Poster Open Access
Emma Esparza-Borges;
Mahmoudreza Oshagh;
Núria Casasayas-Barris;
Enric Pallé
<?xml version='1.0' encoding='utf-8'?> <resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd"> <identifier identifierType="DOI">10.5281/zenodo.5553440</identifier> <creators> <creator> <creatorName>Emma Esparza-Borges</creatorName> <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-2341-3233</nameIdentifier> <affiliation>Instituto de Astrofísica de Canarias</affiliation> </creator> <creator> <creatorName>Mahmoudreza Oshagh</creatorName> <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-0715-8789</nameIdentifier> <affiliation>Instituto de Astrofísica de Canarias</affiliation> </creator> <creator> <creatorName>Núria Casasayas-Barris</creatorName> <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-2891-8222</nameIdentifier> <affiliation>Leiden Observatory</affiliation> </creator> <creator> <creatorName>Enric Pallé</creatorName> <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0003-0987-1593</nameIdentifier> <affiliation>Instituto de Astrofísica de Canarias</affiliation> </creator> </creators> <titles> <title>CHOCOLATE: a new Chromatic Line-Profile Tomography Technique to retrieve Transmission Spectroscopy</title> </titles> <publisher>Zenodo</publisher> <publicationYear>2021</publicationYear> <dates> <date dateType="Issued">2021-10-06</date> </dates> <resourceType resourceTypeGeneral="Text">Poster</resourceType> <alternateIdentifiers> <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5553440</alternateIdentifier> </alternateIdentifiers> <relatedIdentifiers> <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5553439</relatedIdentifier> <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/plato2021</relatedIdentifier> </relatedIdentifiers> <rightsList> <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights> <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights> </rightsList> <descriptions> <description descriptionType="Abstract"><p>Multi-band&nbsp;photometric&nbsp;transit&nbsp;observations&nbsp;or&nbsp;low&nbsp;resolution&nbsp;spectroscopy&nbsp;(spectro-photometry)&nbsp;are&nbsp;normally&nbsp;used&nbsp;to&nbsp;retrieve&nbsp;the&nbsp;broadband&nbsp;transmission&nbsp;spectra&nbsp;of&nbsp;transiting&nbsp;exoplanets&nbsp;in&nbsp;order&nbsp;to&nbsp;assess&nbsp;the&nbsp;chemical&nbsp;composition&nbsp;of&nbsp;their&nbsp;atmospheres.&nbsp;Here,&nbsp;we&nbsp;present&nbsp;an&nbsp;alternative&nbsp;approach&nbsp;for&nbsp;recovering&nbsp;the&nbsp;broadband&nbsp;transmission&nbsp;spectra&nbsp;using&nbsp;chromatic&nbsp;Doppler&nbsp;Tomography.&nbsp;To&nbsp;validate&nbsp;the&nbsp;method&nbsp;and&nbsp;examine&nbsp;its&nbsp;performance,&nbsp;we&nbsp;used&nbsp;new&nbsp;observational&nbsp;data&nbsp;obtained&nbsp;with&nbsp;the&nbsp;ESPRESSO&nbsp;instrument&nbsp;to&nbsp;retrieve&nbsp;the<br> transmission&nbsp;spectra&nbsp;of&nbsp;the&nbsp;archetypal&nbsp;hot&nbsp;Jupiter&nbsp;HD209458b.&nbsp;Our&nbsp;findings&nbsp;indicate&nbsp;that&nbsp;the&nbsp;recovered&nbsp;transmission&nbsp;spectrum&nbsp;is&nbsp;in&nbsp;good&nbsp;agreement&nbsp;with&nbsp;the&nbsp;results&nbsp;presented&nbsp;in&nbsp;previous&nbsp;studies,&nbsp;which&nbsp;used&nbsp;different&nbsp;methodologies&nbsp;to&nbsp;extract&nbsp;the&nbsp;spectrum.</p></description> </descriptions> </resource>
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