Solutions for 10,000 Eclipsing Binaries in the Bulge Fields of OGLE II Using DEBiL
We have developed a fully automated pipeline for systematically identifying and analyzing eclipsing binaries within large data sets of light curves. The pipeline is made up of multiple tiers that subject the light curves to increasing levels of scrutiny. After each tier, light curves that did not co...
Saved in:
| Published in | The Astrophysical journal Vol. 628; no. 1; pp. 411 - 425 |
|---|---|
| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
Chicago, IL
IOP Publishing
20.07.2005
University of Chicago Press |
| Subjects | |
| Online Access | Get full text |
Cover
Loading…
| Abstract | We have developed a fully automated pipeline for systematically identifying and analyzing eclipsing binaries within large data sets of light curves. The pipeline is made up of multiple tiers that subject the light curves to increasing levels of scrutiny. After each tier, light curves that did not conform to a given criteria were filtered out of the pipeline, reducing the load on the following, more computationally intensive tiers. As a central component of the pipeline, we created the fully automated Detached Eclipsing Binary Light curve fitter (DEBiL), which rapidly fits large numbers of light curves to a simple model. Using the results of DEBiL, light curves of interest can be flagged for follow-up analysis. As a test case, we analyzed the 218,699 light curves within the bulge fields of the OGLE II survey and produced 10,862 model fits. We point out a small number of extreme examples, as well as unexpected structure found in several of the population distributions. We expect this approach to become increasingly important as light-curve data sets continue growing in both size and number. |
|---|---|
| AbstractList | We have developed a fully automated pipeline for systematically identifying and analyzing eclipsing binaries within large data sets of light curves. The pipeline is made up of multiple tiers that subject the light curves to increasing levels of scrutiny. After each tier, light curves that did not conform to a given criteria were filtered out of the pipeline, reducing the load on the following, more computationally intensive tiers. As a central component of the pipeline, we created the fully automated Detached Eclipsing Binary Light curve fitter (DEBiL), which rapidly fits large numbers of light curves to a simple model. Using the results of DEBiL, light curves of interest can be flagged for follow-up analysis. As a test case, we analyzed the 218,699 light curves within the bulge fields of the OGLE II survey and produced 10,862 model fits. We point out a small number of extreme examples, as well as unexpected structure found in several of the population distributions. We expect this approach to become increasingly important as light-curve data sets continue growing in both size and number. |
