bluuebunny/crossref_metadata_2025_split huggingface dataset:
DOENÇA DE ALZHEIMER: ESTRATÉGIAS DE CUIDADO DIANTE DAS DIFICULDADES AO PORTADOR E CUIDADOR.
Authors: Da Silva Manuelle Rodrigues , Carvalho Lorena Rocha Batista , Barjud Ludmilla Lustosa Elvas , Da Silva Filho Manoel Lopes 
Published: August 2023

A doença de Alzheimer se caracteriza por ser uma doença neurodegenerativa, com um declínio progressivo de funções cognitivas e motoras. Devido a esse quadro irreversível e apresentar deterioração progressiva, tem efeitos devastadores nos portadores e seus familiares. Este trabalho foi desenvolvido com o objetivo de analisar na literatura os impactos, desafios e as atribuições da enfermagem durante o processo de cuidar da doença de Alzheimer na vida do paciente e do cuidador. Trata-se de uma revisão integrativa de literatura acerca das formas de cuidados e de estratégias de enfermagem ao portador de alzheimer, nos anos de 2015 a 2022, dentro das seguintes bases de dados Biblioteca Virtual de Saúde (BVS), Bases de Dados de Enfermagem (BDENF), Scientific Eletronic Library Online (SCIELO), Literatura Latino- Americana e do Caribe em Ciência da Saúde (LILACS) e Medline, utilizando os descritores: Doença de Alzheimer; mal de Alzheimer; Apoiador; Demência, idoso, enfermagem. Os resultados apresentados demonstraram que tanto os portadores da doença de alzheimer como os cuidadores necessitam de uma atenção mais intensiva dos profissionais de saúde devido ao comprometimento mental e outras co-morbidades como a demência. Essa síndrome demencial possui um forte impacto sobre a qualidade de vida tanto dos portadores quanto dos familiares/cuidadores, é considerada como um dos maiores problemas de saúde pública da atualidade. É necessário que o profissional de saúde, em especial, o enfermeiro atualize seus conhecimentos a respeito do cuidado ao idoso portador de demência de Alzheimer, para que possa construir plano de cuidado e estratégias individuais e coletivas. Desse modo, A doença de Alzheimer se configura como um desafio para a sociedade contemporânea, sendo que a Enfermagem tem papel fundamental no cuidado ao portador e ao cuidador.
Antimicrobial Activity of Endophyte Bacteria Isolated from Seaweed (Padina sp.) on the Growth of Bacteria Escherichia coli and Staphylococcus aureus
Authors: Akay Fanesa , Ngangi Jantje , Lawalata Helen J 
Published: August 2023

Padina sp. seaweed is one of the Chlorophyta which has potential as an antimicrobial. This study aimed to determine the antimicrobial activity of Padina sp. seaweed endophytic bacteria against Escherichia coli and Staphylococcus aureus. The method used in this research is descriptive qualitative. The results of the isolation of endophytic microbes of Padina sp. seaweed obtained were seven isolates DP1, DP2, DP3, DP4, AP1, AP2, and AP3. The results of the antimicrobial activity test showed that the seven isolates of endophytic bacteria had potential as antimicrobials. Incubation time for 24 hours showed that the diameter of the inhibition zone formed was 9.75 – 11.55 mm against S. aureus and 7.15 – 10.0 mm against bacteria. E. coli. The AP3 and DP1 isolates had a wider zone, presumably because their antibacterial substances were higher than the other isolates.
Application of Microgranule from IAA Producing-Endophytic Bacterial as Biofetilizer on Rubber Plants (Hevea brasiliences Muell. Arg.)
Authors: Ardiansyah Agung , Warsito Kabul , Ginting Tri Yanita 
Published: August 2023

