A census of ρ\rho Oph candidate members from Gaia DR2

The Ophiuchus cloud complex is one of the best laboratories to study the earlier stages of the stellar and protoplanetary disc evolution. The wealth of accurate astrometric measurements contained in the Gaia Data Release 2 can be used to update the census of Ophiuchus member candidates. We seek to find potential new members of Ophiuchus and identify those surrounded by a circumstellar disc. We constructed a control sample composed of 188 bona fide Ophiuchus members. Using this sample as a reference we applied three different density-based machine learning clustering algorithms (DBSCAN, OPTICS, and HDBSCAN) to a sample drawn from the Gaia catalogue centred on the Ophiuchus cloud. The clustering analysis was applied in the five astrometric dimensions defined by the three-dimensional Cartesian space and the proper motions in right ascension and declination. The three clustering algorithms systematically identify a similar set of candidate members in a main cluster with astrometric properties consistent with those of the control sample. The increased flexibility of the OPTICS and HDBSCAN algorithms enable these methods to identify a secondary cluster. We constructed a common sample containing 391 member candidates including 166 new objects, which have not yet been discussed in the literature. By combining the Gaia data with 2MASS and WISE photometry, we built the spectral energy distributions from 0.5 to 22\microm for a subset of 48 objects and found a total of 41 discs, including 11 Class II and 1 Class III new discs. Density-based clustering algorithms are a promising tool to identify candidate members of star forming regions in large astrometric databases. If confirmed, the candidate members discussed in this work would represent an increment of roughly 40% of the current census of Ophiuchus.Comment: A&A, Accepted. Abridged abstrac

Variabilidade isoenzimática e sistema de cruzamento de Parapiptadenia rigida em um pomar de sementes.

Por meio da aplicação da técnica de eletroforese de isoenzimas, foram estudados o sistema de cruzamento e a variabilidade genética presentes em um pomar de sementes de angico-gurucaia (Parapiptadenia rigida (Benth.) Brenan). Trinta famílias, com 20 indivíduos, foram amostradas do pomar formado para conservação genética ex situ e produção de sementes geneticamente superiores (pomar de sementes – PS), tendo outra amostra de mesmo tamanho sido obtida de pequenos fragmentos dispostos ao longo da margem brasileira do lago da represa de Itaipu (coleção regional – CR). A partir da interpretação genética de quatro locos polimórficos (Dia-1, Dia-3, 6Pgdh-2 e Sod-2), num total de 11 alelos, estimou-se em 94,8 % a taxa de cruzamento no PS. Os níveis de variação genética nas duas condições amostradas foram similares, com 2,08 e 1,93 alelos por loco polimórfico, 73,34 e 65% de locos polimórficos, valores de heterozigosidade observada (Ho) de 0,2596 e 0,2599 e de heterozigosidade esperada (He) de 0,2276 e 0,2150, para PS e CR, respectivamente. Além disto, não se encontrou diferença entre as estimativas determinadas pelo índice de diversidade de Shannon-Weaver (0,4242 e 0,4265, para PS e CR, respectivamente), com base nas freqüências fenotípicas de sete locos polimórficos (Adh, Dia-1, Dia-3, Est-1, Est-3, Sod-2 e 6Pgdh-2). A dispersão dos grãos de pólen em políades faz com que a maioria dos frutos formados (64%) possua sementes-irmãs completas, o que está diretamente associado à ocorrência de cruzamentos correlacionados na espécie. A formação do pomar de sementes foi potencialmente efetiva para conservação ex situ da variabilidade genética existente na espécie, na região amostrada, e favorável à recombinação gênica entre indivíduos não-aparentados.Tese (Mestrado em Ciência Florestal) - Universidade Federal de Viçosa, 1999

Response of sea bream to handling

Understanding how gilthead sea bream, Sparus aurata L., an important Mediterranean Sea species for aquaculture, respond physiologically to stressors commonly encountered in intensive rearing is important for eiective production, as managing for stress is a major factor in maintaining healthy ¢sh stocks. Our objective was to determine whether holding juvenile gilthead sea bream at a high density (HD), as a chronic stressor, would aiect their physiological responses to a subsequent acute handling stressor. After acclimation at a low density (LD) of 6k g m 3 in 200-L circular tanks containing 33^ 36 g L 1 recirculating seawater at 191C under a normal photoperiod, juvenile 37-g gilthead sea bream were con¢ned for 14 days at a HD of 26 kg m 3 an

Produção de plantas transgênicas de café resistentes ao herbicida glufosinato de amônio

