Aproximación a los factores diferenciales de los centros y zonas comerciales de Santa Cruz de Tenerife

Esta investigación es una aproximación realizada en el periodo mayo – junio del 2022 y que se centra en la características y factores que determinan el atractivo de los centros y zonas comerciales de Santa Cruz de Tenerife, en concreto, analizando el Centro Comercial Meridiano frente a la Zona Comercial Centro. Utilizando datos de estudios previamente realizados y publicados, que se emplearon para llevar a cabo una comparativa con el estudio desarrollado a continuación, además de una encuesta realizada por el propio equipo de investigación, se analiza cuáles son las características determinantes, desde el punto de vista de los consumidores tinerfeños, del atractivo de los distintos factores comerciales. Entre los resultados obtenidos, se observó que la existencia de un aparcamiento en el Centro Comercial Meridiano tiene un peso importante a la hora de determinar el flujo de personas que acude a dicha distribución comercial y su grado de atractivo, además de haberse analizado las posibles mejoras de cada una de las distribuciones comerciales.This research is an approximation carried out in the period of May – June 2022 and it focuses on the characteristics and factors that determine the attractiveness of shopping centers and commercial areas in Santa Cruz de Tenerife, specifically, analyzing Meridiano Shopping Center compared to the Center Zone shopping area. Using data from previously carried out and published studies, that were used to create a comparison with the study developed below, in addition to a survey carried out by the research team itself, the determining characteristics are analyzed, from the point of view of Tenerife´s consumers, of the attractiveness of the different commercial factors. Among the results obtained, it was observed that the existence of a car park in the Meridiano Shopping Center is very important when determining the flow of people who go to said commercial distribution and its level of attractiveness, in addition to having analyzed the possible improvements of each of the commercial distributions

The tenth data release of the Sloan Digital Sky Survey : first spectroscopic data from the SDSS-III Apachhe Point Observatory galactic evolution experiment

The Sloan Digital Sky Survey (SDSS) has been in operation since 2000 April. This paper presents the Tenth Public Data Release (DR10) from its current incarnation, SDSS-III. This data release includes the first spectroscopic data from the Apache Point Observatory Galaxy Evolution Experiment (APOGEE), along with spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS) taken through 2012 July. The APOGEE instrument is a near-infrared R ∼ 22,500 300 fiber spectrograph covering 1.514–1.696μm. The APOGEE survey is studying the chemical abundances and radial velocities of roughly 100,000 red giant star candidates in the bulge, bar, disk, and halo of the MilkyWay. DR10 includes 178,397 spectra of 57,454 stars, each typically observed three or more times, from APOGEE. Derived quantities from these spectra (radial velocities, effective temperatures, surface gravities, and metallicities) are also included. DR10 also roughly doubles the number of BOSS spectra over those included in the Ninth Data Release. DR10 includes a total of 1,507,954 BOSS spectra comprising 927,844 galaxy spectra, 182,009 quasar spectra, and 159,327 stellar spectra selected over 6373.2 deg2

The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment

The Sloan Digital Sky Survey (SDSS) has been in operation since 2000 April. This paper presents the Tenth Public Data Release (DR10) from its current incarnation, SDSS-III. This data release includes the first spectroscopic data from the Apache Point Observatory Galaxy Evolution Experiment (APOGEE), along with spectroscopic data from the Baryon Oscillation Spectroscopic Survey (BOSS) taken through 2012 July. The APOGEE instrument is a near-infrared R similar to 22,500 300 fiber spectrograph covering 1.514-1.696 mu m. The APOGEE survey is studying the chemical abundances and radial velocities of roughly 100,000 red giant star candidates in the bulge, bar, disk, and halo of the Milky Way. DR10 includes 178,397 spectra of 57,454 stars, each typically observed three or more times, from APOGEE. Derived quantities from these spectra (radial velocities, effective temperatures, surface gravities, and metallicities) are also included. DR10 also roughly doubles the number of BOSS spectra over those included in the Ninth Data Release. DR10 includes a total of 1,507,954 BOSS spectra comprising 927,844 galaxy spectra, 182,009 quasar spectra, and 159,327 stellar spectra selected over 6373.2 deg(-2)