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INTEGRAL reloaded: spacecraft, instruments and ground system
ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up to about 47 hr, or 170 ksec, per satellite orbit of 2.7 days) with a large field-of-view (fully coded: 100 deg^2), m...
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creator | Kuulkers, Erik Ferrigno, Carlo Kretschmar, Peter Alfonso-Garzon, Julia Baab, Marius Bazzano, Angela Belanger, Guillaume Benson, Ian Bird, Anthony J Bozzo, Enrico Brandt, Soren Coe, Elliott Caballero, Isabel Cangemi, Floriane Chenevez, Jerome Cenko, Bradley Cinar, Nebil Coleiro, Alexis De Padova, Stefano Diehl, Roland Dietze, Claudia Domingo, Albert Drapes, Mark D'uva, Eleonora Ehle, Matthias Ebrero, Jacobo Edirimanne, Mithrajith Eismont, Natan A Finn, Timothy Fiocchi, Mariateresa Elena Garcia Tomas Gaudenzi, Gianluca Godard, Thomas Goldwurm, Andrea Gotz, Diego Gouiffes, Christian Grebenev, Sergei A Greiner, Jochen Gros, Aleksandra Hanlon, Lorraine Hermsen, Wim Hernandez, Cristina Hernanz, Margarita Huebner, Jutta Jourdain, Elisabeth Giovanni La Rosa Labanti, Claudio Laurent, Philippe Lehanka, Alexander Lund, Niels Madison, James Malzac, Julien Martin, Jim J Miguel Mas-Hesse McBreen, Brian McDonald, Alastair McEnery, Julie Mereghetti, Sandro Natalucci, Lorenzo Ness, Jan-Uwe Oxborrow, Carol Anne Palmer, John Peschke, Sibylle Petrucciani, Francesco Pfeil, Norbert Reichenbaecher, Michael Rodi, James Rodriguez, Jerome Roques, Jean-Pierre Emilio Salazar Donate Salt, Dave Sanchez-Fernandez, Celia Sauvageon, Aymeric Savchenko, Volodymyr Sergey Yu Sazonov Scaglioni, Stefano Schartel, Norbert Siegert, Thomas Southworth, Richard Sunyaev, Rashid A Toma, Liviu Ubertini, Pietro Ed P J van den Heuvel Andreas von Kienlin Nikolai von Krusenstiern Winkler, Christoph Hajdas Wojciech Zannoni, Ugo |
description | ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up to about 47 hr, or 170 ksec, per satellite orbit of 2.7 days) with a large field-of-view (fully coded: 100 deg^2), msec time resolution, keV energy resolution, polarization measurements, as well as additional coverage in the optical. This is realized by two main instruments in the 15 keV to 10 MeV range, the spectrometer SPI (spectral resolution 3 keV at 1.8 MeV) and the imager IBIS (angular resolution 12 arcmin FWHM), complemented by X-ray (JEM-X; 3-35 keV) and optical (OMC; Johnson V-band) monitors. All instruments are co-aligned to simultaneously observe the target region. A particle radiation monitor (IREM) measures charged particle fluxes near the spacecraft. The Anti-coincidence subsystems of the main instruments are also efficient all-sky gamma-ray detectors, which provide omni-directional monitoring above ~75 keV. INTEGRAL can also rapidly (within a couple of hours) re-point and conduct Target of Opportunity observations. INTEGRAL has build an impressive legacy: e.g. discovery of >600 new high-energy sources; first-ever direct detection of 56Ni and 56Co radio-active decay lines from a Type Ia supernova; new insights on positron annihilation in the Galactic bulge and disk; pioneering gamma-ray polarization studies. INTEGRAL is also a successful in multi-messenger astronomy: INTEGRAL found the first prompt electromagnetic radiation in coincidence with a binary neutron star merger. More than 1750 papers based on INTEGRAL data have been published in refereed journals. Here we give a comprehensive update of the satellite status after more than 18 years of operations in a harsh space environment, and an account of the successful Ground Segment. |
