

log

M

∗

/

M

⊙

≤
10.7

, and star formation rates (SFRs) of

−
0.1
<
log

SFR/M
⊙ yr−1 < 2.3. We find galaxies for seven Mg ii absorption systems within 300 kpc of the quasar sight line. The Mg ii radial absorption profile falls off sharply with radius, with most of the absorption extending out to 2–3 R
200 of the host galaxies. Six out of seven Mg ii absorption systems are detected around galaxies with

log

M

∗

/

M

⊙

>

9. The Mg ii absorption kinematics are shifted from the systemic redshifts of host galaxies with a median absolute velocity ≈ 135 km s−1 and standard deviation ≈ 85 km s−1. The high kinematic offset and large radial separation (R > 1.3 R
200), suggest that five out of the seven Mg ii absorption systems are not gravitationally bound to their host galaxy. In contrast, most of the cool circumgalactic medium at z < 1 is gravitationally bound. The high incidence of unbound Mg ii gas in this work suggests that toward the end of reionization, galaxy halos are in a state of remarkable disequilibrium, and are highly efficient in enriching the intergalactic medium. The two strongest Mg ii absorption systems are detected at z ∼ 4.22 and 4.5, the former associated with a merging galaxy system and the latter associated with three kinematically close galaxies. Both of these galaxies reside in local galaxy overdensities, indicating the presence of cool Mg ii absorption in two “protogroups” at z > 4.
The Hunt for Perpendicular Magnetic Field Measurements in Plasma
Authors: Jensen Elizabeth A. , Rahmani Yaser , Simpson Jamesina J. 
Published: February 2024

Abstract
The one consistent technique for remotely estimating the magnetic field in plasma has been Faraday rotation. It is only sensitive to the portion of the vector parallel to the propagation path. We show how to remotely detect the portion of the vector that is perpendicular using a modified measurement. Isolating this electromagnetic propagation wave mode to measure the magnetic field enables us to (i) study more about the magnetic field vector in plasma, (ii) reduce error in total electron content measurements, and (iii) discover new magnetic field information from archived data sets. The Appleton–Hartree equation is used to verify a new approach to calculating the phase change to an electromagnetic wave propagating through a plasma at frequencies larger than the gyrofrequency, the cyclotron frequency, and the upper hybrid frequency. Focusing on the perpendicular propagation modes, the simplified equation for the integrated path effect from a perpendicular magnetic field is calculated. The direction of the perpendicular component is unknown, because the magnetic field is squared. Isolating the magnetic term in the equation with dual frequency waves is shown. We also show how to eliminate the magnetic field contribution to total electron content measurements with a similar approach. In combination with Faraday rotation, the degeneracy of the magnetic field vector direction is reduced to a cone configuration.
The AO327 Drift Survey Catalog and Data Release of Pulsar Detections
Authors: Deneva J. S. , McLaughlin M. , Olszanski T. E. E. , Lewis E. F. , Pang D. , Freire P. C. C. , Bagchi M. , Stovall K. 
Published: February 2024

Abstract
The AO327 drift survey for radio pulsars and transients used the Arecibo telescope from 2010 until its collapse in 2020. AO327 collected ∼3100 hr of data at 327 MHz with a time resolution of 82 μs and a frequency resolution of 24 kHz. While the main motivation for such surveys is the discovery of new pulsars and new, even unforeseen, types of radio transients, they also serendipitously collect a wealth of data on known pulsars. We present an electronic catalog of data and data products of 206 pulsars whose periodic emission was detected by AO327 and are listed in the Australia Telescope National Facility catalog of all published pulsars. The AO327 data products include dedispersed time series at full time resolution, average (“folded”) pulse profiles, Gaussian pulse profile templates, and an absolute phase reference that allows phase aligning the AO327 pulse profiles in a physically meaningful manner with profiles from data taken with other instruments. We also provide machine-readable tables with uncalibrated flux measurements at 327 MHz and pulse widths at 50% and 10% of the pulse peak determined from the fitted Gaussian profile templates. The AO327 catalog data set can be used in applications like population analysis of radio pulsars, pulse profile evolution studies in time and frequency, cone and core emission of the pulsar beam, scintillation, pulse intensity distributions, and others. It also constitutes a ready-made resource for teaching signal-processing and pulsar astronomy techniques.
A Study of Broad Emission Line and Doppler Factor Estimation for Fermi Blazars
Authors: Chen Guohai , Zheng Zepeng , Zeng Xiangtao , Zhang Lixia , Xiao Hubing , Liu Xiang , Cui Lang , Fan Junhui 
Published: February 2024

