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22 results on '"Boatella, C."'

1. From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion

Author

Antonucci, F, Armano, M, Audley, H, Auger, G, Benedetti, M, Binetruy, P, Boatella, C, Bogenstahl, J, Bortoluzzi, D, Bosetti, P, Brandt, N, Caleno, M, Cavalleri, A, Cesa, M, Chmeissani, M, Ciani, G, Conchillo, A, Congedo, G, Cristofolini, I, Cruise, M, Danzmann, K, De Marchi, F, Diaz-Aguilo, M, Diepholz, I, Dixon, G, Dolesi, R, Dunbar, N, Fauste, J, Ferraioli, L, Fertin, D, Fichter, W, Fitzsimons, E, Freschi, M, Marin, A García, Marirrodriga, C García, Gerndt, R, Gesa, L, Giardini, D, Gibert, F, Grimani, C, Grynagier, A, Guillaume, B, Guzmán, F, Harrison, I, Heinzel, G, Hewitson, M, Hollington, D, Hough, J, Hoyland, D, Hueller, M, Huesler, J, Jeannin, O, Jennrich, O, Jetzer, P, Johlander, B, Killow, C, Llamas, X, Lloro, I, Lobo, A, Maarschalkerweerd, R, Madden, S, Mance, D, Mateos, I, McNamara, P W, Mendestì, J, Mitchell, E, Monsky, A, Nicolini, D, Nicolodi, D, Nofrarias, M, Pedersen, F, Perreur-Lloyd, M, Perreca, A, Plagnol, E, Prat, P, Racca, G D, Rais, B, Ramos-Castro, J, Reiche, J, Perez, J A Romera, Robertson, D, Rozemeijer, H, Sanjuan, J, Schleicher, A, Schulte, M, Shaul, D, Stagnaro, L, Strandmoe, S, Steier, F, Sumner, T J, Taylor, A, Texier, D, Trenkel, C, Tombolato, D, Vitale, S, Wanner, G, Ward, H, Waschke, S, Wass, P, Weber, W J, and Zweifel, P

Subjects
General Relativity and Quantum Cosmology, Astrophysics - Instrumentation and Methods for Astrophysics
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 and 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 two 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., Comment: Proceedings of the 8th LISA Symposium. To appear Class. Quantum Grav. 28 (2011)

Published
2010
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2. High-Energy Proton Testing of Sensitive Electronics for use on Modular Infrared Molecules and Ices Sensor (MIRMIS) Instrument

Author

Thirumangalath, S., Briede, E., Näsilä, A., Gupta, V., Boatella, C., Wojciech, H., Kletzl, V., Trops, R., and Bowles, N. E.

Subjects
modular infrared molecules, MIRMIS, Ices Sensor
Abstract

The Comet Interceptor (CI) mission is ESA's first "F" class mission, selected in June 2019. This mission consists of three spacecraft: Spacecraft A (main spacecraft), Spacecraft B1 (supplied by the Japanese space agency JAXA), and Spacecraft B2. In this paper, we highlight the Modular Infrared Molecular and Ices Sensor (MIRMIS) instrument, which is integrated into the CI Spacecraft A's scientific payload. In addition to hardware contributions from Finland (VTT Finland) and the UK (University of Oxford), the MIRMIS instrument team includes members from the University of Helsinki and NASA's Goddard Space Flight Centre. MIRMIS covers the spectral range of 0.9 to ~25 μm. This paper presents the preliminary high-proton-energy radiation test results of MIRMIS’ near-infrared detector arraysensitive electronic components. Proton beam testing is performed to estimate Single Event Effects (SEE) on the PCB boards and SEE and Total Non-Ionizing Dose (TNID)/ Displacement Damage (DD) on the detectors. The tests were conducted at the Paul Scherrer Institute (PSI) Proton Irradiation Facility (PIF), Villigen, Switzerland. The levels for the tests were based on the mission requirements for the ESA Comet Interceptor mission: 3 years (at 1 AU- Segment 1) and 2 years (at 0.9 AU- Segment 2). The DD levels from the analysis were equivalent to 1e11 protons/cm2 with an energy of 50 MeV. The electronics are exposed to high-energy protons causing Single Event Effects (SEE) which may induce potentially destructive and non-destructive effects. The test items primarily included the InGaAs image sensors (SCD Cardinal640, standard and low noise), Xilinx Spartan-6 FPGAs (Field Programmable Gate Arrays), and other proximity electronics. The proton energies were varied from 50 to 200 MeV, at fluxes of 106 to 108 particles/cm2/s. No events were observed on the standard Cardinal640 sensor at target fluences between 1.00E+10 to 1.00E+11 particles/cm2. FPGAs did not show any susceptibility to TNID at fluences up to 1.00E+11 (particles/cm2).

