14 results on '"Søren Møller Pedersen"'
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2. Ariel: Enabling planetary science across light-years
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Giovanna Tinetti, Paul Eccleston, Carole Haswell, Pierre-Olivier Lagage, Jérémy Leconte, Theresa Lüftinger, Giusi Micela, Michel Min, Göran Pilbratt, Ludovic Puig, Mark Swain, Leonardo Testi, Diego Turrini, Bart Vandenbussche, Maria Rosa Zapatero Osorio, Anna Aret, Jean-Philippe Beaulieu, Buchhave, Lars A., Martin Ferus, Matt Griffin, Manuel Guedel, Paul Hartogh, Pedro Machado, Giuseppe Malaguti, Enric Pallé, Mirek Rataj, Tom Ray, Ignasi Ribas, Robert Szabó, Jonathan Tan, Stephanie Werner, Francesco Ratti, Carsten Scharmberg, Jean-Christophe Salvignol, Nathalie Boudin, Jean-Philippe Halain, Martin Haag, Pierre-Elie Crouzet, Ralf Kohley, Kate Symonds, Florian Renk, Andrew Caldwell, Manuel Abreu, Gustavo Alonso, Jerome Amiaux, Michel Berthé, Georgia Bishop, Neil Bowles, Manuel Carmona, Deirdre Coffey, Josep Colomé, Martin Crook, Lucile Désjonqueres, Díaz, José J., Rachel Drummond, Mauro Focardi, Gómez, Jose M., Warren Holmes, Matthijs Krijger, Zsolt Kovacs, Tom Hunt, Richardo Machado, Gianluca Morgante, Marc Ollivier, Roland Ottensamer, Emanuele Pace, Teresa Pagano, Enzo Pascale, Chris Pearson, Søren Møller Pedersen, Moshe Pniel, Stéphane Roose, Giorgio Savini, Richard Stamper, Peter Szirovicza, Janos Szoke, Ian Tosh, Francesc Vilardell, Joanna Barstow, Luca Borsato, Sarah Casewell, Quentin Changeat, Benjamin Charnay, Svatopluk Civiš, Vincent Coudé du Foresto, Athena Coustenis, Nicolas Cowan, Camilla Danielski, Olivier Demangeon, Pierre Drossart, Edwards, Billy N., Gabriella Gilli, Therese Encrenaz, Csaba Kiss, Anastasia Kokori, Masahiro Ikoma, Juan Carlos Morales, Joao Mendonca, Andrea Moneti, Lorenzo Mugnai, Antonio García Muñoz, Ravit Helled, Mihkel Kama, Yamila Miguel, Nikos Nikolaou, Isabella Pagano, Olja Panic, Miriam Rengel, Hans Rickman, Marco Rocchetto, Subhajit Sarkar, Franck Selsis, Jonathan Tennyson, Angelos Tsiaras, Olivia Venot, Krisztián Vida, Waldmann, Ingo P., Sergey Yurchenko, Gyula Szabó, Rob Zellem, Ahmed Al-Refaie, Javier Perez Alvarez, Lara Anisman, Axel Arhancet, Jaume Ateca, Robin Baeyens, Barnes, John R., Taylor Bell, Serena Benatti, Katia Biazzo, Maria Błęcka, Aldo Stefano Bonomo, José Bosch, Diego Bossini, Jeremy Bourgalais, Daniele Brienza, Anna Brucalassi, Giovanni Bruno, Hamish Caines, Simon Calcutt, Tiago Campante, Rodolfo Canestrari, Nick Cann, Giada Casali, Albert Casas, Giuseppe Cassone, Christophe Cara, Ludmila Carone, Nathalie Carrasco, Paolo Chioetto, Fausto Cortecchia, Markus Czupalla, Chubb, Katy L., Angela Ciaravella, Antonio Claret, Riccardo Claudi, Claudio Codella, Maya Garcia Comas, Gianluca Cracchiolo, Patricio Cubillos, Vania Da Peppo, Leen Decin, Clemence Dejabrun, Elisa Delgado-Mena, Anna Di Giorgio, Emiliano Diolaiti, Caroline Dorn, Vanessa Doublier, Eric Doumayrou, Georgina Dransfield, Luc Dumaye, Emma Dunford, Antonio Jimenez Escobar, Vincent Van Eylen, Maria Farina, Davide Fedele, Alejandro Fernández, Benjamin Fleury, Sergio Fonte, Jean Fontignie, Luca Fossati, Bernd Funke, Camille Galy, Zoltán Garai, Andrés García, Alberto García-Rigo, Antonio Garufi, Giuseppe Germano Sacco, Paolo Giacobbe, Alejandro Gómez, Arturo Gonzalez, Francisco Gonzalez-Galindo, Davide Grassi, Caitlin Griffith, Mario Giuseppe Guarcello, Audrey Goujon, Amélie Gressier, Aleksandra Grzegorczyk, Tristan Guillot, Gloria Guilluy, Peter Hargrave, Marie-Laure Hellin, Enrique Herrero, Matt Hills, Benoit Horeau, Yuichi Ito, Niels Christian Jessen, Petr Kabath, Szilárd Kálmán, Yui Kawashima, Tadahiro Kimura, Antonín Knížek, Laura Kreidberg, Ronald Kruid, Kruijssen, Diederik J. M., Petr Kubelík, Luisa Lara, Sebastien Lebonnois, David Lee, Maxence Lefevre, Tim Lichtenberg, Daniele Locci, Matteo Lombini, Alejandro Sanchez Lopez, Andrea Lorenzani, Ryan MacDonald, Laura Magrini, Jesus Maldonado, Emmanuel Marcq, Alessandra Migliorini, Darius Modirrousta-Galian, Karan Molaverdikhani, Sergio Molinari, Paul Mollière, Vincent Moreau, Giuseppe Morello, Gilles Morinaud, Mario Morvan, Moses, Julianne I., Salima Mouzali, Nariman Nakhjiri, Luca Naponiello, Norio Narita, Valerio Nascimbeni, Athanasia Nikolaou, Vladimiro Noce, Fabrizio Oliva, Pietro Palladino, Andreas Papageorgiou, Vivien Parmentier, Giovanni Peres, Javier Pérez, Santiago Perez-Hoyos, Manuel Perger, Cesare Cecchi Pestellini, Antonino