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Showing papers by "Miquel Nofrarías published in 2011"


Journal ArticleDOI
26 Jul 2011-Vaccine
TL;DR: The results clearly demonstrate that targeting antigens to antigen professional cells exponentially enhanced the immune response induced in pigs, albeit that the DNA vaccine was not able to confer protection against lethal viral challenge.

71 citations


Journal ArticleDOI
F. Antonucci1, Michele Armano2, Heather Audley3, G. Auger4, Matteo Benedetti1, Pierre Binétruy4, C. Boatella, J. Bogenstahl3, Daniele Bortoluzzi1, Paolo Bosetti1, M. Caleno2, Antonella Cavalleri1, M. Cesa2, M. Chmeissani5, Giacomo Ciani6, A. Conchillo7, G. Congedo1, I. Cristofolini1, M. Cruise8, Karsten Danzmann3, F. De Marchi1, M. Diaz-Aguilo, Ingo Diepholz3, G. Dixon8, Rita Dolesi1, N. Dunbar9, J. Fauste2, Luigi Ferraioli1, D. Fertin2, Walter Fichter, Ewan Fitzsimons10, M. Freschi2, A. F. Garcia Marin3, C. García Marirrodriga2, R. Gerndt11, Lluis Gesa7, F. Gilbert7, Domenico Giardini12, Catia Grimani, A. Grynagier, B. Guillaume2, Felipe Guzman3, I. Harrison13, Gerhard Heinzel3, Martin Hewitson3, Daniel Hollington14, J. H. Hough10, D. Hoyland8, Mauro Hueller1, J. Huesler2, O. Jeannin4, Oliver Jennrich2, Philippe Jetzer15, B. Johlander2, Christian J. Killow10, X. Llamas, Ivan Lloro7, A. Lobo7, R. Maarschalkerweerd13, S. Madden2, Davor Mance12, Ignacio Mateos7, Paul McNamara2, José F. F. Mendes13, E. Mitchell14, A. Monsky3, D. Nicolini2, Daniele Nicolodi1, Miquel Nofrarías3, F. Pedersen2, Michael Perreur-Lloyd10, A. Perreca1, Eric Plagnol4, P. Prat4, Giuseppe D. Racca2, B. Rais4, Juan Ramos-Castro16, J. Reiche3, J. A. Romera Perez2, David J. Robertson10, H. Rozemeijer2, J. Sanjuan6, A. Schleicher11, M. Schulte14, D. Shaul14, L. Stagnaro2, S. Strandmoe2, Frank Steier3, T. J. Sumner14, A.M. Taylor10, D. Texier2, C. Trenkel9, D. Tombolato1, Stefano Vitale1, Gudrun Wanner3, H. Ward10, S. Waschke14, Peter Wass14, W. J. Weber1, Peter Zweifel12 
TL;DR: LISA Pathfinder as discussed by the authors is a dedicated technology demonstrator for the joint ESA/NASA Laser Interferometer Space Antenna (LISA) mission, which essentially mimics one arm of the LISA constellation by shrinking the 5 million kilometre armlength down to a few tens of centimetres, giving up the sensitivity to gravitational waves, but keeping the measurement technology.
Abstract: LISA Pathfinder, the second of the European Space Agency's Small Missions for Advanced Research in Technology (SMART), is a dedicated technology demonstrator for the joint ESA/NASA Laser Interferometer Space Antenna (LISA) mission. The technologies required for LISA are many and extremely challenging. This coupled with the fact that some flight hardware cannot be fully tested on ground due to Earth-induced noise led to the implementation of the LISA Pathfinder mission to test the critical LISA technologies in a flight environment. LISA Pathfinder essentially mimics one arm of the LISA constellation by shrinking the 5 million kilometre armlength down to a few tens of centimetres, giving up the sensitivity to gravitational waves, but keeping the measurement technology: the distance between the two test masses is measured using a laser interferometric technique similar to one aspect of the LISA interferometry system. The scientific objective of the LISA Pathfinder mission consists then of the first in-flight test of low frequency gravitational wave detection metrology. LISA Pathfinder is due to be launched in 2013 on-board a dedicated small launch vehicle (VEGA). After a series of apogee raising manoeuvres using an expendable propulsion module, LISA Pathfinder will enter a transfer orbit towards the first Sun?Earth Lagrange point (L1). After separation from the propulsion module, the LPF spacecraft will be stabilized using the micro-Newton thrusters, entering a 500?000 km by 800?000 km Lissajous orbit around L1. Science results will be available approximately 2 months after launch.

