222 research outputs found
VLBI measurement of the secular aberration drift
While analyzing decades of very long baseline interferometry (VLBI) data, we
detected the secular aberration drift of the extragalatic radio source proper
motions caused by the rotation of the Solar System barycenter around the
Galactic center. Our results agree with the predicted estimate to be 4-6 micro
arcseconds per year ({\mu}as/yr) towards {\alpha} = 266\circ and {\delta} =
-29\circ. In addition, we tried to detect the quadrupole systematics of the
velocity field. The analysis method consisted of three steps. First, we
analyzed geodetic and astrometric VLBI data to produce radio source coordinate
time series. Second, we fitted proper motions of 555 sources with long
observational histories over the period 1990-2010 to their respective
coordinate time series. Finally, we fitted vector spherical harmonic components
of degrees 1 and 2 to the proper motion field. Within the error bars, the
magnitude and the direction of the dipole component agree with predictions. The
dipole vector has an amplitude of 6.4 \pm 1.5 {\mu}as/yr and is directed
towards equatorial coordinates {\alpha} = 263\circ and {\delta} = -20\circ. The
quadrupole component has not been detected. The primordial gravitational wave
density, integrated over a range of frequencies less than 10-9 Hz, has a limit
of 0.0042 h-2 where h is the normalized Hubble constant is H0/(100 km s-1)
Report of the panel on earth rotation and reference frames, section 7
Objectives and requirements for Earth rotation and reference frame studies in the 1990s are discussed. The objectives are to observe and understand interactions of air and water with the rotational dynamics of the Earth, the effects of the Earth's crust and mantle on the dynamics and excitation of Earth rotation variations over time scales of hours to centuries, and the effects of the Earth's core on the rotational dynamics and the excitation of Earth rotation variations over time scales of a year or longer. Another objective is to establish, refine and maintain terrestrial and celestrial reference frames. Requirements include improvements in observations and analysis, improvements in celestial and terrestrial reference frames and reference frame connections, and improved observations of crustal motion and mass redistribution on the Earth
GAIA: Composition, Formation and Evolution of the Galaxy
The GAIA astrometric mission has recently been approved as one of the next
two `cornerstones' of ESA's science programme, with a launch date target of not
later than mid-2012. GAIA will provide positional and radial velocity
measurements with the accuracies needed to produce a stereoscopic and kinematic
census of about one billion stars throughout our Galaxy (and into the Local
Group), amounting to about 1 per cent of the Galactic stellar population.
GAIA's main scientific goal is to clarify the origin and history of our Galaxy,
from a quantitative census of the stellar populations. It will advance
questions such as when the stars in our Galaxy formed, when and how it was
assembled, and its distribution of dark matter. The survey aims for
completeness to V=20 mag, with accuracies of about 10 microarcsec at 15 mag.
Combined with astrophysical information for each star, provided by on-board
multi-colour photometry and (limited) spectroscopy, these data will have the
precision necessary to quantify the early formation, and subsequent dynamical,
chemical and star formation evolution of our Galaxy. Additional products
include detection and orbital classification of tens of thousands of
extra-Solar planetary systems, and a comprehensive survey of some 10^5-10^6
minor bodies in our Solar System, through galaxies in the nearby Universe, to
some 500,000 distant quasars. It will provide a number of stringent new tests
of general relativity and cosmology. The complete satellite system was
evaluated as part of a detailed technology study, including a detailed payload
design, corresponding accuracy assesments, and results from a prototype data
reduction development.Comment: Accepted by A&A: 25 pages, 8 figure
Comparison of tricuspid inflow and superior vena caval Doppler velocities in acute simulated hypovolemia: new non-invasive indices for evaluating right ventricular preload
BACKGROUND: Assessment of cardiac preload is important for clinical management of some emergencies related to hypovolemia. Effects of acute simulated hypovolemia on Doppler blood flow velocity indices of tricuspid valve (TV) and superior vena cava (SVC) were investigated in order to find sensitive Doppler indices for predicting right ventricular preload. METHODS: Doppler flow patterns of SVC and TV in 12 healthy young men were examined by transthoracic echocardiography (TTE) during graded lower body negative pressure (LBNP) of up to -60 mm Hg which simulated acute hypovolemia. Peak velocities of all waves and their related ratios (SVC S/D and tricuspid E/A) were measured, calculated and statistically analyzed. RESULTS: Except for the velocity of tricuspid A wave, velocities of all waves and their related ratios declined during volume decentralization. Of all indices measured, the peak velocities of S wave and AR wave in SVC correlated most strongly with levels of LBNP (r = -0.744 and -0.771, p < 0.001). CONCLUSION: The S and AR velocities are of good values in assessing right ventricular preload. Monitoring SVC flow may provide a relatively noninvasive means to assess direct changes in right ventricular preload
Aspects anthropologiques du diabète sucré, problème d'équilibration de la maladie dans une ethnie transplantée
The Large Quasar Reference Frame (LQRF) - an optical representation of the ICRS
The large number and all-sky distribution of quasars from different surveys,
along with their presence in large, deep astrometric catalogs,enables the
building of an optical materialization of the ICRS following its defining
principles. Namely: that it is kinematically non-rotating with respect to the
ensemble of distant extragalactic objects; aligned with the mean equator and
dynamical equinox of J2000; and realized by a list of adopted coordinates of
extragalatic sources. Starting from the updated and presumably complete LQAC
list of QSOs, the initial optical positions of those quasars are found in the
USNO B1.0 and GSC2.3 catalogs, and from the SDSS DR5. The initial positions are
next placed onto UCAC2-based reference frames, following by an alignment with
the ICRF, to which were added the most precise sources from the VLBA calibrator
list and the VLA calibrator list - when reliable optical counterparts exist.
