MgII Line Variability of High Luminosity Quasars

We monitored five high-luminosity quasars with lambda L_{3000A} > 10^45 erg s^-1 at 0.4 < z < 0.6 to measure flux variability of the MgII 2798 line and explore feasibility of reverberation mapping using MgII. Over the two year monitoring program, imaging data were obtained with the A Noble Double-Imaging Camera on the 1.3-m telescope at the Cerro Tololo Inter-American Observatory (CTIO), while spectroscopic data were obtained at the same night with the R-C spectrograph on the 1.5-m telescope at the CTIO. By performing differencial photometry using available field stars in each quasar image, we measured variability -- 10%-24% peak-to-peak changes and 3%-8% rms variations -- in the B band, which includes flux changes in the rest-frame UV continuum (~2500A -- ~3600A) as well as the MgII line. Utilizing photometric measurements for spectroscopic flux calibration, we measured the MgII line flux and the continuum flux at 3000\AA from each single-epoch spectrum. Four objects showed MgII line flux variability with 23%-50% peak-to-peak changes and 8%-17% rms variations over 1-1.5 year rest-frame time scales, while one object showed no MgII flux variability within the measurement error (<5%). We also detected 4%-15% rms variations of the MgII line width for all five objects. With synchronous observations for photometry and spectroscopy, we demonstrated the feasibility of the MgII line reverberation mapping for high-luminosity quasars at intermediate redshift.Comment: AJ in press, 8 pages, 8 figures edited versio

Theoretical calculations for precision polarimetry based on Mott scattering

Electron polarimeters based on Mott scattering are extensively used in different fields in physics such as atomic, nuclear or particle physics. This is because spin-dependent measurements gives additional information on the physical processes under study. The main quantity that needs to be understood in very much detail, both experimentally and theoretically, is the spin-polarization function, so called analyzing power or Sherman function. A detailed theoretical analysis on all the contributions to the effective interaction potential that are relevant at the typical electron beam energies and angles commonly used in the calibration of the experimental apparatus is presented. The main contribution leading the theoretical error on the Sherman function is found to correspond to radiative corrections that have been qualitatively estimated to be below the 0.5% for the considered kinematical conditions: unpolarized electron beams of few MeV elastically scattered from a gold and silver targets at backward angles.Comment: Accepted versio

La huella griega en el Senado de los EE.UU.

Se estudian los referentes griegos que pueden rastrearse en la articulación de la cámara alta del poder legislativo de Estados Unidos. El número de representantes, el criterio de selección de los delegados, las competencias otorgadas al órgano senatorial y el salario estipulado permiten comprobar una profunda y deliberada selección de modelos procedentes del escenario político griegoUniversidad de Málaga. Campus de Excelencia Internacional Andalucía Tech

Impact of the symmetry energy on the outer crust of non-accreting neutron stars

The composition and equation of state of the outer crust of non-accreting neutron stars is computed using accurate nuclear mass tables. The main goal of the present study is to understand the impact of the symmetry energy on the structure of the outer crust. First, a simple "toy model" is developed to illustrate the competition between the electronic density and the symmetry energy. Then, realistic mass tables are used to show that models with a stiff symmetry energy - those that generate large neutron skins for heavy nuclei - predict a sequence of nuclei that are more neutron-rich than their softer counterparts. This result may be phrased in the form of a correlation: the larger the neutron skin of 208Pb, the more exotic the composition of the outer crust.Comment: 21 pages, 8 figures, submitted to Physical Review

An Incremental Algorithm for Computing Cylindrical Algebraic Decompositions

In this paper, we propose an incremental algorithm for computing cylindrical algebraic decompositions. The algorithm consists of two parts: computing a complex cylindrical tree and refining this complex tree into a cylindrical tree in real space. The incrementality comes from the first part of the algorithm, where a complex cylindrical tree is constructed by refining a previous complex cylindrical tree with a polynomial constraint. We have implemented our algorithm in Maple. The experimentation shows that the proposed algorithm outperforms existing ones for many examples taken from the literature

COMMON PROPERTY UNDER MANAGEMENT FLEXIBILITY: VALUATION, OPTIMAL EXPLOITATION, AND REGULATION

Evidence shows that fisheries need close and careful attention because it has been observed that common property fisheries might be blamed for at least two sources of inefficiency. On one hand, resource overexploitation; on the other, the "static" or "passive" management applies, as outlined in the traditional fisheries literature. This paper presents a fishery model that embraces a combination of regulatory measures, an ITQ system, and a property tax rate under management flexibility. The model allows for a common property fishery to be exploited with full economic efficiency and flexibility in contrast to the mismanagement described in the traditional literature.Resource /Energy Economics and Policy,