The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable '...
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| creator | Trager, Scott C Aguerri, J Alfonso L Falcón-Barroso, Jesús Hill, Vanessa Iovino, Angela Aragón-Salamanca, Alfonso Babusiaux, Carine Balcells, Marc Barrena, R Belokurov, Vasily Bensby, Thomas Bonifacio, Piercarlo Cornwell, Daniel J Hatch, Nina A Hess, Kelley M Hoskin, Matthew J Knapen, Johan H Lewis, Jim Lucatello, Sara Molaeinezhad, Alireza Morrison, Sean Murphy, David N A Pérez-Ràfols, Ignasi Picó, Sergio Romero-Gómez, Mercè Royer, Frédéric Seabroke, George M Worley, C Clare Amos, Nicholas J Bellazzini, Michele Bernard, Edouard J Bettoni, Daniela Blomqvist, Michael Boeche, Corrado Bosma, Albert Britavskiy, Nikolay Cantat-Gaudin, Tristan Castro-Ginard, Alfred Couto, Guilherme Conrado, Ana M Domínguez-Gómez, Jesús Drake, Alyssa Feltzing, Sofia Ferré-Mateu, Anna Figueras, Francesca Franciosin, Elena Frasca, Antonio Nicola Gentile Fusillo Gledhill, T M González Delgado, Rosa M Guarcello, Mario Giuseppe Gullieuszik, Marco Haines, Christopher P Hardcastle, Martin J Haywood, Misha Helmi, Amina Hernandez, Nauzet Herrero, Artemio Hughes, Sarah Jarvis, Matt J Jordi, Carme Kondapally, Rohit Kordopatis, Georges Lam, Man I Lemasle, Bertrand Lewis, Ian J Lind, Karin Magrin, Laura Marchal, Olivier Martin, Nicolas F Maurogordato, Sophie Merluzzi, Paola Monari, Giacomo Morelli, Lorenzo Negueruela, Ignacio Peirani, Sébastien Peletier, Reynier F Rainer, Monica Röttgering, Huub J A Jose Sabater Montes José San Juan Schiavon, Ricardo P Schultheis, Mathias Serra, Paolo Shimwell, Timothy W Smith, Russell J Sorini, Daniele Steele, Iain A Tsantaki, Maria Mathieu Van der Swaelmen Vergani, Daniela Verro, Kristiina Vioque, Miguel Wegg, Christopher Weijmans, Anne-Marie Williams, Wendy L Wilson, Andrew J Wright, Nicholas J Xylakis-Dornbusch, Theodora Zurita, Cristina |
| description | WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366\(-\)959\,nm at \(R\sim5000\), or two shorter ranges at \(R\sim20\,000\). After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for \(\sim\)3 million stars and detailed abundances for \(\sim1.5\) million brighter field and open-cluster stars; (ii) survey \(\sim0.4\) million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey \(\sim400\) neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in \(z1\) million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at \(z>2\). Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator. |
| doi_str_mv | 10.48550/arxiv.2212.03981 |
| format | Article |
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Aguerri, J Alfonso L ; Falcón-Barroso, Jesús ; Hill, Vanessa ; Iovino, Angela ; Aragón-Salamanca, Alfonso ; Babusiaux, Carine ; Balcells, Marc ; Barrena, R ; Belokurov, Vasily ; Bensby, Thomas ; Bonifacio, Piercarlo ; Cornwell, Daniel J ; Hatch, Nina A ; Hess, Kelley M ; Hoskin, Matthew J ; Knapen, Johan H ; Lewis, Jim ; Lucatello, Sara ; Molaeinezhad, Alireza ; Morrison, Sean ; Murphy, David N A ; Pérez-Ràfols, Ignasi ; Picó, Sergio ; Romero-Gómez, Mercè ; Royer, Frédéric ; Seabroke, George M ; Worley, C Clare ; Amos, Nicholas J ; Bellazzini, Michele ; Bernard, Edouard J ; Bettoni, Daniela ; Blomqvist, Michael ; Boeche, Corrado ; Bosma, Albert ; Britavskiy, Nikolay ; Cantat-Gaudin, Tristan ; Castro-Ginard, Alfred ; Couto, Guilherme ; Conrado, Ana M ; Domínguez-Gómez, Jesús ; Drake, Alyssa ; Feltzing, Sofia ; Ferré-Mateu, Anna ; Figueras, Francesca ; Franciosin, Elena ; Frasca, Antonio ; Nicola Gentile Fusillo ; Gledhill, T M ; González Delgado, Rosa M ; Guarcello, Mario Giuseppe ; Gullieuszik, Marco ; Haines, Christopher P ; Hardcastle, Martin J ; Haywood, Misha ; Helmi, Amina ; Hernandez, Nauzet ; Herrero, Artemio ; Hughes, Sarah ; Jarvis, Matt J ; Jordi, Carme ; Kondapally, Rohit ; Kordopatis, Georges ; Lam, Man I ; Lemasle, Bertrand ; Lewis, Ian J ; Lind, Karin ; Magrin, Laura ; Marchal, Olivier ; Martin, Nicolas F ; Maurogordato, Sophie ; Merluzzi, Paola ; Monari, Giacomo ; Morelli, Lorenzo ; Negueruela, Ignacio ; Peirani, Sébastien ; Peletier, Reynier F ; Rainer, Monica ; Röttgering, Huub J A ; Jose Sabater Montes ; José San Juan ; Schiavon, Ricardo P ; Schultheis, Mathias ; Serra, Paolo ; Shimwell, Timothy W ; Smith, Russell J ; Sorini, Daniele ; Steele, Iain A ; Tsantaki, Maria ; Mathieu Van der Swaelmen ; Vergani, Daniela ; Verro, Kristiina ; Vioque, Miguel ; Wegg, Christopher ; Weijmans, Anne-Marie ; Williams, Wendy L ; Wilson, Andrew J ; Wright, Nicholas J ; Xylakis-Dornbusch, Theodora ; Zurita, Cristina</creator><creatorcontrib>Trager, Scott C ; Aguerri, J Alfonso L ; Falcón-Barroso, Jesús ; Hill, Vanessa ; Iovino, Angela ; Aragón-Salamanca, Alfonso ; Babusiaux, Carine ; Balcells, Marc ; Barrena, R ; Belokurov, Vasily ; Bensby, Thomas ; Bonifacio, Piercarlo ; Cornwell, Daniel J ; Hatch, Nina A ; Hess, Kelley M ; Hoskin, Matthew J ; Knapen, Johan H ; Lewis, Jim ; Lucatello, Sara ; Molaeinezhad, Alireza ; Morrison, Sean ; Murphy, David N A ; Pérez-Ràfols, Ignasi ; Picó, Sergio ; Romero-Gómez, Mercè ; Royer, Frédéric ; Seabroke, George M ; Worley, C Clare ; Amos, Nicholas J ; Bellazzini, Michele ; Bernard, Edouard J ; Bettoni, Daniela ; Blomqvist, Michael ; Boeche, Corrado ; Bosma, Albert ; Britavskiy, Nikolay ; Cantat-Gaudin, Tristan ; Castro-Ginard, Alfred ; Couto, Guilherme ; Conrado, Ana M ; Domínguez-Gómez, Jesús ; Drake, Alyssa ; Feltzing, Sofia ; Ferré-Mateu, Anna ; Figueras, Francesca ; Franciosin, Elena ; Frasca, Antonio ; Nicola Gentile Fusillo ; Gledhill, T M ; González Delgado, Rosa M ; Guarcello, Mario Giuseppe ; Gullieuszik, Marco ; Haines, Christopher P ; Hardcastle, Martin J ; Haywood, Misha ; Helmi, Amina ; Hernandez, Nauzet ; Herrero, Artemio ; Hughes, Sarah ; Jarvis, Matt J ; Jordi, Carme ; Kondapally, Rohit ; Kordopatis, Georges ; Lam, Man I ; Lemasle, Bertrand ; Lewis, Ian J ; Lind, Karin ; Magrin, Laura ; Marchal, Olivier ; Martin, Nicolas F ; Maurogordato, Sophie ; Merluzzi, Paola ; Monari, Giacomo ; Morelli, Lorenzo ; Negueruela, Ignacio ; Peirani, Sébastien ; Peletier, Reynier F ; Rainer, Monica ; Röttgering, Huub J A ; Jose Sabater Montes ; José San Juan ; Schiavon, Ricardo P ; Schultheis, Mathias ; Serra, Paolo ; Shimwell, Timothy W ; Smith, Russell J ; Sorini, Daniele ; Steele, Iain A ; Tsantaki, Maria ; Mathieu Van der Swaelmen ; Vergani, Daniela ; Verro, Kristiina ; Vioque, Miguel ; Wegg, Christopher ; Weijmans, Anne-Marie ; Williams, Wendy L ; Wilson, Andrew J ; Wright, Nicholas J ; Xylakis-Dornbusch, Theodora ; Zurita, Cristina</creatorcontrib><description>WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366\(-\)959\,nm at \(R\sim5000\), or two shorter ranges at \(R\sim20\,000\). After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for \(\sim\)3 million stars and detailed abundances