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1. Calibration of the IXPE focal plane X-ray polarimeters to polarized radiation

Author: Di Marco, Alessandro, Fabiani, Sergio, La Monaca, Fabio, Muleri, Fabio, Rankin, John, Soffitta, Paolo, Xie, Fei, Amici, Fabrizio, attinà, Primo, Bachetti, Matteo, Baldini, Luca, Barbanera, Mattia, Baumgartner, Wayne, Bellazzini, Ronaldo, Borotto, Fabio, Brez, Alessandro, Brienza, Daniele, Caporale, Ciro, Cardelli, Claudia, Carpentiero, Rita, Castellano, Simone, Castronuovo, Marco, Cavalli, Luca, Cavazzuti, Elisabetta, Ceccanti, Marco, Centrone, Mauro, Citraro, Saverio, Costa, Enrico, D'Alba, Elisa, D'Amico, Fabio, Del Monte, Ettore, Di Cosimo, Sergio, Di Lalla, Niccolò, Di Persio, Giuseppe, Donnarumma, Immacolata, Evangelista, Yuri, Ferrazzoli, Riccardo, Latronico, Luca, Lefevre, Carlo, Loffredo, Pasqualino, Lorenzi, Paolo, Lucchesi, Leonardo, Magazzù, Carlo, Magazzù, Guido, Maldera, Simone, Manfreda, Alberto, Mangraviti, Elio, Marengo, Marco, Matt, Giorgio, Mereu, Paolo, Minuti, Massimo, Morbidini, Alfredo, Mosti, Federico, Nasimi, Hikmat, Negri, Barbara, Nuti, Alessio, O'Dell, Stephen L., Orsini, Leonardo, Perri, Matteo, Pesce-Rollins, Melissa, Piazzolla, Raffaele, Pieraccini, Stefano, Pilia, Maura, Pinchera, Michele, Profeti, Alessandro, Puccetti, Simonetta, Ramsey, Brian D., Ratheesh, Ajay, Rubini, Alda, Santoli, Francesco, Sarra, Paolo, Scalise, Emanuele, Sciortino, Andrea, Sgrò, Carmelo, Spandre, Gloria, Tardiola, Marcello, Tennant, Allyn F., Tobia, Antonino, Trois, Alessio, Vimercati, Marco, Weisskopf, Martin C., Zanetti, Davide, and Zanetti, Francesco
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: IXPE (Imaging X-ray Polarimetry Explorer) is a NASA Small Explorer mission -- in partnership with the Italian Space Agency (ASI) -- dedicated to X-ray polarimetry in the 2--8 keV energy band. The IXPE telescope comprises three grazing incidence mirror modules coupled to three detector units hosting each one a Gas Pixel Detector (GPD), a gas detector that allows measuring the polarization degree by using the photoelectric effect. A wide and accurate ground calibration was carried out on the IXPE Detector Units (DUs) at INAF-IAPS, in Italy, where a dedicated facility was set-up at this aim. In this paper, we present the results obtained from this calibration campaign to study the IXPE focal plane detector response to polarized radiation. In particular, we report on the modulation factor, which is the main parameter to estimate the sensitivity of a polarimeter., Comment: Accepted for publication on The Astronomical Journal
Published: 2022
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2. Forecasting Change in Conflict Fatalities with Dynamic Elastic Net

Author: Attinà, Fulvio, Carammia, Marcello, and Iacus, Stefano Maria
Subjects: Statistics - Applications
Abstract: This article illustrates an approach to forecasting change in conflict fatalities designed to address the complexity of the drivers and processes of armed conflicts. The design of this approach is based on two main choices. First, to account for the specificity of conflict drivers and processes over time and space, we model conflicts in each individual country separately. Second, we draw on an adaptive model -- Dynamic Elastic Net, DynENet -- which is able to efficiently select relevant predictors among a large set of covariates. We include over 700 variables in our models, adding event data on top of the data features provided by the con-venors of the forecasting competition. We show that our approach is suitable and computa-tionally efficient enough to address the complexity of conflict dynamics. Moreover, the adaptive nature of our model brings a significant added value. Because for each country our model only selects the variables that are relevant to predict conflict intensity, the retained predictors can be analyzed to describe the dynamic configuration of conflict drivers both across countries and within countries over time. Countries can then be clustered to observe the emergence of broader patterns related to correlates of conflict. In this sense, our ap-proach produces interpretable forecasts, addressing one key limitation of contemporary ap-proaches to forecasting.
Published: 2022

3. The Imaging X-Ray Polarimetry Explorer (IXPE): Pre-Launch

Author: Weisskopf, Martin C., Soffitta, Paolo, Baldini, Luca, Ramsey, Brian D., O'Dell, Stephen L., Romani, Roger W., Matt, Giorgio, Deininger, William D., Baumgartner, Wayne H., Bellazzini, Ronaldo, Costa, Enrico, Kolodziejczak, Jeffery J., Latronico, Luca, Marshall, Herman L., Muleri, Fabio, Bongiorno, Stephen D., Tennant, Allyn, Bucciantini, Niccolo, Dovciak, Michal, Marin, Frederic, Marscher, Alan, Poutanen, Juri, Slane, Pat, Turolla, Roberto, Kalinowski, William, Di Marco, Alessandro, Fabiani, Sergio, Minuti, Massimo, La Monaca, Fabio, Pinchera, Michele, Rankin, John, Sgro', Carmelo, Trois, Alessio, Xie, Fei, Alexander, Cheryl, Allen, D. Zachery, Amici, Fabrizio, Andersen, Jason, Antonelli, Angelo, Antoniak, Spencer, Attina', Primo, Barbanera, Mattia, Bachetti, Matteo, Baggett, Randy M., Bladt, Jeff, Brez, Alessandro, Bonino, Raffaella, Boree, Christopher, Borotto, Fabio, Breeding, Shawn, Brienza, Daniele, Bygott, H. Kyle, Caporale, Ciro, Cardelli, Claudia, Carpentiero, Rita, Castellano, Simone, Castronuovo, Marco, Cavalli, Luca, Cavazzuti, Elisabetta, Ceccanti, Marco, Centrone, Mauro, Citraro, Saverio, Amico, Fabio D', D'Alba, Elisa, Di Gesu, Laura, Del Monte, Ettore, Dietz, Kurtis L., Di Lalla, Niccolo', Di Persio, Giuseppe, Dolan, David, Donnarumma, Immacolata, Evangelista, Yuri, Ferrant, Kevin, Ferrazzoli, Riccardo, Ferrie, MacKenzie, Footdale, Joseph, Forsyth, Brent, Foster, Michelle, Garelick, Benjamin, Gunji, Shuichi, Gurnee, Eli, Head, Michael, Hibbard, Grant, Johnson, Samantha, Kelly, Erik, Kilaru, Kiranmayee, Lefevre, Carlo, Roy, Shelley Le, Loffredo, Pasqualino, Lorenzi, Paolo, Lucchesi, Leonardo, Maddox, Tyler, Magazzu, Guido, Maldera, Simone, Manfreda, Alberto, Mangraviti, Elio, Marengo, Marco, Marrocchesi, Alessandra, Massaro, Francesco, Mauger, David, McCracken, Jeffrey, McEachen, Michael, Mize, Rondal, Mereu, Paolo, Mitchell, Scott, Mitsuishi, Ikuyuki, Morbidini, Alfredo, Mosti, Federico, Nasimi, Hikmat, Negri, Barbara, Negro, Michela, Nguyen, Toan, Nitschke, Isaac, Nuti, Alessio, Onizuka, Mitch, Oppedisano, Chiara, Orsini, Leonardo, Osborne, Darren, Pacheco, Richard, Paggi, Alessandro, Painter, Will, Pavelitz, Steven D., Pentz, Christina, Piazzolla, Raffaele, Perri, Matteo, Pesce-Rollins, Melissa, Peterson, Colin, Pilia, Maura, Profeti, Alessandro, Puccetti, Simonetta, Ranganathan, Jaganathan, Ratheesh, Ajay, Reedy, Lee, Root, Noah, Rubini, Alda, Ruswick, Stephanie, Sanchez, Javier, Sarra, Paolo, Santoli, Francesco, Scalise, Emanuele, Sciortino, Andrea, Schroeder, Christopher, Seek, Tim, Sosdian, Kalie, Spandre, Gloria, Speegle, Chet O., Tamagawa, Toru, Tardiola, Marcello, Tobia, Antonino, Thomas, Nicholas E., Valerie, Robert, Vimercati, Marco, Walden, Amy L., Weddendorf, Bruce, Wedmore, Jeffrey, Welch, David, Zanetti, Davide, and Zanetti, Francesco
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: Scheduled to launch in late 2021, the Imaging X-ray Polarimetry Explorer (IXPE) is a NASA Small Explorer Mission in collaboration with the Italian Space Agency (ASI). The mission will open a new window of investigation - imaging X-ray polarimetry. The observatory features 3 identical telescopes each consisting of a mirror module assembly with a polarization-sensitive imaging X-ray detector at the focus. A coilable boom, deployed on orbit, provides the necessary 4-m focal length. The observatory utilizes a 3-axis-stabilized spacecraft which provides services such as power, attitude determination and control, commanding, and telemetry to the ground. During its 2-year baseline mission, IXPE will conduct precise polarimetry for samples of multiple categories of X-ray sources, with follow-on observations of selected targets.
Published: 2021

4. Calibration of the IXPE instrument

Author: Muleri, Fabio, Lefevre, Carlo, Piazzolla, Raffaele, Morbidini, Alfredo, Amici, Fabrizio, Attinà, Primo, Centrone, Mauro, Del Monte, Ettore, Di Cosimo, Sergio, Di Persio, Giuseppe, Evangelista, Yuri, Fabiani, Sergio, Ferrazzoli, Riccardo, Loffredo, Pasqualino, Maiolo, Luca, Maita, Francesco, Primicino, Leandra, Rankin, John, Rubini, Alda, Santoli, Francesco, Soffitta, Paolo, Tobia, Antonino, Tortosa, Alessia, and Trois, Alessio
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: IXPE scientific payload comprises of three telescopes, each composed of a mirror and a photoelectric polarimeter based on the Gas Pixel Detector design. The three focal plane detectors, together with the unit which interfaces them to the spacecraft, are named IXPE Instrument and they will be built and calibrated in Italy; in this proceeding, we will present how IXPE Instrument will be calibrated, both on-ground and in-flight. The Instrument Calibration Equipment is being finalized at INAF-IAPS in Rome (Italy) to produce both polarized and unpolarized radiation, with a precise knowledge of direction, position, energy and polarization state of the incident beam. In flight, a set of four calibration sources based on radioactive material and mounted on a filter and calibration wheel will allow for the periodic calibration of all of the three IXPE focal plane detectors independently. A highly polarized source and an unpolarized one will be used to monitor the response to polarization; the remaining two will be used to calibrate the gain through the entire lifetime of the mission., Comment: 11 pages, 8 figures
Published: 2021
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5. The IXPE Instrument Calibration Equipment

Author: Muleri, Fabio, Piazzolla, Raffaele, Di Marco, Alessandro, Fabiani, Sergio, La Monaca, Fabio, Lefevre, Carlo, Morbidini, Alfredo, Rankin, John, Soffitta, Paolo, Tobia, Antonino, Xie, Fei, Amici, Fabrizio, Attinà, Primo, Bachetti, Matteo, Brienza, Daniele, Centrone, Mauro, Costa, Enrico, Del Monte, Ettore, Di Cosimo, Sergio, Di Persio, Giuseppe, Evangelista, Yuri, Ferrazzoli, Riccardo, Loffredo, Pasqualino, Perri, Matteo, Pilia, Maura, Puccetti, Simonetta, Ratheesh, Ajay, Rubini, Alda, Santoli, Francesco, Scalise, Emanuele, and Trois, Alessio
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Instrumentation and Detectors
Abstract: The Imaging X-ray Polarimetry Explorer is a mission dedicated to the measurement of X-ray polarization from tens of astrophysical sources belonging to different classes. Expected to be launched at the end of 2021, the payload comprises three mirrors and three focal plane imaging polarimeters, the latter being designed and built in Italy. While calibration is always an essential phase in the development of high-energy space missions, for IXPE it has been particularly extensive both to calibrate the response to polarization, which is peculiar to IXPE, and to achieve a statistical uncertainty below the expected sensitivity. In this paper we present the calibration equipment that was designed and built at INAF-IAPS in Rome, Italy, for the calibration of the polarization-sensitive focal plane detectors on-board IXPE. Equipment includes calibration sources, both polarized and unpolarized, stages to align and move the beam, test detectors and their mechanical assembly. While all these equipments were designed to fit the specific needs of the IXPE Instrument calibration, their versatility could also be used in the future for other projects., Comment: 17 pages, 25 figures
Published: 2021
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6. The Instrument of the Imaging X-ray Polarimetry Explorer

Author: Soffitta, Paolo, Baldini, Luca, Bellazzini, Ronaldo, Costa, Enrico, Latronico, Luca, Muleri, Fabio, Del Monte, Ettore, Fabiani, Sergio, Minuti, Massimo, Pinchera, Michele, Sgrò, Carmelo, Spandre, Gloria, Trois, Alessio, Amici, Fabrizio, Andersson, Hans, Attinà, Primo, Bachetti, Matteo, Barbanera, Mattia, Borotto, Fabio, Brez, Alessandro, Brienza, Daniele, Caporale, Ciro, Cardelli, Claudia, Carpentiero, Rita, Castellano, Simone, Castronuovo, Marco, Cavalli, Luca, Cavazzuti, Elisabetta, Ceccanti, Marco, Centrone, Mauro, Ciprini, Stefano, Citraro, Saverio, Amico, Fabio D', Alba, Elisa D', Di Cosimo, Sergio, Di Lalla, Niccolò, Di Marco, Alessandro, Di Persio, Giuseppe, Donnarumma, Immacolata, Evangelista, Yuri, Ferrazzoli, Riccardo, Hayato, Asami, Kitaguchi, Takao, La Monaca, Fabio, Lefevre, Carlo, Loffredo, Pasqualino, Lorenzi, Paolo, Lucchesi, Leonardo, Magazzu, Carlo, Maldera, Simone, Manfreda, Alberto, Mangraviti, Elio, Marengo, Marco, Matt, Giorgio, Mereu, Paolo, Morbidini, Alfredo, Mosti, Federico, Nakano, Toshio, Nasimi, Hikmat, Negri, Barbara, Nenonen, Seppo, Nuti, Alessio, Orsini, Leonardo, Perri, Matteo, Rollins, Melissa Pesce, Piazzolla, Raffaele, Pilia, Maura, Profeti, Alessandro, Puccetti, Simonetta, Rankin, John, Ratheesh, Ajay, Rubini, Alda, Santoli, Francesco, Sarra, Paolo, Scalise, Emanuele, Sciortino, Andrea, Tamagawa, Toru, Tardiola, Marcello, Tobia, Antonino, Vimercati, Marco, and Xie, Fei
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: While X-ray Spectroscopy, Timing and Imaging have improved verymuch since 1962, when the first astronomical non-solar source was discovered, especially with the launch of Newton/X-ray Multi-Mirror Mission, Rossi/X-ray Timing Explorer and Chandra/Advanced X-ray Astrophysics Facility, the progress of X-ray polarimetry has been meager. This is in part due to the lack of sensitive polarization detectors, in part due to the fate of approved missions and in part because the celestial X-ray sources appeared less polarized than expected. Only one positive measurement has been available until now. Indeed the eight Orbiting Solar Observatory measured the polarization of the Crab nebula in the 70s. The advent of techniques of microelectronics allowed for designing a detector based on the photoelectric effect in gas in an energy range where the optics are efficient in focusing X-rays. Herewe describe the Instrument, which is the major contribution of the Italian collaboration to the SmallExplorer mission called IXPE, the Imaging X-ray Polarimetry Explorer, which will be flown in late 2021. The instrument, is composed of three Detector Units, based on this technique, and a Detector Service Unit. Three Mirror Modules provided by Marshall Space Flight Center focus X-rays onto the detectors. In the following we will show the technological choices, their scientific motivation and the results from the calibration of the Instrument. IXPE will perform imaging, timing and energy resolved polarimetry in the 2-8 keV energy band opening this window of X-ray astronomy to tens of celestial sources of almost all classes., Comment: 25 pages, 12 figures, 5 tables (accepted for publication in Astronomical Journal)
Published: 2021
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7. Design, Construction, and Test of the Gas Pixel Detectors for the IXPE Mission