Plantas transgênicas de Coffea canephora P. resistentes ao herbicida glufosinato de amônio foram regeneradas a partir de explantes foliares cocultivados com Agrobacterium tumefaciens EHA105 contendo o plasmídio pCAMBIA3301, que contém os genes bar e uidA ambos sob controle do promotor 35S ou pIBI3 (3300 contendo o gene da ACC oxidase, antisenso) ou ainda bombardeados com o plasmídio pCAMBIA3301. Embriogênese somática direta foi induzida no meio contendo ¼ dos macros e metade dos micronutrientes do meio MS, constituintes orgânicos do meio B5 e 30 g.L 1 de sacarose, suplementado com 5mM N 6 ? (2isopentenil) adenina (2iP) e 10 mM de glufosinato de amônio para seleção de embriões transgênicos putativos. A presença e a integração do gene bar foram confirmados pelas análises de PCR e Southern blot. As plantas transgênicas pulverizadas com 1600 mg.L 1 do herbicida Finale que contém glufosinato como ingrediente ativo, não apresentaram sintomas de toxidez, mantiveram a coloração e continuaram crescendo normalmente na aclimatação ex vitro

Consequências genéticas da regeneração natural de espécies arbóreas em área antrópica, AC, Brasil.

O cedro (Cedrela odorata L.) e o ipê-amarelo (Tabebuia serratifolia Nichols.) são espécies arbóreas tropicais economicamente valiosas e que têm sido ameaçadas pela exploração madeireira predatória e pela fragmentação florestal. Ambas apresentam dispersão anemocórica e regeneram naturalmente em áreas de pastagem. Esse estudo comparou, para as duas espécies, a diversidade genética de indivíduos estabelecidos em pastagem e em floresta. Trinta indivíduos de ipê-amarelo foram genotipados com cinco locos isoenzimáticos e 54 de cedro, com quatro locos microssatélites. A diversidade genética foi elevada nas duas subpopulações. Para ipê-amarelo, a diversidade genética foi maior na pastagem. Para cedro, observou-se perda de alelos na pastagem (Â = 11,75 alelos/loco) em comparação à floresta (Â = 14,50). Além disso, 31% dos alelos de cedro foram exclusivos da floresta. Não houve divergência genética entre as subpopulações de ipê-amarelo, porém, para cedro, houve divergência significativa, embora baixa (2,2%). Os resultados mostraram que, para as duas espécies, a subpopulação da pastagem não passou por um gargalo genético severo. A colonização de áreas antrópicas mostrou-se eficiente, mas há necessidade de fluxo gênico contínuo, por sucessivas gerações, entre as áreas para restabelecer (cedro) e manter (ipê) os níveis de diversidade genética observados na área de vegetação primária

The Best Brown Dwarf Yet?: A Companion to the Hyades Eclipsing Binary V471 Tau

We have carried out an analysis of about 160 eclipse timings spanning over 30 years of the Hyades eclipsing binary V471 Tauri that shows a long-term quasi-sinusoidal modulation of its observed eclipse arrival times. The O-Cs have been analyzed for the ``light-time'' effect that arises from the gravitational influence of a tertiary companion. The presence of a third body causes the relative distance of the eclipsing pair to the Earth to change as it orbits the barycenter of the triple system. The result of the analysis of the eclipse times yields a light-time semi-amplitude of 137.2+/-12.0 s, an orbital period of P_3 = 30.5+/-1.6 yr and an eccentricity of e_3 = 0.31+/-0.04. The mass of the tertiary component is M_3 sin i_3 = 0.0393+/-0.0038 Mo when a total mass of 1.61+/-0.06 Mo for V471 Tau is adopted. For orbital inclinations i_3 > 35 deg, the mass of the third body would be below the stable hydrogen burning limit of M = 0.07 Mo and it thus would be a brown dwarf. In the next several years (near maximum elongation), it should be feasible to obtain IR images and spectra of V471 Tau C that, when combined with the known mass, age, distance, and [Fe/H], will serve as a benchmark for understanding the physical properties and evolution of brown dwarfs.Comment: 9 pages, 3 figures, accepted for publication in ApJ Letter

Overview of methods used to evaluate the adequacy of nutrient intakes for individuals and populations

