bluuebunny/crossref_metadata_2025_split huggingface dataset:
RELATIONSHIP BETWEEN KNOWLEDGE AND COMMUNITY BEHAVIOR IN PRIMARY PREVENTION OF DHF IN VILLA MAKMUR, BEKASI
Authors: Martina Siska evi 
Published: January 2020

In Indonesia, incidence of Dengue Hemorrhagic Fever (DHF) is increasing dramatically. The purpose of this study was to identify the relationship between knowledge level and community behavior in primary prevention of DHF in Villa Makmur, Bekasi. A cross sectional study was conducted with 144 respondents which is taking by purposive sampling technique. Questionarries thad had been compiled and modified was used as a tool in this study. The questionarries composed of the demographic characteristic and knowledge of DHF prevention. The study found that 72 respondents (50%) were 40-55 years old, 79 respondents were secondary level of education (54.9%), 131 respondents were employed (91%), 70 respondents had an enough knowledge about dengue (48.6%) and 78 respondents had a good behavior in prevention of DHF. There were a correlation between knowledge with primary prevention behavior of dengue fever with p value = 0.000 (p <0,05). Prevention of DHF is very important to reduce the incidence of DHF. The community should be aware and improve the knowledge of DHF prevention.
PENGARUH PELATIHAN MEMOTONG KUKU TERHADAP PERILAKU MEMOTONG KUKU ANAK RETARDASI MENTAL DI SLB DAERAH ISTIMEWA YOGYAKARTA (DIY)
Authors: . Titik Endarwati , Mendri Ni Ketut , Badiah Atik 
Published: January 2020

Menurut data Indonesian Society for Special Needs Education (ISSE) – lembaga yang memfokuskan perhatiannya pada pendidikan anak-anak berkebutuhan khusus di Indonesia terdapat lebih dari 2,6 juta orang anak berkebutuhan khusus yang berusia sekolah di negara ini. Dari jumlah tersebut, yang mengikuti pendidikan di sekolah-sekolah khusus hanya sekitar 48 ribu orang, atau kurang lebih 1,83% saja. Anak retardasi mental juga perlu mendapatkan penanganan khusus dengan melibatkan orang tua dalam mendampingi selama di rumah antara lain melatih memotong kuku pada anak retardasi mental.Tujuan : Diketahui pengaruh pelatihan memotong kuku terhadap perilaku memotong kuku anak retardasi mental di SLB Daerah Istimewa Yogyakarta (DIY)Metode : Jenis penelitian Quasi eksperiment dengan rancangan“Pre test Post test with Control Group Design“. Rancangan ini ada kelompok pembanding (kontrol), observasi dilakukan dua kali. Pengambilan sampel dilakukan secara purposive sampling dengan kriteria anak retardasi mental usia sekolah di SLB Daerah Istimewa Yogyakarta (DIY). Data hasil pemeriksaan dianalisis secara diskriptif dan secara analitik dengan bantuan program SPSS for windows versi 16.0 menggunakan uji pair t-test, wilcoxon, mann whitney dengan taraf signifikan 0,05.Hasil :Memotong kuku pada kelompok eksperimen pre test dan post test dengan nilai p (sig) 0,000 < 0,05. Memotong kuku pada kelompok eksperimen. Memotong kuku pada kelompok kontrol pre test dan post test dengan nilai p (sig) 0,002 < 0,05.Kesimpulan :Ada pengaruh pelatihan memotong kuku terhadap perilaku memotong kuku anak retardasi mental di SLB Daerah Istimewa Yogyakarta (DIY) dengan nilai p (sig) < 0,05 berarti Ha diterima dan Ho ditolak.Saran :Buku saku pelatihan memotong kuku dapat digunakan sebagai model pemberdayaan keluarga pada anak dengan retardasi mental di SLB Daerah Istimewa Yogyakarta (DIY). Kata Kunci :Pelatihan memotong kuku, Perilaku memotong kuku, anak retardasi mental
On the link between attentional search and the oculomotor system: Is preattentive search restricted to the range of eye movements?
Authors: Casteau Soazig , Smith Daniel T. 
Published: January 2020

