273 results on '"Malaspina M"'
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2. Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance
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Mennella, A., Bersanelli, M., Butler, R. C., Curto, A., Cuttaia, F., Davis, R. J., Dick, J., Frailis, M., Galeotta, S., Gregorio, A., Kurki-Suonio, H., Lawrence, C. R., Leach, S., Leahy, J. P., Lowe, S., Maino, D., Mandolesi, N., Maris, M., Martínez-González, E., Meinhold, P. R., Morgante, G., Pearson, D., Perrotta, F., Polenta, G., Poutanen, T., Sandri, M., Seiffert, M. D., Suur-Uski, A. -S., Tavagnacco, D., Terenzi, L., Tomasi, M., Valiviita, J., Villa, F., Watson, R., Wilkinson, A., Zacchei, A., Zonca, A., Aja, B., Artal, E., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., Battaglia, P., Bennett, K., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F. R., Burigana, C., Cabella, P., Cappellini, B., Chen, X., Colombo, L., Cruz, M., Danese, L., D'Arcangelo, O., Davies, R. D., de Gasperis, G., de Rosa, A., de Zotti, G., Dickinson, C., Diego, J. M., Donzelli, S., Efstathiou, G., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Foley, S., Franceschet, C., Franceschi, E., Gaier, T. C., Génova-Santos, R. T., George, D., Gómez, F., González-Nuevo, J., Górski, K. M., Gruppuso, A., Hansen, F. K., Herranz, D., Herreros, J. M., Hoyland, R. J., Hughes, N., Jewell, J., Jukkala, P., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kilpia, V. -H., Kisner, T. S., Knoche, J., Knox, L., Laaninen, M., Lähteenmäki, A., Lamarre, J. -M., Leonardi, R., León-Tavares, J., Leutenegger, P., Lilje, P. B., López-Caniego, M., Lubin, P. M., Malaspina, M., Marinucci, D., Massardi, M., Matarrese, S., Matthai, F., Melchiorri, A., Mendes, L., Miccolis, M., Migliaccio, M., Mitra, S., Moss, A., Natoli, P., Nesti, R., Nørgaard-Nielsen, H. U., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Pettorino, V., Pietrobon, D., Pospieszalski, M., Prézeau, G., Prina, M., Procopio, P., Puget, J. -L., Quercellini, C., Rachen, J. P., Rebolo, R., Reinecke, M., Ricciardi, S., Robbers, G., Rocha, G., Roddis, N., Rubiño-Martín, J. A., Savelainen, M., Scott, D., Silvestri, R., Simonetto, A., Sjoman, P., Smoot, G. F., Sozzi, C., Stringhetti, L., Tauber, J. A., Tofani, G., Toffolatti, L., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Varis, J., Vielva, P., Vittorio, N., Wade, L. A., Watson, C., White, S. D. M., and Winder, F.
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Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit operation is presented. We describe the main optical parameters and discuss photometric calibration, white noise sensitivity, and noise properties. A preliminary evaluation of the impact of the main systematic effects is presented. For each of the performance parameters, we outline the methods used to obtain them from the flight data and provide a comparison with pre-launch ground assessments, which are essentially confirmed in flight., Comment: Published version
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- 2011
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3. Planck pre-launch status: calibration of the Low Frequency Instrument flight model radiometers
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Villa, F., Terenzi, L., Sandri, M., Meinhold, P., Poutanen, T., Battaglia, P., Franceschet, C., Hughes, N., Laaninen, M., Lapolla, P., Bersanelli, M., Butler, R. C., Cuttaia, F., D'Arcangelo, O., Frailis, M., Franceschi, E., Galeotta, S., Gregorio, A., Leonardi, R., Lowe, S. R., Mandolesi, N., Maris, M., Mendes, L., Mennella, A., Morgante, G., Stringhetti, L., Tomasi, M., Valenziano, L., Zacchei, A., Zonca, A., Aja, B., Artal, E., Balasini, M., Bernardino, T., Blackhurst, E., Boschini, L., Cappellini, B., Cavaliere, F., Colin, A., Colombo, F., Davis, R. J., De La Fuente, L., Edgeley, J., Gaier, T., Galtress, A., Hoyland, R., Jukkala, P., Kettle, D., Kilpia, V-H., Lawrence, C. R., Lawson, D., Leahy, J. P., Leutenegger, P., Levin, S., Maino, D., Malaspina, M., Mediavilla, A., Miccolis, M., Pagan, L., Pascual, J. P., Pasian, F., Pecora, M., Pospieszalski, M., Roddis, N., Salmon, M. J., Seiffert, M., Silvestri, R., Simonetto, A., Sjoman, P., Sozzi, C., Tuovinen, J., Varis, J., Wilkinson, A., and Winder, F.
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The Low Frequency Instrument (LFI) on-board the ESA Planck satellite carries eleven radiometer subsystems, called Radiometer Chain Assemblies (RCAs), each composed of a pair of pseudo-correlation receivers. We describe the on-ground calibration campaign performed to qualify the flight model RCAs and to measure their pre-launch performances. Each RCA was calibrated in a dedicated flight-like cryogenic environment with the radiometer front-end cooled to 20K and the back-end at 300K, and with an external input load cooled to 4K. A matched load simulating a blackbody at different temperatures was placed in front of the sky horn to derive basic radiometer properties such as noise temperature, gain, and noise performance, e.g. 1/f noise. The spectral response of each detector was measured as was their susceptibility to thermal variation. All eleven LFI RCAs were calibrated. Instrumental parameters measured in these tests, such as noise temperature, bandwidth, radiometer isolation, and linearity, provide essential inputs to the Planck-LFI data analysis., Comment: 15 pages, 18 figures. Accepted for publication in Astronomy and Astrophysics
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- 2010
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4. A systematic approach to the Planck LFI end-to-end test and its application to the DPC Level 1 pipeline
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Frailis, M., Maris, M., Zacchei, A., Morisset, N., Rohlfs, R., Meharga, M., Binko, P., Turler, M., Galeotta, S., Gasparo, F., Franceschi, E., Butler, R. C., D'Arcangelo, O., Fogliani, S., Gregorio, A., Lowe, S. R., Maggio, G., Malaspina, M., Mandolesi, N., Manzato, P., Pasian, F., Perrotta, F., Sandri, M., Terenzi, L., Tomasi, M., and Zonca, A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
The Level 1 of the Planck LFI Data Processing Centre (DPC) is devoted to the handling of the scientific and housekeeping telemetry. It is a critical component of the Planck ground segment which has to strictly commit to the project schedule to be ready for the launch and flight operations. In order to guarantee the quality necessary to achieve the objectives of the Planck mission, the design and development of the Level 1 software has followed the ESA Software Engineering Standards. A fundamental step in the software life cycle is the Verification and Validation of the software. The purpose of this work is to show an example of procedures, test development and analysis successfully applied to a key software project of an ESA mission. We present the end-to-end validation tests performed on the Level 1 of the LFI-DPC, by detailing the methods used and the results obtained. Different approaches have been used to test the scientific and housekeeping data processing. Scientific data processing has been tested by injecting signals with known properties directly into the acquisition electronics, in order to generate a test dataset of real telemetry data and reproduce as much as possible nominal conditions. For the HK telemetry processing, validation software have been developed to inject known parameter values into a set of real housekeeping packets and perform a comparison with the corresponding timelines generated by the Level 1. With the proposed validation and verification procedure, where the on-board and ground processing are viewed as a single pipeline, we demonstrated that the scientific and housekeeping processing of the Planck-LFI raw data is correct and meets the project requirements., Comment: 20 pages, 7 figures; this paper is part of the Prelaunch status LFI papers published on JINST: http://www.iop.org/EJ/journal/-page=extra.proc5/jinst
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- 2010
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5. LFI Radiometric Chain Assembly (RCA) data handling 'Rachel'
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Malaspina, M., Franceschi, E., Battaglia, P., Binko, P., Butler, R. C., D'Arcangelo, O., Fogliani, S., Frailis, M., Franceschet, C., Galeotta, S., Gasparo, F., Gregorio, A., Lapolla, M., Leonardi, R., Maggio, G., Mandolesi, N., Manzato, P., Maris, M., Meharga, M., Meinhold, P., Morisset, N., Pasian, F., Perrotta, F., Rohlfs, R., Sandri, M., Tomasi, M., Turler, M., Zacchei, A., and Zonca, A.
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
This paper is part of the Prelaunch status LFI papers published on JINST (http://www.iop.org/EJ/journal/-page=extra.proc5/1748-0221). Planck's Low Frequency Instrument is an array of 22 pseudo-correlation radiometers at 30, 44, and 70 GHz. Before integrating the overall array assembly, a first set of tests has been performed for each radiometer chain assembly (RCA), consisting of two radiometers. In this paper, we describe Rachel, a software application which has been purposely developed and used during the RCA test campaign to carry out both near-realtime on-line data analysis and data storage (in FITS format) of the raw output from the radiometric chains., Comment: This is an author-created, un-copyedited version of an article accepted for publication in JINST. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The definitive publisher authenticated version is available online at http://dx.doi.org/10.1088/1748-0221/4/12/T12017
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- 2010
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6. Level 1 on-ground telemetry handling in Planck LFI
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Zacchei, A., Frailis, M., Maris, M., Morisset, N., Rohlfs, R., Meharga, M., Binko, P., Turler, M., Galeotta, S., Gasparo, F., Franceschi, E., Butler, R. C., Cuttaia, F., D'Arcangelo, O., Fogliani, S., Gregorio, A., Leonardi, R., Lowe, S. R., Maino, D., Maggio, G., Malaspina, M., Mandolesi, N., Manzato, P., Meinhold, P., Mendes, L., Mennella, A., Morgante, G., Pasian, F., Perrotta, F., Sandri, M., Stringhetti, L., Terenzi, L., Tomasi, M., and Zonca, A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
The Planck Low Frequency Instrument (LFI) will observe the Cosmic Microwave Background (CMB) by covering the frequency range 30-70 GHz in three bands. The primary instrument data source are the temperature samples acquired by the 22 radiometers mounted on the Planck focal plane. Such samples represent the scientific data of LFI. In addition, the LFI instrument generates the so called housekeeping data by sampling regularly the on-board sensors and registers. The housekeeping data provides information on the overall health status of the instrument and on the scientific data quality. The scientific and housekeeping data are collected on-board into telemetry packets compliant with the ESA Packet Telemetry standards. They represent the primary input to the first processing level of the LFI Data Processing Centre. In this work we show the software systems which build the LFI Level 1. A real-time assessment system, based on the ESA SCOS 2000 generic mission control system, has the main purpose of monitoring the housekeeping parameters of LFI and detect possible anomalies. A telemetry handler system processes the housekeeping and scientific telemetry of LFI, generating timelines for each acquisition chain and each housekeeping parameter. Such timelines represent the main input to the subsequent processing levels of the LFI DPC. A telemetry quick-look system allows the real-time visualization of the LFI scientific and housekeeping data, by also calculating quick statistical functions and fast Fourier transforms. The LFI Level 1 has been designed to support all the mission phases, from the instrument ground tests and calibration to the flight operations, and developed according to the ESA engineering standards., Comment: This paper is part of the Prelaunch status LFI papers published on JINST: http://www.iop.org/EJ/journal/-page=extra.proc5/jinst
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- 2010
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7. Design, development, and verification of the Planck Low Frequency Instrument 70 GHz Front-End and Back-End Modules
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Varis, J., Hughes, N. J., Laaninen, M., Kilpia, V. -H., Jukkala, P., Tuovinen, J., Ovaska, S., Sjoman, P., Kangaslahti, P., Gaier, T., Hoyland, R., Meinhold, P., Mennella, A., Bersanelli, M., Butler, R. C., Cuttaia, F., Franceschi, E., Leonardi, R., Leutenegger, P., Malaspina, M., Mandolesi, N., Miccolis, M., Poutanen, T., Kurki-Suonio, H., Sandri, M., Stringhetti, L., Terenzi, L., Tomasi, M., and Valenziano, L.
