bluuebunny/crossref_metadata_2025_split huggingface dataset:
The results of anterior rectal resection with the formation of a hardware anastomosis in cancer patients
Authors: Kolesnikov E. N. , Snezhko A. V. , Trifanov V. S. , Kozhushko M. A. , Fomenko Yu. A. , Katsieva T. B. , Myagkov R. E. , Sanamyanc S. V. , Averkin M. A. , Egorov G. Yu. 
Published: December 2021

Purpose of the study. A retrospective analysis of the immediate results of performing anterior rectal resections in cancer. Materials and methods. In the Department of Abdominal Oncology No. 1 with a group of X-ray vascular methods of diagnosis and treatment of the clinic of the National Medical Research Centre for Oncology of the Ministry of Health of Russia treatment for rectal cancer operations of anterior rectal resection were performed in 334 patients, while in 143 (42.8 %) cases they were low. As a standard, total mesenteric excision and lymphoid dissection in volume D2 were performed. Combined surgical interventions were performed in 68 (20.4 %) patients for locally spread tumors. As a rule, they were resection in nature and were performed with tumor infiltration of adjacent organs (bladder with ureters, ovaries, uterus, vagina, small intestine, abdominal wall). Colorectal anastomosis using crosslinking devices was formed in all cases, in 316 (94.6 %) cases it was a "side – to-end" junction, in 18 patients – "end-to-end". A preventive proximal intestinal stoma was formed in 73 (21.9 %) cases, where 67 cases it was an ileostomy, and 6 – a transversostomy. The preventive proximal intestinal stoma was not formed among 261 patients. Results. After performing anterior resections for rectal cancer operations, the complications developed in 75 (22.5 %) patients. The most threatening and dangerous complication was the failure of the colorectal anastomosis, which was noted in 12 (3.5 %) cases.This complication occurred in 8.2 % (6 patients out of 73) of preventatively stoma-treated patients, in 2.3 % of patients without a stoma (6 patients out of 261).Conclusion. The use of a preventive proximal intestinal stoma allows you to form a colorectal anastomosis even in the presence of complicated forms of rectal cancer. The number of complications directly referred to the formation of a preventive proximal intestinal stoma is relatively small, but when planning surgery for uncomplicated rectal cancer, the probability of their possible occurrence should be taken into account.
Hipertensi Pada Kehamilan Dan Kejadian BBLR di RSUD Kota Tasikmalaya
Authors: Herliana Lia 
Published: December 2021

Bayi BBLR yang seringkali menjadikan berisiko tidak saja karena komplikasi neonatal yang dialami (misal hiperbilirubinemia dan sindrom gawat nafas) tetapi juga oleh faktor resiko lainnya (misal anomali bawaan yang dikaitkan dengan BBLR). BBLR memerlukan penatalaksanaan yang tepat oleh seorang perawat karena apabila tidak mendapatkan perawatan yang adekuat, BBLR akan menimbulkan dampak terhadap sistem pernafasan, sistem penglihatan, refleks, gerakan-gerakan motorik bahkan dampak jangka panjang yaitu kesulitan belajar dan tingkah laku (neurobehaviour). Penelitian dilatarbelakangi oleh tingginya angka kejadian BBLR di RSUD Kota Tasikmalaya pada setiap tahunnya sehingga diperlukan adanya penelusuran dari penyebab kejadian BBLR yang dialami. Tujuan penelitian untuk mengetahui adanya hubungan antara hipertensi pada kehamilan dengan kejadian BBLR di RSUD Dr. Soekardjo Kota Tasikmalaya. Hipotesis penelitian ada hubungan antara hipertensi pada kehamilan dengan kejadian BBLR. Manfaat penelitian memberikan dasar praktek berbasis bukti ilmiah (evidences based practice) kepada praktisi keperawatan, bahwa ada hubungan antara hipertensi pada kehamilan dengan kejadian BBLR. Metode penelitian kuantitatif dengan pendekatan cross sectional. Pengolahan data menggunakan analisis univariat dan bivariat. Hasil penelitian tidak ada hubungan yang signifikan antara hipertensi pada kehamilan dengan kejadian BBLR di RSUD Kota Tasikmalaya dengan p value>0,05. Saran hendaknya perawat lebih meningkatkan pendidikan kesehatan pada masyarakat agar masyarakat lebih memahami tentang resiko terjadinya BBLR.
Faktor-faktor yang Mempengaruhi Pemeriksaan VCT Pada Ibu Hamil di Puskesmas Puter
Authors: Hennyati Sri , . Rosita , Trianita Nurima 
Published: December 2021

