Optimum repetition rates for dual-comb spectroscopy
The determination of the properties (i.e. line center, width, and amplitude) of a spectral line is simulated using a Monte Carlo method. For dual-comb spectroscopy, ideal repetition rates emerge for both the signal and LO combs that do not correspond to the repetition rates that possess the highest...
Gespeichert in:
Veröffentlicht in: | Optics express 2018-04, Vol.26 (9), p.12049-12056 |
---|---|
Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 12056 |
---|---|
container_issue | 9 |
container_start_page | 12049 |
container_title | Optics express |
container_volume | 26 |
creator | Smith, Brad C Lomsadze, Bachana Cundiff, Steven T |
description | The determination of the properties (i.e. line center, width, and amplitude) of a spectral line is simulated using a Monte Carlo method. For dual-comb spectroscopy, ideal repetition rates emerge for both the signal and LO combs that do not correspond to the repetition rates that possess the highest signal-to-noise ratio. The determination is even more accurate when the repetition rates have an arbitrary near-harmonic ratio. The simulation results are generalized to allow for the comparison of any two spectroscopic systems (i.e. not just comb-based systems) by performing the simulations as a function of the spectral point spacing and signal-to-noise ratio of the acquired data. |
doi_str_mv | 10.1364/OE.26.012049 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_2033377166</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2033377166</sourcerecordid><originalsourceid>FETCH-LOGICAL-c372t-729e9a9476db4d0d4008d43027c7c7f6e9fd9bf1675a9ce2d512bcf4fc4a078d3</originalsourceid><addsrcrecordid>eNpNkDtPwzAURi0EoqWwMaOMDKRcP2rHI6rCQ6qUBWbL8UMKSupgO0P_PUEtCN3hu8PRp3sPQrcY1phy9tjUa8LXgAkweYaWGCQrGVTi_N--QFcpfQJgJqS4RAsiBeaY4CWizZi7YRqK6EaXu9yFfRF1dqnwIRZ20n1pwtAWaXQmx5BMGA_X6MLrPrmbU67Qx3P9vn0td83L2_ZpVxoqSC4FkU5qyQS3LbNgGUBlGQUizDyeO-mtbD3mYqOlccRuMGmNZ94wDaKydIXuj71jDF-TS1kNXTKu7_XehSkpApRSMX_CZ_ThiJr5xhSdV2PsBh0PCoP60aSaWhGujppm_O7UPLWDs3_wrxf6DXe1YhU</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2033377166</pqid></control><display><type>article</type><title>Optimum repetition rates for dual-comb spectroscopy</title><source>DOAJ Directory of Open Access Journals</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>Smith, Brad C ; Lomsadze, Bachana ; Cundiff, Steven T</creator><creatorcontrib>Smith, Brad C ; Lomsadze, Bachana ; Cundiff, Steven T</creatorcontrib><description>The determination of the properties (i.e. line center, width, and amplitude) of a spectral line is simulated using a Monte Carlo method. For dual-comb spectroscopy, ideal repetition rates emerge for both the signal and LO combs that do not correspond to the repetition rates that possess the highest signal-to-noise ratio. The determination is even more accurate when the repetition rates have an arbitrary near-harmonic ratio. The simulation results are generalized to allow for the comparison of any two spectroscopic systems (i.e. not just comb-based systems) by performing the simulations as a function of the spectral point spacing and signal-to-noise ratio of the acquired data.</description><identifier>ISSN: 1094-4087</identifier><identifier>EISSN: 1094-4087</identifier><identifier>DOI: 10.1364/OE.26.012049</identifier><identifier>PMID: 29716121</identifier><language>eng</language><publisher>United States</publisher><ispartof>Optics express, 2018-04, Vol.26 (9), p.12049-12056</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c372t-729e9a9476db4d0d4008d43027c7c7f6e9fd9bf1675a9ce2d512bcf4fc4a078d3</citedby><cites>FETCH-LOGICAL-c372t-729e9a9476db4d0d4008d43027c7c7f6e9fd9bf1675a9ce2d512bcf4fc4a078d3</cites><orcidid>0000-0002-7145-9498 ; 0000-0002-7119-5197</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,777,781,861,27905,27906</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/29716121$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Smith, Brad C</creatorcontrib><creatorcontrib>Lomsadze, Bachana</creatorcontrib><creatorcontrib>Cundiff, Steven T</creatorcontrib><title>Optimum repetition rates for dual-comb spectroscopy</title><title>Optics express</title><addtitle>Opt Express</addtitle><description>The determination of the properties (i.e. line center, width, and amplitude) of a spectral line is simulated using a Monte Carlo method. For dual-comb spectroscopy, ideal repetition rates emerge for both the signal and LO combs that do not correspond to the repetition rates that possess the highest signal-to-noise ratio. The determination is even more accurate when the repetition rates have an arbitrary near-harmonic ratio. The simulation results are generalized to allow for the comparison of any two spectroscopic systems (i.e. not just comb-based systems) by performing the simulations as a function of the spectral point spacing and signal-to-noise ratio of the acquired data.