| Author | Devor, Jonathan |
| Author_xml | – sequence: 1 fullname: Devor, Jonathan |
| BackLink | http://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=17038835$$DView record in Pascal Francis |
| BookMark | eNpl0ctKAzEUBuAgCtbbM8SFLsTRZHKbWdpatVAQ1IK7kEkyNRInYzJd-PbO2GJBV4fD-fgX_zkAu01oLAAnGF1hVPBrSjAWaAeMMCNFRgkTu2CEEKIZJ-J1Hxyk9D6seVmOwNNz8KvOhSbBOkSI0WV_glPtXZtcs4Rj16jobIKugd2bheOVX1p456w3CYYaPt7Pp3A2g4sffTsdu_kR2KuVT_Z4Mw_B4m76MnnI5o_3s8nNPNNEiC7DDGvOhKkKgYQlOeO0qojRSjGsSluYilqOKmZKVSFtNOcIlYYyU3GBclqSQ3C-zm1j-FzZ1MkPl7T1XjU2rJLEgrAcU9rDsw1USStfR9Vol2Qb3YeKX71DpCgI2wbqGFKKtt4SJIdq5braHl7-gdp1amixi8r5__xizV1ofyOHD8jhIZLnhcSSYixbU_f49D_-E_gNIjiOyg |
| CODEN | ASJOAB |
| CitedBy_id | crossref_primary_10_1086_527460 crossref_primary_10_1088_2041_8205_756_2_L39 crossref_primary_10_1093_mnras_stw2262 crossref_primary_10_1016_j_newast_2022_101875 crossref_primary_10_1086_592080 crossref_primary_10_1088_1538_3873_aa682a crossref_primary_10_1088_0004_637X_691_1_342 crossref_primary_10_1086_591783 crossref_primary_10_1088_0004_6256_135_3_850 crossref_primary_10_1088_0004_637X_761_2_123 crossref_primary_10_3847_1538_3881_ab7449 crossref_primary_10_1017_S1743921307004061 crossref_primary_10_1051_eas_0829001 crossref_primary_10_1111_j_1365_2966_2006_10764_x crossref_primary_10_1111_j_1365_2966_2006_10050_x crossref_primary_10_3847_1538_4365_acda31 crossref_primary_10_1016_j_newast_2008_12_002 crossref_primary_10_1093_mnras_stu578 crossref_primary_10_1007_s10511_017_9462_0 crossref_primary_10_1086_506157 crossref_primary_10_3847_1538_3881_153_3_118 crossref_primary_10_1088_0004_637X_797_1_22 crossref_primary_10_1093_mnras_stab389 crossref_primary_10_3847_2515_5172_aacf01 crossref_primary_10_1088_0067_0049_194_2_27 crossref_primary_10_1051_0004_6361_201321317 crossref_primary_10_1088_1674_4527_17_2_15 crossref_primary_10_1086_521702 crossref_primary_10_1017_S1743921309031810 crossref_primary_10_1093_mnras_stw2079 crossref_primary_10_1088_0004_6256_142_2_52 crossref_primary_10_3847_1538_4357_835_2_251 crossref_primary_10_1093_mnras_stv1790 crossref_primary_10_1111_j_1365_2966_2006_10049_x crossref_primary_10_1093_mnras_staa1587 crossref_primary_10_3390_galaxies12030030 crossref_primary_10_1086_523881 crossref_primary_10_3847_1538_4365_ab6bdb crossref_primary_10_1093_mnras_stt675 crossref_primary_10_1093_mnras_stw2282 crossref_primary_10_1109_TSP_2012_2204260 crossref_primary_10_1051_0004_6361_202349079 crossref_primary_10_3847_1538_4365_aad8a9 crossref_primary_10_1088_0004_6256_141_5_166 crossref_primary_10_1007_s10509_006_9155_3 crossref_primary_10_3847_1538_4365_aaec0c crossref_primary_10_1086_508609 crossref_primary_10_1017_S1743921311026809 crossref_primary_10_1088_0004_6256_148_6_125 