"Corrective" Actions in the Public Sphere: How Perceptions of Media and Media Effects Shape Political Behaviors
In: International journal of public opinion research, Band 22, Heft 3, S. 343-363
ISSN: 1471-6909
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In: International journal of public opinion research, Band 22, Heft 3, S. 343-363
ISSN: 1471-6909
In: Colección universitaria
World Affairs Online
In: Relaciones Centroamérica-México
In: International journal of public opinion research, Band 26, Heft 2, S. 135-156
ISSN: 1471-6909
In: International journal of public opinion research, Band 8, Heft 2, S. 163-186
ISSN: 0954-2892
To determine whether an overestimation of media effects on others (ie, the third-person effect) influences one's willingness to restrict various types of communication, the relationship between perceived media effects & procensorship attitudes (regarding the media in general, violence on TV, & pornography) is examined. Analysis of survey responses (N = 133 students from a large midwestern university, unfamiliar with third-person effects theory) confirms that as the gap between perceived first- & third-person effects increases, individuals are more likely to manifest procensorship attitudes -- even when the data are controlled for a variety of potentially confounding demographic, media use, & attitudinal variables. 4 Tables, 49 References. Adapted from the source document.
En el presente escrito se rastrean las concepciones generales y las propuestas de reforma de los estados locales que influenciaron en las dinámicas de transformación llevadas adelante por las administraciones locales desde 1995 en adelante. El foco está puesto en la gestión de las políticas sociales en general y de la política de asistencia y promoción social en particular en las dos gestiones del intendente Miguel Lifchitz en el Municipio de Rosario entre 2003 y 2011. Estos dos gobiernos se analizan a partir de fuentes documentales y de entrevistas a funcionarios/ as y trabajadores/as del área de la asistencia y promoción social. ; In the present paper are crawled general conceptions and the reform proposals of the local states that influenced the dynamics of transformation carried out by local administrations from 1995 onwards. The focus is on the management of social policies and assistance and social promotion policy in particular during Miguel Lifchitz´s mandate in Rosario City Hall between 2003 and 2011. These two governments are analyzed based on documentary sources and interviews with public servants and workers from the area of assistance and social promotion. ; Fil: Garma, María Eugenia. Universidad Nacional de Rosario. Facultad de Ciencia Política y Relaciones Internacionales. Escuela de Trabajo Social; Argentina. ; Fil: Castro Rojas, Ignacio H. Universidad Nacional de Rosario. Facultad de Ciencia Política y Relaciones Internacionales. Escuela de Trabajo Social; Argentina.
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In: International journal of public opinion research, Band 8, Heft 2, S. 163-186
ISSN: 1471-6909
In: Journal of the International AIDS Society, Band 11, Heft Suppl 1, S. P252
ISSN: 1758-2652
The Transiting Exoplanet Survey Satellite, TESS, is currently carrying out an all-sky search for small planets transiting bright stars. In the first year of the TESS survey, a steady progress was made in achieving the mission's primary science goal of establishing bulk densities for 50 planets smaller than Neptune. During that year, the TESS's observations were focused on the southern ecliptic hemisphere, resulting in the discovery of three mini-Neptunes orbiting the star TOI-125, a V = 11.0 K0 dwarf. We present intensive HARPS radial velocity observations, yielding precise mass measurements for TOI-125b, TOI-125c, and TOI-125d. TOI-125b has an orbital period of 4.65 d, a radius of 2.726 ± 0.075 RE, a mass of 9.50 ± 0.88 ME, and is near the 2:1 mean motion resonance with TOI-125c at 9.15 d. TOI-125c has a similar radius of 2.759 ± 0.10 RE and a mass of 6.63 ± 0.99 ME, being the puffiest of the three planets. TOI-125d has an orbital period of 19.98 d and a radius of 2.93 ± 0.17 RE and mass 13.6 ± 1.2 ME. For TOI-125b and d, we find unusual high eccentricities of 0.19 ± 0.04 and 0.17^{+0.08}_{-0.06}, respectively. Our analysis also provides upper mass limits for the two low-SNR planet candidates in the system; for TOI-125.04 (RP = 1.36 RE, P = 0.53 d), we find a 2¿ upper mass limit of 1.6 ME, whereas TOI-125.05 (R_P=4.2^{+2.4}_{-1.4} RE, P = 13.28 d) is unlikely a viable planet candidate with an upper mass limit of 2.7 ME. We discuss the internal structure of the three confirmed planets, as well as dynamical stability and system architecture for this intriguing exoplanet system. ; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)
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