bluuebunny/crossref_metadata_2025_split huggingface dataset:
Eczacılıkta Güncel Araştırmalar
Authors: Erdönmez Elif , Yuca Hafize , Kalaycı Benan , Gökgöz Saime , Paşayeva Leyla , Karaboğa Arslan Ayşe Kübra , Şerbetçi Tuba , Aydoğan Yağmur Merve , Yüce Hande , Şahin Yasemin , Başak Türkmen Neşe , Ünüvar Songül , Küpeli İkbal , Çevikelli Tilbe , Güven Umay Merve , Polat Heybet Kerem , Kurt Nihat , Asan Şeyma , Sevinç Özakar Rukiye , Özakar Emrah , Örgül Dilara , Tuğrak Sakarya Mehtap , Koca Mehmet , Alparslan Bayram , Cengiz Rabia , Kurt Barış 
Published: February 2024

Dermokozmetik Ürünlerde Bulunan Doğal Kaynaklı Hammaddeler
Elif ERDÖNMEZ
Hafize YUCA

Dermatolojide Tıbbi Bitkilerin Önemi
Benan KALAYCI

Helichrysum Plicatum Ssp. Plicatum Bitkisinin Farmakolojik Açıdan Değerlendirilmesi
Saime GÖKGÖZ
Leyla PAŞAYEVA
Ayşe Kübra KARABOĞA ARSLAN

Primer Dismenore Tedavisinde Kullanılan Destekleyici Tıbbi Bitkiler Ve Mikro Besinler
Tuba ŞERBETÇİ
Yağmur Merve AYDOĞAN

Bromelain ve Terapotik Kullanımı
Hande YÜCE
Yasemin ŞAHİN
Neşe BAŞAK TÜRKMEN
Songül ÜNÜVAR

Emodin ve Anti-Tümoral Etkisi
Yasemin ŞAHİN
Hande YÜCE
Neşe BAŞAK TÜRKMEN
Songül ÜNÜVAR

Majistral İlaçlara Güncel Bakış: Leke Tedavisinde Kullanılan Reçeteler
İkbal KÜPELİ
Tilbe ÇEVİKELLİ
Umay Merve GÜVEN

Oküler Hastalıkların Tedavisi İçin Hidrojel Bazlı İlaç Taşıyıcı Sistemler
Heybet Kerem POLAT

Kuru Göz Tedavisi İçin İlaç Taşıyıcı Sistemler
Heybet Kerem POLAT
Nihat KURT

Cilt Hastalıklarında Kullanılan Jel Tipi Dozaj Şekillerine Güncel Bir Bakış
Şeyma ASAN
Rukiye SEVİNÇ ÖZAKAR
Emrah ÖZAKAR

Kanser Tedavisinde Enjekte Edilebilir Hidrojel İlaç Taşıyıcı Sistemler
Dilara ÖRGÜL

COVID-19 ile İlişkili Diabetes Mellitus
Mehtap TUĞRAK SAKARYA

Alkil Sübstitüsyonunun Farmasötik Kimya Açısından Önemi
Mehmet KOCA

Gastrointestinal Disbiyosis ve Hastalıklarla Etiyolojik İlişkisi
Bayram ALPARSLAN
Rabia CENGİZ

Bakteriyofaj Terapisinin Enfeksiyonların Tedavisinde Dünü Bugünü Yarını
Bayram ALPARSLAN
Barış KURT
ANAZARBOS & ANAVARZA CİLT I
Authors: Karagel Eylül , Ünlügenç Ulvi Can , Akyıldız Mustafa , Akıncı Ahmet Can , Kaplan Aytül , Sayar Mustafa H. , Ünal Ahmet , Akçay Tuna , Beşaltı Kenan , Buyruk Hasan , Çakmak Ümit , Demir Faris , Durugönül Serra , Ergeç Rıfat , Dinç Münteha , Gerçek Ayça , Ovacık Arzu , Demir Gülez Fatma , Alanyalı Hüseyin Sabri , Çoksolmaz Ece 
Published: February 2024

Üç İdari Alanın Kesişme Noktasında Kurulmuş Bir Yerleşme: Anavarza Antik Kenti (Dilekkaya) A Settlement Establıshed At The Junctıon Of Three Admınıstratıve Areas: The Ancıent Cıty Of Anazarbos (Anavarza/Dilekkaya)
Eylül Karagel

