bluuebunny/crossref_metadata_2025_split huggingface dataset:
O papel dos mestrados profissionais na área de Planejamento Urbano e Regional
Authors: Piquet Rosélia , Vilani Rodrigo Machado 
Published: January 2017

O presente artigo tem por objetivo apresentar os desafios e as contribuições da consolidação dos mestrados profissionais na pós-graduação brasileira. Apesar dessa modalidade estar prevista desde a idealização da pós-graduação na década de 1950, a implementação de mestrados para a formação profissional no Brasil sofreu críticas ao longo de sua implantação. A pesquisa analisa as normas da CAPES relacionadas ao reconhecimento dos mestrados profissionais e dos dados de sua evolução a partir de 2000, particularmente, da área de Planejamento Urbano e Regional. À guisa de conclusão são tecidas considerações gerais e específicas quanto à importância dos mestrados profissionais no âmbito da pós-graduação nacional, formando profissionais qualificados para realizar uma leitura adequada e propor medidas positivas para a construção de uma sociedade justa e igualitária para as presentes e futuras gerações. Palavras-chave: mestrados profissionais; Planejamento Urbano e Regional; CAPES; qualificação profissional. Abstract: The current article’s purpose is to present the challenges and contributions of the professional masters in the Brazilian post-graduation. Although, this modality has been previewed since its idealization in 1950, the implementation of masters due to professional formation has suffered disapproval throughout its execution in Brazil. The study analyses the CAPES (it is a government agency linked with the Brazilian Education Ministry, in charge of promoting high standards for post-graduation courses in Brazil) requirements related to the professional masters recognition and the development of its data since 2000, particularly in the area of Urban and Regional Policy. Looking forward to concluding, it is mentioned general and specific considerations due to the importance of professional masters in the range of national post-graduations, forming qualified professionals to develop an adequate reading and to put forward positive solutions to build a single and egalitarian society to close and future generation. Keywords: professional masters; Urban and Regional Policy; CAPES; professional qualification.
Urbanização extensiva e o processo de interiorização do estado de São Paulo: um enfoque contemporâneo
Authors: Betarelli Junior Admir Antonio , Monte-Mór Roberto Luís De Melo , Simões Rodrigo Ferreira 
Published: January 2017

O propósito deste trabalho é discutir a formação, produção e organização do espaço urbano no estado de São Paulo a partir do processo de interiorização da indústria paulista no final dos anos 1970. O lócus da análise é a indústria, uma vez que no enfoque contemporâneo o processo de industrialização sempre esteve articulado com a produção da espacialidade urbana. Conciliando o método diferencial-estrutural (shift-share), a Análise de Componentes Principais (ACP) e a análise de cluster, foi possível evidenciar que tal processo teve como resultado o fenômeno de urbanização extensiva. Os resultados “fotográficos” apontam que houve uma extensão virtual das condições gerais do tecido urbano-industrial de forma que centralidades polarizadoras e regiões circunvizinhas apresentam vantagens locacionais e competitivas, formando, assim, aglomerações urbanas no território paulista, principalmente, nas regiões beneficiadas pelo processo de interiorização da indústria. Palavras-chave: urbanização extensiva; análise multivariada; análise de cluster; método diferencial-estrutural; indústria; São Paulo. Abstract: The main aim of this paper is to discuss the formation, organization and production of urban areas in State of São Paulo (Brazil) in the variant of the process of industry’s internalization in the late ‘70s. As industrialization has always been linked to the production of urban spatiality in contemporary approach, the locus of analysis is the industry. Combining the method shift-share (Esteban-Marquillas), Principal Component Analysis (PCA) and cluster analysis, we noted evidence that this process has resulted in the phenomenon of extensive urbanization. The main findings of these applications (“photographic”) indicated that there was a virtual extension in general conditions of the urban-industrial fabric so that polarizing centralities and surrounding regions present locational and competitive advantages, forming, therefore, urban agglomerations in the territory of São Paulo, mainly in the regions benefiting with the process of industry’s internalization. Keywords: extensive urbanization; internalization of the industry; shift-share; multivariate analysis; São Paulo (Brazil).
Urbanismo na cidade desigual: o Rio de Janeiro e os megaeventos
Authors: Novais Pedro 
Published: January 2017