Pemeriksaan VCT merupakan sebuah dialog yang bersifat rahasia antara seseorang dengan petugas kesehatan yaitu konselor yang bertujuan untuk membantu orang itu mengatasi stress dan membuat keputusanâ€“keputusan pribadi berkaitan dengan HIV/AIDS. Penelitian untuk mengetahui faktor yang mempengaruhi pemeriksaan VCT pada ibu hamil di Puskesmas Puter tahun 2017. Desain penelitian menggunakan jenis penelitian deskriptif analitik. Populasi penelitian sebanyak 140 responden. Teknik sampling dalam penelitian ini diambil dengan menggunakan accidental sampling berjumlah 35 responden. Tidak terdapat hubungan antara pendidikan dengan pemeriksaan VCT pada Ibu Hamil dengan p=0,504 > 0,05. Terdapat hubungan pengetahuan dengan pemeriksaan VCT pada Ibu Hamil dengan p=0,027 â‰¤ 0,05, dukungan keluarga dengan pemeriksaan VCT pada Ibu Hamil dengan p=0,001 â‰¤ 0,05, peran tenaga kesehatan dengan pemeriksaan VCT pada Ibu Hamil p=0,015 â‰¤ 0,05, pengetahuan, dukungan suami dan peran tenaga kesehatan dengan pemeriksaan VCT pada Ibu Hamil dengan â‰¤ 0,05. Disarankan kepada ibu hamil agar berperan aktif dalam melaksanakan kegiatan yang bertujuan untuk meningkatkan kesehatan ibu hamil dan keluarganya, dalam hal ini melakukan pemeriksaan VCT sebagai upaya pencegahan penularan HIV dari ibu ke bayi.
Final Targeting Strategy for the Sloan Digital Sky Survey IV Apache Point Observatory Galactic Evolution Experiment 2 North Survey
Authors: Beaton Rachael L. , Oelkers Ryan J. , Hayes Christian R. , Covey Kevin R. , Chojnowski S. D. , De Lee Nathan , Sobeck Jennifer S. , Majewski Steven R. , Cohen Roger E. , Fernández-Trincado José , Longa-Peña Penélope , O’Connell Julia E. , Santana Felipe A. , Stringfellow Guy S. , Zasowski Gail , Aerts Conny , Anguiano Borja , Bender Chad , Cañas Caleb I. , Cunha Katia , Donor John , Fleming Scott W. , Frinchaboy Peter M. , Feuillet Diane , Harding Paul , Hasselquist Sten , Holtzman Jon A. , Johnson Jennifer A. , Kollmeier Juna A. , Kounkel Marina , Mahadevan Suvrath , Price-Whelan Adrian. M. , Rojas-Arriagada Alvaro , Román-Zúñiga Carlos , Schlafly Edward F. , Schultheis Mathias , Shetrone Matthew , Simon Joshua D. , Stassun Keivan G. , Stutz Amelia M. , Tayar Jamie , Teske Johanna , Tkachenko Andrew , Troup Nicholas , Albareti Franco D. , Bizyaev Dmitry , Bovy Jo , Burgasser Adam J. , Comparat Johan , Downes Juan José , Geisler Doug , Inno Laura , Manchado Arturo , Ness Melissa K. , Pinsonneault Marc H. , Prada Francisco , Roman-Lopes Alexandre , Simonian Gregory V. A. , Smith Verne V. , Yan Renbin , Zamora Olga 
Published: December 2021