</description><issn>1094-4087</issn><issn>1094-4087</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNpNkDtPwzAURi0EoqWwMaOMDKRcP2rHI6rCQ6qUBWbL8UMKSupgO0P_PUEtCN3hu8PRp3sPQrcY1phy9tjUa8LXgAkweYaWGCQrGVTi_N--QFcpfQJgJqS4RAsiBeaY4CWizZi7YRqK6EaXu9yFfRF1dqnwIRZ20n1pwtAWaXQmx5BMGA_X6MLrPrmbU67Qx3P9vn0td83L2_ZpVxoqSC4FkU5qyQS3LbNgGUBlGQUizDyeO-mtbD3mYqOlccRuMGmNZ94wDaKydIXuj71jDF-TS1kNXTKu7_XehSkpApRSMX_CZ_ThiJr5xhSdV2PsBh0PCoP60aSaWhGujppm_O7UPLWDs3_wrxf6DXe1YhU</recordid><startdate>20180430</startdate><enddate>20180430</enddate><creator>Smith, Brad C</creator><creator>Lomsadze, Bachana</creator><creator>Cundiff, Steven T</creator><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><orcidid>https://orcid.org/0000-0002-7145-9498</orcidid><orcidid>https://orcid.org/0000-0002-7119-5197</orcidid></search><sort><creationdate>20180430</creationdate><title>Optimum repetition rates for dual-comb spectroscopy</title><author>Smith, Brad C ; Lomsadze, Bachana ; Cundiff, Steven T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c372t-729e9a9476db4d0d4008d43027c7c7f6e9fd9bf1675a9ce2d512bcf4fc4a078d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Smith, Brad C</creatorcontrib><creatorcontrib>Lomsadze, Bachana</creatorcontrib><creatorcontrib>Cundiff, Steven T</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>Optics express</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Smith, Brad C</au><au>Lomsadze, Bachana</au><au>Cundiff, Steven T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Optimum repetition rates for dual-comb spectroscopy</atitle><jtitle>Optics express</jtitle><addtitle>Opt Express</addtitle><date>2018-04-30</date><risdate>2018</risdate><volume>26</volume><issue>9</issue><spage>12049</spage><epage>12056</epage><pages>12049-12056</pages><issn>1094-4087</issn><eissn>1094-4087</eissn><abstract>The determination of the properties (i.e. line center, width, and amplitude) of a spectral line is simulated using a Monte Carlo method. For dual-comb spectroscopy, ideal repetition rates emerge for both the signal and LO combs that do not correspond to the repetition rates that possess the highest signal-to-noise ratio. The determination is even more accurate when the repetition rates have an arbitrary near-harmonic ratio. The simulation results are generalized to allow for the comparison of any two spectroscopic systems (i.e. not just comb-based systems) by performing the simulations as a function of the spectral point spacing and signal-to-noise ratio of the acquired data.</abstract><cop>United States</cop><pmid>29716121</pmid><doi>10.1364/OE.26.012049</doi><tpages>8</tpages><orcidid>https://orcid.org/0000-0002-7145-9498</orcidid><orcidid>https://orcid.org/0000-0002-7119-5197</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1094-4087 |
ispartof | Optics express, 2018-04, Vol.26 (9), p.12049-12056 |
issn | 1094-4087 1094-4087 |
language | eng |
recordid | cdi_proquest_miscellaneous_2033377166 |
source | DOAJ Directory of Open Access Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
title | Optimum repetition rates for dual-comb spectroscopy |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-21T04%3A19%3A20IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Optimum%20repetition%20rates%20for%20dual-comb%20spectroscopy&rft.jtitle=Optics%20express&rft.au=Smith,%20Brad%20C&rft.date=2018-04-30&rft.volume=26&rft.issue=9&rft.spage=12049&rft.epage=12056&rft.pages=12049-12056&rft.issn=1094-4087&rft.eissn=1094-4087&rft_id=info:doi/10.1364/OE.26.012049&rft_dat=%3Cproquest_cross%3E2033377166%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2033377166&rft_id=info:pmid/29716121&rfr_iscdi=true |