On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2
This paper provides a catalogue of stars, quasars, and galaxies for the Southern Photometric Local Universe Survey Data Release 2 (S-PLUS DR2) in the Stripe 82 region. We show that a 12-band filter system (5 Sloan-like and 7 narrow bands) allows better performance for object classification than the...
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creator | Nakazono, L Mendes de Oliveira, C Hirata, N S T Jeram, S Queiroz, C Eikenberry, Stephen S Gonzalez, A H Abramo, R Overzier, R Espadoto, M Martinazzo, A Sampedro, L Herpich, F R Almeida-Fernandes, F Werle, A Barbosa, C E Sodré, L Lima, E V Buzzo, M L Cortesi, A Menéndez-Delmestre, K Akras, S Alvarez-Candal, Alvaro Lopes, A R Telles, E Schoenell, W Kanaan, A Ribeiro, T |
description | This paper provides a catalogue of stars, quasars, and galaxies for the Southern Photometric Local Universe Survey Data Release 2 (S-PLUS DR2) in the Stripe 82 region. We show that a 12-band filter system (5 Sloan-like and 7 narrow bands) allows better performance for object classification than the usual analysis based solely on broad bands (regardless of infrared information). Moreover, we show that our classification is robust against missing values. Using spectroscopically confirmed sources retrieved from the Sloan Digital Sky Survey DR16 and DR14Q, we train a random forest classifier with the 12 S-PLUS magnitudes + 4 morphological features. A second random forest classifier is trained with the addition of the W1 (3.4 \(\mu\)m) and W2 (4.6 \(\mu\)m) magnitudes from the Wide-field Infrared Survey Explorer (WISE). Forty-four percent of our catalogue have WISE counterparts and are provided with classification from both models. We achieve 95.76% (52.47%) of quasar purity, 95.88% (92.24%) of quasar completeness, 99.44% (98.17%) of star purity, 98.22% (78.56%) of star completeness, 98.04% (81.39%) of galaxy purity, and 98.8% (85.37%) of galaxy completeness for the first (second) classifier, for which the metrics were calculated on objects with (without) WISE counterpart. A total of 2,926,787 objects that are not in our spectroscopic sample were labelled, obtaining 335,956 quasars, 1,347,340 stars, and 1,243,391 galaxies. From those, 7.4%, 76.0%, and 58.4% were classified with probabilities above 80%. The catalogue with classification and probabilities for Stripe 82 S-PLUS DR2 is available for download. |
doi_str_mv | 10.48550/arxiv.2106.11986 |
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We show that a 12-band filter system (5 Sloan-like and 7 narrow bands) allows better performance for object classification than the usual analysis based solely on broad bands (regardless of infrared information). Moreover, we show that our classification is robust against missing values. Using spectroscopically confirmed sources retrieved from the Sloan Digital Sky Survey DR16 and DR14Q, we train a random forest classifier with the 12 S-PLUS magnitudes + 4 morphological features. A second random forest classifier is trained with the addition of the W1 (3.4 \(\mu\)m) and W2 (4.6 \(\mu\)m) magnitudes from the Wide-field Infrared Survey Explorer (WISE). Forty-four percent of our catalogue have WISE counterparts and are provided with classification from both models. We achieve 95.76% (52.47%) of quasar purity, 95.88% (92.24%) of quasar completeness, 99.44% (98.17%) of star purity, 98.22% (78.56%) of star completeness, 98.04% (81.39%) of galaxy purity, and 98.8% (85.37%) of galaxy completeness for the first (second) classifier, for which the metrics were calculated on objects with (without) WISE counterpart. A total of 2,926,787 objects that are not in our spectroscopic sample were labelled, obtaining 335,956 quasars, 1,347,340 stars, and 1,243,391 galaxies. From those, 7.4%, 76.0%, and 58.4% were classified with probabilities above 80%. The catalogue with classification and probabilities for Stripe 82 S-PLUS DR2 is available for download.