crossref_primary_10_1051_0004_6361_201118425 crossref_primary_10_1093_mnras_stx3291 crossref_primary_10_1086_521579 crossref_primary_10_1016_j_ascom_2016_05_006 crossref_primary_10_1086_462405 crossref_primary_10_1086_517994 crossref_primary_10_1093_mnras_stz926 crossref_primary_10_1111_j_1365_2966_2012_21338_x crossref_primary_10_3847_1538_3881_153_3_104 crossref_primary_10_1088_0004_6256_150_1_27 crossref_primary_10_3847_1538_3881_aaa435 crossref_primary_10_1111_j_1365_2966_2011_18345_x crossref_primary_10_1017_S1743921308026598 crossref_primary_10_1088_1742_6596_118_1_012064 crossref_primary_10_5140_JASS_2006_23_4_311 crossref_primary_10_1051_0004_6361_201321817 crossref_primary_10_1134_S1063773721020043 crossref_primary_10_1051_0004_6361_201219815 crossref_primary_10_3847_0004_6256_152_6_193 crossref_primary_10_1088_0004_637X_796_2_114 crossref_primary_10_1093_mnras_stw880 crossref_primary_10_1051_0004_6361_201322871 crossref_primary_10_1093_mnras_stt1863 crossref_primary_10_1111_j_1365_2966_2008_14074_x crossref_primary_10_1093_mnras_stac2520 crossref_primary_10_1093_mnras_stv2145 crossref_primary_10_1002_asna_200510654 crossref_primary_10_1088_0004_6256_146_4_101 |
| Cites_doi | 10.1007/BF00639144 10.1086/378058 10.1007/978-94-011-2502-4 10.7551/mitpress/1090.001.0001 10.1086/192242 10.1117/12.456772 10.1086/164140 10.1126/science.293.5537.2037 10.1086/133944 10.1086/382735 10.1086/305984 10.1086/301321 10.1086/346105 10.1086/338691 10.1086/425256 10.1086/112862 10.1051/0004-6361:20040549 10.1086/151524 10.1086/322378 10.1086/150986 10.1086/133464 10.1086/309985 10.1007/978-1-4613-1627-5 10.1086/186602 10.1086/301272 10.1086/344709 10.1016/0021-9991(84)90095-0 10.1051/0004-6361:20030142 10.1117/12.457365 10.1086/300235 10.1086/305017 10.1093/mnras/241.2.153 10.1111/j.1365-2966.2004.07482.x 10.1086/339877 10.1126/science.220.4598.671 10.1086/157581 10.1093/comjnl/7.4.308 10.1086/157588 |
| ContentType | Journal Article |
| Copyright | 2005 INIST-CNRS |
| Copyright_xml | – notice: 2005 INIST-CNRS |
| DBID | AAYXX CITATION IQODW 7TG KL. |
| DOI | 10.1086/431170 |
| DatabaseName | CrossRef Pascal-Francis Meteorological & Geoastrophysical Abstracts Meteorological & Geoastrophysical Abstracts - Academic |
| DatabaseTitle | CrossRef Meteorological & Geoastrophysical Abstracts - Academic Meteorological & Geoastrophysical Abstracts |
| DatabaseTitleList | Meteorological & Geoastrophysical Abstracts - Academic |
| DeliveryMethod | fulltext_linktorsrc |
| Discipline | Astronomy & Astrophysics Physics |
| EISSN | 1538-4357 |
| EndPage | 425 |
| ExternalDocumentID | 17038835 10_1086_431170 |