for \(\sim1.5\) million brighter field and open-cluster stars; (ii) survey \(\sim0.4\) million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey \(\sim400\) neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in \(z<0.5\) cluster galaxies; (vi) survey stellar populations and kinematics in \(\sim25\,000\) field galaxies at \(0.3\lesssim z \lesssim 0.7\); (vii) study the cosmic evolution of accretion and star formation using \(>1\) million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at \(z>2\). Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2212.03981</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Data systems ; Deposition ; Galactic clusters ; Kinematics ; LOFAR ; Milky Way ; Multiplexing ; Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics ; Radio astronomy ; Radio sources (astronomy) ; Spectroscopy ; Star & galaxy formation ; Star formation ; Stars & galaxies ; Stellar evolution ; Stellar kinematics ; Stellar populations ; White dwarf stars</subject><ispartof>arXiv.org, 2023-10</ispartof><rights>2023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27925</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.2212.03981$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1093/mnras/stad557$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Trager, Scott C</creatorcontrib><creatorcontrib>Aguerri, J Alfonso L</creatorcontrib><creatorcontrib>Falcón-Barroso, Jesús</creatorcontrib><creatorcontrib>Hill, Vanessa</creatorcontrib><creatorcontrib>Iovino, 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Bertrand</creatorcontrib><creatorcontrib>Lewis, Ian J</creatorcontrib><creatorcontrib>Lind, Karin</creatorcontrib><creatorcontrib>Magrin, Laura</creatorcontrib><creatorcontrib>Marchal, Olivier</creatorcontrib><creatorcontrib>Martin, Nicolas F</creatorcontrib><creatorcontrib>Maurogordato, Sophie</creatorcontrib><creatorcontrib>Merluzzi, Paola</creatorcontrib><creatorcontrib>Monari, Giacomo</creatorcontrib><creatorcontrib>Morelli, Lorenzo</creatorcontrib><creatorcontrib>Negueruela, Ignacio</creatorcontrib><creatorcontrib>Peirani, Sébastien</creatorcontrib><creatorcontrib>Peletier, Reynier F</creatorcontrib><creatorcontrib>Rainer, Monica</creatorcontrib><creatorcontrib>Röttgering, Huub J A</creatorcontrib><creatorcontrib>Jose Sabater Montes</creatorcontrib><creatorcontrib>José San Juan</creatorcontrib><creatorcontrib>Schiavon, Ricardo P</creatorcontrib><creatorcontrib>Schultheis, Mathias</creatorcontrib><creatorcontrib>Serra, Paolo</creatorcontrib><creatorcontrib>Shimwell, Timothy W</creatorcontrib><creatorcontrib>Smith, Russell J</creatorcontrib><creatorcontrib>Sorini, Daniele</creatorcontrib><creatorcontrib>Steele, Iain A</creatorcontrib><creatorcontrib>Tsantaki, Maria</creatorcontrib><creatorcontrib>Mathieu Van der Swaelmen</creatorcontrib><creatorcontrib>Vergani, Daniela</creatorcontrib><creatorcontrib>Verro, Kristiina</creatorcontrib><creatorcontrib>Vioque, Miguel</creatorcontrib><creatorcontrib>Wegg, Christopher</creatorcontrib><creatorcontrib>Weijmans, Anne-Marie</creatorcontrib><creatorcontrib>Williams, Wendy L</creatorcontrib><creatorcontrib>Wilson, Andrew J</creatorcontrib><creatorcontrib>Wright, Nicholas J</creatorcontrib><creatorcontrib>Xylakis-Dornbusch, Theodora</creatorcontrib><creatorcontrib>Zurita, Cristina</creatorcontrib><title>The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation</title><title>arXiv.org</title><description>WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366\(-\)959\,nm