Results 101 to 110 of about 2,119 (200)

The value creation radar applied to the space engineering sector: the case of deimos engenharia [PDF]

, 2016
This case study illustrates the application of the Value Creation Radar (VCR) to SenSyF, an Earth Observation (EO) system which was developed by Deimos Engenharia S.A. (DME), the Portuguese affiliate of Elecnor Deimos.
Felizardo, Márcio André Ferreira
core  

Loros: laboratory simulations of the Optical RadiOmeter Composed of CHromatic Imagers (OROCHI) experiment of the Martian Moons eXploration (MMX) mission

Progress in Earth and Planetary Science
The Laboratory OROCHI Simulator (LOROS) is an emulator of the Optical RadiOmeter composed of CHromatic Imagers (OROCHI), a multispectral and multiview imaging system for the Japan Aerospace Exploration Agency (JAXA) Martian Moons eXploration (MMX ...
R. Roger Stabbins, S. Shingo Kameda
doaj   +1 more source

The Keck/DEIMOS Stellar Archive. I. Uniform Velocities and Metallicities for 78 Milky Way Dwarf Galaxies and Globular Clusters

The Astrophysical Journal
We present a homogeneous spectroscopic dataset of 22,339 stars in 78 Milky Way dwarf galaxy satellites and globular clusters. All data were taken with the Keck II telescope and Deep Extragalactic Imaging Multiobject Spectrograph (DEIMOS) using the 1200G ...
Marla Geha, Debora Pelliccia, J. Xavier Prochaska, William Cerny, Frederick B. Davies, Joseph Hennawi, Brad Holden, Dusty Reichwein, Kyle B. Westfall   +8 more
doaj   +1 more source

Long-term dynamical evolution of dusty ejecta from Deimos

, 2005
We re-assess expected properties of the presumed dust belt of Mars formed by impact ejecta from Deimos. Previous studies have shown that dynamics of Deimos particles are dominated by two perturbing forces: radiation pressure (RP) and Mars' oblateness (J2)
Makuch, Martin, Krivov, Alexander V., Spahn, Frank (Prof. Dr.)   +2 more
core  

Analytical protocols for Phobos regolith samples returned by the Martian Moons eXploration (MMX) mission. [PDF]

Earth Planets Space, 2021
Fujiya W, Furukawa Y, Sugahara H, Koike M, Bajo KI, Chabot NL, Miura YN, Moynier F, Russell SS, Tachibana S, Takano Y, Usui T, Zolensky ME.   +12 more
europepmc   +1 more source

The MMX InfraRed Spectrometer (MIRS) for the spectral characterization of the Martian system

Progress in Earth and Planetary Science
MIRS (MMX InfraRed Spectrometer) is a push-broom imaging spectrometer onboard of the JAXA sample return MMX mission. It has been built by the French laboratory LESIA, today LIRA (Laboratory for Instrumentation and Research in Astrophysics) of Paris ...
Maria Antonietta Barucci, Pernelle Bernardi, Jean-Michel Reess, Sonia Fornasier, Frederic Merlin, Alain Doressoundiram, Thomas Gautier, Takahiro Iwata, Hiromu Nakagawa, Tomoki Nakamura, Christophe Donny, Sadok Abbaki, Shohei Aoki, Takehiko Arai, Pierre Beck, Marion Bonafous, Martin Boutelier, Jean-Christophe Bouquier, John Robert Brucato, Mickael Bruno, Jean-Tristan Buey, Matthieu Castelnau, Sebastien Charnoz, Marc Chaussidon, Frederic Chapron, Athena Coustenis, Willy D’anna, Gael David, Marco Delbo, Bruno Dubois, Sebastien Etcheverry, Catherine Garat, Stephane Gauffre, Hidenori Genda, Fabrice Glize, Rafik Hassen-Khodja, Valentin Hazard, Gilles Hervet, Ryuki Hyodo, Takeshi Imamura, Christian Imbert, Sophie Jacquinod, Laurent Jorda, Shingo Kameda, Driss Kouach, Toru Kouyama, Takeshi Kuroda, Hiroyuki Kurokawa, Laurent Lapauw, Jeremie Lasue, Laetitia Le Deit, Michel Le Du, Cedric Leyrat, Christophe Mathé, Moe Matsuoka, Maeva Millan, Hideaki Miyamoto, Frederic Moynier, Napoléon Nguyen Tuong, Kazunori Ogohara, Takahito Osawa, Jerome Parisot, Paolo Pilleri, Veronique Piou, Giovanni Poggiali, Nathalie Pons, Benjamin Quertier-Dagorn, Antsa Rasamoela, Sean Raymond, Francis Rocard, Anne Rouvié, Takeshi Sakanoi, Takao M. Sato, Hervé Soulie, Eric Sawyer, Aymeric Spiga, Robin Sultana, Nicolas Theret, Sylvain Trémolières, Pascal Truchelut, Fuminori Tsuchiya, Pierre Vernazza, Antonin Wargnier, Koki Yumoto, Didier Zeganadin   +84 more
doaj   +1 more source

Pre-DEIMOS Pilot Surveys for DEEP

, 2008
DEEP is a multi-institutional program designed to undertake a major spectroscopic survey of 10,000 field galaxies to I 23 with a new instrument (DEIMOS) on the Keck II 10-m telescope.
David Koo Uco, David C. Koo
core  

DEIMOS Throughput Upgrade

DEIMOS is Keck II’s workhorse optical spectrograph.  It acts as an imager, a longslit spectrograph, and a multislit spectrograph.  Its field of view (approximately 5' × 16') and multiplexing factor (up to about 200 slitlets) are the largest of Keck's instruments.
openaire   +2 more sources

Influence of organic ligands on the stoichiometry of magnetite nanoparticles. [PDF]

Nanoscale Adv, 2023
Jungcharoen P, Marsac R, Choueikani F, Masson D, Pédrot M.   +4 more
europepmc   +1 more source

The DEIMOS spectrograph for the Keck II telescope:

, 2007
The DEIMOS spectrograph is a multi-object spectrograph being built for Keck II. DEIMOS was delivered in February 2002, became operational in May, and is now about three-quarters of the way through its commissioning period.
Integration And Testing, J. Burrous, M. Davis, S. M. Faber, A. L. Coil, D. A. Clarke, T. Cantrall, R. I. Kibrick, S. L. Allen, A. C. Phillips, D. J. Cowley   +10 more
core