AbstractIt has been proposed that covert visual search can be fast, efficient, and stimulus driven, particularly when the target is defined by a salient single feature, or slow, inefficient, and effortful when the target is defined by a nonsalient conjunction of features. This distinction between fast, stimulus-driven orienting and slow, effortful orienting can be related to the distinction between exogenous spatial attention and endogenous spatial attention. Several studies have shown that exogenous, covert orienting is limited to the range of saccadic eye movements, whereas covert endogenous orienting is independent of the range of saccadic eye movements. The current study examined whether covert visual search is affected in a similar way. Experiment 1 showed that covert visual search for feature singletons was impaired when stimuli were presented beyond the range of saccadic eye movements, whereas conjunction search was unaffected by array position. Experiment 2 replicated and extended this effect by measuring search times at 6 eccentricities. The impairment in covert feature search emerged only when stimuli crossed the effective oculomotor range and remained stable for locations further into the periphery, ruling out the possibility that the results of Experiment 1 were due to a failure to fully compensate for the effects of cortical magnification. The findings are interpreted in terms of biased competition and oculomotor theories of spatial attention. It is concluded that, as with covert exogenous orienting, biological constraints on overt orienting in the oculomotor system constrain covert, preattentive search.
Testing the Spectroscopic Extraction of Suppression of Convective Blueshift
Authors: Miklos M. , Milbourne T. W. , Haywood R. D. , Phillips D. F. , Saar S. H. , Meunier N. , Cegla H. M. , Dumusque X. , Langellier N. , Maldonado J. , Malavolta L. , Mortier A. , Thompson S. , Watson C. A. , Cecconi M. , Cosentino R. , Ghedina A. , Li C-H. , López-Morales M. , Molinari E. , Poretti Ennio , Sasselov D. , Sozzetti A. , Walsworth R. L. 
Published: January 2020

Abstract
Efforts to detect low-mass exoplanets using stellar radial velocities (RVs) are currently limited by magnetic photospheric activity. Suppression of convective blueshift is the dominant magnetic contribution to RV variability in low-activity Sun-like stars. Due to convective plasma motion, the magnitude of RV contributions from the suppression of convective blueshift is related to the depth of formation of photospheric spectral lines for a given species used to compute the RV time series. Meunier et al. used this relation to demonstrate a method for spectroscopic extraction of the suppression of convective blueshift in order to isolate RV contributions, including planetary RVs, that contribute equally to the time series for each spectral line. Here, we extract disk-integrated solar RVs from observations over a 2.5 yr time span made with the solar telescope integrated with the HARPS-N spectrograph at the Telescopio Nazionale Galileo (La Palma, Canary Islands, Spain). We apply the methods outlined by Meunier et al. We are not, however, able to isolate physically meaningful contributions due to the suppression of convective blueshift from this solar data set, potentially because our data set is taken during solar minimum when the suppression of convective blueshift may not sufficiently dominate activity contributions to RVs. This result indicates that, for low-activity Sun-like stars, one must include additional RV contributions from activity sources not considered in the Meunier et al. model at different timescales, as well as instrumental variation, in order to reach the submeter per second RV sensitivity necessary to detect low-mass planets in orbit around Sun-like stars.
Probing the Properties of the Pulsar Wind in the Gamma-Ray Binary HESS J0632+057 with NuSTAR and VERITAS Observations
Authors: Archer A. , Benbow W. , Bird R. , Brill A. , Brose R. , Buchovecky M. , Christiansen J. L. , Chromey A. J. , Cui W. , Falcone A. , Feng Q. , Finley J. P. , Fortson L. , Furniss A. , Gent A. , Gillanders G. H. , Giuri C. , Gueta O. , Hanna D. , Hassan T. , Hervet O. , Holder J. , Hughes G. , Humensky T. B. , Kaaret P. , Kelley-Hoskins N. , Kertzman M. , Kieda D. , Krause M. , Lang M. J. , Maier G. , Moriarty P. , Mukherjee R. , Nieto D. , Nievas-Rosillo M. , O’Brien S. , Ong R. A. , Otte A. N. , Park N. , Petrashyk A. , Pfrang K. , Pohl M. , Prado R. R. , Pueschel E. , Quinn J. , Ragan K. , Reynolds P. T. , Ribeiro D. , Richards G. T. , Roache E. , Sadeh I. , Santander M. , Schlenstedt S. , Sembroski G. H. , Sushch I. , Weinstein A. , Wilcox P. , Wilhelm A. , Williams D. A. , Williamson T. J ,   (VERITAS Collaboration), Hailey C. J. , Mandel S. , Mori K. ,   (NuSTAR Collaboration)
Published: January 2020