59 citations


Journal ArticleDOI
F. Antonucci1, Michele Armano2, Heather Audley3, G. Auger4, Matteo Benedetti1, Pierre Binétruy4, C. Boatella, J. Bogenstahl3, Daniele Bortoluzzi1, Paolo Bosetti1, N. Brandt5, M. Caleno2, Antonella Cavalleri1, M. Cesa2, M. Chmeissani6, Giacomo Ciani7, A. Conchillo8, G. Congedo1, I. Cristofolini1, M. Cruise9, Karsten Danzmann3, F. De Marchi1, M. Diaz-Aguilo, Ingo Diepholz3, G. Dixon9, Rita Dolesi1, N. Dunbar10, J. Fauste2, Luigi Ferraioli1, D. Fertin2, Walter Fichter, Ewan Fitzsimons11, M. Freschi2, A. F. Garcia Marin3, C. García Marirrodriga2, R. Gerndt5, Lluis Gesa8, Domenico Giardini12, F. Gibert8, Catia Grimani, A. Grynagier, B. Guillaume2, Felipe Guzman13, I. Harrison14, Gerhard Heinzel3, Martin Hewitson3, Daniel Hollington15, J. H. Hough11, D. Hoyland9, Mauro Hueller1, J. Huesler2, O. Jeannin4, Oliver Jennrich2, Philippe Jetzer16, B. Johlander2, Christian J. Killow11, X. Llamas, Ivan Lloro8, A. Lobo8, R. Maarschalkerweerd14, S. Madden2, D. Mance16, Ignacio Mateos8, Paul McNamara2, José F. F. Mendes14, E. Mitchell15, A. Monsky3, D. Nicolini2, Daniele Nicolodi1, Miquel Nofrarías3, F. Pedersen2, Michael Perreur-Lloyd11, A. Perreca1, Eric Plagnol4, P. Prat4, Giuseppe D. Racca2, B. Rais4, Juan Ramos-Castro17, J. Reiche3, J. A. Romera Perez2, David Robertson11, H. Rozemeijer2, J. Sanjuan7, A. Schleicher5, M. Schulte15, D. Shaul15, L. Stagnaro2, S. Strandmoe2, Frank Steier3, T. J. Sumner15, A.M. Taylor11, D. Texier2, C. Trenkel10, D. Tombolato1, Stefano Vitale1, Gudrun Wanner3, H. Ward11, S. Waschke15, Peter Wass15, W. J. Weber1, Peter Zweifel12 
TL;DR: In this article, a quantitative assessment of the performance of the upcoming LISA Pathfinder geodesic explorer mission is presented, based on the results of extensive ground testing and simulation campaigns using flight hardware, flight control and operations algorithms.
Abstract: This paper presents a quantitative assessment of the performance of the upcoming LISA Pathfinder geodesic explorer mission. The findings are based on the results of extensive ground testing and simulation campaigns using flight hardware, flight control and operations algorithms. The results show that, for the central experiment of measuring the stray differential acceleration between the LISA test masses, LISA Pathfinder will be able to verify the overall acceleration noise to within a factor 2 of the LISA requirement at 1 mHz and within a factor 6 at 0.1 mHz. We also discuss the key elements of the physical model of disturbances, coming from LISA Pathfinder and ground measurement that will guarantee the LISA performance.

