bluuebunny/crossref_metadata_2025_split huggingface dataset:
Exérese de cistoadenoma associado à glândula parótida: Relato de caso clínico
Authors: Silva Fábia Rayanne Oliveira e , Santos Silva Mariana Roberta , De Medeiros Albuquerque Maria Eduarda , De Holanda Vasconcellos Ricardo José , Ribeiro Lilian Nunes , De Pontes Felix Larissa Polyanna , Sant'Ana Maria Eduarda Cezar de , Araújo Emerllyn Shayane Martins de , Ugarte Rodrigo Gonzalo Valdivia , Melo Filho Sérgio Murilo Cordeiro de , Da Costa Araújo Fábio Andrey , De Oliveira e Silva Emanuel Dias 
Published: March 2024

O cistoadenoma de glândula salivar é uma neoplasia epitelial benigna rara; Histologicamente, apresenta múltiplas cavidades císticas contendo projeções papilares intraluminais e áreas de diferenciação oncocítica. A terapia de eleição é a excisão cirúrgica e casos de recidiva estão associados a remoção incompleta da lesão. Objetivo: O presente trabalho visa relatar um caso clínico raro de cistoadenoma da glândula parótida em um paciente do sexo masculino jovem, descrevendo os aspectos clínicos e histopatológicos da lesão e a abordagem terapêutica realizada. Relato de caso: Paciente do sexo masculino, 25 anos, relatou aumento de volume assintomático na região de glândula parótida direita há 8 meses. O paciente foi tratado com excisão cirúrgica da lesão e análise anatomopatológica concluiu cistoadenoma da glândula parótida. O paciente encontra-se em acompanhamento sem sinais clínicos de recidiva. Conclusão: Apesar de ser uma patologia rara das glândulas salivares, o conhecimento das patologias das glândulas salivares associados a correta indicação de exames imaginológicos e biópsias são indicadores de um prognóstico previsível. A excisão cirúrgica se mostra como o tratamento de eleição para esta patologia, que apresenta prognóstico favorável e poucos relatos de recidiva associados à excisão cirúrgica incompleta da lesão, dificultada pela ausência de cápsula que a delimite.
MANEJO DA GRAVIDEZ DE RISCO E ASSISTÊNCIA AO PRÉ-NATAL
Authors: Ditzel Adriana Nunes , Júnior Eliel Pessôa de Souza , Breitkreitz Victória Schneider , Andrade Carolina Okuyama , Valente Maria Clara , Lima Gabriel Ferreira , Andrade Beatriz Carrijo , Dias Zaine Dupim , Brasil Bruno Sergio Costa , Castro Nathalia Salvagni , Neto Antônio Carlos de Araújo , Santos Luciana ferreira dos , Filho Artur Clímaco Da Silva , Sanches Juliana Dias Gondim 
Published: March 2024

O manejo da gravidez de risco envolve acompanhamento médico mais frequente, exames adicionais e, às vezes, repouso. A assistência ao pré-natal é crucial para monitorar a saúde da mãe e do bebê, permitindo intervenções precoces se necessário. Recomenda-se seguir as orientações médicas e manter um estilo de vida saudável durante esse período. O pré-natal é o cuidado médico que uma mulher recebe durante a gestação para garantir uma gravidez saudável. Isso inclui consultas regulares, exames, orientações sobre nutrição, atividade física e preparação para o parto. É fundamental para monitorar o desenvolvimento do feto e tratar qualquer problema de saúde materna que possa surgir. O objetivo desse artigo foi compreender a importância do pré-natal e além disso evidenciar as complicações de uma gravidez de risco. Foram utilizadas as bases de dados Pubmed, Scielo, Medline, Scopus e Web of Science, com artigos publicados nos idiomas inglês ou português. Em conclusão, o pré-natal é uma parte essencial do cuidado materno durante a gravidez, assegurando um acompanhamento adequado da saúde da mãe e do feto. Ao seguir as orientações médicas, realizar exames regulares e adotar um estilo de vida saudável, contribuímos para o bem-estar geral, favorecendo um parto seguro e a saúde a longo prazo tanto da mãe quanto do bebê.
OPTIMASI SUHU ANNEALING PROSES PCR AMPLIFIKASI GEN ATP1 A1 SAPI JABRES DAN GALEKAN
Authors: Dewi Khosiya Robba  , Tuwi Ramsiati Dyah , Indah Wulansari Wahyuni , Chanafi Mochammad , Asepriyadi  , Ariyanti Rina , Nihaya Ullin 
Published: March 2024

