Determinação fotométrica do ácido ascórbico

The photometric determination of ascorbic acid with the "E. E. L. portable colorimeter" can be carried" out rapid and conveniently using either 3% HPO3 or 0,4% (COOH) 2 as protective agent. The standards would contain from 2 to 20 micrograms of ascorbic acid per ml of metaphosphoric or oxalic acid solutions. We mix 10 ml of these solutions with 3 ml of the adequate citrate buffer solutions, and we pipet 5 ml of the resulting mixture to a matched test tube containing 5 ml of sodium - 2,6 - dichlorobenzenoneindophenol (80 mg per liter); then we shake well and after 15 seconds the extintion is read using green filter. The readings are subtracted from the blank one. Designating the differences by x and the concentrations of ascorbic acid/ml in the standards by y, we get, with the acid of the method of least squares, the following regression equations: for the metaphosphoric acid Y = 0,543x + 0,629 for the oxalic acid Y = 0,516x + 0,422, which permit, by interpolating, the determination of the ascorbic acid content in plant materials.

Towards Detecting Changes in Underwater Image Sequences

Detecting changes between images of the same scene taken at different times is of great interest for monitoring and understanding the environment. It is widely used for on-land application but suffers from different constraints. Unfortunately, Change detection algorithms require highly accurate geometric and photometric registration. This requirement has precluded their use in underwater imagery in the past. In this paper, the change detection techniques available nowadays for on-land application were analyzed and a method to automatically detect the changes in sequences of underwater images is proposed. Target application scenarios are habitat restoration sites, or area monitoring after sudden impacts from hurricanes or ship groundings. The method is based on the creation of a 3D terrain model from one image sequence over an area of interest. This model allows for synthesizing textured views that correspond to the same viewpoints of a second image sequence. The generated views are photometrically matched and corrected against the corresponding frames from the second sequence. Standard change detection techniques are then applied to find areas of difference. Additionally, the paper shows that it is possible to detect false positives, resulting from non-rigid objects, by applying the same change detection method to the first sequence exclusively. The developed method was able to correctly find the changes between two challenging sequences of images from a coral reef taken one year apart and acquired with two different cameras

Physiopathologie du coeur embryonnaire soumis à l'anoxie-réoxygénation: rôle protecteur du NO et des canaux KATP

