27 research outputs found
Designing Behavioral Interventions That Work: The Triple T – Triple R Competing Pathways Model
Increasing numbers of children are entering our nation’s schools with mental or behavioral health problems. Although many of these children are included in general education programs, teachers report feeling under- or unprepared to manage problematic behaviors. This is not surprising given that reviews of teacher training programs have evidenced limited coursework in classroom management. Within this paper, we present a framework, the Triple T – Triple R Competing Pathways Model, that is grounded in the tenets of Applied Behavior Analysis (ABA). ABA has decades of empirical evidence to support its use in the classroom. Triple T – Triple R simplifies the competing pathways chart frequently utilized within ABA, rendering our model accessible to teachers who might not have previous training or experience with application of behavioral tenets
Qualificação dos Programas de Prevenção do Câncer de Colo de Útero e do Câncer de Mama em Mulheres na Esf Glória/Imigrante em Santa Cruz do Sul-RS
Trabalho descritivo realizado na UBS/ESF GlĂłria Imigrante em Santa Cruz do Sul em que se buscou melhorar as ações de prevenção do câncer de colo do Ăştero e do câncer de mama em mulheres de 25 a 64 anos e de 50 a 69 anos da área adstrita. O protocolo utilizado como manual tĂ©cnico foi o caderno de controle dos cânceres de colo do Ăştero e de mama do MinistĂ©rio da SaĂşde, atualizado em 2013. Entre os meses de agosto a outubro de 2014 foi realizada intervenção na qual se estabeleceram seis objetivos especĂficos, os quais buscaram ampliação da cobertura de detecção precoce do câncer de colo do Ăştero para 56% e do câncer de mama para 59%, a melhoria da qualidade do atendimento, a melhoria da adesĂŁo Ă realização do citopatolĂłgico e da mamografia, a melhoria do registro das informações, a avaliação de risco para câncer de colo de Ăştero e mama e a promoção Ă saĂşde destas mulheres. As metas de cobertura foram estabelecidas visando as microáreas atendidas por agentes comunitárias de saĂşde (microáreas um, trĂŞs e cinco). Ao fim de doze semanas de intervenção foi atingida a cobertura de 54,8% de mulheres com CP em dia e 27,5% das mulheres com mamografia em dia. As metas referentes Ă qualidade do serviço prestado foram alcançadas integralmente. Isto significa que se obteve 100% de coleta de amostras satisfatĂłrias do CP, que foram pesquisados sinais de alerta para câncer de colo de Ăştero e de mama em 100% das mulheres cadastradas na intervenção, orientou-se 100% das mulheres cadastradas sobre doenças sexualmente transmissĂveis (DST) e fatores de risco para câncer de colo de Ăştero e de mama entre outras ações. AtravĂ©s destas atividades se percebeu a importância das equipes de ESF realizarem seu trabalho guiadas por protocolos que definem as ações de saĂşde ideais a serem realizadas com cada publico alvo. Desta forma Ă© possĂvel se aproximar de uma atenção Ă saĂşde integral e eficiente, de acordo com os princĂpios do SUS para a atenção básica
Extending the feeding period beyond 8.0 mm of subcutaneous fat reduces feed efficiency without improving meat colour and tenderness of non-implanted feedlot steers
The effect of extending the pen-feeding period of non-implanted feedlot steers beyond the 8.0 mm fat thickness (FT) endpoint on performance, carcass and meat traits was evaluated. Sixty-four medium-sized British steers (308 ± 26 kg) were grouped into four blocks by weight and housed in 16 pens. Pens within each block were assigned to one of four finishing periods: 64, 91, 119 and 147 days on feed (DOF). The first harvest (64 DOF) was defined as the projected days to attain 8.0 mm FT. From the 8.0–13.8 mm FT endpoints (64 and 147 DOF, respectively), daily shrunk body weight (SBW) feed conversion increased from 9.98 to 15.76 kg/kg (P 0.10). Overall, the 8.0 mm FT endpoint for non-implanted steers corresponded to proper performance and adequate meat quality.EEA Marcos JuárezFil: Zurbriggen, Guillermo Alberto. Instituto Nacional de TecnologĂa Agropecuaria (INTA). EstaciĂłn Experimental Agropecuaria Marcos Juárez; Argentina. Universidad Nacional de Mar del Plata. Facultad de Ciencias Agrarias; Argentina. Universidad Nacional de Rosario. Facultad de Ciencias Agrarias. Departamento de ProducciĂłn Animal; ArgentinaFil: Maglietti, Carlos Sebastián. Instituto Nacional de TecnologĂa Agropecuaria (INTA). EstaciĂłn Experimental Agropecuaria Balcarce; Argentina.Fil: Pouzo, Laura Beatriz. Instituto Nacional de TecnologĂa Agropecuaria (INTA). EstaciĂłn Experimental Agropecuaria Balcarce; Argentina. Universidad Nacional de Mar del Plata, Facultad de Ciencias Agrarias; ArgentinaFil: Testa, MarĂa Laura. Instituto Nacional de TecnologĂa Agropecuaria (INTA). EstaciĂłn Experimental Agropecuaria Balcarce; Argentina.Fil: Riffel, S. Actividad privada; ArgentinaFil: Elizalde, J. C. Actividad privada; ArgentinaFil: Pavan, Enrique. Instituto Nacional de TecnologĂa Agropecuaria (INTA). EstaciĂłn Experimental Agropecuaria Balcarce; Argentina
AssistĂŞncia de Enfermagem na aplicação do sulfato de magnĂ©sio em pacientes portadoras de prĂ©-eclâmpsia grave e eclâmpsia no Hospital de ClĂnicas de Porto Alegre - HCPA