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
70 GHz radiometer front-end and back-end modules for the Low Frequency Instrument of the European Space Agencys Planck Mission were built and tested. The operating principles and the design details of the mechanical structures are described along with the key InP MMIC low noise amplifiers and phase switches of the units. The units were tested in specially designed cryogenic vacuum chambers capable of producing the operating conditions required for Planck radiometers, specifically, a physical temperature of 20 K for the front-end modules, 300 K for the back-end modules and 4 K for the reference signal sources. Test results of the low noise amplifiers and phase switches, the front and back-end modules, and the combined results of both modules are discussed. At 70 GHz frequency, the system noise temperature of the front and back end is 28 K; the effective bandwidth 16 GHz, and the 1/f spectrum knee frequency is 38 mHz. The test results indicate state-of-the-art performance at 70 GHz frequency and fulfil the Planck performance requirements., Comment: 16 pages, 15 figures. This paper is part of of the prelaunch status Planck LFI papers published on JINST: http://www.iop.org/EJ/journal/-page=extra.proc5/jinst
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- 2010
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8. Off-line radiometric analysis of Planck/LFI data
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Tomasi, M., Mennella, A., Galeotta, S., Lowe, S. R., Mendes, L., Leonardi, R., Villa, F., Cappellini, B., Gregorio, A., Meinhold, P., Sandri, M., Cuttaia, F., Terenzi, L., Maris, M., Valenziano, L., Salmon, M. J., Bersanelli, M., Binko, P., Butler, R. C., D'Arcangelo, O., Fogliani, S., Frailis, M., Franceschi, E., Gasparo, F., Maggio, G., Maino, D., Malaspina, M., Mandolesi, N., Manzato, P., Meharga, M., Morgante, G., Morisset, N., Pasian, F., Perrotta, F., Rohlfs, R., Turler, M., Zacchei, A., and Zonca, A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
The Planck Low Frequency Instrument (LFI) is an array of 22 pseudo-correlation radiometers on-board the Planck satellite to measure temperature and polarization anisotropies in the Cosmic Microwave Background (CMB) in three frequency bands (30, 44 and 70 GHz). To calibrate and verify the performances of the LFI, a software suite named LIFE has been developed. Its aims are to provide a common platform to use for analyzing the results of the tests performed on the single components of the instrument (RCAs, Radiometric Chain Assemblies) and on the integrated Radiometric Array Assembly (RAA). Moreover, its analysis tools are designed to be used during the flight as well to produce periodic reports on the status of the instrument. The LIFE suite has been developed using a multi-layered, cross-platform approach. It implements a number of analysis modules written in RSI IDL, each accessing the data through a portable and heavily optimized library of functions written in C and C++. One of the most important features of LIFE is its ability to run the same data analysis codes both using ground test data and real flight data as input. The LIFE software suite has been successfully used during the RCA/RAA tests and the Planck Integrated System Tests. Moreover, the software has also passed the verification for its in-flight use during the System Operations Verification Tests, held in October 2008., Comment: Planck LFI technical papers published by JINST: http://www.iop.org/EJ/journal/-page=extra.proc5/1748-0221
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- 2010
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9. Noise Properties of the Planck-LFI Receivers
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Meinhold, P., Leonardi, R., Aja, B., Artal, E., Battaglia, P., Bersanelli, M., Blackhurst, E., Butler, C. R., Cuevas, L. P., Cuttaia, F., D'Arcangelo, O., Davis, R., de la Fuente, M. L., Frailis, M., Franceschet, C., Franceschi, E., Gaier, T., Galeotta, S., Gregorio, A., Hoyland, R., Hughes, N., Jukkala, P., Kettle, D., Laaninen, M., Leutenegger, P., Lowe, S. R., Malaspina, M., Mandolesi, R., Maris, M., Martínez-González, E., Mendes, L., Mennella, A., Miccolis, M., Morgante, G., Roddis, N., Sandri, M., Seiffert, M., Salmón, M., Stringhetti, L., Poutanen, T., Terenzi, L., Tomasi, M., Tuovinen, J., Varis, J., Valenziano, L., Villa, F., Wilkinson, A., Winder, F., Zacchei, A., and Zonca, A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
The Planck Low Frequency Instrument (LFI) radiometers have been tested extensively during several dedicated campaigns. The present paper reports the principal noise properties of the LFI radiometers., Comment: this paper is part of the Prelaunch status LFI papers published on JINST: http://www.iop.org/EJ/journal/-page=extra.proc5/jinst
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- 2010
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10. Optimization of Planck/LFI on--board data handling
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Maris, M., Tomasi, M., Galeotta, S., Miccolis, M., Hildebrandt, S., Frailis, M., Rohlfs, R., Morisset, N., Zacchei, A., Bersanelli, M., Binko, P., Burigana, C., Butler, R. C., Cuttaia, F., Chulani, H., D'Arcangelo, O., Fogliani, S., Franceschi, E., Gasparo, F., Gomez, F., Gregorio, A., Herreros, J. M., Leonardi, R., Leutenegger, P., Maggio, G., Maino, D., Malaspina, M., Mandolesi, N., Manzato, P., Meharga, M., Meinhold, P., Mennella, A., Pasian, F., Perrotta, F., Rebolo, R., Turler, M., and Zonca, A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Computer Science - Information Theory - Abstract
To asses stability against 1/f noise, the Low Frequency Instrument (LFI) onboard the Planck mission will acquire data at a rate much higher than the data rate allowed by its telemetry bandwith of 35.5 kbps. The data are processed by an onboard pipeline, followed onground by a reversing step. This paper illustrates the LFI scientific onboard processing to fit the allowed datarate. This is a lossy process tuned by using a set of 5 parameters Naver, r1, r2, q, O for each of the 44 LFI detectors. The paper quantifies the level of distortion introduced by the onboard processing, EpsilonQ, as a function of these parameters. It describes the method of optimizing the onboard processing chain. The tuning procedure is based on a optimization algorithm applied to unprocessed and uncompressed raw data provided either by simulations, prelaunch tests or data taken from LFI operating in diagnostic mode. All the needed optimization steps are performed by an automated tool, OCA2, which ends with optimized parameters and produces a set of statistical indicators, among them the compression rate Cr and EpsilonQ. For Planck/LFI the requirements are Cr = 2.4 and EpsilonQ <= 10% of the rms of the instrumental white noise. To speedup the process an analytical model is developed that is able to extract most of the relevant information on EpsilonQ and Cr as a function of the signal statistics and the processing parameters. This model will be of interest for the instrument data analysis. The method was applied during ground tests when the instrument was operating in conditions representative of flight. Optimized parameters were obtained and the performance has been verified, the required data rate of 35.5 Kbps has been achieved while keeping EpsilonQ at a level of 3.8% of white noise rms well within the requirements., Comment: 51 pages, 13 fig.s, 3 tables, pdflatex, needs JINST.csl, graphicx, txfonts, rotating; Issue 1.0 10 nov 2009; Sub. to JINST 23Jun09, Accepted 10Nov09, Pub.: 29Dec09; This is a preprint, not the final version
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- 2010
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11. Planck pre-launch status: Low Frequency Instrument calibration and expected scientific performance
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Mennella, A., Bersanelli, M., Butler, R. C., Cuttaia, F., D'Arcangelo, O., Davis, R. J., Frailis, M., Galeotta, S., Gregorio, A., Lawrence, C. R., Leonardi, R., Lowe, S. R., Mandolesi, N., Maris, M., Meinhold, P., Mendes, L., Morgante, G., Sandri, M., Stringhetti, L., Terenzi, L., Tomasi, M., Valenziano, L., Villa, F., Zacchei, A., Zonca, A., Balasini, M., Franceschet, C., Battaglia, P., Lapolla, P. M., Leutenegger, P., Miccolis, M., Pagan, L., Silvestri, R., Aja, B., Artal, E., Baldan, G., Bastia, P., Bernardino, T., Boschini, L., Cafagna, G., Cappellini, B., Cavaliere, F., Colombo, F., de La Fuente, L., Edgeley, J., Falvella, M. C., Ferrari, F., Fogliani, S., Franceschi, E., Gaier, T., Gomez, F., Herreros, J. M., Hildebrandt, S., Hoyland, R., Hughes, N., Jukkala, P., Kettle, D., Laaninen, M., Lawson, D., Leahy, P., Levin, S., Lilje, P. B., Maino, D., Malaspina, M., Manzato, P., Marti-Canales, J., Martinez-Gonzalez, E., Mediavilla, A., Pasian, F., Pascual, J. P., Pecora, M., Peres-Cuevas, L., Platania, P., Pospieszalsky, M., Poutanen, T., Rebolo, R., Roddis, N., Salmon, M., Seiffert, M., Simonetto, A., Sozzi, C., Tauber, J., Tuovinen, J., Varis, J., Wilkinson, A., and Winder, F.