Anavarza Antik Kenti (Adana-Osmaniye) Civarının Jeolojisi Ve Depremselliği Hakkında Genel Bilgiler General Informatıon On The Geology And Seısmıcıty Of Anavarza Ancıent Cıty And Its Surroundıngs (Adana-Osmaniye)
Ulvi Can Ünlügenç, Mustafa Akyıldız Ahmet Can Akıncı

Anavarza’nın Çevre Yerleşim Yerleri, Bölgeler Arası Yol Güzergâhları, Üretim Ve Ulaşımın Ekonomik Getirileri Anavarza’s Neıghbourhood Settlements, Road Routes Between Regıons And Economıc Returns Of Prodıctıon And Transport
Aytül Kaplan

Anazarbos’un M.S. 2 Ve 3 Yy.’Larda Roma Ordusunun Doğu Seferine Katılan Birlikleri İçin Oynadığı Lojistik Rol Kapsamında Garnizon Şehir Ve Emekli Askerlerin İskan Bölgesi Olmasına İlişkin Düşüncüler Some Consıderatıons On Anazarbos’ Logıctıc Role In The 2nd And 3rd Centurıes Ad As A Garrıson Cıty For The Roman Army Unıts In Expedıtıon Orıentıs And A Settlement Area For The Veterans
Mustafa H. Sayar

Eski Anadolu Coğrafyası’nın Önemli Kentlerinden Puduhepa’nın Memleketi Luhusatia/Lawazantiya/Luhuzzantiya Lawazantiya, A Noteworthy Urban Center Of Ancıent Anatolıa And Hometown Of The Queen Puduhepa
Ahmet Ünal

Anazarbus’ta Bulunan Kurban Sunağı Ve 3b Modelleme Yöntemleriyle Sunağın Canlandırılması Sacrıfıcıal Altar In Anazarbus And Revıtalızatıon Of Altar Wıth 3d Modelıng Technıques
Tuna Akçay

Anazarbos Aşağı Kent Surları The Lower Cıty Walls Of Anazarbos
Kenan Beşaltıvi

Anavarza Kenti’nin Su Sistemleriwater Systems Of Anavarza Antıque Cıty
Hasan Buyruk

Anavarza Kalesi The Castle Of Anavarza
Hasan Buyruk

Geç Antik Dönem’de Anazarbos ve Çevresi: Kırsal Yerleşimler ve Ekonomik Durumın The Late Antıquıty Anazarbos And Surroundıngs: Rural Settlements And Economıcal Sıtuatıon
Ümit Çakmak

Anazarbos Mozaikleri Üzerine Notlarnotes On The Anazarbos Mosaıcs
Faris Demır

Anazarbos’un Kılıkıa Bölgesi Heykeltıraşlığı’ndaki Yerithe Status Of Anazarbos In Cılıcıan Sculpture
Serra DURUGÖNÜL, F. Fatih GÜLŞEN

Anazarbos Freskli Oda Mezarıanazarbos Frescoed Chamber Tomb
Rifat Ergeç, Münteha Dinç

Roma Dönemi Anazarbos Lâhitleri Roman Perıod Anazarbos Sarcophagus
Rifat Ergeç

Roma İmparatorluğu’nda Siyaset Ve Mimari İlişkisinin Anazarbos’a Yansımasıreflectıon Of The Relatıonshıp Between Polıtıcs And Archıtecture In The Roman Empıre On Anazarbos
Ayça Gerçek

Geçmişten Günümüze Anavarza Kazıları Ve Bölge İçin Önemianavarza Excavatıons From Past To Present And Theır Importance For The Regıon
Arzu Ovacık, Fatma Demir Gülez

Tiyatro – Stadıon – Amphıtiyatro Çalışmalarıstudıes On Theatre – Stadıum – Amphıtheatre
Hüseyin Sabri ALANYALI, Ece ÇOKSOLMAZ
Mekanisme Pembayaran Pajak Bumi Dan Bangunan Perdesaan Dan Perkotaan (PBB-P2) Pada Badan Pendapatan Daerah (BAPENDA) Kabupaten Subang
Authors: Hirawan Zaenal , Nurasiatin Dewi 
Published: February 2024