Rubber plant (Hevea brasiliensis Muell.Arg) is the main commodity of plantations, some of whose products are exported and some to meet domestic needs as raw materials for industrial purposes. Purpose on research diversity and crateristics of endophytic bacteria producing hormone IAA from rubber plants. Then the effectiveness treatment of microgranules addition and immersion of endophite bacterial suspension and rubber seed soaking suspension to spur the growth of rubber plants. This research was conducted using the factorial CRD (Completely Randomized Design) method consisting of 16 treatments with 2 replications. The first factor was immersion of endophite bacterial suspension consisting of R0 = 0 hours; R1 = 12 hours; R2 = 24 hours and R3 = 36 hours and the second factor was the addition of microgranules consisting of J0 = 0 gr; J1 = 10 gr; J2 = 15 gr; J3 = 20 gr. The results of this study showed that the results on the isolation of endophite bacteria from the tea plant from the roots and stems of the tea plant yielded 3 isolates from plant roots and 2 isolates from plant stems. For IAA levels, the five isolates were positive. The use of endophytic bacteria as an alternative biofertilizer has a significant effect on the parameters observed
Exposição crônica ao inseticida Piretróide Deltametrina: Implicações hepáticas e energéticas em morcego frugívoro artibeus lituratus
Authors: Pereira de Freitas Renata Maria , Rizzoli Moreno Ariane Maria , Neves Ana Carolina , Moraes de Castro Mariana , Bontempo Freita Mariella , de Oliveira Jerusa Maria 
Published: August 2023

Inseticidas piretroides foram incorporados no mercado como alternativa menos tóxica para animais não alvo. No entanto, a deltametrina, um inseticida dessa classe, é conhecida por causar toxicidade em exposição aguda e crônica em diferentes animais. Os morcegos são animais não alvo que estão constantemente expostos a pesticidas durante o forrageio e isso pode impactar sua sobrevivência. Objetivou-se avaliar o efeito da exposição crônica Ã deltametrina no estado redox e metabolismo energético de morcegos frugívoros da espécie Artibeus lituratus. Para isso os morcegos foram coletados (n=12) e separados em: grupo controle (Controle; n=6), alimentado com frutos não tratados; grupo deltametrina (DM; n = 6), alimentado com frutos tratados com deltametrina na concentração 1.00 mL/L mais espalhante adesivo (0,015 g/L). Após um período de exposição crônica (35 dias), o estado redox do fígado e rim, as alterações histológicas no fígado, a concentração de glicose e as reservas energéticas foram analisados. A exposição a doses comerciais de deltamentrina induziu estresse oxidativo e alterações morfológicas no fígado, além de causar hipoglicemia e reduzir as reservas energéticas dos morcegos. Considerando que os morcegos estão expostos naturalmente aos pesticidas durante o forrageio, o impacto dessa exposição pode alterar as reservas energéticas e induzir alterações no funcionamento normal do fígado, prejudicando a sobrevivência desses animais e, consequentemente, os serviços ecossistêmicos prestados por eles.
Effectiveness of an Auto-stable Bicanaliculus Intubation Stent in the Management of Acquired Punctal Stenosis
Authors: Sameen Murtaza , Shahid Muhammad , Adnan Muhammad , . Rebecca , Teyyeb Azeem Muhammad 
Published: August 2023