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2106.11986</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Classification ; Classifiers ; Completeness ; Galaxies ; Infrared analysis ; Infrared astronomy ; Local group (astronomy) ; Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics ; Purity ; Quasars ; Sky surveys (astronomy) ; Southern Hemisphere ; Stars ; Stars & galaxies</subject><ispartof>arXiv.org, 2021-11</ispartof><rights>2021. 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/10.48550/arXiv.2106.11986$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1093/mnras/stab1835$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Nakazono, L</creatorcontrib><creatorcontrib>Mendes de Oliveira, C</creatorcontrib><creatorcontrib>Hirata, N S T</creatorcontrib><creatorcontrib>Jeram, S</creatorcontrib><creatorcontrib>Queiroz, C</creatorcontrib><creatorcontrib>Eikenberry, Stephen S</creatorcontrib><creatorcontrib>Gonzalez, A H</creatorcontrib><creatorcontrib>Abramo, R</creatorcontrib><creatorcontrib>Overzier, R</creatorcontrib><creatorcontrib>Espadoto, M</creatorcontrib><creatorcontrib>Martinazzo, A</creatorcontrib><creatorcontrib>Sampedro, L</creatorcontrib><creatorcontrib>Herpich, F R</creatorcontrib><creatorcontrib>Almeida-Fernandes, F</creatorcontrib><creatorcontrib>Werle, A</creatorcontrib><creatorcontrib>Barbosa, C E</creatorcontrib><creatorcontrib>Sodré, L</creatorcontrib><creatorcontrib>Lima, E V</creatorcontrib><creatorcontrib>Buzzo, M L</creatorcontrib><creatorcontrib>Cortesi, A</creatorcontrib><creatorcontrib>Menéndez-Delmestre, K</creatorcontrib><creatorcontrib>Akras, S</creatorcontrib><creatorcontrib>Alvarez-Candal, Alvaro</creatorcontrib><creatorcontrib>Lopes, A R</creatorcontrib><creatorcontrib>Telles, E</creatorcontrib><creatorcontrib>Schoenell, W</creatorcontrib><creatorcontrib>Kanaan, A</creatorcontrib><creatorcontrib>Ribeiro, T</creatorcontrib><title>On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2</title><title>arXiv.org</title><description>This paper provides a catalogue of stars, quasars, and galaxies for the Southern Photometric Local Universe Survey Data Release 2 (S-PLUS DR2) in the Stripe 82 region. We show that a 12-band filter system (5 Sloan-like and 7 narrow bands) allows better performance for object classification than the usual analysis based solely on broad bands (regardless of infrared information). Moreover, we show that our classification is robust against missing values. Using spectroscopically confirmed sources retrieved from the Sloan Digital Sky Survey DR16 and DR14Q, we train a random forest classifier with the 12 S-PLUS magnitudes + 4 morphological features. A second random forest classifier is trained with the addition of the W1 (3.4 \(\mu\)m) and W2 (4.6 \(\mu\)m) magnitudes from the Wide-field Infrared Survey Explorer (WISE). Forty-four percent of our catalogue have WISE counterparts and are provided with classification from both models. We achieve 95.76% (52.47%) of quasar purity, 95.88% (92.24%) of quasar completeness, 99.44% (98.17%) of star purity, 98.22% (78.56%) of star completeness, 98.04% (81.39%) of galaxy purity, and 98.8% (85.37%) of galaxy completeness for the first (second) classifier, for which the metrics were calculated on objects with (without) WISE counterpart. A total of 2,926,787 objects that are not in our spectroscopic sample were labelled, obtaining 335,956 quasars, 1,347,340 stars, and 1,243,391 galaxies. From those, 7.4%, 76.0%, and 58.4% were classified with probabilities above 80%. The catalogue with classification and probabilities for Stripe 82 S-PLUS DR2 is available for download.