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Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
We give the calibration and scientific performance parameters of the Planck Low Frequency Instrument (LFI) measured during the ground cryogenic test campaign. These parameters characterise the instrument response and constitute our best pre-launch knowledge of the LFI scientific performance. The LFI shows excellent $1/f$ stability and rejection of instrumental systematic effects; measured noise performance shows that LFI is the most sensitive instrument of its kind. The set of measured calibration parameters will be updated during flight operations through the end of the mission., Comment: Accepted for publications in Astronomy and Astrophysics. Astronomy & Astrophysics, 2010 (acceptance date: 12 Jan 2010)
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- 2010
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12. Planck pre-launch status: Design and description of the Low Frequency Instrument
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Bersanelli, M., Mandolesi, N., Butler, R. C., Mennella, A., Villa, F., Aja, B., Artal, E., Artina, E., Baccigalupi, C., Balasini, M., Baldan, G., Banday, A., Bastia, P., Battaglia, P., Bernardino, T., Blackhurst, E., Boschini, L., Burigana, C., Cafagna, G., Cappellini, B., Cavaliere, F., Colombo, F., Crone, G., Cuttaia, F., D'Arcangelo, O., Danese, L., Davies, R. D., Davis, R. J., De Angelis, L., De Gasperis, G. C., De La Fuente, L., De Rosa, A., De Zotti, G., Falvella, M. C., Ferrari, F., Ferretti, R., Figini, L., Fogliani, S., Franceschet, C., Franceschi, E., Gaier, T., Garavaglia, S., Gomez, F., Gorski, K., Gregorio, A., Guzzi, P., Herreros, J. M., Hildebrandt, S. R., Hoyland, R., Hughes, N., Janssen, M., Jukkala, P., Kettle, D., Kilpia, V. H., Laaninen, M., Lapolla, P. M., Lawrence, C. R., Leahy, J. P., Leonardi, R., Leutenegger, P., Levin, S., Lilje, P. B., Lowe, S. R., Lubin, D. Lawson P. M., Maino, D., Malaspina, M., Maris, M., Marti-Canales, J., Martinez-Gonzalez, E., Mediavilla, A., Meinhold, P., Miccolis, M., Morgante, G., Natoli, P., Nesti, R., Pagan, L., Paine, C., Partridge, B., Pascual, J. P., Pasian, F., Pearson, D., Pecora, M., Perrotta, F., Platania, P., Pospieszalski, M., Poutanen, T., Prina, M., Rebolo, R., Roddis, N., Rubino-Martin, J. A., Salmon, n M. J., Sandri, M., Seiffert, M., Silvestri, R., Simonetto, A., Sjoman, P., Smoot, G. F., Sozzi, C., Stringhetti, L., Taddei, E., Tauber, J., Terenzi, L., Tomasi, M., Tuovinen, J., Valenziano, L., Varis, J., Vittorio, N., Wade, L. A., Wilkinson, A., Winder, F., Zacchei, A., and Zonca, A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
In this paper we present the Low Frequency Instrument (LFI), designed and developed as part of the Planck space mission, the ESA program dedicated to precision imaging of the cosmic microwave background (CMB). Planck-LFI will observe the full sky in intensity and polarisation in three frequency bands centred at 30, 44 and 70 GHz, while higher frequencies (100-850 GHz) will be covered by the HFI instrument. The LFI is an array of microwave radiometers based on state-of-the-art Indium Phosphide cryogenic HEMT amplifiers implemented in a differential system using blackbody loads as reference signals. The front-end is cooled to 20K for optimal sensitivity and the reference loads are cooled to 4K to minimise low frequency noise. We provide an overview of the LFI, discuss the leading scientific requirements and describe the design solutions adopted for the various hardware subsystems. The main drivers of the radiometric, optical and thermal design are discussed, including the stringent requirements on sensitivity, stability, and rejection of systematic effects. Further details on the key instrument units and the results of ground calibration are provided in a set of companion papers., Comment: 23 pages, 31 figures, accepted by Astronomy and Astrophysics, Planck LFI technical papers published by JINST: http://www.iop.org/EJ/journal/-page=extra.proc5/1748-0221
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- 2010
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13. Planck pre-launch status: the Planck-LFI programme
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Mandolesi, N., Bersanelli, M., Butler, R. C., Artal, E., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Bartelmann, M., Bennett, K., Bhandari, P., Bonaldi, A., Borrill, J., Bremer, M., Burigana, C., Bowman, R. C., Cabella, P., Cantalupo, C., Cappellini, B., Courvoisier, T., Crone, G., Cuttaia, F., Danese, L., D'Arcangelo, O., Davies, R. D., Davis, R. J., De Angelis, L., de Gasperis, G., De Rosa, A., De Troia, G., de Zotti, G., Dick, J., Dickinson, C., Diego, J. M., Donzelli, S., Dörl, U., Dupac, X., Enßlin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Frailis, M., Franceschi, E., Gaier, T., Galeotta, S., Gasparo, F., Giardino, G., Gomez, F., Gonzalez-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Hansen, F., Hell, R., Herranz, D., Herreros, J. M., Hildebrandt, S., Hovest, W., Hoyland, R., Huffenberger, K., Janssen, M., Jaffe, T., Keihänen, E., Keskitalo, R., Kisner, T., Kurki-Suonio, H., Lähteenmäki, A., Lawrence, C. R., Leach, S. M., Leahy, J. P., Leonardi, R., Levin, S., Lilje, P. B., López-Caniego, M., Lowe, S. R., Lubin, P. M., Maino, D., Malaspina, M., Maris, M., Marti-Canales, J., Martinez-Gonzalez, E., Massardi, M., Matarrese, S., Matthai, F., Meinhold, P., Melchiorri, A., Mendes, L., Mennella, A., Morgante, G., Morigi, G., Morisset, N., Moss, A., Nash, A., Natoli, P., Nesti, R., Paine, C., Partridge, B., Pasian, F., Passvogel, T., Pearson, D., Pérez-Cuevas, L., Perrotta, F., Polenta, G., Popa, L. A., Poutanen, T., Prezeau, G., Prina, M., Rachen, J. P., Rebolo, R., Reinecke, M., Ricciardi, S., Riller, T., Rocha, G., Roddis, N., Rohlfs, R., Rubiño-Martin, J. A., Salerno, E., Sandri, M., Scott, D., Seiffert, M., Silk, J., Simonetto, A., Smoot, G. F., Sozzi, C., Sternberg, J., Stivoli, F., Stringhetti, L., Tauber, J., Terenzi, L., Tomasi, M., Tuovinen, J., Türler, M., Valenziano, L., Varis, J., Vielva, P., Villa, F., Vittorio, N., Wade, L., White, M., White, S., Wilkinson, A., Zacchei, A., and Zonca, A.
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Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
This paper provides an overview of the Low Frequency Instrument (LFI) programme within the ESA Planck mission. The LFI instrument has been developed to produce high precision maps of the microwave sky at frequencies in the range 27-77 GHz, below the peak of the cosmic microwave background (CMB) radiation spectrum. The scientific goals are described, ranging from fundamental cosmology to Galactic and extragalactic astrophysics. The instrument design and development are outlined, together with the model philosophy and testing strategy. The instrument is presented in the context of the Planck mission. The LFI approach to ground and inflight calibration is described. We also describe the LFI ground segment. We present the results of a number of tests demonstrating the capability of the LFI data processing centre (DPC) to properly reduce and analyse LFI flight data, from telemetry information to calibrated and cleaned time ordered data, sky maps at each frequency (in temperature and polarization), component emission maps (CMB and diffuse foregrounds), catalogs for various classes of sources (the Early Release Compact Source Catalogue and the Final Compact Source Catalogue). The organization of the LFI consortium is briefly presented as well as the role of the core team in data analysis and scientific exploitation. All tests carried out on the LFI flight model demonstrate the excellent performance of the instrument and its various subunits. The data analysis pipeline has been tested and its main steps verified. In the first three months after launch, the commissioning, calibration, performance, and verification phases will be completed, after which Planck will begin its operational life, in which LFI will have an integral part., Comment: 25 pages, 16 figures. In press on Astronomy and Astrophysics
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- 2010
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14. The Planck Low Frequency Instrument
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Mandolesi, N., Burigana, C., Butler, R. C., Cuttaia, F., De Rosa, A., Finelli, F., Franceschi, E., Gruppuso, A., Malaspina, M., Morgante, G., Morigi, G., Popa, L., Sandri, M., Stringhetti, L., Terenzi, L., Valenziano, L., and Villa, F.
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Astrophysics - Abstract
Planck is the third generation of mm-wave instruments designed for space observations of the cosmic microwave background (CMB) anisotropies within the new Cosmic Vision 2020 ESA Science Program. Planck will map the whole sky with unprecedented sensitivity, angular resolution, and frequency coverage, and it likely leads us to the final comprehension of the CMB anisotropies. The Low Frequency Instrument (LFI), operating in the 30-70 GHz range, is one of the two instruments onboard Planck satellite, sharing the focal region of a 1.5 meter off-axis dual reflector telescope together with the High Frequency Instrument (HFI) operating at 100-857 GHz. We present LFI and discuss the major instrumental systematic effects that could degrade the measurements and the solutions adopted in the design and data analysis phase in order to adequately reduce and control them., Comment: 5 pages, 1 figure, On behalf of LFI Consortium,to be published in proc. JENAM 2004 meeting "The many scales in the Universe", Granada, Spain, 13-17 Sept. 2004
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- 2004
15. Planck Low Frequency Instrument: Beam Patterns
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Sandri, M., Bersanelli, M., Burigana, C., Butler, R. C., Malaspina, M., Mandolesi, N., Mennella, A., Morgante, G., Terenzi, L., Valenziano, L., and Villa, F.
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Astrophysics - Abstract
The Low Frequency Instrument on board the ESA Planck satellite is coupled to the Planck 1.5 meter off-axis dual reflector telescope by an array of 27 corrugated feed horns operating at 30, 44, 70, and 100 GHz. We briefly present here a detailed study of the optical interface devoted to optimize the angular resolution (10 arcmin at 100 GHz as a goal) and at the same time to minimize all the systematics coming from the sidelobes of the radiation pattern. Through optical simulations, we provide shapes, locations on the sky, angular resolutions, and polarization properties of each beam., Comment: On behalf of the Planck collaboration. 3 pages, 1 figure. Article published in the Proceedings of the 2K1BC Experimental Cosmology at millimetre wavelengths
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- 2003
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16. A preliminary study on destriping techniques of PLANCK/LFI measurements versus observational strategy
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Burigana, C., Malaspina, M., Mandolesi, N., Danse, L., Maino, D., Bersanelli, M., and Maltoni, M.