Abstrak
Tujuan dari Penelitian ini yaitu untuk mengetahui dan menjelaskan Mekanisme Pembayaran PBB-P2 pada BAPENDA Kabupaten Subang. Penelitian ini bermanfaat untuk menambah wawasan tentang mekanisme pembayaran PBB-P2 pada BAPENDA Kabupaten Subang. Metode yang digunakan dalam penelitian ini yaitu metode kualitatif deskriptif yaitu pencarian fakta dengan interpretasi yang tepat. Metode yang digunakan dalam penelitian ini yaitu metode kualitatif deskriptif yaitu pencarian fakta dengan interpretasi yang tepat : Observasi, Dokumentasi, Wawancara, Studi Pustaka atau Kepustakaan.
Alur pembayaran PBB-P2 yang sedang berjalan di Bank ke Badan Pendapatan Daerah Kab. Subang yaitu Wajib Pajak menyerahkan SPPT kepada teller, setelah berkas lengkap teller membuat slip setoran dan menyerahkan kepada bagian Analisa Pajak. Analisa Pajak membuat penerimaan PBB-P2 dan menyerahkan kepada teller. Setelah itu teller membuat laporan mutasi penerimaan PBB-P2 dan menyerahkan kepada Pimpinan Bank dan Bapenda. Dan sebenarnya BAPENDA berpihak sebagai koordinator Pajak Daerah tersebut, jadi BAPENDA memiliki catatan penerimaan Pajak Daerah.
Maka disimpulkan Mekanisme Pembayaran PBB-P2 pada BAPENDA Kabupaten Subang Wajib Pajak mendapatkan SPPT, setelah itu Wajib Pajak melakukan pembayaran melalui outlet yang sudah ditentukan.
Kata kunci : Mekanisme, PBB-P2, Alur Pembayaran

Abstract
The purpose of this study is to find out and explain the PBB-P2 Payment Mechanism at the BAPENDA of Subang Regency. This research is useful for adding insight into the PBB-P2 payment mechanism at the Subang Regency BAPENDA. The method used in this research is descriptive qualitative method, namely fact finding with the right interpretation. The method used in this research is descriptive qualitative method, namely fact finding with the right interpretation: Observation, Documentation, Interviews, Library Studies or Literature.
The PBB-P2 payment flow that is currently running at the Bank to the District Revenue Agency. Subang, namely the Taxpayer submits the SPPT to the teller, after the complete file the teller makes a deposit slip and submits it to the Tax Analysis section. Tax analysis makes PBB-P2 receipts and submits them to tellers. After that the teller makes a transfer report on PBB-P2 receipts and submits it to the leadership of the Bank and Bapenda. And actually BAPENDA takes sides as the Regional Tax coordinator, so BAPENDA has records of Regional Tax receipts.
So it was concluded that the PBB-P2 Payment Mechanism at BAPENDA of Subang Regency Taxpayers get SPPT, after that the Taxpayers make payments through predetermined outlets
Keywords : Mechanism, PBB-P2, Payment Flow
Prospects for Detecting Gaps in Globular Cluster Stellar Streams in External Galaxies with the Nancy Grace Roman Space Telescope
Authors: Aganze Christian , Pearson Sarah , Starkenburg Tjitske , Contardo Gabriella , Johnston Kathryn V. , Tavangar Kiyan , Price-Whelan Adrian M. , Burgasser Adam J. 
Published: February 2024