Author: Baldini, L., Barbanera, M., Bellazzini, R., Bonino, R., Borotto, F., Brez, A., Caporale, C., Cardelli, C., Castellano, S., Ceccanti, M., Citraro, S., Di Lalla, N., Latronico, L., Lucchesi, L., Magazzù, C., Magazzù, G., Maldera, S., Manfreda, A., Marengo, M., Marrocchesi, A., Mereu, P., Minuti, M., Mosti, F., Nasimi, H., Nuti, A., Oppedisano, C., Orsini, L., Pesce-Rollins, M., Pinchera, M., Profeti, A., Sgrò, C., Spandre, G., Tardiola, M., Zanetti, D., Amici, F., Andersson, H., Attinà, P., Bachetti, M., Baumgartner, W., Brienza, D., Carpentiero, R., Castronuovo, M., Cavalli, L., Cavazzuti, E., Centrone, M., Costa, E., D'Alba, E., D'Amico, F., Del Monte, E., Di Cosimo, S., Di Marco, A., Di Persio, G., Donnarumma, I., Evangelista, Y., Fabiani, S., Ferrazzoli, R., Kitaguchi, T., La Monaca, F., Lefevre, C., Loffredo, P., Lorenzi, P., Mangraviti, E., Matt, G., Meilahti, T., Morbidini, A., Muleri, F., Nakano, T., Negri, B., Nenonen, S., O'Dell, S. L., Perri, M., Piazzolla, R., Pieraccini, S., Pilia, M., Puccetti, S., Ramsey, B. D., Rankin, J., Ratheesh, A., Rubini, A., Santoli, F., Sarra, P., Scalise, E., Sciortino, A., Soffitta, P., Tamagawa, T., Tennant, A. F., Tobia, A., Trois, A., Uchiyama, K., Vimercati, M., Weisskopf, M. C., Xie, F., Zanetti, F., and Zhou, Y.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Physics - Instrumentation and Detectors
Abstract: Due to be launched in late 2021, the Imaging X-Ray Polarimetry Explorer (IXPE) is a NASA Small Explorer mission designed to perform polarization measurements in the 2-8 keV band, complemented with imaging, spectroscopy and timing capabilities. At the heart of the focal plane is a set of three polarization-sensitive Gas Pixel Detectors (GPD), each based on a custom ASIC acting as a charge-collecting anode. In this paper we shall review the design, manufacturing, and test of the IXPE focal-plane detectors, with particular emphasis on the connection between the science drivers, the performance metrics and the operational aspects. We shall present a thorough characterization of the GPDs in terms of effective noise, trigger efficiency, dead time, uniformity of response, and spectral and polarimetric performance. In addition, we shall discuss in detail a number of instrumental effects that are relevant for high-level science analysis -- particularly as far as the response to unpolarized radiation and the stability in time are concerned., Comment: To be published in Astroparticle Physics
Published: 2021
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8. Observing strategy of the THESEUS mission

Author: Frontera, F., Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Campana, R., Fuschino, F., Labanti, C., Orlandini, M., Attinà, P., Contini, C., and Morelli, B.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We will discuss the observing strategy of the Transient High Energy Sky and Early Universe Surveyor (THESEUS) mission proposed to ESA as a response to the M5 call for proposals. The description of THESEUS and its science goals can be found in the white paper by Amati et al. (2017)., Comment: To be published in the Proceedings of the THESEUS Workshop 2017 (http://www.isdc.unige.ch/theseus/workshop2017.html), Journal of the Italian Astronomical Society (Mem.SAIt), Editors L. Amati, E. Bozzo, M. Della Valle, D. Gotz, P. O'Brien. Details on the THESEUS mission concept can be found in the white paper Amati et al. 2017 (arXiv:171004638) and Stratta et al. 2017 (arXiv:1712.08153)
Published: 2018

9. The THESEUS space mission concept: science case, design and expected performances

Author: Amati, L., O'Brien, P., Goetz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Floch, E. Le, Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Pata, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szecsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., and Zicha, J.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5-1 arcmin localization, an energy band extending from several MeV down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift $\sim$10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late '20s / early '30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA)., Comment: Accepted for publication in Advances in Space Research. Partly based on the proposal submitted on October 2016 in response to the ESA Call for next M5 mission, with expanded and updated science sections
Published: 2017
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10. XIPE: the x-ray imaging polarimetry explorer

Author: Soffitta, Paolo, Bellazzini, Ronaldo, Bozzo, Enrico, Burwitz, Vadim, Castro Tirado, Alberto, Costa, Enrico, Courvoisier, Thierry, Feng, Hua, Gburek, Szymon, Goosmann, Rene', Karas, Vladimir, Matt, Giorgio, Muleri, Fabio, Nandra, Kirpal, Pearce, Mark, Poutanen, Juri, Reglero, Victor, Graziati, Maria Dolores, Santangelo, Andrea, Tagliaferri, Gianpiero, Tenzer, Christopher, Vink, Jacco, Weisskopf, Martin, Zane, Silvia, Agudo, I, Antonelli, A, Attina, P, Baldini, L, Bykov, A, Carpentiero, R, Cavazzuti, E, Churazov, E, Del Monte, E, De Martino, D, Donnarumma, I, Doroshenko, V, Evangelista, Y, Ferreira, I, Gallo, E, Grosso, N, Kaaret, P, Kuulkers, E, Laranaga, J, Latronico, L, Lumb, DH, Macian, J, Malzac, J, Marin, F, Massaro, E, Minuti, M, Mundell, C, Ness, JU, Oosterbroek, T, Paltani, S, Pareschi, G, Perna, R, Petrucci, P-O, Pinazo, HB, Pinchera, M, Rodriguez, JP, Roncadelli, M, Santovincenzo, A, Sazonov, S, Sgro, C, Spiga, D, Svoboda, J, Theobald, C, Theodorou, T, Turolla, R, Wilhelmi de Ona, E, Winter, B, Akbar, AM, Allan, H, Aloisio, R, Altamirano, D, Amati, L, Amato, E, Angelakis, E, Arezu, J, Atteia, J-L, Axelsson, M, Bachetti, M, Ballo, L, Balman, S, Bandiera, R, Barcons, X, Basso, S, Baykal, A, Becker, W, Behar, E, Beheshtipour, B, Belmont, R, Berger, E, Bernardini, F, Bianchi, S, Bisnovatyi-Kogan, G, Blasi, P, Blay, P, Bodaghee, A, and Boer, M
Subjects: X-ray Astronomy, Polarimetry, X-ray optics, Gas Pixel Detector
Abstract: XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially-resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror but with a low weight. The payload is compatible with the fairing of the Vega launcher. XIPE is designed as an observatory for X-ray astronomers with 75 % of the time dedicated to a Guest Observer competitive program and it is organized as a consortium across Europe with main contributions from Italy, Germany, Spain, United Kingdom, Poland, Sweden.
Published: 2016

11. XIPE: The X-ray imaging polarimetry explorer

Author: Soffitta, P, Bellazzini, R, Bozzo, E, Burwitz, V, Castro-Tirado, AJ, Costa, E, Courvoisier, T, Feng, H, Gburek, S, Goosmann, R, Karas, V, Matt, G, Muleri, F, Nandra, K, Pearce, M, Poutanen, J, Reglero, V, Sabau Maria, D, Santangelo, A, Tagliaferri, G, Tenzer, C, Vink, J, Weisskopf, MC, Zane, S, Agudo, I, Antonelli, A, Attina, P, Baldini, L, Bykov, A, Carpentiero, R, Cavazzuti, E, Churazov, E, Del Monte, E, De Martino, D, Donnarumma, I, Doroshenko, V, Evangelista, Y, Ferreira, I, Gallo, E, Grosso, N, Kaaret, P, Kuulkers, E, Laranaga, J, Latronico, L, Lumb, DH, Macian, J, Malzac, J, Marin, F, Massaro, E, Minuti, M, Mundell, C, Ness, JU, Oosterbroek, T, Paltani, S, Pareschi, G, Perna, R, Petrucci, PO, Pinazo, HB, Pinchera, M, Rodriguez, JP, Roncadelli, M, Santovincenzo, A, Sazonov, S, Sgro, C, Spiga, D, Svoboda, J, Theobald, C, Theodorou, T, Turolla, R, Wilhelmi De Ona, E, Winter, B, Akbar, AM, Allan, H, Aloisio, R, Altamirano, D, Amati, L, Amato, E, Angelakis, E, Arezu, J, Atteia, JL, Axelsson, M, Bachetti, M, Ballo, L, Balman, S, Bandiera, R, Barcons, X, Basso, S, Baykal, A, Becker, W, Behar, E, Beheshtipour, B, Belmont, R, Berger, E, Bernardini, F, Bianchi, S, Bisnovatyi-Kogan, G, Blasi, P, Blay, P, Bodaghee, A, and Boer, M
Subjects: X-ray Astronomy, Polarimetry, X-ray optics, Gas Pixel Detector
Abstract: XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially-resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror but with a low weight. The payload is compatible with the fairing of the Vega launcher. XIPE is designed as an observatory for X-ray astronomers with 75 % of the time dedicated to a Guest Observer competitive program and it is organized as a consortium across Europe with main contributions from Italy, Germany, Spain, United Kingdom, Poland, Sweden.
Published: 2016

12. XIPE: the X-ray Imaging Polarimetry Explorer

Author: Soffitta, Paolo, Barcons, Xavier, Bellazzini, Ronaldo, Braga, João, Costa, Enrico, Fraser, George W., Gburek, Szymon, Huovelin, Juhani, Matt, Giorgio, Pearce, Mark, Poutanen, Juri, Reglero, Victor, Santangelo, Andrea, Sunyaev, Rashid A., Tagliaferri, Gianpiero, Weisskopf, Martin, Aloisio, Roberto, Amato, Elena, Attiná, Primo, Axelsson, Magnus, Baldini, Luca, Basso, Stefano, Bianchi, Stefano, Blasi, Pasquale, Bregeon, Johan, Brez, Alessandro, Bucciantini, Niccoló, Burderi, Luciano, Burwitz, Vadim, Casella, Piergiorgio, Churazov, Eugene, Civitani, Marta, Covino, Stefano, da Silva, Rui Miguel Curado, Cusumano, Giancarlo, Dadina, Mauro, D'Amico, Flavio, De Rosa, Alessandra, Di Cosimo, Sergio, Di Persio, Giuseppe, Di Salvo, Tiziana, Dovciak, Michal, Elsner, Ronald, Eyles, Chris J., Fabian, Andrew C., Fabiani, Sergio, Feng, Hua, Giarrusso, Salvatore, Goosmann, René W., Grandi, Paola, Grosso, Nicolas, Israel, Gianluca, Jackson, Miranda, Kaaret, Philip, Karas, Vladimir, Kuss, Michael, Lai, Dong, La Rosa, Giovanni, Larsson, Josefin, Larsson, Stefan, Latronico, Luca, Maggio, Antonio, Maia, Jorge, Marin, Frédéric, Massai, Marco Maria, Mineo, Teresa, Minuti, Massimo, Moretti, Elena, Muleri, Fabio, O'Dell, Stephen L., Pareschi, Giovanni, Peres, Giovanni, Pesce, Melissa, Petrucci, Pierre-Olivier, Pinchera, Michele, Porquet, Delphine, Ramsey, Brian, Rea, Nanda, Reale, Fabio, Rodrigo, Juana Maria, Różańska, Agata, Rubini, Alda, Rudawy, Pawel, Ryde, Felix, Salvati, Marco, Júnior, Valdivino Alexandre de Santiago, Sazonov, Sergey, Sgró, Carmelo, Silver, Eric, Spandre, Gloria, Spiga, Daniele, Stella, Luigi, Tamagawa, Toru, Tamborra, Francesco, Tavecchio, Fabrizio, Dias, Teresa Teixeira, van Adelsberg, Matthew, Wu, Kinwah, and Zane, Silvia
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract: X-ray polarimetry, sometimes alone, and sometimes coupled to spectral and temporal variability measurements and to imaging, allows a wealth of physical phenomena in astrophysics to be studied. X-ray polarimetry investigates the acceleration process, for example, including those typical of magnetic reconnection in solar flares, but also emission in the strong magnetic fields of neutron stars and white dwarfs. It detects scattering in asymmetric structures such as accretion disks and columns, and in the so-called molecular torus and ionization cones. In addition, it allows fundamental physics in regimes of gravity and of magnetic field intensity not accessible to experiments on the Earth to be probed. Finally, models that describe fundamental interactions (e.g. quantum gravity and the extension of the Standard Model) can be tested. We describe in this paper the X-ray Imaging Polarimetry Explorer (XIPE), proposed in June 2012 to the first ESA call for a small mission with a launch in 2017 but not selected. XIPE is composed of two out of the three existing JET-X telescopes with two Gas Pixel Detectors (GPD) filled with a He-DME mixture at their focus and two additional GPDs filled with pressurized Ar-DME facing the sun. The Minimum Detectable Polarization is 14 % at 1 mCrab in 10E5 s (2-10 keV) and 0.6 % for an X10 class flare. The Half Energy Width, measured at PANTER X-ray test facility (MPE, Germany) with JET-X optics is 24 arcsec. XIPE takes advantage of a low-earth equatorial orbit with Malindi as down-link station and of a Mission Operation Center (MOC) at INPE (Brazil)., Comment: 49 pages, 14 figures, 6 tables. Paper published in Experimental Astronomy http://link.springer.com/journal/10686
Published: 2013
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13. FTO-mediated cytoplasmic m6Am demethylation adjusts stem-like properties in colorectal cancer cell

Author: Relier, Sébastien, Ripoll, Julie, Guillorit, Hélène, Amalric, Amandine, Achour, Cyrinne, Boissière, Florence, Vialaret, Jérôme, Attina, Aurore, Debart, Françoise, Choquet, Armelle, Macari, Françoise, Marchand, Virginie, Motorin, Yuri, Samalin, Emmanuelle, Vasseur, Jean-Jacques, Pannequin, Julie, Aguilo, Francesca, Lopez-Crapez, Evelyne, Hirtz, Christophe, Rivals, Eric, Bastide, Amandine, and David, Alexandre
Published: 2021
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14. The LAUE project for broadband gamma-ray focusing lenses

Author: Virgilli, E., Frontera, F., Valsan, V., Liccardo, V., Caroli, E., Stephen, J. B., Cassese, F., Recanatesi, L., Pecora, M., Mottini, S., Attiná, P., and Negri, B.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We present the LAUE project devoted to develop an advanced technology for building a high focal length Laue lens for soft gamma--ray astronomy (80-600 keV). The final goal is to develop a focusing optics that can improve the current sensitivity in the above energy band by 2 orders of magnitude., Comment: 7 pages, 6 figures, presented at the SPIE conference on "Optics for EUV, X-ray, and Gamma-ray Astronomy". To be published in the Proceedings of SPIE, vol.8147, 2011
Published: 2011
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15. POLARIX: a pathfinder mission of X-ray polarimetry

Author: Costa, Enrico, Bellazzini, Ronaldo, Tagliaferri, Gianpiero, Matt, Giorgio, Argan, Andrea, Attina', Primo, Baldini, Luca, Basso, Stefano, Brez, Alessandro, Citterio, Oberto, Di Cosimo, Sergio, Cotroneo, Vincenzo, Fabiani, Sergio, Feroci, Marco, Ferri, Antonella, Latronico, Luca, Lazzarotto, Francesco, Minuti, Massimo, Morelli, Ennio, Muleri, Fabio, Nicolini, Lucio, Pareschi, Giovanni, Di Persio, Giuseppe, Pinchera, Michele, Razzano, Massimiliano, Reboa, Luigia, Rubini, Alda, Salonico, Antonio Maria, Sgro', Carmelo, Soffitta, Paolo, Spandre, Gloria, Spiga, Daniele, and Trois, Alessio
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Since the birth of X-ray astronomy, spectral, spatial and timing observation improved dramatically, procuring a wealth of information on the majority of the classes of the celestial sources. Polarimetry, instead, remained basically unprobed. X-ray polarimetry promises to provide additional information procuring two new observable quantities, the degree and the angle of polarization. POLARIX is a mission dedicated to X-ray polarimetry. It exploits the polarimetric response of a Gas Pixel Detector, combined with position sensitivity, that, at the focus of a telescope, results in a huge increase of sensitivity. Three Gas Pixel Detectors are coupled with three X-ray optics which are the heritage of JET-X mission. POLARIX will measure time resolved X-ray polarization with an angular resolution of about 20 arcsec in a field of view of 15 arcmin $\times$ 15 arcmin and with an energy resolution of 20 % at 6 keV. The Minimum Detectable Polarization is 12 % for a source having a flux of 1 mCrab and 10^5 s of observing time. The satellite will be placed in an equatorial orbit of 505 km of altitude by a Vega launcher.The telemetry down-link station will be Malindi. The pointing of POLARIX satellite will be gyroless and it will perform a double pointing during the earth occultation of one source, so maximizing the scientific return. POLARIX data are for 75 % open to the community while 25 % + SVP (Science Verification Phase, 1 month of operation) is dedicated to a core program activity open to the contribution of associated scientists. The planned duration of the mission is one year plus three months of commissioning and SVP, suitable to perform most of the basic science within the reach of this instrument., Comment: 42 pages, 28 figures
Published: 2011
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16. LOFT - a Large Observatory For x-ray Timing

