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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Veröffentlicht in:arXiv.org 2023-03
Hauptverfasser: 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
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container_title arXiv.org
container_volume
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
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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. 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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 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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>PHGZM</scope><scope>PHGZT</scope><scope>PIMPY</scope><scope>PKEHL</scope><scope>PQEST</scope><scope>PQGLB</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20230314</creationdate><title>SKA Science Data Challenge 2: analysis and results</title><author>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</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</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>
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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
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