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Since then, it has been providing long, uninterrupted observations (up to about 47 hr, or 170 ksec, per satellite orbit of 2.7 days) with a large field-of-view (fully coded: 100 deg^2), msec time resolution, keV energy resolution, polarization measurements, as well as additional coverage in the optical. This is realized by two main instruments in the 15 keV to 10 MeV range, the spectrometer SPI (spectral resolution 3 keV at 1.8 MeV) and the imager IBIS (angular resolution 12 arcmin FWHM), complemented by X-ray (JEM-X; 3-35 keV) and optical (OMC; Johnson V-band) monitors. All instruments are co-aligned to simultaneously observe the target region. A particle radiation monitor (IREM) measures charged particle fluxes near the spacecraft. The Anti-coincidence subsystems of the main instruments are also efficient all-sky gamma-ray detectors, which provide omni-directional monitoring above ~75 keV. INTEGRAL can also rapidly (within a couple of hours) re-point and conduct Target of Opportunity observations. INTEGRAL has build an impressive legacy: e.g. discovery of >600 new high-energy sources; first-ever direct detection of 56Ni and 56Co radio-active decay lines from a Type Ia supernova; new insights on positron annihilation in the Galactic bulge and disk; pioneering gamma-ray polarization studies. INTEGRAL is also a successful in multi-messenger astronomy: INTEGRAL found the first prompt electromagnetic radiation in coincidence with a binary neutron star merger. More than 1750 papers based on INTEGRAL data have been published in refereed journals. 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Donate</creatorcontrib><creatorcontrib>Salt, Dave</creatorcontrib><creatorcontrib>Sanchez-Fernandez, Celia</creatorcontrib><creatorcontrib>Sauvageon, Aymeric</creatorcontrib><creatorcontrib>Savchenko, Volodymyr</creatorcontrib><creatorcontrib>Sergey Yu Sazonov</creatorcontrib><creatorcontrib>Scaglioni, Stefano</creatorcontrib><creatorcontrib>Schartel, Norbert</creatorcontrib><creatorcontrib>Siegert, Thomas</creatorcontrib><creatorcontrib>Southworth, Richard</creatorcontrib><creatorcontrib>Sunyaev, Rashid A</creatorcontrib><creatorcontrib>Toma, Liviu</creatorcontrib><creatorcontrib>Ubertini, Pietro</creatorcontrib><creatorcontrib>Ed P J van den Heuvel</creatorcontrib><creatorcontrib>Andreas von Kienlin</creatorcontrib><creatorcontrib>Nikolai von Krusenstiern</creatorcontrib><creatorcontrib>Winkler, Christoph</creatorcontrib><creatorcontrib>Hajdas Wojciech</creatorcontrib><creatorcontrib>Zannoni, Ugo</creatorcontrib><title>INTEGRAL reloaded: spacecraft, instruments and ground system</title><title>arXiv.org</title><description>ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up to about 47 hr, or 170 ksec, per satellite orbit of 2.7 days) with a large field-of-view (fully coded: 100 deg^2), msec time resolution, keV energy resolution, polarization measurements, as well as additional coverage in the optical. This is realized by two main instruments in the 15 keV to 10 MeV range, the spectrometer SPI (spectral resolution 3 keV at 1.8 MeV) and the imager IBIS (angular resolution 12 arcmin FWHM), complemented by X-ray (JEM-X; 3-35 keV) and optical (OMC; Johnson V-band) monitors. All instruments are co-aligned to simultaneously observe the target region. A particle radiation monitor (IREM) measures charged particle fluxes near the spacecraft. The Anti-coincidence subsystems of the main instruments are also efficient all-sky gamma-ray detectors, which provide omni-directional monitoring above ~75 keV. INTEGRAL can also rapidly (within a couple