SDSS-IV MaNGA: drivers of stellar metallicity in nearby galaxies

The distribution of stellar metallicities within and across galaxies is an excellent relic of the chemical evolution across cosmic time. We present a detailed analysis of spatially resolved stellar populations based on >2.6 million spatial bins from 7439 nearby galaxies in the Sloan Digital Sky Survey-IV (SDSS-IV) Mapping Nearby Galaxies at APO (MaNGA) survey. To account for accurate inclination corrections, we derive an equation for morphology-dependent determination of galaxy inclinations. Our study goes beyond the well-known global mass-metallicity relation and radial metallicity gradients by providing a statistically sound exploration of local relations between stellar metallicity [Z/H], stellar surface mass density Σ∗, and galactocentric distance in the global mass-morphology plane. We find a significant resolved mass density-metallicity relation Σ ZR for galaxies of all types and masses above 109.8 M⊙. Different radial distances make an important contribution to the spread of the relation. Particularly, in low- and intermediate-mass galaxies, we find that at fixed Σ∗ metallicity increases with radius independently of morphology. For high masses, this radial dependence is only observed in high Σ∗ regions of spiral galaxies. This result calls for a driver of metallicity, in addition to Σ∗ that promotes chemical enrichment in the outer parts of galaxies more strongly than in the inner parts. We discuss gas accretion, outflows, recycling, and radial migration as possible scenarios.The Science and Technology Facilities Council is acknowledged for support through the Consolidated Grant Cosmology and Astrophysics at Portsmouth, ST/S000550/1. JL is supported by the National Science Foundation under Grant No. 2009993. JKB-B acknowledges support from the grant IA-100420 (DGAPA-PAPIIT, UNAM), and funding from the CONACYT grants CF 19-39578, CB-285080, and FC-2016-01-1916

Floristic, ecological and ethnobotanical aspects of Mammillaria deherdtiana subsp. dodsonii (Cactaceae), an endemic and threatened plant

Antecedentes y Objetivos: En Oaxaca, México, se reportan 26 especies del género Mammillaria; siete de ellas endémicas. Mammillaria deherdtiana subsp. dodsonii está catalogada como amenazada. Los objetivos del trabajo fueron describir las características demográficas, reproductivas y aspectos etnobotánicos de su uso, así como los aspectos florísticos y bioclimáticos de las localidades estudiadas. Métodos: En enero de 2015 se encontraron dos localidades de Mammillaria deherdtiana subsp. dodsonii en la Sierra Norte. Entre enero y marzo se ubicaron cinco transectos de 5 m2 en una de ellas, en los cuales se registró el número de individuos, se establecieron categorías de tamaño y se obtuvo la estructura poblacional. Para la marcha floral se eligieron diez flores y cada dos horas se registró el diámetro de la apertura del perianto. Se registraron las especies de plantas vasculares que crecían cerca de ella y se obtuvieron datos de las variables climáticas. Se entrevistó a los pobladores para documentar el conocimiento y uso que le dan a esta cactácea.Resultados clave: La estructura poblacional es multimodal. Los individuos juveniles conforman 65% y los adultos reproductivos 33% en la localidad estudiada. La antesis dura siete horas; se observó dicogamia y hercogamia, lo cual indica un sistema de cruza xenógamo. La subespecie es reconocida con nombres en español y zapoteco y es usada de manera ocasional como alimento, medicina y ornamento. Se registraron 15 especies pertenecientes al bosque de Pinus y Abies. Las preferencias ambientales de la subespecie son temperaturas de 9.6-12.7 °C y precipitación de 1009-1405 mm.Conclusiones: El sistema de cruza xenógamo resulta preocupante por la observación de un solo visitante floral. La presencia de cerdas y espinas radiales sugiere adaptaciones morfofisiológicas de esta subespecie al frío. Se sugiere profundizar en la presencia y efectividad de los polinizadores y en la dinámica de reclutamiento de la subespecie.Background and Aims: In Oaxaca, Mexico, 26 species of the genus Mammillaria are reported, seven of them being endemic. Mammillaria deherdtiana subsp. dodsonii is listed as threatened. The objectives of this paper were to describe the demographic, reproductive and ethnobotanical aspects of its use, as well as the floristic and bioclimatic aspects of the studied localities.Methods: In January 2015, two localities of Mammillaria deherdtiana subsp. dodsonii were found in the Sierra Norte. Between January and March, five transects of 5 m2 were located in one of them, in which the number of individuals was recorded, size categories were established, and the population structure was obtained. For the flowering process, ten flowers were chosen, and the perianth diameter was recorded every two hours. The vascular plants surrounding the sampled site were recorded and data on climatic variables were obtained. The inhabitants were interviewed to document the local knowledge and uses of this cactus.Key results: The population structure is multimodal. Juvenile individuals make up 65% and reproductive adults 33% in the studied locality. Anthesis lasts seven hours; dichogamy and hercogamy were observed, indicating a xenogamous breeding system. The subspecies is recognized with names in Spanish and Zapotec and is occasionally used as food, medicine, and ornament. Fifteen species belonging to the Pinus and Abies forest were recorded. The environmental preferences of the subspecies are temperatures of 9.6-12.7 °C, and precipitation of 1009-1405 mm.Conclusions: The xenogamous breeding system is worrisome due to the observation of just one floral visitor. The presence of bristles and radial spines in this subspecies suggests morphophysiological adaptations to cold. It is advisable to delve into the presence and effectiveness of pollinators and the recruitment dynamics of the subspecies