57 citations


Journal ArticleDOI
TL;DR: In this paper, a Mycobacterium caprae infection model has been developed in goats, where 11 6-month-old goats were infected by the endobronchial route with 1.5 × 10(3) CFU, and two other goats were kept as noninfected controls.
Abstract: Caprine tuberculosis (TB) has increased in recent years, highlighting the need to address the problem the infection poses in goats. Moreover, goats may represent a cheaper alternative for testing of prototype vaccines in large ruminants and humans. With this aim, a Mycobacterium caprae infection model has been developed in goats. Eleven 6-month-old goats were infected by the endobronchial route with 1.5 × 10(3) CFU, and two other goats were kept as noninfected controls. The animals were monitored for clinical and immunological parameters throughout the experiment. After 14 weeks, the goats were euthanized, and detailed postmortem analysis of lung lesions was performed by multidetector computed tomography (MDCT) and direct observation. The respiratory lymph nodes were also evaluated and cultured for bacteriological analysis. All infected animals were positive in a single intradermal comparative cervical tuberculin (SICCT) test at 12 weeks postinfection (p.i.). Gamma interferon (IFN-γ) antigen-specific responses were detected from 4 weeks p.i. until the end of the experiment. The humoral response to MPB83 was especially strong at 14 weeks p.i. (13 days after SICCT boost). All infected animals presented severe TB lesions in the lungs and associated lymph nodes. M. caprae was recovered from pulmonary lymph nodes in all inoculated goats. MDCT allowed a precise quantitative measure of TB lesions. Lesions in goats induced by M. caprae appeared to be more severe than those induced in cattle by M. bovis over a similar period of time. The present work proposes a reliable new experimental animal model for a better understanding of caprine tuberculosis and future development of vaccine trials in this and other species.

51 citations


01 Jan 2011
TL;DR: The present work proposes a reliable new experimental animal model for a better understanding of caprine tuberculosis and future development of vaccine trials in this and other species.

47 citations


Journal ArticleDOI
Heather Audley1, Karsten Danzmann1, A. F. Garcia Marin1, Gerhard Heinzel1, A. Monsky1, Miquel Nofrarías1, Frank Steier1, D. Gerardi, R. Gerndt, Gerald Hechenblaikner, Ulrich Johann, P. Luetzow-Wentzky, V. Wand, F. Antonucci2, Michele Armano3, G. Auger4, Matteo Benedetti2, Pierre Binétruy4, C. Boatella, J. Bogenstahl1, Daniele Bortoluzzi2, Paolo Bosetti2, M. Caleno3, Antonella Cavalleri2, M. Cesa3, M. Chmeissani5, Giacomo Ciani6, A. Conchillo7, G. Congedo2, I. Cristofolini2, M. Cruise8, F. De Marchi2, M. Diaz-Aguilo, Ingo Diepholz1, G. Dixon8, Rita Dolesi2, J. Fauste3, Luigi Ferraioli2, D. Fertin3, Walter Fichter, Ewan Fitzsimons9, M. Freschi3, C. García Marirrodriga3, Lluis Gesa7, F. Gibert7, Domenico Giardini10, Catia Grimani, A. Grynagier, B. Guillaume3, Felipe Guzman1, I. Harrison11, Martin Hewitson1, Daniel Hollington12, J. H. Hough9, D. Hoyland8, Mauro Hueller2, J. Huesler3, O. Jeannin4, Oliver Jennrich3, Philippe Jetzer13, B. Johlander3, Christian J. Killow9, X. Llamas, Ivan Lloro7, A. Lobo7, R. Maarschalkerweerd11, S. Madden3, Davor Mance10, Ignacio Mateos7, Paul McNamara3, José F. F. Mendes11, E. Mitchell12, D. Nicolini3, Daniele Nicolodi2, F. Pedersen3, Michael Perreur-Lloyd9, A. Perreca2, Eric Plagnol4, P. Prat4, Giuseppe D. Racca3, B. Rais4, Juan Ramos-Castro14, J. Reiche1, J. A. Romera Perez3, D. I. Robertson9, H. Rozemeijer3, J. Sanjuan6, M. Schulte12, D. Shaul12, L. Stagnaro3, S. Strandmoe3, T. J. Sumner12, A.M. Taylor9, D. Texier3, C. Trenkel15, D. Tombolato2, Stefano Vitale2, Gudrun Wanner1, H. Ward9, S. Waschke12, Peter Wass12, W. J. Weber2, Peter Zweifel10 
TL;DR: The first complete integration and testing of the space-qualified hardware and are the first tests on an optical system level were performed at the Albert Einstein Institute, Hannover, Germany as discussed by the authors.
Abstract: Preparations for the LISA Pathfinder mission have reached an exciting stage. Tests of the engineering model (EM) of the optical metrology system have recently been completed at the Albert Einstein Institute, Hannover, and flight model tests are now underway. Significantly, they represent the first complete integration and testing of the space-qualified hardware and are the first tests on an optical system level. The results and test procedures of these campaigns will be utilized directly in the ground-based flight hardware tests, and subsequently during in-flight operations. In addition, they allow valuable testing of the data analysis methods using the MATLAB-based LTP data analysis toolbox. This paper presents an overview of the results from the EM test campaign that was successfully completed in December 2009.

