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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/48AE23B
Repositorysid.inpe.br/mtc-m21d/2023/01.02.11.03   (restricted access)
Last Update2023:01.02.11.03.49 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2023/01.02.11.03.49
Metadata Last Update2023:01.10.17.38.27 (UTC) administrator
DOI10.1007/s10569-022-10110-7
ISSN0923-2958
Citation KeyCarrubaAljCarDomMar:2022:OpArNe
TitleOptimization of artificial neural networks models applied to the identification of images of asteroids’ resonant arguments
Year2022
MonthDec.
Access Date2024, May 14
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3772 KiB
2. Context
Author1 Carruba, Valério
2 Aljbaae, Safwan
3 Caritá, Gabriel Antonio
4 Domingos, R. C.
5 Martins, B.
ORCID1 0000-0003-2786-0740
Group1
2 DIMEC-CGCE-INPE-MCTI-GOV-BR
3 CMC-ETES-DIPGR-INPE-MCTI-GOV-BR
Affiliation1 Universidade Estadual Paulista (UNESP)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Universidade Estadual Paulista (UNESP)
5 Universidade Estadual Paulista (UNESP)
Author e-Mail Address1 valerio.carruba@unesp.br
2 safwan.aljbaae@gmail.com
3 gabrielcarita@gmail.com
JournalCelestial Mechanics and Dynamical Astronomy
Volume134
Number6
Pagese59
Secondary MarkA2_ENGENHARIAS_III B1_INTERDISCIPLINAR B1_ASTRONOMIA_/_FÍSICA B2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B3_ENSINO B3_CIÊNCIA_DA_COMPUTAÇÃO
History (UTC)2023-01-02 11:03:49 :: simone -> administrator ::
2023-01-02 11:03:50 :: administrator -> simone :: 2022
2023-01-02 11:04:29 :: simone -> administrator :: 2022
2023-01-04 07:39:06 :: administrator -> simone :: 2022
2023-01-04 12:03:09 :: simone -> administrator :: 2022
2023-01-10 17:38:27 :: administrator -> simone :: 2022
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAsteroids
General
Minor planets
Time domain astronomy
Time series analysis
AbstractThe asteroidal main belt is crossed by a web of mean motion and secular resonances that occur when there is a commensurability between fundamental frequencies of the asteroids and planets. Traditionally, these objects were identified by visual inspection of the time evolution of their resonant argument, which is a combination of orbital elements of the asteroid and the perturbing planet(s). Since the population of asteroids affected by these resonances is, in some cases, of the order of several thousand, this has become a taxing task for a human observer. Recent works used convolutional neural network (CNN) models to perform such task automatically. In this work, we compare the outcome of such models with those of some of the most advanced and publicly available CNN architectures, like the VGG, Inception, and ResNet. The performance of such models is first tested and optimized for overfitting issues, using validation sets and a series of regularization techniques like data augmentation, dropout, and batch normalization. The three best-performing models were then used to predict the labels of larger testing databases containing thousands of images. The VGG model, with and without regularizations, proved to be the most efficient method to predict labels of large datasets. Since the Vera C. Rubin observatory is likely to discover up to four million new asteroids in the next few years, the use of these models might become quite valuable to identify populations of resonant minor bodies.
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4. Conditions of access and use
Languageen
Target Files10569-022-10110-7.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2021/06.04.03.40.25
Next Higher Units8JMKD3MGPCW/3F2UALS
8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.17.52 4
sid.inpe.br/bibdigital/2013/10.14.00.13 1
DisseminationWEBSCI; PORTALCAPES.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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