Este trabalho é o resultado de questionamentos levantados pelas autoras quanto ao esquema de utilização do sulfato de magnésio no tratamento da pré-eclâmpsia grave e eclâmpsia (esquema de Pritchard), adotado pela equipe médica do HCPA, e as recomendações da literatura sobre aplicação de medicamentos por via intramuscular. A pesquisa apresenta os resultados da opinião de 29 enfermeiros que aplicam sulfato de magnésio em pacientes obstétricas, no que se refere ao esquema, técnica, material utilizado, bem como sinais e sintomas apresentados pelas pacientes na aplicação
The Black Hole Mass of NGC 4151. II. Stellar Dynamical Measurement from Near-Infrared Integral Field Spectroscopy
We present a revised measurement of the mass of the central black hole (Mbh)
in the Seyfert 1 galaxy NGC 4151. The new stellar dynamical mass measurement is
derived by applying an axisymmetric orbit-superposition code to near-infrared
integral field data obtained using adaptive optics with the Gemini NIFS
spectrograph. When our models attempt to fit both the NIFS kinematics and
additional low spatial resolution kinematics, our results depend sensitively on
how chi-squared is computed--probably a consequence of complex bar kinematics
that manifest immediately outside the nuclear region. The most robust results
are obtained when only the high spatial resolution kinematic constraints in the
nuclear region are included in the fit. Our best estimates for the BH mass and
H-band mass-to-light ratio are Mbh~(3.76+/-1.15)E7 Msun (1-sigma error) and
M/L(H-band)~0.34+/-0.03 Msun/Lsun (3-sigma error), respectively (the quoted
errors reflect the model uncertainties). Our BH mass measurement is consistent
with estimates from both reverberation mapping (3.57[+0.45/-0.37]E7 Msun) and
gas kinematics (3.0[+0.75/-2.2]E7 Msun; 1-sigma errors), and our best-fit
mass-to-light ratio is consistent with the photometric estimate of
M/L(H-band)=0.4+/-0.2 Msun/Lsun. The NIFS kinematics give a central bulge
velocity dispersion sigma_c=116+/-3 km/s, bringing this object slightly closer
to the M-sigma relation for quiescent galaxies. Although NGC 4151 is one of
only a few Seyfert 1 galaxies in which it is possible to obtain a direct
dynamical BH mass measurement--and thus, an independent calibration of the
reverberation mapping mass scale--the complex bar kinematics makes it less than
ideally suited for this purpose.Comment: 21 pages, 15 figures. Accepted for publication in Ap
A Blueprint for Schoolwide Positive Behavior Support: Implementation of Three Components
This article provides a case study (focus on an eighth-grader with autism) within a case study (focus on an urban middle school) in terms of the implementation of positive behavior support (PBS). Information is provided on the characteristics of three key components of schoolwide PBS-universal support, group support, and individual support. For each component, information is presented on policy, assessment, and intervention in terms of an evolving approach to schoolwide PBS with descriptions of how the components were implemented at the middle school with a particular emphasis on the eighth-grade student. The authors conclude with implications for practice in terms of assessing current resources, providing professional development, and intensifying universal support within urban schools to address some of the complex issues associated with poverty
The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
This paper documents the 16th data release (DR16) from the Sloan Digital Sky Surveys (SDSS), the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of data from the Southern Hemisphere survey of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2); new data from APOGEE-2 North are also included. DR16 is also notable as the final data release for the main cosmological program of the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and all raw and reduced spectra from that project are released here. DR16 also includes all the data from the Time Domain Spectroscopic Survey and new data from the SPectroscopic IDentification of ERosita Survey programs, both of which were co-observed on eBOSS plates. DR16 has no new data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey (or the MaNGA Stellar Library "MaStar"). We also preview future SDSS-V operations (due to start in 2020), and summarize plans for the final SDSS-IV data release (DR17)
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The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
This paper documents the 16th data release (DR16) from the Sloan Digital Sky Surveys (SDSS), the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of data from the Southern Hemisphere survey of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2); new data from APOGEE-2 North are also included. DR16 is also notable as the final data release for the main cosmological program of the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and all raw and reduced spectra from that project are released here. DR16 also includes all the data from the Time Domain Spectroscopic Survey and new data from the SPectroscopic IDentification of ERosita Survey programs, both of which were co-observed on eBOSS plates. DR16 has no new data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey (or the MaNGA Stellar Library "MaStar"). We also preview future SDSS-V operations (due to start in 2020), and summarize plans for the final SDSS-IV data release (DR17)