26 citations


Journal ArticleDOI
TL;DR: Boar lines were used to inseminate sows from the same genetic line and total post-weaning mortality (PWM), PWM associated to PMWS (PMWS-PWM) and body weight (BW) evolution and BW was influenced by interactions between genetics and both farm and pig age, and was lower in piglets from farm-2.

21 citations


Journal ArticleDOI
F. Antonucci1, Michele Armano, Heather Audley2, G. Auger3, Matteo Benedetti1, Pierre Binétruy3, C. Boatella, J. Bogenstahl2, Daniele Bortoluzzi1, Paolo Bosetti1, M. Caleno4, Antonella Cavalleri1, M. Cesa4, M. Chmeissani5, Giacomo Ciani6, A. Conchillo7, G. Congedo1, I. Cristofolini1, M. Cruise8, Karsten Danzmann2, F. De Marchi1, M. Diaz-Aguilo, Ingo Diepholz2, G. Dixon8, Rita Dolesi1, J. Fauste, Luigi Ferraioli1, D. Fertin4, Walter Fichter, Ewan Fitzsimons9, M. Freschi, A. F. Garcia Marin2, C. García Marirrodriga4, Lluis Gesa7, Domenico Giardini10, Catia Grimani, A. Grynagier, B. Guillaume4, Felipe Guzman2, I. Harrison11, Gerhard Heinzel2, Martin Hewitson2, Daniel Hollington12, J. H. Hough9, D. Hoyland8, Mauro Hueller1, J. Huesler4, O. Jeannin3, Oliver Jennrich4, Philippe Jetzer13, B. Johlander4, Christian J. Killow9, X. Llamas, Ivan Lloro7, A. Lobo7, R. Maarschalkerweerd11, S. Madden4, D. Mance13, Ignacio Mateos7, Paul McNamara4, José F. F. Mendes11, E. Mitchell12, A. Monsky2, D. Nicolini4, Daniele Nicolodi1, Miquel Nofrarías2, F. Pedersen4, Michael Perreur-Lloyd9, A. Perreca1, Eric Plagnol3, P. Prat3, Giuseppe D. Racca4, B. Rais3, Juan Ramos-Castro14, J. Reiche2, J. A. Romera Perez4, D. I. Robertson9, H. Rozemeijer4, J. Sanjuan6, M. Schulte12, D. Shaul12, L. Stagnaro4, S. Strandmoe4, Frank Steier2, T. J. Sumner12, A.M. Taylor9, D. Texier, C. Trenkel15, D. Tombolato1, Stefano Vitale1, Gudrun Wanner2, H. Ward9, S. Waschke12, Peter Wass12, W. J. Weber1, Peter Zweifel10 
TL;DR: In this article, the authors describe the various aspects of the full data analysis chain that are needed to successfully characterize the LISA Pathfinder and build up the noise budget during mission operations.
Abstract: As the launch of LISA Pathfinder (LPF) draws near, more and more effort is being put in to the preparation of the data analysis activities that will be carried out during the mission operations. The operations phase of the mission will be composed of a series of experiments that will be carried out on the satellite. These experiments will be directed and analysed by the data analysis team, which is part of the operations team. The operations phase will last about 90 days, during which time the data analysis team aims to fully characterize the LPF, and in particular, its core instrument the LISA Technology Package. By analysing the various couplings present in the system, the different noise sources that will disturb the system, and through the identification of the key physical parameters of the system, a detailed noise budget of the instrument will be constructed that will allow the performance of the different subsystems to be assessed and projected towards LISA. This paper describes the various aspects of the full data analysis chain that are needed to successfully characterize the LPF and build up the noise budget during mission operations.