Published
2022

4. Direct Ionization Impact on Accelerator Mixed-Field Soft Error Rate

Author

Alía, R. G., Tali, M., Brugger, M., Cecchetto, M., Cerutti, F., Cononetti, A., Danzeca, S., Esposito, L., Fernández-Martínez, P., Gilardoni, S., Infantino, A., Kastriotou, M., Kerboub, N., Lerner, G., Wyrwoll, V., Ferlet-Cavrois, V., Boatella, C., Javanainen, A., Kettunen, H., Morilla, Y., Martín-Holgado, P., Gaillard, R., Wrobel, F., Cazzaniga, C., Alexandrescu, D., Glorieux, M., and Puchner, H.

Subjects
mikroelektroniikka, säteilyfysiikka, ionisoiva säteily
Abstract

We investigate, through measurements and simulations, the possible direct ionization impact in the accelerator soft error rate, not considered in standard qualification approaches. Results show that, for a broad variety of state-of-the art commercial components considered in the 65 nm to 16 nm technological range, indirect ionization is still expected to dominate the overall soft-error rate in the accelerator mixed-field. However, the derived critical charges of the most sensitive parts, corresponding to ∼0.7 fC, are expected to be at the limit of rapid direct ionization dominance and soft-error increase. peerReviewed

Published
2020

5. LISA Pathfinder: Mission and status

Author

Antonucci, F, Armano, M, Audley, H, Auger, G, Benedetti, M, Binetruy, P, Boatella, C, Bogenstahl, J, Bortoluzzi, D, Bosetti, P, Caleno, M, Cavalleri, A, Cesa, M, Chmeissani, M, Ciani, G, Conchillo, A, Congedo, G, Cristofolini, I, Cruise, M, Danzmann, K, De Marchi, F, Diaz-Aguilo, M, Diepholz, I, Dixon, G, and Dolesi, R

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. © 2011 IOP Publishing Ltd.

