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Multiplicity Boost of Transit Signal Classifiers: Validation of 69 New Exoplanets using the Multiplicity Boost of ExoMiner
Most existing exoplanets are discovered using validation techniques rather than being confirmed by complementary observations. These techniques generate a score that is typically the probability of the transit signal being an exoplanet ( y ( x ) = exoplanet) given some information related to that si...
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Published in: | The Astronomical journal 2023-07, Vol.166 (1), p.28 |
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creator | Valizadegan, Hamed Martinho, Miguel J. S. Jenkins, Jon M. Caldwell, Douglas A. Twicken, Joseph D. Bryson, Stephen T. |
description | Most existing exoplanets are discovered using validation techniques rather than being confirmed by complementary observations. These techniques generate a score that is typically the probability of the transit signal being an exoplanet (
y
(
x
) = exoplanet) given some information related to that signal (represented by
x
). Except for the validation technique in Rowe et al. (2014), which uses multiplicity information to generate these probability scores, the existing validation techniques ignore the multiplicity boost information. In this work, we introduce a framework with the following premise: given an existing transit-signal vetter (classifier), improve its performance using multiplicity information. We apply this framework to several existing classifiers, which include
vespa
,
Robovetter
,
AstroNet
,
ExoNet
,
GPC
and
RFC
, and
ExoMiner
, to support our claim that this framework is able to improve the performance of a given classifier. We then use the proposed multiplicity boost framework for
ExoMiner
V1.2, which addresses some of the shortcomings of the original
ExoMiner
classifier, and validate 69 new exoplanets for systems with multiple Kepler Objects of Interests from the Kepler catalog. |
doi_str_mv | 10.3847/1538-3881/acd344 |
format | article |
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y
(
x
) = exoplanet) given some information related to that signal (represented by
x
). Except for the validation technique in Rowe et al. (2014), which uses multiplicity information to generate these probability scores, the existing validation techniques ignore the multiplicity boost information. In this work, we introduce a framework with the following premise: given an existing transit-signal vetter (classifier), improve its performance using multiplicity information. We apply this framework to several existing classifiers, which include
vespa
,
Robovetter
,
AstroNet
,
ExoNet
,
GPC
and
RFC
, and
ExoMiner
, to support our claim that this framework is able to improve the performance of a given classifier. We then use the proposed multiplicity boost framework for
ExoMiner
V1.2, which addresses some of the shortcomings of the original
ExoMiner
classifier, and validate 69 new exoplanets for systems with multiple Kepler Objects of Interests from the Kepler catalog.</description><identifier>ISSN: 0004-6256</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.3847/1538-3881/acd344</identifier><language>eng</language><publisher>Madison: The American Astronomical Society</publisher><subject>Astronomy ; Classifiers ; Convolutional neural networks ; Exoplanet astronomy ; Exoplanet catalogs ; Exoplanet detection methods ; Exoplanet systems ; Exoplanets ; Extrasolar planets ; Neural networks ; Performance enhancement ; Signal classification</subject><ispartof>The Astronomical journal, 2023-07, Vol.166 (1), p.28</ispartof><rights>2023. The Author(s). Published by the American Astronomical Society.</rights><rights>2023. The Author(s). Published by the American Astronomical Society. 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><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c444t-e5cdeb87186b9b1ca2092aa4bb58e6909e06392725779263acb4fa2a93a0ff043</citedby><cites>FETCH-LOGICAL-c444t-e5cdeb87186b9b1ca2092aa4bb58e6909e06392725779263acb4fa2a93a0ff043</cites><orcidid>0000-0003-1963-9616 ; 0000-0002-4715-9460 ; 0000-0002-2188-0807 ; 0000-0002-6778-7552 ; 0000-0003-0081-1797 ; 0000-0001-6732-0840</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,864,2102,27924,27925</link.rule.ids></links><search><creatorcontrib>Valizadegan, Hamed</creatorcontrib><creatorcontrib>Martinho, Miguel J. S.</creatorcontrib><creatorcontrib>Jenkins, Jon M.</creatorcontrib><creatorcontrib>Caldwell, Douglas A.</creatorcontrib><creatorcontrib>Twicken, Joseph D.</creatorcontrib><creatorcontrib>Bryson, Stephen T.</creatorcontrib><title>Multiplicity Boost of Transit Signal Classifiers: Validation of 69 New Exoplanets using the Multiplicity Boost of ExoMiner</title><title>The Astronomical journal</title><addtitle>AJ</addtitle><addtitle>Astron. J</addtitle><description>Most existing exoplanets are discovered using validation techniques rather than being confirmed by complementary observations. These techniques generate a score that is typically the probability of the transit signal being an exoplanet (