Finally, the LQRF axes are inspected through spherical harmonics, contemplating
to define right ascension, declination and magnitude terms. The LQRF contains
J2000 referred equatorial coordinates for 100,165 quasars, well represented
across the sky, from -83.5 to +88.5 degrees in declination, and with 10 arcmin
being the average distance between adjacent elements. The global alignment with
the ICRF is 1.5 mas, and the individual position accuracies are represented by
a Poisson distribution that peaks at 139 mas in right ascension and 130 mas in
declination. It is complemented by redshift and photometry information from the
LQAC. The LQRF is designed to be an astrometric frame, but it is also the basis
for the GAIA mission initial quasars' list, and can be used as a test bench for
quasars' space distribution and luminosity function studies.Comment: 23 pages, 23 figures, 6 tables Accepted for publication by Astronomy
& Astrophysics, on 25 May 200
Hemodynamic parameters to guide fluid therapy
The clinical determination of the intravascular volume can be extremely difficult in critically ill and injured patients as well as those undergoing major surgery. This is problematic because fluid loading is considered the first step in the resuscitation of hemodynamically unstable patients. Yet, multiple studies have demonstrated that only approximately 50% of hemodynamically unstable patients in the intensive care unit and operating room respond to a fluid challenge. Whereas under-resuscitation results in inadequate organ perfusion, accumulating data suggest that over-resuscitation increases the morbidity and mortality of critically ill patients. Cardiac filling pressures, including the central venous pressure and pulmonary artery occlusion pressure, have been traditionally used to guide fluid management. However, studies performed during the past 30 years have demonstrated that cardiac filling pressures are unable to predict fluid responsiveness. During the past decade, a number of dynamic tests of volume responsiveness have been reported. These tests dynamically monitor the change in stroke volume after a maneuver that increases or decreases venous return (preload) and challenges the patients' Frank-Starling curve. These dynamic tests use the change in stroke volume during mechanical ventilation or after a passive leg raising maneuver to assess fluid responsiveness. The stroke volume is measured continuously and in real-time by minimally invasive or noninvasive technologies, including Doppler methods, pulse contour analysis, and bioreactance
Digital Image Correlation technique: Application to early fatigue damage detection in stainless steel
In the context of development of a numerical model, to accurately predict the fatigue life of a structural component, it is fundamental to consider both the initiation stage and the propagation stage of micro-cracks. Such a development requires dedicated experimental tools both to provide the physical understanding needed for designing models and to validate the proposed approaches and models. Thus, this paper presents the experimental means that need to be used for such a purpose. The approach is based on the analysis of displacement field measurements by digital image correlation (DIC) during low-cycle fatigue tests. A specific filtering tool is also presented to minimize the committed errors when derivative operation is performed for strain calculation. Therefore, in this quite recent application of DIC, the reproducibility of the method has to be questioned and validated, with help of some more conventional strain measurements devices. It seems that the experimental conditions have to be carefully controlled, so that the results can be interpreted in terms of mechanical phenomena
Homogenization in compiling ICRF combined catalogs
Context. The International Astronomical Union (IAU) recommendations regarding the International Celestial Reference Frame
(ICRF) realizations require the construction of radio sources catalogs obtained using very-long-baseline interferometry (VLBI) methods.
The improvement of these catalogs is a necessary procedure for the further densification of the ICRF over the celestial sphere.
Aims. The different positions obtained from several catalogs using common sources to the ICRF make it necessary to critically revise
the different methods employed in improving the ICRF from several radio sources catalogs. In this sense, a revision of the analytical
and the statistical methods is necessary in line with their advantages and disadvantages. We have a double goal: first, we propose
an adequate treatment of the residual of several catalogs to obtain a homogeneous catalog; second, we attempt to discern whether a
combined catalog is homogeneous.
