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<ri:Resource created="2019-09-27T14:00:42Z" 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>HST and Chandra obs. of the GLIMPSE-C01 star cluster</title><shortName>J/ApJ/865/33</shortName><identifier>ivo://CDS.VizieR/J/ApJ/865/33</identifier><altIdentifier>doi:10.26093/cds/vizier.18650033</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hare J.</name></creator><creator><name>Kargaltsev O.</name></creator><creator><name>Rangelov B.</name></creator><date role="Updated">2020-03-26T14:19:11Z</date><date role="Created">2019-09-27T14:00:42Z</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>globular-star-clusters</subject><subject>x-ray-sources</subject><subject>hst-photometry</subject><subject>infrared-photometry</subject><description>We report the results of Hubble Space Telescope and Chandra X-Ray Observatory observations of the GLIMPSE-C01 (hereafter GC01) star cluster. Color-magnitude and color-color diagrams suggest a cluster age of &gt;~2Gyr up to ~10Gyr (dependent on GC01's metallicity), a distance of 3.3-3.5kpc, and strong differential reddening with A_V_=14-22. After performing astrometric corrections, we find that nine of the 15 X-ray sources have at least one near-infrared (NIR) counterpart within the 2{sigma} Chandra positional error circles. However, given the very high density of NIR sources in the cluster, most of these counterparts are likely due to chance coincidence. We jointly analyze the X-ray and NIR properties to assess the likelihood of true associations. Based primarily on their X-ray properties, we identify a low-mass X-ray binary candidate (source X2), a cataclysmic variable (CV) candidate (source X1), and an active binary (AB) candidate (source X9). Source X11 is detected during an X-ray flaring episode with a flare luminosity (L_X_=2.1x10^33^erg/s) and has a quiescent luminosity L_X_&lt;8.0x10^30^erg/s, in 0.5-8keV at the distance of GC01, suggesting that the source is either an AB or CV. We also discuss the limits on an intermediate-mass black hole at the center of GC01 and the challenges of X-ray source classification imposed by the limitations of the existing data and instrumentation along with future prospects in the James Webb Space Telescope era.</description><source format="bibcode">2018ApJ...865...33H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/865/33</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/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource 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Uncertainty of F127M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF127M</name><description>[9/4177]? Signal-to-noise ratio of the source in the F127M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF127M</name><description>[-0.03/0.03] Sharpness value of the source in the F127M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>crdF127M</name><description>[0.003/0.2]? Crowding value of the source in the F127M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F139Mmag</name><description>[11.4/22]? WFC3/IR F139M magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F139Mmag</name><description>[0/0.06]? Uncertainty of F139M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF139M</name><description>[18/5226]? Signal-to-noise ratio of the source in the F139M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF139M</name><description>[-0.03/0.03]? Sharpness value of the source in the F139M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF139M</name><description>[0.005/0.2]? Crowding value of the source in the F139M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F153Mmag</name><description>[10.5/21.2]? WFC3/IR F153M magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F153Mmag</name><description>[0/0.04]? Uncertainty of F153M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF153M</name><description>[27/7033]? Signal-to-noise ratio of the source in the F153M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF153M</name><description>[-0.03/0.03]? Sharpness value of the source in the F153M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF153M</name><description>[0.006/0.2]? Crowding value of the source in the F153M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/865/33/127roi</name><description>WFC3/UVIS+IR catalog for the circular ROI region shown in Figure 8, derived using the drizzled F127M image for source extraction, and plotted in the left panel of Figure 9</description><column><name>F127Mmag</name><description>[12/23]? WFC3/IR F127M magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[282.19/282.23] Source Right Ascension (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-1.53/-1.48] Source Declination (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>F814Wmag</name><description>[15.7/35.4]? WFC3/UVIS F814W magnitude (2)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814Wmag</name><description>[0.001/10]? Uncertainty of F814W magnitude (2)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF814W</name><description>[0/736]? Signal-to-noise ratio of the source in the F814W image (2)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF814W</name><description>[-3.4/5.8]? Sharpness value of the source in the F814W image (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF814W</name><description>[0/7.7]? Crowding value of the source in the F814W image (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F127Mmag</name><description>[0/0.2]? Uncertainty of F127M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF127M</name><description>[9/4177]? Signal-to-noise ratio of the source in the F127M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF127M</name><description>[-0.03/0.03] Sharpness value of the source in the F127M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>crdF127M</name><description>[0.003/0.2]? Crowding