| GroupedDBID | 123 1JI 23N 2WC 4.4 85S 8RP AAGCD AAJIO AALHV ABFLS ABPTK ACGFS ACNCT ADKFC AEFHF AENEX AFDAS ALMA_UNASSIGNED_HOLDINGS ASPBG ATQHT AVWKF AZFZN CJUJL CS3 DZ EBS EJD F5P G8K IOP KOT MVM N5L O3W O43 OHT OK1 RIN RNS RPA SJN SY9 T37 TN5 VOH WH7 X ZY4 -DZ -~X 2FS 6J9 6TJ AAFWJ AAYXX ABDPE ABHWH ACBEA ACHIP ADACN AFPKN AKPSB CITATION CRLBU FRP GROUPED_DOAJ IJHAN M~E PJBAE TR2 WHG XOL XSW 41~ 6TS 9M8 ADIYS ADXHL AETEA AI. FA8 IQODW ROL VH1 YYP ZCG ZKB 7TG KL. |
| ID | FETCH-LOGICAL-c377t-151c657db8707e32564bb3dcaa51a9e8db4e60b5d9ab0cdc66009d45db6702493 |
| IEDL.DBID | IOP |
| ISSN | 0004-637X |
| IngestDate | Fri Jul 11 09:43:04 EDT 2025 Mon Jul 21 09:16:00 EDT 2025 Thu Apr 24 22:51:02 EDT 2025 Tue Jul 01 04:24:09 EDT 2025 Tue Nov 10 14:26:49 EST 2020 Mon May 13 14:49:18 EDT 2019 |
| IsDoiOpenAccess | false |
| IsOpenAccess | true |
| IsPeerReviewed | true |
| IsScholarly | true |
| Issue | 1 |
| Keywords | Eclipsing binary stars surveys binaries: eclipsing Galaxy: bulge Galaxy bulge stars: statistics |
| Language | English |
| License | CC BY 4.0 |
| LinkModel | DirectLink |
| MergedId | FETCHMERGED-LOGICAL-c377t-151c657db8707e32564bb3dcaa51a9e8db4e60b5d9ab0cdc66009d45db6702493 |
| Notes | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
| OpenAccessLink | https://iopscience.iop.org/article/10.1086/431170/pdf |
| PQID | 17352144 |
| PQPubID | 23462 |
| PageCount | 15 |
| ParticipantIDs | pascalfrancis_primary_17038835 crossref_primary_10_1086_431170 crossref_citationtrail_10_1086_431170 iop_primary_10_1086_431170 proquest_miscellaneous_17352144 |
| ProviderPackageCode | CITATION AAYXX |
| PublicationCentury | 2000 |
| PublicationDate | 2005-07-20 |
| PublicationDateYYYYMMDD | 2005-07-20 |
| PublicationDate_xml | – month: 07 year: 2005 text: 2005-07-20 day: 20 |
| PublicationDecade | 2000 |
| PublicationPlace | Chicago, IL |
| PublicationPlace_xml | – name: Chicago, IL |
| PublicationTitle | The Astrophysical journal |
| PublicationYear | 2005 |
| Publisher | IOP Publishing University of Chicago Press |
| Publisher_xml | – name: IOP Publishing – name: University of Chicago Press |
| References | Udalski A. (rf46_1741) 1994; 44 rf50_1745 rf11_1706 rf28_1723 rf31_1726 Etzel P. B. (rf17_1712) 1991; 45 rf18_1713 rf21_1716 rf29_1724 Udalski A. (rf47_1742) 2002; 52 rf20_1715 rf40_1735 rf48_1743 Gorda S. Y. (rf19_1714) 1998; 42 Nelder J. A. (rf30_1725) 1965; 7 rf38_1733 rf3_1698 rf32_1727 rf12_1707 Udalski A. (rf45_1740) 1997; 47 rf9_1704 rf41_1736 rf44_1739 rf27_1722 Popper D. M. (rf36_1731) 1981; 6 Schwarzenberg-Czerny A. (rf39_1734) 1989; 241 rf24_1719 rf53_1748 rf14_1709 rf25_1720 rf7_1702 rf34_1729 Alard C. (rf2_1697) 1997; 326 rf16_1711 rf23_1718 Beaulieu J. P. (rf8_1703) 1995; 299 rf43_1738 rf35_1730 rf33_1728 rf5_1700 rf49_1744 rf10_1705 rf4_1699 Duquennoy A. (rf15_1710) 1991; 248 rf13_1708 rf26_1721 rf42_1737 Wozniak P. R. (rf52_1747) 2002; 52 rf1_1696 Antonello E. (rf6_1701) 1980; 72 rf37_1732 rf22_1717 rf51_1746 rf54_1749 |