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Astrophysics - Abstract
We present here the basic issues of our simulations of PLANCK/LFI observations focussing on the study of the stripes generated by the 1/f noise, including realistic estimates of the 1/f knee frequency, based on the Seiffert et al. (1997) study of the properties of the PLANCK/LFI radiometers. The destriping method presented in the report on the PLANCK PHASE A study has been implemented to be applied to different scanning strategies with the freedom of choosing more or less stringent crossing conditions. Numerical methods for saving the amount of required RAM in the solution of the destriping linear system are presented. We provide preliminary results of the efficiency of this destriping technique for different scanning strategies. We focus here on methodological aspects and remind the reader to the Maino et al. (1999) paper (astro-ph/9906010) for further analyses and a more complete discussion., Comment: 27 pages + 4 PS figures, Internal Report at ITeSRE
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- 1999
17. The Planck-LFI instrument: analysis of the 1/f noise and implications for the scanning strategy
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Maino, D., Burigana, C., Maltoni, M., Wandelt, B. D., Gorski, K. M., Malaspina, M., Bersanelli, M., Mandolesi, N., Banday, A. J., and Hivon, E.
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Astrophysics - Abstract
We study the impact of the 1/f noise on the PLANCK Low Frequency Instrument (LFI) osbervations (Mandolesi et al 1998) and describe a simple method for removing striping effects from the maps for a number of different scanning stategies. A configuration with an angle between telescope optical axis and spin-axis just less than 90 degrees (namely 85 degress) shows good destriping efficiency for all receivers in the focal plane, with residual noise degradation < 1-2 %. In this configuration, the full sky coverage can be achieved for each channel separately with a 5 degrees spin-axis precession to maintain a constant solar aspect angle., Comment: submitted to Astronomy and Astrophysics, 12 pages, 15 PostSript figures
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- 1999
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18. An experimental protocol to access immersiveness in video games
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Saibene, A, Corchs, S, Fontana, S, Solé-Casals, J, Malaspina, M, Amianto Barbato, J, Cremaschi, M, Gasparini, F, Grossi, A, Amianto Barbato, J., Cremaschi, M., Gasparini F., Grossi A., Saibene, A., Saibene, A, Corchs, S, Fontana, S, Solé-Casals, J, Malaspina, M, Amianto Barbato, J, Cremaschi, M, Gasparini, F, Grossi, A, Amianto Barbato, J., Cremaschi, M., Gasparini F., Grossi A., and Saibene, A.
- Abstract
In the video game industry, great importance is given to the experience that the user has while playing a game. In particular, this experience benefits from the players' perceived sense of being in the game or immersion. The level of user immersion depends not only on the game's content but also on how the game is displayed, thus on its User Interface (UI ) and the Head’s-Up Display (HUD). Another factor influencing immersiveness that has been found in the literature is the player's expertise: the more experience the user has with a specific game, the less they need information on the screen to be immersed in the game. Player's level of immersion can be accessed by using both questionnaires of their perceived experience and exploiting their behavioural and physiological responses while playing the target game. Therefore, in this paper, we propose an experimental protocol to access immersiveness of gamers while playing a third-person shooter (Fortnite) with UIs with a standard, a dietetic, and a proposed HUD. A subjective evaluation of the immersion will be provided by completing the Immersive Experience Questionnaire (IEQ), while objective indicators will be provided by face tracking, behaviour and physiological responses analyses. The ultimate goal of this study is to define guidelines for video game UI development that can enhance the players' immersion.
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- 2023
19. Evaluation of agrobiodiversity and its trophic interactions as an indicator of sustainability in productive systems
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Taraborelli, P, primary, Carrasco, N, additional, Malaspina, M, additional, Domínguez, MC, additional, Belaus, A, additional, López, A, additional, Scavone, AS, additional, Barbera, A, additional, and Zamora, MY, additional
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- 2022
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20. PIANO DI PROGRAMMAZIONE 2022 Attività annuale di Comunicazione istituzionale e Public engagement della Struttura per la comunicazione
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Aloisio, Francesca M., Coero Borga, D., Ferroni, E., MIGNONE, CLAUDIA, Boccato, C., GALLIANI, MARCO, Malaspina, M., PERNA, CORRADO, and CAPRIO, Francesco
- Abstract
Questo documento sintetizza la programmazione 2022 della Struttura per la Comunicazione di Presidenza. l'Istituto Nazionale di Astrofisica (INAF) vuole proseguire anche nel 2022 con decisione sulla strada di un forte engagement del pubblico, intrapresa negli ultimi anni e realizzata attraverso una variegata offerta di prodotti di comunicazione. Focalizzare la programmazione su alcuni argomenti di punta, ricorrenze ed eventi astronomici permetterà di sfruttare con maggiore efficienza la sinergia dei vari canali di comunicazione diretta dell'Ente, che si arricchiranno quest'anno della rivista 'Universi', un vero e proprio house organ di cui sarà cruciale anche definire una puntuale lista di indirizzi istituzionali cui farlo avere, da concertare con la segreteria di presidenza. L’Ufficio Stampa, Media Inaf e il Coordinamento nazionale della comunità di Didattica e Divulgazione – le tre anime della Struttura di Comunicazione di Presidenza – lavoreranno di concerto con Edu Inaf e Play Inaf, ulteriori risorse che ampliano l’impatto della grande ‘potenza di fuoco’ della comunicazione dell’Istituto. Tutto nell'ottica di dare un'immagine quanto mai univoca e identificabile di un Ente che negli anni ha guadagnato una notevole visibilità, grazie alla vasta rete di contatti intrattenuta a tutti i livelli. Un Ente che oggi può, e deve, fare un salto di qualità e rendere la sua azione di comunicazione quanto mai incisiva. L’argomento della nostra ricerca rende il compito più lieve e più oneroso al tempo stesso: mostrare la bellezza dell'Universo in tutta la sua meraviglia e complessità, rendendola intellegibile e vicina a tutti. La strategia in atto vuole essere di breve periodo, tenuto anche conto che la realizzazione di una grande mostra in uno spazio espositivo di prestigio della Capitale non potrà ragionevolmente avvenire prima della fine dell'anno, stante il benestare sul titolo e sul progetto proposto: Macchine del Tempo. L'Inaf ha in programma anche per quest'anno la partecipazione a una fitta serie di eventi e festival. La partecipazione dell'Ente dovrà tener conto dei temi proposti dai vari organizzatori, cercando di declinare i temi di nostro interesse su quelli dei festival, non il contrario. Le attività proposte nella presente programmazione potranno essere modificate su richiesta del Presidente.
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- 2022
21. The Focal Attention Window Size Explains Letter Substitution Errors in Reading
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Daini, R, Primativo, S, Albonico, A, Veronelli, L, Malaspina, M, Corbo, M, Martelli, M, Arduino, L, Daini, Roberta, Primativo, Silvia, Albonico, Andrea, Veronelli, Laura, Malaspina, Manuela, Corbo, Massimo, Martelli, Marialuisa, Arduino, Lisa S., Daini, R, Primativo, S, Albonico, A, Veronelli, L, Malaspina, M, Corbo, M, Martelli, M, Arduino, L, Daini, Roberta, Primativo, Silvia, Albonico, Andrea, Veronelli, Laura, Malaspina, Manuela, Corbo, Massimo, Martelli, Marialuisa, and Arduino, Lisa S.
- Abstract
Acquired Neglect Dyslexia is often associated with right-hemisphere brain damage and is mainly characterized by omissions and substitutions in reading single words. Martelli et al. proposed in 2011 that these two types of error are due to different mechanisms. Omissions should depend on neglect plus an oculomotor deficit, whilst substitutions on the difficulty with which the letters are perceptually segregated from each other (i.e., crowding phenomenon). In this study, we hypothesized that a deficit of focal attention could determine a pathological crowding effect, leading to imprecise letter identification and consequently substitution errors. In Experiment 1, three brain-damaged patients, suffering from peripheral dyslexia, mainly characterized by substitutions, underwent an assessment of error distribution in reading pseudowords and a T detection task as a function of cue size and timing, in order to measure focal attention. Each patient, when compared to a control group, showed a deficit in adjusting the attentional focus. In Experiment 2, a group of 17 right-brain-damaged patients were asked to perform the focal attention task and to read single words and pseudowords as a function of inter-letter spacing. The results allowed us to confirm a more general association between substitution-type reading errors and the performance in the focal attention task.
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- 2021
22. Contrasting shared- and specific-mechanism accounts of developmental prosopagnosia: A new approach
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Malaspina M, Andrea Albonico, Tirta Susilo, Barton Jjs, Randi Starrfelt, and Christian Gerlach
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Cognitive science ,bepress|Life Sciences|Neuroscience and Neurobiology ,PsyArXiv|Neuroscience|Cognitive Neuroscience ,PsyArXiv|Social and Behavioral Sciences ,PsyArXiv|Neuroscience ,Computer science ,bepress|Social and Behavioral Sciences ,bepress|Life Sciences|Neuroscience and Neurobiology|Cognitive Neuroscience ,Mechanism (sociology) - Abstract
The understanding of developmental prosopagnosia (DP) is dominated by two opposing views: (i) that DP reflects malfunction of a mechanism shared by face and object recognition, but which is more critical for face than for object recognition, or (ii) that DP is due to malfunction of a mechanism specific to faces, but where object recognition deficits may co-occur due to collateral damage. Here we address some of the limitations in DP studies on this point by examining face and car recognition in a large cohort of healthy subjects selected in an unbiased manner. At the group level we find evidence of a general association between face and car recognition performance but at the individual level we also find occasional dissociations. We discuss the methodological implications of these findings for cognitive neuropsychology in general (association vs. dissociation) but also the theoretical implications for the current understanding of DP more specifically.
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- 2020
23. The Planck LFI RCA flight model test campaign
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Terenzi, L., Villa, F., Mennella, A., Bersanelli, M., Butler, R.C., Cuttaia, F., D’Arcangelo, O., Franceschi, E., Galeotta, S., Maino, D., Malaspina, M., Mandolesi, N., Morgante, G., Sandri, M., Stringhetti, L., Tomasi, M., Valenziano, L., Burigana, C., Finelli, F., Galaverni, M., Gruppuso, A., Paci, F., Popa, L., Procopio, P., and Zuccarelli, J.
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- 2007
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24. The low frequency instrument on-board the Planck satellite: Characteristics and performance
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Valenziano, L., Sandri, M., Morgante, G., Burigana, C., Bersanelli, M., Butler, R.C., Cuttaia, F., Finelli, F., Franceschi, E., Galaverni, M., Gruppuso, A., Malaspina, M., Mandolesi, N., Mennella, A., Paci, F., Popa, L., Procopio, P., Stringhetti, L., Terenzi, L., Tomasi, M., Villa, F., and Zuccarelli, J.
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- 2007
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25. Planck-LFI scientific goals: Implications for the reionization history
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Popa, L.A., Burigana, C., Mandolesi, N., Butler, R.C., Cuttaia, F., Finelli, F., Franceschi, E., Galaverni, M., Gruppuso, A., Malaspina, M., Morgante, G., Paci, F., Procopio, P., Sandri, M., Stringhetti, L., Terenzi, L., Valenziano, L., Villa, F., and Zuccarelli, J.