Objective: To determine the effectiveness of an autostable bicanaliculus Intubation stent in the management of acquired punctal stenosis in adults.Study Design: Quasi-experimental study.Place and Duration of Study: The study was carried at the Armed Forces Institute of Ophthalmology (AFIO), Rawalpindi, Pakistan, from April 2022 to November 2022.Materials and Methods: This Quasi-experimental study is being conducted from April 2022 to November 2022 after approval from the hospital ethical review committee. A sum of 16 subjects were included in this study, of which 11 were females, and 4 were males, while one patient did not fulfill the follow-up criteria of our study, so was not included. In adult patients with proximal punctual stenosis, bicanalicular auto-stable self-retaining stents were implanted after performing probing sac syringing. Follow-up was done up to 06 months, and anatomical and functional success was determined with the help of munk score system of epiphora, which states 0 means no epiphora and 5 means constant epiphora.Results: Out of 15 subjects, 11 (73.3%) were females, and 4 (26.7%)) were males, who underwent bicanalicular stents. In 14 (93.3%) subjects, anatomical and functional success was noticed, while in one (6.7%) patient, extrusion of the tube occurred.Conclusion: The treatment of proximal punctual stenosis in adults can be easily done with the help of bicanalicular auto-stable self-retaining stents which not only improve the anatomical success rate but also improves the functioning of the puncti.
Hypoglycemia with Beta-Blocker in Patients with Type II Diabetes
Authors: Wali Rehmat , Muhammad Noor , Rahman Naseem Ur , Khan Tahir Ullah , Waqas Muhammad , Umair Khan Muhammad 
Published: August 2023

Objective: To ascertain the frequency of hypoglycemia in diabetic patients using beta blockers.Study Design: A descriptive cross-sectional study.Place and Duration of Study: The study was conducted in the Department of Nephrology and Medicine, Lady Reading Hospital Peshawar, Pakistan, from 10th October 2021 to 10th April 2022.Materials and Methods: The total number of diabetic patients with hypoglycemia was 196, who were included in this study. The patients’ medical record was assessed, and the use of beta-blocker was noted and recorded.Results: This study included those patients whose ages ranged from 30 to 70 years, with a mean age of 51.964±6.38 years. The average duration of diabetes was 7.989±2.74 years, and an average weight of 87.178 kg. Male patients were 71.9%, and females were 28.1%, 43.9% of diabetic patients who had hypoglycemia used beta blockers. Conclusion: According to this study, diabetic people who take oral beta-blockers have a higher risk of developing hypoglycemia. This research shows that Beta Blocker use causes increased chances of hypoglycemia in people with diabetes.
Analisis Kontekstual Terhadap Ahl al Kitab
Authors: Lailatul Rif’ah  
Published: August 2023

Yahudi dan Nasrani disebut sebagai Ahl kitab adalah karena Allah telah menggutus Nabi-nabi ditengah-tengah mereka dan membawa kitab masing-masing. Kitab Taurah kapada nabi Musa As yang kemudian isinya dirubah. Umat tersebut disebut yahudi dan kitab Injil kepada nabi Isa As. Yang kemudian pengikutnya disebut sebagai nasrani. Mereka disebut ahl kitab karena pada dasarnya kitab yang diturunkan adalah murni dari Allah. berbeda dengan agama yang dibuat berdasarkan kepercayaan yang dikolaborasi oleh budaya, adat istiadat tatakrama dan filosofi sebuah masyarakat. Dalam hal ini penulis berpedoman pada kitab Mu’jam Mufahras li Alfādẓ Al-Qur’ān Al-Karīm dan Mu’jam Al-Mauḍūi li Ᾱyat Al-Qur’ᾱn Al-Karῑm. Dari kitab Mu’jam Mufahras li Alfādẓ Al-Qur’ān Al karim. Penelitian ini merupakan penelitian perpustakaan (library research) yaitu penelitian yang dilakukan dengan mempelajari literatur seperti kitab kuning atau buku-buku serta karya-karya ilmiah yang menuju pada keterangan yang dibahas sebagai sumber data. Adapun teknis analisis data yang digunakan dalam penelitian ini adalah metode deskriptif analisis. Metode deskriptif adalah metode yang mana memaparkan data dan memberikan penjelasan secara mendalam mengenai sebuah data. Metode ini untuk menyelidiki dengan menuturkan data, kemudahan menjelaskan data tersebut. Hasil dari penelitian imi ditemukan bahwa Al quran, didalamnya menyebutkan sekitar 30 ayat yang berada dalam 9 surat mengenai lafaẓ yang berhubungan dengan Ahl al Kitab. Sebagian golongan ahl al kitab akan masuk surga karena di dalam hati mereka ada keimaman kepada Tuhan yang Esa. Pada surat al Mᾱidah ayat 66 dan 68 juga berisi tentang pujian kepada ahl al kitab. Dalam surat al Bayyinah ayat 6 juga menjelaskan tentang orang musyrik dan orang kafir dari golongan ahl kitab akan masuk surga karena mereka menemukan bukti kebenaran tuhan sehingga hati mereka condong pada agama Islam
LULC geospatial OLI/Landsat -7 -8 -9 analysis of Sitakunda Container Depot: MLE and Kappa accuracy for Coastal Urban Sprawl and Infrastructure Change
Authors: Polverino Salvatore , Coppola Antonio 
Published: August 2023