| References_xml | – ident: rf35_1730 – volume: 72 start-page: 359 year: 1980 ident: rf6_1701 publication-title: Ap&SS doi: 10.1007/BF00639144 – ident: rf25_1720 doi: 10.1086/378058 – volume: 52 start-page: 217 year: 2002 ident: rf47_1742 publication-title: Acta Astron. – ident: rf14_1709 doi: 10.1007/978-94-011-2502-4 – ident: rf16_1711 – ident: rf20_1715 doi: 10.7551/mitpress/1090.001.0001 – ident: rf9_1704 doi: 10.1086/192242 – ident: rf44_1739 doi: 10.1117/12.456772 – ident: rf33_1728 doi: 10.1086/164140 – volume: 44 start-page: 165 year: 1994 ident: rf46_1741 publication-title: Acta Astron. – ident: rf34_1729 – ident: rf43_1738 doi: 10.1126/science.293.5537.2037 – volume: 45 start-page: 25 year: 1991 ident: rf17_1712 publication-title: IAPPP Commun. – ident: rf28_1723 doi: 10.1086/133944 – ident: rf7_1702 doi: 10.1086/382735 – ident: rf3_1698 doi: 10.1086/305984 – ident: rf1_1696 doi: 10.1086/301321 – ident: rf38_1733 – ident: rf13_1708 – ident: rf41_1736 doi: 10.1086/346105 – ident: rf24_1719 doi: 10.1086/338691 – volume: 47 start-page: 319 year: 1997 ident: rf45_1740 publication-title: Acta Astron. – ident: rf5_1700 doi: 10.1086/425256 – volume: 42 start-page: 793 year: 1998 ident: rf19_1714 publication-title: Astron. Rep. – volume: 299 start-page: 168 year: 1995 ident: rf8_1703 publication-title: A&A – ident: rf37_1732 doi: 10.1086/112862 – volume: 52 start-page: 129 year: 2002 ident: rf52_1747 publication-title: Acta Astron. – ident: rf27_1722 doi: 10.1051/0004-6361:20040549 – ident: rf31_1726 doi: 10.1086/151524 – ident: rf53_1748 doi: 10.1086/322378 – ident: rf51_1746 doi: 10.1086/150986 – volume: 248 start-page: 485 year: 1991 ident: rf15_1710 publication-title: A&A – ident: rf50_1745 doi: 10.1086/133464 – ident: rf40_1735 doi: 10.1086/309985 – ident: rf32_1727 doi: 10.1007/978-1-4613-1627-5 – ident: rf12_1707 doi: 10.1086/186602 – ident: rf26_1721 doi: 10.1086/301272 – ident: rf29_1724 doi: 10.1086/344709 – volume: 6 start-page: 99 year: 1981 ident: rf36_1731 publication-title: Rev. Mex. AA – ident: rf48_1743 doi: 10.1016/0021-9991(84)90095-0 – ident: rf10_1705 doi: 10.1051/0004-6361:20030142 – ident: rf21_1716 doi: 10.1117/12.457365 – ident: rf22_1717 doi: 10.1086/300235 – ident: rf4_1699 doi: 10.1086/305017 – volume: 241 start-page: 153 year: 1989 ident: rf39_1734 publication-title: MNRAS doi: 10.1093/mnras/241.2.153 – ident: rf42_1737 doi: 10.1111/j.1365-2966.2004.07482.x – ident: rf54_1749 doi: 10.1086/339877 – ident: rf23_1718 doi: 10.1126/science.220.4598.671 – volume: 326 start-page: 1 year: 1997 ident: rf2_1697 publication-title: A&A – ident: rf18_1713 doi: 10.1086/157581 – ident: rf11_1706 – volume: 7 start-page: 308 year: 1965 ident: rf30_1725 publication-title: Comput. J. doi: 10.1093/comjnl/7.4.308 – ident: rf49_1744 doi: 10.1086/157588 |
| SSID | ssj0004299 |
| Score | 2.1536777 |