of hours) re-point and conduct Target of Opportunity observations. INTEGRAL has build an impressive legacy: e.g. discovery of >600 new high-energy sources; first-ever direct detection of 56Ni and 56Co radio-active decay lines from a Type Ia supernova; new insights on positron annihilation in the Galactic bulge and disk; pioneering gamma-ray polarization studies. INTEGRAL is also a successful in multi-messenger astronomy: INTEGRAL found the first prompt electromagnetic radiation in coincidence with a binary neutron star merger. More than 1750 papers based on INTEGRAL data have been published in refereed journals. Here we give a comprehensive update of the satellite status after more than 18 years of operations in a harsh space environment, and an account of the successful Ground Segment.</description><subject>Aerospace environments</subject><subject>Angular resolution</subject><subject>Astrophysics</subject><subject>Binary stars</subject><subject>Charged particles</subject><subject>Electromagnetic radiation</subject><subject>Energy resolution</subject><subject>Field of view</subject><subject>Fluxes</subject><subject>Galactic bulge</subject><subject>Gamma ray detectors</subject><subject>Gamma rays</subject><subject>High energy astronomy</subject><subject>Integrals</subject><subject>Neutron stars</subject><subject>Polarization</subject><subject>Positron annihilation</subject><subject>Radiation</subject><subject>Radio sources (astronomy)</subject><subject>Satellite orbits</subject><subject>Spacecraft</subject><subject>Spectral resolution</subject><subject>Subsystems</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNpjYuA0MjY21LUwMTLiYOAtLs4yMDAwMjM3MjU15mSw8fQLcXUPcvRRKErNyU9MSU2xUiguSExOTS5KTCvRUcjMKy4pKs1NzSspVkjMS1FIL8ovBVLFlcUlqbk8DKxpiTnFqbxQmptB2c01xNlDt6Aov7A0tbgkPiu_tCgPKBVvZGpiYm5gYGlgbkycKgDpazcY</recordid><startdate>20210623</startdate><enddate>20210623</enddate><creator>Kuulkers, Erik</creator><creator>Ferrigno, Carlo</creator><creator>Kretschmar, Peter</creator><creator>Alfonso-Garzon, Julia</creator><creator>Baab, Marius</creator><creator>Bazzano, Angela</creator><creator>Belanger, Guillaume</creator><creator>Benson, Ian</creator><creator>Bird, Anthony J</creator><creator>Bozzo, Enrico</creator><creator>Brandt, Soren</creator><creator>Coe, Elliott</creator><creator>Caballero, Isabel</creator><creator>Cangemi, Floriane</creator><creator>Chenevez, 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20210623</creationdate><title>INTEGRAL reloaded: spacecraft, instruments and ground system</title><author>Kuulkers, Erik ; Ferrigno, Carlo ; Kretschmar, Peter ; Alfonso-Garzon, Julia ; Baab, Marius ; Bazzano, Angela ; Belanger, Guillaume ; Benson, Ian ; Bird, Anthony J ; Bozzo, Enrico ; Brandt, Soren ; Coe, Elliott ; Caballero, Isabel ; Cangemi, Floriane ; Chenevez, Jerome ; Cenko, Bradley ; Cinar, Nebil ; Coleiro, Alexis ; De Padova, Stefano ; Diehl, Roland ; Dietze, Claudia ; Domingo, Albert ; Drapes, Mark ; D'uva, Eleonora ; Ehle, Matthias ; Ebrero, Jacobo ; Edirimanne, Mithrajith ; Eismont, Natan A ; Finn, Timothy ; Fiocchi, Mariateresa ; Elena Garcia Tomas ; Gaudenzi, Gianluca ; Godard, Thomas ; Goldwurm, Andrea ; Gotz, Diego ; Gouiffes, Christian ; Grebenev, Sergei A ; Greiner, Jochen ; Gros, Aleksandra ; Hanlon, Lorraine ; Hermsen, Wim ; Hernandez, Cristina ; Hernanz, Margarita ; Huebner, Jutta ; Jourdain, Elisabeth ; Giovanni La Rosa ; Labanti, Claudio ; Laurent, Philippe ; Lehanka, Alexander ; Lund, Niels ; Madison, James ; Malzac, Julien ; Martin, Jim ; J Miguel Mas-Hesse ; McBreen, Brian ; McDonald, Alastair ; McEnery, Julie ; Mereghetti, Sandro ; Natalucci, Lorenzo ; Ness, Jan-Uwe ; Oxborrow, Carol Anne ; Palmer, John ; Peschke, Sibylle ; Petrucciani, Francesco ; Pfeil, Norbert ; Reichenbaecher, Michael ; Rodi, James ; Rodriguez, Jerome ; Roques, Jean-Pierre ; Emilio Salazar Donate ; Salt, Dave ; Sanchez-Fernandez, Celia ; Sauvageon, Aymeric ; Savchenko, Volodymyr ; Sergey Yu Sazonov ; Scaglioni, Stefano ; Schartel, Norbert ; Siegert, Thomas ; Southworth, Richard ; Sunyaev, Rashid A ; Toma, Liviu ; Ubertini, Pietro ; Ed P J van den Heuvel ; Andreas von Kienlin ; Nikolai von Krusenstiern ; Winkler, Christoph ; Hajdas Wojciech ; Zannoni, Ugo</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_25447009073</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Aerospace environments</topic><topic>Angular resolution</topic><topic>Astrophysics</topic><topic>Binary stars</topic><topic>Charged particles</topic><topic>Electromagnetic radiation</topic><topic>Energy resolution</topic><topic>Field of view</topic><topic>Fluxes</topic><topic>Galactic bulge</topic><topic>Gamma ray detectors</topic><topic>Gamma rays</topic><topic>High energy astronomy</topic><topic>Integrals</topic><topic>Neutron stars</topic><topic>Polarization</topic><topic>Positron annihilation</topic><topic>Radiation</topic><topic>Radio sources (astronomy)</topic><topic>Satellite orbits</topic><topic>Spacecraft</topic><topic>Spectral resolution</topic><topic>Subsystems</topic><toplevel>online_resources</toplevel><creatorcontrib>Kuulkers, Erik</creatorcontrib><creatorcontrib>Ferrigno, Carlo</creatorcontrib><creatorcontrib>Kretschmar, Peter</creatorcontrib><creatorcontrib>Alfonso-Garzon, Julia</creatorcontrib><creatorcontrib>Baab, Marius</creatorcontrib><creatorcontrib>Bazzano, Angela</creatorcontrib><creatorcontrib>Belanger, Guillaume</creatorcontrib><creatorcontrib>Benson, Ian</creatorcontrib><creatorcontrib>Bird, Anthony J</creatorcontrib><creatorcontrib>Bozzo, Enrico</creatorcontrib><creatorcontrib>Brandt, Soren</creatorcontrib><creatorcontrib>Coe, Elliott</creatorcontrib><creatorcontrib>Caballero, Isabel</creatorcontrib><creatorcontrib>Cangemi, Floriane</creatorcontrib><creatorcontrib>Chenevez, Jerome</creatorcontrib><creatorcontrib>Cenko, Bradley</creatorcontrib><creatorcontrib>Cinar, Nebil</creatorcontrib><creatorcontrib>Coleiro, Alexis</creatorcontrib><creatorcontrib>De Padova, Stefano</creatorcontrib><creatorcontrib>Diehl, Roland</creatorcontrib><creatorcontrib>Dietze, Claudia</creatorcontrib><creatorcontrib>Domingo, Albert</creatorcontrib><creatorcontrib>Drapes, Mark</creatorcontrib><creatorcontrib>D'uva, Eleonora</creatorcontrib><creatorcontrib>Ehle, Matthias</creatorcontrib><creatorcontrib>Ebrero, Jacobo</creatorcontrib><creatorcontrib>Edirimanne, Mithrajith</creatorcontrib><creatorcontrib>Eismont, Natan A</creatorcontrib><creatorcontrib>Finn, Timothy</creatorcontrib><creatorcontrib>Fiocchi, Mariateresa</creatorcontrib><creatorcontrib>Elena Garcia Tomas</creatorcontrib><creatorcontrib>Gaudenzi, Gianluca</creatorcontrib><creatorcontrib>Godard, Thomas</creatorcontrib><creatorcontrib>Goldwurm, Andrea</creatorcontrib><creatorcontrib>Gotz, Diego</creatorcontrib><creatorcontrib>Gouiffes, Christian</creatorcontrib><creatorcontrib>Grebenev, Sergei A</creatorcontrib><creatorcontrib>Greiner, Jochen</creatorcontrib><creatorcontrib>Gros, Aleksandra</creatorcontrib><creatorcontrib>Hanlon, Lorraine</creatorcontrib><creatorcontrib>Hermsen, Wim</creatorcontrib><creatorcontrib>Hernandez, Cristina</creatorcontrib><creatorcontrib>Hernanz, Margarita</creatorcontrib><creatorcontrib>Huebner, Jutta</creatorcontrib><creatorcontrib>Jourdain, Elisabeth</creatorcontrib><creatorcontrib>Giovanni