SKA Science Data Challenge 2: analysis and results
The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomers will be correspondingly large and complex, requiring the application of advanced analysis techniques to extract key sc...
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creator | Hartley, P Bonaldi, A Braun, R J N H S Aditya Aicardi, S Alegre, L Chakraborty, A Chen, X Choudhuri, S Clarke, A O Coles, J Collinson, J S Cornu, D Darriba, L M Delli Veneri brich, J Garrido, J Gubanov, F Håkansson, H Hardcastle, M J Heneka, C Herranz, D Hess, K M Jaiswal, S Jurek, R J Korber, D Kitaeff, S Kleiner, D Lao, B X Lu Mazumder, A Moldón, J Mondal, R S Ni Önnheim, M Parra, M Patra, N Peel, A Salomé, P Sánchez-Expósito, S Sargent, M Semelin, B Serra, P Shaw, A K Shen, A X Sjöberg, A Smith, L Soroka, A Stolyarov, V Tolley, E Toribio, M C J M van der Hulst A Vafaei Sadr Verdes-Montenegro, L Westmeier, T K Yu Zhang, L Zhang, X Zhang, Y Alberdi, A Ashdown, M Bom, C R Brüggen, M Cannon, J Chen, R Combes, F Courbin, F Fourestey, G Freundlich, J Gao, L Gheller, C Guo, Q Gustavsson, E Jirstrand, M Jones, M G Kamphuis, P J -P Kneib Lindqvist, M Liu, B Liu, Y Mao, Y Marchal, A Márquez, I Meshcheryakov, A Olberg, M Oozeer, N Pandey-Pommier, M Peng, B Sabater, J Sorgho, A Starck, J L Tasse, C Wang, A Wang, Y H Xi Yang, X Zhang, H Zhang, J Zhao, M Zuo, S |
description | The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomers will be correspondingly large and complex, requiring the application of advanced analysis techniques to extract key science findings. To this end, SKAO is conducting a series of Science Data Challenges, each designed to familiarise the scientific community with SKAO data and to drive the development of new analysis techniques. We present the results from Science Data Challenge 2 (SDC2), which invited participants to find and characterise 233245 neutral hydrogen (Hi) sources in a simulated data product representing a 2000~h SKA MID spectral line observation from redshifts 0.25 to 0.5. Through the generous support of eight international supercomputing facilities, participants were able to undertake the Challenge using dedicated computational resources. Alongside the main challenge, `reproducibility awards' were made in recognition of those pipelines which demonstrated Open Science best practice. The Challenge saw over 100 participants develop a range of new and existing techniques, with results that highlight the strengths of multidisciplinary and collaborative effort. The winning strategy -- which combined predictions from two independent machine learning techniques to yield a 20 percent improvement in overall performance -- underscores one of the main Challenge outcomes: that of method complementarity. It is likely that the combination of methods in a so-called ensemble approach will be key to exploiting very large astronomical datasets. |
doi_str_mv | 10.48550/arxiv.2303.07943 |
format | Article |
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SKAO data products made available to astronomers will be correspondingly large and complex, requiring the application of advanced analysis techniques to extract key science findings. To this end, SKAO is conducting a series of Science Data Challenges, each designed to familiarise the scientific community with SKAO data and to drive the development of new analysis techniques. We present the results from Science Data Challenge 2 (SDC2), which invited participants to find and characterise 233245 neutral hydrogen (Hi) sources in a simulated data product representing a 2000~h SKA MID spectral line observation from redshifts 0.25 to 0.5. Through the