Methods. We define homogeneity as applied to our problem in a dual sense: the first deals with the spatial distribution of the data over
the celestial sphere. The second has a statistical meaning, as we consider that homogeneity exists when the residual between a given
catalog and the ICRF behaves as a unimodal pure Gaussian. We use a nonparametrical method, which enables us to homogeneously
extend the statistical properties of the residual over the entire sphere. This intermediate adjustment allows for subsequent computation
of the coefficients for any parametrical adjustment model that has a higher accuracy and greater stability, and it prevents problems
related with direct adjustments using the models. On the other hand, the homogeneity of the residuals in a catalog is tested using
different weights. Our procedure also serves to propose the most suitable weights to maintain homogeneity in the final results. We
perform a test using the ICRF-Ext2, JPL, and USNO quasar catalogs.
Results. We show that a combination of catalogs can only be homogeneous if we configure the weights carefully. In addition, we
provide a procedure to detect inhomogeneities, which could introduce deformities, in these combined catalogs.
Conclusions. An inappropriate use of analytical adjustment methods provides erroneous results. Analogously, it is not possible to
obtain homogeneous-combined catalogs unless we use the adequate weights.Part of this work was supported by a grant P1-1B2009-07 from Fundacio Caixa Castello BANCAIXA and a grant P1-061I455.01/1 from Bancaja.Marco Castillo, FJ.; Martínez Uso, MJ.; Lopez Orti, JA. (2013). Homogenization in compiling ICRF combined catalogs. Astronomy and Astrophysics. 558(1):1-10. https://doi.org/10.1051/0004-6361/201321995S1105581Arias, E. F., Feissel, M., & Lestrade, J. F. 1988, Annual Report for 1987, Observatoire de Paris, Paris, D-113Ayant, Y., & Borg, M. 1971, Fonctions spéciales à l’usage des étudiants en physique (Paris: Dunod)Cucker, F., & Smale, S. (2001). On the mathematical foundations of learning. Bulletin of the American Mathematical Society, 39(01), 1-50. doi:10.1090/s0273-0979-01-00923-5Fan, J., & Gijbels, I. (1992). Variable Bandwidth and Local Linear Regression Smoothers. The Annals of Statistics, 20(4), 2008-2036. doi:10.1214/aos/1176348900Fey, A. L., Ma, C., Arias, E. F., Charlot, P., Feissel-Vernier, M., Gontier, A.-M., … MacMillan, D. S. (2004). The Second Extension of the International Celestial Reference Frame: ICRF-EXT.1. The Astronomical Journal, 127(6), 3587-3608. doi:10.1086/420998Fey, A., Gordon, D., & Jacobs, C. 2009, IERS Technical Note 35, The Second realization of the International Celestial Reference Frame by Very Long Baseline Interferometry, Frankfurt am Main 2010: Verlag des Bundesamts für Kartographie und GeodäsieIERS 1999, 1998 IERS Annual Report, Observatoire de Paris, D. Gambis (Editor)Heiskanen, W. A., & Moritz H. 1967, Physical Geodesy (San Francisco: Freeman)Ma, C., Arias, E. F., Eubanks, T. M., Fey, A. L., Gontier, A.-M., Jacobs, C. S., … Charlot, P. (1998). The International Celestial Reference Frame as Realized by Very Long Baseline Interferometry. The Astronomical Journal, 116(1), 516-546. doi:10.1086/300408Marco, F. J., Martínez, M. J., & López, J. A. (2004). A critical discussion on parametric and nonparametric regression methods applied to Hipparcos-FK5 residuals. Astronomy & Astrophysics, 418(3), 1159-1170. doi:10.1051/0004-6361:20034441Marco, F. J., Martnez, M. J., & Lpez, J. A. (2004). Analysis of Systematic Differences of Astrometric Catalogs in a Band. The Astronomical Journal, 127(1), 549-559. doi:10.1086/380235Sfikas et al. 2005, in ICANN 2005, LNCS 3697, eds. W. Duch et al., 835Sokolova, J., & Malkin, Z. (2007). On comparison and combination of catalogues of radio source positions. Astronomy & Astrophysics, 474(2), 665-670. doi:10.1051/0004-6361:20077450Walter, S., & Sovers, O. J. 2000, Astrometry of fundamental catalogs. The evolution from optical to radio reference frames (Berlin: Springer-Verlag)Wand, M. P., & Jones, M. C. 1995, Kernel Smoothing (London: Chapman and Hall)Yatskiv, YA S., & Kuryakova. 1990, in Inertial Coordinate System on the Sky, Proc. 141th, eds. J.H. Lieske, & V. K. Abalakin, IAU Symp., 295Yu, M., Manchester, R. N., Hobbs, G., Johnston, S., Kaspi, V. M., Keith, M., … Xu, R. X. (2012). Detection of 107 glitches in 36 southern pulsars. Monthly Notices of the Royal Astronomical Society, 429(1), 688-724. doi:10.1093/mnras/sts36
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