| SecondaryResourceType | review_article |
| Snippet | We have developed a fully automated pipeline for systematically identifying and analyzing eclipsing binaries within large data sets of light curves. The... |
| SourceID | proquest pascalfrancis crossref iop |
| SourceType | Aggregation Database Index Database Enrichment Source Publisher |
| StartPage | 411 |
| Title | Solutions for 10,000 Eclipsing Binaries in the Bulge Fields of OGLE II Using DEBiL |
| URI | http://iopscience.iop.org/0004-637X/628/1/411 https://www.proquest.com/docview/17352144 |
| Volume | 628 |
| hasFullText | 1 |
| inHoldings | 1 |
| isFullTextHit | |
| isPrint | |
| link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwjV3db9MwELfGpEm88LGB1gHDEhtPpHXixE4eV2i3om2dEBN9s_w5VYykIu0D_PWcnfSDVUK8RJZycqLz2fc73xdCJ2DgZNJKGinNXJRSA3uOFCSyecZcIqnSIUPu6ppd3KafJ9lknaw-rWbtyd-FYfDke9QRMconPZbkvbiXhkxe0Pze1BqNb9ZZkEnRgt2GfqOTEGjJ2Lcj3lA9j2B-Hwgpa-CFa5pYbJ3HQckMn6LrZapOE1vyvbuYq67-vV258f_-_xl60sJNfNbIx3O0Y8t9dHhW-wvw6scv_B6HcXO_Ue-jvZtmdIC-rC7MMOBaHJMP8Ak80N51AOoO930iL5jZeFpiAJG4v7i_s3joA-JqXDk8Pr8c4NEIh5gE_GnQn16-QLfDwdePF1HbgCHSlPN5BGhAs4wbBZuaW1hVlipFjZYyi2Vhc6NSy4jKTCEV0UYzQE-FSTOjGPelCOlLtFtWpT1EOFea5BwEIHYyTVyinCXcgTVjDTNEph10ulwbodvq5L5Jxr0IXvKciWYNO-jtim7W1OPYongHrF-99OwXnv0C2C9iAewXM-M66GiT6uEUx3_JxZqM--I5NIO_WAqKgO3ofSyytNWiBgpAtGCkHv1r_lfocagASzgcUq_R7vznwr4BbDNXx0Gk4Tmm3_4AXlvu-w |
| linkProvider | IOP Publishing |
| linkToPdf | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwfV1bb9MwFLa2IRAvEwzQusFmicsTYU58Sx5X1rJC2SbERN8sX9GkkVSkfeDfcxyn3cYk3izlxLHOF_tcfC4IvQEDh2uvaWasCBmjDvYcqUjmSy5CoamxXYbc1zNxesk-z_hsA_F1Lkwz74_-DzBMhYITC49WbYFA5OWSHM1d2EQPOJVFLJl_Tn_cpEMWVa_1skxQObvVUii9e0cGbcJ3YkSkboEpIXWzuHcwd9Jm_ARt92oiPk6Leoo2fL2Ddo_b6Lhufv3B73A3Tn6Jdgc9vEijZ-jb2tGFQR_FOXkPK8QjG13-IKbwMCbggnmMr2oMyh8eLq9_ejyOgWwtbgI-_zQd4ckEd7EE-GQ0vJo-R5fj0fePp1nfOCGzVMpFBlLcCi6dgc0oPaAhmDHUWa15ritfOsO8IIa7ShtinRWg9VSOcWeEjCUE6Qu0VTe130W4NJaUEoDLg2ZFKEzwRAawQrwTjmg2QG9XrFS2ryoem1tcq-52uxQqsXyADtd081RH4x7Fa0Bi_TCipyJ6ShSlyhUDQwUgH6C921T_TnFwB8YbMhmL3lAOq1jhqmAbxbsRXftm2QIFaKJgXO79b_5D9OjiZKymk7Mv--hxV8SVSDhnXqKtxe-lfwXqycIcdD_jX8XI2mw |
| openUrl | ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Solutions+for+10%2C000+Eclipsing+Binaries+in+the+Bulge+Fields+of+OGLE+II+Using+DEBiL&rft.jtitle=The+Astrophysical+journal&rft.au=Devor%2C+Jonathan&rft.date=2005-07-20&rft.pub=IOP+Publishing&rft.issn=0004-637X&rft.eissn=1538-4357&rft.volume=628&rft.spage=411&rft_id=info:doi/10.1086%2F431170&rft.externalDBID=n%2Fa&rft.externalDocID=10_1086_431170 |
| thumbnail_l | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0004-637X&client=summon |
| thumbnail_m | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0004-637X&client=summon |
| thumbnail_s | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0004-637X&client=summon |