Author: Feroci, M., Stella, L., Vacchi, A., Labanti, C., Rapisarda, M., Attinà, P., Belloni, T., Campana, R., Campana, S., Costa, E., Del Monte, E., Donnarumma, I., Evangelista, Y., Israel, G. L., Muleri, F., Porta, P., Rashevsky, A., Zampa, G., Zampa, N., Baldazzi, G., Bertuccio, G., Bonvicini, V., Bozzo, E., Burderi, L., Corongiu, A., Covino, S., Dall'Osso, S., De Martino, D., Di Cosimo, S., Di Persio, G., Di Salvo, T., Fuschino, F., Grassi, M., Lazzarotto, F., Malcovati, P., Marisaldi, M., Mastropietro, M., Mereghetti, S., Morelli, E., Orio, M., Pellizzoni, A., Pacciani, L., Papitto, A., Picolli, L., Possenti, A., Rubini, A., Soffitta, P., Turolla, R., and Zampieri, L.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The high time resolution observations of the X-ray sky hold the key to a number of diagnostics of fundamental physics, some of which are unaccessible to other types of investigations, such as those based on imaging and spectroscopy. Revealing strong gravitational field effects, measuring the mass and spin of black holes and the equation of state of ultradense matter are among the goals of such observations. At present prospects for future, non-focused X-ray timing experiments following the exciting age of RXTE/PCA are uncertain. Technological limitations are unavoidably faced in the conception and development of experiments with effective area of several square meters, as needed in order to meet the scientific requirements. We are developing large-area monolithic Silicon Drift Detectors offering high time and energy resolution at room temperature, which require modest resources and operation complexity (e.g., read-out) per unit area. Based on the properties of the detector and read-out electronics that we measured in the lab, we developed a realistic concept for a very large effective area mission devoted to X-ray timing in the 2-30 keV energy range. We show that effective areas in the range of 10-15 square meters are within reach, by using a conventional spacecraft platform and launcher of the small-medium class., Comment: 13 pages, 8 figures, 1 table, Proceedings of SPIE Vol. 7732, Paper No. 7732-66, 2010
Published: 2010
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17. Simbol-X Background Minimization: Mirror Spacecraft Passive Shielding Trade-Off Study

Author: Fioretti, V., Malaguti, G., Bulgarelli, A., Palumbo, G. G. C., Ferri, A., and Attina', P.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The present work shows a quantitative trade-off analysis of the Simbol-X Mirror Spacecraft (MSC) passive shielding, in the phase space of the various parameters: mass budget, dimension, geometry, and composition. A simplified physical (and geometrical) model of the sky screen, implemented by means of a GEANT4 simulation, has been developed to perform a performance-driven mass optimization and evaluate the residual background level on Simbol-X focal plane., Comment: 3 pages, 6 figures, to appear in the proceedings of the second Simbol-X International Symposium "Simbol-X - Focusing on the Hard X-ray Universe", AIP Conf. Proc. Series, P. Ferrando and J. Rodriguez eds
Published: 2009
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18. The Building of Regional Security Partnership and the Security Culture Divide in the Mediterranean Region

Author: Attina (Attinà), Fulvio
Subjects: comparative, European studies, Institute of European studies, integration, international, working paper
Abstract: Fulvio Attinà examines the concept of "regional security partnership" both theoretically and in the context of Euro-Mediterranean region-building. He argues that this partnership is an intermediate venture on the road to the possible appearance of a Euro-Mediterranean security community. By discussing the difficulties of negotiating a security partnership in the framework of the Euro-Mediterranean Partnership, Attinà highlights the security culture divide on both sides of Mediterranean. The differences in the security culture between European and Arab states have deepened in recent years in view of regional and global developments, constituting a major obstacle to the implementation of a security partnership. Attinà argues, however, that the interaction between the two shores of the Mediterranean in coping with globalization-driven problems may prevail over the factors that have led to a deepening of the security culture divide in recent years.
Published: 2004

19. Mass Spectrometry-Based Pipeline for Identifying RNA Modifications Involved in a Functional Process: Application to Cancer Cell Adaptation.

Author: Amalric, Amandine, Attina, Aurore, Bastide, Amandine, Buffard, Marion, Mateus, Stéphanie, Planque, Chris, Rivals, Eric, Hirtz, Christophe, and David, Alexandre
Published: 2024
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20. Cross-Language Perception of Cantonese Vowels Spoken by Native and Non-Native Speakers

Author: So, Connie K. and Attina, Virginie
Abstract: This study examined the effect of native language background on listeners' perception of native and non-native vowels spoken by native (Hong Kong Cantonese) and non-native (Mandarin and Australian English) speakers. They completed discrimination and an identification task with and without visual cues in clear and noisy conditions. Results indicated that visual cues did not facilitate perception, and performance was better in clear than in noisy conditions. More importantly, the Cantonese talker's vowels were the easiest to discriminate, and the Mandarin talker's vowels were as intelligible as the native talkers' speech. These results supported the interlanguage speech native intelligibility benefit patterns proposed by Hayes-Harb et al. ("J Phonetics" 36:664-679, 2008). The Mandarin and English listeners' identification patterns were similar to those of the Cantonese listeners, suggesting that they might have assimilated Cantonese vowels to their closest native vowels. In addition, listeners' perceptual patterns were consistent with the principles of Best's Perceptual Assimilation Model ("Best in Speech perception and linguistic experience: issues in cross-language research." York Press, Timonium, 1995).
Published: 2014
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21. Perceptual assimilation of lexical tone: The roles of language experience and visual information

Author: Reid, Amanda, Burnham, Denis, Kasisopa, Benjawan, Reilly, Ronan, Attina, Virginie, Rattanasone, Nan Xu, and Best, Catherine T.
Published: 2015
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22. CTA – the World’s largest ground-based gamma-ray observatory

Author: Zanin, Roberta, primary, Abdalla, H., additional, Abe, H., additional, Abe, S., additional, Abusleme, A., additional, Acero, F., additional, Acharyya, A., additional, Acin Portella, V., additional, Ackley, K., additional, Adam, R., additional, Adams, C., additional, Adhikari, S.S., additional, Aguado Ruesga, I., additional, Agudo, I., additional, Aguilera, R., additional, Aguirre Santaella, A., additional, Aharonian, F., additional, Alberdi, A., additional, Alfaro, R., additional, Alfaro, J., additional, Alispach, C., additional, Aloisio, R., additional, Alves Batista, R., additional, Amans, J.P., additional, Amati, L., additional, Amato, E., additional, Ambrogi, L., additional, Ambrosi, G., additional, Ambrosio, M., additional, Ammendola, R., additional, Anderson, J., additional, Anduze, M., additional, Anguner, E.O., additional, Antonelli, L.A., additional, Antonuccio, V., additional, Antoranz, P., additional, Anutarawiramkul, R., additional, Aragunde Gutierrez, J., additional, Aramo, C., additional, Araudo, A., additional, Araya, M., additional, Arbet Engels, A., additional, Arcaro, C., additional, Arendt, V., additional, Armand, C., additional, Armstrong, T., additional, Arqueros, F., additional, Arrabito, L., additional, Arsioli, B., additional, Artero, M., additional, Asano, K., additional, Ascasibar, Y., additional, Aschersleben, J., additional, Ashley, M., additional, Attina, P., additional, Aubert, P., additional, B. Singh, C., additional, Baack, D., additional, Babic, A., additional, Backes, M., additional, Baena, V., additional, Bajtlik, S., additional, Baktash, A., additional, Balazs, C., additional, Balbo, M., additional, Ballester, O., additional, Ballet, J., additional, Balmaverde, B., additional, Bamba, A., additional, Bandiera, R., additional, Baquero Larriva, A., additional, Barai, P., additional, Barbier, C., additional, Barbosa Martins, V., additional, Barcelo, M., additional, Barkov, M., additional, Barnard, M., additional, Baroncelli, L., additional, Barres de Almeida, U., additional, Barrio, J.A., additional, Bastieri, D., additional, Batista, P.I., additional, Batkovic, I., additional, Bauer, C., additional, Bautista González, R., additional, Baxter, J., additional, Becciani, U., additional, Becerra González, J., additional, Becherini, Y., additional, Beck, G., additional, Becker Tjus, J., additional, Bednarek, W., additional, Belfiore, A., additional, Bellizzi, L., additional, Belmont, R., additional, Benbow, W., additional, Berge, D., additional, Bernardini, E., additional, Bernardos, M.I., additional, Bernlöhr, K., additional, Berti, A., additional, Berton, M., additional, Bertucci, B., additional, Beshley, V., additional, Bhatt, N., additional, Bhattacharyya, S., additional, Bhattacharyya, W., additional, Bi, B. Y., additional, Bicknell, G., additional, Biederbeck, N., additional, Bigongiari, C., additional, Biland, A., additional, Bird, R., additional, Bissaldi, E., additional, Biteau, J., additional, Bitossi, M., additional, Blanch, O., additional, Blank, M., additional, Blazek, J., additional, Bobin, J., additional, Boccato, C., additional, Bocchino, F., additional, Boehm, C., additional, Bohacova, M., additional, Boisson, C., additional, Boix, J., additional, Bolle, J.P., additional, Bolmont, J., additional, Bonanno, G., additional, Bonavolontà, C., additional, Bonneau Arbeletche, L., additional, Bonnoli, G., additional, Bordas, P., additional, Borkowski, J., additional, Bose, R., additional, Bose, D., additional, Bosnjak, Z., additional, Bottacini, E., additional, Böttcher, Markus, additional, Botticella, M.T., additional, Boutonnet, C., additional, Bouyjou, F., additional, Bozhilov, V., additional, Bozzo, E., additional, Brahimi, L., additional, Braiding, C., additional, Brau Nogue, S., additional, Breen, S., additional, Bregeon, J., additional, Breuhaus, M., additional, Brill, A., additional, Brisken, W., additional, Brocato, E., additional, Brown, A.M., additional, Brügge, K., additional, Brun, P., additional, Brun, F., additional, Brunetti, L., additional, Brunetti, G., additional, Bruno, P., additional, Bruno, A., additional, Bruzzese, A., additional, Bucciantini, N., additional, Buckley, J. H., additional, Bühler, R., additional, Bulgarelli, A., additional, Bulik, T., additional, Bünning, M., additional, Bunse, M., additional, Burton, M., additional, Burtovoi, A., additional, Buscemi, M., additional, Buschjager, S., additional, Busetto, G., additional, Buss, J., additional, Byrum, K., additional, Caccianiga, A., additional, Cadoux, F., additional, Calanducci, A., additional, Calderon, C., additional, Calvo Tovar, J., additional, Cameron, R. A., additional, Campana, P., additional, Canestrari, R., additional, Cangemi, F., additional, Cantlay, B., additional, Capalbi, M., additional, Capasso, M., additional, Cappi, M., additional, Caproni, A., additional, Capuzzo Dolcetta, R., additional, Caraveo, P., additional, Cárdenas, V., additional, Cardiel, L., additional, Cardillo, M., additional, Carlile, C., additional, Caroff, S., additional, Carosi, R., additional, Carosi, A., additional, Carquin, E., additional, Carrere, M., additional, Casandjian, J.M., additional, Casanova, S., additional, Cassol, F., additional, Catalani, F., additional, Catalano, O., additional, Cauz, D., additional, Ceccanti, A., additional, Celestino Silva, C., additional, Cerny, K., additional, Cerruti, M., additional, Chabanne, E., additional, Chadwick, P., additional, Chai, Y., additional, Chambery, P., additional, Champion, C., additional, Chaty, S., additional, Chen, A., additional, Cheng, K., additional, Chernyakova, M., additional, Chiaro, G., additional, Chiavassa, A., additional, Chikawa, M., additional, Chitnis, V.R., additional, Chudoba, J., additional, Chytka, L., additional, Cikota, S., additional, Circiello, A., additional, Clark, P., additional, Colak, M., additional, Colombo, E., additional, Colonges, S., additional, Comastri, A., additional, Compagnino, A., additional, Conforti, V., additional, Congiu, E., additional, Coniglione, R., additional, Conrad, J., additional, Conte, F., additional, Contreras, J.L., additional, Coppi, P., additional, Cornat, R., additional, Coronado Blazquez, J., additional, Cortina, J., additional, Costa, A., additional, Costantini, H., additional, Cotter, G., additional, Courty, B., additional, Covino, S., additional, Crestan, S., additional, Cristofari, P., additional, Crocker, R., additional, Croston, J., additional, Cubuk, K., additional, Cuevas, O., additional, Cui, X., additional, Cusumano, G., additional, Cutini, S., additional, D'Amico, G., additional, D'Ammando, F., additional, D'Avanzo, P., additional, Da Vela, P., additional, Dadina, M., additional, Dai, S., additional, Dalchenko, M., additional, Dall'Ora, M., additional, Daniel, M.K., additional, Dauguet, J., additional, Davids, I., additional, Davies, J., additional, Dawson, B., additional, De Angelis, A., additional, de Araujo Carvalho, A.E., additional, de Bony de Lavergne, M., additional, De Cesare, G., additional, de Frondat, F., additional, de la Calle, I., additional, de Gouveia Dal Pino, E., additional, De Lotto, B., additional, De Luca, A., additional, De Martino, D., additional, de Naurois, M., additional, de Ona Wilhelmi, E., additional, De Palma Persio, F., additional, De Simone, N., additional, de Souza Valle, V., additional, Delagnes, E., additional, Deleglise Reznicek, G., additional, Delgado, C., additional, Delgado Giler, A.G., additional, Delgado Mengual Valle, J., additional, della Volpe, D., additional, Depaoli, D., additional, Devin, J., additional, Di Girolamo, T., additional, Di Giulio Pierro, C., additional, Di Venere, L., additional, Díaz, C., additional, Dib, C., additional, Diebold, S., additional, Digel, S., additional, Djannati Atai, A., additional, Djuvsland, J., additional, Dmytriiev, A., additional, Docher, K., additional, Domínguez, A., additional, Dominis Prester, D., additional, Donini, A., additional, Dorner, D., additional, Doro, M., additional, dos Anjos, Rita Cassia, additional, Dournaux, J.L., additional, Downes, T., additional, Drake, G., additional, Drass, H., additional, Dravins, D., additional, Duangchan, C., additional, Duara, A., additional, Dubus, G., additional, Ducci, L., additional, Duffy, C., additional, Dumora, D., additional, Dundas Mora, K., additional, Durkalec, A., additional, Dwarkadas, V.V., additional, Ebr, J., additional, Eckner, C., additional, Eder, J., additional, Edy, E., additional, Egberts, K., additional, Einecke, S., additional, Eleftheriadis, C., additional, Elsässer, D., additional, Emery, G., additional, Emmanoulopoulos, D., additional, Ernenwein, J.P., additional, Errando, M., additional, Escarate, P., additional, Escudero, J., additional, Espinoza, C., additional, Ettori, S., additional, Eungwanichayapant, A., additional, Evans, P., additional, Evoli, C., additional, Fairbairn, M., additional, Falceta Goncalves, D., additional, Falcone, A., additional, Fallah Ramazanı, V., additional, Falomo, R., additional, Farakos, K., additional, Fasola, G., additional, Fattorini, A., additional, Favre, Y., additional, Fedora, R., additional, Fedorova, E., additional, Feijen, K., additional, Feng, Q., additional, Ferrand, G., additional, Ferrara, G., additional, Ferreira, O., additional, Fesquet, M., additional, Fiandrini, E., additional, Fiasson, A., additional, Filipovic, M., additional, Fink, D., additional, Finley, J.P., additional, Fioretti, V., additional, Fiorillo, D.F.G., additional, Fiorini, M., additional, Flis, S., additional, Flores, H., additional, Foffano, L., additional, Fohr, C., additional, Fonseca, M.V., additional, Font, L., additional, Fontaine, G., additional, Fornieri, O., additional, Fortin, P., additional, Fortson, L., additional, Fouque, N., additional, Fraga, B., additional, Franceschini, A., additional, Franco, F.J., additional, Freixas Coromina, L., additional, Fresnillo, L., additional, Fugazza, D., additional, Fujita, Y., additional, Fukami, S., additional, Fukazawa, Y., additional, Fulla, D., additional, Funk, S., additional, Furniss, A., additional, Gabici, S., additional, Gaggero, D., additional, Galanti, G., additional, Galdemard, P., additional, Gallant, Y. A., additional, Galloway, D., additional, Gallozzi, S., additional, Gammaldi, V., additional, Garcia, R., additional, García-Muñoz, L. 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M., additional, Martin, P. 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Rando, R., additional, Razzaque, S., additional, Recchia, S., additional, Reichherzer, P., additional, Reimer, O., additional, Reisenegger, A., additional, Remy, Q., additional, Renaud, M., additional, Reposeur, T., additional, Reville, B., additional, Reymond, J.M., additional, Reynolds, J., additional, Ribeiro, D., additional, Ribo, M., additional, Richards, G., additional, Rico, J., additional, Rieger, F., additional, Riitano, L., additional, Riquelme, M., additional, Riquelme, D., additional, Rivoire, S., additional, Rizi, V., additional, Roache, E., additional, Roche, M., additional, Rodriguez, J., additional, Rodriguez Fernandez, G., additional, Rodriguez Ramirez, J.C., additional, Rodriguez Vazquez, J.J., additional, Rojas, G., additional, Romano, P., additional, Romeo Lobato, G., additional, Romoli, C., additional, Roncadelli, M., additional, Rosado, J., additional, Rosales de Leon, A., additional, Rowell, G., additional, Rugliancich, A., additional, Ruiz del Mazo, J.E., 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P., additional, Schussler, F., additional, Schwab, B., additional, Schwanke, U., additional, Schwarz, J., additional, Sciacca, E., additional, Scuderi, S., additional, Seglar Arroyo, M., additional, Seitenzahl, I., additional, Semikoz, D., additional, Sergijenko, O., additional, Serna Franco, J.E., additional, Seweryn, Karol, additional, Sguera, V., additional, Shalchi, A., additional, Shang, R.Y., additional, Sharma, P., additional, Sidoli, L., additional, Sieiro, J., additional, Siejkowski, H., additional, Sillanpaa, A., additional, Singh, B.B., additional, Singh, K.K., additional, Sinha, A., additional, Siqueira, C., additional, Sitarek, J., additional, Sizun, P., additional, Sliusar, V., additional, Sobczynska, D., additional, Sobrinho, R.W., additional, Sol, H., additional, Sottile, G., additional, Spackman, H., additional, Spencer, S., additional, Spengler, G., additional, Spiga, D., additional, Springer, W., additional, Stamerra, A., additional, Stanic, S., additional, Starling, 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L., additional, Wierzcholska, A., additional, Wiesand, S., additional, Wijers, R., additional, Wilkinson, M., additional, Will, M., additional, Williams, J., additional, Williamson, T. J., additional, Wolter, A., additional, Wong, Y.W., additional, Wood, M., additional, Yamamoto, T., additional, Yamamoto, H., additional, Yamane, Y., additional, Yamazaki, R., additional, Yanagita, S., additional, Yang, L., additional, Yoo, S., additional, Yoshida, T., additional, Yoshikoshi, T., additional, Yu, P., additional, Yusafzai, A., additional, Zacharias, Michael, additional, Zaldivar, B., additional, Zampieri, L., additional, Zanin, R., additional, Zanmar Sanchez, R., additional, Zaric, D., additional, Zavrtanik, M., additional, Zavrtanik, D., additional, Zdziarski, Andrzej, additional, Zech, A., additional, Zechlin, H., additional, Zenin, A., additional, Zerwekh, A., additional, Ziętara, K., additional, Zink, A., additional, Ziolkowski, J., additional, Zivec, M., additional, and Zmija, A., additional
Published: 2021
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23. E4F1 coordinates pyruvate metabolism and the activity of the elongator complex to ensure translation fidelity during brain development