The extent of this research aims to demonstrate a Land Use/Land Cover (LULC) change over a coastal-industrial area of Sitakunda, part of Chittagong region in Bangladesh. Its reference information has included important drivers for this industrial area of 4.00 km2, that highlight its suburban growth that uncontrollably has disaggregated the rural landscape, in a period ranging from 2009 to 2022. Our geospatial analysis has started with the observation of the BM Container Warehouse, that has been recently interested by a dreadful fire.
Young Stellar Object Candidates in IC 417
Authors: Rebull L. M. , Anderson R. L. , Hall G. , Kirkpatrick J. D. , Koenig X. , Odden C. E. , Rodriguez B. , Sanchez R. , Senson B. , Urbanowski V. , Austin M. , Blood K. , Kerman E. , Long J. , Roosa N. 
Published: August 2023

Abstract
IC 417 is in the Galactic plane, and likely part of the Aur OB2 association; it is ∼2 kpc away. Stock 8 is one of the densest cluster constituents; off of it to the east, there is a “nebulous stream” (NS) that is dramatic in the infrared (IR). We have assembled a list of literature-identified young stellar objects (YSOs), new candidate YSOs from the NS, and new candidate YSOs from IR excesses. We vetted this list via inspection of the images, spectral energy distributions (SEDs), and color–color/color–magnitude diagrams. We placed the 710 surviving YSOs and candidate YSOs in ranked bins, nearly two-thirds of which have more than 20 points defining their SEDs. The lowest-ranked bins include stars that are confused, or likely carbon stars. There are 503 in the higher-ranked bins; half are SED Class III, and ∼40% are SED Class II. Our results agree with the literature in that we find that the NS and Stock 8 are at about the same distance from Earth (as are the rest of the YSOs), and that the NS is the youngest region, with Stock 8 being a little older. We do not find any evidence for an age spread within the NS, consistent with the idea that the star formation trigger came from the north. We do not find that the other literature-identified clusters here are as young as either the NS or Stock 8; at best, they are older than Stock 8, and they may not all be legitimate clusters.
Fine Structures of Radio Bursts from Flare Star AD Leo with FAST Observations
Authors: Zhang Jiale , Tian Hui , Zarka Philippe , Louis Corentin K. , Lu Hongpeng , Gao Dongyang , Sun Xiaohui , Yu Sijie , Chen Bin , Cheng Xin , Wang Ke 
Published: August 2023

Abstract
Radio bursts from nearby active M-dwarfs have been frequently reported and extensively studied in solar or planetary paradigms. Whereas, their substructures or fine structures remain rarely explored despite their potential significance in diagnosing the plasma and magnetic field properties of the star. Such studies in the past have been limited by the sensitivity of radio telescopes. Here we report the inspiring results from the high time-resolution observations of a known flare star AD Leo with the Five-hundred-meter Aperture Spherical radio Telescope. We detected many radio bursts in the 2 days of observations with fine structures in the form of numerous millisecond-scale sub-bursts. Sub-bursts on the first day display stripe-like shapes with nearly uniform frequency drift rates, which are possibly stellar analogs to Jovian S-bursts. Sub-bursts on the second day, however, reveal a different blob-like shape with random occurrence patterns and are akin to solar radio spikes. The new observational results suggest that the intense emission from AD Leo is driven by electron cyclotron maser instability, which may be related to stellar flares or interactions with a planetary companion.
Orbital Period Variations in HT Cas: Evidence for Additional Angular Momentum Loss and a High-eccentricity Giant Planet
Authors: Han Z.-T , Qian S.-B , Han Q.-W , Zang L. , Soonthornthum B. , Li L.-J , Zhu L.-Y. , Liu W. , Fernández Lajús E. , Dai Z.-B , Na W.-W 
Published: August 2023

