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Data-efficient classification of radio galaxies
ABSTRACT The continuum emission from radio galaxies can be generally classified into different morphological classes such as FRI, FRII, bent, or compact. In this paper, we explore the task of radio galaxy classification based on morphology using deep learning methods with a focus on using a small-sc...
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Published in: | Monthly notices of the Royal Astronomical Society 2022-01, Vol.509 (2), p.2269-2280 |
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creator | Samudre, Ashwin George, Lijo T Bansal, Mahak Wadadekar, Yogesh |
description | ABSTRACT
The continuum emission from radio galaxies can be generally classified into different morphological classes such as FRI, FRII, bent, or compact. In this paper, we explore the task of radio galaxy classification based on morphology using deep learning methods with a focus on using a small-scale data set (∼2000 samples). We apply few-shot learning techniques based on twin networks and transfer learning techniques using a pre-trained DenseNet model with advanced techniques like cyclical learning rate and discriminative learning to train the model rapidly. We achieve a classification accuracy of over 92 per cent using our best-performing model with the biggest source of confusion being between bent- and FRII-type galaxies. Our results show that focusing on a small but curated data set along with the use of best practices to train the neural network can lead to good results. Automated classification techniques will be crucial for upcoming surveys with next-generation radio telescopes that are expected to detect hundreds of thousands of new radio galaxies in the near future. |
doi_str_mv | 10.1093/mnras/stab3144 |
format | article |
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The continuum emission from radio galaxies can be generally classified into different morphological classes such as FRI, FRII, bent, or compact. In this paper, we explore the task of radio galaxy classification based on morphology using deep learning methods with a focus on using a small-scale data set (∼2000 samples). We apply few-shot learning techniques based on twin networks and transfer learning techniques using a pre-trained DenseNet model with advanced techniques like cyclical learning rate and discriminative learning to train the model rapidly. We achieve a classification accuracy of over 92 per cent using our best-performing model with the biggest source of confusion being between bent- and FRII-type galaxies. Our results show that focusing on a small but curated data set along with the use of best practices to train the neural network can lead to good results. Automated classification techniques will be crucial for upcoming surveys with next-generation radio telescopes that are expected to detect hundreds of thousands of new radio galaxies in the near future.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/stab3144</identifier><language>eng</language><publisher>Oxford University Press</publisher><ispartof>Monthly notices of the Royal Astronomical Society, 2022-01, Vol.509 (2), p.2269-2280</ispartof><rights>2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society 2021</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c273t-7c3f7cbb36ffd99222b0e9404dcc7726a88b6d5a86fc6c64b4ea8a8b95dfbffb3</citedby><orcidid>0000-0003-0287-5022 ; 0000-0001-8136-7645</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,1604,27923,27924</link.rule.ids><linktorsrc>$$Uhttps://dx.doi.org/10.1093/mnras/stab3144$$EView_record_in_Oxford_University_Press$$FView_record_in_$$GOxford_University_Press</linktorsrc></links><search><creatorcontrib>Samudre, Ashwin</creatorcontrib><creatorcontrib>George, Lijo T</creatorcontrib><creatorcontrib>Bansal, Mahak</creatorcontrib><creatorcontrib>Wadadekar, Yogesh</creatorcontrib><title>Data-efficient classification of radio galaxies</title><title>Monthly notices of the Royal Astronomical Society</title><description>ABSTRACT
The continuum emission from radio galaxies can be generally classified into different morphological classes such as FRI, FRII, bent, or compact. In this paper, we explore the task of radio galaxy classification based on morphology using deep learning methods with a focus on using a small-scale data set (∼2000 samples). We apply few-shot learning techniques based on twin networks and transfer learning techniques using a pre-trained DenseNet model with advanced techniques like cyclical learning rate and discriminative learning to train the model rapidly. We achieve a classification accuracy of over 92 per cent using our best-performing model with the biggest source of confusion being between bent- and FRII-type galaxies. Our results show that focusing on a small but curated data set along with the use of best practices to train the neural network can lead to good results. Automated classification techniques will be crucial for upcoming surveys with next-generation radio telescopes that are expected to detect hundreds of thousands of new radio galaxies in the near future.</description><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNqFj0tLxDAUhYMoWGfcuu7WRaZ5NY-ljE8YcOOsy02aK5FOOyQV9N87Orp2dThwvgMfIVecrThzstmNGUpTZvCSK3VCKi51S4XT-pRUjMmWWsP5Obko5Y0xpqTQFWluYQYaEVNIcZzrMEAp6dBgTtNYT1hn6NNUv8IAHymWJTlDGEq8_M0F2d7fvawf6eb54Wl9s6FBGDlTEySa4L3UiL1zQgjPolNM9SEYIzRY63XfgtUYdNDKqwgWrHdtjx7RywVZHX9DnkrJEbt9TjvInx1n3bdu96Pb_ekegOsjML3v_9t-AVxtWgE</recordid><startdate>20220101</startdate><enddate>20220101</enddate><creator>Samudre, Ashwin</creator><creator>George, Lijo T</creator><creator>Bansal, Mahak</creator><creator>Wadadekar, Yogesh</creator><general>Oxford University Press</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0003-0287-5022</orcidid><orcidid>https://orcid.org/0000-0001-8136-7645</orcidid></search><sort><creationdate>20220101</creationdate><title>Data-efficient classification of radio galaxies</title><author>Samudre, Ashwin ; George, Lijo T ; Bansal, Mahak ; Wadadekar, Yogesh</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c273t-7c3f7cbb36ffd99222b0e9404dcc7726a88b6d5a86fc6c64b4ea8a8b95dfbffb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Samudre, Ashwin</creatorcontrib><creatorcontrib>George, Lijo T</creatorcontrib><creatorcontrib>Bansal, Mahak</creatorcontrib><creatorcontrib>Wadadekar, Yogesh</creatorcontrib><collection>CrossRef</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Samudre, Ashwin</au><au>George, Lijo T</au><au>Bansal, Mahak</au><au>Wadadekar, Yogesh</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Data-efficient classification of radio galaxies</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2022-01-01</date><risdate>2022</risdate><volume>509</volume><issue>2</issue><spage>2269</spage><epage>2280</epage><pages>2269-2280</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>ABSTRACT
The continuum emission from radio galaxies can be generally classified into different morphological classes such as FRI, FRII, bent, or compact. In this paper, we explore the task of radio galaxy classification based on morphology using deep learning methods with a focus on using a small-scale data set (∼2000 samples). We apply few-shot learning techniques based on twin networks and transfer learning techniques using a pre-trained DenseNet model with advanced techniques like cyclical learning rate and discriminative learning to train the model rapidly. We achieve a classification accuracy of over 92 per cent using our best-performing model with the biggest source of confusion being between bent- and FRII-type galaxies. Our results show that focusing on a small but curated data set along with the use of best practices to train the neural network can lead to good results. Automated classification techniques will be crucial for upcoming surveys with next-generation radio telescopes that are expected to detect hundreds of thousands of new radio galaxies in the near future.</abstract><pub>Oxford University Press</pub><doi>10.1093/mnras/stab3144</doi><tpages>12</tpages><orcidid>https://orcid.org/0000-0003-0287-5022</orcidid><orcidid>https://orcid.org/0000-0001-8136-7645</orcidid></addata></record> |
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title | Data-efficient classification of radio galaxies |
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