Abstract
HESS J0632+057 is a gamma-ray binary composed of a compact object orbiting a Be star with a period of about 315 days. Extensive X-ray and TeV gamma-ray observations have revealed a peculiar light curve containing two peaks, separated by a dip. We present the results of simultaneous observations in hard X-rays with NuSTAR and in TeV gamma-rays with VERITAS, performed in 2017 November and December. These observations correspond to the orbital phases ϕ ≈ 0.22 and 0.3, where the fluxes are rising toward the first light-curve peak. A significant variation of the spectral index from 1.77 ± 0.05 to 1.56 ± 0.05 is observed in the X-ray data. The multiwavelength spectral energy distributions (SED) derived from the observations are interpreted in terms of a leptonic model, in which the compact object is assumed to be a pulsar and nonthermal radiation is emitted by high-energy electrons accelerated at the shock formed by the collision between the stellar and pulsar wind. The results of the SED fitting show that our data can be consistently described within this scenario, and allow us to estimate the magnetization of the pulsar wind at the location of the shock formation. The constraints on the pulsar wind magnetization provided by our results are shown to be consistent with those obtained from other systems.
Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single-star and Binary Merger Progenitor Models for SN 1987A
Authors: Ono Masaomi , Nagataki Shigehiro , Ferrand Gilles , Takahashi Koh , Umeda Hideyuki , Yoshida Takashi , Orlando Salvatore , Miceli Marco 
Published: January 2020

Abstract
We perform three-dimensional hydrodynamic simulations of aspherical core-collapse supernovae, focusing on the matter mixing in SN 1987A. The impacts of four progenitor (pre-supernova) models and parameterized aspherical explosions are investigated. The four pre-supernova models include a blue supergiant (BSG) model based on a slow-merger scenario developed recently for the progenitor of SN 1987A (Urushibata et al. 2018). The others are a BSG model based on a single-star evolution and two red supergiant (RSG) models. Among the investigated explosion (simulation) models, a model with the binary merger progenitor model and an asymmetric bipolar-like explosion, which invokes a jetlike explosion, best reproduces constraints on the mass of high-velocity 56Ni, as inferred from the observed [Fe ii] line profiles. The advantage of the binary merger progenitor model for the matter mixing is the flat and less extended ρ
r
3 profile of the C+O core and the helium layer, which may be characterized by the small helium core mass. From the best explosion model, the direction of the bipolar explosion axis (the strongest explosion direction) and the neutron star (NS) kick velocity and direction are predicted. Other related implications and future prospects are also given.
HST Imaging of the Ionizing Radiation from a Star-forming Galaxy at z = 3.794
Authors: Ji Zhiyuan , Giavalisco Mauro , Vanzella Eros , Siana Brian , Pentericci Laura , Jaskot Anne , Liu Teng , Nonino Mario , Ferguson Henry C. , Castellano Marco , Mannucci Filippo , Schaerer Daniel , Fynbo Johan Peter Uldall , Papovich Casey , Carnall Adam C. , Amorin Ricardo , Simons Raymond C. , Hathi Nimish , Cullen Fergus , McLeod Derek 
Published: January 2020

Abstract
We report on the Hubble Space Telescope (HST) detection of the Lyman-continuum (LyC) radiation emitted by a galaxy at redshift z = 3.794 dubbed Ion1. The LyC from Ion1 is detected at 820−890 Å with HST WFC3/UVIS in the F410M band (m
410 = 27.60 ± 0.36 m
AB, peak signal-to-noise ratio (S/N) = 4.17 in an r = 0.″12 aperture) and 700−830 Å with the Very Large Telescope (VLT)/VIMOS in the U band (m

U
= 27.84 ± 0.19 m
AB, peak S/N = 6.7 with an r = 0.″6 aperture). A 20 hr VLT/VIMOS spectrum shows low- and high-ionization interstellar metal absorption lines and the P Cygni profile of C iv and Lyα in absorption. The latter spectral feature differs from what observed in known LyC emitters, which show strong Lyα emission. An HST far-UV color map reveals that the LyC emission escapes from a region of the galaxy that is bluer than the rest. The F410M image shows that the centroid of the LyC emission is offset from the centroid of the nonionizing UV emission by 0.″12 ± 0.″03, corresponding to 0.85 ± 0.21 kpc, and that its morphology is likely moderately resolved. These morphological characteristics favor a scenario where the LyC photons produced by massive stars escape from low H i column density “cavities” in the interstellar medium. We also collect the VIMOS U-band images of 107 Lyman-break galaxies at 3.40 < z
spec < 3.95, i.e., sampling the LyC, and stack them with inverse-variance weights. No LyC emission is detected in the stacked image, resulting in a 32.5 m
AB flux limit (1σ) and an upper limit of absolute LyC escape fraction f
esc
abs ≤ 0.63%.
The Strength of the 2175 Å Feature in the Attenuation Curves of Galaxies at 0.1 < z ≲ 3
Authors: Battisti A. J. , Cunha E. da , Shivaei I. , Calzetti D. ,   (COSMOS collaboration)
Published: January 2020