Petralia, Anne Philippon, Arianna Piccialli, Marco Pignatari, Giampaolo Piotto, Linda Podio, Gianluca Polenta, Giampaolo Preti, Theodor Pribulla, Manuel Lopez Puertas, Monica Rainer, Jean-Michel Reess, Paul Rimmer, Séverine Robert, Albert Rosich, Loic Rossi, Duncan Rust, Ayman Saleh, Nicoletta Sanna, Eugenio Schisano, Laura Schreiber, Victor Schwartz, Antonio Scippa, Bálint Seli, Sho Shibata, Caroline Simpson, Oliver Shorttle, Skaf, N., Konrad Skup, Mateusz Sobiecki, Sergio Sousa, Alessandro Sozzetti, Judit Šponer, Lukas Steiger, Paolo Tanga, Paul Tackley, Jake Taylor, Matthias Tecza, Luca Terenzi, Pascal Tremblin, Andrea Tozzi, Amaury Triaud, Loïc Trompet, Shang-Min Tsai, Maria Tsantaki, Diana Valencia, Ann Carine Vandaele, Mathieu Van der Swaelmen, Adibekyan Vardan, Gautam Vasisht, Allona Vazan, Ciro Del Vecchio, Dave Waltham, Piotr Wawer, Thomas Widemann, Paulina Wolkenberg, Gordon Hou Yip, Yuk Yung, Mantas Zilinskas, Tiziano Zingales, Paola Zuppella, University College of London [London] (UCL), Space Science and Technology Department [Didcot] (RAL Space), STFC Rutherford Appleton Laboratory (RAL), Science and Technology Facilities Council (STFC)-Science and Technology Facilities Council (STFC), Université de Bordeaux (UB), Agence Spatiale Européenne = European Space Agency (ESA), SRON Netherlands Institute for Space Research (SRON), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Catholic University of Leuven - Katholieke Universiteit Leuven (KU Leuven), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astronomico di Bologna (OABO), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Institut d'astrophysique spatiale (IAS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA (UMR_7583)), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB), European Space Agency, Agence Spatiale Européenne (ESA), European Space Agency (ESA), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Giovanna Tinetti, Paul Eccleston, Carole Haswell, Pierre-Olivier Lagage, Jérémy Leconte, Theresa Lüftinger, Giusi Micela, Michel Min, Göran Pilbratt, Ludovic Puig, Mark Swain, Leonardo Testi, Diego Turrini, Bart Vandenbussche, Maria Rosa Zapatero Osorio, Anna Aret, Jean-Philippe Beaulieu, Lars Buchhave, Martin Feru, Matt Griffin, Manuel Guedel, Paul Hartogh, Pedro Machado, Giuseppe Malaguti, Enric Pallé, Mirek Rataj, Tom Ray, Ignasi Riba, Robert Szabó, Jonathan Tan, Stephanie Werner, Francesco Ratti, Carsten Scharmberg, Jean-Christophe Salvignol, Nathalie Boudin, Jean-Philippe Halain, Martin Haag, Pierre-Elie Crouzet, Ralf Kohley, Kate Symond, Florian Renk, Andrew Caldwell, Manuel Abreu, Gustavo Alonso, Jerome Amiaux, Michel Berthé, Georgia Bishop, Neil Bowle, Manuel Carmona, Deirdre Coffey, Josep Colomé, Martin Crook, Lucile Désjonquere, José J. Díaz, Rachel Drummond, Mauro Focardi, Jose M. Gómez, Warren Holme, Matthijs Krijger, Zsolt Kovac, Tom Hunt, Richardo Machado, Gianluca Morgante, Marc Ollivier, Roland Ottensamer, Emanuele Pace, Teresa Pagano, Enzo Pascale, Chris Pearson, Søren Møller Pedersen, Moshe Pniel, Stéphane Roose, Giorgio Savini, Richard Stamper, Peter Szirovicza, Janos Szoke, Ian Tosh, Francesc Vilardell, Joanna Barstow, Luca Borsato, Sarah Casewell, Quentin Changeat, Benjamin Charnay, Svatopluk Civiš, Vincent Coudé du Foresto, Athena Cousteni, Nicolas Cowan, Camilla Danielski, Olivier Demangeon, Pierre Drossart, Billy N. Edward, Gabriella Gilli, Therese Encrenaz, Csaba Ki, Anastasia Kokori, Masahiro Ikoma, Juan Carlos Morale, João Mendonça, Andrea Moneti, Lorenzo Mugnai, Antonio García Muñoz, Ravit Helled, Mihkel Kama, Yamila Miguel, Nikos Nikolaou, Isabella Pagano, Olja Panic, Miriam Rengel, Hans Rickman, Marco Rocchetto, Subhajit Sarkar, Franck Selsi, Jonathan Tennyson, Angelos Tsiara, Olivia Venot, Krisztián Vida, Ingo P. Waldmann, Sergey Yurchenko, Gyula Szabó, Rob Zellem, Ahmed Al-Refaie, Javier Perez Alvarez, Lara Anisman, Axel Arhancet, Jaume Ateca, Robin Baeyen, John R. Barne, Taylor Bell, Serena Benatti, Katia Biazzo, Maria Błęcka, Aldo Stefano Bonomo, José Bosch, Diego Bossini, Jeremy Bourgalai, Daniele Brienza, Anna Brucalassi, Giovanni Bruno, Hamish Caine, Simon Calcutt, Tiago Campante, Rodolfo Canestrari, Nick Cann, Giada Casali, Albert Casa, Giuseppe Cassone, Christophe Cara, Ludmila Carone, Nathalie Carrasco, Paolo Chioetto, Fausto Cortecchia, Markus Czupalla, Katy L. Chubb, Angela Ciaravella, Antonio Claret, Riccardo Claudi, Claudio Codella, Maya Garcia Coma, Gianluca