at \(R\sim5000\), or two shorter ranges at \(R\sim20\,000\). After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for \(\sim\)3 million stars and detailed abundances for \(\sim1.5\) million brighter field and open-cluster stars; (ii) survey \(\sim0.4\) million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey \(\sim400\) neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in \(z<0.5\) cluster galaxies; (vi) survey stellar populations and kinematics in \(\sim25\,000\) field galaxies at \(0.3\lesssim z \lesssim 0.7\); (vii) study the cosmic evolution of accretion and star formation using \(>1\) million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at \(z>2\). Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.</description><subject>Data systems</subject><subject>Deposition</subject><subject>Galactic clusters</subject><subject>Kinematics</subject><subject>LOFAR</subject><subject>Milky Way</subject><subject>Multiplexing</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><subject>Radio astronomy</subject><subject>Radio sources (astronomy)</subject><subject>Spectroscopy</subject><subject>Star & galaxy formation</subject><subject>Star formation</subject><subject>Stars & galaxies</subject><subject>Stellar evolution</subject><subject>Stellar kinematics</subject><subject>Stellar populations</subject><subject>White dwarf 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Maria</creator><creator>Mathieu Van der Swaelmen</creator><creator>Vergani, Daniela</creator><creator>Verro, Kristiina</creator><creator>Vioque, Miguel</creator><creator>Wegg, Christopher</creator><creator>Weijmans, Anne-Marie</creator><creator>Williams, Wendy L</creator><creator>Wilson, Andrew J</creator><creator>Wright, Nicholas J</creator><creator>Xylakis-Dornbusch, Theodora</creator><creator>Zurita, Cristina</creator><general>Cornell University Library, 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><scope>GOX</scope></search><sort><creationdate>20231031</creationdate><title>The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation</title><author>Trager, Scott C ; Aguerri, J Alfonso L ; Falcón-Barroso, Jesús ; Hill, Vanessa ; Iovino, Angela ; Aragón-Salamanca, Alfonso ; Babusiaux, Carine ; Balcells, Marc ; Barrena, R ; Belokurov, Vasily ; Bensby, Thomas ; Bonifacio, Piercarlo ; Cornwell, Daniel J ; Hatch, Nina A ; Hess, Kelley M ; Hoskin, Matthew J ; Knapen, Johan H ; Lewis, Jim ; Lucatello, Sara ; Molaeinezhad, Alireza ; Morrison, Sean ; Murphy, David N A ; Pérez-Ràfols, Ignasi ; Picó, Sergio ; Romero-Gómez, Mercè ; Royer, Frédéric ; Seabroke, George M ; Worley, C Clare ; Amos, Nicholas J ; Bellazzini, Michele ; Bernard, Edouard J ; Bettoni, Daniela ; Blomqvist, Michael ; Boeche, Corrado ; Bosma, Albert ; Britavskiy, Nikolay ; Cantat-Gaudin, Tristan ; Castro-Ginard, Alfred ; Couto, Guilherme ; Conrado, Ana M ; Domínguez-Gómez, Jesús ; Drake, Alyssa ; Feltzing, Sofia ; Ferré-Mateu, Anna ; Figueras, Francesca ; Franciosin, Elena ; Frasca, Antonio ; Nicola Gentile Fusillo ; Gledhill, T M ; González Delgado, Rosa M ; Guarcello, Mario Giuseppe ; Gullieuszik, Marco ; Haines, Christopher P ; Hardcastle, Martin J ; Haywood, Misha ; Helmi, Amina ; Hernandez, Nauzet ; Herrero, Artemio ; Hughes, Sarah ; Jarvis, Matt J ; Jordi, Carme ; Kondapally, Rohit ; Kordopatis, Georges ; Lam, Man