18 citations


Journal ArticleDOI
TL;DR: In this paper, the design, implementation, and characterization of fully digital control loops for laser frequency stabilization, differential phase-locking, and performance optimization of the optical metrology system on-board the LISA Pathfinder space mission is described.
Abstract: We report on the design, implementation, and characterization of fully digital control loops for laser frequency stabilization, differential phase-locking, and performance optimization of the optical metrology system on-board the LISA Pathfinder space mission. The optical metrology system consists of a laser with modulator, four Mach-Zehnder interferometers, a phase-meter and a digital processing unit for data analysis. The digital loop design has the advantage of easy and flexible controller implementation and loop calibration, automated and flexible locking and resetting, and improved performance over analog circuitry. Using the practical ability of our system to modulate the laser frequency allows us to accurately determine the open-loop transfer function and other system properties. Various noise sources and their impact on system performance are investigated in detail.

16 citations


Journal ArticleDOI
TL;DR: The requirements and performance of this instrumentation, specially focusing on the Radiation Monitor and the DMU, are reviewed, as well as the status of their programmed use during mission operations, on which work is ongoing at the time of writing.
Abstract: The LISA Pathfinder DMU (Data Management Unit) flight model was formally accepted by ESA and ASD on 11 February 2010, after all hardware and software tests had been successfully completed. The diagnostics items are scheduled to be delivered by the end of 2010. In this paper, we review the requirements and performance of this instrumentation, specially focusing on the Radiation Monitor and the DMU, as well as the status of their programmed use during mission operations, on which work is ongoing at the time of writing.

15 citations


Journal ArticleDOI
TL;DR: In this article, the authors discuss two main problems associated with the analysis of the data from LISA Pathfinder (LPF): i) Excess noise detection and ii) Noise parameter identification.
Abstract: In this paper we discuss two main problems associated with the analysis of the data from LISA Pathfinder (LPF): i) Excess noise detection and ii) Noise parameter identification. The mission is focused on the low frequency region ([0.1; 10] mHz) of the available signal spectrum. In such a region the signal is dominated by the force noise acting on test masses. Noise analysis is expected to deal with a limited amount of non-Gaussian data, since the spectrum statistics will be far from Gaussian and the lowest available frequency is limited by the data length. In this paper we analyze the details of the expected statistics for spectral data and develop two suitable excess noise estimators. One is based on the statistical properties of the integrated spectrum, the other is based on Kolmogorov-Smirnov test. The sensitivity of the estimators is discussed theoretically for independent data, then the algorithms are tested on LPF synthetic data. The test on realistic LPF data allows the effect of spectral data correlations on the efficiency of the different noise excess estimators to be highlighted. It also reveals the versatility of the Kolmogorov-Smirnov approach, which can be adapted to provide reasonable results on correlated data from a modified version of the standard equations for the inversion of the test statistic. Closely related to excess noise detection, the problem of noise parameter identification in non-Gaussian data is approached in two ways. One procedure is based on maximum likelihood estimator and another is based on the Kolmogorov-Smirnov goodness of fit estimator. Both approaches provide unbiased and accurate results for noise parameter estimation and demonstrate superior performance with respect to standard weighted least-squares and Huber's norm.