Published
2016

7. LISA Pathfinder: mission and status

Author

Antonucci, F, Armano, M, Audley, H, Auger, G, Benedetti, M, Binetruy, P, Boatella, C, Bogenstahl, J, Bortoluzzi, D, Bosetti, P, Caleno, M, Cavalleri, A, Cesa, M, Chmeissani, M, Ciani, G, Conchillo, A, Congedo, G, Cristofolini, I, Cruise, M, Danzmann, K, De Marchi, F, Diaz-Aguilo, M, Diepholz, I, Dixon, G, Dolesi, R, Dunbar, N, Fauste, J, Ferraioli, L, Fertin, D, Fichter, W, Fitzsimons, E, Freschi, M, Marin, AG, Marirrodriga, CG, Gerndt, R, Gesa, L, Gilbert, F, Giardini, D, Grimani, C, Grynagier, A, Guillaume, B, Guzmán, F, Harrison, I, Heinzel, G, Hewitson, M, Hollington, D, Hough, J, Hoyland, D, Hueller, M, Huesler, J, Jeannin, O, Jennrich, O, Jetzer, P, Johlander, B, Killow, C, Llamas, X, Lloro, I, Lobo, A, Maarschalkerweerd, R, Madden, S, Mance, D, Mateos, I, McNamara, PW, Mendes, J, Mitchell, E, Monsky, A, Nicolini, D, Nicolodi, D, Nofrarias, M, Pedersen, F, Perreur-Lloyd, M, Perreca, A, Plagnol, E, Prat, P, Racca, GD, Rais, B, Ramos-Castro, J, Reiche, J, Perez, JAR, Robertson, D, Rozemeijer, H, Sanjuan, J, Schleicher, A, Schulte, M, Shaul, D, Stagnaro, L, Strandmoe, S, Steier, F, Sumner, TJ, Taylor, A, Texier, D, Trenkel, C, Tombolato, D, Vitale, S, Wanner, G, Ward, H, Waschke, S, Wass, P, Weber, WJ, Zweifel, P, Gruppo Collegato di Trento, National Institute for Nuclear Physics ( INFN ), European Space Astronomy Centre, European Space Agency ( ESA ), Max-Planck-Institut für Gravitationsphysik, Universitat Hannover, AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Centre National d'Etudes Spatiales ( CNES ), European Space Technology Centre, IFAE, Universitat Autònoma de Barcelona [Barcelona] ( UAB ), Department of Physics [Gainesville], University of Florida [Gainesville], ICE, Institut d'Estudis Espacials de Catalunya ( IEEC-CSIC ), School of Physics and Astronomy [Birmingham], University of Birmingham [Birmingham], EPSC, Astrium Ltd, Institut für Flugmechanik und Flugregelung, Department of Physics and Astronomy, University of Glasgow, Astrium GmbH, Institut für Geophysik [Zürich], Eidgenössische Technische Hochschule [Zürich] ( ETH Zürich ), Istituto di Fisica, NASA Goddard Space Flight Center ( GSFC ), European Space Operations Centre, Blackett Laboratory, Imperial College London, Institut für Theoretische Physik, Universität Zürich [Zürich] ( UZH ), NTE-SENER, Departament d'Enginyeria Electrònica [Barcelona], Istituto Nazionale di Fisica Nucleare (INFN), European Space Astronomy Centre (ESAC), Agence Spatiale Européenne = European Space Agency (ESA), Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), European Space Research and Technology Centre (ESTEC), Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Institut d'Estudis Espacials de Catalunya (IEEC-CSIC), SUPA School of Physics and Astronomy [Glasgow], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), NASA Goddard Space Flight Center (GSFC), Universität Zürich [Zürich] = University of Zurich (UZH), National Institute for Nuclear Physics (INFN), European Space Agency (ESA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Universitat Autònoma de Barcelona [Barcelona] (UAB), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich), Universität Zürich [Zürich] (UZH), Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)

Subjects
Physics and Astronomy (miscellaneous), Physical Sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], ComputingMilieux_MISCELLANEOUS, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
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. © 2011 IOP Publishing Ltd.

Published
2011

8. In-flight Diagnostics in LISA Pathfinder

Author

Universitat Politècnica de Catalunya. Departament de Física Aplicada, Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica, Lobo Gutiérrez, José Alberto, Nofrarías, M., Ramos Castro, Juan José, Sanjuan, J., Conchillo, A, Ortega, J.A., Xirgu, X, Araujo, H., Boatella, C., Chmeissani, M., Grimani, C., Puigdengoles, C., Wass, P., García-Berro Montilla, Enrique, García, S., Martínez, L.M., Montero, G., Universitat Politècnica de Catalunya. Departament de Física Aplicada, Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica, Lobo Gutiérrez, José Alberto, Nofrarías, M., Ramos Castro, Juan José, Sanjuan, J., Conchillo, A, Ortega, J.A., Xirgu, X, Araujo, H., Boatella, C., Chmeissani, M., Grimani, C., Puigdengoles, C., Wass, P., García-Berro Montilla, Enrique, García, S., Martínez, L.M., and Montero, G.

Abstract

LISA PathFinder (LPF) will be flown with the objective to test in space key technologies for LISA. However its sensitivity goals are, for good reason, one order of magnitude less than those which LISA will have to meet, both in drag-free and optical metrology requirements, and in the observation frequency band. While the expected success of LPF will of course be of itself a major step forward to LISA, one might not forget that a further improvement by an order of magnitude in performance will still be needed. Clues for the last leap are to be derived from proper disentanglement of the various sources of noise which contribute to the total noise, as measured in flight during the PathFinder mission. This paper describes the principles, workings and requirements of one of the key tools to serve the above objective: the diagnostics subsystem. This consists in sets of temperature, magnetic field, and particle counter sensors, together with generators of controlled thermal and magnetic perturbations. At least during the commissioning phase, the latter will be used to identify feed-through coefficients between diagnostics sensor readings and associated actual noise contributions. A brief progress report of the current state of development of the diagnostics subsystem will be given as well., Peer Reviewed

