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<ri:Resource created="2021-09-13T09:30:10Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>X-ray &amp; MIR luminosities of the GBT galaxies</title><shortName>J/ApJ/892/18</shortName><identifier>ivo://CDS.VizieR/J/ApJ/892/18</identifier><altIdentifier>doi:10.26093/cds/vizier.18920018</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kuo C.Y.</name></creator><creator><name>Hsiang J.Y.</name></creator><creator><name>Chung H.H.</name></creator><creator><name>Constantin A.</name></creator><creator><name>Chang Y.-Y.</name></creator><creator><name>da Cunha E.,Pesce D.</name></creator><creator><name>Chien W.T.</name></creator><creator><name>Chen B.Y.</name></creator><creator><name>Braatz J.A.</name></creator><creator><name>Zaw I.</name></creator><creator><name>Matsushita S.,Lin J.C.</name></creator><date role="Updated">2022-01-19T08:55:44Z</date><date role="Created">2021-09-13T09:30:10Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>active-galactic-nuclei</subject><subject>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>x-ray-sources</subject><subject>radio-sources</subject><subject>infrared-astronomy</subject><subject>redshifted</subject><description>We present an investigation of the dependence of H_2_O maser detection rates and properties on the mid-IR active galactic nucleus (AGN) luminosity, L_AGN_, and the obscuring column density, N_H_, based on mid-IR and hard X-ray photometry. Based on spectral energy distribution fitting that allows for decomposition of the black hole accretion and star formation components in the mid-infrared, we show that the megamaser (disk maser) detection rate increases sharply for galaxies with 12{mu}m AGN luminosity L_12um_^AGN^ greater than 10^42^erg/s, from &lt;~3% (&lt;~2%) to ~12% (~5%). By using the ratio of the observed X-ray to mid-IR AGN luminosity as an indicator of N_H_, we also find that megamaser (disk maser) detection rates are boosted to 15% (7%) and 20% (9%) for galaxies with N_H_&gt;=10^23^/cm^2^ and N_H_&gt;=10^24^cm^-2^, respectively. Combining these column density cuts with a constraint for high L_12um_^AGN^ (&gt;=10^42^erg/s) predicts further increases in the megamaser (disk maser) detection rates to 19% (8%) and 27% (14%), revealing unprecedented potential increases of the megamaser and disk maser detection rates by a factor of 7-15 relative to the current rates, depending on the chosen sample selection criteria. A noteworthy aspect of these new predictions is that the completeness rates are only compromised mildly, with the rates remaining at the level of ~95% (~50%) for sources with N_H_&gt;=10^23^/cm^2^ (N_H_&gt;=10^24^/cm^2^). Applying these selection methods to current X-ray AGN surveys predicts the detection of &gt;~15 new megamaser disks.</description><source format="bibcode">2020ApJ...892...18K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/892/18</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/xmm">B/xmm : XMM-Newton Obs. 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