Cracchiolo, Patricio Cubillo, Vania Da Peppo, Leen Decin, Clemence Dejabrun, Elisa Delgado-Mena, Anna Di Giorgio, Emiliano Diolaiti, Caroline Dorn, Vanessa Doublier, Eric Doumayrou, Georgina Dransfield, Luc Dumaye, Emma Dunford, Antonio Jimenez Escobar, Vincent Van Eylen, Maria Farina, Davide Fedele, Alejandro Fernández, Benjamin Fleury, Sergio Fonte, Jean Fontignie, Luca Fossati, Bernd Funke, Camille Galy, Zoltán Garai, Andrés García, Alberto García-Rigo, Antonio Garufi, Giuseppe Germano Sacco, Paolo Giacobbe, Alejandro Gómez, Arturo Gonzalez, Francisco Gonzalez-Galindo, Davide Grassi, Caitlin Griffith, Mario Giuseppe Guarcello, Audrey Goujon, Amélie Gressier, Aleksandra Grzegorczyk, Tristan Guillot, Gloria Guilluy, Peter Hargrave, Marie-Laure Hellin, Enrique Herrero, Matt Hill, Benoit Horeau, Yuichi Ito, Niels Christian Jessen, Petr Kabath, Szilárd Kálmán, Yui Kawashima, Tadahiro Kimura, Antonín Knížek, Laura Kreidberg, Ronald Kruid, Diederik J. M. Kruijssen, Petr Kubelík, Luisa Lara, Sebastien Lebonnoi, David Lee, Maxence Lefevre, Tim Lichtenberg, Daniele Locci, Matteo Lombini, Alejandro Sanchez Lopez, Andrea Lorenzani, Ryan MacDonald, Laura Magrini, Jesus Maldonado, Emmanuel Marcq, Alessandra Migliorini, Darius Modirrousta-Galian, Karan Molaverdikhani, Sergio Molinari, Paul Mollière, Vincent Moreau, Giuseppe Morello, Gilles Morinaud, Mario Morvan, Julianne I. Mose, Salima Mouzali, Nariman Nakhjiri, Luca Naponiello, Norio Narita, Valerio Nascimbeni, Athanasia Nikolaou, Vladimiro Noce, Fabrizio Oliva, Pietro Palladino, Andreas Papageorgiou, Vivien Parmentier, Giovanni Pere, Javier Pérez, Santiago Perez-Hoyo, Manuel Perger, Cesare Cecchi Pestellini, Antonino Petralia, Anne Philippon, Arianna Piccialli, Marco Pignatari, Giampaolo Piotto, Linda Podio, Gianluca Polenta, Giampaolo Preti, Theodor Pribulla, Manuel Lopez Puerta, Monica Rainer, Jean-Michel Ree, Paul Rimmer, Séverine Robert, Albert Rosich, Loic Rossi, Duncan Rust, Ayman Saleh, Nicoletta Sanna, Eugenio Schisano, Laura Schreiber, Victor Schwartz, Antonio Scippa, Bálint Seli, Sho Shibata, Caroline Simpson, Oliver Shorttle, N. Skaf, Konrad Skup, Mateusz Sobiecki, Sergio Sousa, Alessandro Sozzetti, Judit Šponer, Lukas Steiger, Paolo Tanga, Paul Tackley, Jake Taylor, Matthias Tecza, Luca Terenzi, Pascal Tremblin, Andrea Tozzi, Amaury Triaud, Loïc Trompet, Shang-Min Tsai, Maria Tsantaki, Diana Valencia, Ann Carine Vandaele, Mathieu Van der Swaelmen, Adibekyan Vardan, Gautam Vasisht, Allona Vazan, Ciro Del Vecchio, Dave Waltham, Piotr Wawer, Thomas Widemann, Paulina Wolkenberg, Gordon Hou Yip, Yuk Yung, Mantas Zilinska, Tiziano Zingale, Paola Zuppella, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS Paris), and Cardon, Catherine
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[SDU] Sciences of the Universe [physics] ,Earth and Planetary Astrophysics (astro-ph.EP) ,[SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Settore FIS/05 - Astronomia E Astrofisica ,[SDU]Sciences of the Universe [physics] ,[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] ,[SDU.ASTR.EP] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] ,FOS: Physical sciences ,Astrophysics - Instrumentation and Methods for Astrophysic ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Astrophysics - Earth and Planetary Astrophysics ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] - Abstract
Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. During its 4-year mission, Ariel will study what exoplanets are made of, how they formed and how they evolve, by surveying a diverse sample of about 1000 extrasolar planets, simultaneously in visible and infrared wavelengths. It is the first mission dedicated to measuring the chemical composition and thermal structures of hundreds of transiting exoplanets, enabling planetary science far beyond the boundaries of the Solar System. The payload consists of an off-axis Cassegrain telescope (primary mirror 1100 mm x 730 mm ellipse) and two separate instruments (FGS and AIRS) covering simultaneously 0.5-7.8 micron spectral range. The satellite is best placed into an L2 orbit to maximise the thermal stability and the field of regard. The payload module is passively cooled via a series of V-Groove radiators; the detectors for the AIRS are the only items that require active cooling via an active Ne JT cooler. The Ariel payload is developed by a consortium of more than 50 institutes from 16 ESA countries, which include the UK, France, Italy, Belgium, Poland, Spain, Austria, Denmark, Ireland, Portugal, Czech Republic, Hungary, the Netherlands, Sweden, Norway, Estonia, and a NASA contribution., Comment: Ariel Definition Study Report, 147 pages. Reviewed by ESA Science Advisory Structure in November 2020. Original document available at: https://www.cosmos.esa.int/documents/1783156/3267291/Ariel_RedBook_Nov2020.pdf/