Published
2006

11. The LISA Pathfinder interferometry—hardware and system testing

Author

Audley, H, primary, Danzmann, K, additional, Marín, A García, additional, Heinzel, G, additional, Monsky, A, additional, Nofrarias, M, additional, Steier, F, additional, Gerardi, D, additional, Gerndt, R, additional, Hechenblaikner, G, additional, Johann, U, additional, Luetzow-Wentzky, P, additional, Wand, V, additional, Antonucci, F, additional, Armano, M, additional, Auger, G, additional, Benedetti, M, additional, Binetruy, P, additional, Boatella, C, additional, Bogenstahl, J, additional, Bortoluzzi, D, additional, Bosetti, P, additional, Caleno, M, additional, Cavalleri, A, additional, Cesa, M, additional, Chmeissani, M, additional, Ciani, G, additional, Conchillo, A, additional, Congedo, G, additional, Cristofolini, I, additional, Cruise, M, additional, De Marchi, F, additional, Diaz-Aguilo, M, additional, Diepholz, I, additional, Dixon, G, additional, Dolesi, R, additional, Fauste, J, additional, Ferraioli, L, additional, Fertin, D, additional, Fichter, W, additional, Fitzsimons, E, additional, Freschi, M, additional, Marirrodriga, C García, additional, Gesa, L, additional, Gibert, F, additional, Giardini, D, additional, Grimani, C, additional, Grynagier, A, additional, Guillaume, B, additional, Guzmán, F, additional, Harrison, I, additional, Hewitson, M, additional, Hollington, D, additional, Hough, J, additional, Hoyland, D, additional, Hueller, M, additional, Huesler, J, additional, Jeannin, O, additional, Jennrich, O, additional, Jetzer, P, additional, Johlander, B, additional, Killow, C, additional, Llamas, X, additional, Lloro, I, additional, Lobo, A, additional, Maarschalkerweerd, R, additional, Madden, S, additional, Mance, D, additional, Mateos, I, additional, McNamara, P W, additional, Mendes, J, additional, Mitchell, E, additional, Nicolini, D, additional, Nicolodi, D, additional, Pedersen, F, additional, Perreur-Lloyd, M, additional, Perreca, A, additional, Plagnol, E, additional, Prat, P, additional, Racca, G D, additional, Rais, B, additional, Ramos-Castro, J, additional, Reiche, J, additional, Perez, J A Romera, additional, Robertson, D, additional, Rozemeijer, H, additional, Sanjuan, J, additional, Schulte, M, additional, Shaul, D, additional, Stagnaro, L, additional, Strandmoe, S, additional, Sumner, T J, additional, Taylor, A, additional, Texier, D, additional, Trenkel, C, additional, Tombolato, D, additional, Vitale, S, additional, Wanner, G, additional, Ward, H, additional, Waschke, S, additional, Wass, P, additional, Weber, W J, additional, and Zweifel, P, additional

Published
2011
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12. LISA Pathfinder data analysis

Author

Antonucci, F, primary, Armano, M, additional, Audley, H, additional, Auger, G, additional, Benedetti, M, additional, Binetruy, P, additional, Boatella, C, additional, Bogenstahl, J, additional, Bortoluzzi, D, additional, Bosetti, P, additional, Caleno, M, additional, Cavalleri, A, additional, Cesa, M, additional, Chmeissani, M, additional, Ciani, G, additional, Conchillo, A, additional, Congedo, G, additional, Cristofolini, I, additional, Cruise, M, additional, Danzmann, K, additional, De Marchi, F, additional, Diaz-Aguilo, M, additional, Diepholz, I, additional, Dixon, G, additional, Dolesi, R, additional, Fauste, J, additional, Ferraioli, L, additional, Fertin, D, additional, Fichter, W, additional, Fitzsimons, E, additional, Freschi, M, additional, Marin, A García, additional, Marirrodriga, C García, additional, Gesa, L, additional, Giardini, D, additional, Grimani, C, additional, Grynagier, A, additional, Guillaume, B, additional, Guzmán, F, additional, Harrison, I, additional, Heinzel, G, additional, Hewitson, M, additional, Hollington, D, additional, Hough, J, additional, Hoyland, D, additional, Hueller, M, additional, Huesler, J, additional, Jeannin, O, additional, Jennrich, O, additional, Jetzer, P, additional, Johlander, B, additional, Killow, C, additional, Llamas, X, additional, Lloro, I, additional, Lobo, A, additional, Maarschalkerweerd, R, additional, Madden, S, additional, Mance, D, additional, Mateos, I, additional, McNamara, P W, additional, Mendes, J, additional, Mitchell, E, additional, Monsky, A, additional, Nicolini, D, additional, Nicolodi, D, additional, Nofrarias, M, additional, Pedersen, F, additional, Perreur-Lloyd, M, additional, Perreca, A, additional, Plagnol, E, additional, Prat, P, additional, Racca, G D, additional, Rais, B, additional, Ramos-Castro, J, additional, Reiche, J, additional, Perez, J A Romera, additional, Robertson, D, additional, Rozemeijer, H, additional, Sanjuan, J, additional, Schulte, M, additional, Shaul, D, additional, Stagnaro, L, additional, Strandmoe, S, additional, Steier, F, additional, Sumner, T J, additional, Taylor, A, additional, Texier, D, additional, Trenkel, C, additional, Tombolato, D, additional, Vitale, S, additional, Wanner, G, additional, Ward, H, additional, Waschke, S, additional, Wass, P, additional, Weber, W J, additional, and Zweifel, P, additional