Adanya kenaikan suhu pada lingkungan sekitar ternak sapi lokal Jabres dan sapi Galekan memiliki efek negatif terhadap perkembangan, pertumbuhan, produktivitas dan reproduksi-nya. Untuk itu, diperlukan metode untuk mengetahui kemampuan adaptasi sapi terhadap cekaman panas. Pada penelitian ini, sampel yang digunakan adalah DNA sapi lokal Jabres dan sapi Galekan dengan menggunakan metode penelitian molekuler in-vitro seperti isolasi DNA, Amplifikasi gen ATP1 A1 dengan Optimasi PCR, elektroforesis dan hasil visualisasinya. Isolasi DNA pada 8 sampel darah sapi Jabres dan sapi Galekan menunjukkan hasil isolasi DNA yang tepat dan sesuai dengan ditandai munculnya pita DNA yang terang dan tebal. Sedangkan, suhu annealing pada proses optimasi PCR yang digunakan untuk menempelkan primer forward ATP1 A1 5'- TCC CCA AGC TAG TGA CCA AG -3' dan primer reverse ATP1 A1 5'- TCT GTG GCT CTG ATT CTC CC -3' adalah 57oC, 57,3oC, 58,1oC, 59,3oC, 60,7oC, 61,9oC, 62,7oC, 63oC. Hasil optimasi PCR dielektroforesis dengan 100 volt selama 35 menit kemudian gel agarose hasil elektroforesis divisualisasikan menggunakan UV transilluminator sehingga didapatkan hasil suhu annealing yang optimal pada suhu 57 oC.

Kata Kunci : Sapi, PCR, gen ATP1A1, Annealing
POTENSI DAYA DUKUNG LIMBAH TANAMAN PANGAN DAN HIJAUAN SEBAGAI SUMBER PAKAN TERNAK RUMINANSIA DI KECAMATAN PANCA RIJANG DAN KECAMATAN KULO KABUPATEN SIDENRENG RAPPANG
Authors: Yusuf Subaedy , Hazairin Zubair  , Arif Samsu 
Published: March 2024

Penelitian ini bertujuan untuk mengetahui potensi daya dukung limbah tanaman pangan dan hijauan di Kecamatan Pancarijang dan Kulo, Kabupaten Sidenreng Rappang sebagai sumber pemetaan wilayah terhadap pengembangan peternakan. Penelitian ini dilakukan menggunakan data sekunder yaitu populasi ternak ruminansia dan luas panen tanaman pangan dan hijauan. Hasil penelitian menunjukkan produksi bahan kering limbah tanaman pangan dan hijauan di Kecamatan Pancarijang yaitu 21.661,77 ton bahan kering (BK) dan Kecamatan Kulo sebesar 28.837,86 ton BK. Produksi limbah tanaman pangan dan hijauan tertinggi berasal dari Desa Rijangpanua, Kecamatan Kulo yaitu sebesar 8964,48 ton BK. Daya dukung untuk pakan yang berasal dari limbah jerami padi, jagung dan hijauan yaitu sebanyak 19.001,56 satuan ternak (ST) di Kecamatan Pancarijang dan 25.296,37 ST di Kecamatan Kulo. Hasil analisis location quotient (LQ) di Kecamatan Pancarijang menunjukkan LQ >1 untuk jerami padi terdapat berada pada lima Desa yaitu Rappang, Lalebata, Macorawalie, Kadidi, dan Timureengpanua, sementara Desa tempat program DKS memiliki LQ <1 untuk jerami padi, namun mempunyai keunggulan LQ>1 berasal dari jerami jagung dan hijauan. Demikian nilai LQ >1 di Kecamatan Kulo untuk jerami padi terdapat empat Desa yaitu Kulo, Maddenra, Bina Baru dan Abbokongang, sedangkan Desa Mario dan Rijangpanua memiliki LQ<1. Namun, kedua Desa tersebut memiliki keunggulan yang sama dengan wilayah DKS di Kecamatan Pancarijang yaitu memiliki jerami jagung dan hijauan yang dapat mendukung ketersediaan limbah tanaman pangan berdasarkan bahan kering sebagai pakan ternak ruminansia.

