Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/34892| Title: | NIOMADA PFM design definition file | Authors: | Martin, Laurent Grupp, Frank GUIZZO, GIAN PAOLO MORGANTE, GIANLUCA Wimmer, Carolin Charles, Yannick Lamesan, Mikel Radaelli, Paolo Hormuth,Felix Pamplona, tony Bonnefoi, Anne Clemens, Jean-Claude Costille, Anne Solheim, Bjarte Barriere, Jean-Christophe |
Issue Date: | 2016 | Number: | EUCL-LAM-RP-7-055 | Abstract: | Euclid is an ESA mission to map the geometry of the dark Universe. The mission will investigate the distance-redshift relationship and the evolution of cosmic structures. It achieves this by measuring shapes and redshifts of galaxies and clusters of galaxies out to redshifts ~2, or equivalently to a lookback time of 10 billion years. It will therefore cover the entire period over which dark energy played a significant role in accelerating the expansion. The Near IR Spectrometer Photometer (NISP) role is to measure the galaxies' redshift. The baseline for NISP is an Infrared instrument allowing observation in slit less "spectrometry" mode thanks to several Grisms, or in "Photometry" mode using several filters. The NISP instrument is provided by the EUCLID consortium, led by the Laboratoire d'Astrophysique de Marseille (LAM). | URI: | http://hdl.handle.net/20.500.12386/34892 | Fulltext: | reserved |
| Appears in Collections: | 4.03 Rapporti di progetto |
Files in This Item:
| File | Description | Size | Format | Existing users please |
|---|---|---|---|---|
| EUCL-LAM-RP-7-055_v1-0_NIOMADA PFM DDF.pdf | [Administrators only] | 6.28 MB | Adobe PDF |
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