Abstract
We update the spectral modeling code MAGPHYS to include a 2175 Å absorption feature in its UV to near-IR dust attenuation prescription. This allows us to determine the strength of this feature and the shape of the dust attenuation curve in ∼5000 star-forming galaxies at

in the COSMOS field. We find that a 2175 Å absorption feature of ∼1/3 the strength of that in the Milky Way is required for models to minimize residuals. We characterize the total effective dust attenuation curves as a function of several galaxy properties and find that the UV slopes of the attenuation curve for COSMOS galaxies show a strong dependence on star formation rate (SFR) and total dust attenuation (A

V
), such that galaxies with higher SFR and A

V
have shallower curves and vice versa. These results are consistent with expectations from radiative transfer that attenuation curves become shallower as the effective dust optical depth increases. We do not find significant trends in the strength of the 2175 Å absorption feature as a function of galaxy properties, but this may result from the high uncertainties associated with this measurement. The updated code is publicly available online (following acceptance).
Effectiveness of Tocilizumab in Patients with Rheumatoid Arthritis Is Unaffected by Comorbidity Burden or Obesity: Data from a US Registry
Authors: Pappas Dimitrios A. , Etzel Carol J. , Crabtree Margaux , Blachley Taylor , Best Jennie , Zlotnick Steve , Kremer Joel M. 
Published: January 2020

ObjectiveComorbidity burden and obesity may affect treatment response in patients with rheumatoid arthritis (RA). Few real-world studies have evaluated the effect of comorbidity burden or obesity on the effectiveness of tocilizumab (TCZ). This study evaluated TCZ effectiveness in treating RA patients with high versus low comorbidity burden and obesity versus nonobesity in US clinical practice.MethodsPatients in the Corrona RA registry who initiated TCZ were stratified by low or high comorbidity burden using a modified Charlson Comorbidity Index (mCCI) and by obese or nonobese status using body mass index (BMI). Improvements in disease activity and functionality after TCZ initiation were compared for the above strata of patients at 6 and 12 months after adjusting for statistically significant differences in baseline characteristics.ResultsWe identified patients with high (mCCI ≥ 2; n = 195) and low (mCCI < 2; n = 575) comorbidity burden and patients categorized as obese (BMI ≥ 30; n = 356) and nonobese (BMI < 30; n = 449) who were treated with TCZ. Most patients (> 95%) were biologic experienced and about one-third of patients received TCZ as monotherapy, with no significant differences between patients by comorbidity burden or obesity status. Improvement in disease activity and functionality at 6 and 12 months was similar between groups, regardless of comorbidity burden or obesity status.ConclusionIn this real-world analysis, TCZ was frequently used to treat patients with high comorbidity burden or obesity. Effectiveness of TCZ did not differ by comorbidity or obesity status.
Premières rencontres
Authors: Fauré Christine 
Published: January 2020

C’est un récit personnel de mes premières rencontres avec Simone de Beauvoir. À quelle occasion l’ai-je rencontrée ? Quel a été le sujet de nos échanges ? Sur la compatibilité de la carrière intellectuelle et de la maternité. Quelle a été l’importance de Mai 68 pour Simone de Beauvoir ? Nos discussions en 1975 autour de la vie de Sartre lors du projet de documentaire La traversée du siècle portent sur la nature des mouvements révolutionnaires contemporains et la place des femmes dans l’histoire des révolutions.
Chère Simone…
Authors: Lévy-Willard Annette 
Published: January 2020

À la fin des années 70, une rencontre arrosée avec Simone de Beauvoir autour du « Sexisme ordinaire » va susciter une vocation. D’où ma lettre émue au « Castor », écrivain (sans « e »), journaliste, philosophe, amoureuse passionnée, engagée et… féministe sans le vouloir. Si libre, si moderne, qui m’a dit ce jour-là : « Et si vous écriviez un article pour Les Temps Modernes sur la révolution féministe aux USA ? » Le Deuxième sexe allait changer la vie de femmes dans le monde entier, Beauvoir allait changer la mienne. Je suis devenue journaliste.
Une vie juste
Authors: Naïr Sami 
Published: January 2020

Exercice de remémoration aussi bien de la manière d’être et de travailler de Simone de Beauvoir, que de mes propres relations avec elle. Femme de convictions et de courage, solidaire jusqu’à la fin de ses jours avec les opprimés, les femmes et tous ceux qui, pour une raison ou une autre, ont à souffrir de l’exclusion et de la domination. Intellectuelle refusant les compromis médiatiques, écrivaine engagée, elle cherchait toujours à donner un sens à son action, et à maintenir Les Temps modernes dans la voie qu’elle avait définie dès l’origine avec Sartre, celle de l’indépendance totale par rapport à tous les pouvoirs et de la fidélité d’abord avec le « penser contre soi », gage d’honnêteté intellectuelle et de salutaire liberté d’esprit.
La tragédie grecque et l’histoire
Authors: Saïd Suzanne 
Published: January 2020