RESUME Introduction : Dans le coeur adulte, l'ischémie et la reperfusion entraînent des perturbations électriques, mécaniques, biochimiques et structurales qui peuvent causer des dommages réversibles ou irréversibles selon la sévérité de l'ischémie. Malgré les récents progrès en cardiologie et en chirurgie foetales, la connaissance des mécanismes impliqués dans la réponse du myocarde embryonnaire à un stress hypoxique transitoire demeure lacunaire. Le but de ce travail a donc été de caractériser les effets chrono-, dromo- et inotropes de l'anoxie et de la réoxygénation sur un modèle de coeur embryonnaire isolé. D'autre part, les effets du monoxyde d'azote (NO) et de la modulation des canaux KATP mitochondriaux (mito KATP) sur la récupération fonctionnelle postanoxique ont été étudiés. La production myocardique de radicaux d'oxygène (ROS) et l'activité de MAP Kinases (ERK et JNK) impliquées dans la signalisation cellulaire ont également été déterminées. Méthodes : Des coeurs d'embryons de poulet âgés de 4 jours battant spontanément ont été placés dans une chambre de culture puis soumis à une anoxie de 30 min suivie d'une réoxygénation de 60 min. L'activité électrique (ECG), les contractions de l'oreillette, du ventricule et du conotroncus (détectées par photométrie), la production de ROS (mesure de la fluorescence du DCFH) et l'activité kinase de ERK et JNK dans le ventricule ont été déterminées au cours de l'anoxie et de la réoxygénation. Les coeurs ont été traités avec un bloqueur des NO synthases (L-NAME), un donneur de NO (DETA-NONOate), un activateur (diazoxide) ou un inhibiteur (5-HD) des canaux mitoKATP un inhibiteur non-spécifique des PKC (chélérythrine) ou un piégeur de ROS (MPG). Résultats : L'anoxie et la réoxygénation entraînaient des arythmies (essentiellement d'origine auriculaire) semblables à celles observées chez l'adulte, des troubles de la conduction (blocs auriculo-ventriculaires de 1er, 2ème et 3ème degré) et un ralentissement marqué du couplage excitation-contraction (E-C) ventriculaire. En plus de ces arythmies, la réoxygénation déclenchait le phénomène de Wenckelbach, de rares échappements ventriculaires et une sidération myocardique. Aucune fibrillation, conduction rétrograde ou activité ectopique n'ont été observées. Le NO exogène améliorait la récupération postanoxique du couplage E-C ventriculaire alors que L'inhibition des NOS la ralentissait. L'activation des canaux mito KATP augmentait la production mitochondriale de ROS à la réoxygénation et accélérait la récupération de la conduction (intervalle PR) et du couplage E-C ventriculaire. La protection de ce couplage était abolie par le MPG, la chélérythrine ou le L-NAME. Les fonctions électrique et contractile de tous les coeurs récupéraient après 30-40 min de réoxygénation. L'activité de ERK et de JNK n'était pas modifiée par L'anoxie, mais doublait et quadruplait, respectivement, après 30 min de réoxygénation. Seule l'activité de JNK était diminuée (-60%) par l'activation des canaux mitoKATP. Cet effet inhibiteur était partiellement abolit par le 5-HD. Conclusion: Dans le coeur immature, le couplage E-C ventriculaire semble être un paramètre particulièrement sensible aux conditions d'oxygénation. Sa récupération postanoxique est améliorée par l'ouverture des canaux mitoKATP via une signalisation impliquant les ROS Ies PKC et le NO. Une réduction de l'activité de JNK semble également participer à cette protection. Nos résultats suggèrent que les mitochondries jouent un rôle central dans la modulation des voies de signalisation cellulaire, en particulier lorsque les conditions métaboliques deviennent défavorables. Le coeur embryonnaire isolé représente donc un modèle expérimental utile pour mieux comprendre les mécanismes associés à une hypoxie in utero et pour améliorer les stratégies thérapeutiques en cardiologie et chirurgie foetales. ABSTRACT Physiopathology of the anoxic-reoxygenated embryonic heart: Protective role of NO and KATP channel Aim: In the adult heart, the electrical, mechanical, biochemical and structural disturbances induced by ischemia and reperfusion lead to reversible or irreversible damages depending on the severity and duration of ischemia. In spite of recent advances in fetal cardiology and surgery, little is known regarding the cellular mechanisms involved in hypoxia-induced dysfunction in the developing heart. The aim of this study was to precisely characterize the chrono-, dromo- and inotropic disturbances associated with anoxia-reoxygenation in an embryonic heart model. Furthermore, the roles that nitric oxide (NO), reactive oxygen species (ROS), mitochondrial KATP, (mito KATP) channel and MAP Kinases could play in the stressed developing heart have been investigated. Methods: Embryonic chick hearts (4-day-old) were isolated and submitted in vitro to 30 min anoxia followed by 60 min reoxygenation. Electrical (ECG) and contractile activities of atria, ventricle and conotruncus (photometric detection), ROS production (DCFH fluorescence) and ERK and JNK activity were determined in the ventricle throughout anoxia-reoxygenation. Hearts were treated with NO synthase inhibitor (L-NAME), NO donor (DETA-NONOate), mitoKATP channel opener (diazoxide) or blocket (5-HD), PKC inhibitor (chelerythrine) and ROS scavenger (MPG). Results: Anoxia and reoxygenation provoked arrhythxnias (mainly originating from atrial region), troubles of conduction (st, 2nd, and 3rd degree atrio-ventricular blocks) and disturbances of excitation-contraction (E-C) coupling. In addition to these types of arrhythmias, reoxygenation triggered Wenckebach phenomenon and rare ventricular escape beats. No fibrillations, no ventricular ectopic beats and no electromechanical dissociation were observed. Myocardial stunning was observed during the first 30 min of reoxygenation. All hearts fully recovered their electrical and mechanical functions after 30-40 min of reoxygenation. Exogenous NO improved while NOS inhibition delayed E-C coupling recovery. Mito KATP, channel opening increased reoxygenation-induced ROS production and improved E-C coupling and conduction (PR) recovery. MPG, chelerythrine or L-NAME reversed this effect. Reoxygenation increased ERK and JNK activities land 4-fold, respectively, while anoxia had no effect. MitoKATP channel opening abolished the reoxygenation-induced activation of JNK but had no effect on ERK activity. This inhibitory effect was partly reversed by mitoKATP channel blocker but not by MPG. Conclusion: In the developing heart, ventricular E-C coupling was found to be specially sensitive to hypoxia-reoxygenation and its postanoxic recovery was improved by mitoKATP channel activation via a ROS-, PKC- and NO-dependent pathway. JNK inhibition appears to be involved in this protection. Thus, mitochondria can play a pivotal role in the cellular signalling pathways, notably under critical metabolic conditions. The model of isolated embryonic heart appears to be useful to better understand the mechanisms underlying the myocardial dysfunction induced by an in utero hypoxia and to improve therapeutic strategies in fetal cardiology and surgery.

