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xmlns:vodm="http://www.ivoa.net/xml/DataModel/v1" xmlns:voe="http://www.ivoa.net/xml/VOEventRegExt/v2" xmlns:vosi10="http://www.ivoa.net/xml/VOSITables/v1.0" xmlns:vot="http://www.ivoa.net/xml/VOTable/v1.2" xmlns:vot0="http://www.ivoa.net/xml/VOTable/v1.3" xmlns:vot1="http://www.ivoa.net/xml/VOTable/v1.1" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vr0="https://www.ivoa.net/xml/VOResource/v1.0" xmlns:vr1="http://www.ivoa.net/xml/VOResource/v1.1" xmlns:vr2="http://Www.ivoa.net/xml/VOResource/v1.0" xmlns:vr3="http://www.ivoa.net/xml/VOResource/v1%20.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:vs0="http://www.ivoa.net/xml/VODataService/v1.0" xmlns:vs1="https://www.ivoa.net/xml/VODataService/v1.0" xmlns:vstd="http://www.ivoa.net/xml/StandardsRegExt/v1.0" xmlns:xdtn="http://www.w3.org/2004/07/xpath-datatypes" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xlink0="https://www.w3.org/1999/xlink" xmlns:xsd="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:xsi0="https://www.w3.org/2001/XMLSchema-instance" xmlns:xu="http://www.xmldb.org/xupdate"><oai:identifier>ivo://CDS.VizieR/J/A+A/707/A20</oai:identifier><oai:datestamp>2026-03-02T00:34:06Z</oai:datestamp><oai:setSpec>J.A_A</oai:setSpec></oai:header><oai:metadata><eudc:resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:eudc="http://schema.eudat.eu/schema/kernel-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:oai="http://www.openarchives.org/OAI/2.0/" xmlns:dachs="urn:dachs" xsi:schemaLocation="http://schema.eudat.eu/schema/kernel-1           http://docs.g-vo.org/schemata/eudat-core.xsd"><eudc:community>IVOA</eudc:community><eudc:titles><eudc:title>NGC 1068 vel.-int. intensities and luminosities</eudc:title></eudc:titles><eudc:descriptions><eudc:description>We investigated the interplay between dense molecular gas, star formation, and active galactic nucleus (AGN) feedback in the luminous IR galaxy NGC 1068 at sub-kiloparsec scales. We present the HCN (4-3) and HCO+ (4-3) maps of NGC 1068 obtained with JCMT as part of the Mapping the dense molecular gas in the strongest star-forming galaxies (MALATANG) project, and perform spatially resolved analyses of their correlations with IR luminosity and soft X-ray emission. The spatially resolved relations between the luminosities of IR dust emission and dense molecular gas tracers (LIR-L'dense) are found to be nearly linear, without clear evidence of excess contributions from AGN activity. The spatially resolved X-ray emission (L^gas^_0.5-2KeV_) displays a radially dependent twofold correlation with the star formation rate (SFR), suggesting distinct gas-heating mechanisms are at play in areas between the galaxy center and the outer regions. A super-linear scaling is obtained in galactic center regions with SFR surface densities ({SIGMA}SFR)&gt;8.2x10^-6^M_{sun}/yr/kpc^2^:log(L^gas^_0.5-2KeV_/erg/s) = 2.2log(SFR/M_{sun}/yr)+39.1. We further find a statistically significant super-linear correlation (beta=1.34+/-0.86) between L^gas^_0.5-2KeV_/SFR and the HCN(4-3)/CO(1-0) intensity ratio, whereas no such trend is seen for HCO+(4-3)/CO(1-0) or CO(3-2)/CO(1-0). These findings indicate that AGN feedback does not dominate star formation regulation on sub-kiloparsec scales, and that the excitation of dense gas traced by HCN (4-3) may be more directly influenced by high-energy feedback processes compared to HCO+ (4-3) and CO (3-2).</eudc:description></eudc:descriptions><eudc:keywords><eudc:keyword>active-galactic-nuclei</eudc:keyword><eudc:keyword>interstellar-medium</eudc:keyword><eudc:keyword>millimeter-astronomy</eudc:keyword><eudc:keyword>submillimeter-astronomy</eudc:keyword><eudc:keyword>spectroscopy</eudc:keyword><eudc:keyword>galactic-and-extragalactic-astronomy</eudc:keyword><eudc:keyword>high-energy-astrophysics</eudc:keyword><eudc:keyword>observational-astronomy</eudc:keyword><eudc:keyword>interdisciplinary-astronomy</eudc:keyword></eudc:keywords><eudc:identifiers><eudc:identifier identifierType="URL">https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/707/A20</eudc:identifier></eudc:identifiers><eudc:relatedIdentifiers><eudc:relatedIdentifier relatedIdentifierType="URL">https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/707/A20</eudc:relatedIdentifier><eudc:relatedIdentifier relatedIdentifierType="bibcode">2026A&amp;A...707A..20L</eudc:relatedIdentifier><eudc:relatedIdentifier relatedIdentifierType="URL">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/707/A20</eudc:relatedIdentifier><eudc:description>Cone search capability for table J/A+A/707/A20/tablea1 (*Velocity-integrated intensities and luminosities of NGC 1068 at sub kpc scale)</eudc:description></eudc:relatedIdentifiers><eudc:creators><eudc:creator><eudc:creatorName>Lin S.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Feng S.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Zhang Z.-Y.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Zhang C.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Tan Q.-H.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Wang J.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Gao Y.,Jiang X.-J.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Gao Y.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Wang X.-L.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Wang J.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Wang J.-F.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Matsushita S.,Chung A.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Kohno K.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Tomoka T.</eudc:creatorName></eudc:creator><eudc:creator><eudc:creatorName>Greve R.T.</eudc:creatorName></eudc:creator></eudc:creators><eudc:publishers><eudc:publisher>CDS</eudc:publisher></eudc:publishers><eudc:instruments/><eudc:publicationYear>2026</eudc:publicationYear><eudc:rightsList><eudc:rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</eudc:rights></eudc:rightsList><eudc:fundingReferences/><eudc:contacts><eudc:contact>CDS support team &lt;cds-question@unistra.fr&gt;</eudc:contact></eudc:contacts><eudc:resourceTypes><eudc:resourceType>Dataset</eudc:resourceType><eudc:resourceType>AstroObjects</eudc:resourceType></eudc:resourceTypes><eudc:disciplines><eudc:discipline>astronomy</eudc:discipline></eudc:disciplines></eudc:resource></oai:metadata></oai:record></oai:GetRecord></oai:OAI-PMH>