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- 2021
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3. The ARIEL payload: A technical overview
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Berend Winter, Ian Tosh, Aymen Saleh, José M. Gómez, Konrad Skup, Emanuele Pace, Vincent Moreau, Enzo Pascale, Andre Wong, L. Puig, C. J. Simpson, Edward C. Tong, Paul Eccleston, Josep Colomé, Jérôme Amiaux, Gustavo Alonso, Miroslaw Rataj, Rachel Drummond, Warren Holmes, Marshall D. Perrin, Nathalie Boudin, R. Stamper, Mark R. Swain, Marc Ollivier, Andrew Caldwell, P. Zuppella, Piotr Wawer, Anne Philippon, Vania Da Deppo, Kevin Middleton, Lucile Desjonqueres, Marie-Laure Hellin, Nicholas Siegler, Lisa Gambicorti, Martin Crook, Michel Berthé, Mauro Focardi, Javier Perez Alvarez, Francesc Vilardell, Niels Christian Jessen, Steve Roose, Mateusz Sobiecki, Peter Charles Hargrave, Natalie Batalha, Gianluca Morgante, Matthew Joseph Griffin, Nick Cann, Matthew Hills, Chris Pearson, Martin Linder, Matthijs Krijger, Christophe Cara, Göran Pilbratt, T. Hunt, Makenzie Lystrup, Georgia Bishop, Hanno Ertel, Jean-Philippe Halain, Markus Czupalla, Giuseppe Malaguti, Martin Frericks, Giovanna Tinetti, Roland Ottensamer, Duncan Rust, and Søren Møller Pedersen
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Cosmic Vision ,Spectrometer ,Spacecraft ,business.industry ,Payload ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Photometer ,Exoplanet ,law.invention ,Telescope ,Photometry (astronomy) ,law ,Environmental science ,Astrophysics::Earth and Planetary Astrophysics ,Aerospace engineering ,business ,Astrophysics::Galaxy Astrophysics - Abstract
The Atmospheric Remote-Sensing Infrared Exoplanet Large-survey, ARIEL, has been selected to be the next (M4) medium class space mission in the ESA Cosmic Vision programme. From launch in 2028, and during the following 4 years of operation, ARIEL will perform precise spectroscopy of the atmospheres of ~1000 known transiting exoplanets using its metre-class telescope. A three-band photometer and three spectrometers cover the 0.5 µm to 7.8 µm region of the electromagnetic spectrum. This paper gives an overview of the mission payload, including the telescope assembly, the FGS (Fine Guidance System) - which provides both pointing information to the spacecraft and scientific photometry and low-resolution spectrometer data, the ARIEL InfraRed Spectrometer (AIRS), and other payload infrastructure such as the warm electronics, structures and cryogenic cooling systems.
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- 2020
4. The X/Gamma-ray Imaging Spectrometer (XGIS) on-board THESEUS: Design, main characteristics, and concept of operation
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Sandro Mereghetti, Lorenzo Amati, J. L. Gasent-Blesa, Denis Tcherniak, Piero Malcovati, F. Fuschino, Piero Rosati, P. Bellutti, Natalia Auricchio, Giacomo Borghi, A. de Rosa, Irfan Kuvvetli, Francesco Ficorella, M. Fiorini, Andrea Santangelo, E. Demenev, Giuseppe Bertuccio, A. Picciotto, C. Guidorzi, G. Zampa, Giuseppe Sottile, Riccardo Campana, Raffaele Piazzolla, Søren Møller Pedersen, F. Evangelisti, Pedro Rodríguez-Martínez, Mauro Orlandini, Paolo Lorenzi, Luca Terenzi, Nadia Zorzi, M. Melchiorri, M. Winkler, Paolo Sarra, Filippo Frontera, E. Virgilli, I. Rashevskaya, C. Tenzer, P. H. Connell, J. Navarro-González, A. Vacchi, Miriam Grassi, V. Reglero, F. Mele, V. Da Ronco, J. B. Stephen, V. Zanini, Piotr Orleanski, A. Volpe, A. J. Castro-Tirado, N. Zampa, Paul Hedderman, A. Rachevski, Giuseppe Baldazzi, Alessio Trois, M. Gandola, Benjamin Pinazo-Herrero, R. C. Butler, Gianluca Morgante, G. La Rosa, Claudio Labanti, S. Squerzanti, den Herder, Jan-Willem A., Labanti C., Amati L., Frontera F., Mereghetti S., Gasent-Blesa J.L., Tenzer C., Orleanski P., Kuvvetli I., Campana R., Fuschino F., Terenzi L., Virgilli E., Morgante G., Orlandini M., Butler R.C., Stephen J.B., Auricchio N., de Rosa A., da Ronco V., Evangelisti F., Melchiorri M., Squerzanti S., Fiorini M., Bertuccio