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<ri:Resource created="2009-11-22T17:03:44Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Mock spectro-photometric catalog of galaxies</title><shortName>J/A+A/504/359</shortName><identifier>ivo://CDS.VizieR/J/A+A/504/359</identifier><altIdentifier>doi:10.26093/cds/vizier.35040359</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jouvel S.</name></creator><creator><name>Kneib J-P</name></creator><creator><name>Ilbert O.</name></creator><creator><name>Bernstein G.</name></creator><creator><name>Arnouts S.</name></creator><creator><name>Dahlen T.,Ealet A.</name></creator><creator><name>Milliard B.</name></creator><creator><name>Aussel H.</name></creator><creator><name>Capak P.</name></creator><creator><name>Le Brun V.</name></creator><creator><name>McCracken H.,Capak P.</name></creator><creator><name>Salvato M.</name></creator><creator><name>Scoville N.</name></creator><date role="Updated">2017-06-21T08:21:43Z</date><date role="Created">2009-11-22T17:03:44Z</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>astronomical-models</subject><subject>photometry</subject><subject>spectroscopy</subject><description>Future dark energy space missions such as JDEM and EUCLID are being designed to survey the galaxy population to trace the geometry of the universe and the growth of structure, which both depend on the cosmological model. To reach the goal of high precision cosmology they need to evaluate the capabilities of different instrument designs based on realistic mock catalog. The aim of this paper is to construct realistic and flexible mock catalogs based on our knowledge of galaxy population from current deep surveys. We explore two categories of mock catalog : (i) based on luminosity functions fit of observations (GOODS, UDF, COSMOS, VVDS) using the Le Phare software (ii) based on the observed COSMOS galaxy distribution which benefits from all the properties of the data-rich COSMOS survey. For these two catalogs, we have produced simulated number counts in several bands, color diagrams and redshift distribution for validation against real observational data. We also derive some basic requirements to help designing future Dark Energy mission in terms of number of galaxies available for the weak-lensing analysis as a function of the PSF size and depth of the survey. We also compute the spectroscopic success rate for future spectroscopic redshift surveys (i) aiming at measuring BAO in the case of the wide field spectroscopic redshift survey, and (ii) for the photometric redshift calibration survey which is required to achieve weak lensing tomography with great accuracy. They will be publicly accessible at http://lamwws.oamp.fr/cosmowiki/RealisticSpectroPhotCat, or by request to the first author of this paper.</description><source format="bibcode">2009A&amp;A...504..359J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/504/359</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/258">II/258 : Hubble Ultra Deep Field Catalog (UDF) (STScI, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/261">II/261 : GOODS initial results (Giavalisco+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/286">II/286 : VIRMOS deep imaging survey. VVDS-F02 catalog (VIRMOSteam, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/449/951">J/A+A/449/951 : GOODS-MUSIC sample: multicolour catalog (Grazian+, 2006)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/504/359</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/504/359</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/504/359</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/504/359</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/504/359</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/504/359</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/504/359/glfc</name><description>GOODS Luminosity Function based catalog of mock galaxies (magnitudes in AB system)</description><column><name>Seq</name><description>[1,641785] Sequential number</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>z</name><description>[0.02,6] Redshift bin</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mod</name><description>[1,66] Model of galaxy (G1)</description><ucd>stat.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LF</name><description>[1,3] Luminosity Function (2)</description><ucd>phys.luminosity.fun</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>M*</name><description>M* Luminosity Function parameter (3)</description><unit>mag</unit><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>phi*</name><description>{phi}^*^ Luminosity Function parameter (3)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>alpha</name><description>{alpha} Luminosity Function parameter (3)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F435W</name><description>[16,105] Theoretical magnitude in F435W band</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F435W</name><description>?=-1 Errors on magnitude in F435W band</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F606W</name><description>[15,33] Theoretical magnitude in F606W band</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F606W</name><description>? 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xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FHb</name><description>[-99.9,0.04] Theoretical flux in Hb</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FcHb</name><description>[-99.9,4.03e-14] Continuum flux in Hb</description><unit>mW.m**-2.Hz**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lOIIIa</name><description>[-99.9,34713] Wavelength in OIII(4959)</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FOIIIa</name><description>[-99.9,0.008] Theoretical flux in OIII(4959)</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FcOIIIa</name><description>[-99.9,4.2e-14] Continuum flux in OIII(4959)</description><unit>mW.m**-2.Hz**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lOIIIb</name><description>[-99.9,35049] Wavelength in OIII(5007)</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FOIIIb</name><description>[-99.9,0.03] Theoretical flux in OIII(5007)</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FcOIIIb</name><description>[-99.9,4.2e-14] Continuum flux in OIII(5007)</description><unit>mW.m**-2.Hz**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>lHa</name><description>[-99.9,45941] Wavelength in H{alpha}</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FHa</name><description>[-99.9,0.13] Theoretical flux in Ha</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FcHa</name><description>[-99.9,0.8e-13] Continuum flux in Ha</description><unit>mW.m**-2.Hz**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FHbr</name><description>[-106,0.03] Randomized flux in Ly</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FOIIIar</name><description>[-431.06,0.02] Randomized flux in OIII(4959)</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FOIIIbr</name><description>[-332.855,0.04] Randomized flux in OIII(5007)</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FHar</name><description>[-114.779,0.10] Randomized flux in Ha</description><unit>mW.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>