Kata kunci: Daya dukung, Hijauan, Limbah tanaman pangan, Location quotient, Produksi bahan kering
PENGGUNAAN TEPUNG MAGGOT BSF (Hermetia illucens) DALAM RANSUM TERHADAP PERFORMA PERTUMBUHAN AYAM PETELUR JANTAN
Authors: Susanto Jepri , Kaharuddin Desia , Kususiyah  
Published: March 2024

Penelitian ini bertujuan untuk mengevaluasi pengunaan tepung maggot BSF (Hermetia illucens) dalam ransum terhadap performa pertumbuhan ayam petelur jantan. Penelitian menggunakan Rancangan Acak Lengkap (RAL) 4 perlakuan dengan 5 ulangan dan setiap ulangan menggunakkan 8 ekor ayam petelur jantan strain Lohmann Brown. Faktor pembeda antar perlakuan adalah level penggunaan tepung maggot dalam ransum, yaitu: 0% (P0), 4% (P1), 8% (P2), dan 12% (P3). Variabel pengamatan yaitu konsumsi ransum, bobot badan, pertambahan bobot badan dan konversi ransum. Hasil penelitian menunjukkan bahwa penggunaan tepung maggot berpengaruh nyata (P<0,05) terhadap performa pertumbuhan ayam petelur jantan. Konsumsi ransum, bobot badan dan pertambahan bobot badan P0 dan P1 nyata lebih tinggi dibandingkan P2 dan P3, sedangkan konversi ransum P0, P1, dan P2 lebih rendah dibandingkan P3. Dapat disimpulkan bahwa tepung maggot dapat digunakan sampai level 4% tanpa menurunkan konsumsi ransum, bobot badan dan pertambahan bobot badan, sedangkan efisiensi ransum menurun pada level 12%.

Kata kunci : Ayam Petelur Jantan, Performa Pertumbuhan, Tepung Maggot.
PERAN KELOMPOK WANITA DALAM PENGEMBANGAN PETERNAKAN KAMBING PE: KONTRIBUSI TERHADAP PENCAPAIAN SUSTAINABLE DEVELOPMENT GOALS (SDGs)
Authors: Rosa Zulfikhar  , Budi Purwo Widiarso  , Sukadi  , Wardi  
Published: March 2024

Penelitian ini bertujuan untuk mengetahui pengaruh lima variabel karakteristik inovasi, antara lain keuntungan relatif, keselarasan, kerumitan, dapat dicoba, dan dapat diamati, terhadap persepsi peran wanita dalam mengembangkan peternakan kambing Peranakan Etawa (PE) serta kontribusi pencapaian sustainable development goals (SDGs). Terdiri dari kelompok Wanita tani di Desa Ngargoretno, kecamatan Salaman, kabupaten Magelang. Penentuan lokasi penelitian dilakukan secara purposive berdasarkan pertimbangan bahwa kabupaten magelang digunakan untuk pengembangan kambing PE. Metode penelitian menggunakan analisis kuantitatif deskriptif untuk mendapatkan 30 anggota kelompok tani wanita sebagai responden. Selanjutnya variabel yang diteliti adalah karakteristik inovasi dan persepsi petani yang diukur dengan model matematika menggunakan kategori skor masing-masing variabel dan program SPPS. Hasil penelitian menunjukkan bahwa persepsi petani terhadap kelima variabel tersebut termasuk dalam kategori setuju. Hal ini mendapat dukungan positif dari responden dengan melihat keuntungan penerapan paket teknologi pada pengembangan kambing PE. Ditinjau dari aspek peran wanita dalam pengembangan kambing PE dapat mengambarkan kesetaran gender dalam dunia peternakan. Selanjutnya dapat menjadi pencapaian sustainable development goals (SDGs).