generous support of eight international supercomputing facilities, participants were able to undertake the Challenge using dedicated computational resources. Alongside the main challenge, `reproducibility awards' were made in recognition of those pipelines which demonstrated Open Science best practice. The Challenge saw over 100 participants develop a range of new and existing techniques, with results that highlight the strengths of multidisciplinary and collaborative effort. The winning strategy -- which combined predictions from two independent machine learning techniques to yield a 20 percent improvement in overall performance -- underscores one of the main Challenge outcomes: that of method complementarity. It is likely that the combination of methods in a so-called ensemble approach will be key to exploiting very large astronomical datasets.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2303.07943</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Best practice ; Line spectra ; Machine learning ; Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Instrumentation and Methods for Astrophysics ; Science</subject><ispartof>arXiv.org, 2023-03</ispartof><rights>2023. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.1093/mnras/stad1375$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.2303.07943$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Hartley, P</creatorcontrib><creatorcontrib>Bonaldi, A</creatorcontrib><creatorcontrib>Braun, R</creatorcontrib><creatorcontrib>J N H S Aditya</creatorcontrib><creatorcontrib>Aicardi, S</creatorcontrib><creatorcontrib>Alegre, 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G</creatorcontrib><creatorcontrib>Kamphuis, P</creatorcontrib><creatorcontrib>J -P Kneib</creatorcontrib><creatorcontrib>Lindqvist, M</creatorcontrib><creatorcontrib>Liu, B</creatorcontrib><creatorcontrib>Liu, Y</creatorcontrib><creatorcontrib>Mao, Y</creatorcontrib><creatorcontrib>Marchal, A</creatorcontrib><creatorcontrib>Márquez, I</creatorcontrib><creatorcontrib>Meshcheryakov, A</creatorcontrib><creatorcontrib>Olberg, M</creatorcontrib><creatorcontrib>Oozeer, N</creatorcontrib><creatorcontrib>Pandey-Pommier, M</creatorcontrib><creatorcontrib>Peng, B</creatorcontrib><creatorcontrib>Sabater, J</creatorcontrib><creatorcontrib>Sorgho, A</creatorcontrib><creatorcontrib>Starck, J L</creatorcontrib><creatorcontrib>Tasse, C</creatorcontrib><creatorcontrib>Wang, A</creatorcontrib><creatorcontrib>Wang, Y</creatorcontrib><creatorcontrib>H Xi</creatorcontrib><creatorcontrib>Yang, X</creatorcontrib><creatorcontrib>Zhang, H</creatorcontrib><creatorcontrib>Zhang, J</creatorcontrib><creatorcontrib>Zhao, M</creatorcontrib><creatorcontrib>Zuo, S</creatorcontrib><title>SKA Science Data Challenge 2: analysis and results</title><title>arXiv.org</title><description>The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomers will be correspondingly large and complex, requiring the application of advanced analysis techniques to extract key science findings. To this end, SKAO is conducting a series of Science Data Challenges, each designed to familiarise the scientific community with SKAO data and to drive the development of new analysis techniques. We present the results from Science Data Challenge 2 (SDC2), which invited participants to find and characterise 233245 neutral hydrogen (Hi) sources in a simulated data product representing a 2000~h SKA MID spectral line observation from redshifts 0.25 to 0.5. Through the generous support of eight international supercomputing facilities, participants were able to undertake the Challenge using dedicated computational resources. Alongside the main