Abstract
We present a timing study of the short-period eclipsing cataclysmic variable (CV) HT Cas. Based on new eclipse times derived from our photometric monitoring and archival optical data, combined with historical timings, spanning ∼42 yr, we detect a secular decrease in the orbital period at a rate of

P

̇

=
−
1.32
×

10

−
12

ss

−
1

and a cyclic period wiggle with an amplitude of 79.3 s and a period of 30.28 yr. We find that neither gravitational radiation nor magnetic braking can explain the observed decrease rate, suggesting the presence of additional angular momentum loss (AML). The empirical consequential AML (eCAML) model developed by Schreiber et al. can well match the observed orbital decay in HT Cas, and the physical mechanism for eCAML is most likely attributable to the frictional AML following nova eruptions. As for the cyclic variation, the best explanation is the influence of an unseen companion in orbit around the binary. The derived orbital parameters reveal that the hypothetical third body could be a giant planet with mass of M
3 ≃ 14M
Jup that is moving on a highly eccentric orbit (e = 0.82). Taken together the results of the present study suggest that HT Cas is a unique triple system containing a high-eccentricity giant planet and it has the potential to become an ideal laboratory in which to test models of CV evolution.
On Secular Gravitational Instability in Vertically Stratified Disks
Authors: Tominaga Ryosuke T. , Inutsuka Shu-ichiro , Takahashi Sanemichi Z. 
Published: August 2023

Abstract
Secular gravitational instability (GI) is one promising mechanism for explaining planetesimal formation. Previous studies of secular GI utilized a razor-thin disk model and derived the growth condition in terms of vertically integrated physical values such as dust-to-gas surface density ratio. However, in weakly turbulent disks where secular GI can operate, a dust disk can be orders of magnitude thinner than a gas disk, and analyses treating the vertical structures are necessary to clarify the interplay of the midplane dust motion and the upper gas motion. In this work, we perform vertically global linear analyses of secular GI with a vertical domain size of a few gas scale heights. We find that dust grains accumulate radially around the midplane while gas circulates over the whole vertical region. We obtain well-converged growth rates when the outer gas boundary is above two gas scale heights. The growth rates are underestimated if we assume the upper gas to be steady and regard it just as the source of external pressure to the dusty lower layer. Therefore, treating the upper gas motion is important even when the dust disk is much thinner than the gas disk. Conducting a parameter survey, we represent the growth condition in terms of the Toomre Q value for dust and dust-to-gas surface density ratio. The critical dust disk mass for secular GI is ∼10−4
M
* for a dust-to-gas surface density ratio of 0.01, a Stokes number of 0.1, and a radial dust diffusivity of 10−4
c
s
H, where c
s is the gas sound speed, and H is the gas scale height.
First Results from the JWST Early Release Science Program Q3D: The Warm Ionized Gas Outflow in z ∼ 1.6 Quasar XID 2028 and Its Impact on the Host Galaxy
Authors: Veilleux Sylvain , Liu Weizhe , Vayner Andrey , Wylezalek Dominika , Rupke David S. N. , Zakamska Nadia L. , Ishikawa Yuzo , Bertemes Caroline , Barrera-Ballesteros Jorge K. , Chen Hsiao-Wen , Diachenko Nadiia , Goulding Andy D. , Greene Jenny E. , Hainline Kevin N. , Hamann Fred , Heckman Timothy , Johnson Sean D. , Grace Lim Hui Xian , Lutz Dieter , Lützgendorf Nora , Mainieri Vincenzo , Maiolino Roberto , McCrory Ryan , Murphree Grey , Nesvadba Nicole P. H. , Ogle Patrick , Sankar Swetha , Sturm Eckhard , Whitesell Lillian 
Published: August 2023