Kata kunci: KWT Bugenvil, Persepsi, SDGs, Wanita
New records of herbivory of Leucothyreus MacLeay, 1819 (Coleoptera: Scarabaeidae: Geniatini) on Cecropia Loefl. (Urticaceae)
Authors: Aguiar Daniel P. P. , Bento Matheus 
Published: March 2024

Species in the genus Cecropia Loefl. (Urticaceae) are important food sources for a handful of species belonging to the insect orders Orthoptera (grasshoppers), Lepidoptera (caterpillars), Hymenoptera (leafcutter ants), and Coleoptera (beetles). Among the leaf chafer beetles, specimens of the scarab genus Leucothyreus MacLeay, 1819 (Scarabaeidae: Geniatini) have been barely recorded as defoliators of Cecropia spp., and information about the identity of the involved plant and beetle species is scarce and imprecise. The present paper records for the first time the incidence of two species of Leucothyreus on four species of Cecropia in Central Amazon (Brazil), with short behavioral notes regarding their feeding habits.
A Large and Variable Leading Tail of Helium in a Hot Saturn Undergoing Runaway Inflation
Authors: Gully-Santiago Michael , Morley Caroline V. , Luna Jessica , MacLeod Morgan , Oklopčić Antonija , Ganesh Aishwarya , Tran Quang H. , Zhang Zhoujian , Bowler Brendan P. , Cochran William D. , Krolikowski Daniel M. , Mahadevan Suvrath , Ninan Joe P. , Stefánsson Guđmundur , Vanderburg Andrew , Zalesky Joseph A. , Zeimann Gregory R. 
Published: March 2024

Abstract
Atmospheric escape shapes the fate of exoplanets, with statistical evidence for transformative mass loss imprinted across the mass–radius–insolation distribution. Here, we present transit spectroscopy of the highly irradiated, low-gravity, inflated hot Saturn HAT-P-67 b. The Habitable Zone Planet Finder spectra show a detection of up to 10% absorption depth of the 10833 Å helium triplet. The 13.8 hr of on-sky integration time over 39 nights sample the entire planet orbit, uncovering excess helium absorption preceding the transit by up to 130 planetary radii in a large leading tail. This configuration can be understood as the escaping material overflowing its small Roche lobe and advecting most of the gas into the stellar—and not planetary—rest frame, consistent with the Doppler velocity structure seen in the helium line profiles. The prominent leading tail serves as direct evidence for dayside mass loss with a strong day-/nightside asymmetry. We see some transit-to-transit variability in the line profile, consistent with the interplay of stellar and planetary winds. We employ one-dimensional Parker wind models to estimate the mass-loss rate, finding values on the order of 2 × 1013 g s−1, with large uncertainties owing to the unknown X-ray and ultraviolet (XUV) flux of the F host star. The large mass loss in HAT-P-67 b represents a valuable example of an inflated hot Saturn, a class of planets recently identified to be rare, as their atmospheres are predicted to evaporate quickly. We contrast two physical mechanisms for runaway evaporation: ohmic dissipation and XUV irradiation, slightly favoring the latter.
Powerful Radio-loud Quasars Are Triggered by Galaxy Mergers in the Cosmic Bright Ages
Authors: Breiding Peter , Chiaberge Marco , Lambrides Erini , Meyer Eileen T. , Willner S. P. , Hilbert Bryan , Haas Martin , Miley George , Perlman Eric S. , Barthel Peter , O’Dea Christopher P. , Capetti Alessandro , Wilkes Belinda , Baum Stefi A. , Macchetto Duccio F. , Sparks William , Tremblay Grant , Norman Colin 
Published: March 2024