y
(
x
) = exoplanet) given some information related to that signal (represented by
x
). Except for the validation technique in Rowe et al. (2014), which uses multiplicity information to generate these probability scores, the existing validation techniques ignore the multiplicity boost information. In this work, we introduce a framework with the following premise: given an existing transit-signal vetter (classifier), improve its performance using multiplicity information. We apply this framework to several existing classifiers, which include
vespa
,
Robovetter
,
AstroNet
,
ExoNet
,
GPC
and
RFC
, and
ExoMiner
, to support our claim that this framework is able to improve the performance of a given classifier. We then use the proposed multiplicity boost framework for
ExoMiner
V1.2, which addresses some of the shortcomings of the original
ExoMiner
classifier, and validate 69 new exoplanets for systems with multiple Kepler Objects of Interests from the Kepler catalog.</description><subject>Astronomy</subject><subject>Classifiers</subject><subject>Convolutional neural networks</subject><subject>Exoplanet astronomy</subject><subject>Exoplanet catalogs</subject><subject>Exoplanet detection methods</subject><subject>Exoplanet systems</subject><subject>Exoplanets</subject><subject>Extrasolar planets</subject><subject>Neural networks</subject><subject>Performance enhancement</subject><subject>Signal classification</subject><issn>0004-6256</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>DOA</sourceid><recordid>eNp9kUtv1DAURi0EEkNhz9JSt6T1K47NDkalrdTCoi1b68aPwaMQB9sjKL--CUFlU7GydHXu-Wx_CL2l5IQr0Z3SlquGK0VPwTouxDO0eRw9RxtCiGgka-VL9KqUPSGUKiI26Pf1YahxGqKN9R5_TKlUnAK-zTCWWPFN3I0w4O0ApcQQfS7v8VcYooMa07iQUuPP_ic--5WmAUZfCz6UOO5w_ebx0-4ZvY6jz6_RiwBD8W_-nkfo7tPZ7faiufpyfrn9cNVYIURtfGud71VHlex1Ty0wohmA6PtWeamJ9kRyzTrWdp1mkoPtRQAGmgMJgQh-hC5Xr0uwN1OO3yHfmwTR_BmkvDOQa7SDNxzmKB46B64VNnBFZ6tzrYTWBmJhdh2vrimnHwdfqtmnQ56_qBimmFZc6m5JJCtlcyol-_CYSolZ2jJLNWapxqxtzSvv1pWYpn_O_-DHT-Dza6iUhs53MZML_AGbmKNf</recordid><startdate>20230701</startdate><enddate>20230701</enddate><creator>Valizadegan, Hamed</creator><creator>Martinho, Miguel J. 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S.</creatorcontrib><creatorcontrib>Jenkins, Jon M.</creatorcontrib><creatorcontrib>Caldwell, Douglas A.</creatorcontrib><creatorcontrib>Twicken, Joseph D.</creatorcontrib><creatorcontrib>Bryson, Stephen T.</creatorcontrib><collection>Open Access: IOP Publishing Free Content</collection><collection>IOPscience (Open Access)</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Valizadegan, Hamed</au><au>Martinho, Miguel J. 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y
(
x
) = exoplanet) given some information related to that signal (represented by
x
). Except for the validation technique in Rowe et al. (2014), which uses multiplicity information to generate these probability scores, the existing validation techniques ignore the multiplicity boost information. In this work, we introduce a framework with the following premise: given an existing transit-signal vetter (classifier), improve its performance using multiplicity information. We apply this framework to several existing classifiers, which include
vespa
,
Robovetter
,
AstroNet
,
ExoNet
,
GPC
and
RFC
, and
ExoMiner
, to support our claim that this framework is able to improve the performance of a given classifier. We then use the proposed multiplicity boost framework for
ExoMiner
V1.2, which addresses some of the shortcomings of the original
ExoMiner
classifier, and validate 69 new exoplanets for systems with multiple Kepler Objects of Interests from the Kepler catalog.</abstract><cop>Madison</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-3881/acd344</doi><tpages>20</tpages><orcidid>https://orcid.org/0000-0003-1963-9616</orcidid><orcidid>https://orcid.org/0000-0002-4715-9460</orcidid><orcidid>https://orcid.org/0000-0002-2188-0807</orcidid><orcidid>https://orcid.org/0000-0002-6778-7552</orcidid><orcidid>https://orcid.org/0000-0003-0081-1797</orcidid><orcidid>https://orcid.org/0000-0001-6732-0840</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Astronomy Classifiers Convolutional neural networks Exoplanet astronomy Exoplanet catalogs Exoplanet detection methods Exoplanet systems Exoplanets Extrasolar planets Neural networks Performance enhancement Signal classification |
title | Multiplicity Boost of Transit Signal Classifiers: Validation of 69 New Exoplanets using the Multiplicity Boost of ExoMiner |
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