Published
2011
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13. From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion

Author

Antonucci, F, primary, Armano, M, additional, Audley, H, additional, Auger, G, additional, Benedetti, M, additional, Binetruy, P, additional, Boatella, C, additional, Bogenstahl, J, additional, Bortoluzzi, D, additional, Bosetti, P, additional, Brandt, N, additional, Caleno, M, additional, Cavalleri, A, additional, Cesa, M, additional, Chmeissani, M, additional, Ciani, G, additional, Conchillo, A, additional, Congedo, G, additional, Cristofolini, I, additional, Cruise, M, additional, Danzmann, K, additional, De Marchi, F, additional, Diaz-Aguilo, M, additional, Diepholz, I, additional, Dixon, G, additional, Dolesi, R, additional, Dunbar, N, additional, Fauste, J, additional, Ferraioli, L, additional, Fertin, D, additional, Fichter, W, additional, Fitzsimons, E, additional, Freschi, M, additional, García Marin, A, additional, Marirrodriga, C García, additional, Gerndt, R, additional, Gesa, L, additional, Giardini, D, additional, Gibert, F, additional, Grimani, C, additional, Grynagier, A, additional, Guillaume, B, additional, Guzmán, F, additional, Harrison, I, additional, Heinzel, G, additional, Hewitson, M, additional, Hollington, D, additional, Hough, J, additional, Hoyland, D, additional, Hueller, M, additional, Huesler, J, additional, Jeannin, O, additional, Jennrich, O, additional, Jetzer, P, additional, Johlander, B, additional, Killow, C, additional, Llamas, X, additional, Lloro, I, additional, Lobo, A, additional, Maarschalkerweerd, R, additional, Madden, S, additional, Mance, D, additional, Mateos, I, additional, McNamara, P W, additional, Mendes, J, additional, Mitchell, E, additional, Monsky, A, additional, Nicolini, D, additional, Nicolodi, D, additional, Nofrarias, M, additional, Pedersen, F, additional, Perreur-Lloyd, M, additional, Perreca, A, additional, Plagnol, E, additional, Prat, P, additional, Racca, G D, additional, Rais, B, additional, Ramos-Castro, J, additional, Reiche, J, additional, Perez, J A Romera, additional, Robertson, D, additional, Rozemeijer, H, additional, Sanjuan, J, additional, Schleicher, A, additional, Schulte, M, additional, Shaul, D, additional, Stagnaro, L, additional, Strandmoe, S, additional, Steier, F, additional, Sumner, T J, additional, Taylor, A, additional, Texier, D, additional, Trenkel, C, additional, Tombolato, D, additional, Vitale, S, additional, Wanner, G, additional, Ward, H, additional, Waschke, S, additional, Wass, P, additional, Weber, W J, additional, and Zweifel, P, additional

Published
2011
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15. LISAandLISA PathFinder, the endeavour to detect low frequency GWs

Author

Araújo, H, primary, Boatella, C, additional, Chmeissani, M, additional, Conchillo, A, additional, García-Berro, E, additional, Grimani, C, additional, Hajdas, W, additional, Lobo, A, additional, Martínez, Ll, additional, Nofrarias, M, additional, Ortega, J A, additional, Puigdengoles, C, additional, Ramos-Castro, J, additional, Sanjuán, J, additional, Wass, P, additional, and Xirgu, X, additional