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- 2007
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26. 15th-century printed Italian editions of Aesopian texts
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Malaspina, M and Dondi, C
- Abstract
My thesis provides the first comprehensive and detailed account of the impact of the introduction of movable-type printing on the production and circulation of Aesopian texts in Italy in the second half of the 15th century. It highlights how the introduction of the new medium did not correspond, at least within the first decades, to a standardisation in the written circulation of the rich Aesopian corpus; on the contrary, it fostered the composition of new versions, translations and rewritings, contributing to enhance its varied and multiform nature. The goal of my thesis is to unveil this process, and to examine the parallel development of textual and figurative traditions of Aesopian texts in the earliest editions produced in Italy, in order to reassess their place in the wider context of the circulation of Aesopian texts in print. Chapter I introduces the main features of the manuscript transmission of those among Aesopian texts, which ended up in print in the first years after the introduction of the new medium. It also focuses on the cultural and historical circumstances of the production of the first editions in the European context. Chapter II presents, in chronological order, all the texts included in the Italian incunable editions, contextualising their authors, their main textual and stylistic features and the circumstances of their composition. Chapters III and IV respectively examine the evolution of the tradition of the different Aesopian texts in print and the evolution of the figurative and iconographic cycles of images illustrating Italian incunable editions of the Vita and the Fabulae. They present a synthesis and assessment of the first-hand data gathered in the Catalogue included in the appendix. The Catalogue in appendix offers a detailed and complete overview of the characteristics of all seventy Aesopian editions printed in Italy in the 15th century. Each edition is analysed with special attention to its bibliographic and textual features, its illustrations, and provenance information concerning the copies examined. The Conclusions focus on the originality of certain texts created specifically for the press, on the people who played an important role in the composition and printing of Aesopian texts, on the identification of new lines of transmission in print, on the distinction and analysis of different iconographic lines of descent in the illustrated editions, and on the discovery of noteworthy cases of provenance evidence, which suggest how the consumption of Aesopian Italian incunables transversely engaged people at different social and cultural levels.
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- 2019
27. TRIP: a cold telescope for measurements of the Near Infrared Cosmological Background at balloon altitudes
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Ventura, G., Malaspina, M., Boscaleri, A., Morigi, G., Attolini, M. R., Brighenti, A., Cazzola, P., Calzolari, P., Cortiglioni, S., Giovannini, G., Mandolesi, N., and Palazzi, E.
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- 1995
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28. Self-face and self-body advantages in congenital prosopagnosia: evidence for a common mechanism
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Malaspina, M, Albonico, A, Daini, R, Malaspina, M, Albonico, A, and Daini, R
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Prosopagnosia is a disorder leading to difficulties in recognizing faces. However, recent evidence suggests that individuals with congenital prosopagnosia can achieve considerable accuracy when they have to recognize their own faces (self-face advantage). Yet, whether this advantage is face-specific or not is still unclear. Here, we aimed to investigate whether individuals with congenital prosopagnosia show a self-advantage also in recognizing other self body-parts and, if so, whether the advantage for the body parts differs from the one characterizing the self-face. Eight individuals with congenital prosopagnosia and 22 controls underwent a delayed matching task in which they were required to recognize faces, hands, and feet belonging to the self or to others. Controls showed a similar self-advantage for all the stimuli tested; by contrast, individuals with congenital prosopagnosia showed a larger self-advantage with faces compared to hands and feet, mainly driven by their deficit with others’ faces. In both groups the self-advantages for the different body parts were strongly and significantly correlated. Our data suggest that the self-face advantage showed by individuals with congenital prosopagnosia is not face-specific and that the same mechanism could be responsible for both the self-face and self body-part advantages.
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- 2019
29. Italian Twin Registry: Web-based Recruitment
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Dukic, T, Malaspina, M, Palumbo, L, D'Ippolito, C, Rotondi, D, Patriarca, V, Giannantonio, L, Toccaceli, V, and Stazi, MA
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- 2007
30. Mapping self-face recognition strategies in congenital prosopagnosia
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Malaspina, M, Albonico, A, Lao, J, Caldara, R, Daini, R, Malaspina, M, Albonico, A, Lao, J, Caldara, R, and Daini, R
- Abstract
Objective: Recent evidence showed that individuals with congenital face processing impairment (congenital prosopagnosia [CP]) are highly accurate when they have to recognize their own face (self-face advantage) in an implicit matching task, with a preference for the right-half of the self-face (right perceptual bias). Yet the perceptual strategies underlying this advantage are unclear. Here, we aimed to verify whether both the self-face advantage and the right perceptual bias emerge in an explicit task, and whether those effects are linked to a different scanning strategy between the self-face and unfamiliar faces. Method: Eye movements were recorded from 7 CPs and 13 controls, during a self/other discrimination task of stimuli depicting the self-face and another unfamiliar face, presented upright and inverted. Results: Individuals with CP and controls differed significantly in how they explored faces. In particular, compared with controls, CPs used a distinct eye movement sampling strategy for processing inverted faces, by deploying significantly more fixations toward the nose and mouth areas, which resulted in more efficient recognition. Moreover, the results confirmed the presence of a self-face advantage in both groups, but the eye movement analyses failed to reveal any differences in the exploration of the self-face compared with the unfamiliar face. Finally, no bias toward the right-half of the self-face was found. Conclusions: Our data suggest that the self-face advantage emerges both in implicit and explicit recognition tasks in CPs as much as in good recognizers, and it is not linked to any specific visual exploration strategies.
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- 2018
31. Target Type Modulates the Effect of Task Demand on Reflexive Focal Attention
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Albonico, A, Malaspina, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, DAINI, ROBERTA, Albonico, A, Malaspina, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, and DAINI, ROBERTA
- Abstract
Focusing attention on a limited space within the environment allows us to concentrate our resources selectively on that location while ignoring the rest of the space. In this study we investigated how the deployment of the focal attention in foveal vision can be affected by task and stimuli specificity. In particular, we measured the cue-size effect in four experiments: shape detection (Experiment 1), shape discrimination (Experiment 2), letter detection (Experiment 3), and letter discrimination (Experiment 4). Our results highlight that, although the focal component can be elicited by different tasks (i.e., detection or discrimination) and by using different types of stimuli (i.e., shapes or letters), those effects interact with each other. Specifically, the effect of focal attention is more noticeable when letter stimuli are used in the case of a detection task, while no difference between letters and geometrical shapes is observed in the discrimination task. Furthermore, the analysis of the cue-size effect across the four experiments confirmed that the deployment of focal attention in foveal vision is mainly reflexive
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- 2017
32. Investigating face-specificity through congenital prosopagnosia: studies on perceptual phenomena and eye movement patterns
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Malaspina, M, DAINI, ROBERTA, MALASPINA, MANUELA, Malaspina, M, DAINI, ROBERTA, and MALASPINA, MANUELA
- Abstract
Congenital prosopagnosia consists of the failure to develop normal face recognition ability despite intact low-level perceptual and intellectual functioning, and in the context of normal exposure to faces throughout the individual’s life. Typically, these individuals are able to perceive facial stimuli as faces but fail to identify a face as familiar or unfamiliar and to identify it. Despite the large amount of studies that have investigated face recognition in individuals with typical development and in congenital prosopagnosics over the last twenty years, we are still far from a complete understanding of the mechanisms underlying typical and atypical face recognition, and some research questions are still open. For this reason, the present dissertation investigates some perceptual effects in individuals with a selective deficit in face recognition processing in order to reach a better understanding of what happens during a successful and unsuccessful face recognition process. In particular, by using a combination of behavioural and eye-tracking methods, I investigated whether the left perceptual bias and the self-face advantage are shown by individuals with congenital prosopagnosia and are truly face-specific or not. My results demonstrate that, whereas the left perceptual bias seems to characterize the recognition of unfamiliar faces in good recognizers, individuals with congenital prosopagnosia seem to show an opposite bias (i.e., a right perceptual bias) during the recognition of the self-face. Moreover, despite their face recognition impairment, congenital prosopagnosics consistently show high accuracy in recognizing their own face (i.e., a self-face advantage). Furthermore, some of the studies I conducted on the visual scanning strategies of this population demonstrated that the self-face advantage phenomenon is not associated with a different exploration of the face stimuli, suggesting that it could reflect a more general self-advantage and not be face-speci
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- 2017
33. Italian normative data and validation of two neuropsychological tests of face recognition: Benton Facial Recognition Test and Cambridge Face Memory Test
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Albonico, A, Malaspina, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, DAINI, ROBERTA, Albonico, A, Malaspina, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, and DAINI, ROBERTA
- Abstract
The Benton Facial Recognition Test (BFRT) and Cambridge Face Memory Test (CFMT) are two of the most common tests used to assess face discrimination and recognition abilities and to identify individuals with prosopagnosia. However, recent studies highlighted that participant–stimulus match ethnicity, as much as gender, has to be taken into account in interpreting results from these tests. Here, in order to obtain more appropriate normative data for an Italian sample, the CFMT and BFRT were administered to a large cohort of young adults. We found that scores from the BFRT are not affected by participants’ gender and are only slightly affected by participant–stimulus ethnicity match, whereas both these factors seem to influence the scores of the CFMT. Moreover, the inclusion of a sample of individuals with suspected face recognition impairment allowed us to show that the use of more appropriate normative data can increase the BFRT efficacy in identifying individuals with face discrimination impairments; by contrast, the efficacy of the CFMT in classifying individuals with a face recognition deficit was confirmed. Finally, our data show that the lack of inversion effect (the difference between the total score of the upright and inverted versions of the CFMT) could be used as further index to assess congenital prosopagnosia. Overall, our results confirm the importance of having norms derived from controls with a similar experience of faces as the “potential” prosopagnosic individuals when assessing face recognition abilities.