La Rosa</creatorcontrib><creatorcontrib>Labanti, Claudio</creatorcontrib><creatorcontrib>Laurent, Philippe</creatorcontrib><creatorcontrib>Lehanka, Alexander</creatorcontrib><creatorcontrib>Lund, Niels</creatorcontrib><creatorcontrib>Madison, James</creatorcontrib><creatorcontrib>Malzac, Julien</creatorcontrib><creatorcontrib>Martin, Jim</creatorcontrib><creatorcontrib>J Miguel Mas-Hesse</creatorcontrib><creatorcontrib>McBreen, Brian</creatorcontrib><creatorcontrib>McDonald, Alastair</creatorcontrib><creatorcontrib>McEnery, Julie</creatorcontrib><creatorcontrib>Mereghetti, Sandro</creatorcontrib><creatorcontrib>Natalucci, Lorenzo</creatorcontrib><creatorcontrib>Ness, Jan-Uwe</creatorcontrib><creatorcontrib>Oxborrow, Carol Anne</creatorcontrib><creatorcontrib>Palmer, John</creatorcontrib><creatorcontrib>Peschke, Sibylle</creatorcontrib><creatorcontrib>Petrucciani, Francesco</creatorcontrib><creatorcontrib>Pfeil, Norbert</creatorcontrib><creatorcontrib>Reichenbaecher, Michael</creatorcontrib><creatorcontrib>Rodi, James</creatorcontrib><creatorcontrib>Rodriguez, Jerome</creatorcontrib><creatorcontrib>Roques, Jean-Pierre</creatorcontrib><creatorcontrib>Emilio Salazar Donate</creatorcontrib><creatorcontrib>Salt, Dave</creatorcontrib><creatorcontrib>Sanchez-Fernandez, Celia</creatorcontrib><creatorcontrib>Sauvageon, Aymeric</creatorcontrib><creatorcontrib>Savchenko, Volodymyr</creatorcontrib><creatorcontrib>Sergey Yu Sazonov</creatorcontrib><creatorcontrib>Scaglioni, Stefano</creatorcontrib><creatorcontrib>Schartel, Norbert</creatorcontrib><creatorcontrib>Siegert, Thomas</creatorcontrib><creatorcontrib>Southworth, Richard</creatorcontrib><creatorcontrib>Sunyaev, Rashid A</creatorcontrib><creatorcontrib>Toma, Liviu</creatorcontrib><creatorcontrib>Ubertini, Pietro</creatorcontrib><creatorcontrib>Ed P J van den Heuvel</creatorcontrib><creatorcontrib>Andreas von Kienlin</creatorcontrib><creatorcontrib>Nikolai von Krusenstiern</creatorcontrib><creatorcontrib>Winkler, Christoph</creatorcontrib><creatorcontrib>Hajdas Wojciech</creatorcontrib><creatorcontrib>Zannoni, Ugo</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</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>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</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 China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kuulkers, Erik</au><au>Ferrigno, Carlo</au><au>Kretschmar, Peter</au><au>Alfonso-Garzon, Julia</au><au>Baab, Marius</au><au>Bazzano, Angela</au><au>Belanger, Guillaume</au><au>Benson, Ian</au><au>Bird, Anthony J</au><au>Bozzo, Enrico</au><au>Brandt, Soren</au><au>Coe, Elliott</au><au>Caballero, Isabel</au><au>Cangemi, Floriane</au><au>Chenevez, Jerome</au><au>Cenko, Bradley</au><au>Cinar, Nebil</au><au>Coleiro, Alexis</au><au>De Padova, Stefano</au><au>Diehl, Roland</au><au>Dietze, Claudia</au><au>Domingo, Albert</au><au>Drapes, Mark</au><au>D'uva, Eleonora</au><au>Ehle, Matthias</au><au>Ebrero, Jacobo</au><au>Edirimanne, Mithrajith</au><au>Eismont, Natan A</au><au>Finn, Timothy</au><au>Fiocchi, Mariateresa</au><au>Elena Garcia Tomas</au><au>Gaudenzi, Gianluca</au><au>Godard, Thomas</au><au>Goldwurm, Andrea</au><au>Gotz, Diego</au><au>Gouiffes, Christian</au><au>Grebenev, Sergei A</au><au>Greiner, Jochen</au><au>Gros, Aleksandra</au><au>Hanlon, Lorraine</au><au>Hermsen, Wim</au><au>Hernandez, Cristina</au><au>Hernanz, Margarita</au><au>Huebner, Jutta</au><au>Jourdain, Elisabeth</au><au>Giovanni La Rosa</au><au>Labanti, Claudio</au><au>Laurent, Philippe</au><au>Lehanka, Alexander</au><au>Lund, Niels</au><au>Madison, James</au><au>Malzac, Julien</au><au>Martin, Jim</au><au>J