Après une étude rapide des rares tragédies qui empruntent leur sujet à l’histoire, S. Saïd propose une analyse des rapports complexes ente la tragédie et l’histoire dans la critique contemporaine. Après une critique de la « méthode historique » illustrée par les travaux d’E. Delebecque, R. Goossens et A. Podlecki qui s’attachent aux allusions ponctuelles à l’actualité politique et à ses acteurs, elle rend compte des travaux plus récents qui tentent de définir plus largement « le moment historique de la tragédie » et mettent l’accent sur un message politique qui permet, grâce à la distance instaurée par le mythe, une exploration des relations entre l’élite et la masse et une « négociation » entre leurs intérêts respectifs.
Se réunir, contester, manifester
Authors: Dréano Bernard 
Published: January 2020

Depuis la fin du siècle dernier, des « Forums » et autres « contre-sommets » internationaux se tiennent régulièrement, soit en contestation de rencontres internationales institutionnelles, soit en totale indépendance. À la fois convergence de mouvements issus des société civiles, lieu de débats et d’expression des altermondialistes, occasions de manifestations, moyen d’influencer les politiques, ces rencontres ont-elles une efficacité ? La voix des ONG, en particulier en marge des conférences onusiennes, a rendu visible des problèmes fondamentaux et proposer des solutions, mais elle est de plus en plus étouffée, voire diffamée. Loin d’être stériles, les Forums ont pourtant permis de mettre en place des campagnes et réseaux internationaux. Mais ils doivent se reconfigurer pour inclure les acteurs des nouvelles formes de mobilisation qui se développent depuis un dizaine d’années dans le monde.
Sublime catastrophe
Authors: Tenezakis Xenophon 
Published: January 2020

Quelles représentations de la crise écologique conduisent à l’action ? À celles de l’effondrement correspondent les affects de peur, mais aussi du sublime et du sadisme. Il faudrait plutôt solliciter des affects qui rappellent à l’homme sa finitude : l’inquiétude, le grotesque, la joie, l’abnégation.
Cyberespace
Authors: Huyghe François-Bernard 
Published: January 2020

La notion de cyberespace est née sous la plume d’auteurs de science-fiction. Elle renvoie à l’interface entre le contenu de nos esprits et les machines qui engendrent et font circuler images et informations. Sans profondeur, sans distance, sans surface, voué à la seule circulation instantanée de bits informatiques, est-il une simple métaphore ? Et pourtant, outre ses « couches » logicielle (les algorithmes qui le font exister) et sémantique (dans nos têtes qui interprètent les signes venus de l’écran), le cyberespace repose sur une couche matérielle qui est bien quelque part où elle peut être contrôlée ou sabotée. Pour preuve : on parle de sa « balkanisation », et des souverainetés territoriales se la partagent et se la disputent.
La conquête spatiale, de la guerre froide à la coopération internationale
Authors: Clervoy Jean-François , Clervoy Patrick 
Published: January 2020

Durant une grande partie du xx e siècle, la rivalité politique entre les États-Unis et l’Union soviétique fut le vecteur principal de la conquête spatiale. L’effondrement du bloc soviétique ainsi que les crises économiques du bloc occidental ont ensuite conduit les principales puissances spatiales à mettre en place des programmes de coopération durable à l’échelle internationale, qui ont permis des réalisations ambitieuses comme la station spatiale internationale. Demain, avec l’arrivée de nouveaux pays maîtrisant les vols spatiaux, comme la Chine, et de partenaires du secteur privé, ces forces évolueront avec une accélération des programmes d’exploration de l’espace.
Enseigner : philosophes et professeurs de philosophie : Canguilhem et « les hommes exemplaires »
Authors: Fabiani Jean-Louis 
Published: January 2020

La défense canguilhemienne de l’institution philosophique s’inscrit dans une lignée républicaine ; cette attitude diffère de celle propre à certains de ses contemporains (Nizan), ou de ses cadets (Althusser, Foucault). Canguilhem a toujours défendu l’importance de la philosophie quand elle était menacée par les sciences humaines et sociales, tant au moment du succès de l’existentialisme que pendant le structuralisme des années 1960 ; il fut, en même temps, le critique de certaines manières de concevoir la philosophie (existentialiste ou spiritualiste), de certaines modes de sa pratique (journalistique ou littéraire), et un innovateur en matière de pédagogie.