Abstract
In this work, we obtained a sample of 979 Fermi blazars with broad emission lines, including 701 objects collected from published works and 278 objects developed in this work. For the 278 objects, we made a crossmatch from three catalogs, the Fermi Large Area Telescope Fourth Source Catalog (4FGL), the Sloan Digital Sky Survey, and the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, and calculated the broad-line region (BLR) luminosity. Then, we estimated the Doppler factor and studied the correlations between the BLR luminosities and the γ-ray luminosities, the synchrotron peak frequency (ν

p
), and Doppler factor (δ) for the whole sample. Our analyses and discussions came to the following main conclusions: For the 278 blazars, their BLR luminosity (log L
BLR) ranges from 40.44 to 45.45 erg s−1, with a mean value of 43.39 erg s−1. The Doppler factor ranges from δ = 0.45 to δ = 88.52, with a mean value of 12.99 for the 979 Fermi blazars, which is consistent with the results in the literature. Both the BLR luminosity and the Doppler factor exhibit positive correlations with the γ-ray luminosity. The BLR luminosity is anticorrelated with synchrotron peak frequency, implying a Compton cooling. A line of

log

L
BLR

=
1.58
log

ν
p

−
19.46

separating BL Lacertae objects and flat-spectrum radio quasars was obtained in the diagram of

log

L

BLR

against

log

ν
p

using a machine-learning method. Based on the analysis of the equivalent width and the Doppler factors, we proposed five changing-look blazar candidates.
Trends in the Clinical Presentation of Uveal Melanoma During the COVID-19 Pandemic
Authors: Adams Olufemi E. , Tanke Laurel B. , Mundae Rusdeep , Sodhi Guneet S. , Yu Michael D. , Yonekawa Yoshihiro , Dalvin Lauren A. , Tang Peter H. 
Published: February 2024

Background and Objective:
The objective was to evaluate factors associated with clinical presentation of uveal melanoma (UM) during the initial two years of the coronavirus disease 2019 pandemic.

Patients and Methods:
This was a multi-site, retrospective cohort study of patients treated for uveal melanoma during the first (early) and second (late) year of the pandemic compared with the year prior (control).

Results:

A total of 48, 67, and 75 patients were in the control, early, and late cohorts, respectively. The early cohort had a higher frequency of large tumors (control: 29.2%, early: 40.3%, late: 29.3%;
P
< 0.001) at presentation. Both the early and late cohorts had higher rates of enucleation (control: 8.33%, early: 20.9%, late: 18.67%;
P
≤ 0.0338) compared to the control cohort.

Conclusions:
While there was an increase in large tumors along with a rise in enucleation during the first year of the pandemic, enucleation rates remained elevated even while tumor sizes normalized.

[
Ophthalmic Surg Lasers Imaging Retina
2024;55:278–284.]
Investigating the Effect of Aspirin on apoAI-Induced ATP Binding Cassette Transporter 1 Protein Expression and Cholesterol Efflux in Human Astrocytes
Authors: Nazeri Zahra , Abdeveiszadeh Neda , Zarezade Vahid , Azizidoost Shirin , Cheraghzadeh Maryam , Aberumand Mohammad , Kheirollah Alireza 
Published: February 2024

Abstract

Background:
Neurons need a high amount of cholesterol to maintain the stability of their membrane-rich structures. Astrocytes synthesize and distribute cholesterol to neurons, and ABCA1 is a key mediator of cholesterol efflux to generate HDL for cholesterol transport in the brain. Several studies imply the effect of aspirin on ABCA1 expression in peripheral cells such as macrophages. Here, we compared the effect of aspirin with apoA-I on ABCA1 protein expression and cholesterol efflux in human astrocytes.

Materials and Methods:
Human astrocytes were cultured, and the effects of aspirin on the expression and protein levels of ABCA1 were investigated through RT-PCR and Western blot analysis. Additionally, the effect of co-treatment with apoA-I and aspirin on ABCA1 protein level and cholesterol efflux was evaluated.

Results:
Dose and time-course experiments showed that the maximum effect of aspirin on ABCA1 expression occurred at a concentration of 0.5 mM after 12 h of incubation. RT-PCR and western blot data showed that aspirin upregulates ABCA1 expression by up to 4.7-fold and its protein level by 67%. Additionally, co-treatment with aspirin and apoA-I increased cholesterol release from astrocytes, indicating an additive effect of aspirin on apoAI-mediated cholesterol efflux.

Conclusions:
The results suggest a potential role of aspirin in increasing ABCA1 expression and cholesterol efflux in astrocytes, similar to the effect of apoA-I. This indicates that aspirin could potentially regulate brain cholesterol balance and can be considered in certain neurological diseases, in particular in some neurological disorders related to cholesterol accumulation such as Alzheimer’s disease.