Designing Efficient Subsidy Policies in a Regional Economy: A Multicriteria Decision-Making (MCDM)-Computable General Equilibrium (CGE) Approach

Since policy-makers usually pursue several conflicting objectives, policy-making can be understood as a multicriteria decision problem. Following the methodological proposal by André and Cardenete (2005) André, F. J. and Cardenete, M. A. 2005. Multicriteria Policy Making. Defining Efficient Policies in a General Equilibrium Model, Seville: Centro de Estudios Andaluces. Working Paper No. E2005/04, multi-objective programming is used in connection with a computable general equilibrium model to represent optimal policy-making and to obtain so-called efficient policies in an application to a regional economy (Andalusia, Spain). This approach is applied to the design of subsidy policies under two different scenarios. In the first scenario, it is assumed that the government is concerned just about two objectives: ensuring the profitability of a key strategic sector and increasing overall output. Finally, the scope of the exercise is enlarged by solving a problem with seven policy objectives, including both general and sectorial objectives. It is concluded that the observed policy could have been Pareto-improved in several directions.

Coaliciones promotoras y transparencia en México: el caso de las políticas de derecho de acceso a la información en la administración pública federal 2002-2014

Mexico is now one of the countries with better policies on transparency and access to public information, according to various indicators and academics. Just fifteen years ago, Mexico was a country that lacked legal instruments thereon, whereby the institutions were deeply opaque and citizens could not exercise this right of access to public information. The development of the right of access to public information, in both law and public policy, a milestone in the history of Mexico. It has been, therefore gestation, as its formulation and implementation. In Mexico there have existed diverse social movements that have promoted democratization and the defense of human rights. In the framework of these movements the fight registers for the right of access to the public information that one presents as a successful model of civic action and government intervention, without for it, not to know the challenges that his deepening has still and take root both in the company and in the political class in general. How was it achieved to construct a new institutional of transparency that was functional? How was it possible that the above mentioned change was achieved? These are questions that interests formulated to the political science and to the public administration for the analysis of the change and improvement of institutions. The study of the political change is relevant since the public policies precisely try to solve a problem, to transform a reality but not always the change is achieved, is not even realized of successful form. In a nascent democratic regime, it turns out important to know what factors can collaborate in the conformation of a public successful sustainable politics in the time. Even more, on having treated itself about a substantive politics that it gives content and viability itself to the democracy in a marked country historically and culturally for the opaqueness and the corruption...

Large-scale clustering measurements with photometric redshifts: comparing the dark matter haloes of X-ray AGN, star-forming and passive galaxies at z ≈ 1

We combine multi-wavelength data in the AEGIS-XD and C-COSMOS surveys to measure the typical dark matter halo mass of X-ray selected active galactic nuclei (AGN) [L_X(2–10 keV) > 10^42 erg s^− 1] in comparison with far-infrared selected star-forming galaxies detected in the Herschel/PEP survey (PACS Evolutionary Probe; L_IR > 10^11 L_⊙) and quiescent systems at z ≈ 1. We develop a novel method to measure the clustering of extragalactic populations that uses photometric redshift probability distribution functions in addition to any spectroscopy. This is advantageous in that all sources in the sample are used in the clustering analysis, not just the subset with secure spectroscopy. The method works best for large samples. The loss of accuracy because of the lack of spectroscopy is balanced by increasing the number of sources used to measure the clustering. We find that X-ray AGN, far-infrared selected star-forming galaxies and passive systems in the redshift interval 0.6 < z < 1.4 are found in haloes of similar mass, log M_DMH/(M_⊙ h^−1) ≈ 13.0. We argue that this is because the galaxies in all three samples (AGN, star-forming, passive) have similar stellar mass distributions, approximated by the J-band luminosity. Therefore, all galaxies that can potentially host X-ray AGN, because they have stellar masses in the appropriate range, live in dark matter haloes of log M_DMH/(M_⊙ h^−1) ≈ 13.0 independent of their star formation rates. This suggests that the stellar mass of X-ray AGN hosts is driving the observed clustering properties of this population. We also speculate that trends between AGN properties (e.g. luminosity, level of obscuration) and large-scale environment may be related to differences in the stellar mass of the host galaxies.