Miguel Mas-Hesse</au><au>McBreen, Brian</au><au>McDonald, Alastair</au><au>McEnery, Julie</au><au>Mereghetti, Sandro</au><au>Natalucci, Lorenzo</au><au>Ness, Jan-Uwe</au><au>Oxborrow, Carol Anne</au><au>Palmer, John</au><au>Peschke, Sibylle</au><au>Petrucciani, Francesco</au><au>Pfeil, Norbert</au><au>Reichenbaecher, Michael</au><au>Rodi, James</au><au>Rodriguez, Jerome</au><au>Roques, Jean-Pierre</au><au>Emilio Salazar Donate</au><au>Salt, Dave</au><au>Sanchez-Fernandez, Celia</au><au>Sauvageon, Aymeric</au><au>Savchenko, Volodymyr</au><au>Sergey Yu Sazonov</au><au>Scaglioni, Stefano</au><au>Schartel, Norbert</au><au>Siegert, Thomas</au><au>Southworth, Richard</au><au>Sunyaev, Rashid A</au><au>Toma, Liviu</au><au>Ubertini, Pietro</au><au>Ed P J van den Heuvel</au><au>Andreas von Kienlin</au><au>Nikolai von Krusenstiern</au><au>Winkler, Christoph</au><au>Hajdas Wojciech</au><au>Zannoni, Ugo</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>INTEGRAL reloaded: spacecraft, instruments and ground system</atitle><jtitle>arXiv.org</jtitle><date>2021-06-23</date><risdate>2021</risdate><eissn>2331-8422</eissn><abstract>ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up to about 47 hr, or 170 ksec, per satellite orbit of 2.7 days) with a large field-of-view (fully coded: 100 deg^2), msec time resolution, keV energy resolution, polarization measurements, as well as additional coverage in the optical. This is realized by two main instruments in the 15 keV to 10 MeV range, the spectrometer SPI (spectral resolution 3 keV at 1.8 MeV) and the imager IBIS (angular resolution 12 arcmin FWHM), complemented by X-ray (JEM-X; 3-35 keV) and optical (OMC; Johnson V-band) monitors. All instruments are co-aligned to simultaneously observe the target region. A particle radiation monitor (IREM) measures charged particle fluxes near the spacecraft. The Anti-coincidence subsystems of the main instruments are also efficient all-sky gamma-ray detectors, which provide omni-directional monitoring above ~75 keV. INTEGRAL can also rapidly (within a couple of hours) re-point and conduct Target of Opportunity observations. INTEGRAL has build an impressive legacy: e.g. discovery of >600 new high-energy sources; first-ever direct detection of 56Ni and 56Co radio-active decay lines from a Type Ia supernova; new insights on positron annihilation in the Galactic bulge and disk; pioneering gamma-ray polarization studies. INTEGRAL is also a successful in multi-messenger astronomy: INTEGRAL found the first prompt electromagnetic radiation in coincidence with a binary neutron star merger. More than 1750 papers based on INTEGRAL data have been published in refereed journals. Here we give a comprehensive update of the satellite status after more than 18 years of operations in a harsh space environment, and an account of the successful Ground Segment.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2021-06 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2544700907 |
source | Publicly Available Content Database |
subjects | Aerospace environments Angular resolution Astrophysics Binary stars Charged particles Electromagnetic radiation Energy resolution Field of view Fluxes Galactic bulge Gamma ray detectors Gamma rays High energy astronomy Integrals Neutron stars Polarization Positron annihilation Radiation Radio sources (astronomy) Satellite orbits Spacecraft Spectral resolution Subsystems |
title | INTEGRAL reloaded: spacecraft, instruments and ground system |
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