</description><subject>Classification</subject><subject>Classifiers</subject><subject>Completeness</subject><subject>Galaxies</subject><subject>Infrared analysis</subject><subject>Infrared astronomy</subject><subject>Local group (astronomy)</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>Purity</subject><subject>Quasars</subject><subject>Sky surveys (astronomy)</subject><subject>Southern Hemisphere</subject><subject>Stars</subject><subject>Stars & galaxies</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotUE1PwkAU3JiYSJAf4MlNvFp8-7bbdo8GPzAhwQiePDSvZVeWQAu7LcK_t4KnmcPMZGYYuxEwjDOl4IH8we2HKCAZCqGz5IL1UEoRZTHiFRuEsAIATFJUSvbY17TizdLwhQtlvTf-yGvLQ0M-3PNdS-FEqFrwb1rTwZnA3dkwq9sOfMXHZuPCtqOG_7hmyWfR--Rzxp8-8JpdWloHM_jHPpu_PM9H42gyfX0bPU4iUigiVWSoU1smqiSlSxAo7QJKDTFRkcUgEtQgC0htZsoCQYtEa2VJo01NUpDss9tz7Gl5vvVuQ_6Y_z2Qnx7oFHdnxdbXu9aEJl_Vra-6TjmqOE4BNAr5C6YCXME</recordid><startdate>20211104</startdate><enddate>20211104</enddate><creator>Nakazono, L</creator><creator>Mendes de Oliveira, C</creator><creator>Hirata, N S T</creator><creator>Jeram, S</creator><creator>Queiroz, C</creator><creator>Eikenberry, Stephen S</creator><creator>Gonzalez, A H</creator><creator>Abramo, R</creator><creator>Overzier, R</creator><creator>Espadoto, M</creator><creator>Martinazzo, A</creator><creator>Sampedro, L</creator><creator>Herpich, F R</creator><creator>Almeida-Fernandes, F</creator><creator>Werle, A</creator><creator>Barbosa, C E</creator><creator>Sodré, L</creator><creator>Lima, E V</creator><creator>Buzzo, M L</creator><creator>Cortesi, A</creator><creator>Menéndez-Delmestre, K</creator><creator>Akras, S</creator><creator>Alvarez-Candal, Alvaro</creator><creator>Lopes, A R</creator><creator>Telles, E</creator><creator>Schoenell, W</creator><creator>Kanaan, A</creator><creator>Ribeiro, T</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>20211104</creationdate><title>On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2</title><author>Nakazono, L ; Mendes de Oliveira, C ; Hirata, N S T ; Jeram, S ; Queiroz, C ; Eikenberry, Stephen S ; Gonzalez, A H ; Abramo, R ; Overzier, R ; Espadoto, M ; Martinazzo, A ; Sampedro, L ; Herpich, F R ; Almeida-Fernandes, F ; Werle, A ; Barbosa, C E ; Sodré, L ; Lima, E V ; Buzzo, M L ; Cortesi, A ; Menéndez-Delmestre, K ; Akras, S ; Alvarez-Candal, Alvaro ; Lopes, A R ; Telles, E ; Schoenell, W ; Kanaan, A ; Ribeiro, T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a521-5b8297fc65ca59c0123fd0c904aab840162903b07f8ecb20916995fa92f7e6ba3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Classification</topic><topic>Classifiers</topic><topic>Completeness</topic><topic>Galaxies</topic><topic>Infrared analysis</topic><topic>Infrared astronomy</topic><topic>Local group (astronomy)</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>Purity</topic><topic>Quasars</topic><topic>Sky surveys (astronomy)</topic><topic>Southern Hemisphere</topic><topic>Stars</topic><topic>Stars & galaxies</topic><toplevel>online_resources</toplevel><creatorcontrib>Nakazono, L</creatorcontrib><creatorcontrib>Mendes de Oliveira, C</creatorcontrib><creatorcontrib>Hirata, N S T</creatorcontrib><creatorcontrib>Jeram, S</creatorcontrib><creatorcontrib>Queiroz, C</creatorcontrib><creatorcontrib>Eikenberry, Stephen S</creatorcontrib><creatorcontrib>Gonzalez, A H</creatorcontrib><creatorcontrib>Abramo, R</creatorcontrib><creatorcontrib>Overzier, R</creatorcontrib><creatorcontrib>Espadoto, M</creatorcontrib><creatorcontrib>Martinazzo, A</creatorcontrib><creatorcontrib>Sampedro, L</creatorcontrib><creatorcontrib>Herpich, F