value of the source in the F127M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F139Mmag</name><description>[11.4/22]? WFC3/IR F139M magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F139Mmag</name><description>[0/0.06]? Uncertainty of F139M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF139M</name><description>[18/5226]? Signal-to-noise ratio of the source in the F139M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF139M</name><description>[-0.03/0.03]? Sharpness value of the source in the F139M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF139M</name><description>[0.005/0.2]? Crowding value of the source in the F139M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F153Mmag</name><description>[10.5/21.2]? WFC3/IR F153M magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F153Mmag</name><description>[0/0.04]? Uncertainty of F153M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF153M</name><description>[27/7033]? Signal-to-noise ratio of the source in the F153M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF153M</name><description>[-0.03/0.03]? Sharpness value of the source in the F153M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF153M</name><description>[0.006/0.2]? Crowding value of the source in the F153M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/865/33/814roi</name><description>WFC3/UVIS+IR catalog for the circular ROI region shown in Figure 8, derived using the drizzled F814W image for source extraction, and plotted in Figure 10</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[282.19/282.22] Source Right Ascension (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-1.51/-1.48] Source Declination (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>F814Wmag</name><description>[17/26.1]? WFC3/UVIS F814W magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814Wmag</name><description>[0.002/0.3]? Uncertainty of F814W magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF814W</name><description>[4/661]? Signal-to-noise ratio of the source in the F814W image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF814W</name><description>[-0.1/0.1]? Sharpness value of the source in the F814W image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF814W</name><description>[0/0.2]? Crowding value of the source in the F814W image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F127Mmag</name><description>[12.4/21.1]? WFC3/IR F127M magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F127Mmag</name><description>[0/0.03]? Uncertainty of F127M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF127M</name><description>[41/3548]? Signal-to-noise ratio of the source in the F127M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF127M</name><description>[-0.03/0.02]? Sharpness value of the source in the F127M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF127M</name><description>[0.004/0.2]? Crowding value of the source in the F127M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F139Mmag</name><description>[11.5/20.6]? WFC3/IR F139M magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F139Mmag</name><description>[0/0.03]? Uncertainty of F139M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF139M</name><description>[48/5113]? Signal-to-noise ratio of the source in the F139M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF139M</name><description>[-0.04/0.03]? Sharpness value of the source in the F139M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF139M</name><description>[0.005/0.4]? Crowding value of the source in the F139M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F153Mmag</name><description>[10.6/20.2]? WFC3/IR F153M magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F153Mmag</name><description>[0/0.02]? Uncertainty of F153M magnitude</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SNRF153M</name><description>[54/6661]? Signal-to-noise ratio of the source in the F153M image</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>shpF153M</name><description>[-0.05/0.03]? Sharpness value of the source in the F153M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>crdF153M</name><description>[0.007/0.5]? Crowding value of the source in the F153M image</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/865/33/table3</name><description>Potential NIR counterparts to X-ray sources and their magnitudes in the WFC3 IR and UVIS filters</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>Counterpart name (X-ray source identifier)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>m_ID</name><description>Multiple counterpart component identifier</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>f_ID</name><description>Counterpart flag(s) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>RAJ2000</name><description>Counterpart RA, decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Counterpart DEC, decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>F814Wmag</name><description>? WFC3/UVIS F814W VEGAMAG magnitude (2)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814Wmag</name><description>? uncertainty of F814W magnitude (3)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F127Wmag</name><description>WFC3/UVIS F127W VEGAMAG magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F127Wmag</name><description>uncertainty of F127W magnitude (3)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F139Wmag</name><description>WFC3/UVIS F139W VEGAMAG magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F139Wmag</name><description>uncertainty of F139W magnitude (3)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F153Wmag</name><description>WFC3/UVIS F153W VEGAMAG magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F153Wmag</name><description>uncertainty of F153W magnitude (3)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>