G., Mele F., Gandola M., Malcovati P., Grassi M., Bellutti P., Borghi G., Ficorella F., Picciotto A., Zanini V., Zorzi N., Demenev E., Rashevskaya I., Rachevski A., Zampa G., Vacchi A., Zampa N., Baldazzi G., la Rosa G., Sottile G., Volpe A., Winkler M., Reglero V., Connell P., Pinazo-Herrero B., Navarro-Gonzalez J., Rodriguez-Martinez P., Castro-Tirado A.J., Santangelo A., Hedderman P., Lorenzi P., Sarra P., Pedersen S.M., Tcherniak A.D., Guidorzi C., Rosati P., Trois A., Piazzolla R., Agenzia Spaziale Italiana, European Space Agency, Ministerio de Ciencia e Innovación (España), European Commission, National Science Centre (Poland), Foundation for Polish Science, ITA, DEU, ESP, DNK, POL, Herder, Jan-Willem A. den, Nikzad, Shouleh, and Nakazawa, Kazuhiro
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Cosmic Vision ,ESA Missions ,Gamma-ray detectors ,Astrophysics::High Energy Astrophysical Phenomena ,Infrared telescope ,Imaging spectrometer ,X-ray detector ,FOS: Physical sciences ,Silicon Drift Detectors ,Scintillator ,01 natural sciences ,law.invention ,Telescope ,ESA Mission ,Optics ,law ,Coded Mask Imaging ,0103 physical sciences ,Gamma ray astronomy ,XGIS ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,010303 astronomy & astrophysics ,Physics ,Spectrometer ,010308 nuclear & particles physics ,business.industry ,Gamma Ray Bursts ,Astrophysics::Instrumentation and Methods for Astrophysics ,X-ray detectors ,Gamma-ray astronomy ,Gamma Ray Burst ,THESEUS ,Astrophysics - Instrumentation and Methods for Astrophysics ,business ,Gamma-ray Bursts - Abstract
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray; Virtual, Online; United States; 14 December 2020 through 18 December 2020; Code 166330.--Proceedings of SPIE - The International Society for Optical Engineering Volume 11444, 2020, Article number 114442K.--Full list of authors: Labanti, C.; Amati, L.; Frontera, F.; Mereghetti, S.; Gasent-Blesa, J. L.; Tenzer, C.; Orleanski, P.; Kuvvetli, I.; Campana, R.; Fuschino, F.; Terenzi, L.; Virgilli, E.; Morgante, G.; Orlandini, M.; Butler, R. C.; Stephen, J. B.; Auricchio, N.; De Rosa, A.; Da Ronco, V.; Evangelisti, F. Melchiorri, M.; Squerzanti, S.; Fiorini, M.; Bertuccio, G.; Mele, F.; Gandola, M.; Malcovati, P.; Grassi, M.; Bellutti, P.; Borghi, G.; Ficorella, F.; Picciotto, A.; Zanini, V.; Zorzi, N.; Demenev, E.; Rashevskaya, I.; Rachevski, A.; Zampa, G.; Vacchi, A.; Zampa, N.; Baldazzi, G.; La Rosa, G.; Sottile, G.; Volpe, A.; Winkler, M.; Reglero, V.; Connell, P. H.; Pinazo-Herrero, B.; Navarro-González, J.; Rodríguez-Martínez, P.; Castro-Tirado, A. J.; Santangelo, A.; Hedderman, P.; Lorenzi, P.; Sarra, P.; Pedersen, S. M.; Tcherniak, D.; Guidorzi, C.; Rosati, P.; Trois, A.; Piazzolla, R., THESEUS (Transient High Energy Sky and Early Universe Surveyor) is one of the three missions selected by ESA as fifth medium class mission (M5) candidates in its Cosmic Vision science program, currently under assessment in a phase A study with a planned launch date in 2032. THESEUS is designed to carry on-board two wide and deep sky monitoring instruments for X/gamma-ray transients detection: a wide-field soft X-ray monitor with imaging capability (Soft X-ray Imager, SXI, 0.3 - 5 keV), a hard X-ray, partially-imaging spectroscopic instrument (X and Gamma Imaging Spectrometer, XGIS, 2 keV - 10 MeV), and an optical/near-IR telescope with both imaging and spectroscopic capability (InfraRed Telescope, IRT, 0.7 - 1.8 µm). The spacecraft will be capable of performing fast repointing of the IRT to the error region provided by the monitors, thus allowing it to detect and localize the transient sources down to a few arcsec accuracy, for immediate identification and redshift determination. The prime goal of the XGIS will be to detect transient sources, with monitoring timescales down to milliseconds, both independently of, or following up, SXI detections, and identify the sources performing localisation at, The Phase A study of the THESEUS/XGIS instrument is supported by ASI-INAF Agreement n. 2018-29-HH.0, OHB Italia/ - INAF-OASBo Agreement n.2331/2020/01, by the European Space Agency ESA through the M5/NPMC Programme and by the AHEAD2020 project funded by UE through H2020-INFRAIA-2018-2020. By the Spanish Ministerio de Ciencia e Innovación, PID2019-109269RB-C41. By Polish National Science Center, Project 2019/35/B/ST9/03944 and Foundation for Polish Science, Project POIR.04.04.00-00-5C65/17-00.