Abstract
The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is a dual-hemisphere, near-infrared (NIR), spectroscopic survey with the goal of producing a chemodynamical mapping of the Milky Way. The targeting for APOGEE-2 is complex and has evolved with time. In this paper, we present the updates and additions to the initial targeting strategy for APOGEE-2N presented in Zasowski et al. (2017). These modifications come in two implementation modes: (i) “Ancillary Science Programs” competitively awarded to Sloan Digital Sky Survey IV PIs through proposal calls in 2015 and 2017 for the pursuit of new scientific avenues outside the main survey, and (ii) an effective 1.5 yr expansion of the survey, known as the Bright Time Extension (BTX), made possible through accrued efficiency gains over the first years of the APOGEE-2N project. For the 23 distinct ancillary programs, we provide descriptions of the scientific aims, target selection, and how to identify these targets within the APOGEE-2 sample. The BTX permitted changes to the main survey strategy, the inclusion of new programs in response to scientific discoveries or to exploit major new data sets not available at the outset of the survey design, and expansions of existing programs to enhance their scientific success and reach. After describing the motivations, implementation, and assessment of these programs, we also leave a summary of lessons learned from nearly a decade of APOGEE-1 and APOGEE-2 survey operations. A companion paper, F. Santana et al. (submitted; AAS29036), provides a complementary presentation of targeting modifications relevant to APOGEE-2 operations in the Southern Hemisphere.
Mysterious Dust-emitting Object Orbiting TIC 400799224
Authors: Powell Brian P. , Kostov Veselin B. , Rappaport Saul A. , Tokovinin Andrei , Shporer Avi , Collins Karen A. , Corbett Hank , Borkovits Tamás , Gary Bruce L. , Chiang Eugene , Rodriguez Joseph E. , Law Nicholas M. , Barclay Thomas , Gagliano Robert , Vanderburg Andrew , Olmschenk Greg , Kruse Ethan , Schlieder Joshua E. , Soto Alan Vasquez , Goeke Erin , Jacobs Thomas L. , Kristiansen Martti H. , LaCourse Daryll M. , Omohundro Mark , Schwengeler Hans M. , Terentev Ivan A. , Schmitt Allan R. 
Published: December 2021

Abstract
We report the discovery of a unique object of uncertain nature—but quite possibly a disintegrating asteroid or minor planet—orbiting one star of the widely separated binary TIC 400799224. We initially identified the system in data from TESS Sector 10 via an abnormally shaped fading event in the light curve (hereafter “dips”). Follow-up speckle imaging determined that TIC 400799224 is actually two stars of similar brightness at 0.″62 separation, forming a likely bound binary with projected separation of ∼300 au. We cannot yet determine which star in the binary is host to the dips in flux. ASAS-SN and Evryscope archival data show that there is a strong periodicity of the dips at ∼19.77 days, leading us to believe that an occulting object is orbiting the host star, though the duration, depth, and shape of the dips vary substantially. Statistical analysis of the ASAS-SN data shows that the dips only occur sporadically at a detectable threshold in approximately one out of every three to five transits, lending credence to the possibility that the occulter is a sporadically emitted dust cloud. The cloud is also fairly optically thick, blocking up to 37% or 75% of the light from the host star, depending on the true host. Further observations may allow for greater detail to be gleaned as to the origin and composition of the occulter, as well as to a determination of which of the two stars comprising TIC 400799224 is the true host star of the dips.
Radio Observations of SN2004dk with VLITE Confirm Late-time Rebrightening
Authors: Balasubramanian A. , Corsi A. , Polisensky E. , Clarke T. E. , Kassim N. E. 
Published: December 2021

Abstract
The study of stripped-envelope core-collapse supernovae (SNe), with evidence for strong interaction of SN ejecta with the circumstellar medium (CSM), provides insights into the pre-supernova progenitor, and a fast-forwarded view of the progenitor mass-loss history. In this context, we present late-time radio observations of SN 2004dk, a Type Ibc supernova located in the galaxy NGC 6118, at a distance of d