Abstract
While supermassive black holes are ubiquitous features of galactic nuclei, only a small minority are observed during episodes of luminous accretion. The physical mechanism(s) driving the onset of fueling and ignition in these active galactic nuclei (AGN) are still largely unknown for many galaxies and AGN-selection criteria. Attention has focused on AGN triggering by means of major galaxy mergers gravitationally funneling gas toward the galactic center, with evidence both for and against this scenario. However, several recent studies have found that radio-loud AGN overwhelmingly reside in ongoing or recent major galaxy mergers. In this study, we test the hypothesis that major galaxy mergers are important triggers for radio-loud AGN activity in powerful quasars during cosmic noon (1 ≲ z ≲ 2). To this end, we compare Hubble Space Telescope WFC3/IR observations of the z > 1 3CR radio-loud broad-lined quasars to three matched radio-quiet quasar control samples. We find strong evidence for major-merger activity in nearly all radio-loud AGN, in contrast to the much lower merger fraction in the radio-quiet AGN. These results suggest major galaxy mergers are key ingredients in launching powerful radio jets. Given many of our radio-loud quasars are blue, our results present a possible challenge to the “blowout” paradigm of galaxy evolution models in which blue quasars are the quiescent end result following a period of red quasar feedback initiated by a galaxy merger. Finally, we find a tight correlation between black hole mass and host galaxy luminosity for these different high-redshift AGN samples that is inconsistent with those observed for local elliptical galaxies.
Dust and Volatiles in the Disintegrating Comet C/2019 Y4 (ATLAS)
Authors: Zhao Ruining , Li Aigen , Yang Bin , Wang Liang , Wang Huijuan , Liu Yu-Juan , Liu Jifeng 
Published: March 2024

Abstract
C/2019 Y4 (ATLAS) is an Oort cloud comet with an orbital period of ∼5895 yr. Starting in 2020 March, its nucleus underwent disintegration. In order to investigate the gas and dust properties of C/2019 Y4 (ATLAS) during its disintegration, we obtained long-slit spectra at 3600–8700 Å and BVRI multiband images with the Xinglong 2.16 m Telescope in 2020 April. Our observations revealed that C/2019 Y4 (ATLAS) exhibited strong emission bands of CN, C2, C3, and NH2, which are superimposed on a dust-scattering continuum, typical of cometary spectra in the optical. The production rates of CN, C2, and C3 derived using the Haser model and the corresponding C2/CN and C3/CN ratios suggest that C/2019 Y4 (ATLAS) is a “typical” Oort cloud comet under the A’Hearn classification, although it appears less dusty, as revealed by the Af
ρ quantities. Its dust-scattering reflectivity is slightly red, with a gradient of ∼5% per 103Å. We model the reflectivity gradient in terms of porous dust and find that the red color is accounted for by porous dust.
A Comprehensive Investigation of Gamma-Ray Burst Afterglows Detected by TESS
Authors: Roxburgh Hugh , Ridden-Harper Ryan , Lane Zachary G. , Rest Armin , Hubley Lancia , Hounsell Rebekah , Wang Qinan , Gomez Sebastian , Pierel Justin , Guolo Muryel , Rest Sofia , von Coelln Sophie 
Published: March 2024

Abstract
Gamma-ray bursts produce afterglows that can be observed across the electromagnetic spectrum and can provide insight into the nature of their progenitors. While most telescopes that observe afterglows are designed to rapidly react to trigger information, the Transiting Exoplanet Survey Satellite (TESS) continuously monitors sections of the sky at cadences between 30 minutes and 200 s. This provides TESS with the capability of serendipitously observing the optical afterglow of GRBs. We conduct the first extensive search for afterglows of known GRBs in archival TESS data reduced with the TESSreduce package, and detect 11 candidate signals that are temporally coincident with reported burst times. We classify three of these as high-likelihood GRB afterglows previously unknown to have been detected by TESS, one of which has no other afterglow detection reported on the Gamma-ray Coordinates Network. We classify five candidates as tentative and the remainder as unlikely. Using the afterglowpy package, we model each of the candidate light curves with a Gaussian and a top-hat model to estimate burst parameters; we find that a mean time delay of 740 ± 690 s between the explosion and afterglow onset is required to perform these fits. The high cadence and large field of view make TESS a powerful instrument for localising GRBs, with the potential to observe afterglows in cases when no other backup photometry is possible, and at timescales previously unreachable by optical telescopes.
Detection of Extragalactic Anomalous Microwave Emission in NGC 2903 Using KVN Single-dish Observations
Authors: Poojon Panomporn , Chung Aeree , Hoang Thiem , Baek Junhyun , Nakanishi Hiroyuki , Hirota Tomoya , Tsai Chao-Wei 
Published: March 2024