- Published
- 2020
5. The XGIS instrument on-board THESEUS: the detection plane and on-board electronics
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Paolo Lorenzi, G. Zampa, Miriam Grassi, I. Rashevskaya, M. Winkler, Lorenzo Amati, Piero Malcovati, Lucas Christoffer Bune Jensen, P. Bellutti, Giacomo Borghi, Francesco Ficorella, Giuseppe Sottile, A. Picciotto, Alessandro Gemelli, F. Mele, E. Virgilli, Riccardo Campana, Søren Møller Pedersen, F. Fuschino, Ifran Kuvvetli, G. La Rosa, Piotr Orleanski, Claudio Labanti, Andrea Santangelo, Denis Tcherniak, Paul Hedderman, A. Rachevski, Luca Terenzi, C. Tenzer, A. Vacchi, M. Gandola, Nicola Zorzi, Paolo Sarra, N. Zampa, Giuseppe Bertuccio, A. den Herder, Jan-Willem, Nikzad, Shouleh, and Nakazawa, Kazuhiro
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Scintillation ,Cosmic Vision ,Spectrometer ,Physics::Instrumentation and Detectors ,business.industry ,Computer science ,ASIC ,Detector ,Electrical engineering ,FOS: Physical sciences ,Photodetector ,Chipset ,Integrated circuit ,law.invention ,ORION ,law ,Scintillator crystals ,Silicon Drift Detector ,THESEUS mission ,Redundancy (engineering) ,Electronics ,Astrophysics - Instrumentation and Methods for Astrophysics ,business ,Instrumentation and Methods for Astrophysics (astro-ph.IM) - Abstract
The X and Gamma Imaging Spectrometer instrument on-board the THESEUS mission (selected by ESA in the framework of the Cosmic Vision M5 launch opportunity, currently in phase A) is based on a detection plane composed of several thousands of single active elements. Each element comprises a 4.5x4.5x30 mm 3 CsI(Tl) scintillator bar, optically coupled at both ends to Silicon Drift Detectors (SDDs). The SDDs acts both as photodetectors for the scintillation light and as direct X-ray sensors. In this paper the design of the XGIS detection plane is reviewed, outlining the strategic choices in terms of modularity and redundancy of the system. Results on detector-electronics prototypes are also described. Moreover, the design and development of the low-noise front-end electronics is presented, emphasizing the innovative architectural design based on custom-designed Application-Specific Integrated Circuits (ASICs)., Comment: Proceedings of the SPIE 2020, paper 11444-277
- Published
- 2020
6. Testing NISP instrument on ground
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Anne Costille, Christophe Fabron, A. N. Sorensen, Michael I. Andersen, M. Pons, Søren Møller Pedersen, T. Maciaszek, Eric Prieto, M. Carle, N. C. Jensen, Sodnik, Zoran, Karafolas, Nikos, and Cugny, Bruno
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Ground support equipment ,Computer science ,Payload ,business.industry ,Optical instrument ,Detector ,Metrology ,Blank ,law.invention ,Telescope ,Laser tracker ,law ,NISP ,ERIOS ,Calibration ,Aerospace engineering ,business ,Telescope simulator - Abstract
The Laboratoire d’Astrophysique de Marseille (LAM) is deeply involved in the development and the test of the NISP (Near Infrared Spectro-Photometer) instrument for the ESA EUCLID mission that will be launched in 2020. The goal of the mission is to understand the nature of the dark energy responsible for the accelerating expansion of the Universe. NISP is one of its two instruments operating in the near-IR spectral region (0.9-2μm) to map the geometry of the dark Universe. The integration of the NISP flight model (FM) has been started at LAM to allow its delivery in 2019 to the payload after vibration test and two thermal vacuum test campaigns to demonstrate the performance of the instrument. The thermal vacuum test will take place in ERIOS chamber, a 90m3 chamber developed by LAM to test optical instruments at cryogenics temperature and high vacuum. In addition to the chamber, a full and specialised set of ground support equipment called the Verification Ground System (VGS) is developed to fill the goal of the NISP test campaign. The test campaign combines functional tests of the detectors and wheels, performance tests of the instrument, calibration procedure validation and observations scenario test, all done at LAM. One of the main objectives of the test campaign is the measurement of NISP focus position with respect to the EUCLID object plane. The VGS is made of i) a telescope simulator to simulate the EUCLID telescope for optical performance tests, ii) a thermal environment to simulate the Euclid PLM thermal interfaces, iii) the NISP Electrical GSE (EGSE) to control the instrument during the test and iv) a Metrology Verification System (MVS) to measure the positions of NISP and the telescope simulator during the test. We present the set of GSE developed for NISP and their performance already validated during two blank tests: thermal blank test and metrology blank test. In addition, a blank test with all the VGS parts (thermal, optical, metrology) is scheduled in the coming months to validate the overall performance of this GSE including the telescope simulator. The goal is to measure with a high precision the focus distance of the telescope simulator at cold and the stability of the focus in time, and to demonstrate the functionality of the telescope simulator for NISP test campaign needs. Finally, we describe the thermal vacuum test configuration for the “end to end� test on the NISP flight model foreseen by beginning of 2019.
- Published
- 2019
7. Atmosphere-Space Interactions Monitor, Instrument and First Results
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J. Polny, Carl Budtz-Jørgensen, Nikolai Østgaard, Carol Anne Oxborrow, Peter Brauer, Freddy Christiansen, Ib Lundgaard Rasmussen, Lasse Husbjerg, Torsten Neubert, Per Lundahl Thomsen, Søren Møller Pedersen, Irfan Kuvvetli, Steen Savstrup Kristensen, Niels Christian Jessen, Denis Tcherniak, Victor Reglero, Olivier Chanrion, C. Stoltze, Jan E. Balling, and Krystallia Dimitriadou
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010504 meteorology & atmospheric sciences ,business.industry ,Multispectral image ,Modular design ,Space (mathematics) ,01 natural sciences ,Lightning ,Atmosphere ,Observatory ,0103 physical sciences ,International Space Station ,Thunderstorm ,Environmental science ,business ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Remote sensing - Abstract
The Atmosphere-Space Interaction Monitor (ASIM) is an observatory mounted outside the Columbus module on the International Space Station. It has been operational since April 13th, 2018. It contains two instruments: The Modular X- and Gamma-ray Sensor (MXGS) and The Modular Multispectral Imaging Array (MMIA). The objective of ASIM is to monitor thunderstorms and auroras, including lightning discharges, especially discharges upwards above thunderstorms. This paper presents the instrument package and some first results.