L
≈ 23 Mpc. About 10 yr after explosion, SN 2004dk has shown evidence for Hα emission, possibly linked to the SN ejecta interacting with a H-rich CSM. Using data from the VLA Low Band Ionosphere and Transient Experiment (VLITE), we confirm the presence of a late-time radio rebrightening accompanying the observed Hα emission. We model the SN 2004dk radio light curves within the (spherically symmetric) synchrotron-self-absorption (SSA) model. Within this model, our VLITE observations combined with previously collected VLA data favor an interpretation of SN 2004dk as a strongly CSM-interacting radio SN going through a complex environment shaped by nonsteady mass loss from the SN progenitor.
GASP and MaNGA Surveys Shed Light on the Enigma of the Gas Metallicity Gradients in Disk Galaxies
Authors: Franchetto Andrea , Mingozzi Matilde , Poggianti Bianca M. , Vulcani Benedetta , Bacchini Cecilia , Gullieuszik Marco , Moretti Alessia , Tomičić Neven , Fritz Jacopo 
Published: December 2021

Abstract
Making use of both MUSE observations of 85 galaxies from the survey GASP (GAs Stripping Phenomena in galaxies with MUSE) and a large sample from MaNGA (Mapping Nearby Galaxies at Apache Point Observatory survey), we investigate the distribution of gas metallicity gradients as a function of stellar mass for local cluster and field galaxies. Overall, metallicity profiles steepen with increasing stellar mass up to 1010.3
M
⊙ and flatten out at higher masses. Combining the results from the metallicity profiles and the stellar mass surface density gradients, we propose that the observed steepening is a consequence of local metal enrichment due to in situ star formation during the inside-out formation of disk galaxies. The metallicity gradient−stellar mass relation is characterized by a rather large scatter, especially for 109.8 < M
⋆/M
⊙ < 1010.5, and we demonstrate that metallicity gradients anti-correlate with the galaxy gas fraction. Focusing on the galaxy environment, at any given stellar mass, cluster galaxies have systematically flatter metallicity profiles than their field counterparts. Many subpopulations coexist in clusters: galaxies with shallower metallicity profiles appear to have fallen into their present host halo sooner and have experienced the environmental effects for a longer time than cluster galaxies with steeper metallicity profiles. Recent galaxy infallers, like galaxies currently undergoing ram pressure stripping, show metallicity gradients more similar to those of field galaxies, suggesting they have not felt the effect of the cluster yet.
The Robustness of Synthetic Observations in Producing Observed Core Properties: Predictions for the TolTEC Clouds to Cores Legacy Survey
Authors: Betti S. K. , Gutermuth R. , Offner S. , Wilson G. , Sokol A. , Pokhrel R. 
Published: December 2021

Abstract
We use hydrodynamical simulations of star-forming gas with stellar feedback and sink particles—proxies for young stellar objects (YSOs)—to produce and analyze synthetic 1.1 mm continuum observations at different distances (150–1000 pc) and ages (0.49–1.27 Myr). We characterize how the inferred core properties, including mass, size, and clustering with respect to diffuse natal gas structure, change with distance, cloud evolution, and the presence of YSOs. We find that atmospheric filtering and core segmentation treatments have distance-dependent impacts on the resulting core properties for d < 300 pc and 500 pc, respectively, which dominate over evolutionary differences. Concentrating on synthetic observations at further distances (650–1000 pc), we find a growing separation between the inferred sizes and masses of cores with and without YSOs in the simulations, which is not seen in recent observations of the Monoceros R2 (Mon R2) cloud at 860 pc. We find that the synthetic cores cluster in smaller groups, and that their mass densities are correlated with gas column density over a much narrower range, than those in the Mon R2 observations. Such differences limit the applicability of the evolutionary predictions we report here, but will motivate our future efforts to adapt our synthetic observation and analysis framework to next generation simulations, such as Star Formation in Gaseous Environments (STARFORGE). These predictions and systematic characterizations will help to guide the analysis of cores on the upcoming TolTEC Clouds to Cores Legacy Survey on the Large Millimeter Telescope Alfonso Serrano.
NGC 1605a and NGC 1605b: An Old Binary Open Cluster in the Galaxy
Authors: Camargo Denilso 
Published: December 2021