Abstract
We present the results of the single-dish observations using the Korean VLBI Network to search for anomalous microwave emission (AME) in nearby galaxies. The targets were selected from ‘Mapping the dense molecular gas in the strongest star-forming galaxies' (MALATANG), a legacy survey project of the James Clerk Maxwell Telescope. The MALATANG galaxies are good representatives of local galaxies with enhanced nuclear activity associated with star formation and/or active galactic nuclei (AGNs), providing IR-bright galaxy samples; thus, they are good candidates for AME hosts. Combining with ancillary data, we investigated the radio–IR spectral energy distribution (SED), while searching for AME signals in five galaxies. The AME in NGC 2903 was well detected at a significant confidence level, whereas that in NGC 2146 and M82 was marginal. NGC 1068 and Arp 299 indicated no significant hints, and we provide upper limits for the AME. The best-fit SED exhibited local peaks of the AME components at higher frequencies and with stronger peak fluxes than those in previous studies. This suggested that AME originates from denser environments such as molecular clouds or photodissociation regions rather than warm neutral/ionized medium as commonly suggested by previous studies. Further, our AME-detected targets were observed to exhibit higher specific star formation rates than the other extragalactic AME hosts. Furthermore, AME favored starburst galaxies among our sample rather than AGN hosts. Consequently, this might imply that AGNs are excessively harsh environments for tiny dust to survive.
Complex K: Supernova Origin of Anomalous-velocity H i Structure
Authors: Verschuur G. L. , Schmelz J. T. , Escorza A. , Jorissen A. 
Published: March 2024

Abstract
We address one of the lingering mysteries of high-velocity clouds: If the anomalous negative velocities are the result of the approaching gas from old supernovae, then where are the receding counterparts of the expanding shells? Data from the λ-21 cm Galactic neutral hydrogen EBHIS survey (Winkel et al.) show multiple signatures of the expanding shells. The near-side (approaching) H i shells form part of Complex K. The high blueshifted velocities result from the H i moving into the low-density environment of inter-arm space. The H i data also show a distinctive, bow-shaped feature, the signature of the far-side (receding) emission of an expanding shell. The low redshifted velocity results from the gas expanding into volumes of space with a higher density. If we make the simplifying assumptions that the expansion of the shells is uniform and spherically symmetric, then the explosions took place about ⪅3 × 105 yr ago. The momentum, p ∼ 7 × 104
M
⊙ km s−1, agrees with recent model estimates for supernova evolution. Supernova explosions attributed to the unseen companion in several binary systems identified by the Third Gaia Data Release may be responsible for anomalous-velocity H i gas in Complex K. Four binary star systems with neutron-star candidates are located at the edge of the Sagittarius spiral arm and used to determine the distance to the H i features discussed here.
On the Existence, Rareness, and Uniqueness of Quenched H i-rich Galaxies in the Local Universe
Authors: Li Xiao , Li Cheng , Mo H. J. , Hu Jianhong , Wang Jing , Xiao Ting 
Published: March 2024

Abstract
Using data from ALFALFA, xGASS, H i-MaNGA, and the Sloan Digital Sky Survey (SDSS), we identify a sample of 47 “red but H i-rich” (RR) galaxies with near-UV (NUV) − r > 5 and unusually high H i-to-stellar mass ratios. We compare the optical properties and local environments between the RR galaxies and a control sample of “red and H i-normal” (RN) galaxies that are matched in stellar mass and color. The two samples are similar in the optical properties typical of massive red (quenched) galaxies in the local Universe. The RR sample tends to be associated with slightly lower-density environments and has lower clustering amplitudes and smaller neighbor counts at scales from several hundred kiloparsecs to a few megaparsecs. The results are consistent with the RR galaxies being preferentially located at the center of low-mass halos, with a median halo mass ∼1012
h
−1
M
⊙ compared to ∼1012.5
h
−1
M
⊙ for the RN sample. This result is confirmed by the SDSS group catalog, which reveals a central fraction of 89% for the RR sample, compared to ∼60% for the RN sample. If assumed to follow the H i size–mass relation of normal galaxies, the RR galaxies have an average H i-to-optical radius ratio of R
HI/R
90 ∼ 4, four times the average ratio for the RN sample. We compare our RR sample with similar samples in previous studies, and quantify the population of RR galaxies using the SDSS complete sample. We conclude that the RR galaxies form a unique but rare population, accounting for only a small fraction of the massive quiescent galaxy population. We discuss the formation scenarios of the RR galaxies.