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- 2017
34. What Do Eye Movements Tell Us About the Visual Perception of Individuals With Congenital Prosopagnosia?
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Malaspina, M, Albonico, A, Toneatto, C, Daini, R, MALASPINA, MANUELA, ALBONICO, ANDREA, TONEATTO, CARLO, DAINI, ROBERTA, Malaspina, M, Albonico, A, Toneatto, C, Daini, R, MALASPINA, MANUELA, ALBONICO, ANDREA, TONEATTO, CARLO, and DAINI, ROBERTA
- Abstract
Objective: The lack of inversion effect for face recognition in congenital prosopagnosia (CP) is consistent with the hypothesis of a failure in holistic processing. However, although CPs' abnormal gaze behavior for upright faces has already been demonstrated, neither their scanning strategy for inverted faces, nor the possibility that their abnormal gaze behavior with upright faces is because of reasons other than the holistic deficit have been investigated yet. Method: We recorded the eye movements of a congenital prosopagnosic and a control group during the encoding of unknown faces, objects, and flowers. Two types of stimuli (faces and objects) were presented upright and inverted. Results: CPs explored upright and inverted faces in the same way (i.e., similar number of fixations of the same duration and similarly distributed), whereas controls increased the number of fixations and their duration during the presentation of inverted faces. By contrast, the 2 groups showed a similar inversion effect during the encoding of objects. Finally, CPs showed anomalous exploration of within-class objects (i.e., flowers) and impairment in subordinate-level object discrimination. Conclusions: Our results demonstrate that: (a) CPs use the same part-based strategy in encoding both upright and inverted faces, suggesting a possible interpretation of the lack of inversion effect in this population; (b) CPs' lack of inversion effect is face-specific and does not affect objects
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- 2017
35. Do people have insight into their face recognition abilities?
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Palermo, R, Rossion, B, Rhodes, G, Laguesse, R, Tez, T, Hall, B, Albonico, A, Malaspina, M, Daini, R, Irons, J, Al Janabi, S, Taylor, L, Rivolta, D, Mckone, E, Taylor, LC, Mckone, E., ALBONICO, ANDREA, MALASPINA, MANUELA, DAINI, ROBERTA, Palermo, R, Rossion, B, Rhodes, G, Laguesse, R, Tez, T, Hall, B, Albonico, A, Malaspina, M, Daini, R, Irons, J, Al Janabi, S, Taylor, L, Rivolta, D, Mckone, E, Taylor, LC, Mckone, E., ALBONICO, ANDREA, MALASPINA, MANUELA, and DAINI, ROBERTA
- Abstract
Diagnosis of developmental or congenital prosopagnosia (CP) involves self-report of everyday face recognition difficulties, which are corroborated with poor performance on behavioural tests. This approach requires accurate self-evaluation. We examine the extent to which typical adults have insight into their face recognition abilities across four experiments involving nearly 300 participants. The experiments used five tests of face recognition ability: two that tap into the ability to learn and recognize previously unfamiliar faces [the Cambridge Face Memory Test, CFMT; Duchaine, B., & Nakayama, K. (2006). The Cambridge Face Memory Test: Results for neurologically intact individuals and an investigation of its validity using inverted face stimuli and prosopagnosic participants. Neuropsychologia, 44(4), 576–585. doi:10.1016/j.neuropsychologia.2005.07.001; and a newly devised test based on the CFMT but where the study phases involve watching short movies rather than viewing static faces—the CFMT-Films] and three that tap face matching [Benton Facial Recognition Test, BFRT; Benton, A., Sivan, A., Hamsher, K., Varney, N., & Spreen, O. (1983). Contribution to neuropsychological assessment. New York: Oxford University Press; and two recently devised sequential face matching tests]. Self-reported ability was measured with the 15-item Kennerknecht et al. questionnaire [Kennerknecht, I., Ho, N. Y., & Wong, V. C. (2008). Prevalence of hereditary prosopagnosia (HPA) in Hong Kong Chinese population. American Journal of Medical Genetics Part A, 146A(22), 2863–2870. doi:10.1002/ajmg.a.32552]; two single-item questions assessing face recognition ability; and a new 77-item meta-cognition questionnaire. Overall, we find that adults with typical face recognition abilities have only modest insight into their ability to recognize faces on behavioural tests. In a fifth experiment, we assess self-reported face recognition ability in people with CP and find that some people who expect to
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- 2017
36. Screening for colorectal cancer in Italy: 2011-2012 survey
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Zorzi, Manuel, Da Re, Filippo, Mantellini, Paola, Naldoni, Carlo, De Bianchi, Priscilla Sassoli, Senore, Carlo, Turrin, Anna, Visioli, Carmen Beatriz, Zappa, Marco, Crotta, S., Senore, C., Polizzi, S., Sartori, M., Alibrandi, M. P., Germinetti, F., Bestagini, P., Orione, L., Miroglio, T., Faragli, G., Cereda, D., Coppola, L., Zerbi, L., Gramegna, M., Tessandri, L., Imbrogno, P., Rocca, G., Pesenti, B., Schivardi, M., Crisetig, M., Grassi, E., Speziani, F., Gola, G., Gotti, S., Dal Soldà, M., Boldori, L., Moretti, G., Ilardo, A., Ieni, A, Belloni, A., Rossetti, E., Marazza, G., Anghinoni, E., Silvestri, A., Tidone, E., Frammartino, B., Leonardo, N., Deandrea, S., Ceresa, P., Beghi, G., Lucchini, R., Acerbi, L., Lo Buono, F., Cavalieri D'Oro, L., Magenes, G., Camana, L., Cioccarelli, A. M., Fanetti, A. C., Cecconami, L., Bardelli, R., Violini, M., Sambo, F., Domenighini, S., Pieracci, G., Pertile, R., Piffer, S., Fedato, C., Franzo, A., Fabro, J., Gobbato, M., Zanier, L., Bonelli, L., Orlando, M., Vaccari, D., Franxo, A., Scotto, M., Valle, I., Ferrari Bravo, M., Sticchi, C., Maddalo, F., Pensa, F., Naldoni, C., Sassoli De Bianchi, P., Landi, P., Borciani, E., Fornari, F., Gatti, G., Zurlini, C., Zatelli, M., Maradini, F., Paterlini, L., Campari, C., Sassatelli, R., Corradini, R., Goldoni, C., Pasquini, A., Manfredi, M., Baldazzi, P., Nannini, R., Caprara, L., Carpanelli, M. C., Zoli, G., Matarese, V., Triossi, O., Serafini, M., Vitali, B., Falcini, F., Colamartini, A., Giuliani, O., Vattiato, R., Palazzi, M., Imolesi, C., Pazzi, P., Canuti, D., Casale, C., Giovanardi, M., Monticelli, G., Nicolai, C., Vivani, P., Giorgi, D., Finucci, G., Rapanà, M., Epifani, C., Abdelghani, L., Allegrini, G., Maffei, C., Turillazzi, R., Mirri, F., Ceccatelli, P., Rosati, R., Piacentini, P., Visioli, C. B., Falini, P., Amico, P., Ciabattoni, C., Giaimo, M., Prandini, S., Vinti, G., Di Marco, A., Malaspina, M., Corvetti, R., Di Furia, L., Barca, A., Baiocchi, D., Quadrino, F., Di Giacomo, M., Lattanzio, F. M., Minna, M., Di Credico, A., Pizzuti, R., Sigillito, A., Montesi, M. P., Landro, T., Giorno, A., Santino, M., Magrì, G., Ferrara, G., and Masala, R.
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Flexible sigmoidoscopy ,National survey ,Faecal immunochemical test ,Italy ,Colorectal cancer ,Screening ,Epidemiology ,Public Health, Environmental and Occupational Health ,Environmental and Occupational Health ,Public Health - Published
- 2015
37. Characteristics of the colorectal cancers diagnosed in the early 2000s in Italy. Figures from the IMPATTO study on colorectal cancer screening [Caratteristiche dei tumori del colon retto diagnosticati in Italia nei primi anni Duemila. Dati dello studio IMPATTO sdelo screening colorettale]
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Zorzi, Manuel, Mangone, Lucia, Anghinoni, Emanuela, Baracco, Susanna, Borciani, Elisabetta, Caldarella, Adele, Falcini, Fabio, Fanetti, Anna Clara, Ferretti, Stefano, Rossi, Paolo Giorgi, Michiara, Maria, Randi, Giorgia, Stracci, Fabrizio, Vicentini, Massimo, Zucchetto, Antonella, Zappa, Marco, Giacomin, A., Azzoni, A., Baldazzi, P., Collina, N., Pandolfi, P., Biavati, P., Gualandi, G., Sciacca, S., Pesce, P., Torrisi, A., Sciacchitano, C., Fidelbo, M., Finarelli, A. C., Naldoni, C., De'Bianchi, P. Sassoli, Landi, P., Matarese, V., De Togni, A., Palmonari, C., Crocetti, E., Grazzini, G., Manneschi, G., Mantellini, P., Serraino, D., Bidoli, E., Taborelli, M., Gini, A., Virdone, S., Puppo, A., Casella, C., Celesia, M., Cogno, R., Marani, E., Bugliarello, E., Fattoruso, S., Tamburo, L., Tamburrino, S., Bellardini, P., Autelitano, M., Frammartino, B., Bisanti, L., Ghilardi, S., Leone, R., Corradini, R., De Girolamo, F., Valla, K., Palombino, R., Gigli, L., Spena, S. Russo, Vitale, M. F., Cascio, M. A., Mannino, R., Mazzucco, W., Mistretta, A., Ravazzolo, B., Sgarzi, P., Bozzani, F., Zatelli, M., Zurlini, C., Caruana, P., Seghini, P., Gatti, G., Prazzoli, R., Campari, C., Paterlini, L., Cassetti, T., Sassatelli, R., Imolesi, C., Casale, C., Serafini, M., Vattiato, R., Giuliani, O., Cesaraccio, R., Sechi, O., Budroni, M., Madeddu, A., Contrino, M. L., Ziino, A. Colanino, Russo, M., Tisano, F., Fanetti, A. C., Maspero, S., Moroni, E., Cometti, I., Gentilini, M., Piffer, S., De Pretis, G., Caciagli, P., Pertile, R., Bianconi, F., Bucchi, D., Galeotti, M. E., Malaspina, M., Greco, A., Fiore, A. R., Stocco, C. F., and Fedato, C.
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Colorectal cancer ,Colorectal cancer screening ,Italy ,Epidemiology ,Public Health, Environmental and Occupational Health ,Environmental and Occupational Health ,Socio-culturale ,Public Health - Published
- 2015
38. Temporal dissociation between the focal and orientation components of spatial attention in central and peripheral vision
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Albonico, A, Malaspina, M, Bricolo, E, Martelli, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, BRICOLO, EMANUELA, DAINI, ROBERTA, Albonico, A, Malaspina, M, Bricolo, E, Martelli, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, BRICOLO, EMANUELA, and DAINI, ROBERTA
- Abstract
Selective attention, i.e. the ability to concentrate one's limited processing resources on one aspect of the environment, is a multifaceted concept that includes different processes like spatial attention and its subcomponents of orienting and focusing. Several studies, indeed, have shown that visual tasks performance is positively influenced not only by attracting attention to the target location (orientation component), but also by the adjustment of the size of the attentional window according to task demands (focal component). Nevertheless, the relative weight of the two components in central and peripheral vision has never been studied. We conducted two experiments to explore whether different components of spatial attention have different effects in central and peripheral vision. In order to do so, participants underwent either a detection (Experiment 1) or a discrimination (Experiment 2) task where different types of cues elicited different components of spatial attention: a red dot, a small square and a big square (an optimal stimulus for the orientation component, an optimal and a sub-optimal stimulus for the focal component respectively). Response times and cue-size effects indicated a stronger effect of the small square or of the dot in different conditions, suggesting the existence of a dissociation in terms of mechanisms between the focal and the orientation components of spatial attention. Specifically, we found that the orientation component was stronger in periphery, while the focal component was noticeable only in central vision and characterized by an exogenous nature.