Author: Di Michele, Michela, Attina, Aurore, Roux, Pierre-François, Tabet, Imène, Laguesse, Sophie, Florido, Javier, Houdeville, Morane, Choquet, Armelle, Encislai, Betty, Arena, Giuseppe, De Blasio, Carlo, Wendling, Olivia, Frenois, François-Xavier, Papon, Laura, Stuani, Lucille, Fuentes, Maryse, Jahannault Talignani, Céline, Rousseau, Mélanie, Guégan, Justine, Buscail, Yoan, Dupré, Pierrick, Michaud, Henri-Alexandre, Rodier, Geneviève, Bellvert, Floriant, Kulyk, Hanna, Ferraro Peyret, Carole, Mathieu, Hugo, Close, Pierre, Rapino, Francesca, Chaveroux, Cédric, Pirot, Nelly, Rubio, Lucie, Torro, Adeline, Sorg, Tania, Ango, Fabrice, Hirtz, Christophe, Compan, Vincent, Lebigot, Elise, Legati, Andrea, Ghezzi, Daniele, Nguyen, Laurent, David, Alexandre, Sardet, Claude, Lacroix, Matthieu, and Le Cam, Laurent
Published: 2025
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24. Conservative and Surgical Treatment of Chronic Anal Fissure: Prospective Longer Term Results

Author: Sileri, Pierpaolo, Stolfi, Vito M., Franceschilli, Luana, Grande, Michele, Di Giorgio, Alessandra, D’Ugo, Stefano, Attina’, Grazia, D’Eletto, Marco, and Gaspari, Achille L.
Published: 2010
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25. Multivariate Analysis of RNA Chemistry Marks Uncovers Epitranscriptomics-Based Biomarker Signature for Adult Diffuse Glioma Diagnostics.

Author: Relier, S., Amalric, A., Attina, A., Koumare, I.B., Rigau, V., Burel Vandenbos, F., Fontaine, D., Baroncini, M., Hugnot, J.P., Duffau, H., Bauchet, L., Hirtz, C., Rivals, E., and David, A.
Published: 2022
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26. Recent advances and low cost concept for the gamma-ray lens project MAX

Author: Leyre, Xavier, Sghedoni, Michel, Arbusti, Francis, Attina, Primo, and von Ballmoos, Peter
Published: 2005
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27. Update of penetrance estimates in Birt-Hogg-Dubé syndrome

Author: Bruinsma, Fiona Jane, Dowty, James G, Win, Aung Ko, Goddard, Laura C, Agrawal, Prachi, Attina', Domenico, Bissada, Nabil, De Luise, Monica, Eisen, Daniel B, Furuya, Mitsuko, Gasparre, Giuseppe, Genuardi, Maurizio, Gerdes, Anne-Marie, Hansen, Thomas Van Overeem, Houweling, Arjan C, Johannesma, Paul Christiaan, Lencastre, André, Lim, Derek, Lindor, Noralane M, Luzzi, Valentina, Lynch, Maeve, Maffé, Antonella, Menko, Fred H, Michels, Guido, Pulido, Jose S, Ryu, Jay H, Sattler, Elke C, Steinlein, Ortrud K, Tomassetti, Sara, Tucker, Kathy, Turchetti, Daniela, van de Beek, Irma, van Riel, Lore, van Steensel, Maurice, Zenone, Thierry, Zompatori, Maurizo, Walsh, Jennifer, Bondavalli, Davide, Maher, Eamonn R, and Winship, Ingrid M
Abstract: BackgroundBirt-Hogg-Dubé (BHD) syndrome is a rare genetic syndrome caused by pathogenic or likely pathogenic germline variants in the FLCNgene. Patients with BHD syndrome have an increased risk of fibrofolliculomas, pulmonary cysts, pneumothorax and renal cell carcinoma. There is debate regarding whether colonic polyps should be added to the criteria. Previous risk estimates have mostly been based on small clinical case series.MethodsA comprehensive review was conducted to identify studies that had recruited families carrying pathogenic or likely pathogenic variants in FLCN. Pedigree data were requested from these studies and pooled. Segregation analysis was used to estimate the cumulative risk of each manifestation for carriers of FLCNpathogenic variants.ResultsOur final dataset contained 204 families that were informative for at least one manifestation of BHD (67 families informative for skin manifestations, 63 for lung, 88 for renal carcinoma and 29 for polyps). By age 70 years, male carriers of the FLCNvariant have an estimated 19% (95% CI 12% to 31%) risk of renal tumours, 87% (95% CI 80% to 92%) of lung involvement and 87% (95% CI 78% to 93%) of skin lesions, while female carriers had an estimated 21% (95% CI 13% to 32%) risk of renal tumours, 82% (95% CI 73% to 88%) of lung involvement and 78% (95% CI 67% to 85%) of skin lesions. The cumulative risk of colonic polyps by age 70 years old was 21% (95% CI 8% to 45%) for male carriers and 32% (95% CI 16% to 53%) for female carriers.ConclusionsThese updated penetrance estimates, based on a large number of families, are important for the genetic counselling and clinical management of BHD syndrome.
Published: 2023
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28. The THESEUS space mission concept: science case, design and expected performances

Author: Amati, L, O'Brien, P, Götz, D, Bozzo, E, Tenzer, C, Frontera, F, Ghirlanda, G, Labanti, C, Osborne, J, Stratta, G, Tanvir, N, Willingale, R, Attina, P, Campana, R, Castro-Tirado, A, Contini, C, Fuschino, F, Gomboc, A, Hudec, R, Orleanski, P, Renotte, E, Rodic, T, Bagoly, Z, Blain, A, Callanan, P, Covino, S, Ferrara, A, Le Floch, E, Marisaldi, M, Mereghetti, S, Rosati, P, Vacchi, A, D'Avanzo, P, Giommi, P, Piranomonte, S, Piro, L, Reglero, V, Rossi, A, Santangelo, A, Salvaterra, R, Tagliaferri, G, Vergani, S, Vinciguerra, S, Briggs, M, Campolongo, E, Ciolfi, R, Connaughton, V, Cordier, B, Morelli, B, Orlandini, M, Adami, C, Argan, A, Atteia, J, Auricchio, N, Balazs, L, Baldazzi, G, Basa, S, Basak, R, Bellutti, P, Bernardini, M, Bertuccio, G, Braga, J, Branchesi, M, Brandt, S, Brocato, E, Budtz-Jorgensen, C, Bulgarelli, A, Burderi, L, Camp, J, Capozziello, S, Caruana, J, Casella, P, Cenko, B, Chardonnet, P, Ciardi, B, Colafrancesco, S, Dainotti, M, D'Elia, V, De Martino, D, De Pasquale, M, Del Monte, E, Della Valle, M, Drago, A, Evangelista, Y, Feroci, M, Finelli, F, Fiorini, M, Fynbo, J, Gal-Yam, A, Gendre, B, Ghisellini, G, Grado, A, Guidorzi, C, Hafizi, M, Hanlon, L, Hjorth, J, Izzo, L, Kiss, L, Kumar, P, Kuvvetli, I, Lavagna, M, Li, T, Longo, F, Lyutikov, M, Maio, U, Maiorano, E, Malcovati, P, Malesani, D, Margutti, R, Martin-Carrillo, A, Masetti, N, Mcbreen, S, Mignani, R, Morgante, G, Mundell, C, Nargaard-Nielsen, H, Nicastro, L, Palazzi, E, Paltani, S, Panessa, F, Pareschi, G, Pe'Er, A, Penacchioni, A, Pian, E, Piedipalumbo, E, Piran, T, Rauw, G, Razzano, M, Read, A, Rezzolla, L, Romano, P, Ruffini, R, Savaglio, S, Sguera, V, Schady, P, Skidmore, W, Song, L, Stanway, E, Starling, R, Topinka, M, Troja, E, van Putten, M, Vanzella, E, Vercellone, S, Wilson-Hodge, C, Yonetoku, D, Zampa, G, Zampa, N, Zhang, B, Zhang, S, Antonelli, A, Bianco, F, Boci, S, Boer, M, Botticella, M, Boulade, O, Butler, C, Campana, S, Capitanio, F, Celotti, A, Chen, Y, Colpi, M, Comastri, A, Cuby, J, Dadina, M, De Luca, A, Dong, Y, Ettori, S, Gandhi, P, Geza, E, Greiner, J, Guiriec, S, Harms, J, Hernanz, M, Hornstrup, A, Hutchinson, I, Israel, G, Jonker, P, Kaneko, Y, Kawai, N, Wiersema, K, Korpela, S, Lebrun, V, Lu, F, Macfadyen, A, Malaguti, G, Maraschi, L, Melandri, A, Modjaz, M, Morris, D, Omodei, N, Paizis, A, Páta, P, Petrosian, V, Rachevski, A, Rhoads, J, Ryde, F, Sabau-Graziati, L, Shigehiro, N, Sims, M, Soomin, J, Szécsi, D, Urata, Y, Uslenghi, M, Valenziano, L, Vianello, G, Vojtech, S, Watson, D, Zicha, J, Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., Zicha, J., Amati, L, O'Brien, P, Götz, D, Bozzo, E, Tenzer, C, Frontera, F, Ghirlanda, G, Labanti, C, Osborne, J, Stratta, G, Tanvir, N, Willingale, R, Attina, P, Campana, R, Castro-Tirado, A, Contini, C, Fuschino, F, Gomboc, A, Hudec, R, Orleanski, P, Renotte, E, Rodic, T, Bagoly, Z, Blain, A, Callanan, P, Covino, S, Ferrara, A, Le Floch, E, Marisaldi, M, Mereghetti, S, Rosati, P, Vacchi, A, D'Avanzo, P, Giommi, P, Piranomonte, S, Piro, L, Reglero, V, Rossi, A, Santangelo, A, Salvaterra, R, Tagliaferri, G, Vergani, S, Vinciguerra, S, Briggs, M, Campolongo, E, Ciolfi, R, Connaughton, V, Cordier, B, Morelli, B, Orlandini, M, Adami, C, Argan, A, Atteia, J, Auricchio, N, Balazs, L, Baldazzi, G, Basa, S, Basak, R, Bellutti, P, Bernardini, M, Bertuccio, G, Braga, J, Branchesi, M, Brandt, S, Brocato, E, Budtz-Jorgensen, C, Bulgarelli, A, Burderi, L, Camp, J, Capozziello, S, Caruana, J, Casella, P, Cenko, B, Chardonnet, P, Ciardi, B, Colafrancesco, S, Dainotti, M, D'Elia, V, De Martino, D, De Pasquale, M, Del Monte, E, Della Valle, M, Drago, A, Evangelista, Y, Feroci, M, Finelli, F, Fiorini, M, Fynbo, J, Gal-Yam, A, Gendre, B, Ghisellini, G, Grado, A, Guidorzi, C, Hafizi, M, Hanlon, L, Hjorth, J, Izzo, L, Kiss, L, Kumar, P, Kuvvetli, I, Lavagna, M, Li, T, Longo, F, Lyutikov, M, Maio, U, Maiorano, E, Malcovati, P, Malesani, D, Margutti, R, Martin-Carrillo, A, Masetti, N, Mcbreen, S, Mignani, R, Morgante, G, Mundell, C, Nargaard-Nielsen, H, Nicastro, L, Palazzi, E, Paltani, S, Panessa, F, Pareschi, G, Pe'Er, A, Penacchioni, A, Pian, E, Piedipalumbo, E, Piran, T, Rauw, G, Razzano, M, Read, A, Rezzolla, L, Romano, P, Ruffini, R, Savaglio, S, Sguera, V, Schady, P, Skidmore, W, Song, L, Stanway, E, Starling, R, Topinka, M, Troja, E, van Putten, M, Vanzella, E, Vercellone, S, Wilson-Hodge, C, Yonetoku, D, Zampa, G, Zampa, N, Zhang, B, Zhang, S, Antonelli, A, Bianco, F, Boci, S, Boer, M, Botticella, M, Boulade, O, Butler, C, Campana, S, Capitanio, F, Celotti, A, Chen, Y, Colpi, M, Comastri, A, Cuby, J, Dadina, M, De Luca, A, Dong, Y, Ettori, S, Gandhi, P, Geza, E, Greiner, J, Guiriec, S, Harms, J, Hernanz, M, Hornstrup, A, Hutchinson, I, Israel, G, Jonker, P, Kaneko, Y, Kawai, N, Wiersema, K, Korpela, S, Lebrun, V, Lu, F, Macfadyen, A, Malaguti, G, Maraschi, L, Melandri, A, Modjaz, M, Morris, D, Omodei, N, Paizis, A, Páta, P, Petrosian, V, Rachevski, A, Rhoads, J, Ryde, F, Sabau-Graziati, L, Shigehiro, N, Sims, M, Soomin, J, Szécsi, D, Urata, Y, Uslenghi, M, Valenziano, L, Vianello, G, Vojtech, S, Watson, D, Zicha, J, Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., and Zicha, J.
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5–1 arcmin localization, an energy band extending from several MeV down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift ∼10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ’20s/early ’30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).
Published: 2018