O trabalho discute o modo como o tema da desigualdade é considerado no urbanismo no Rio de Janeiro. Para tal, trata das representações populares e científicas da cidade, que se encontram em um continuum entre a coesão e a fragmentação. O texto apoia-se na relação entre espaço físico e espaço social para, em seguida, demonstrar o papel do espaço físico e das representações do espaço na reprodução de relações sociais. Argumenta-se que o urbanismo no Rio de Janeiro sofreu uma inflexão nos anos 1990, resultando em experiências teoricamente inovadoras e politicamente conservadoras. Duas práticas discutidas são o "urbanismo de fragmentos" e os "grandes projetos urbanos". O desconhecimento ou a naturalização da temática da desigualdade sugere a impossibilidade de o urbanismo contemporâneo, em suas versões cariocas, dar respostas às questões sociais.
Projeto BRA/13/008 Consolidação da Cooperação Técnica Sul- Sul Brasileira Resgate e Valorização do Patrimônio Cultural Fronteiriço Inventário do Patrimônio Cultural de Cerro Largo- Uruguai
Authors: Bagé, RS Prefeitura Municipal de Bagé , Departamento de Cerro Largo Intendência Departamental de Cerro Largo , Ministério das Relações Exteriores Agência Brasileira de Cooperação , Pinto da Costa Rodrigues Berenice , Bentancor Pérez María , GilVillaamil Germán , Fernández Alejandro , Entenza José Miguel , Maciel Mastrantonio Tiago , Porciúncula Leal Rita Terezinha , Porciuncula González José Ottoni 
Published: January 2017

O Projeto“Resgate e Valorização do Patrimônio Cultural Fronteiriço” foi elaborado em conjunto pela Intendência de Cerro Largo, Uruguai, e o Município de Bagé, RS, Brasil. O Município de Bagé, então, apresentou-se ao chamado realizado pelo Programa de Projetos de Cooperação Técnica Descentralizada Sul-Sul, da Subchefia de Assuntos Federativos da Presidência da República(SAF/PR) e a Agência Brasileira de Cooperação (ABC/MRE). Em Abril de 2015, vencendo processo licitatório, a empresa Parnaso Arquitetura, inicia o trabalho, divido em cinco produtos:Levantamento do Patrimônio Cultural do Departamento de CerroLargo;Plano Departamental de preservação;Elaboração de Manual de Manutenção de Edifícios Patrimoniais;Normativa resultante do inventário;ElaboraçãodeAnteprojetoparaarestauraçãodeumaconstruçãodevalorpatrimonial. A equipe de trabalho está composta por profissionais brasileiros e uruguaios. O primeiro produto, que está concluído, é o tema de nossa apresentação. Foram visitados todos os locais identificados pela Intendência de Cerro largo como de interesse a preservação e os bens declarados Monumentos Históricos Nacionais Uruguaios através da Lei 14.040 de 20/10/1971, Estes locais compreendem obras arquitetônicas, de engenharia, monumentos, lugares históricos e paisagens, tanto urbanos como rurais. Foram ainda acrescidos, pela equipe de consultoria, exemplares destas categorias, além da identificação de acervos documentais e museológicos, bibliotecas e locais com potencial arqueológico e paleontológico, além do patrimônio imaterial.
Patrimônio Cultural e Políticas Culturais
Authors: De Ávila Cristiane Bartz , Ribeiro Angela Mara Bento , Ribeiro Maria de Fátima Bento 
Published: January 2017

O presente trabalho tem por objetivo analisar como as políticas culturais relacionadas aos estudos sobre o Patrimônio Cultural Imaterial tem se desenvolvido ao longo destes últimos anos. Sabemos que as primeiras iniciativas de preservação do patrimônio estavam atreladas ao patrimônio material, o qual denominamos “pedra e cal”. A partir de discussões sobre a valorização de culturas dos grupos denominados “minorias”[1], há uma preocupação com o patrimônio imaterial, tais como danças e saberes-fazeres.[1] Sobre o uso do termo “minoritários”, ver Appadurai (2009).
GAPS IN PROTOPLANETARY DISKS AS SIGNATURES OF PLANETS. III. POLARIZATION
Authors: Jang-Condell Hannah 
Published: January 2017

