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The imaging and slitless spectroscopy instrument for surveys (ISSIS) for the world space observatory-ultraviolet (WSO-UV)
ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory-Ultraviolet (WSO-UV) mission. ISSIS is a multipurpose instrument designed to carry out high resolution (
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| Published in: | Astrophysics and space science 2011-09, Vol.335 (1), p.283-289 |
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| Main Authors: | , , , , , , , , , |
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| cites | cdi_FETCH-LOGICAL-c446t-1e3e7ca738e84bf03938d612f4c76d5ee6bdf13a6c84239b71cc4a96ec334b1e3 |
| container_end_page | 289 |
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| container_title | Astrophysics and space science |
| container_volume | 335 |
| creator | Gómez de Castro, Ana I. Maíz, Jesús Rodriguez, Pablo Gómez, Maite Larruquert, Juan A. Méndez, José A. Belenguer, Tomas Rodrigo-Gudiel, Victor López-Martínez, Fátima Sestito, Paola |
| description | ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory-Ultraviolet (WSO-UV) mission. ISSIS is a multipurpose instrument designed to carry out high resolution ( |
| doi_str_mv | 10.1007/s10509-011-0695-9 |
| format | article |
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. ISSIS has two acquisition channels: the High Sensitivity Channel (HSC) and the Channel for Surveys (CfS). The HSC is equipped with an MCP-type detector to guarantee high sensitivity in the 1150–1750 Å range and high rejection of lower energy radiation. The CfS is equipped with a large CCD detector (4k×4k) to obtain images from the far UV to the red (1150–8500 Å); the CfS is implemented to allow observing UV bright sources such as reflection nebulae or nearby massive star forming regions. The design drivers and the current status of the instrument are described in this contribution.</description><identifier>ISSN: 0004-640X</identifier><identifier>EISSN: 1572-946X</identifier><identifier>DOI: 10.1007/s10509-011-0695-9</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Astrobiology ; Astronomy ; Astrophysics ; Astrophysics and Astroparticles ; Channels ; Charge coupled devices ; Cosmology ; Detectors ; Imaging ; Massive stars ; Observations and Techniques ; Original Article ; Physics ; Physics and Astronomy ; Scientific apparatus & instruments ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Space telescopes ; Spectroscopy ; Spectrum analysis ; Surveys ; Ultraviolet astronomy</subject><ispartof>Astrophysics and space science, 2011-09, Vol.335 (1), p.283-289</ispartof><rights>Springer Science+Business Media B.V. 2011</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c446t-1e3e7ca738e84bf03938d612f4c76d5ee6bdf13a6c84239b71cc4a96ec334b1e3</citedby><cites>FETCH-LOGICAL-c446t-1e3e7ca738e84bf03938d612f4c76d5ee6bdf13a6c84239b71cc4a96ec334b1e3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,777,781,27905,27906</link.rule.ids></links><search><creatorcontrib>Gómez de Castro, Ana I.</creatorcontrib><creatorcontrib>Maíz, Jesús</creatorcontrib><creatorcontrib>Rodriguez, Pablo</creatorcontrib><creatorcontrib>Gómez, Maite</creatorcontrib><creatorcontrib>Larruquert, Juan A.</creatorcontrib><creatorcontrib>Méndez, José A.</creatorcontrib><creatorcontrib>Belenguer, Tomas</creatorcontrib><creatorcontrib>Rodrigo-Gudiel, Victor</creatorcontrib><creatorcontrib>López-Martínez, Fátima</creatorcontrib><creatorcontrib>Sestito, Paola</creatorcontrib><title>The imaging and slitless spectroscopy instrument for surveys (ISSIS) for the world space observatory-ultraviolet (WSO-UV)</title><title>Astrophysics and space science</title><addtitle>Astrophys Space Sci</addtitle><description>ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory-Ultraviolet (WSO-UV) mission. ISSIS is a multipurpose instrument designed to carry out high resolution (<0.1 arcsec) imaging in the far UV with fields of view ≥2×2 arcmin
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. ISSIS has two acquisition channels: the High Sensitivity Channel (HSC) and the Channel for Surveys (CfS). The HSC is equipped with an MCP-type detector to guarantee high sensitivity in the 1150–1750 Å range and high rejection of lower energy radiation. The CfS is equipped with a large CCD detector (4k×4k) to obtain images from the far UV to the red (1150–8500 Å); the CfS is implemented to allow observing UV bright sources such as reflection nebulae or nearby massive star forming regions. The design drivers and the current status of the instrument are described in this contribution.