R</creatorcontrib><creatorcontrib>Almeida-Fernandes, F</creatorcontrib><creatorcontrib>Werle, A</creatorcontrib><creatorcontrib>Barbosa, C E</creatorcontrib><creatorcontrib>Sodré, L</creatorcontrib><creatorcontrib>Lima, E V</creatorcontrib><creatorcontrib>Buzzo, M L</creatorcontrib><creatorcontrib>Cortesi, A</creatorcontrib><creatorcontrib>Menéndez-Delmestre, K</creatorcontrib><creatorcontrib>Akras, S</creatorcontrib><creatorcontrib>Alvarez-Candal, Alvaro</creatorcontrib><creatorcontrib>Lopes, A R</creatorcontrib><creatorcontrib>Telles, E</creatorcontrib><creatorcontrib>Schoenell, W</creatorcontrib><creatorcontrib>Kanaan, A</creatorcontrib><creatorcontrib>Ribeiro, T</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>Nakazono, L</au><au>Mendes de Oliveira, C</au><au>Hirata, N S T</au><au>Jeram, S</au><au>Queiroz, C</au><au>Eikenberry, Stephen S</au><au>Gonzalez, A H</au><au>Abramo, R</au><au>Overzier, R</au><au>Espadoto, M</au><au>Martinazzo, A</au><au>Sampedro, L</au><au>Herpich, F R</au><au>Almeida-Fernandes, F</au><au>Werle, A</au><au>Barbosa, C E</au><au>Sodré, L</au><au>Lima, E V</au><au>Buzzo, M L</au><au>Cortesi, A</au><au>Menéndez-Delmestre, K</au><au>Akras, S</au><au>Alvarez-Candal, Alvaro</au><au>Lopes, A R</au><au>Telles, E</au><au>Schoenell, W</au><au>Kanaan, A</au><au>Ribeiro, T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2</atitle><jtitle>arXiv.org</jtitle><date>2021-11-04</date><risdate>2021</risdate><eissn>2331-8422</eissn><abstract>This paper provides a catalogue of stars, quasars, and galaxies for the Southern Photometric Local Universe Survey Data Release 2 (S-PLUS DR2) in the Stripe 82 region. We show that a 12-band filter system (5 Sloan-like and 7 narrow bands) allows better performance for object classification than the usual analysis based solely on broad bands (regardless of infrared information). Moreover, we show that our classification is robust against missing values. Using spectroscopically confirmed sources retrieved from the Sloan Digital Sky Survey DR16 and DR14Q, we train a random forest classifier with the 12 S-PLUS magnitudes + 4 morphological features. A second random forest classifier is trained with the addition of the W1 (3.4 \(\mu\)m) and W2 (4.6 \(\mu\)m) magnitudes from the Wide-field Infrared Survey Explorer (WISE). Forty-four percent of our catalogue have WISE counterparts and are provided with classification from both models. We achieve 95.76% (52.47%) of quasar purity, 95.88% (92.24%) of quasar completeness, 99.44% (98.17%) of star purity, 98.22% (78.56%) of star completeness, 98.04% (81.39%) of galaxy purity, and 98.8% (85.37%) of galaxy completeness for the first (second) classifier, for which the metrics were calculated on objects with (without) WISE counterpart. A total of 2,926,787 objects that are not in our spectroscopic sample were labelled, obtaining 335,956 quasars, 1,347,340 stars, and 1,243,391 galaxies. From those, 7.4%, 76.0%, and 58.4% were classified with probabilities above 80%. The catalogue with classification and probabilities for Stripe 82 S-PLUS DR2 is available for download.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2106.11986</doi><oa>free_for_read</oa></addata></record> |
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subjects | Classification Classifiers Completeness Galaxies Infrared analysis Infrared astronomy Local group (astronomy) Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Purity Quasars Sky surveys (astronomy) Southern Hemisphere Stars Stars & galaxies |
title | On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2 |
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