29. A newborn with multiple fractures as first presentation of infantile myofibromatosis

Author: Buonuomo, P S, Ruggiero, A, Zampino, G, Maurizi, P, Attina, G, and Riccardi, R
Published: 2006
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30. Aromatic substitution in the complexes formed upon addition of gaseous arenium ions to proelectrophiles. A FT-ICR study

Author: Aschi, Massimiliano, Attina, Marina, and Cacace, Fulvio
Published: 1996
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31. XIPE: the x-ray imaging polarimetry explorer

Author: Soffitta, P., Bellazzini, R., Bozzo, E., Burwitz, V., Castro Tirado, A. J., Costa, E., Courvoisier, T., Feng, H., Gburek, S., Goosmann, R., Karas, V., Boettcher, M., Bogdanov, S., Bombaci, I., Bonino, R., Braga, J., Brandt, W., Brez, A., Bucciantini, N., Burderi, L., Caiazzo, I., Matt, G., Campana, R., Campana, S., Capitanio, F., Cappi, M., Cardillo, M., Casella, P., Catmabacak, O., Cenko, B., Cerda Duran, P., Cerruti, C., Muleri, F., Chaty, S., Chauvin, M., Chen, Y., Chenevez, J., Chernyakova, M., Cheung Teddy, C. C., Christodoulou, D., Connell, P., Corbet, R., Coti Zelati, F., Nandra, K., Covino, S., Cui, W., Cusumano, G., D'Ai, A., D'Ammando, F., Dadina, M., Dai, Z., De Rosa, A., De Ruvo, L., Degenaar, N., Pearce, M., Del Santo, M., Del Zanna, L., Dewangan, G., Di Cosimo, S., Di Lalla, N., Di Persio, G., Di Salvo, T., Dias, T., Done, C., Dovciak, M., Poutanen, J., Doyle, G., Ducci, L., Elsner, R., Enoto, T., Escada, J., Esposito, P., Eyles, C., Fabiani, S., Falanga, M., Falocco, S., Reglero, V., Fan, Y., Fender, R., Feroci, M., Ferrigno, C., Forman, W., Foschini, L., Fragile, C., Fuerst, F., Fujita, Y., Gasent Blesa, J. L., Sabau Maria, D., Gelfand, J., Gendre, B., Ghirlanda, G., Ghisellini, G., Giroletti, M., Goetz, D., Gogus, E., Gomez, J. 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J., Costa, E., Courvoisier, T., Feng, H., Gburek, S., Goosmann, R., Karas, V., Matt, G., Muleri, F., Nandra, K., Pearce, M., Poutanen, J., Reglero, V., Sabau Maria, D., Santangelo, A., Tagliaferri, G., Tenzer, C., Vink, J., Weisskopf, M. C., Zane, S., Agudo, I., Antonelli, A., Attina, P., Baldini, L., Bykov, A., Carpentiero, R., Cavazzuti, E., Churazov, E., Del Monte, E., De Martino, D., Donnarumma, I., Doroshenko, V., Evangelista, Y., Ferreira, I., Gallo, E., Grosso, N., Kaaret, P., Kuulkers, E., Laranaga, J., Latronico, L., Lumb, D. H., Macian, J., Malzac, J., Marin, F., Massaro, E., Minuti, M., Mundell, C., Ness, J. U., Oosterbroek, T., Paltani, S., Pareschi, G., Perna, R., Petrucci, P. -O., Pinazo, H. B., Pinchera, M., Rodriguez, J. P., Roncadelli, M., Santovincenzo, A., Sazonov, S., Sgro, C., Spiga, D., Svoboda, J., Theobald, C., Theodorou, T., Turolla, R., Wilhelmi De Ona, E., Winter, B., Akbar, A. M., Allan, H., Aloisio, R., Altamirano, D., Amati, L., Amato, E., Angelakis, E., Arezu, J., Atteia, J. -L., Axelsson, M., Bachetti, M., Ballo, L., Balman, S., Bandiera, R., Barcons, X., Basso, S., Baykal, A., Becker, W., Behar, E., Beheshtipour, B., Belmont, R., Berger, E., Bernardini, F., Bianchi, S., Bisnovatyi-Kogan, G., Blasi, P., Blay, P., Bodaghee, A., Boer, M., Boettcher, M., Bogdanov, S., Bombaci, I., Bonino, R., Braga, J., Brandt, W., Brez, A., Bucciantini, N., Burderi, L., Caiazzo, I., Campana, R., Campana, S., Capitanio, F., Cappi, M., Cardillo, M., Casella, P., Catmabacak, O., Cenko, B., Cerda-Duran, P., Cerruti, C., Chaty, S., Chauvin, M., Chen, Y., Chenevez, J., Chernyakova, M., Cheung Teddy, C. C., Christodoulou, D., Connell, P., Corbet, R., Coti Zelati, F., Covino, S., Cui, W., Cusumano, G., D'Ai, A., D'Ammando, F., Dadina, M., Dai, Z., De Rosa, A., De Ruvo, L., Degenaar, N., Del Santo, M., Del Zanna, L., Dewangan, G., Di Cosimo, S., Di Lalla, N., Di Persio, G., Di Salvo, T., Dias, T., Done, C., Dovciak, M., Doyle, G., Ducci, L., Elsner, R., Enoto, T., Escada, J., Esposito, P., Eyles, C., Fabiani, S., Falanga, M., Falocco, S., Fan, Y., Fender, R., Feroci, M., Ferrigno, C., Forman, W., Foschini, L., Fragile, C., Fuerst, F., Fujita, Y., Gasent-Blesa, J. L., Gelfand, J., Gendre, B., Ghirlanda, G., Ghisellini, G., Giroletti, M., Goetz, D., Gogus, E., Gomez, J. -L., Gonzalez, D., Gonzalez-Riestra, R., Gotthelf, E., Gou, L., Grandi, P., Grinberg, V., Grise, F., Guidorzi, C., Gurlebeck, N., Guver, T., Haggard, D., Hardcastle, M., Hartmann, D., Haswell, C., Heger, A., Hernanz, M., Heyl, J., Ho, L., Hoormann, J., Horak, J., Huovelin, J., Huppenkothen, D., Iaria, R., Inam Sitki, C., Ingram, A., Israel, G., Izzo, L., Burgess, M., Jackson, M., Ji, L., Jiang, J., Johannsen, T., Jones, C., Jorstad, S., Kajava, J. J. E., Kalamkar, M., Kalemci, E., Kallman, T., Kamble, A., Kislat, F., Kiss, M., Klochkov, D., Koerding, E., Kolehmainen, M., Koljonen, K., Komossa, S., Kong, A., Korpela, S., Kowalinski, M., Krawczynski, H., Kreykenbohm, I., Kuss, M., Lai, D., Lan, M., Larsson, J., Laycock, S., Lazzati, D., Leahy, D., Li, H., Li, J., Li, L. -X., Li, T., Li, Z., Linares, M., Lister, M., Liu, H., Lodato, G., Lohfink, A., Longo, F., Luna, G., Lutovinov, A., Mahmoodifar, S., Maia, J., Mainieri, V., Maitra, C., Maitra, D., Majczyna, A., Maldera, S., Malyshev, D., Manfreda, A., Manousakis, A., Manuel, R., Margutti, R., Marinucci, A., Markoff, S., Marscher, A., Marshall, H., Massaro, F., Mclaughlin, M., Medina-Tanco, G., Mehdipour, M., Middleton, M., Mignani, R., Mimica, P., Mineo, T., Mingo, B., Miniutti, G., Mirac, S. M., Morlino, G., Motlagh, A. V., Motta, S. E., Mushtukov, A., Nagataki, S., Nardini, F., Nattila, J., Navarro, G. 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S., Schwope, A., Severgnini, P., Sharon, M., Shaw, A., Shearer, A., Shesheng, X., Shih, I. -C., Silva, K., Silva, R., Silver, E., Smale, A., Spada, F., Spandre, G., Stamerra, A., Stappers, B., Starrfield, S., Stawarz, L., Stergioulas, N., Stevens, A., Stiele, H., Suleimanov, V., Sunyaev, R., Slowikowska, A., Tamborra, F., Tavecchio, F., Taverna, R., Tiengo, A., Tolos, L., Tombesi, F., Tomsick, J., Tong, H., Torok, G., Torres, D. F., Tortosa, A., Tramacere, A., Trimble, V., Trinchieri, G., Tsygankov, S., Tuerler, M., Turriziani, S., Ursini, F., Uttley, P., Varniere, P., Vincent, F., Vurgun, E., Wang, C., Wang, Z., Watts, A., Wheeler, J. C., Wiersema, K., Wijnands, R., Wilms, J., Wolter, A., Wood, K., Wu, K., Wu, X., Xiangyu, W., Xie, F., Xu, R., Yan, S. -P., Yang, J., Yu, W., Yuan, F., Zajczyk, A., Zanetti, D., Zanin, R., Zanni, C., Zappacosta, L., Zdziarski, A. A., Zech, A., Zhang, H., Zhang, S., Zhang, W., Zoghbi, A., Jan-Willem A. den Herder, Tadayuki Takahashi, Marshall Bautz, Castro-Tirado, A., Weisskopf, M., Lumb, D., Ness, J., Petrucci, P., Pinazo, H., Akbar, A., Atteia, J., Cheung Teddy, C., Gasent-Blesa, J., Gomez, J., Kajava, J., Li, L., Mirac, S., Motlagh, A., Motta, S., Navarro, G., Paliya, V., Pili, A., Rossi, M., Schulz, N., Shih, I., Torres, D., Wheeler, J., Yan, S., and Zdziarski, A.
Subjects: X-ray Astronomy, High-energy astronomy, Polarimetry, X-ray optics, X-ray telescope, Condensed Matter Physic, 01 natural sciences, Observatory, 0103 physical sciences, Electronic, Optical and Magnetic Materials, Spectral resolution, Electrical and Electronic Engineering, 010303 astronomy & astrophysics, Gas Pixel Detector, Physics, X-ray astronomy, ta115, 010308 nuclear & particles physics, Electronic, Optical and Magnetic Material, Applied Mathematics, Vega, Astronomy, Computer Science Applications1707 Computer Vision and Pattern Recognition, Condensed Matter Physics, Computer Science Applications, Applied Mathematic, Electronic, Optical and Magnetic Materials, Computer Vision and Pattern Recognition, X-ray optic
Abstract: XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror but with a low weight. The payload is compatible with the fairing of the Vega launcher. XIPE is designed as an observatory for X-ray astronomers with 75 % of the time dedicated to a Guest Observer competitive program and it is organized as a consortium across Europe with main contributions from Italy, Germany, Spain, United Kingdom, Poland, Sweden.
Published: 2016

32. Characteristics of preeclampsia in donor cell gestations.

Author: Ervaala, Attina, Laivuori, Hannele, Gissler, Mika, Kere, Juha, Kivinen, Katja, Pouta, Anneli, Kajantie, Eero, Heinonen, Seppo, and Wedenoja, Satu
Abstract: Pregnancies conceived through donor oocytes or sperm show increased risk for preeclampsia. We studied this issue in a preeclampsia case-control cohort (n = 2778), and found overrepresentation of donor cell gestations among women with preeclampsia (14/1627, 0.86%; OR 1.81; 95% CI: 1.07-3.08; P = 0.025) compared to the population data. Moreover, we observed excess of male births from donor cell pregnancies (male-to-female ratio 2.5 vs. 0.97; OR 2.57; 95% CI 1.02-6.36; P = 0.043). Maternal age (36.7 vs. 30.2; P < 0.0001) and preterm deliveries (64% vs. 38%; P = 0.046) distinguished donor cell gestations from other pregnancies with preeclampsia. These results support foreign fetal antigens as modulators of preeclampsia. [ABSTRACT FROM AUTHOR]
Published: 2022
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33. The THESEUS space mission concept: science case, design and expected performances

Author: Amati, L., primary, O’Brien, P., additional, Götz, D., additional, Bozzo, E., additional, Tenzer, C., additional, Frontera, F., additional, Ghirlanda, G., additional, Labanti, C., additional, Osborne, J.P., additional, Stratta, G., additional, Tanvir, N., additional, Willingale, R., additional, Attina, P., additional, Campana, R., additional, Castro-Tirado, A.J., additional, Contini, C., additional, Fuschino, F., additional, Gomboc, A., additional, Hudec, R., additional, Orleanski, P., additional, Renotte, E., additional, Rodic, T., additional, Bagoly, Z., additional, Blain, A., additional, Callanan, P., additional, Covino, S., additional, Ferrara, A., additional, Le Floch, E., additional, Marisaldi, M., additional, Mereghetti, S., additional, Rosati, P., additional, Vacchi, A., additional, D’Avanzo, P., additional, Giommi, P., additional, Piranomonte, S., additional, Piro, L., additional, Reglero, V., additional, Rossi, A., additional, Santangelo, A., additional, Salvaterra, R., additional, Tagliaferri, G., additional, Vergani, S., additional, Vinciguerra, S., additional, Briggs, M., additional, Campolongo, E., additional, Ciolfi, R., additional, Connaughton, V., additional, Cordier, B., additional, Morelli, B., additional, Orlandini, M., additional, Adami, C., additional, Argan, A., additional, Atteia, J.-L., additional, Auricchio, N., additional, Balazs, L., additional, Baldazzi, G., additional, Basa, S., additional, Basak, R., additional, Bellutti, P., additional, Bernardini, M.G., additional, Bertuccio, G., additional, Braga, J., additional, Branchesi, M., additional, Brandt, S., additional, Brocato, E., additional, Budtz-Jorgensen, C., additional, Bulgarelli, A., additional, Burderi, L., additional, Camp, J., additional, Capozziello, S., additional, Caruana, J., additional, Casella, P., additional, Cenko, B., additional, Chardonnet, P., additional, Ciardi, B., additional, Colafrancesco, S., additional, Dainotti, M.G., additional, D’Elia, V., additional, De Martino, D., additional, De Pasquale, M., additional, Del Monte, E., additional, Della Valle, M., additional, Drago, A., additional, Evangelista, Y., additional, Feroci, M., additional, Finelli, F., additional, Fiorini, M., additional, Fynbo, J., additional, Gal-Yam, A., additional, Gendre, B., additional, Ghisellini, G., additional, Grado, A., additional, Guidorzi, C., additional, Hafizi, M., additional, Hanlon, L., additional, Hjorth, J., additional, Izzo, L., additional, Kiss, L., additional, Kumar, P., additional, Kuvvetli, I., additional, Lavagna, M., additional, Li, T., additional, Longo, F., additional, Lyutikov, M., additional, Maio, U., additional, Maiorano, E., additional, Malcovati, P., additional, Malesani, D., additional, Margutti, R., additional, Martin-Carrillo, A., additional, Masetti, N., additional, McBreen, S., additional, Mignani, R., additional, Morgante, G., additional, Mundell, C., additional, Nargaard-Nielsen, H.U., additional, Nicastro, L., additional, Palazzi, E., additional, Paltani, S., additional, Panessa, F., additional, Pareschi, G., additional, Pe’er, A., additional, Penacchioni, A.V., additional, Pian, E., additional, Piedipalumbo, E., additional, Piran, T., additional, Rauw, G., additional, Razzano, M., additional, Read, A., additional, Rezzolla, L., additional, Romano, P., additional, Ruffini, R., additional, Savaglio, S., additional, Sguera, V., additional, Schady, P., additional, Skidmore, W., additional, Song, L., additional, Stanway, E., additional, Starling, R., additional, Topinka, M., additional, Troja, E., additional, van Putten, M., additional, Vanzella, E., additional, Vercellone, S., additional, Wilson-Hodge, C., additional, Yonetoku, D., additional, Zampa, G., additional, Zampa, N., additional, Zhang, B., additional, Zhang, B.B., additional, Zhang, S., additional, Zhang, S.-N., additional, Antonelli, A., additional, Bianco, F., additional, Boci, S., additional, Boer, M., additional, Botticella, M.T., additional, Boulade, O., additional, Butler, C., additional, Campana, S., additional, Capitanio, F., additional, Celotti, A., additional, Chen, Y., additional, Colpi, M., additional, Comastri, A., additional, Cuby, J.-G., additional, Dadina, M., additional, De Luca, A., additional, Dong, Y.-W., additional, Ettori, S., additional, Gandhi, P., additional, Geza, E., additional, Greiner, J., additional, Guiriec, S., additional, Harms, J., additional, Hernanz, M., additional, Hornstrup, A., additional, Hutchinson, I., additional, Israel, G., additional, Jonker, P., additional, Kaneko, Y., additional, Kawai, N., additional, Wiersema, K., additional, Korpela, S., additional, Lebrun, V., additional, Lu, F., additional, MacFadyen, A., additional, Malaguti, G., additional, Maraschi, L., additional, Melandri, A., additional, Modjaz, M., additional, Morris, D., additional, Omodei, N., additional, Paizis, A., additional, Páta, P., additional, Petrosian, V., additional, Rachevski, A., additional, Rhoads, J., additional, Ryde, F., additional, Sabau-Graziati, L., additional, Shigehiro, N., additional, Sims, M., additional, Soomin, J., additional, Szécsi, D., additional, Urata, Y., additional, Uslenghi, M., additional, Valenziano, L., additional, Vianello, G., additional, Vojtech, S., additional, Watson, D., additional, and Zicha, J., additional
Published: 2018
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34. VERT-X: A VERTical X-ray raster-scan facility for ATHENA calibration. The concept design.