challenge, `reproducibility awards' were made in recognition of those pipelines which demonstrated Open Science best practice. The Challenge saw over 100 participants develop a range of new and existing techniques, with results that highlight the strengths of multidisciplinary and collaborative effort. The winning strategy -- which combined predictions from two independent machine learning techniques to yield a 20 percent improvement in overall performance -- underscores one of the main Challenge outcomes: that of method complementarity. It is likely that the combination of methods in a so-called ensemble approach will be key to exploiting very large astronomical datasets.</description><subject>Best practice</subject><subject>Line spectra</subject><subject>Machine learning</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Science</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotj01Lw0AURQdBsNT-AFcOuE588-Yr465UrWLBRbsPz8lEU2JaZxKx_97Yurp3cbmcw9iVgFwVWsMtxZ_mO0cJMgfrlDxjE5RSZIVCvGCzlLYAgMai1nLCcP0y52vfhM4Hfk898cUHtW3o3gPHO04dtYfUpLFUPIY0tH26ZOc1tSnM_nPKNo8Pm8VTtnpdPi_mq4w06sxgbYMWVAVC66tgnNWFAVV4DwjGA5hKCwVW1c4Jr4KvR3rloHrzipSTU3Z9uj0KlfvYfFI8lH9i5VFsXNycFvu4-xpC6svtbogjcSrRFhaEQ6HlL01JTcU</recordid><startdate>20230314</startdate><enddate>20230314</enddate><creator>Hartley, P</creator><creator>Bonaldi, A</creator><creator>Braun, R</creator><creator>J N H S Aditya</creator><creator>Aicardi, S</creator><creator>Alegre, L</creator><creator>Chakraborty, A</creator><creator>Chen, X</creator><creator>Choudhuri, S</creator><creator>Clarke, A O</creator><creator>Coles, J</creator><creator>Collinson, J 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Lu ; Mazumder, A ; Moldón, J ; Mondal, R ; S Ni ; Önnheim, M ; Parra, M ; Patra, N ; Peel, A ; Salomé, P ; Sánchez-Expósito, S ; Sargent, M ; Semelin, B ; Serra, P ; Shaw, A K ; Shen, A X ; Sjöberg, A ; Smith, L ; Soroka, A ; Stolyarov, V ; Tolley, E ; Toribio, M C ; J M van der Hulst ; A Vafaei Sadr ; Verdes-Montenegro, L ; Westmeier, T ; K Yu ; Zhang, L ; Zhang, X ; Zhang, Y ; Alberdi, A ; Ashdown, M ; Bom, C R ; Brüggen, M ; Cannon, J ; Chen, R ; Combes, F ; Courbin, F ; Fourestey, G ; Freundlich, J ; Gao, L ; Gheller, C ; Guo, Q ; Gustavsson, E ; Jirstrand, M ; Jones, M G ; Kamphuis, P ; J -P Kneib ; Lindqvist, M ; Liu, B ; Liu, Y ; Mao, Y ; Marchal, A ; Márquez, I ; Meshcheryakov, A ; Olberg, M ; Oozeer, N ; Pandey-Pommier, M ; Peng, B ; Sabater, J ; Sorgho, A ; Starck, J L ; Tasse, C ; Wang, A ; Wang, Y ; H Xi ; Yang, X ; Zhang, H ; Zhang, J ; Zhao, M ; Zuo, S</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a525-62f7e51adea27cde697586048cc0206c006d514074f991c4ecf550490dbc4a493</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Best practice</topic><topic>Line spectra</topic><topic>Machine learning</topic><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Science</topic><toplevel>online_resources</toplevel><creatorcontrib>Hartley, P</creatorcontrib><creatorcontrib>Bonaldi, A</creatorcontrib><creatorcontrib>Braun, R</creatorcontrib><creatorcontrib>J N H S Aditya</creatorcontrib><creatorcontrib>Aicardi, S</creatorcontrib><creatorcontrib>Alegre, L</creatorcontrib><creatorcontrib>Chakraborty, A</creatorcontrib><creatorcontrib>Chen, X</creatorcontrib><creatorcontrib>Choudhuri, 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J</creatorcontrib><creatorcontrib>Mondal, R</creatorcontrib><creatorcontrib>S Ni</creatorcontrib><creatorcontrib>Önnheim, M</creatorcontrib><creatorcontrib>Parra, M</creatorcontrib><creatorcontrib>Patra, N</creatorcontrib><creatorcontrib>Peel, A</creatorcontrib><creatorcontrib>Salomé, P</creatorcontrib><creatorcontrib>Sánchez-Expósito, S</creatorcontrib><creatorcontrib>Sargent, M</creatorcontrib><creatorcontrib>Semelin, B</creatorcontrib><creatorcontrib>Serra, P</creatorcontrib><creatorcontrib>Shaw, A