The objective of the present paper is to review the methods of measuring micronutrient intake adequacy for individuals and for populations in order to ascertain best practice. A systematic review was conducted to locate studies on the methodological aspects of measuring nutrient adequacy. The results showed that for individuals, qualitative methods (to find probability of adequacy) and quantitative methods (to find confidence of adequacy) have been proposed for micronutrients where there is enough data to set an average nutrient requirement (ANR). If micronutrients do not have ANR, an adequate intake (AI) is often defined and can be used to assess adequacy, provided the distribution of daily intake over a number of days is known. The probability of an individual's intake being excessive can also be compared with the upper level of safe intake and the confidence of this estimate determined in a similar way. At the population level, adequacy can be judged from the ANR using the probability approach or its short cut – the estimated average requirement cut-point method. If the micronutrient does not have an ANR, adequacy cannot be determined from the average intake and must be expressed differently. The upper level of safe intake can be used for populations in a similar way to that of individuals. All of the methodological studies reviewed were from the American continent and all used the methodology described in the Institute of Medicine publications. The present methodology should now be adapted for use in Europe

The Distance to the Large Magellanic Cloud from the Eclipsing Binary HV2274

The distance to the Large Magellanic Cloud (LMC) is crucial for the calibration of the Cosmic Distance Scale. We derive a distance to the LMC based on an analysis of ground-based photometry and HST-based spectroscopy and spectrophotometry of the LMC eclipsing binary system HV2274. Analysis of the optical light curve and HST/GHRS radial velocity curve provides the masses and radii of the binary components. Analysis of the HST/FOS UV/optical spectrophotometry provides the temperatures of the component stars and the interstellar extinction of the system. When combined, these data yield a distance to the binary system. After correcting for the location of HV2274 with respect to the center of the LMC, we find d(LMC) = 45.7 +/- 1.6 kpc or DM(LMC) = 18.30 +/- 0.07 mag. This result, which is immune to the metallicity-induced zero point uncertainties that have plagued other techniques, lends strong support to the ``short'' LMC distance scale as derived from a number of independent methods.Comment: 6 pages, including 2 pages of figures. Newly available optical (B and V) photometry has revealed -- and allowed the elimination of -- a systematic error in the previously reported determination of E(B-V) for HV2274. The new result is E(B-V) = 0.12 mag (as compared to the value of 0.083 reported in the original submission) and produces a DECREASE in the distance modulus of HV2274 by 0.12 mag. ApJ Letters, in pres

Progressive loss functions for speech enhancement with deep neural networks

The progressive paradigm is a promising strategy to optimize network performance for speech enhancement purposes. Recent works have shown different strategies to improve the accuracy of speech enhancement solutions based on this mechanism. This paper studies the progressive speech enhancement using convolutional and residual neural network architectures and explores two criteria for loss function optimization: weighted and uniform progressive. This work carries out the evaluation on simulated and real speech samples with reverberation and added noise using REVERB and VoiceHome datasets. Experimental results show a variety of achievements among the loss function optimization criteria and the network architectures. Results show that the progressive design strengthens the model and increases the robustness to distortions due to reverberation and noise

First detection of thermal radio jets in a sample of proto-brown dwarf candidates

We observed with the JVLA at 3.6 and 1.3 cm a sample of 11 proto-brown dwarf candidates in Taurus in a search for thermal radio jets driven by the most embedded brown dwarfs. We detected for the first time four thermal radio jets in proto-brown dwarf candidates. We compiled data from UKIDSS, 2MASS, Spitzer, WISE and Herschel to build the Spectral Energy Distribution (SED) of the objects in our sample, which are similar to typical Class~I SEDs of Young Stellar Objects (YSOs). The four proto-brown dwarf candidates driving thermal radio jets also roughly follow the well-known trend of centimeter luminosity against bolometric luminosity determined for YSOs, assuming they belong to Taurus, although they present some excess of radio emission compared to the known relation for YSOs. Nonetheless, we are able to reproduce the flux densities of the radio jets modeling the centimeter emission of the thermal radio jets using the same type of models applied to YSOs, but with corresponding smaller stellar wind velocities and mass-loss rates, and exploring different possible geometries of the wind or outflow from the star. Moreover, we also find that the modeled mass outflow rates for the bolometric luminosities of our objects agree reasonably well with the trends found between the mass outflow rates and bolometric luminosities of YSOs, which indicates that, despite the "excess" centimeter emission, the intrinsic properties of proto-brown dwarfs are consistent with a continuation of those of very low mass stars to a lower mass range. Overall, our study favors the formation of brown dwarfs as a scaled-down version of low-mass stars.Comment: 18 pages, 8 figures, 14 tables, accepted by the Astrophysical Journa