Síntese e avaliação dos revestimentos base fluoreto utilizando fontes alternativas ao HF sobre a liga dos magnesio Elektron 21 para a fabricação de implantes ortopédicos biodegradáveis

Magnesium has been postulated as an excellent candidate for fabrication of biodegradable implants because of its degradability, biocompatibility and excellent mechanical properties comparable to bone’s those. Nevertheless, its high corrosion rate represents a great disadvantage, allowing the approach of modifying its electrochemical behaviour by the design of biodegradable coatings. In this regard, the most common synthesis route employed is chemical conversion in HF (up to 48%v) to produce biodegradable magnesium fluoride coatings. However, it is well known that HF is an extremely hazardous acid. Thus, one of the main targets is to find other alternative routes to avoid its use or, at least, to reduce its concentration. In the present investigation HF(4%v) -NaF and H3PO4-NaF solutions were evaluated as alternatives of the HF route to produce biodegradable coatings on the Elektron 21 magnesium alloy. Characterization of the conversion coatings was carried out by scanning electron microscopy and X-ray diffraction, whereas their corrosion resistance was evaluated by electrochemical and gravimetric measurements in Hank solution at 37°C. The results showed that the addition of NaF to the reactive solution promotes the formation of a double layer of MgF2-x(OH)x/NaMgF3. The presence of the NaMgF3 prevents the pitting corrosion attack of the coating/alloy system and leads a more uniform degradation mechanism. Particularly, the coating synthesized using H3PO4 1.6%v-NaF 0.5M solution exhibited an excellent electrochemical behaviour, better that obtained employing HF solutions so that, it might be proposed as excellent candidate to replace the HF in the synthesis of biodegradable coatings.Na atualidade, postularam-se ligas de magnésio como uma alternativa promissora na fabricação de implantes biodegradáveis por sua excelente degradabilidade, biocompatibilidade e propriedades mecânicas comparáveis às do osso. No entanto, sua elevada taxa de corrosão precisa a elaboração de revestimentos biodegradáveis, entre os quais destacam-se os sintetizados por conversão química em meio HF (até 48%v). Porém, a utilização deste ácido gera grandes problemas em termos de segurança, pois é altamente tóxico. Isso leva à necessidade de encontrar formas alternativas para substituir o ácido ou limitar sua utilização em pequenas quantidades. Neste trabalho foram avaliados misturas HF (4%v) -NaF e H3PO4-NaF como alternativas ao uso do HF na síntese de recobrimentos biodegradáveis na liga de magnésio Elektron 21. A caracterização microestrutural dos revestimentos foi realizada por microscopia eletrônica de varredura e difração de raios X, enquanto a resistência à corrosão foi avaliada por testes electroquímicos e gravimétricos em solução de Hank a 27°C. Os resultados mostraram que na presença de NaF, os recobrimentos sintetizados são constituídos de uma bicamada MgF2-x(OH)x/NaMgF3, onde a presença de NaMgF3 impede a corrosão localizada, causando que a degradação dos revestimentos seja uniforme e progressiva. Especialmente, os recobrimentos sintetizados sob a condição H3PO4 1,6%v-NaF 0,5M mostraram excelente desempenho, superiores aos obtidos com a utilização do HF, portanto são recomendados como excelentes candidatos para a substituição imediata desse ácido.En la actualidad se han postulado las aleaciones de magnesio como una alternativa prometedora en la fabricación de implantes biodegradables debido a su excelente degradabilidad, biocompatibilidad y propiedades mecánicas comparables a las del hueso; sin embargo, su elevada velocidad de corrosión hace necesario el diseño de recubrimientos biodegradables, entre los que se destaca aquellos sintetizados por conversión química en medio HF(hasta 48%v). No obstante, el empleo de este ácido genera grandes problemas en términos de seguridad, ya que es altamente tóxico. Surge entonces la necesidad de hallar vías alternativas que permitan sustituir dicho ácido o limitar su uso a cantidades reducidas. En el presente trabajo se evaluaron mezclas HF (4%v) -NaF y H3PO4-NaF como alternativas al empleo de HF en la síntesis de recubrimientos biodegradables sobre la aleación de magnesio Elektron 21. La caracterización microestructural de los recubrimientos se realizó mediante microscopía electrónica de barrido y difracción de rayos X, mientras que la resistencia a la corrosión se evaluó mediante ensayos electroquímicos y gravimétricos en solución Hank a 27°C. Los resultados mostraron que en presencia de NaF, los recubrimientos sintetizados están constituidos por una bicapa MgF2-x(OH)x/NaMgF3, donde la presencia de NaMgF3 evita el ataque localizado por picadura, haciendo que el proceso de degradación de los recubrimientos sea uniforme y progresivo. Particularmente, los recubrimientos sintetizados bajo la condición H3PO4 1,6%v-NaF 0,5M mostraron un excelente comportamiento, superior a los obtenidos con el empleo de HF, por lo que se postulan como excelentes candidatos para el reemplazo inmediato de este ácido