The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy

Observations of the extraordinarily bright optical afterglow (OA) of GRB 991208 started 2.1 d after the event. The flux decay constant of the OA in the R-band is -2.30 +/- 0.07 up to 5 d, which is very likely due to the jet effect, and after that it is followed by a much steeper decay with constant -3.2 +/- 0.2, the fastest one ever seen in a GRB OA. A negative detection in several all-sky films taken simultaneously to the event implies either a previous additional break prior to 2 d after the occurrence of the GRB (as expected from the jet effect). The existence of a second break might indicate a steepening in the electron spectrum or the superposition of two events. Once the afterglow emission vanished, contribution of a bright underlying SN is found, but the light curve is not sufficiently well sampled to rule out a dust echo explanation. Our determination of z = 0.706 indicates that GRB 991208 is at 3.7 Gpc, implying an isotropic energy release of 1.15 x 10E53 erg which may be relaxed by beaming by a factor > 100. Precise astrometry indicates that the GRB coincides within 0.2' with the host galaxy, thus given support to a massive star origin. The absolute magnitude is M_B = -18.2, well below the knee of the galaxy luminosity function and we derive a star-forming rate of 11.5 +/- 7.1 Mo/yr. The quasi-simultaneous broad-band photometric spectral energy distribution of the afterglow is determined 3.5 day after the burst (Dec 12.0) implying a cooling frequency below the optical band, i.e. supporting a jet model with p = -2.30 as the index of the power-law electron distribution.

UBVRI-CCD photometry of Cepheus OB3 association

Johnson CCD photometry was performed in the two subgroups of the association Cepheus OB3, for selected fields each containing at least one star with previous UBV photoelectric photometry. Photometry for about 1000 stars down to visual magnitude 21 is provided, although the completeness tests show that the sample is complete down to V=19mag. Individual errors were assigned to the magnitude and colours for each star. Colour-colour and colour-magnitude diagrams are shown. Astrometric positions of the stars are also given. Description of the reduction procedure is fully detailed.

An analysis of the currently available calibrations inStromgren photometry by using open clusters

In recent years, several authors have revised the calibrations used to compute physical parameters (tex2html_wrap_inline498, tex2html_wrap_inline500, log g, [Fe/H]) from intrinsic colours in the tex2html_wrap_inline504 photometric system. For reddened stars, these intrinsic colours can be computed through the standard relations among colour indices for each of the regions defined by Strömgren (1966) on the HR diagram. We present a discussion of the coherence of these calibrations for main-sequence stars. Stars from open clusters are used to carry out this analysis. Assuming that individual reddening values and distances should be similar for all the members of a given open cluster, systematic differences among the calibrations used in each of the photometric regions might arise when comparing mean reddening values and distances for the members of each region. To classify the stars into Strömgren's regions we extended the algorithm presented by Figueras et al. (1991) to a wider range of spectral types and luminosity classes. The observational ZAMS are compared with the theoretical ZAMS from stellar evolutionary models, in the range tex2html_wrap_inline506 K. The discrepancies are also discussed.