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- 2016
39. Congenital prosopagnosia is associated with a genetic variation in the oxytocin receptor (OXTR) gene: An exploratory study
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Cattaneo, Z, Daini, R, Malaspina, M, Manai, F, Lillo, M, Fermi, V, Schiavi, S, Suchan, B, Comincini, S, CATTANEO, ZAIRA, DAINI, ROBERTA, MALASPINA, MANUELA, SCHIAVI, SUSANNA, Comincini, S., Cattaneo, Z, Daini, R, Malaspina, M, Manai, F, Lillo, M, Fermi, V, Schiavi, S, Suchan, B, Comincini, S, CATTANEO, ZAIRA, DAINI, ROBERTA, MALASPINA, MANUELA, SCHIAVI, SUSANNA, and Comincini, S.
- Abstract
Face-recognition deficits, referred to with the term prosopagnosia (i.e., face blindness), may manifest during development in the absence of any brain injury (from here the term congenital prosopagnosia, CP). It has been estimated that approximately 2.5% of the population is affected by face-processing deficits not depending on brain lesions, and varying a lot in severity. The genetic bases of this disorder are not known. In this study we tested for genetic association between single-nucleotide polymorphisms (SNPs) in the oxytocin receptor gene (OXTR) and CP in a restricted cohort of Italian participants. We found evidence of an association between the common genetic variants rs53576 and rs2254298 OXTR SNPs and prosopagnosia. This association was also found when including an additional group of German individuals classified as prosopagnosic in the analysis. Our preliminary data provide initial support for the involvement of genetic variants of OXTR in a relevant cognitive impairment, whose genetic bases are still largely unexplored.
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- 2016
40. Right perceptual bias and self-face recognition in individuals with congenital prosopagnosia
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Malaspina, M, Albonico, A, Daini, R, MALASPINA, MANUELA, ALBONICO, ANDREA, DAINI, ROBERTA, Malaspina, M, Albonico, A, Daini, R, MALASPINA, MANUELA, ALBONICO, ANDREA, and DAINI, ROBERTA
- Abstract
The existence of a drift to base judgments more on the right half-part of facial stimuli, which falls in the observer's left visual field (left perceptual bias (LPB)), in normal individuals has been demonstrated. However, less is known about the existence of this phenomenon in people affected by face impairment from birth, namely congenital prosopagnosics. In the current study, we aimed to investigate the presence of the LPB under face impairment conditions using chimeric stimuli and the most familiar face of all: the self-face. For this purpose we tested 10 participants with congenital prosopagnosia and 21 healthy controls with a face matching task using facial stimuli, involving a spatial manipulation of the left and the right hemi-faces of self-photos and photos of others. Even though congenital prosopagnosics performance was significantly lower than that of controls, both groups showed a consistent self-face advantage. Moreover, congenital prosopagnosics showed optimal performance when the right side of their face was presented, that is, right perceptual bias, suggesting a differential strategy for self-recognition in those subjects. A possible explanation for this result is discussed.
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- 2016
41. Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance
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Poutanen, T., Lähteenmäki, A., León-Tavares, J., Polenta, G., Natoli, P., Falvella, M.C., Bartlett, J.G., Smoot, G.F., Bonavera, L., Banday, A.J., Seiffert, M.D., Paladini, R., Prézeau, G., Rocha, G., Lilje, P.B., Hughes, N., Jukkala, P., Kilpia, V.-H., Sjoman, P., Nørgaard-Nielsen, Hans Ulrik, Toffolatti, L., Aja, B., Artal, E., Cruz, M., Moss, A., Scott, D., Colombo, L., Kurki-Suonio, H., Suur-Uski, A.-S., Juvela, M., Keihänen, E., Keskitalo, R., Savelainen, M., Knox, L., Meinhold, P.R., Zonca, A., Leonardi, R., Lubin, P.M., Bartolo, N., Matarrese, S., Melchiorri, A., Mennella, A., Maino, D., Tomasi, M., Franceschet, C., Gregorio, A., Cabella, P., De Gasperis, G., Migliaccio, M., Quercellini, C., Vittorio, N., Marinucci, D., Génova-Santos, R.T., Rebolo, R., Rubi No-Martín, J.A., Mendes, L., Foley, S., Watson, C., Bennett, K., Tauber, J.A., Partridge, B., Nesti, R., Tofani, G., Umana, G., Bonaldi, A., De Zotti, G., Massardi, M., Frailis, M., Galeotta, S., Maris, M., Tavagnacco, D., Zacchei, A., Pasian, F., Butler, R.C., Cuttaia, F., Mandolesi, N., Morgante, G., Sandri, M., Terenzi, L., Villa, F., Burigana, C., De Rosa, A., Finelli, F., Franceschi, E., Gruppuso, A., Malaspina, M., Paoletti, D., Procopio, P., Ricciardi, S., Stringhetti, L., Valenziano, L., Cappellini, B., Donzelli, S., Türler, M., Chen, X., Puget, J.-L., Bouchet, F.R., Efstathiou, G., Valiviita, J., Eriksen, H.K., Hansen, F.K., Gómez, F., Herreros, J.M., Hoyland, R.J., Curto, A., Martínez-González, E., Barreiro, R.B., Diego, J.M., Herranz, D., López-Caniego, M., Vielva, P., D'Arcangelo, O., Simonetto, A., Sozzi, C., Lawrence, C.R., Pearson, D., Gaier, T.C., Górski, K.M., Jewell, J., Kangaslahti, P., Mitra, S., Pagano, L., Pietrobon, D., Prina, M., Wade, L.A., Davis, R.J., Leahy, J.P., Lowe, S., Watson, R., Wilkinson, A., Davies, R.D., Dickinson, C., Roddis, N., Winder, F., Lamarre, J.-M., Borrill, J., Kisner, T.S., Enßlin, T.A., Knoche, J., Matthai, F., Rachen, J.P., Reinecke, M., Robbers, G., White, S.D.M., Tuovinen, J., Varis, J., Pospieszalski, M., Laaninen, M., Dick, J., Leach, S., Perrotta, F., Baccigalupi, C., Danese, L., González-Nuevo, J., Pettorino, V., George, D., Battaglia, P., Leutenegger, P., Miccolis, M., Silvestri, R., APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, 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)-Observatoire de Paris, 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), PLANCK, Universidad de Cantabria, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), 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)-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), 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)-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), Mennella, A., Bersanelli, M., Butler, R. C., Curto, A., Cuttaia, F., Davis, R. J., Dick, J., Frailis, M., Galeotta, S., Gregorio, Anna, Kurki Suonio, H., Lawrence, C. R., Leach, S., Leahy, J. P., Lowe, S., Maino, D., Mandolesi, N., Maris, M., Mart'inez González, E., Meinhold, P. R., Morgante, G., Pearson, D., Perrotta, F., Polenta, G., Poutanen, T., Sandri, M., Seiffert, M. D., Suur Uski, A. S., Tavagnacco, Daniele, Terenzi, L., Tomasi, M., Valiviita, J., Villa, F., Watson, R., Wilkinson, A., Zacchei, A., Zonca, A., Aja, B., Artal, E., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Bartolo, N., Battaglia, P., Bennett, K., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F. R., Burigana, C., Cabella, P., Cappellini, B., Chen, X., Colombo, L., Cruz, M., Danese, L., D'Arcangelo, O., Davies, R. D., de Gasperis, G., de Rosa, A., de Zotti, G., Dickinson, C., Diego, J. M., Donzelli, S., Efstathiou, G., Ensslin, T. A., Eriksen, H. K., Falvella, M. C., Finelli, F., Foley, S., Franceschet, C., Franceschi, E., Gaier, T. C., Génova Santos, R. T., George, D., Gómez, F., González Nuevo, J., Górski, K. M., Gruppuso, A., Hansen, F. K., Herranz, D., Herreros, J. M., Hoyland, R. J., Hughes, N., Jewell, J., Jukkala, P., Juvela, M., Kangaslahti, P., Keihänen, E., Keskitalo, R., Kilpia, V. H., Kisner, T. S., Knoche, J., Knox, L., Laaninen, M., Lähteenmäki, A., Lamarre, J. M., Leonardi, R., León Tavares, J., Leutenegger, P., Lilje, P. B., López Caniego, M., Lubin, P. M., Malaspina, M., Marinucci, D., Massardi, M., Matarrese, S., Matthai, F., Melchiorri, A., Mendes, L., Miccolis, M., Migliaccio, M., Mitra, S., Moss, A., Natoli, P., Nesti, R., Norgaard Nielsen, H. U., Pagano, L., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Pettorino, V., Pietrobon, D., Pospieszalski, M., Prézeau, G., Prina, M., Procopio, P., Puget, J. L., Quercellini, C., Rachen, J. P., Rebolo, R., Reinecke, M., Ricciardi, S., Robbers, G., Rocha, G., Roddis, N., Rubino Martín, J. A., Savelainen, M., Scott, D., Silvestri, R., Simonetto, A., Sjoman, P., Smoot, G. F., Sozzi, C., Stringhetti, L., Tauber, J. A., Tofani, G., Tuovinen, J., Türler, M., Umana, G., Valenziano, L., Varis, J., Vielva, P., Vittorio, N., Wade, L. A., Watson, C., White, S., Winder, F., Department of Physics, and Helsinki Institute of Physics
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[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,education ,Cosmic background radiation ,FOS: Physical sciences ,Astrophysics ,cosmic background radiation ,Low frequency ,Cosmic backround radiation ,7. Clean energy ,01 natural sciences ,instruments [Space vehicles] ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,symbols.namesake ,Settore FIS/05 - Astronomia e Astrofisica ,CMB physics ,0103 physical sciences ,Space vehicles: instruments ,Instrumentation: detectors ,Planck ,cosmology: observations ,space vehicles: instruments ,instrumentation: detectors ,observations [Cosmology] ,010303 astronomy & astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,detectors [Instrumentation] ,detectors ,Physics ,010308 nuclear & particles physics ,Planck ESA mission ,Cosmology: observations ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy and Astrophysics ,115 Astronomy, Space science ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,observations ,Early results ,Space and Planetary Science ,symbols ,space vehicles ,Astrophysics - Instrumentation and Methods for Astrophysics ,cosmology ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
29 páginas, 31 figuras, 15 tablas.-- Planck Collaboration: et al., The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit operation is presented. We describe the main optical parameters and discuss photometric calibration, white noise sensitivity, and noise properties. A preliminary evaluation of the impact of the main systematic effects is presented. For each of the performance parameters, we outline the methods used to obtain them from the flight data and provide a comparison with pre-launch ground assessments, which are essentially confirmed in flight., The Consortia are led by the Principal Investigators: J.-L. Puget in France for HFI (funded principally by CNES and CNRS/INSU-IN2P3) and N. Mandolesi in Italy for LFI (funded principally via ASI). NASA’s US Planck Project, based at JPL and involving scientists at many US institutions, contributes significantly to the efforts of these two Consortia. In Finland, the Planck LFI 70 GHz work was supported by the Finnish Funding Agency for Technology and Innovation (Tekes). This work was also supported by the Academy of Finland, CSC, and DEISA (EU).