Author: Moretti, A., Pareschi, G., Uslenghi, M., Tordi, M., Bressan, R., Valsecchi, G., Zocchi, F., Attina, P., Amisano, F., Sironi, G., Salmaso, B., Basso, S., Tagliaferri, G., Spiga, D., La Palombara, N., Fiorini, M., Dury, F., Spinola, M., Marioni, F., and Parissenti, G.
Published: 2019
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35. The THESEUS space mission concept : science case, design and expected performances

Author: Amati, L., O'Brien, P., Gotz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V, Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V, Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J-L, Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, Rupal, Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V, De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I, Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. , V, Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V, Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S-N, Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J-G, Dadina, M., De Luca, A., Dong, Y-W, Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I, Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V, Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Pata, P., Petrosian, V, Rachevski, A., Rhoads, J., Ryde, Felix, Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szecsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., Zicha, J., Amati, L., O'Brien, P., Gotz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V, Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V, Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J-L, Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, Rupal, Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V, De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I, Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. , V, Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V, Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S-N, Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J-G, Dadina, M., De Luca, A., Dong, Y-W, Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I, Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V, Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Pata, P., Petrosian, V, Rachevski, A., Rhoads, J., Ryde, Felix, Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szecsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., and Zicha, J.
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1 sr) with 0.5-1 arcmin localization, an energy band extending from several MeV down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift similar to 10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late '20s/early '30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA)., QC 20180718
Published: 2018
Full Text: View/download PDF

36. The THESEUS space mission concept:science case, design and expected performances

Author: Amati, L., O'Brien, Paul, Götz, D, Bozzo, E., Tenzer, C, Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A, Contini, E., Fuschino, F., Gomboc, A, Hudec, R., Hjorth, Jens, Fynbo, Johan Peter Uldall, Malesani, Daniele, Watson, Darach Jafar, Amati, L., O'Brien, Paul, Götz, D, Bozzo, E., Tenzer, C, Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A, Contini, E., Fuschino, F., Gomboc, A, Hudec, R., Hjorth, Jens, Fynbo, Johan Peter Uldall, Malesani, Daniele, and Watson, Darach Jafar
Published: 2018

37. The THESEUS space mission concept: science case, design and expected performances

Author: Agenzia Spaziale Italiana, European Commission, Czech Grant Agency, Amati, L., O'Brien, P., Götz, Diego, Bozz, Enrico, Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, Julian Paul, Stratta, G., Tanvir, N., Cenko, B., Marisaldi, M., Lavagna, M., Israel, G., Rhoads, J., Ryde, F., Basa, S., Sabau-Graziati, L., Capozziello, Salvatore, Kuvvetli, I., Korpela, S., Li, T., Maiorano, E., Renotte, E., Camp, J., Kumar, P., McBreen, S., Adami, C., Skidmore, W., Nargaard-Nielsen, H. U., Balazs, L., Topinka, M., Savaglio, S., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Evangelista, Y., Pasquale, Massimiliano de, Ciardi, B., Uslenghi, M., Willingale, R., Basak, R., Campana, R., Valenziano, L., D'Avanzo, P., Dainotti, M. G., Giommi, Paolo, Kiss, L., Romano, P., Schady, P., Martino, Domitilla de, Izzo, L., Capitanio, F., Starling, R., Drago, Alessandro, Comastri, Andrea, Boulade, O., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, Andrea, Palazzi, E., Mundell, C., Masetti, N., Maio, U., Salvaterra, R., Ruffini, R., Finelli, F., Boci, S., Tagliaferri, G., Bellutti, P., Malcovati, P., Paltani, S., Bernardini, M. G., Rezzolla, L., Boer, M., Campana, Sergio, Margutti, R., Read, A., Maraschi, L., Colpi, Monica, Morgante, G., Omodei, Nicola, De Luca, A., Lebrun, V., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Troja, Eleonora, Stanway, E., Sguera, V., Budtz-Jørgensen, C., Panessa, F., Bulgarelli, A., Botticella, M.T., Nicastro, L., Kawai, N., Burderi, L., Fiorini, M., Fynbo, J., Putten, M. van, Gal-Yam, Avishay, Bianco, F., Kaneko, Y., Wiersema, K., MacFadyen, A., Martin-Carrillo, A., Antonelli, L. A., Hudec, René, Morris, D., Song, L., Callanan, P., Petrosian, V., Castro-Tirado, Alberto J., Zicha, J., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Dadina, M., Chen, Y., Butler, C., Hanlon, L., Vanzella, E., Longo, F., Hjorth, Jens, Attina, P., Fuschino, F., Pareschi, G., Jonker, P., Watson, D., Blain, A., Celotti, A., Orlandini, M., Floch, E. le, Cuby, Jean-Gabriel, Auricchio, N., Connaughton, Valerie, Pe'er, Asaf, Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Páta, P., Modjaz, M., Lu, F., Rauw, G., Rodic, T., Dong, Y. -W., Briggs, M., Razzano, M., Vercellone, S., Malaguti, G., Wilson-Hodge, C., Vojtech, S., Campolongo, E., Morelli, B., Melandri, A., Vianello, G., D'Elia, V., Atteia, J. L., Paizis, A., Della Valle, M., Chardonnet, P., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Mereghetti, S., Ferrara, Andrea, Bagoly, Z., Contini, C., Zhang, S., Ciolfi, Riccardo, Rachevski, A., Caruana, J., Zhang, Shuang-Nan, Ettori, S., Gomboc, A., Rosati, P., Gandhi, P., Vinciguerra, S., Casella, P., Colafrancesco, S., Orleanski, P., Vergani, S., Malesani, D., Monte, E. del, Covino, Stefano, Mignani, R., Feroci, Marco, Lyutikov, M., Geza, E., Greiner, Jochen, Guiriec, Sylvain, Harms, J., Hernanz, Margarita, Baldazzi, G., Argan, A., Cordier, B., Hornstrup, A., Vacchi, A., Hutchinson, I., Agenzia Spaziale Italiana, European Commission, Czech Grant Agency, Amati, L., O'Brien, P., Götz, Diego, Bozz, Enrico, Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, Julian Paul, Stratta, G., Tanvir, N., Cenko, B., Marisaldi, M., Lavagna, M., Israel, G., Rhoads, J., Ryde, F., Basa, S., Sabau-Graziati, L., Capozziello, Salvatore, Kuvvetli, I., Korpela, S., Li, T., Maiorano, E., Renotte, E., Camp, J., Kumar, P., McBreen, S., Adami, C., Skidmore, W., Nargaard-Nielsen, H. U., Balazs, L., Topinka, M., Savaglio, S., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Evangelista, Y., Pasquale, Massimiliano de, Ciardi, B., Uslenghi, M., Willingale, R., Basak, R., Campana, R., Valenziano, L., D'Avanzo, P., Dainotti, M. G., Giommi, Paolo, Kiss, L., Romano, P., Schady, P., Martino, Domitilla de, Izzo, L., Capitanio, F., Starling, R., Drago, Alessandro, Comastri, Andrea, Boulade, O., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, Andrea, Palazzi, E., Mundell, C., Masetti, N., Maio, U., Salvaterra, R., Ruffini, R., Finelli, F., Boci, S., Tagliaferri, G., Bellutti, P., Malcovati, P., Paltani, S., Bernardini, M. G., Rezzolla, L., Boer, M., Campana, Sergio, Margutti, R., Read, A., Maraschi, L., Colpi, Monica, Morgante, G., Omodei, Nicola, De Luca, A., Lebrun, V., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Troja, Eleonora, Stanway, E., Sguera, V., Budtz-Jørgensen, C., Panessa, F., Bulgarelli, A., Botticella, M.T., Nicastro, L., Kawai, N., Burderi, L., Fiorini, M., Fynbo, J., Putten, M. van, Gal-Yam, Avishay, Bianco, F., Kaneko, Y., Wiersema, K., MacFadyen, A., Martin-Carrillo, A., Antonelli, L. A., Hudec, René, Morris, D., Song, L., Callanan, P., Petrosian, V., Castro-Tirado, Alberto J., Zicha, J., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Dadina, M., Chen, Y., Butler, C., Hanlon, L., Vanzella, E., Longo, F., Hjorth, Jens, Attina, P., Fuschino, F., Pareschi, G., Jonker, P., Watson, D., Blain, A., Celotti, A., Orlandini, M., Floch, E. le, Cuby, Jean-Gabriel, Auricchio, N., Connaughton, Valerie, Pe'er, Asaf, Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Páta, P., Modjaz, M., Lu, F., Rauw, G., Rodic, T., Dong, Y. -W., Briggs, M., Razzano, M., Vercellone, S., Malaguti, G., Wilson-Hodge, C., Vojtech, S., Campolongo, E., Morelli, B., Melandri, A., Vianello, G., D'Elia, V., Atteia, J. L., Paizis, A., Della Valle, M., Chardonnet, P., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Mereghetti, S., Ferrara, Andrea, Bagoly, Z., Contini, C., Zhang, S., Ciolfi, Riccardo, Rachevski, A., Caruana, J., Zhang, Shuang-Nan, Ettori, S., Gomboc, A., Rosati, P., Gandhi, P., Vinciguerra, S., Casella, P., Colafrancesco, S., Orleanski, P., Vergani, S., Malesani, D., Monte, E. del, Covino, Stefano, Mignani, R., Feroci, Marco, Lyutikov, M., Geza, E., Greiner, Jochen, Guiriec, Sylvain, Harms, J., Hernanz, Margarita, Baldazzi, G., Argan, A., Cordier, B., Hornstrup, A., Vacchi, A., and Hutchinson, I.
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift 10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ¿20s/early ¿30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).© 2018 COSPAR
Published: 2018

38. The Imaging X-Ray Polarimetry Explorer (IXPE): technical overview IV

Author: Siegmund, Oswald H., Ramsey, Brian D., Attina, Primo, Baldini, Luca, Barbanera, Mattia, Baumgartner, Wayne H., Bellazzini, Ronaldo, Bladt, Jeff, Bongiorno, Stephen D., Brez, Alessandro, Castellano, Simone, Carpentiero, Rita, Castronuovo, Marco, Cavalli, Luca, Cavazutti, Elisabetta, D'Amico, Fabio, Citraro, Saverio, Costa, Enrico, Deininger, William D., D'Alba, Elisa, Delmonte, Ettore, Dietz, Kurtis L., Di Lalla, Niccolo, Di Marco, Alessandro, Di Persio, Giusseppe, Donnarumma, Immacolata, Fabiani, Sergio, Ferrazzoli, Riccardo, Footdale, Joseph, Head, Michael, Kalinowski, William, Kolodziejczak, Jeffery J., Latronico, Luca, Lefevre, Carlo, Lorenzi, Paolo, Lucchesi, Leonardo, Maldera, Simone, Manfreda, Alberto, Mangravati, Elio, Marshall, Herman L., Matt, Giorgio, Minuti, Massimo, Mize, Rondal, Muleri, Fabio, Nasimi, Hikmat, Negri, Barbara, Nuti, Alessio, O'Dell, Stephen, Orsini, Leonardo, Osborne, Darren, Pentz, Christina, Pilia, Maura, Perri, Matteo, Pesce-Rollins, Melissa, Peterson, Colin, Pinchera, Michele, Puccetti, Simonetta, Rankin, John, Ratheesh, Ajay, Romani, Roger W., Sarra, Paolo, Santoli, Francesco, Sciortino, Andrea, Schroeder, Christopher, Sgro, Carmelo, Soffitta, Paolo, Spandre, Gloria, Tennant, Allyn, Tobia, Antonino, Thomas, Nicholas E., Trois, Alessio, Vimercati, Marco, Wedmore, Jeffery, Weisskopf, Martin C., Xie, Fei, Zanetti, Francesco, Alexander, Cheryl, Allen, D. Zachery, Amici, Fabrizio, Andersen, Jason, Antonelli, Angelo, Antoniak, Spencer, Bachetti, Matteo, Baggett, Randy M., Bonino, Rafaella, Boree, Christopher, Borotto, Fabio, Breeding, Shawn, Brienza, Daniele, Byggott, H. Kyle, Caporale, Ciro, Cardelli, Claudia, Ceccanti, Marco, Centrone, Mauro, Dolan, David, Evangelista, Yuri, Ferrant, Kevin, Ferrie, MacKenzie, Forsyth, Brent, Foster, Michelle, Garelick, Benjamin, Gunji, Shuichi, Gurnee, Eli, Hibbard, Grant, Johnson, Samantha, Kelly, Eric, Kilaru, Kiranmayee, La Monaca, Fabio, Le Roy, Shelley, Lofredo, Pasqualino, Maddox, Tyler, Magazzu, Guido, Marengo, Marco, Marrocchesi, Alessandra, Massaro, Francesco, Mauger, David, McCracken, Jeffrey, McEachen, Michael, Mereu, Paolo, Mitchell, Scott, Mitsuishi, Ikuyuki, Morbidini, Alfredo, Mosti, Federico, Nguyen, Toan, Negro, Michela, Nitschke, Isaac, Onizuka, Mitch, Oppedisano, Chiara, Pacheco, Richard, Paggi, Alessandro, Painter, Will, Pavelitz, Steven D., Piazzolla, Raffaele, Profeti, Alessandro, Ranganathan, Jaganathan, Reedy, Lee, Root, Noah, Rubini, Alda, Ruswick, Stephanie, Sanchez, Javier, Scalise, Emanuele, Seek, Tim, Sosdian, Kalie, Speegle, Chet O., Tamagawa, Toru, Tardiola, Marcello, Valerie, Robert, Walden, Amy L., Weddendorf, Bruce, and Welch, David
Published: 2021
Full Text: View/download PDF

