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<ri:Resource created="2014-11-05T09:11:53Z" 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>Chandra Local Volume Survey: NGC 404 sources</title><shortName>J/ApJ/763/128</shortName><identifier>ivo://CDS.VizieR/J/ApJ/763/128</identifier><altIdentifier>doi:10.26093/cds/vizier.17630128</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Binder B.</name></creator><creator><name>Williams B.F.</name></creator><creator><name>Eracleous M.</name></creator><creator><name>Gaetz T.J.</name></creator><creator><name>Kong A.K.H.,Skillman E.D.</name></creator><creator><name>Weisz D.R.</name></creator><date role="Updated">2017-07-12T15:35:06Z</date><date role="Created">2014-11-05T09:11:53Z</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>galaxies</subject><subject>x-ray-sources</subject><subject>hst-photometry</subject><subject>surveys</subject><subject>x-ray-binary-stars</subject><description>We present a comprehensive X-ray point-source catalog of NGC 404 obtained as part of the Chandra Local Volume Survey. A new 97ks Chandra ACIS-S observation of NGC 404 was combined with archival observations for a total exposure of ~123ks. Our survey yields 74 highly significant X-ray point sources and is sensitive to a limiting unabsorbed luminosity of ~6x10^35^erg/s in the 0.35-8keV band. To constrain the nature of each X-ray source, cross-correlations with multi-wavelength data were generated. We searched overlapping Hubble Space Telescope observations for optical counterparts to our X-ray detections, but find only two X-ray sources with candidate optical counterparts. We find 21 likely low-mass X-ray binaries (LMXBs), although this number is a lower limit due to the difficulties in separating LMXBs from background active galactic nuclei. The X-ray luminosity functions (XLFs) in both the soft and hard energy bands are presented. The XLFs in the soft band (0.5-2keV) and the hard band (2-8keV) have a limiting luminosity at the 90% completeness limit of 10^35^erg/s and 10^36^erg/s, respectively, significantly lower than previous X-ray studies of NGC 404. We find the XLFs to be consistent with those of other X-ray populations dominated by LMXBs. However, the number of luminous (&gt;10^37^erg/s) X-ray sources per unit stellar mass in NGC 404 is lower than is observed for other galaxies. The relative lack of luminous XRBs may be due to a population of LMXBs with main-sequence companions formed during an epoch of elevated star formation ~0.5Gyr ago.</description><source format="bibcode">2013ApJ...763..128B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/763/128</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/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/45">IX/45 : The Chandra Source Catalog, Release 1.1 (Evans+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/312">II/312 : GALEX-DR5 (GR5) sources from AIS and MIS (Bianchi+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/284">I/284 : The USNO-B1.0 Catalog (Monet+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/15">J/ApJ/758/15 : Chandra X-ray point sources of NGC 300 (Binder+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/737/45">J/ApJ/737/45 : Variable 1.4GHz radio sources from NVSS &amp; FIRST (Ofek+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/734/L22">J/ApJ/734/L22 : ACS Nearby Galaxy Survey Treasury (Williams+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/192/10">J/ApJS/192/10 : Chandra ACIS survey in 383 nearby galaxies. 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Upper limit uncertainty in Net5</description><unit>ct</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Net5</name><description>? Lower limit uncertainty in Net5</description><unit>ct</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_Net6</name><description>Limit flag on Net6</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Net6</name><description>[0.9/342] Net counts in the 1.1-2.6keV energy band</description><unit>ct</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Net6</name><description>? Upper limit uncertainty in Net6</description><unit>ct</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Net6</name><description>? Lower limit uncertainty in Net6</description><unit>ct</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logF0</name><description>[-7/-4] Log of 0.5-8keV energy band photon flux (4)</description><unit>log(cm**-2.s**-1)</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logF2</name><description>Log of 0.5-2keV energy band photon flux (4)</description><unit>log(cm**-2.s**-1)</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logF3</name><description>Log of 2-8keV energy band photon flux (4)</description><unit>log(cm**-2.s**-1)</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logF4</name><description>Log of 0.35-8keV energy band photon flux (4)</description><unit>log(cm**-2.s**-1)</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logF5</name><description>Log of 0.35-1.1keV energy band photon flux (4)</description><unit>log(cm**-2.s**-1)</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logF6</name><description>Log of 1.1-2.6keV energy band photon flux (4)</description><unit>log(cm**-2.s**-1)</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HR1</name><description>[-0.8/0.7] The "soft" color (5)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_HR1</name><description>Uncertainty in HR1</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HR2</name><description>[-0.7/0.8] The "hard" color (5)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_HR2</name><description>Uncertainty in HR2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hcl</name><description>Classification from hardness ratios (HRs) (G2)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Fit</name><description>Spectral fit ("apec" = Astrophysical Plasma Emission Code, Smith et al. 2001ApJ...556L..91S)</description><ucd>meta.note</ucd></column><column><name>Var</name><description>Variability (long or rapid)</description><ucd>meta.code;src.var</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>d</name><description>[0/6.3] Galactocentric distance</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>XID</name><description>Wavelength counterpart(s)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>Class</name><description>Object classification (background AGN, XRB, SSS:super-soft source or FS: forground star)</description><ucd>meta.code.class;instr.background</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column></table></schema></tableset></ri:Resource>