- Published
- 2019
8. The Modular X- and Gamma-Ray Sensor (MXGS)of the ASIM Payload on the International Space Station
- Author
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Shiming Yang, Pavlo Kochkin, Irfan Kuvvetli, Steen Savstrup Kristensen, B. H. Qureshi, Yngve Skogseide, Pawel Grudzinski, Waldemar Bujwan, J. Navarro-González, Brant Carlson, J. M. Rodrigo, Thomas Riis Bjørnsen, Johan Stadsnes, A. Solberg, Victor Reglero, C. J. Eyles, Georgi Genov, Kjetil Ullaland, Jan E. Balling, Torsten Neubert, Carl Budtz-Jørgensen, Anja Kohfeldt, Peter Brauer, M. D. Sabau, Maja Elise Rostad, Freddy Christiansen, Søren Møller Pedersen, Nikolai Østgaard, M. Reina, Kare Njoten, P. Connell, Linga Reddy Cenkeramaddi, Piotr Orleanski, Per Lundahl Thomsen, and Dominik Fehlker
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Modular Multi-Spectral Imaging Assembly ,Physics - Instrumentation and Detectors ,010504 meteorology & atmospheric sciences ,Modular X- and Gamma-ray Sensor ,FOS: Physical sciences ,Terrestrial Gamma-ray Flashes ,International Space Station ,01 natural sciences ,Physics - Space Physics ,0103 physical sciences ,010303 astronomy & astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Atmosphere-Space Interaction Monitor ,0105 earth and related environmental sciences ,Remote sensing ,Physics ,business.industry ,Payload ,Gamma ray ,X- and Gamma-ray detector for space ,Astronomy and Astrophysics ,Instrumentation and Detectors (physics.ins-det) ,Modular design ,Lightning ,Space Physics (physics.space-ph) ,Photometry (astronomy) ,Space and Planetary Science ,Transient (oscillation) ,Astrophysics - Instrumentation and Methods for Astrophysics ,business - Abstract
The Modular X- and Gamma-ray Sensor (MXGS) is an imaging and spectral X- and Gamma-ray instrument mounted on the starboard side of the Columbus module on the International Space Station. Together with the Modular Multi-Spectral Imaging Assembly (MMIA) (Chanrion et al. this issue) MXGS constitutes the instruments of the Atmosphere-Space Interactions Monitor (ASIM) (Neubert et al. this issue). The main objectives of MXGS are to image and measure the spectrum of X- and γ-rays from lightning discharges, known as Terrestrial Gamma-ray Flashes (TGFs), and for MMIA to image and perform high speed photometry of Transient Luminous Events (TLEs) and lightning discharges. With these two instruments specifically designed to explore the relation between electrical discharges, TLEs and TGFs, ASIM is the first mission of its kind. With an imaging system and a large detector area MXGS will, for the first time, allow estimation of the location of the source region and characterization of the energy spectrum of individual events. The sensors have fast readout electronics to minimize pileup effects, giving high time resolution of photon detection for comparison with measurements on μs-time scales of lightning processes measured by the MMIA and other sensors in space or on the ground. The detectors cover the large energy range of the relevant photon energies. In this paper we describe the scientific objectives, design, performance, imaging capabilities and operational modes of the MXGS instrument. publishedVersion
- Published
- 2019
- Full Text
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9. Readout for intersatellite laser interferometry: Measuring low frequency phase fluctuations of high-frequency signals with microradian precision
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Michael Tröbs, Christian Diekmann, Gerhard Heinzel, Zoran Sodnik, Anders Engaard, N. Brause, Simon Barke, J. Reiche, Oliver Jennrich, Torben Vendt Hansen, Juan José Delgado, Ioury Bykov, Torben Rasmussen, Karsten Danzmann, Søren Møller Pedersen, Joachim Kullmann, Oliver Gerberding, Martin Suess, and Thomas S. Schwarze
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Physics ,Physics - Instrumentation and Detectors ,business.industry ,Gravitational wave ,Physics::Instrumentation and Detectors ,Detector ,Beat (acoustics) ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,Low frequency ,Breadboard ,Technology development ,symbols.namesake ,Laser interferometry ,Optics ,symbols ,business ,Instrumentation ,Doppler effect - Abstract
Precision phase readout of optical beat note signals is one of the core techniques required for intersatellite laser interferometry. Future space based gravitational wave detectors like eLISA require such a readout over a wide range of MHz frequencies, due to orbit induced Doppler shifts, with a precision in the order of $\mu \textrm{rad}/\sqrt{\textrm{Hz}}$ at frequencies between $0.1\,\textrm{mHz}$ and $1\,\textrm{Hz}$. In this paper, we present phase readout systems, so-called phasemeters, that are able to achieve such precisions and we discuss various means that have been employed to reduce noise in the analogue circuit domain and during digitisation. We also discuss the influence of some non-linear noise sources in the analogue domain of such phasemeters. And finally, we present the performance that was achieved during testing of the elegant breadboard model of the LISA phasemeter, that was developed in the scope of an ESA technology development activity., Comment: submitted to Review of Scientific Instruments on April 30th 2015
- Published
- 2015
10. JEM–X inflight performance
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A. A. Zdziarski, C. Gomez, M. Morawski, Osmi Vilhu, E. Morelli, Niels Lund, Niels Jørgen Stenfeldt Westergaard, K. H. Andersen, G. Giulianelli, S. Maisala, R. Carli, Enrico Costa, G. Sarri, J. Polny, S. Larrson, T. Andersson, K. Omø, M. Rezazad, R. Much, Carl Budtz-Jørgensen, S. Laursen, Victor Reglero, A. Rubini, Juhani Huovelin, S. Martínez Núñez, M. Feroci, G. Juchnikowski, V. Carassiti, Carol Anne Oxborrow, P. L. Jensen, A. J. Castro-Tirado, Massimo Rapisarda, Allan Hornstrup, Herbert W. Schnopper, Peter Kretschmar, Astrid Orr, F. Cordero, Michael Schmidt, C. Pelliciari, Jérôme Chenevez, Filippo Frontera, M. Goria, G. Loffredo, Ib Lundgaard Rasmussen, H. Andersson, Søren Møller Pedersen, R. Svensson, Søren Brandt, and P. A. Jensen