K</creatorcontrib><creatorcontrib>Shen, A X</creatorcontrib><creatorcontrib>Sjöberg, A</creatorcontrib><creatorcontrib>Smith, L</creatorcontrib><creatorcontrib>Soroka, A</creatorcontrib><creatorcontrib>Stolyarov, V</creatorcontrib><creatorcontrib>Tolley, E</creatorcontrib><creatorcontrib>Toribio, M C</creatorcontrib><creatorcontrib>J M van der Hulst</creatorcontrib><creatorcontrib>A Vafaei Sadr</creatorcontrib><creatorcontrib>Verdes-Montenegro, L</creatorcontrib><creatorcontrib>Westmeier, T</creatorcontrib><creatorcontrib>K Yu</creatorcontrib><creatorcontrib>Zhang, L</creatorcontrib><creatorcontrib>Zhang, X</creatorcontrib><creatorcontrib>Zhang, Y</creatorcontrib><creatorcontrib>Alberdi, A</creatorcontrib><creatorcontrib>Ashdown, M</creatorcontrib><creatorcontrib>Bom, C R</creatorcontrib><creatorcontrib>Brüggen, M</creatorcontrib><creatorcontrib>Cannon, J</creatorcontrib><creatorcontrib>Chen, R</creatorcontrib><creatorcontrib>Combes, F</creatorcontrib><creatorcontrib>Courbin, F</creatorcontrib><creatorcontrib>Fourestey, G</creatorcontrib><creatorcontrib>Freundlich, J</creatorcontrib><creatorcontrib>Gao, L</creatorcontrib><creatorcontrib>Gheller, C</creatorcontrib><creatorcontrib>Guo, Q</creatorcontrib><creatorcontrib>Gustavsson, E</creatorcontrib><creatorcontrib>Jirstrand, M</creatorcontrib><creatorcontrib>Jones, M G</creatorcontrib><creatorcontrib>Kamphuis, P</creatorcontrib><creatorcontrib>J -P Kneib</creatorcontrib><creatorcontrib>Lindqvist, M</creatorcontrib><creatorcontrib>Liu, B</creatorcontrib><creatorcontrib>Liu, Y</creatorcontrib><creatorcontrib>Mao, Y</creatorcontrib><creatorcontrib>Marchal, A</creatorcontrib><creatorcontrib>Márquez, I</creatorcontrib><creatorcontrib>Meshcheryakov, A</creatorcontrib><creatorcontrib>Olberg, M</creatorcontrib><creatorcontrib>Oozeer, N</creatorcontrib><creatorcontrib>Pandey-Pommier, M</creatorcontrib><creatorcontrib>Peng, B</creatorcontrib><creatorcontrib>Sabater, J</creatorcontrib><creatorcontrib>Sorgho, A</creatorcontrib><creatorcontrib>Starck, J L</creatorcontrib><creatorcontrib>Tasse, C</creatorcontrib><creatorcontrib>Wang, A</creatorcontrib><creatorcontrib>Wang, Y</creatorcontrib><creatorcontrib>H Xi</creatorcontrib><creatorcontrib>Yang, X</creatorcontrib><creatorcontrib>Zhang, H</creatorcontrib><creatorcontrib>Zhang, J</creatorcontrib><creatorcontrib>Zhao, M</creatorcontrib><creatorcontrib>Zuo, S</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>ProQuest Central (New)</collection><collection>ProQuest One Academic (New)</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Middle East (New)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Applied & Life Sciences</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>Hartley, P</au><au>Bonaldi, A</au><au>Braun, R</au><au>J N H S Aditya</au><au>Aicardi, S</au><au>Alegre, L</au><au>Chakraborty, A</au><au>Chen, X</au><au>Choudhuri, S</au><au>Clarke, A O</au><au>Coles, J</au><au>Collinson, J S</au><au>Cornu, D</au><au>Darriba, L</au><au>M Delli Veneri</au><au>brich, J</au><au>Garrido, J</au><au>Gubanov, F</au><au>Håkansson, H</au><au>Hardcastle, M J</au><au>Heneka, C</au><au>Herranz, D</au><au>Hess, K M</au><au>Jaiswal, S</au><au>Jurek, R J</au><au>Korber, D</au><au>Kitaeff, S</au><au>Kleiner, D</au><au>Lao, B</au><au>X Lu</au><au>Mazumder, A</au><au>Moldón, J</au><au>Mondal, R</au><au>S Ni</au><au>Önnheim, M</au><au>Parra, M</au><au>Patra, N</au><au>Peel, A</au><au>Salomé, P</au><au>Sánchez-Expósito, S</au><au>Sargent, M</au><au>Semelin, B</au><au>Serra, P</au><au>Shaw, A