ABSTRACT
Polarimetric observations of T Tauri and Herbig Ae/Be stars are a powerful way to image protoplanetary disks. However, interpretation of these images is difficult because the degree of polarization is highly sensitive to the angle of scattering of stellar light off the disk surface. We examine how disks with and without gaps created by planets appear in scattered polarized light as a function of inclination angle. Isophotes of inclined disks without gaps are distorted in polarized light, giving the appearance that the disks are more eccentric or more highly inclined than they truly are. Apparent gap locations are unaffected by polarization, but the gap contrast changes. In face-on disks with gaps, we find that the brightened far edge of the gap scatters less polarized light than the rest of the disk, resulting in slightly decreased contrast between the gap trough and the brightened far edge. In inclined disks, gaps can take on the appearance of being localized “holes” in brightness rather than full axisymmetric structures. Photocenter offsets along the minor axis of the disk in both total intensity and polarized intensity images can be readily explained by the finite thickness of the disk. Alone, polarized scattered light images of disks do not necessarily reveal intrinsic disk structure. However, when combined with total intensity images, the orientation of the disk can be deduced and much can be learned about disk structure and dust properties.
THE EFFECT OF AGN FEEDBACK ON THE INTERSTELLAR MEDIUM OF EARLY-TYPE GALAXIES: 2D HYDRODYNAMICAL SIMULATIONS OF THE LOW-ROTATION CASE
Authors: Ciotti Luca , Pellegrini Silvia , Negri Andrea , Ostriker Jeremiah P. 
Published: January 2017

ABSTRACT
We present two-dimensional hydrodynamical simulations for the evolution of early-type galaxies containing central massive black holes (MBHs), starting at an age of

. The code contains accurate and physically consistent radiative and mechanical active galactic nucleus (AGN) wind feedback, with parsec-scale central resolution. Mass input comes from stellar evolution; energy input includes Type Ia (SNIa) and II supernovae and stellar heating; star formation (SF) is included. Realistic, axisymmetric dynamical galaxy models are built solving the Jeans’ equations. The lowest mass models (

) develop global outflows sustained by SNIa heating, ending with a lower amount of hot gas and new stars. In more massive models, nuclear outbursts last to the present epoch, with large and frequent fluctuations in nuclear emission and from the gas (

). Each burst lasts

years, during which cold, inflowing, and hot, outflowing gas phases coexist. The

relation for the gas matches that of local galaxies. AGN activity causes positive feedback for SF. Roughly half of the total mass loss is recycled into new stars (

), just ≃3% of it is accreted on the MBH, the remainder being ejected from the galaxy. The ratio between the mass of gas expelled to that in new stars, the load factor, is

. Rounder galaxy shapes lead to larger final MBH masses,

, and

. Almost all of the time is spent at very low nuclear luminosities, yet one quarter of the total energy is emitted at an Eddington ratio

. The duty-cycle of AGN activity is approximately 4%.
ALMA MEASUREMENTS OF CIRCUMSTELLAR MATERIAL IN THE GQ LUP SYSTEM
Authors: MacGregor Meredith A. , Wilner David J. , Czekala Ian , Andrews Sean M. , Dai Y. Sophia , Herczeg Gregory J. , Kratter Kaitlin M. , Kraus Adam L. , Ricci Luca , Testi Leonardo 
Published: January 2017

ABSTRACT
We present Atacama Large Millimeter/submillimeter Array observations of the GQ Lup system, a young Sun-like star with a substellar-mass companion in a wide-separation orbit. These observations of 870 μm continuum and CO J = 3–2 line emission with beam size ∼0.″3 (∼45 au) resolve the disk of dust and gas surrounding the primary star, GQ Lup A, and provide deep limits on any circumplanetary disk surrounding the companion, GQ Lup b. The circumprimary dust disk is compact with an FWHM of 59 ± 12 au, while the gas has a larger extent with a characteristic radius of 46.5 ± 1.8 au. By forward-modeling the velocity field of the circumprimary disk based on the CO emission, we constrain the mass of GQ Lup A to be M
* = (1.03 ± 0.05) ∗ (d/156 pc) M
⊙, where d is a known distance, and determine that we view the disk at an inclination angle of 60.°5 ± 0.°5 and a position angle of 346° ± 1°. The 3σ upper limit on the 870 μm flux density of any circumplanetary disk associated with GQ Lup b of <0.15 mJy implies an upper limit on the dust disk mass of <0.04 M
⊕ for standard assumptions about optically thin emission. We discuss proposed mechanisms for the formation of wide-separation substellar companions given the non-detection of circumplanetary disks around GQ Lup b and other similar systems.
HARMONIC SPACE ANALYSIS OF PULSAR TIMING ARRAY REDSHIFT MAPS
Authors: Roebber Elinore , Holder Gilbert 
Published: January 2017