39. XIPE

Author: Soffitta, P., Bellazzini, R., Bozzo, E., Burwitz, V., Castro-Tirado, A. J., Costa, E., Courvoisier, T., Feng, H., Gburek, S., Goosmann, R., Karas, V., Matt, G., Muleri, F., Nandra, K., Pearce, M., Poutanen, J., Reglero, V., Sabau Maria, D., Santangelo, A., Tagliaferri, G., Tenzer, C., Vink, J., Weisskopf, M. C., Zane, S., Agudo, I., Antonelli, A., Attina, P., Baldini, L., Bykov, A., Carpentiero, R., Cavazzuti, E., Churazov, E., Del Monte, E., De Martino, D., Donnarumma, I., Doroshenko, V., Evangelista, Y., Ferreira, I., Gallo, E., Grosso, N., Kaaret, P., Kuulkers, E., Laranaga, J., Latronico, L., Lumb, D. H., Macian, J., Malzac, J., Marin, F., Massaro, E., Minuti, M., Mundell, C., Ness, J. U., Oosterbroek, T., Paltani, S., Pareschi, G., Perna, R., Petrucci, P. O., Pinazo, H. B., Pinchera, M., Rodriguez, J. P., Roncadelli, M., Santovincenzo, A., Sazonov, S., Sgro, C., Spiga, D., Svoboda, J., Theobald, C., Theodorou, T., Turolla, R., Wilhelmi De Ona, E., Winter, B., Akbar, A. M., Allan, H., Aloisio, R., Altamirano, D., Amati, L., Amato, E., Angelakis, E., Arezu, J., Atteia, J. L., Axelsson, M., Bachetti, M., Ballo, L., Balman, S., Bandiera, R., Barcons, X., Basso, S., Baykal, A., Becker, W., Behar, E., Beheshtipour, B., Belmont, R., Berger, E., Bernardini, F., Bianchi, S., Bisnovatyi-Kogan, G., Blasi, P., Blay, P., Bodaghee, A., Boer, M., Boettcher, M., Bogdanov, S., Bombaci, I., Bonino, R., Braga, J., Brandt, W., Brez, A., Bucciantini, N., Burderi, L., Caiazzo, I., Campana, R., Campana, S., Capitanio, F., Cappi, M., Cardillo, M., Casella, P., Catmabacak, O., Cenko, B., Cerda-Duran, P., Cerruti, C., Chaty, S., Chauvin, M., Chen, Y., Chenevez, J., Chernyakova, M., Cheung Teddy, C. C., Christodoulou, D., Connell, P., Corbet, R., Coti Zelati, F., Covino, S., Cui, W., Cusumano, G., D'Ai, A., D'Ammando, F., Dadina, M., Dai, Z., De Rosa, A., De Ruvo, L., Degenaar, N., Del Santo, M., Del Zanna, L., Dewangan, G., Di Cosimo, S., Di Lalla, N., Di Persio, G., Di Salvo, T., Dias, T., Done, C., Dovciak, M., Doyle, G., Ducci, L., Elsner, R., Enoto, T., Escada, J., Esposito, P., Eyles, C., Fabiani, S., Falanga, M., Falocco, S., Fan, Y., Fender, R., Feroci, M., Ferrigno, C., Forman, W., Foschini, L., Fragile, C., Fuerst, F., Fujita, Y., Gasent-Blesa, J. L., Gelfand, J., Gendre, B., Ghirlanda, G., Ghisellini, G., Giroletti, M., Goetz, D., Gogus, E., Gomez, J. L., Gonzalez, D., Gonzalez-Riestra, R., Gotthelf, E., Gou, L., Grandi, P., Grinberg, V., Grise, F., Guidorzi, C., Gurlebeck, N., Guver, T., Haggard, D., Hardcastle, M., Hartmann, D., Haswell, C., Heger, A., Hernanz, M., Heyl, J., Ho, L., Hoormann, J., Horak, J., Huovelin, J., Huppenkothen, D., Iaria, R., Inam Sitki, C., Ingram, A., Israel, G., Izzo, L., Burgess, M., Jackson, M., Ji, L., Jiang, J., Johannsen, T., Jones, C., Jorstad, S., Kajava, J. J E, Kalamkar, M., Kalemci, E., Kallman, T., Kamble, A., Kislat, F., Kiss, M., Klochkov, D., Koerding, E., Kolehmainen, M., Koljonen, K., Komossa, S., Kong, A., Korpela, S., Kowalinski, M., Krawczynski, H., Kreykenbohm, I., Kuss, M., Lai, D., Lan, M., Larsson, J., Laycock, S., Lazzati, D., Leahy, D., Li, H., Li, J., Li, L. X., Li, T., Li, Z., Linares, M., Lister, M., Liu, H., Lodato, G., Lohfink, A., Longo, F., Luna, G., Lutovinov, A., Mahmoodifar, S., Maia, J., Mainieri, V., Maitra, C., Maitra, D., Majczyna, A., Maldera, S., Malyshev, D., Manfreda, A., Manousakis, A., Manuel, R., Margutti, R., Marinucci, A., Markoff, S., Marscher, A., Marshall, H., Massaro, F., McLaughlin, M., Medina-Tanco, G., Mehdipour, M., Middleton, M., Mignani, R., Mimica, P., Mineo, T., Mingo, B., Miniutti, G., Mirac, S. M., Morlino, G., Motlagh, A. V., Motta, S. E., Mushtukov, A., Nagataki, S., Nardini, F., Nattila, J., Navarro, G. J., Negri, B., Negro, M., Nenonen, S., Neustroev, V., Nicastro, F., Norton, A., Nucita, A., O'Brien, P., O'Dell, S., Odaka, H., Olmi, B., Omodei, N., Orienti, M., Orlandini, M., Osborne, J., Pacciani, L., Paliya, V. S., Papadakis, I., Papitto, A., Paragi, Z., Pascal, P., Paul, B., Pavan, L., Pellizzoni, A., Perinati, E., Pesce-Rollins, M., Piconcelli, E., Pili, A. G., Pilia, M., Pohl, Martin, Ponti, G., Porquet, D., Possenti, A., Postnov, K., Prandoni, I., Produit, N., Puehlhofer, G., Ramsey, B., Razzano, M., Rea, N., Reig, P., Reinsch, K., Reiprich, T., Reynolds, M., Risaliti, G., Roberts, T., Rodriguez, J., Rossi, M. E., Rosswog, S., Rozanska, A., Rubini, A., Rudak, B., Russell, D., Ryde, F., Sabatini, S., Sala, G., Salvati, M., Sasaki, M., Savolainen, T., Saxton, R., Scaringi, S., Schawinski, K., Schulz, N. S., Schwope, A., Severgnini, P., Sharon, M., Shaw, A., Shearer, A., Shesheng, X., Shih, I. C., Silva, K., Silva, R., Silver, E., Smale, A., Spada, F., Spandre, G., Stamerra, A., Stappers, B., Starrfield, S., Stawarz, L., Stergioulas, N., Stevens, A., Stiele, H., Suleimanov, V., Sunyaev, R., Slowikowska, A., Tamborra, F., Tavecchio, F., Taverna, R., Tiengo, A., Tolos, L., Tombesi, F., Tomsick, J., Tong, H., Torok, G., Torres, D. F., Tortosa, A., Tramacere, A., Trimble, V., Trinchieri, G., Tsygankov, S., Tuerler, M., Turriziani, S., Ursini, F., Uttley, P., Varniere, P., Vincent, F., Vurgun, E., Wang, C., Wang, Z., Watts, A., Wheeler, J. C., Wiersema, K., Wijnands, R., Wilms, J., Wolter, A., Wood, K., Wu, K., Wu, X., Xiangyu, W., Xie, F., Xu, R., Yan, S. P., Yang, J., Yu, W., Yuan, F., Zajczyk, A., Zanetti, D., Zanin, R., Zanni, C., Zappacosta, L., Zdziarski, A. A., Zech, A., Zhang, H., Zhang, S., Zhang, W., Zoghbi, A., den Herder, Jan-Willem A., Takahashi, Tadayuki, Bautz, Marshall, Istituto di Astrofisica e Planetologia Spaziali, University of Pisa, University of Geneva, Max Planck Institute for Extraterrestrial Physics, CSIC, Tsinghua University, Polish Academy of Sciences, Université de Strasbourg, Czech Academy of Sciences, Roma Tre University, KTH Royal Institute of Technology, University of Turku, Universidad de Valencia, Instituto Nacional de Tecnica Aeroespacial, University of Tübingen, INAF—Osservatorio Astronomico di Brera, University of Amsterdam, National Aeronautics and Space Administration, University College London, ASI Science Data Center, Ioffe Institute, Agenzia Spaziale Italiana, Max-Planck-Institut für Astrophysik, INAF Osservatorio Astronomico di Capodimonte, European Space Research and Technology Centre, University of Michigan, Ann Arbor, Michigan State University, INFN, Sezione di Torino, IRAP, Università La Sapienza, INFN Pisa, University of Bath, European Space Astronomy Centre, Stony Brook University, Université Grenoble Alpes, Istituto Nazionale di Fisica Nucleare (INFN), Russian Academy of Sciences, University of Padova, Autonomous University of Barcelona, Effat University, Danmarks Tekniske Universitet, Osservatorio Astrofisico Di Arcetri, Florence, Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna, Max Planck Institute for Radio Astronomy, Buein Zahra Technical University, Osservatorio Astronomico Cagliari, Middle East Technical University, Universidad de Cantabria, Osservatorio Astronomicodi Roma, Technion-Israel Institute of Technology, Washington University St. Louis, Harvard University, New York University Abu Dhabi, Space Research Institute of the Russian Academy of Sciences, Georgia College, Centre National de la Recherche Scientifique (CNRS), North West University, Columbia University, Sapienza University of Rome, Instituto Nacional de Pesquisas Espaciais, Pennsylvania State University, University of Cagliari, University of British Columbia, INAF/IASF Bologna, INAF, Osservatorio Astronomico di Roma, Sabanci University, Université Paris Diderot, Nanjing University, Dublin City University, Naval Research Laboratory, University of Massachusetts Lowell, University of Maryland, Baltimore, Purdue University, INAF-IASF Palermo, University of Palermo, Inter-University Centre for Astronomy and Astrophysics India, Durham University, Armagh Observatory, NASA Goddard Space Flight Center, Universidade de Coimbra, INAF/IASF Milano, International Space Science Institute, University of Naples Federico II, CAS - Purple Mountain Observatory, University of Oxford, College of Charleston, California Institute of Technology, Osaka University, University of the Virgin Islands, European Space Agency - ESA, Chinese Academy of Sciences, Massachusetts Institute of Technology, University of Bremen, Istanbul University, McGill University, University of Hertfordshire, Clemson University, Open University Milton Keynes, Monash University, University of Helsinki, Cardiff University, CAS - Institute of High Energy Physics, Fudan University, Perimeter Institute for Theoretical Physics, Boston University, Radboud University Nijmegen, National Tsing Hua University, Friedrich-Alexander University Erlangen-Nürnberg, Cornell University, Oregon State University, University of Calgary, Kavli Institute for Astronomy and Astrophysics, XiangTan University, Guangxi University, University of Milano, University of Cambridge, Università Degli Studi di Trieste, Universidad de Buenos Aires, European Southern Observatory, Wheaton College, National Centre for Nuclear Research, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, New York University, West Virginia University, Universidad Nacional Autónoma de México, SRON Netherlands Institute for Space Research, University of Leicester, Gran Sasso Science Institute, RIKEN, Keele University, Oxford Instruments Analytical Oy, University of Salento, JAXA Institute of Space and Astronautical Science, University of Florence, Kavli Institute for Particle Astrophysics and Cosmology, University of Crete, Joint Institute for VLBI in Europe, Université Paul Sabatier, Raman Research Institute, Lomonosov Moscow State University, Foundation for Research and Technology - Hellas, University of Göttingen, Argelander-Institut für Astronomie, Leiden University, Stockholm University, Polytechnic University of Catalonia, Metsähovi Radio Observatory, Swiss Federal Institute of Technology Zurich, Leibniz Institut für Astrophysik Potsdam, University of Alberta, University of Southampton, National University of Ireland, Galway, Paris Observatory, INAF—Osservatorio Astrofisico di Torino, University of Manchester, Arizona State University, Jagiellonian University in Kraków, Aristotle University of Thessaloniki, University of Zielona Gora, Istituto Universitario di Studi Superiori di Pavia, University of Maryland, College Park, University of California Berkeley, Silesian University in Opava, University of California Irvine, Università di Roma Tor Vergata, Institut national de physique nucléaire et de physique des particules, Université Pierre and Marie Curie, Tongji University, University of Texas at Austin, Peking University, CAS - Shanghai Astronomical Observatory, Technische Universität Darmstadt, Los Alamos National Laboratory, Aalto-yliopisto, and Aalto University
Subjects: X-ray Astronomy, X-ray optics, Polarimetry, Gas Pixel Detector
Abstract: XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially-resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror but with a low weight. The payload is compatible with the fairing of the Vega launcher. XIPE is designed as an observatory for X-ray astronomers with 75 % of the time dedicated to a Guest Observer competitive program and it is organized as a consortium across Europe with main contributions from Italy, Germany, Spain, United Kingdom, Poland, Sweden.
Published: 2016

40. XIPE: the x-ray imaging polarimetry explorer

Author: Soffitta, Paolo, primary, Bellazzini, Ronaldo, additional, Bozzo, Enrico, additional, Burwitz, Vadim, additional, Castro Tirado, Alberto, additional, Costa, Enrico, additional, Courvoisier, Thierry, additional, Feng, Hua, additional, Gburek, Szymon, additional, Goosmann, Rene', additional, Karas, Vladimir, additional, Matt, Giorgio, additional, Muleri, Fabio, additional, Nandra, Kirpal, additional, Pearce, Mark, additional, Poutanen, Juri, additional, Reglero, Victor, additional, Graziati, Maria Dolores, additional, Santangelo, Andrea, additional, Tagliaferri, Gianpiero, additional, Tenzer, Christopher, additional, Vink, Jacco, additional, Weisskopf, Martin, additional, Zane, Silvia, additional, Agudo, I., additional, Antonelli, A., additional, Attina, P., additional, Baldini, L., additional, Bykov, A., additional, Carpentiero, R., additional, Cavazzuti, E., additional, Churazov, E., additional, Del Monte, E., additional, De Martino, D., additional, Donnarumma, I., additional, Doroshenko, V., additional, Evangelista, Y., additional, Ferreira, I., additional, Gallo, E., additional, Grosso, N., additional, Kaaret, P., additional, Kuulkers, E., additional, Laranaga, J., additional, Latronico, L., additional, Lumb, D. H., additional, Macian, J., additional, Malzac, J., additional, Marin, F., additional, Massaro, E., additional, Minuti, M., additional, Mundell, C., additional, Ness, J. U., additional, Oosterbroek, T., additional, Paltani, S., additional, Pareschi, G., additional, Perna, R., additional, Petrucci, P.-O., additional, Pinazo, H. B., additional, Pinchera, M., additional, Rodriguez, J. P., additional, Roncadelli, M., additional, Santovincenzo, A., additional, Sazonov, S., additional, Sgro, C., additional, Spiga, D., additional, Svoboda, J., additional, Theobald, C., additional, Theodorou, T., additional, Turolla, R., additional, Wilhelmi de Ona, E., additional, Winter, B., additional, Akbar, A. M., additional, Allan, H., additional, Aloisio, R., additional, Altamirano, D., additional, Amati, L., additional, Amato, E., additional, Angelakis, E., additional, Arezu, J., additional, Atteia, J.-L., additional, Axelsson, M., additional, Bachetti, M., additional, Ballo, L., additional, Balman, S., additional, Bandiera, R., additional, Barcons, X., additional, Basso, S., additional, Baykal, A., additional, Becker, W., additional, Behar, E., additional, Beheshtipour, B., additional, Belmont, R., additional, Berger, E., additional, Bernardini, F., additional, Bianchi, S., additional, Bisnovatyi-Kogan, G., additional, Blasi, P., additional, Blay, P., additional, Bodaghee, A., additional, Boer, M., additional, Boettcher, M., additional, Bogdanov, S., additional, Bombaci, I., additional, Bonino, R., additional, Braga, J., additional, Brandt, W., additional, Brez, A., additional, Bucciantini, N., additional, Burderi, L., additional, Caiazzo, I., additional, Campana, R., additional, Campana, S., additional, Capitanio, F., additional, Cappi, M., additional, Cardillo, M., additional, Casella, P., additional, Catmabacak, O., additional, Cenko, B., additional, Cerda-Duran, P., additional, Cerruti, C., additional, Chaty, S., additional, Chauvin, M., additional, Chen, Y., additional, Chenevez, J., additional, Chernyakova, M., additional, Cheung, C. C. T., additional, Christodoulou, D., additional, Connell, P., additional, Corbet, R., additional, Coti Zelati, F., additional, Covino, S., additional, Cui, W., additional, Cusumano, G., additional, D’Ai, A., additional, D’Ammando, F., additional, Dadina, M., additional, Dai, Z., additional, De Rosa, A., additional, de Ruvo, L., additional, Degenaar, N., additional, Del Santo, M., additional, Del Zanna, L., additional, Dewangan, G., additional, Di Cosimo, S., additional, Di Lalla, N., additional, Di Persio, G., additional, Di Salvo, T., additional, Dias, T., additional, Done, C., additional, Dovciak, M., additional, Doyle, G., additional, Ducci, L., additional, Elsner, R., additional, Enoto, T., additional, Escada, J., additional, Esposito, P., additional, Eyles, C., additional, Fabiani, S., additional, Falanga, M., additional, Falocco, S., additional, Fan, Y., additional, Fender, R., additional, Feroci, M., additional, Ferrigno, C., additional, Forman, W., additional, Foschini, L., additional, Fragile, C., additional, Fuerst, F., additional, Fujita, Y., additional, Gasent-Blesa, J. L., additional, Gelfand, J., additional, Gendre, B., additional, Ghirlanda, G., additional, Ghisellini, G., additional, Giroletti, M., additional, Goetz, D., additional, Gogus, E., additional, Gomez, J.-L., additional, Gonzalez, D., additional, Gonzalez-Riestra, R., additional, Gotthelf, E., additional, Gou, L., additional, Grandi, P., additional, Grinberg, V., additional, Grise, F., additional, Guidorzi, C., additional, Gurlebeck, N., additional, Guver, T., additional, Haggard, D., additional, Hardcastle, M., additional, Hartmann, D., additional, Haswell, C., additional, Heger, A., additional, Hernanz, M., additional, Heyl, J., additional, Ho, L., additional, Hoormann, J., additional, Horak, J., additional, Huovelin, J., additional, Huppenkothen, D., additional, Iaria, R., additional, Inam Sitki, C., additional, Ingram, A., additional, Israel, G., additional, Izzo, L., additional, Burgess, M., additional, Jackson, M., additional, Ji, L., additional, Jiang, J., additional, Johannsen, T., additional, Jones, C., additional, Jorstad, S., additional, Kajava, J. J. E., additional, Kalamkar, M., additional, Kalemci, E., additional, Kallman, T., additional, Kamble, A., additional, Kislat, F., additional, Kiss, M., additional, Klochkov, D., additional, Koerding, E., additional, Kolehmainen, M., additional, Koljonen, K., additional, Komossa, S., additional, Kong, A., additional, Korpela, S., additional, Kowalinski, M., additional, Krawczynski, H., additional, Kreykenbohm, I., additional, Kuss, M., additional, Lai, D., additional, Lan, M., additional, Larsson, J., additional, Laycock, S., additional, Lazzati, D., additional, Leahy, D., additional, Li, H., additional, Li, J., additional, Li, L., additional, Li, T., additional, Li, Z., additional, Linares, M., additional, Lister, M., additional, Liu, H., additional, Lodato, G., additional, Lohfink, A., additional, Longo, F., additional, Luna, G., additional, Lutovinov, A., additional, Mahmoodifar, S., additional, Maia, J., additional, Mainieri, V., additional, Maitra, C., additional, Maitra, D., additional, Majczyna, A., additional, Maldera, S., additional, Malyshev, D., additional, Manfreda, A., additional, Manousakis, A., additional, Manuel, R., additional, Margutti, R., additional, Marinucci, A., additional, Markoff, S., additional, Marscher, A., additional, Marshall, H., additional, Massaro, F., additional, McLaughlin, M., additional, Medina-Tanco, G., additional, Mehdipour, M., additional, Middleton, M., additional, Mignani, R., additional, Mimica, P., additional, Mineo, T., additional, Mingo, B., additional, Miniutti, G., additional, Mirac, S. M., additional, Morlino, G., additional, Motlagh, A. V., additional, Motta, S., additional, Mushtukov, A., additional, Nagataki, S., additional, Nardini, F., additional, Nattila, J., additional, Navarro, G. J., additional, Negri, B., additional, Negro, Matteo, additional, Nenonen, S., additional, Neustroev, V., additional, Nicastro, F., additional, Norton, A., additional, Nucita, A., additional, O’Brien, P., additional, O’Dell, S., additional, and Turriziani, S., additional
Published: 2016
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41. The COBRA IRIDES Experiment