Secondary UBVRI-CCD standard stars in the neighbourhood of Landolt standard stars

A list of 681 UBVRI secondary standard stars for CCD photometry is presented. Visual magnitude ranges from 9.7 to 19.4, and the B-V colour index varies from 1.15 to 1.97. The stars are grouped into 11 different fields, each of them is generally observable in a single CCD frame. The stars are located near Landolt UBVRI equatorial standards, accessible to telescopes in both hemispheres, and mainly within the 5 - 8 hours range of right ascension. Photometry, equatorial coordinates and finding charts are provided.

UBVRI photoelectric photometry of nearby stars

In order to complete the photometric data of the Gliese (1969) 'Catalog of Nearby Stars', and in addition use these data for the Hipparcos space astrometry mission, program stars have been selected from the catalog and its supplements on the basis of their having an incomplete set of UBVRI photometric data of magnitude lower than 13. The program developed rejects determinations of any magnitude or color index having a residual greater than 2(sigma-prime), where sigma-prime is the standard deviation for the determinations of unit weight.

New measurements of radial velocities in clusters of galaxies

Redshifts for 100 galaxies in 10 clusters of galaxies are presented based on data obtained between March 1984 and March 1985 from Calar Alto, La Palma, and ESO, and on data from Mauna Kea. Data for individual galaxies are given, and the accuracy of the velocities of the four instruments is discussed. Comparison with published data shows the present velocities to be shifted by + 4.0 km/s on average, with a standard deviation in the difference of 89.7 km/s, consistent with the rms of redshift measurements which range from 50-100 km/s.

UVBY-Beta Photometry for 67 Stars in the Region of Alpha-Persei

UVBY-Beta photometric data are presented for 67 stars in the region of alpha-Persei and their relationship to the cluster is analyzed. These data allowed us to confirm at least 16 new members of the alpha-Persei open cluster.

Analysis of IRAS stellar sources in Alpha Persei region

The present study is an analysis of IR sources in the Alpha Persei open cluster region from the IRAS Point Source Catalog and from ground-based photometric observations. Cross-identification between stars in the region and IRAS Point Source Catalog was performed and nine new associations were found. BVRI Johnson photometry for 24 of the matched objects have been carried out. Physical identity of visual and IRAS sources and relationship to the Alpha Persei open cluster are discussed.

On the binary nature of the γ-ray sources AGL J2241+4454 (= MWC 656) and HESS J0632+057 (= MWC 148)

We present optical spectroscopy of MWC 656 and MWC 148, the proposed optical counterparts of the gamma-ray sources AGL J2241+4454 and HESS J0632+0 57, respectively. The main parameters of the Halpha emission line (EW, FWHM and centroid velocity) in these stars are modulated on the proposed orbital periods of 60.37 and 321 days, respectively. These modulations are likely produced by the resonant interaction of the Be discs with compact stars in eccentric orbits. We also present radial velocity curves of the optical stars folded on the above periods and obtain the first orbital elements of the two gamma-ray sources thus confirming their binary nature. Our orbital solution support eccentricities e~0.4 and 0.83+-0.08 for MWC 656 and MWC 148, respectively. Further, our orbital elements imply that the X-ray outbursts in HESS J0632+057/MWC 148 are delayed ~0.3 orbital phases after periastron passage, similarly to the case of LS I +61 303. In addition, the optical photometric light curve maxima in AGL J2241+4454/MWC 656 occur ~0.25 phases passed periastron, similar to what is seen in LS I +61 303. We also find that the orbital eccentricity is correlated with orbital period for the known gamma-ray binaries. This is explained by the fact that small stellar separations are required for the efficient triggering of VHE radiation. Another correlation between the EW of Halpha and orbital period is also observed, similarly to the case of Be/X-ray binaries. These correlations are useful to provide estimates of the key orbital parameters Porb and e from the Halpha line in future Be gamma-ray binary candidates.

Metal-Nitride-oxide-semiconductor light-emitting devices for general lighting.