I ; Lemasle, Bertrand ; Lewis, Ian J ; Lind, Karin ; Magrin, Laura ; Marchal, Olivier ; Martin, Nicolas F ; Maurogordato, Sophie ; Merluzzi, Paola ; Monari, Giacomo ; Morelli, Lorenzo ; Negueruela, Ignacio ; Peirani, Sébastien ; Peletier, Reynier F ; Rainer, Monica ; Röttgering, Huub J A ; Jose Sabater Montes ; José San Juan ; Schiavon, Ricardo P ; Schultheis, Mathias ; Serra, Paolo ; Shimwell, Timothy W ; Smith, Russell J ; Sorini, Daniele ; Steele, Iain A ; Tsantaki, Maria ; Mathieu Van der Swaelmen ; Vergani, Daniela ; Verro, Kristiina ; Vioque, Miguel ; Wegg, Christopher ; Weijmans, Anne-Marie ; Williams, Wendy L ; Wilson, Andrew J ; Wright, Nicholas J ; Xylakis-Dornbusch, Theodora ; Zurita, Cristina</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a951-ab58a38add084f7d2640e20bbb45daff0a1015f842d20c1464d136c9539814673</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Data systems</topic><topic>Deposition</topic><topic>Galactic clusters</topic><topic>Kinematics</topic><topic>LOFAR</topic><topic>Milky Way</topic><topic>Multiplexing</topic><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><topic>Radio astronomy</topic><topic>Radio sources (astronomy)</topic><topic>Spectroscopy</topic><topic>Star & galaxy formation</topic><topic>Star formation</topic><topic>Stars & galaxies</topic><topic>Stellar evolution</topic><topic>Stellar kinematics</topic><topic>Stellar populations</topic><topic>White dwarf stars</topic><toplevel>online_resources</toplevel><creatorcontrib>Trager, Scott C</creatorcontrib><creatorcontrib>Aguerri, J Alfonso L</creatorcontrib><creatorcontrib>Falcón-Barroso, Jesús</creatorcontrib><creatorcontrib>Hill, Vanessa</creatorcontrib><creatorcontrib>Iovino, Angela</creatorcontrib><creatorcontrib>Aragón-Salamanca, Alfonso</creatorcontrib><creatorcontrib>Babusiaux, Carine</creatorcontrib><creatorcontrib>Balcells, Marc</creatorcontrib><creatorcontrib>Barrena, R</creatorcontrib><creatorcontrib>Belokurov, Vasily</creatorcontrib><creatorcontrib>Bensby, Thomas</creatorcontrib><creatorcontrib>Bonifacio, Piercarlo</creatorcontrib><creatorcontrib>Cornwell, Daniel J</creatorcontrib><creatorcontrib>Hatch, Nina A</creatorcontrib><creatorcontrib>Hess, Kelley M</creatorcontrib><creatorcontrib>Hoskin, Matthew J</creatorcontrib><creatorcontrib>Knapen, Johan H</creatorcontrib><creatorcontrib>Lewis, 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J</creatorcontrib><creatorcontrib>Wright, Nicholas J</creatorcontrib><creatorcontrib>Xylakis-Dornbusch, Theodora</creatorcontrib><creatorcontrib>Zurita, Cristina</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</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><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Trager, Scott C</au><au>Aguerri, J Alfonso L</au><au>Falcón-Barroso, Jesús</au><au>Hill, Vanessa</au><au>Iovino, Angela</au><au>Aragón-Salamanca, Alfonso</au><au>Babusiaux, Carine</au><au>Balcells, Marc</au><au>Barrena, R</au><au>Belokurov, Vasily</au><au>Bensby, Thomas</au><au>Bonifacio, Piercarlo</au><au>Cornwell, Daniel J</au><au>Hatch, Nina A</au><au>Hess, Kelley M</au><au>Hoskin, Matthew J</au><au>Knapen, Johan H</au><au>Lewis, Jim</au><au>Lucatello, Sara</au><au>Molaeinezhad, Alireza</au><au>Morrison, Sean</au><au>Murphy, David N A</au><au>Pérez-Ràfols, Ignasi</au><au>Picó, Sergio</au><au>Romero-Gómez, Mercè</au><au>Royer, Frédéric</au><au>Seabroke, George M</au><au>Worley, C