Journal ArticleDOI
22 Sep 2011
TL;DR: In this paper, the main LISA concepts are presented, in particular, emphasis will be placed on LISAPathFinder, the ESA precursor of LISA, in which our research group in Barcelona is heavily involved.
Abstract: Ground based GW detectors are limited at their lower frequency band (1-10 Hz) by settlement gravity gradients and seismic noise, and their sensitivity peaks at around 100 Hz. Sources in this band are mostly short duration signals, and their rates uncertain. Going down to milli-Hertz frequencies significantly increases the number and types of available sources. LISA was planned with the idea to explore a likely richer region of the GW spectrum, beyond that accessible to ground detectors; the latter are however expected to produce the first GW observations. In this paper I will present the main LISA concepts; in particular, emphasis will be placed on LISAPathFinder, the ESA precursor of LISA, in which our research group in Barcelona is heavily involved.

Posted Content
TL;DR: In this paper, the analysis of simulated LTP data is indicated that the major contribution to the force noise power spectral density uncertainties is coming from the statistical properties of the spectrum estimator.
Abstract: The analysis of the noise sources perturbing a test mass (TM) geodesic motion is the main scientific objective of the LISA Technology Package experiment (LTP) on board of the LISA Pathfinder space mission. Information on force noise acting on TMs are obtained with a data reduction procedure involving system parameters. Such parameters can be estimated from dedicated experimental runs. Therefore the final estimation of force noise is affected by two sources of uncertainty. One is statistical and connected to the random nature of noisy signals. The other is connected to the uncertainties on the system parameters. The analysis of simulated LTP data is indicating that the major contribution to the force noise power spectral density uncertainties is coming from the statistical properties of the spectrum estimator.


Journal ArticleDOI
TL;DR: The LISA Pathfinder data analysis toolbox as discussed by the authors allows all the data analysis functionalities for the mission, while storing the history of all operations performed to the data, thus easing traceability and reproducibility of the analysis.
Abstract: The LISA Pathfinder data analysis team has been developing in the last years the infrastructure and methods required to run the mission during flight operations. These are gathered in the LTPDA toolbox, an object oriented MATLAB toolbox that allows all the data analysis functionalities for the mission, while storing the history of all operations performed to the data, thus easing traceability and reproducibility of the analysis. The parameter estimation methods in the toolbox have been applied recently to data sets generated with the OSE (Off-line Simulations Environment), a detailed LISA Pathfinder non-linear simulator that will serve as a reference simulator during mission operations. These operational exercises aim at testing the on-orbit experiments in a realistic environment in terms of software and time constraints. These simulations, so called operational exercises, are the last verification step before translating these experiments into tele-command sequences for the spacecraft, producing therefore very relevant datasets to test our data analysis methods. In this contribution we report the results obtained with three different parameter estimation methods during one of these operational exercises.

Posted Content
TL;DR: In this article, the LTPDA Toolbox is used for non-linear analysis of the LISA Technology Package (LTP) in the framework of object-oriented MATLAB data analysis.
Abstract: The precursor ESA mission LISA-Pathfinder, to be flown in 2013, aims at demonstrating the feasibility of the free-fall, necessary for LISA, the upcoming space-born gravitational wave observatory. LISA Technology Package (LTP) is planned to carry out a number of experiments, whose main targets are to identify and measure the disturbances on each test-mass, in order to reach an unprecedented low-level residual force noise. To fulfill this plan, it is then necessary to correctly design, set-up and optimize the experiments to be performed on-flight and do a full system parameter estimation. Here we describe the progress on the non-linear analysis using the methods developed in the framework of the \textit{LTPDA Toolbox}, an object-oriented MATLAB Data Analysis environment: the effort is to identify the critical parameters and remove the degeneracy by properly combining the results of different experiments coming from a closed-loop system like LTP.