Abstract
Stellar streams form through the tidal disruption of satellite galaxies or globular clusters orbiting a host galaxy. Globular cluster streams are exciting since they are thin (dynamically cold) and therefore sensitive to perturbations from low-mass subhalos. Since the subhalo mass function differs depending on the dark matter composition, these gaps can provide unique constraints on dark matter models. However, current samples are limited to the Milky Way. With its large field of view, deep imaging sensitivity, and high angular resolution, the upcoming Nancy Grace Roman Space Telescope (Roman) presents a unique opportunity to increase the number of observed streams and gaps significantly. This paper presents a first exploration of the prospects for detecting gaps in streams in M31 and other nearby galaxies with resolved stars. We simulate the formation of gaps in a Palomar 5–like stream and generate mock observations of these gaps with background stars in M31 and foreground Milky Way stellar fields. We assess Roman's ability to detect gaps out to 10 Mpc through visual inspection and with the gap-finding tool FindTheGap. We conclude that gaps of ≈1.5 kpc in streams that are created from subhalos of masses ≥5 × 106
M
⊙ are detectable within a 2–3 Mpc volume in exposure times of 1000 s to 1 hr. This volume contains ≈150 galaxies, including ≈eight galaxies with luminosities >109
L
⊙. Large samples of stream gaps in external galaxies will open up a new era of statistical analyses of gap characteristics in stellar streams and help constrain dark matter models.
Segregation and Collisions in Galactic Nuclei: Rates of Destructive Events Near a Supermassive Black Hole
Authors: Balberg Shmuel 
Published: February 2024

Abstract
The centers of galaxies host a supermassive black hole (SMBH) surrounded by a dense stellar cluster. The cluster is expected to develop mass segregation, in which gravitational scatterings among the stars cause heavier objects to sink closer to the central black hole, while lighter objects will tend to be overconcentrated in the outer regions. This work focuses on the implications of mass segregation on the different channels for violent destruction of stars in the cluster: tidal disruptions, gravitational-wave-driven inspirals and high-velocity destructive collisions between stars. All such events occur close to the central black hole, where the heavier objects congregate. The analysis is based on a simplified Monte Carlo simulation, which evolves a two-mass population in a cluster surrounding a Milky Way–like SMBH. The simulation is based on the single-mass scheme used by Sari & Fragione and Balberg & Yassur, which has been extended to allow for the dynamical friction effects typical of unequal-mass populations. The effects of mass segregation on the rates of the different destruction channels are analyzed self-consistently in the overall evolution of the cluster. Also considered are stars which are injected into the cluster after being disrupted from a binary system by the SMBH. Such stars are captured in the inner regions of the cluster, and so their orbital evolution, as well as their destruction rate, are therefore influenced by heavy objects that might be abundant in the vicinity of the SMBH.
Reaction Pathway and Rovibrational Analysis of Aluminum Nitride Species as Potential Dust Grain Nucleation Agents
Authors: Palmer C. Zachary , Fortenberry Ryan C. 
Published: February 2024

Abstract
A dust nucleating agent may be present in interstellar or circumstellar media that has gone seemingly undetected and unstudied for decades. Some analyses of the Murchison CM2 meteorite suggest that at least some of the aluminum present within condensed as aluminum nitrides instead of the long-studied, but heretofore undetected suite of aluminum oxides. The present theoretical study utilizes explicitly correlated coupled cluster theory and density functional theory to provide a formation pathway from alane (AlH3) and ammonia to the cyclic structure Al2N2H4, which has the proper Al/N ratio expected of bulk aluminum nitrides. Novel rovibrational spectroscopic constants are computed for alane and the first two formed structures, AlNH6 and AlNH4, along the reaction pathway for use as reference in possible laboratory or observational studies. The ν
8 bending frequency for AlNH6 at 755.7 cm−1 (13.23 μm) presents a vibrational transition intensity of 515 km mol−1, more intense than the antisymmetric C−O stretch of carbon dioxide, and contains a dipole moment of 5.40 D, which is ∼3× larger than that of water. Thus, the present reaction pathway and rovibrational spectroscopic analysis may potentially assist in the astrophysical detection of novel, inorganic species which may be indicative of larger dust grain nucleation.
Properties of an Interplanetary Shock Observed at 0.07 and 0.7 au by Parker Solar Probe and Solar Orbiter
Authors: Trotta Domenico , Larosa Andrea , Nicolaou Georgios , Horbury Timothy S. , Matteini Lorenzo , Hietala Heli , Blanco-Cano Xochitl , Franci Luca , Chen C. H. K , Zhao Lingling , Zank Gary P. , Cohen Christina M. S. , Bale Stuart D. , Laker Ronan , Fargette Nais , Valentini Francesco , Khotyaintsev Yuri , Kieokaew Rungployphan , Raouafi Nour , Davies Emma , Vainio Rami , Dresing Nina , Kilpua Emilia , Karlsson Tomas , Owen Christopher J. , Wimmer-Schweingruber Robert F. 
Published: February 2024