The potential for application of silicon nitride-based light sources to general lighting is reported. The mechanism of current injection and transport in silicon nitride layers and silicon oxide tunnel layers is determined by electro-optical characterization of both bi- and tri-layers. It is shown that red luminescence is due to bipolar injection by direct tunneling, whereas Poole-Frenkel ionization is responsible for blue-green emission. The emission appears warm white to the eye, and the technology has potential for large-area lighting devices. A photometric study, including color rendering, color quality and luminous efficacy of radiation, measured under various AC excitation conditions, is given for a spectrum deemed promising for lighting. A correlated color temperature of 4800K was obtained using a 35% duty cycle of the AC excitation signal. Under these conditions, values for general color rendering index of 93 and luminous efficacy of radiation of 112 lm/W are demonstrated. This proof of concept demonstrates that mature silicon technology, which is extendable to lowcost, large-area lamps, can be used for general lighting purposes. Once the external quantum efficiency is improved to exceed 10%, this technique could be competitive with other energy-efficient solid-state lighting options. ©2011 Optical Society of America OCIS codes: (230.2090) Electro-optical devices; (150.2950) Illumination.

Ultraviolet optical and microstructural properties of MgF2 and LaF3 coatings deposited by ion-beam sputtering and boat and electron-beam evaporation

Single layers of MgF2 and LaF3 were deposited upon superpolished fused-silica and CaF2 substrates by ion-beam sputtering (IBS) as well as by boat and electron beam (e-beam) evaporation and were characterized by a variety of complementary analytical techniques. Besides undergoing photometric and ellipsometric inspection, the samples were investigated at 193 and 633 nm by an optical scatter measurement facility. The structural properties were assessed with atomic-force microscopy, x-ray diffraction, TEM techniques that involved conventional thinning methods for the layers. For measurement of mechanical stress in the coatings, special silicon substrates were coated and analyzed. The dispersion behavior of both deposition materials, which was determined on the basis of various independent photometric measurements and data reduction techniques, is in good agreement with that published in the literature and with the bulk properties of the materials. The refractive indices of the MgF2 coatings ranged from 1.415 to 1.440 for the wavelength of the ArF excimer laser (193 nm) and from 1.435 to 1.465 for the wavelength of the F2 excimer laser (157 nm). For single layers of LaF3 the refractive indices extended from 1.67 to 1.70 at 193 nm to ~1.80 at 157 nm. The IBS process achieves the best homogeneity and the lowest surface roughness values (close to 1 nmrms) of the processes compared in the joint experiment. In contrast to MgF2 boat and e-beam evaporated coatings, which exhibit tensile mechanical stress ranging from 300 to 400 MPa, IBS coatings exhibit high compressive stress of as much as 910 MPa. A similar tendency was found for coating stress in LaF3 single layers. Experimental results are discussed with respect to the microstructural and compositional properties as well as to the surface topography of the coatings.

Gaia photometry for white dwarfs

Context. White dwarfs can be used to study the structure and evolution of the Galaxy by analysing their luminosity function and initial mass function. Among them, the very cool white dwarfs provide the information for the early ages of each population. Because white dwarfs are intrinsically faint only the nearby (~ 20 pc) sample is reasonably complete. The Gaia space mission will drastically increase the sample of known white dwarfs through its 5-6 years survey of the whole sky up to magnitude V = 20-25. Aims. We provide a characterisation of Gaia photometry for white dwarfs to better prepare for the analysis of the scientific output of the mission. Transformations between some of the most common photometric systems and Gaia passbands are derived. We also give estimates of the number of white dwarfs of the different galactic populations that will be observed. Methods. Using synthetic spectral energy distributions and the most recent Gaia transmission curves, we computed colours of three different types of white dwarfs (pure hydrogen, pure helium, and mixed composition with H/He = 0.1). With these colours we derived transformations to other common photometric systems (Johnson-Cousins, Sloan Digital Sky Survey, and 2MASS). We also present numbers of white dwarfs predicted to be observed by Gaia. Results. We provide relationships and colourcolour diagrams among different photometric systems to allow the prediction and/or study of the Gaia white dwarf colours. We also include estimates of the number of sources expected in every galactic population and with a maximum parallax error. Gaia will increase the sample of known white dwarfs tenfold to about 200 000. Gaia will be able to observe thousands of very cool white dwarfs for the first time, which will greatly improve our understanding of these stars and early phases of star formation in our Galaxy.