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

The data analysis pipeline for the SDSS-IV MaNGA IFU Galaxy Survey : overview

Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is acquiring integral-field spectroscopy for the largest sample of galaxies to date. By 2020, the MaNGA Survey - one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV) - will have observed a statistically representative sample of 104 galaxies in the local Universe z ∼99%) of analyzed spectra. We summarize assessments of the precision and accuracy of our measurements as a function of signal-to-noise, and provide specific guidance to users regarding the limitations of the data. The MaNGA DAP software is publicly available and we encourage community involvement in its development.PostprintPeer reviewe

The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years of operation (2014 July–2017 July). This is the third data release for SDSS-IV, and the 15th from SDSS (Data Release Fifteen; DR15). New data come from MaNGA—we release 4824 data cubes, as well as the first stellar spectra in the MaNGA Stellar Library (MaStar), the first set of survey-supported analysis products (e.g., stellar and gas kinematics, emission-line and other maps) from the MaNGA Data Analysis Pipeline, and a new data visualization and access tool we call "Marvin." The next data release, DR16, will include new data from both APOGEE-2 and eBOSS; those surveys release no new data here, but we document updates and corrections to their data processing pipelines. The release is cumulative; it also includes the most recent reductions and calibrations of all data taken by SDSS since first light. In this paper, we describe the location and format of the data and tools and cite technical references describing how it was obtained and processed. The SDSS website (www.sdss.org) has also been updated, providing links to data downloads, tutorials, and examples of data use. Although SDSS-IV will continue to collect astronomical data until 2020, and will be followed by SDSS-V (2020–2025), we end this paper by describing plans to ensure the sustainability of the SDSS data archive for many years beyond the collection of data

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 2014 July. This paper describes the second data release from this phase, and the 14th from SDSS overall (making this Data Release Fourteen or DR14). This release makes the data taken by SDSS-IV in its first two years of operation (2014–2016 July) public. 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; 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 the 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 web site (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

The 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point Observatory

The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) began observations in July 2014. It pursues three core programs: APOGEE-2,MaNGA, and eBOSS. In addition, eBOSS contains two major subprograms: TDSS and SPIDERS. This paper describes the first data release from SDSS-IV, Data Release 13 (DR13), which contains new data, reanalysis of existing data sets and, like all SDSS data releases, is inclusive of previously released data. DR13 makes publicly available 1390 spatially resolved integral field unit observations of nearby galaxies from MaNGA,the first data released from this survey. It includes new observations from eBOSS, completing SEQUELS. In addition to targeting galaxies and quasars, SEQUELS also targeted variability-selected objects from TDSS and X-ray selected objects from SPIDERS. DR13 includes new reductions ofthe SDSS-III BOSS data, improving the spectrophotometric calibration and redshift classification. DR13 releases new reductions of the APOGEE-1data from SDSS-III, with abundances of elements not previously included and improved stellar parameters for dwarf stars and cooler stars. For the SDSS imaging data, DR13 provides new, more robust and precise photometric calibrations. Several value-added catalogs are being released in tandem with DR13, in particular target catalogs relevant for eBOSS, TDSS, and SPIDERS, and an updated red-clump catalog for APOGEE.This paper describes the location and format of the data now publicly available, as well as providing references to the important technical papers that describe the targeting, observing, and data reduction. The SDSS website, http://www.sdss.org, provides links to the data, tutorials and examples of data access, and extensive documentation of the reduction and analysis procedures. DR13 is the first of a scheduled set that will contain new data and analyses from the planned ~6-year operations of SDSS-IV.PostprintPeer reviewe

Sloan Digital Sky Survey IV: mapping the Milky Way, nearby galaxies, and the distant universe

We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratios in the near-infrared. The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies (median ). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between and 3.5 to constrain cosmology using baryon acoustic oscillations, redshift space distortions, and the shape of the power spectrum. Within eBOSS, we are conducting two major subprograms: the SPectroscopic IDentification of eROSITA Sources (SPIDERS), investigating X-ray AGNs and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5 m Sloan Foundation Telescope at the Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5 m du Pont Telescope at Las Campanas Observatory, with observations beginning in early 2017. Observations at both facilities are scheduled to continue through 2020. In keeping with previous SDSS policy, SDSS-IV provides regularly scheduled public data releases; the first one, Data Release 13, was made available in 2016 July