Abstract
The Parker Solar Probe (PSP) and Solar Orbiter (SolO) missions opened a new observational window in the inner heliosphere, which is finally accessible to direct measurements. On 2022 September 5, a coronal mass ejection (CME)-driven interplanetary (IP) shock was observed as close as 0.07 au by PSP. The CME then reached SolO, which was radially well-aligned at 0.7 au, thus providing us with the opportunity to study the shock properties at different heliocentric distances. We characterize the shock, investigate its typical parameters, and compare its small-scale features at both locations. Using the PSP observations, we investigate how magnetic switchbacks and ion cyclotron waves are processed upon shock crossing. We find that switchbacks preserve their V–B correlation while compressed upon the shock passage, and that the signature of ion cyclotron waves disappears downstream of the shock. By contrast, the SolO observations reveal a very structured shock transition, with a population of shock-accelerated protons of up to about 2 MeV, showing irregularities in the shock downstream, which we correlate with solar wind structures propagating across the shock. At SolO, we also report the presence of low-energy (∼100 eV) electrons scattering due to upstream shocklets. This study elucidates how the local features of IP shocks and their environments can be very different as they propagate through the heliosphere.
Host Galaxy and Nuclear Properties of IR-selected AGNs with and without Outflow Signatures
Authors: Oio Gabriel A. , Dai 戴 Y. Sophia 昱 , Bornancini C. G. , Li Zi-Jian 
Published: February 2024

Abstract
Active galactic nucleus (AGN) driven outflows can have a significant impact on the evolution of the host galaxy. In this work, we compare the properties of galaxies that host AGNs with and without outflows. Our sample consists of 103 AGNs identified by mid-IR color–color selection and confirmed with optical spectroscopy at a redshift range of 0.3 ≲ z ≲ 0.9. We fit the [O iii] λ5007 line using spectra from the zCOSMOS survey to identify and study the occurrence of outflows. We find that ionized outflows are present in ∼25% of our sample, with the largest incidence at the highest [O iii] and X-ray luminosity bins. The fastest outflows are found in the more extended and massive galaxies. We do not observe a difference in the star formation rate of AGNs with outflows compared to AGNs without outflows. From visual inspection and nonparametric morphological studies, we obtain that outflows are preferentially observed in galaxies with disk-type and elliptical morphologies.
Dynamical Friction Models for Black Hole Binary Formation in Active Galactic Nucleus Disks
Authors: Qian Kecheng , Li Jiaru , Lai Dong 
Published: February 2024

Abstract
Stellar-mass black holes (sBHs) embedded in gaseous disks of active galactic nuclei (AGN) can be important sources of detectable gravitational radiation for LIGO/Virgo when they form binaries and coalesce due to orbital decay. In this paper, we study the effect of dynamical friction (DF) on the formation of BH binaries in AGN disks using N-body simulations. We employ two simplified models of DF, with the force on the BH depending on Δ
v
, the velocity of the sBH relative to the background Keplerian gas. We integrate the motion of two sBHs initially on circular orbits around the central supermassive black hole (SMBH) and evaluate the probability of binary formation under various conditions. We find that both models of DF (with different dependence of the frictional coefficient on ∣Δ
v
∣) can foster the formation of binaries when the effective friction timescale τ satisfies ΩK
τ ≲ 20–30 (where ΩK is the Keplerian frequency around the SMBH): prograde binaries are formed when the DF is stronger (smaller τ), while retrograde binaries dominate when the DF is weaker (larger τ). We determine the distribution of both prograde and retrograde binaries as a function of initial orbital separation and the DF strength. Using our models of DF, we show that for a given sBH number density in the AGN disk, the formation rate of sBH binaries increases with decreasing τ and can reach a moderate value with a sufficiently strong DF.
A Unified Model for Multiepoch Neutrino Events and Broadband Spectral Energy Distribution of TXS 0506+056
Authors: Wang Zhen-Jie , Liu Ruo-Yu , Wang Ze-Rui , Wang Junfeng 
Published: February 2024