Abstract
This work communicates the discovery of a binary open cluster within the Galaxy. NGC 1605 presents an unusual morphology with a sparse stellar distribution and a double core in close angular proximity. The 2MASS and Gaia-EDR3 field-star decontaminated color–magnitude diagrams (CMDs) show two distinct stellar populations located at the same heliocentric distance of ∼2.6 kpc, suggesting that there are two clusters in the region, NGC 1605a and NGC 1605b, with ages of 2 Gyr and 600 Myr, respectively. Both Gaia parallax and PM distributions are compact and very similar indicating that they are open clusters (OCs) and share the same kinematics. The large age difference, 1.4 Gyr, point to a formation by tidal capture during a close encounter and the close spatial proximity and similar kinematics suggest an ongoing merger event. There is some prominent tidal debris that appears to trace the cluster's orbits during the close encounter and, unexpectedly, some of them appear to be bound structures; this may suggest that in addition to the evaporation, the merging clusters are being broken apart into smaller structures by the combination of the Galactic disk, the Perseus arm, and mutual tidal interactions. In this sense, the newly found binary cluster may be a key object in the observational validation of theoretical studies on binary cluster pairs formation by tidal capture as well as in the formation of massive clusters by merging, and tidal disruption of stellar systems.
Ubiquitous [O ii] Emission in Quiescent Galaxies at z ≈ 0.85 from the LEGA-C Survey*
Authors: Maseda Michael V. , van der Wel Arjen , Franx Marijn , Bell Eric F. , Bezanson Rachel , Muzzin Adam , Sobral David , D’Eugenio Francesco , Gallazzi Anna , de Graaff Anna , Leja Joel , Straatman Caroline , Whitaker Katherine E. , Williams Christina C. , Wu Po-Feng 
Published: December 2021

Abstract
Using deep rest-frame optical spectroscopy from the Large Early Galaxy Astrophysical Census (LEGA-C) survey, conducted using VIMOS on the ESO Very Large Telescope, we search for low-ionization [O ii] λ
λ 3726,3729 emission in the spectra of a mass-complete sample of z ≈ 0.85 galaxies. We find that 59% of UVJ-quiescent (i.e., non-star-forming) galaxies in the sample have [O ii] emission detected above our completeness limit of 1.5 Å, and the median-stacked spectrum of the remaining sample also shows [O ii] emission. The overall fraction of sources with [O ii] above our equivalent width limit is comparable to what we find in the low-redshift universe from GAMA and MASSIVE, except perhaps at the highest stellar masses (>1011.5
M
⊙). However, stacked spectra for the individual low-equivalent-width systems uniquely indicates ubiquitous [O ii] emission in the higher-z LEGA-C sample, with typical [O ii] luminosities per unit stellar mass that are a factor of ×3 larger than the lower-z GAMA sample. Star formation at higher-z could play a role in producing the [O ii] emission, although it is unlikely to provide the bulk of the ionizing photons. More work is required to fully quantify the contributions of evolved stellar populations or active galactic nuclei to the observed spectra.
Multiwavelength Observation Campaign of the TeV Gamma-Ray Binary HESS J0632 + 057 with NuSTAR, VERITAS, MDM, and Swift
Authors: Tokayer Y. M. , An H. , Halpern J. P. , Kim J. , Mori K. , Hailey C. J. ,   (NuSTAR Collaboration, MDM), Adams C. B. , Benbow W. , Brill A. , Buckley J. H. , Capasso M. , Errando M. , Falcone A. , Farrell K. A , Foote G. M , Fortson L. , Furniss A. , Gent A. , Giuri C. , Hanna D. , Hassan T. , Hervet O. , Holder J. , Hona B. , Humensky T. B. , Jin W. , Kaaret P. , Kertzman M. , Kieda D. , Lang M. J. , Maier G. , McGrath C. E , Moriarty P. , Mukherjee R. , Nievas-Rosillo M. , O’Brien S. , Ong R. A. , Otte A. N. , Park N. , Patel S. , Pfrang K. , Pohl M. , Prado R. R. , Pueschel E. , Quinn J. , Ragan K. , Reynolds P. T. , Ribeiro D. , Roache E. , Ryan J. L. , Santander M. , Schlenstedt S. , Sembroski G. H. , Weinstein A. , Williams D. A. , Williamson T. J ,   (VERITAS Collaboration)
Published: December 2021