Published
2007
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16. The LISA Pathfinder Radiation Monitor

Author

Wass, P. J., primary, Araújo, H., additional, Boatella, C., additional, Chmeissani, M., additional, Hajdas, W., additional, Lobo, A., additional, Puigdengoles, C., additional, and Sumner, T., additional

Published
2006
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18. In-flight Diagnostics in LISA Pathfinder

Author

Lobo, A., primary, Nofrarias, M., additional, Ramos-Castro, J., additional, Sanjuan, J., additional, Conchillo, A., additional, Ortega, J. A., additional, Xirgu, X., additional, Araujo, H., additional, Boatella, C., additional, Chmeissani, M., additional, Grimani, C., additional, Puigdengoles, C., additional, Wass, P., additional, García-Berro, E., additional, García, S., additional, Martínez, L. M., additional, and Montero, G., additional

Published
2006
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19. The LTP experiment on the LISA Pathfinder mission

Author

Anza, S, primary, Armano, M, additional, Balaguer, E, additional, Benedetti, M, additional, Boatella, C, additional, Bosetti, P, additional, Bortoluzzi, D, additional, Brandt, N, additional, Braxmaier, C, additional, Caldwell, M, additional, Carbone, L, additional, Cavalleri, A, additional, Ciccolella, A, additional, Cristofolini, I, additional, Cruise, M, additional, Lio, M Da, additional, Danzmann, K, additional, Desiderio, D, additional, Dolesi, R, additional, Dunbar, N, additional, Fichter, W, additional, Garcia, C, additional, Garcia-Berro, E, additional, Marin, A F Garcia, additional, Gerndt, R, additional, Gianolio, A, additional, Giardini, D, additional, Gruenagel, R, additional, Hammesfahr, A, additional, Heinzel, G, additional, Hough, J, additional, Hoyland, D, additional, Hueller, M, additional, Jennrich, O, additional, Johann, U, additional, Kemble, S, additional, Killow, C, additional, Kolbe, D, additional, Landgraf, M, additional, Lobo, A, additional, Lorizzo, V, additional, Mance, D, additional, Middleton, K, additional, Nappo, F, additional, Nofrarias, M, additional, Racca, G, additional, Ramos, J, additional, Robertson, D, additional, Sallusti, M, additional, Sandford, M, additional, Sanjuan, J, additional, Sarra, P, additional, Selig, A, additional, Shaul, D, additional, Smart, D, additional, Smit, M, additional, Stagnaro, L, additional, Sumner, T, additional, Tirabassi, C, additional, Tobin, S, additional, Vitale, S, additional, Wand, V, additional, Ward, H, additional, Weber, W J, additional, and Zweifel, P, additional

Published
2005
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20. Data and Diagnostics in LISA PathFinder.

Author

Lobo, A., Nofrarias, M., Ramos, J., Sanjuan, J., Conchillo, A., Ortega, J. A., Xirgu, X., Araujo, H., Boatella, C., Chmeissani, M., Grimani, C., Puigdengoles, C., Wass, P., Anza, S., Díaz Michelena, M., García-Berro, E., and Pérez del Real, R.

Subjects
GRAVITY waves, ASTRONOMICAL perturbation, GRAVITY, HYDRODYNAMICS, PHYSICS
Abstract

The Diagnostics measurement set is a subsystem of the LTP which is intended to monitor a number of spurious disturbances, even if the satellite complies with all cleanliness requirements. It monitors thermal and magnetic perturbations, and incorporates a charged particle counter. The purpose of this communication is to discuss the conceptual aspects of the mentioned subsystem, and to summarise its current status of development. © 2006 American Institute of Physics [ABSTRACT FROM AUTHOR]

Published
2006
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22. SEP flux mapping with PHOEBUS.

Author

Grimani, C., Bagni, G., Fabi, M., Vicerè, A., Marconi, L., Stanga, R., Bosi, L., Vocca, H., Araújo, H., Shaul, D., Sumner, T., Wass, P., Boatella, C., Lobo, A., Chmeissani, M., and Martinez, I.

Published
2006
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