Abstract
Quasar feedback may regulate the growth of supermassive black holes, quench coeval star formation, and impact galaxy morphology and the circumgalactic medium. However, direct evidence for quasar feedback in action at the epoch of peak black hole accretion at z ≈ 2 remains elusive. A good case in point is the z = 1.6 quasar WISEA J100211.29+013706.7 (XID 2028), where past analyses of the same ground-based data have come to different conclusions. Here, we revisit this object with the integral-field unit of the Near Infrared Spectrograph on board the JWST as part of Early Release Science program Q3D. The excellent angular resolution and sensitivity of the JWST data reveal new morphological and kinematic substructures in the outflowing gas plume. An analysis of the emission-line ratios indicates that photoionization by the central quasar dominates the ionization state of the gas with no obvious sign for a major contribution from hot young stars anywhere in the host galaxy. The rest-frame near-UV emission aligned along the wide-angle cone of outflowing gas is interpreted as a scattering cone. The outflow has cleared a channel in the dusty host galaxy, through which some of the quasar ionizing radiation is able to escape and heat the surrounding interstellar and circumgalactic media. Although the warm ionized outflow is not powerful enough to impact the host galaxy via mechanical feedback, radiative feedback by the active galactic nucleus, aided by the outflow, may help to explain the unusually small molecular gas mass fraction in the galaxy host.
Systematic Multiepoch Monitoring of LkCa 15: Dynamic Dust Structures on Solar System Scales
Authors: Sallum Steph , Eisner Josh , Skemer Andy , Murray-Clay Ruth 
Published: August 2023

Abstract
We present the highest-angular-resolution infrared monitoring of LkCa 15, a young solar analog hosting a transition disk. This system has been the subject of a number of direct-imaging studies from the millimeter through the optical, which have revealed multiple protoplanetary disk rings as well as three orbiting protoplanet candidates detected in infrared continuum emission (one of which was simultaneously seen at Hα). We use high-angular-resolution infrared imaging from 2014 to 2020 to systematically monitor these infrared signals and determine their physical origin. We find that three self-luminous protoplanets cannot explain the positional evolution of the infrared sources since the longer time baseline images lack the coherent orbital motion that would be expected for companions. However, the data still strongly prefer a time-variable morphology that cannot be reproduced by static scattered-light disk models. The multiepoch observations suggest the presence of complex and dynamic substructures moving through the forward-scattering side of the disk at ∼20 au or quickly varying shadowing by closer-in material. We explore whether the previous Hα detection of one candidate would be inconsistent with this scenario and in the process develop an analytical signal-to-noise penalty for Hα excesses detected near forward-scattered light. Under these new noise considerations, the Hα detection is not strongly inconsistent with forward scattering, making the dynamic LkCa 15 disk a natural explanation for both the infrared and Hα data.
Abundances of Helium, Neon, Magnesium and Phosphorus in the Atmosphere of the Bp He-weak Star HD 175156
Authors: Monier Richard 
Published: August 2023

Abstract
The synthesis of two spectral intervals in the optical range allows to determine LTE abundances of helium, magnesium, phosphorus and neon for this evolved B subgiant. Compared to the solar abundances, helium, neon and phosphorus are found to be overabundant by a factor of 5, magnesium by a factor of 4. The helium line at 4471 Å recorded by two different instruments about ten years apart does not vary. Additional information on the abundances of other elements was also inferred: carbon, oxygen, aluminum, sulfur and iron have abundances very close to the solar values, in contrast nitrogen, titanium and xenon require mild overabundances.