Abstract
The blazar TXS 0506+056 has been proposed as a high-energy neutrino emitter. However, it has been shown that the standard one-zone model cannot produce sufficiently high neutrino flux due to constraints from the X-ray data, implying more complex properties of the radiation zones in the blazar than that described by the standard one-zone model. In this work, we investigate multiepoch high-energy muon-neutrino events associated with the blazar TXS 0506+056 that occurred in 2014–2015, 2017–2018, 2021–2022, and 2022–2023, respectively. We applied the so-called “stochastic dissipation model” to account for the neutrino-blazar associations detected in the four epochs simultaneously. This model describes a scenario in which the emission of the blazar arises from the superimposition of two components: a persistent component related to the quasi-stable state of the blazar and a transient component responsible for the sudden enhancement of the blazar’s flux, either in electromagnetic radiation or in neutrino emission. The latter component could form at a random distance along the jet by a strong energy dissipation event. Under such an assumption, the multiepoch broadband spectral energy distribution can be well explained, and the expected number of high-energy neutrino events is statistically realistic. The expected number of neutrino events in half year is around 8.2, 0.07, 0.73, and 0.41, corresponding to the epoch in 2014–2015, 2017–2018, 2021–2022, and 2022–2023, respectively. Hence, our model self-consistently explains the episodic neutrino emission from TXS 0506+056.
Broadband Multiwavelength Study of LHAASO-detected Active Galactic Nuclei
Authors: Wang Ze-Rui , Xue Rui , Xiong Dingrong , Wang Hai-Qin , Sun Lu-Ming , Peng Fang-Kun , Mao Jirong 
Published: February 2024

Abstract
Recently, the Large High Altitude Air Shower Observatory (LHAASO) collaboration presented the first catalog of γ-ray sources using 508 days of LHAASO data, from 2021 March to 2022 September. This catalog contains four blazars and a possible LINER-type active galactic nucleus (AGN) counterpart. In this work, we establish averaged multiwavelength spectral energy distributions (SEDs) by combining data from the Fermi-Large Area Telescope, Swift, Zwicky Transient Facility, and Wide-field Infrared Survey Explorer (WISE) covering the same period as the LHAASO detection. In general, these five AGNs are found in low states at all wavelengths. To study the multiwavelength properties of these AGNs, several jet emission models, including the one-zone leptonic model, the one-zone leptonic and hadronuclear (pp) model, the one-zone proton-synchrotron model, and the spine-layer model, are applied to reproduce their averaged SEDs. We find that the one-zone leptonic model can reproduce most of the SEDs, except for the high-energy tail of the LHAASO spectra of Mrk 421 and Mrk 501. To improve the fitting, emission from pp interactions is favored in the framework of a one-zone model. The spine-layer model, which can be treated as a multizone scenario, can also provide good spectral fits. The influence of different extragalactic background light models on fitting a LHAASO energy spectrum is also discussed.
Classifying Optical (Out)bursts in Cataclysmic Variables: The Distinct Observational Characteristics of Dwarf Novae, Micronovae, Stellar Flares, and Magnetic Gating
Authors: Iłkiewicz Krystian , Scaringi Simone , Veresvarska Martina , De Martino Domitilla , Littlefield Colin , Knigge Christian , Paice John A. , Sahu Anwesha 
Published: February 2024

Abstract
Cataclysmic variables can experience short optical brightenings, which are commonly attributed to phenomena such as dwarf novae outbursts, micronovae, donor flares, or magnetic gating bursts. Since these events exhibit similar observational characteristics, their identification has often been ambiguous. In particular, magnetic gating bursts and micronovae have been suggested as alternative interpretations of the same phenomena. Here we show that the timescales and energies separate the optical brightenings into separate clusters consistent with their different classifications. This suggests that micronovae and magnetic gating bursts are in fact separate phenomena. Based on our findings, we develop diagnostic diagrams that can distinguish between these bursts/flares based on their properties. We demonstrate the effectiveness of this approach on observations of a newly identified intermediate polar, CTCV J0333-4451, which we classify as a magnetic gating system. CTCV J0333-4451 is the third highest spin-to-orbital period ratio intermediate polar with magnetic gating, suggesting that these bursts are common among these rare systems.