Tertiary succesion of the Los Pozuelos creek (Vinchina Basin): Its stratigraphic and paleogeographic importance for the Andean foreland

Se presenta el perfil de la espesa sucesión terciaria aflorante en la quebrada de Los Pozuelos, norte de la cuenca de Vinchina (La Rioja). Se identificaron ocho secciones estratigráficas (SE) que abarcan a la Formación Vallecito (SE1, eólico y SE2, interacción eólica-fluvial), los miembros inferior (SE3, sistemas fluviales arenosos efímeros y SE4, ríos entrelazados a anastomosados) y superior de la Formación Vinchina (SE5 y SE6, ríos entrelazados areno-gravosos amalgamados a sistemas fluviales con mayor sinuosidad y planicies) y el miembro inferior de la Formación Toro Negro (SE7, planicie entrelazada gravo-arenosa confinada y SE8, ríos anastomosados areno-gravosos con incremento en depósitos finos). La presencia de la Formación Vallecito, permite establecer la base de la Formación Vinchina e indica un cambio significativo en la evolución de la cuenca de antepaís andina. Los depósitos de las SE3 y SE4 (retroarco transpresivo temprano) presentan continuidad y relativa homogeneidad a lo largo de toda la cuenca de antepaís mientras que las SE5 y SE6 (retroarco transpresivo tardío) no, ya que los bloques de basamento han particionado el retroarco en depocentros aislados (antepaís fracturado). Las SE7 y SE8 (antepaís transpresivo) evidencian la compleja interacción entre la faja corrida y los bloques de basamentos. Los cambios de facies como la disminución en el tamaño de grano de norte-sur a partir del miembro superior de la Formación Vinchina, con respecto al perfil de La Troya, permite inferir que la Sierra de Toro Negro actuó como un alto topográfico para la cuenca desde el Mioceno temprano.The description and interpretation of a thick Tertiary sedimentary succession cropping out along the Los Pozuelos creek, northern part of the Vinchina basin is presented here. The sedimentary column was divided into eight stratigraphic sections (SE), including the Vallecito Formation (SE1, aeolian; SE2, fluvial-aeolian interaction), the lower member of the Vinchina Formation (SE3, ephemeral sandy fluvial systems; SE4, braided to anastomosed fluvial systems), the upper member of the Vinchina Formation (SE5 and SE6, amalgamated sandy-gravel braided and high sinuosity fluvial systems) and the lower member of the Toro Negro Formation (SE7, confined gravelly to sandy braid plain; SE8, gravelly to sandy anastomosing fluvial systems). The unconformity between the Vallecito and Vinchina formations represents a major change in the evolution of the Andean foreland basin. SE3 and SE4 deposits (early transpressive retroarc stage) are continuous and homogeneous along strike, while SE5 and SE6 deposits (late transpressive retroarc stage) are not; indicating that uplifted basement blocks partitioned the foreland into isolated depocenters (broken-foreland basin). Rocks belonging to SE7 and SE8 show the complex relationship between the fold and thrust belt and the basement blocks. Facies changes and decreasing grain-size in a North to South direction recorded in the upper member of the Vinchina Formation when comparing the northern exposures (Los Pozuelos creek) and the central section along the La Troya River indicate that the Toro Negro Range acted as a local positive element since the early Miocene.Fil: Ciccioli, Patricia Lucia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Basicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Basicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Gómez O Connell, Mariana. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Geología; ArgentinaFil: Limarino, Carlos Oscar. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Basicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Basicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Marenssi, Sergio Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Basicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Basicas, Aplicadas y Ambientales de Buenos Aires; Argentin

The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment

The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) has been in operation since July 2014. This paper describes the second data release from this phase, and the fourteenth from SDSS overall (making this, Data Release Fourteen or DR14). This release makes public data taken by SDSS-IV in its first two years of operation (July 2014-2016). Like all previous SDSS releases, DR14 is cumulative, including the most recent reductions and calibrations of all data taken by SDSS since the first phase began operations in 2000. New in DR14 is the first public release of data from the extended Baryon Oscillation Spectroscopic Survey (eBOSS); the first data from the second phase of the Apache Point Observatory (APO) Galactic Evolution Experiment (APOGEE-2), including stellar parameter estimates from an innovative data driven machine learning algorithm known as "The Cannon"; and almost twice as many data cubes from the Mapping Nearby Galaxies at APO (MaNGA) survey as were in the previous release (N = 2812 in total). This paper describes the location and format of the publicly available data from SDSS-IV surveys. We provide references to the important technical papers describing how these data have been taken (both targeting and observation details) and processed for scientific use. The SDSS website (www.sdss.org) has been updated for this release, and provides links to data downloads, as well as tutorials and examples of data use. SDSS-IV is planning to continue to collect astronomical data until 2020, and will be followed by SDSS-V.Comment: SDSS-IV collaboration alphabetical author data release paper. DR14 happened on 31st July 2017. 19 pages, 5 figures. Accepted by ApJS on 28th Nov 2017 (this is the "post-print" and "post-proofs" version; minor corrections only from v1, and most of errors found in proofs corrected