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- 2011
- Full Text
- View/download PDF
42. PLANCK pre-launch status: Low Frequency Instrument calibration and scientific performance
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MENNELLA A, BERSANELLI M, BUTLER R. C, CUTTAIA F, DARCANGELO O, DAVIS R. J, FRAILIS M, GALEOTTA S, LAWRENCE C. R, LEONARDI R, LOWE S. R, MANDOLESI N, MARIS M, MEINHOLD P, MENDES L, MORGANTE G, SANDRI M, STRINGHETTI L, TERENZI L, TOMASI M, VALENZIANO L, VILLA F, ZACCHEI A, ZONCA A, BALASINI M, FRANCESCHET C, BATTAGLIA P, LAPOLLA P. M, LEUTENEGGER P, MICCOLIS M, PAGAN L, SILVESTRI R, AJA B, ARTAL E, BALDAN G, BASTIA P, BERNARDINO T, BOSCHINI L, CAFAGNA G, CAPPELLINI B, CAVALIERE F, COLOMBO F, DE LA FUENTE L, EDGELEY J, FALVELLA M. C, FERRARI F, FOGLIANI S, FRANCESCHI E, GAIER T, GOMEZ F, HERREROS J. M, HILDEBRANDT S, HOYLAND R, HUGHES N, JUKKALA P, KETTLE D, LAANINEN M, LAWSON D, LEAHY P, LEVIN S, LILJE P. B, MAINO D, MALASPINA M, MANZATO P, MARTI CANALES J, MARTINEZ GONZALEZ E, MEDIAVILLA A, PASIAN F, PASCUAL J. P, PECORA M, PERES CUEVAS L, PLATANIA P, POSPIESZALSKY M, POUTANEN T, REBOLO R, RODDIS N, SALMON M, SEIFFERT M, SIMONETTO A, SOZZI C, TAUBER J, TUOVINEN J, VARIS J, WILKINSON A, WINDER F., GREGORIO, ANNA, Mennella, A, Bersanelli, M, BUTLER R., C, Cuttaia, F, Darcangelo, O, DAVIS R., J, Frailis, M, Galeotta, S, Gregorio, Anna, LAWRENCE C., R, Leonardi, R, LOWE S., R, Mandolesi, N, Maris, M, Meinhold, P, Mendes, L, Morgante, G, Sandri, M, Stringhetti, L, Terenzi, L, Tomasi, M, Valenziano, L, Villa, F, Zacchei, A, Zonca, A, Balasini, M, Franceschet, C, Battaglia, P, LAPOLLA P., M, Leutenegger, P, Miccolis, M, Pagan, L, Silvestri, R, Aja, B, Artal, E, Baldan, G, Bastia, P, Bernardino, T, Boschini, L, Cafagna, G, Cappellini, B, Cavaliere, F, Colombo, F, DE LA FUENTE, L, Edgeley, J, FALVELLA M., C, Ferrari, F, Fogliani, S, Franceschi, E, Gaier, T, Gomez, F, HERREROS J., M, Hildebrandt, S, Hoyland, R, Hughes, N, Jukkala, P, Kettle, D, Laaninen, M, Lawson, D, Leahy, P, Levin, S, LILJE P., B, Maino, D, Malaspina, M, Manzato, P, MARTI CANALES, J, MARTINEZ GONZALEZ, E, Mediavilla, A, Pasian, F, PASCUAL J., P, Pecora, M, PERES CUEVAS, L, Platania, P, Pospieszalsky, M, Poutanen, T, Rebolo, R, Roddis, N, Salmon, M, Seiffert, M, Simonetto, A, Sozzi, C, Tauber, J, Tuovinen, J, Varis, J, Wilkinson, A, and Winder, F.
- Subjects
Planck ESA mission ,CMB physics - Abstract
We present the calibration and scientific performance parameters of the Planck Low Frequency Instrument (LFI) measured during the ground cryogenic test campaign. These parameters characterise the instrument response and constitute our optimal pre-launch knowledge of the LFI scientific performance. The LFI shows excellent 1/ f stability and rejection of instrumental systematic effects; its measured noise performance shows that LFI is the most sensitive instrument of its kind. The calibration parameters will be updated during flight operations until the end of the mission.
- Published
- 2010
43. Something in the way people move: The benefit of facial movements in face identification
- Author
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Albonico, A, Malaspina, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, DAINI, ROBERTA, Albonico, A, Malaspina, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, and DAINI, ROBERTA
- Abstract
While the dissociation between invariant aspects of a face and emotional expressions has been studied extensively, the role of non-emotional changeable aspects in face recognition has been considered in the literature rarely. The purpose of the present study was to understand whether information on changeable aspects (with and without emotional content) can help those individuals with poor face recognition abilities (when based on invariant features) in recognizing famous faces. From a population of 80 university students we selected two groups of participants, one with poor performance (experimental group, EG) and the other with good performance (control group, CG). By means of a preliminary experiment, we selected videos of 16 Italian celebrities that were presented in three different conditions: motionless, with non-emotional expressions, and with emotional expressions. While the CG did not differ in the three conditions, the EG showed a significantly better performance in the two conditions with facial movements, which did not differ between each other. These results suggest a role of changeable aspects in the identification of famous faces, rising only in the case invariant features are not analyzed properly.
- Published
- 2015
44. A geometrical model for mechanical media described in the frame of extended irreversible thermodynamics with internal variables
- Author
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Malaspina, M. E., Mazzeo Maria, Paola., and Restuccia, L.
- Subjects
Extended irreversible thermodynamics ,mechanical media with internal variables ,thermodynamic geometrical models - Published
- 2012
45. Documento GISCI:Raccomandazioni sul test HR-HPV come test di screening primario e rivisitazione del ruolo del Pap test
- Author
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Beccati, D., Confortini, M., Passamonti, B., Carozzi, F., Angeloni, C., Barbarino, P., Benevolo, M., Benini, S., Billetti, S., Cogo, C., Dalla Palma, P., Del Mistro, A. R., De Marco, L., French, D., Gillio Tos, A., Giorgi Rossi, P., Giovannelli, L., Iossa, A., Lattanzi, A., Maccalini, V., Maestri, Iva, Malaspina, M., Montanari, G., Morigi, F., Paganini, I., Pellegrini, A., Reggi, T., Sandri, M. T., Sani, C., Schiboni, M. L., Stornelli, V., Tufi, M. C., and Zorzi, M.
- Published
- 2010
46. Differential effects of the size of the attentional window in central and peripheral vision
- Author
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Albonico, A, Malaspina, M, Bricolo, E, Martelli, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, BRICOLO, EMANUELA, DAINI, ROBERTA, Albonico, A, Malaspina, M, Bricolo, E, Martelli, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, BRICOLO, EMANUELA, and DAINI, ROBERTA
- Published
- 2014
47. Dissociazione tra la componente selettiva e la componente focale dell’attenzione visuo-spaziale in visione centrale e periferica
- Author
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Albonico, A, Malaspina, M, Bricolo, E, Martelli, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, BRICOLO, EMANUELA, DAINI, ROBERTA, Albonico, A, Malaspina, M, Bricolo, E, Martelli, M, Daini, R, ALBONICO, ANDREA, MALASPINA, MANUELA, BRICOLO, EMANUELA, and DAINI, ROBERTA
- Published
- 2014
48. Is Congenital Prosopagnosics’ eye movements pattern specific in self compared to others’ faces discrimination?
- Author
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Malaspina, M, Albonico, A, Daini, R, MALASPINA, MANUELA, ALBONICO, ANDREA, DAINI, ROBERTA, Malaspina, M, Albonico, A, Daini, R, MALASPINA, MANUELA, ALBONICO, ANDREA, and DAINI, ROBERTA
- Published
- 2014
49. L’io è diverso dall’altro? Uno studio sui movimenti oculari nella Prosopagnosia Congenita
- Author
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Malaspina, M, Albonico, A, Daini, R, MALASPINA, MANUELA, ALBONICO, ANDREA, DAINI, ROBERTA, Malaspina, M, Albonico, A, Daini, R, MALASPINA, MANUELA, ALBONICO, ANDREA, and DAINI, ROBERTA
- Published
- 2014
50. Elaborazione delle espressioni facciali, emotive e non, in soggetti affetti da sindrome di Asperger o autismo ad alto funzionamento
- Author
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Malaspina, M, Albonico, A, Daini, R, Ricciardelli, P, MALASPINA, MANUELA, ALBONICO, ANDREA, DAINI, ROBERTA, RICCIARDELLI, PAOLA, Malaspina, M, Albonico, A, Daini, R, Ricciardelli, P, MALASPINA, MANUELA, ALBONICO, ANDREA, DAINI, ROBERTA, and RICCIARDELLI, PAOLA
- Abstract
The aim of the present study was to investigate the processing of the emotional and non-emotional facial expression and facial features of unfamiliar faces in individuals with Asperger's syndrome (AS) and High-Functioning Autism (HFA). To this end, we tested 14 Adults with AS and HFA and 12 typically developing individuals, matched for age and education level, in a recognition task of faces in which internal features (e.g., eyes size), emotional and non-emotional facial expressions could or could not have been manipulated. Participants were asked first to undergo the recognition task and then a change detection task of the manipulation. Results show not only a face recognition impairment (lower accuracy) in the autistic group, but also a difference in the processing of facial changeable and unchangeable features, and between emotional and non-emotional expressions.
- Published
- 2014
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