ABSTRACT
In this paper, we propose a new framework for treating the angular information in the pulsar timing array (PTA) response to a gravitational wave (GW) background based on standard cosmic microwave background techniques. We calculate the angular power spectrum of the all-sky gravitational redshift pattern induced at the Earth for both a single bright source of gravitational radiation and a statistically isotropic, unpolarized Gaussian random GW background. The angular power spectrum is the harmonic transform of the Hellings & Downs curve. We use the power spectrum to examine the expected variance in the Hellings & Downs curve in both cases. Finally, we discuss the extent to which PTAs are sensitive to the angular power spectrum and find that the power spectrum sensitivity is dominated by the quadrupole anisotropy of the gravitational redshift map.
THE MOUNT WILSON OBSERVATORY S-INDEX OF THE SUN
Authors: Egeland Ricky , Soon Willie , Baliunas Sallie , Hall Jeffrey C. , Pevtsov Alexei A. , Bertello Luca 
Published: January 2017

ABSTRACT
The most commonly used index of stellar magnetic activity is the instrumental flux scale of singly ionized calcium H & K line core emission, S, developed by the Mount Wilson Observatory (MWO) HK Project, or the derivative index

. Accurately placing the Sun on the S scale is important for comparing solar activity to that of the Sun-like stars. We present previously unpublished measurements of the reflected sunlight from the Moon using the second-generation MWO HK photometer during solar cycle 23 and determine cycle minimum

, amplitude

, and mean

. By establishing a proxy relationship with the closely related National Solar Observatory Sacramento Peak calcium K emission index, itself well correlated with the Kodaikanal Observatory plage index, we extend the MWO S time series to cover cycles 15–24 and find on average

,

,

. Our measurements represent an improvement over previous estimates that relied on stellar measurements or solar proxies with non-overlapping time series. We find good agreement from these results with measurements by the Solar-Stellar Spectrograph at Lowell Observatory, an independently calibrated instrument, which gives us additional confidence that we have accurately placed the Sun on the S-index flux scale.
THE MOSDEF SURVEY: AGN MULTI-WAVELENGTH IDENTIFICATION, SELECTION BIASES, AND HOST GALAXY PROPERTIES
Authors: Azadi Mojegan , Coil Alison L. , Aird James , Reddy Naveen , Shapley Alice , Freeman William R. , Kriek Mariska , Leung Gene C. K. , Mobasher Bahram , Price Sedona H. , Sanders Ryan L. , Shivaei Irene , Siana Brian 
Published: January 2017

ABSTRACT
We present results from the MOSFIRE Deep Evolution Field (MOSDEF) survey on the identification, selection biases, and host galaxy properties of 55 X-ray, IR, and optically selected active galactic nuclei (AGNs) at

. We obtain rest-frame optical spectra of galaxies and AGNs and use the BPT diagram to identify optical AGNs. We examine the uniqueness and overlap of the AGNs identified at different wavelengths. There is a strong bias against identifying AGNs at any wavelength in low-mass galaxies, and an additional bias against identifying IR AGNs in the most massive galaxies. AGN hosts span a wide range of star formation rates (SFRs), similar to inactive galaxies once stellar mass selection effects are accounted for. However, we find (at ∼2–3σ significance) that IR AGNs are in less dusty galaxies with relatively higher SFR and optical AGNs in dusty galaxies with relatively lower SFR. X-ray AGN selection does not display a bias with host galaxy SFR. These results are consistent with those from larger studies at lower redshifts. Within star-forming galaxies, once selection biases are accounted for, we find AGNs in galaxies with similar physical properties as inactive galaxies, with no evidence for AGN activity in particular types of galaxies. This is consistent with AGNs being fueled stochastically in any star-forming host galaxy. We do not detect a significant correlation between SFR and AGN luminosity for individual AGN hosts, which may indicate the timescale difference between the growth of galaxies and their supermassive black holes.
THE TIP OF THE RED GIANT BRANCH DISTANCES TO TYPE IA SUPERNOVA HOST GALAXIES. IV. COLOR DEPENDENCE AND ZERO-POINT CALIBRATION
Authors: Jang In Sung , Lee Myung Gyoon 
Published: January 2017