Abstract
HESS J0632+057 belongs to a rare subclass of binary systems that emit gamma rays above 100 GeV. It stands out for its distinctive high-energy light curve, which features a sharp “primary” peak and broader “secondary” peak. We present the results of contemporaneous observations by NuSTAR and VERITAS during the secondary peak between 2019 December and 2020 February, when the orbital phase (ϕ) is between 0.55 and 0.75. NuSTAR detected X-ray spectral evolution, while VERITAS detected TeV emission. We fit a leptonic wind-collision model to the multiwavelength spectra data obtained over the four NuSTAR and VERITAS observations, constraining the pulsar spin-down luminosity and the magnetization parameter at the shock. Despite long-term monitoring of the source from 2019 October to 2020 March, the MDM observatory did not detect significant variation in Hα and Hβ line equivalent widths, an expected signature of Be-disk interaction with the pulsar. Furthermore, fitting folded Swift-XRT light-curve data with an intrabinary shock model constrained the orbital parameters, suggesting two orbital phases (at ϕ

D
= 0.13 and 0.37), where the pulsar crosses the Be-disk, as well as phases for the periastron (ϕ
0 = 0.30) and inferior conjunction (ϕ
IFC = 0.75). The broadband X-ray spectra with Swift-XRT and NuSTAR allowed us to measure a higher neutral hydrogen column density at one of the predicted disk-passing phases.
Ecological data in Darwin Core: the case of earthworm surveys
Authors: Shashkov Maxim , Ivanova Natalya , Wieczorek John 
Published: December 2021

This sampling-event dataset provides primary data about species diversity, age structure, abundance (in terms of biomass and density) and seasonal activity of earthworms (Lumbricidae). The study was carried out in old-growth broad-leaved and young forests of two protected areas ("Kaluzhskiye Zaseki" Nature Reserve and Ugra National Park) of Kaluga Oblast (Russia).The published dataset provides new data about earthworm communities in European Russia. We propose a new schema according to Darwin Core for the standardisation of the soil invertebrates survey data.
Database of digital media publications on maternal (family) capital in Russia in 2006–2019
Authors: Kalabikhina Irina E. , Klimenko Herman A. , Banin Evgeny P. , Vorobyeva Ekaterina K. , Lameeva Anna D. 
Published: December 2021

The database contains data from publications of digital Russian-language media registered in the Russian Federation on the topic of maternity capital published in the period from May 10, 2006 to June 30, 2019. The database includes general data on publications on maternity capital in .csv formats (UTF-8 encoding). Full texts of publications are presented in .xml format.
A specialized request was generated for the aggregator of publications of Russian-language digital mass media public.ru. In total, the database consists of 457,888 publications of 7,665 publishing houses from 1,251 settlements located in 85 regions of Russia. The database includes information about the date and type of publication, publisher, place of publication (municipality), texts about maternity capital, and numbers of unique positive, negative, and neutral words and phrases according to the RuSentiLex2017 dictionary, as well as full texts of publications.
Explorer les futurs du travail à l’aide des arts et de la fiction : retour d’expérience
Authors: Kandelman Ingrid , Kaplan Daniel 
Published: December 2021

La prospective est une discipline qui vise à agir dans le présent de manière à influencer le futur. Elle connaît aujourd’hui une forme de « tournant fictionnel » qui vise à mieux explorer des futurs en rupture, à rendre la pratique prospective plus inclusive et à permettre aux individus de prendre conscience de leur capacité à transformer leur environnement. L’article rend compte d’une expérimentation sur les futurs du travail fondée sur l’usage de la fiction. Entre 2018 et 2020, trois ateliers ont testé différentes approches auprès de publics issus d’entreprises. Ils ont montré que le recours à la fiction facilite l’établissement du dialogue au sein de groupes hétérogènes, qu’il aide les individus à s’abstraire des discours dominants sur le futur, et qu’il leur permet de se percevoir comme des acteurs du changement. En revanche, des méthodes restent à développer pour faciliter le passage entre l’imagination de futurs alternatifs et la construction de chemins concrets de transformation.