</description><subject>Astrobiology</subject><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Channels</subject><subject>Charge coupled devices</subject><subject>Cosmology</subject><subject>Detectors</subject><subject>Imaging</subject><subject>Massive stars</subject><subject>Observations and Techniques</subject><subject>Original Article</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Scientific apparatus & instruments</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Space telescopes</subject><subject>Spectroscopy</subject><subject>Spectrum analysis</subject><subject>Surveys</subject><subject>Ultraviolet astronomy</subject><issn>0004-640X</issn><issn>1572-946X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNp9kUFv1DAQhS0EEkvhB3CzuLA9GOzYcewjqgpdqVIP20JvluOdLKmycfA4i_LvcbtISEhwGs3oe0-a9wh5K_gHwXnzEQWvuWVcCMa1rZl9Rlaibipmlb5_Tlacc8W04vcvySvEh7JabZsVWW6_A-0Pft-Pe-rHHcWhzwMgUpwg5BQxxGmh_Yg5zQcYM-1iojinIyxI15vtdrM9f7rlYvQzpqFYTD4AjS1COvoc08LmISd_7OMAma6_bW_Y3dfz1-RF5weEN7_nGbn7fHl7ccWub75sLj5ds6CUzkyAhCb4Rhowqu24tNLstKg6FRq9qwF0u-uE9DoYVUnbNiIE5a2GIKVqi_qMvD_5Tin-mAGzO_QYYBj8CHFGZ6wV0tZcFnL9X1LoRlRSmUoX9N1f6EOc01j-cMYIKWtreIHECQolRkzQuSmVqNPiBHePrblTa6605h5bc7ZoqpMGCzvuIf0x_rfoF7exmw4</recordid><startdate>20110901</startdate><enddate>20110901</enddate><creator>Gómez de Castro, Ana I.</creator><creator>Maíz, Jesús</creator><creator>Rodriguez, Pablo</creator><creator>Gómez, Maite</creator><creator>Larruquert, Juan A.</creator><creator>Méndez, José A.</creator><creator>Belenguer, Tomas</creator><creator>Rodrigo-Gudiel, Victor</creator><creator>López-Martínez, Fátima</creator><creator>Sestito, Paola</creator><general>Springer Netherlands</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20110901</creationdate><title>The imaging and slitless spectroscopy instrument for surveys (ISSIS) for the world space observatory-ultraviolet (WSO-UV)</title><author>Gómez de Castro, Ana I. ; Maíz, Jesús ; Rodriguez, Pablo ; Gómez, Maite ; Larruquert, Juan A. ; Méndez, José A. ; Belenguer, Tomas ; Rodrigo-Gudiel, Victor ; López-Martínez, Fátima ; Sestito, Paola</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c446t-1e3e7ca738e84bf03938d612f4c76d5ee6bdf13a6c84239b71cc4a96ec334b1e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Astrobiology</topic><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Astrophysics and Astroparticles</topic><topic>Channels</topic><topic>Charge coupled devices</topic><topic>Cosmology</topic><topic>Detectors</topic><topic>Imaging</topic><topic>Massive stars</topic><topic>Observations and Techniques</topic><topic>Original Article</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Scientific apparatus & instruments</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Space telescopes</topic><topic>Spectroscopy</topic><topic>Spectrum analysis</topic><topic>Surveys</topic><topic>Ultraviolet astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gómez de Castro, Ana I.</creatorcontrib><creatorcontrib>Maíz, Jesús</creatorcontrib><creatorcontrib>Rodriguez, Pablo</creatorcontrib><creatorcontrib>Gómez, Maite</creatorcontrib><creatorcontrib>Larruquert, Juan A.</creatorcontrib><creatorcontrib>Méndez, José A.</creatorcontrib><creatorcontrib>Belenguer, Tomas</creatorcontrib><creatorcontrib>Rodrigo-Gudiel, Victor</creatorcontrib><creatorcontrib>López-Martínez, Fátima</creatorcontrib><creatorcontrib>Sestito, Paola</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Astrophysics and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gómez de Castro, Ana I.</au><au>Maíz, Jesús</au><au>Rodriguez, Pablo</au><au>Gómez, Maite</au><au>Larruquert, Juan A.</au><au>Méndez, José A.</au><au>Belenguer, Tomas</au><au>Rodrigo-Gudiel, Victor</au><au>López-Martínez, Fátima</au><au>Sestito, Paola</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The imaging and slitless spectroscopy instrument for surveys (ISSIS) for the world space observatory-ultraviolet (WSO-UV)</atitle><jtitle>Astrophysics and space science</jtitle><stitle>Astrophys Space Sci</stitle><date>2011-09-01</date><risdate>2011</risdate><volume>335</volume><issue>1</issue><spage>283</spage><epage>289</epage><pages>283-289</pages><issn>0004-640X</issn><eissn>1572-946X</eissn><abstract>ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory-Ultraviolet (WSO-UV) mission. ISSIS is a multipurpose instrument designed to carry out high resolution (<0.1 arcsec) imaging in the far UV with fields of view ≥2×2 arcmin
2
. ISSIS has two acquisition channels: the High Sensitivity Channel (HSC) and the Channel for Surveys (CfS). The HSC is equipped with an MCP-type detector to guarantee high sensitivity in the 1150–1750 Å range and high rejection of lower energy radiation. The CfS is equipped with a large CCD detector (4k×4k) to obtain images from the far UV to the red (1150–8500 Å); the CfS is implemented to allow observing UV bright sources such as reflection nebulae or nearby massive star forming regions. The design drivers and the current status of the instrument are described in this contribution.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s10509-011-0695-9</doi><tpages>7</tpages></addata></record> |
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| ispartof | Astrophysics and space science, 2011-09, Vol.335 (1), p.283-289 |
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| source | Springer Nature |
| subjects | Astrobiology Astronomy Astrophysics Astrophysics and Astroparticles Channels Charge coupled devices Cosmology Detectors Imaging Massive stars Observations and Techniques Original Article Physics Physics and Astronomy Scientific apparatus & instruments Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Space telescopes Spectroscopy Spectrum analysis Surveys Ultraviolet astronomy |
| title | The imaging and slitless spectroscopy instrument for surveys (ISSIS) for the world space observatory-ultraviolet (WSO-UV) |
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