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Gómez de Castro, Ana Inés and Sánchez, Néstor and Sestito, Paola and Rodríguez, Pablo and Teresa Gómez, Maite and Seijas, Juan and López-Martinez, Fátima and Quintana, Jose and Ubierna, Marcos and Muñoz, Jacinto (2012) ISSIS: the Imaging and Slitless Spectroscopy Instrument for Surveys in the World Space Observatory Ultraviolet telescope. In pace Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. Proceedings of SPIE (8443). Society of Photo-Optical Instrumentation Engineers (SPIE). ISBN 978-0-8194-9144-2
Official URL: http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1361072
Abstract
ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory - Ultraviolet (WSO-UV), a 170 cm space telescope to be launched in late 2015. ISSIS is a multipurpose instrument designed to carry out high resolution and high sensitivity imaging and slitless spectroscopy in the ultraviolet range. ISSIS has two acquisition channels: the Far Ultraviolet Channel (FUV) covering the 1150-1750 angstrom wavelength range and the Near Ultraviolet Channel (NUV) in the 1850-3200 angstrom range. Both channels are equipped with Multi Channel Plate detectors to guarantee high sensitivity and high rejection of lower energy radiation. ISSIS will be the first UV imager into a high altitude Earth orbit and it will provide unique information on star formation, accretion physics, astronomical engines and planets
Item Type: | Book Section |
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Additional Information: | Conference on Space Telescopes and Instrumentation 2012 - Ultraviolet to Gamma Ray, Amsterdam, NETHERLANDS, JUL 01-06, 2012 |
Subjects: | Sciences > Mathematics > Astronomy Sciences > Mathematics > Astrophysics |
ID Code: | 19948 |
Deposited On: | 13 Feb 2013 09:53 |
Last Modified: | 13 Feb 2013 09:53 |
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