ABSTRACT
We present a revised Tip of the Red Giant Branch (TRGB) calibration, accurate to 2.7% of distance. A modified TRGB magnitude corrected for its color dependence, the QT magnitude, is introduced for better measurement of the TRGB. We determine the color–magnitude relation of the TRGB from photometry of deep images of HST/ACS fields around eight nearby galaxies. The zero-point of the TRGB at the fiducial metallicity ([Fe/H] = −1.6 (

)) is obtained from photometry of two distance anchors, NGC 4258 (M106) and the Large Magellanic Cloud (LMC), to which precise geometric distances are known: M
QT,TRGB = −4.023 ± 0.073 mag from NGC 4258 and M
QT,TRGB = −4.004 ± 0.096 mag from the LMC. A weighted mean of the two zero-points is M
QT,TRGB = −4.016 ± 0.058 mag. Quoted uncertainty is ∼2× smaller than those of previous calibrations. We compare the empirical TRGB calibration derived in this study with theoretical stellar models, finding that there are significant discrepancies, especially for red color (

). We provide the revised TRGB calibration in several magnitude systems for future studies.
Detailed Analysis of the Articular Domain in Patients with Primary Sjögren Syndrome
Authors: Moerman Rada V. , Arends Suzanne , Meiners Petra M. , Vissink Arjan , Spijkervet Frederik K.L. , Kroese Frans G.M. , Brouwer Elisabeth , Bootsma Hendrika 
Published: January 2017

Objective.We used the 28-joint Disease Activity Score (DAS28) and the European League Against Rheumatism Sjögren’s Syndrome Disease Activity Index (ESSDAI) articular domain to assess the effect of rituximab (RTX) and abatacept (ABA) on articular involvement in primary Sjögren syndrome (pSS).Methods.Patients with pSS treated with RTX (n = 18) or ABA (n = 13) and having a DAS28 erythrocyte sedimentation rate (ESR)/C-reactive protein (CRP) level ≥ 3.2 at baseline were selected. Generalized estimating equations were used to analyze the DAS28 and ESSDAI articular domain over time.Results.In the RTX group, DAS28-ESR/CRP decreased significantly up to 48 weeks. In the ABA group, DAS28-ESR/CRP decreased significantly up to 24 weeks. DAS28 correlated significantly with ESSDAI articular domain.Conclusion.DAS28 is useful to evaluate the effect of biologicals on articular involvement in patients with pSS.
Cardiopulmonary Disease Development in Anti-RNA Polymerase III-positive Systemic Sclerosis: Comparative Analyses from an Unselected, Prospective Patient Cohort
Authors: Hoffmann-Vold Anna-Maria , Midtvedt Øyvind , Tennøe Anders H. , Garen Torhild , Lund May Brit , Aaløkken Trond M. , Andreassen Arne K. , Elhage Fadi , Brunborg Cathrine , Taraldsrud Eli , Molberg Øyvind 
Published: January 2017

Objective.Extensive skin disease and renal crisis are hallmarks of anti-RNA polymerase III (RNAP)-positive systemic sclerosis (SSc), while lung and heart involvement data are conflicting. Here, the aims were to perform time-course analyses of interstitial lung disease (ILD) and pulmonary hypertension (PH) in the RNAP subset of a prospective unselected SSc cohort and to use the other autoantibody subsets as comparators.Methods.The study cohort included 279 patients with SSc from the observational Oslo University Hospital cohort with complete data on (1) SSc-related autoantibodies, (2) paired, serial analyses of lung function and fibrosis by computed tomography, and (3) PH verified by right heart catheterization.Results.RNAP was positive in 33 patients (12%), 79% of which had diffuse cutaneous SSc. Pulmonary findings were heterogeneous; 49% had no signs of fibrosis while 18% had > 20% fibrosis at followup. Forced vital capacity at followup was < 80% in 39% of the RNAP subset, comparable to the antitopoisomerase subset (ATA; 47%), but higher than anticentromere (ACA; 13%). Accumulated frequency of PH in the RNAP subset (12%) was lower than in ACA (18%). At 93% and 78%, the 5- and 10-year survival rates in RNAP were comparable to the ATA and ACA subsets.Conclusion.In this cohort, the RNAP subset was marked by cardiopulmonary heterogeneity, ranging from mild ILD to development of severe ILD in 18%, and PH development in 12%. These data indicate that cardiopulmonary risk stratification early in the disease course is particularly important in RNAP-positive SSc.