K</au><au>Shen, A X</au><au>Sjöberg, A</au><au>Smith, L</au><au>Soroka, A</au><au>Stolyarov, V</au><au>Tolley, E</au><au>Toribio, M C</au><au>J M van der Hulst</au><au>A Vafaei Sadr</au><au>Verdes-Montenegro, L</au><au>Westmeier, T</au><au>K Yu</au><au>Zhang, L</au><au>Zhang, X</au><au>Zhang, Y</au><au>Alberdi, A</au><au>Ashdown, M</au><au>Bom, C R</au><au>Brüggen, M</au><au>Cannon, J</au><au>Chen, R</au><au>Combes, F</au><au>Courbin, F</au><au>Fourestey, G</au><au>Freundlich, J</au><au>Gao, L</au><au>Gheller, C</au><au>Guo, Q</au><au>Gustavsson, E</au><au>Jirstrand, M</au><au>Jones, M G</au><au>Kamphuis, P</au><au>J -P Kneib</au><au>Lindqvist, M</au><au>Liu, B</au><au>Liu, Y</au><au>Mao, Y</au><au>Marchal, A</au><au>Márquez, I</au><au>Meshcheryakov, A</au><au>Olberg, M</au><au>Oozeer, N</au><au>Pandey-Pommier, M</au><au>Peng, B</au><au>Sabater, J</au><au>Sorgho, A</au><au>Starck, J L</au><au>Tasse, C</au><au>Wang, A</au><au>Wang, Y</au><au>H Xi</au><au>Yang, X</au><au>Zhang, H</au><au>Zhang, J</au><au>Zhao, M</au><au>Zuo, S</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>SKA Science Data Challenge 2: analysis and results</atitle><jtitle>arXiv.org</jtitle><date>2023-03-14</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomers will be correspondingly large and complex, requiring the application of advanced analysis techniques to extract key science findings. To this end, SKAO is conducting a series of Science Data Challenges, each designed to familiarise the scientific community with SKAO data and to drive the development of new analysis techniques. We present the results from Science Data Challenge 2 (SDC2), which invited participants to find and characterise 233245 neutral hydrogen (Hi) sources in a simulated data product representing a 2000~h SKA MID spectral line observation from redshifts 0.25 to 0.5. Through the generous support of eight international supercomputing facilities, participants were able to undertake the Challenge using dedicated computational resources. Alongside the main challenge, `reproducibility awards' were made in recognition of those pipelines which demonstrated Open Science best practice. The Challenge saw over 100 participants develop a range of new and existing techniques, with results that highlight the strengths of multidisciplinary and collaborative effort. The winning strategy -- which combined predictions from two independent machine learning techniques to yield a 20 percent improvement in overall performance -- underscores one of the main Challenge outcomes: that of method complementarity. It is likely that the combination of methods in a so-called ensemble approach will be key to exploiting very large astronomical datasets.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2303.07943</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2023-03 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_2303_07943 |
source | arXiv.org; Free E- Journals |
subjects | Best practice Line spectra Machine learning Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Instrumentation and Methods for Astrophysics Science |
title | SKA Science Data Challenge 2: analysis and results |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-21T17%3A17%3A44IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=SKA%20Science%20Data%20Challenge%202:%20analysis%20and%20results&rft.jtitle=arXiv.org&rft.au=Hartley,%20P&rft.date=2023-03-14&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2303.07943&rft_dat=%3Cproquest_arxiv%3E2787019215%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2787019215&rft_id=info:pmid/&rfr_iscdi=true |