Clare</au><au>Amos, Nicholas J</au><au>Bellazzini, Michele</au><au>Bernard, Edouard J</au><au>Bettoni, Daniela</au><au>Blomqvist, Michael</au><au>Boeche, Corrado</au><au>Bosma, Albert</au><au>Britavskiy, Nikolay</au><au>Cantat-Gaudin, Tristan</au><au>Castro-Ginard, Alfred</au><au>Couto, Guilherme</au><au>Conrado, Ana M</au><au>Domínguez-Gómez, Jesús</au><au>Drake, Alyssa</au><au>Feltzing, Sofia</au><au>Ferré-Mateu, Anna</au><au>Figueras, Francesca</au><au>Franciosin, Elena</au><au>Frasca, Antonio</au><au>Nicola Gentile Fusillo</au><au>Gledhill, T M</au><au>González Delgado, Rosa M</au><au>Guarcello, Mario Giuseppe</au><au>Gullieuszik, Marco</au><au>Haines, Christopher P</au><au>Hardcastle, Martin J</au><au>Haywood, Misha</au><au>Helmi, Amina</au><au>Hernandez, Nauzet</au><au>Herrero, Artemio</au><au>Hughes, Sarah</au><au>Jarvis, Matt J</au><au>Jordi, Carme</au><au>Kondapally, Rohit</au><au>Kordopatis, Georges</au><au>Lam, Man I</au><au>Lemasle, Bertrand</au><au>Lewis, Ian J</au><au>Lind, Karin</au><au>Magrin, Laura</au><au>Marchal, Olivier</au><au>Martin, Nicolas F</au><au>Maurogordato, Sophie</au><au>Merluzzi, Paola</au><au>Monari, Giacomo</au><au>Morelli, Lorenzo</au><au>Negueruela, Ignacio</au><au>Peirani, Sébastien</au><au>Peletier, Reynier F</au><au>Rainer, Monica</au><au>Röttgering, Huub J A</au><au>Jose Sabater Montes</au><au>José San Juan</au><au>Schiavon, Ricardo P</au><au>Schultheis, Mathias</au><au>Serra, Paolo</au><au>Shimwell, Timothy W</au><au>Smith, Russell J</au><au>Sorini, Daniele</au><au>Steele, Iain A</au><au>Tsantaki, Maria</au><au>Mathieu Van der Swaelmen</au><au>Vergani, Daniela</au><au>Verro, Kristiina</au><au>Vioque, Miguel</au><au>Wegg, Christopher</au><au>Weijmans, Anne-Marie</au><au>Williams, Wendy L</au><au>Wilson, Andrew J</au><au>Wright, Nicholas J</au><au>Xylakis-Dornbusch, Theodora</au><au>Zurita, Cristina</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation</atitle><jtitle>arXiv.org</jtitle><date>2023-10-31</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366\(-\)959\,nm at \(R\sim5000\), or two shorter ranges at \(R\sim20\,000\). After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for \(\sim\)3 million stars and detailed abundances for \(\sim1.5\) million brighter field and open-cluster stars; (ii) survey \(\sim0.4\) million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey \(\sim400\) neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in \(z<0.5\) cluster galaxies; (vi) survey stellar populations and kinematics in \(\sim25\,000\) field galaxies at \(0.3\lesssim z \lesssim 0.7\); (vii) study the cosmic evolution of accretion and star formation using \(>1\) million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at \(z>2\). Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2212.03981</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2023-10 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_2212_03981 |
| source | arXiv.org; Free E- Journals |
| subjects | Data systems Deposition Galactic clusters Kinematics LOFAR Milky Way Multiplexing Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Radio astronomy Radio sources (astronomy) Spectroscopy Star & galaxy formation Star formation Stars & galaxies Stellar evolution Stellar kinematics Stellar populations White dwarf stars |
| title | The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation |
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