Author: Peters, T. V., Escorial Olmos, D., Pellacani, A., Avilés Rodrigálvarez, M., Lavagna, Michèle, Ferrari, Fabio, Attina, P., and Parissenti, G.
Published: 2014

42. VERT-X: VERTical X-ray raster-scan facility for ATHENA calibration. The concept design.

Author: O'Dell, Stephen L., Pareschi, Giovanni, Moretti, A., Pareschi, G., Uslenghi, M., Tordi, M., Bressan, R., Valsecchi, G., Zocchi, F., Attina, P., Amisano, F., Sironi, G., Salmaso, B., Basso, S., Tagliaferri, G., Spiga, D., La Palombara, N., Fiorini, M., Dury, F., Marioni, F., Parissenti, G., Parodi, G., Wille, E., Corradi, P., Bavdaz, M., and Ferreira, I.
Published: 2019
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43. SIMBOL-X: A SPACECRAFT FORMATION FOR X-RAY OBSERVATIONS

Author: Canuto, Enrico, Castillo, S, Ospina, JOSE ALEJANDRO, Sechi, G, Attina, P, and Piermaria, M.
Published: 2008

44. Calibration of the IXPE instrument

Author: den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Muleri, Fabio, Lefevre, Carlo, Piazzolla, Raffaele, Morbidini, Alfredo, Amici, Fabrizio, Attina, Primo, Centrone, Mauro, Del Monte, Ettore, Di Cosimo, Sergio, Di Persio, Giuseppe, Evangelista, Yuri, Fabiani, Sergio, Ferrazzoli, Riccardo, Loffredo, Pasqualino, Maiolo, Luca, Maita, Francesco, Primicino, Leandra, Rankin, John, Rubini, Alda, Santoli, Francesco, Soffitta, Paolo, Tobia, Antonino, Tortosa, Alessia, and Trois, Alessio
Published: 2018
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45. Epigenetic Modifiers MMSET and EZH2 Physically Interact and Cooperate to Support Multiple Myeloma Pathophysiology

Author: Varlet, Emmanuel, Alaterre, Elina, Thomas, Morgane, De Boussac, Hugues, Vincent, Laure, Cartron, Guillaume, Herbaux, Charles, Bret, Caroline, Herviou, Laurie, Martinez, Anne Marie, Hirtz, Christophe, Attina, Aurore, Vialaret, Jerome, Cavalli, Giacomo, Moreaux, Jerome, and Ovejero, Sara
Abstract: Multiple myeloma (MM) is a malignant B cell dyscrasia characterized by the accumulation of clonal plasma cells (PC) within the bone marrow (1). Genome sequencing studies have revealed great heterogeneity and genomic instability, a complex mutational landscape and a branching pattern of clonal evolution (2-4). Epigenetic factors are also involved in MM initiation, progression, and occurrence of chemoresistance (5). Among them, EZH2 and MMSET are associated with poor prognosis values and contribute to MM disease. EZH2 is the main catalytic subunit of the Polycomb Repressive Complex 2 (PRC2) and deposits H3K27me3 on chromatin (6), whereas MMSET, coded by the gene NSD2, which is the target oncogene of t(4;14) primary translocation, is a histone methyltransferase that methylates H3K36me2 (7).
Published: 2023
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46. Exposure to bisphenols and phthalates and association with oxidant stress, insulin resistance, and endothelial dysfunction in children

Author: Kataria, Anglina, Levine, Dov, Wertenteil, Sara, Vento, Suzanne, Xue, Jingchuan, Rajendiran, Karthikraj, Kannan, Kurunthachalam, Thurman, Joshua M., Morrison, Debra, Brody, Rachel, Urbina, Elaine, Attina, Teresa, Trasande, Leonardo, and Trachtman, Howard
Abstract: Background:The health effects of bisphenol A (BPA) and di-(2-ethylhexyl) phthalate (DEHP) have been studied extensively in children. The impact of other chemicals in these two classes has not been investigated as fully.Methods:We conducted a cross-sectional pilot study of 10–13 y old healthy children. We assessed descriptive, univariable, and multivariable associations of urinary metabolites of bisphenols and phthalates with oxidant stress, insulin resistance, body mass, and endothelial dysfunction. Possible associations with brachial artery distensibility, pulse wave velocity (markers of vascular stiffness), and serum endothelial cell-derived microparticle levels were also assessed.Results:We enrolled 41 participants, 12.1 ± 1.0 y, most of whom were Mexican Americans (42%) or other Hispanics (34%). Increased BPA levels were associated with increased levels of F2-isoprostane (ng/ml) (P = 0.02), with a similar trend for DEHP metabolites. Each log unit increase of high molecular weight (HMW) phthalate metabolites was associated with a 0.550 increase in Homeostatic Model Assessment of insulin resistance (HOMA-IR) units (P = 0.019) and altered circulating levels of activated endothelial cell-derived microparticles (% per ml) (P = 0.026). Bisphenol S (BPS), a replacement for BPA, was associated with increased albumin (mg):creatinine (g) ratio (P = 0.04). Metabolites of HMW phthalates were also associated with decreased brachial artery distensibility (P = 0.047).Conclusion:Exposure to bisphenols and phthalates, including a BPA replacement, is associated with increased oxidant stress, insulin resistance, albuminuria, as well as disturbances in vascular function in healthy children.
Published: 2017
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47. JEM-X: The X-ray monitor aboard INTEGRAL

Author: Lund, Niels, Budtz-Jørgensen, Carl, Westergaard, Niels Jørgen Stenfeldt, Brandt, Søren Kristian, Rasmussen, Ib Lundgaard, Hornstrup, Allan, Oxborrow, Carol Anne, Chenevez, Jérôme, Jensen, Poul Anker, Laursen, Steen, Andersen, KH., Mogensen, P.B., Rasmussen, Ib, Omo, K., Pedersen, Søren Møller, Polny, Jozef, Andersson, H., Andersson, T., Kamarainen, V., Vilhu, O., Huovelin, J., Maisala, S., Morawski, M., Juchnikowski, G., Costa, E., Feroci, M., Rubini, A., Rapisarda, M., Morelli, E., Carassiti, V., Frontera, F., Pelliciari, C., Loffredo, G., Nunez, S.M., Reglero, V., Velasco, T., Larsson, S., Svensson, R., Zdziarski, A.A., Castro-Tirado, A., Attina, P., Goria, M., Giulianelli, G., Cordero, F., Rezazad, M., Schmidt, M.N., Carli, R., Gomez, C., Jensen, Peter Løkke, Sarri, G., Tiemon, A., Orr, A., Much, R., Kretschmar, P., Schnopper, H.W., Lund, Niels, Budtz-Jørgensen, Carl, Westergaard, Niels Jørgen Stenfeldt, Brandt, Søren Kristian, Rasmussen, Ib Lundgaard, Hornstrup, Allan, Oxborrow, Carol Anne, Chenevez, Jérôme, Jensen, Poul Anker, Laursen, Steen, Andersen, KH., Mogensen, P.B., Rasmussen, Ib, Omo, K., Pedersen, Søren Møller, Polny, Jozef, Andersson, H., Andersson, T., Kamarainen, V., Vilhu, O., Huovelin, J., Maisala, S., Morawski, M., Juchnikowski, G., Costa, E., Feroci, M., Rubini, A., Rapisarda, M., Morelli, E., Carassiti, V., Frontera, F., Pelliciari, C., Loffredo, G., Nunez, S.M., Reglero, V., Velasco, T., Larsson, S., Svensson, R., Zdziarski, A.A., Castro-Tirado, A., Attina, P., Goria, M., Giulianelli, G., Cordero, F., Rezazad, M., Schmidt, M.N., Carli, R., Gomez, C., Jensen, Peter Løkke, Sarri, G., Tiemon, A., Orr, A., Much, R., Kretschmar, P., and Schnopper, H.W.
Abstract: The JEM-X monitor provides X-ray spectra and imaging with arcminute angular resolution in the 3 to 35 keV band. The good angular resolution and the low energy response of JEM-X plays an important role in the identification of gamma ray sources and in the analysis and scientific interpretation of the combined X-ray and gamma ray data. JEM-X is a coded aperture instrument consisting of two identical, coaligned telescopes. Each of the detectors has a sensitive area of 500 cm(2), and views the sky through its own coded aperture mask. The two coded masks are inverted with respect to each other and provides an angular resolution of 3' across an effective field of view of about 10degrees diameter.
Published: 2003

48. Association of exposure to di-2-ethylhexylphthalate replacements with increased blood pressure in children and adolescents.

Author: Trasande, Leonardo and Attina, Teresa M
Abstract: Phthalates are environmental chemicals widely used in consumer and personal care products. In this study, we examined associations of urinary phthalates with blood pressure, triglycerides, and lipoproteins in children and adolescents, performing a cross-sectional analysis of a subsample of US children 6 to 19 years of age who participated in the National Health and Nutrition Examination Survey between the years 2009 and 2012. We quantified exposure to common environmental phthalates, with a focus on the dietary contaminant di-2-ethylhexylphthalate and 2 increasingly used replacements, di-isononyl phthalate and di-isodecyl phthalate, based on micromolar concentration of urinary metabolites. We assessed descriptive, univariate, and multivariable associations with blood pressure and lipids. Controlling for an array of sociodemographic and behavioral factors, as well as diet and body mass, metabolites of di-2-ethylhexylphthalate, di-isononyl phthalate, and di-isodecyl phthalate were associated with higher age-, sex- and height-standardized blood pressure. For each log unit increase in di-isodecyl phthalate metabolites, a 0.105 standard deviation unit increase in systolic blood pressure z score was identified (P=0.004); for di-isononyl phthalate metabolites, a 0.113 standard deviation unit increment was identified (P=0.008). For di-2-ethylhexylphthalate metabolites, a 0.103 standard deviation unit increment (P=0.013) was detected. Metabolites of low molecular weight phthalates commonly found in cosmetics and personal care products showed an association with blood pressure (≥90th percentile) in univariate analysis, but this was no longer significant in our full multivariable model, suggesting specificity. Phthalate metabolites were not associated with triglycerides or high-density lipoproteins. Further, longitudinal studies are needed to confirm these associations and to assess opportunities for intervention. [ABSTRACT FROM AUTHOR]
Published: 2015
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49. JEM–X: The X-ray monitor aboard INTEGRAL

Author: Lund, N., primary, Budtz-Jørgensen, C., additional, Westergaard, N. J., additional, Brandt, S., additional, Rasmussen, I. L., additional, Hornstrup, A., additional, Oxborrow, C. A., additional, Chenevez, J., additional, Jensen, P. A., additional, Laursen, S., additional, Andersen, K. H., additional, Mogensen, P. B., additional, Rasmussen, I., additional, Omø, K., additional, Pedersen, S. M., additional, Polny, J., additional, Andersson, H., additional, Andersson, T., additional, Kämäräinen, V., additional, Vilhu, O., additional, Huovelin, J., additional, Maisala, S., additional, Morawski, M., additional, Juchnikowski, G., additional, Costa, E., additional, Feroci, M., additional, Rubini, A., additional, Rapisarda, M., additional, Morelli, E., additional, Carassiti, V., additional, Frontera, F., additional, Pelliciari, C., additional, Loffredo, G., additional, Martínez Núñez, S., additional, Reglero, V., additional, Velasco, T., additional, Larsson, S., additional, Svensson, R., additional, Zdziarski, A. A., additional, Castro-Tirado, A., additional, Attina, P., additional, Goria, M., additional, Giulianelli, G., additional, Cordero, F., additional, Rezazad, M., additional, Schmidt, M., additional, Carli, R., additional, Gomez, C., additional, Jensen, P. L., additional, Sarri, G., additional, Tiemon, A., additional, Orr, A., additional, Much, R., additional, Kretschmar, P., additional, and Schnopper, H. W., additional
Published: 2003
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50. Temporal Measures of Hand and Speech Coordination During French Cued Speech Production.

Author: Gibet, Sylvie, Courty, Nicolas, Kamp, Jean-François, Attina, Virginie, Cathiard, Marie-Agnès, and Beautemps, Denis
Abstract: Cued Speech is an efficient method that allows orally educated deaf people to perceive a complete oral message through the visual channel. Using this system, speakers can clarify what they say with the complement of hand cues near the face; similar lip shapes are disambiguated by the addition of a manual cue. In this context, Cued Speech represents a unique system that closely links hand movements and speech since it is based on spoken language. In a previous study, we investigated the temporal organization of French Cued Speech production for a single cueing talker. A specific pattern of coordination was found: the hand anticipates the lips and speech sounds. In the present study, we investigated the cueing behavior of three additional professional cueing talkers. The same pattern of hand cues anticipation was found. Results are discussed with respect to inter-subject variability. A general pattern of coordination is proposed. [ABSTRACT FROM AUTHOR]
Published: 2006
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