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Physics ,Instrumentation: detectors ,X-rays: general ,010308 nuclear & particles physics ,Detectors ,X–rays ,JEM-X ,Astronomy and Astrophysics ,UNESCO::ASTRONOMÍA Y ASTROFÍSICA ,ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO] ,01 natural sciences ,Space and Planetary Science ,0103 physical sciences ,Calibration ,UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia ,010303 astronomy & astrophysics ,ASTRONOMÍA Y ASTROFÍSICA [UNESCO] ,Remote sensing - Abstract
We summarize the inflight performance of JEM-X, the X-ray monitor on the INTEGRAL mission during the initial ten months of operations. The JEM-X instruments have now been tuned to stable operational conditions. The performance is found to be close to the pre-launch expectations. The ground calibrations and the inflight calibration data permit to determine the instruments characteristics to fully support the scientific data analysis. Reglero Velasco, Victor, Victor.Reglero@uv.es ; Martinez Nuñez, Silvia, Silvia.Martinez@uv.es
- Published
- 2003
11. The design of the wide field monitor for the LOFT mission
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Piotr Orleanski, René Hudec, Flemming Hansen, A. Vacchi, G. Zampa, P. Azzarello, E. Del Monte, M. Pohl, A. A. Zdziarski, D. Gotz, Christian Schmid, Niels Lund, A. Argan, C. Tenzer, Poul Erik Holmdahl Olsen, Juhani Huovelin, A. Rachevski, J. L. Galvez Sanchez, M. Michalska, F. Zwart, J. J. M. in 't Zand, Enrico Bozzo, Stéphane Schanne, D. Karelin, S. Korpela, Andrea Santangelo, J. W. den Herder, Didier Barret, Riccardo Campana, Søren Møller Pedersen, Alain Cros, M. Hernanz, N. Zampa, Carl Budtz-Jørgensen, B. Artigues, Jörn Wilms, I. Donnarumma, Y. Evangelista, S. Brandt, Dom Walton, Silvia Zane, Laura Alvarez, Marco Feroci, and Slawomir Suchy
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Cosmic Vision ,Computer science ,media_common.quotation_subject ,Silicon Drift Detectors ,SA Missions ,7. Clean energy ,Collimated light ,Coded Mask Imaging ,Compact Objects ,Gamma Ray Bursts ,LOFT Wide Field Monitor ,Electronic, Optical and Magnetic Materials ,Condensed Matter Physics ,Computer Science Applications1707 Computer Vision and Pattern Recognition ,Applied Mathematics ,Electrical and Electronic Engineering ,Observatory ,Electronic ,Sensitivity (control systems) ,Optical and Magnetic Materials ,Remote sensing ,media_common ,Sky ,Transient (oscillation) ,Gamma-ray burst ,Energy (signal processing) - Abstract
LOFT (Large Observatory For x-ray Timing) is one of the ESA M3 missions selected within the Cosmic Vision program in 2011 to carry out an assessment phase study and compete for a launch opportunity in 2022-2024. The phase-A studies of all M3 missions were completed at the end of 2013. LOFT is designed to carry on-board two instruments with sensitivity in the 2-50 keV range: a 10 m2 class Large Area Detector (LAD) with a
- Published
- 2014
12. JEM-X: three years in space
- Author
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Niels J. Westergaard, A. A. Zdziarski, J. Polny, M. Feroci, S. Larsson, Carl Budtz-Jørgensen, Jérôme Chenevez, I. Lundgaard Rasmussen, F. Frontera, S. Martínez-Núñez, S. Laursen, Niels Lund, G. Juchnikowski, Osmi Vilhu, Carol Anne Oxborrow, Victor Reglero, Peter Kretschmar, Søren Møller Pedersen, S. Fahmy, and S. Brandt
- Subjects
Physics ,Software ,Optics ,business.industry ,Systems engineering ,Orbit (dynamics) ,Analysis software ,Duration (project management) ,Orbital mechanics ,Space (commercial competition) ,business ,Silicon microstrip detectors ,Space environment - Abstract
We report on the technical and scientific performance of JEM-X, the X-ray monitor on ESA's INTEGRAL mission. INTEGRAL has now been in orbit for more than three years, and the mission is foreseen to be extended until the end of 2010. Overall, JEM-X performs very well, and can be expected to continue to do so for the duration of the mission. We discuss in some detail the operational experiences and the problems encountered with the microstrip detectors caused by the space environment and give one example of the interesting scientific results obtained. The analysis software is still being improved on, and we discuss briefly the significance of these improvements.
- Published
- 2006
13. JEM-X: The X-ray monitor aboard INTEGRAL
- Author
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Niels Lund, Carl Budtz-Jørgensen, Niels Jørgen Stenfeldt Westergaard, Søren Brandt, Ib Lundgaard Rasmussen, Allan Hornstrup, Carol Anne Oxborrow, Jérôme Chenevez, Poul Anker Jensen, Steen Laursen, Kh, Andersen, Mogensen, P. B., Ib Rasmussen, Omo, K., Søren Møller Pedersen, Jozef Polny, 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., Peter Løkke Jensen, Sarri, G., Tiemon, A., Orr, A., Much, R., Kretschmar, P., and Schnopper, H. W.
14. JEM-X inflight performance
- Author
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Søren Brandt, Carl Budtz-Jørgensen, Niels Lund, Niels Jørgen Stenfeldt Westergaard, Ib Lundgaard Rasmussen, Andersen, K. H., Jérôme Chenevez, Allan Hornstrup, Poul Anker Jensen, Steen Laursen, Omo, K., Carol Anne Oxborrow, Søren Møller Pedersen, Jozef Polny, Andersson, H., Andersson, T., Vilhu, O., Huovelin, J., Maisala, S., Morawski, M., Juchnikowski, G., Costa, E., Feroci, M., Rubini, A., Rapisarda, M., Morelli, E., Frontera, F., Pelliciari, C., Loffredo, G., Carassiti, V., Reglero, V., Nunez, S. M., Larsson, S., Svensson, R., Zdziarski, A. A., Castro-Tirado, A., Goria, M., Giulianelli, G., Rezazad, M., Carli, R., Peter Løkke Jensen, Cordero, F., Schmidt, M. N., Sarri, G., Gomez, C., Orr, A., Much, R., Schnopper, H. W., and Kretschmar, P.
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