@prefix dcat: <http://www.w3.org/ns/dcat#> .
@prefix dct: <http://purl.org/dc/terms/> .
@prefix foaf: <http://xmlns.com/foaf/0.1/> .
@prefix vcard: <http://www.w3.org/2006/vcard/ns#> .
@prefix xsd: <http://www.w3.org/2001/XMLSchema#> .

<https://data.amerigeoss.org/dataset/02b7ab37-ad4e-45fb-80aa-857092cb2690> a dcat:Dataset ;
    dct:description "Apparently diffuse X-ray emission has been known to exist along the central quarter of the Galactic Plane since the beginning of X-ray astronomy; this is referred to as the Galactic Ridge X-ray emission (GRXE). Recent deep X-ray observations have shown that numerous X-ray point sources account for a large fraction of the GRXE in the hard band (2 - 8 keV). However, the nature of these sources is poorly understood. Using the deepest X-ray observations made in the Chandra bulge field, the authors present the result of a coherent photometric and spectroscopic analysis of individual X-ray point sources for the purpose of constraining their nature and deriving their fractional contributions to the hard-band continuum and Fe K line emission of the GRXE. Based on the X-ray color-color diagram, they divided the point sources into three groups: A (hard), B (soft and broad spectrum), and C (soft and peaked spectrum). The group A sources are further decomposed spectrally into thermal and non-thermal sources with different fractions in different flux ranges. From their X-ray properties, the authors speculate that the group A non-thermal sources are mostly active galactic nuclei and the thermal sources are mostly white dwarf (WD) binaries such as magnetic and non-magnetic cataclysmic variables (CVs), pre-CVs, and symbiotic stars, whereas the group B and C sources are X-ray active stars in flares and quiescence, respectively. In the log N - log S curve of the 2 - 8 keV band, the group A non-thermal sources are dominant above ~10&lt;sup&gt;-14&lt;/sup&gt; erg/cm&lt;sup&gt;2&lt;/sup&gt;/s, which is gradually taken over by Galactic sources in the fainter flux ranges. The Fe K-alpha emission is mostly from the group A thermal (WD binaries) and the group B (X-ray active stars) sources. The authors retrieved 10 archived data sets of the Chandra bulge field (CBF) taken with the Advanced CCD Imaging Spectrometer-I (ACIS-I; 0.5 - 8.0 keV energy band with a spectral resolution of ~280 eV for the full width at half-maximum at 5.9keV) array on board Chandra. The observations were carried out from 2008 May to August with a total exposure time of ~900 ks. The authors first extracted point-source candidates using the wavdetect algorithm in the CIAO package. They set the significance threshold at 2.5 x 10&lt;sup&gt;-5&lt;/sup&gt;, implying that one false positive detection would be expected at every 4 x 10&lt;sup&gt;4&lt;/sup&gt; trials. As a result, 2596 source candidates were found. The number of their source candidates is nearly the same as that found by Revnivtsev et al.(2009, A&amp;A, 507, 1211) in the same region. To select significant point sources from the candidates, the authors examined their validity based on their photometric significance (PS) and the probability of no source (P&lt;sub&gt;B&lt;/sub&gt;). The PS is defined as the background-subtracted source counts (C&lt;sub&gt;net&lt;/sub&gt;) divided by its background counts normalized by the area. P&lt;sub&gt;B&lt;/sub&gt; is the probability that the source is attributable to a background fluctuation, assuming Poisson statistics. The authors recognized a source to be valid if it satisfied both these criteria: PS &gt;= 1.0 and P&lt;sub&gt;B&lt;/sub&gt; &lt;= 1.0 x 10&lt;sup&gt;-2&lt;/sup&gt;. As a result, they obtained 2002 valid point sources. This table was created by the HEASARC in December 2014 based on &lt;a href=\"https://cdsarc.cds.unistra.fr/ftp/cats/J/ApJ/766/14\"&gt;CDS catalog J/ApJ/766/14&lt;/a&gt; file table2.dat. This is a service provided by NASA HEASARC ." ;
    dct:identifier "ivo://nasa.heasarc/cbfgrxecxo" ;
    dct:issued "2025-09-23T15:37:36.032676"^^xsd:dateTime ;
    dct:modified "2025-09-10"^^xsd:date ;
    dct:publisher <https://data.amerigeoss.org/organization/727dbdd5-3f98-4ac0-9d28-5e344558139b> ;
    dct:title "Chandra Bulge Field X-Ray Point Source Catalog" ;
    dcat:contactPoint [ a vcard:Organization ;
            vcard:fn "Tess Jaffe" ;
            vcard:hasEmail <mailto:tess.jaffe@nasa.gov> ] ;
    dcat:distribution <https://data.amerigeoss.org/dataset/02b7ab37-ad4e-45fb-80aa-857092cb2690/resource/696daf96-c920-4f8e-969a-723221be4d8d>,
        <https://data.amerigeoss.org/dataset/02b7ab37-ad4e-45fb-80aa-857092cb2690/resource/ffcf3eab-2b82-4c75-a0d7-c5b502796869> ;
    dcat:keyword "AmeriGEO",
        "AmeriGEOSS",
        "CKAN",
        "GEO",
        "GEOSS",
        "National",
        "North America",
        "United States",
        "na" ;
    dcat:theme <%7BAstrophysics%7D> .

<https://data.amerigeoss.org/dataset/02b7ab37-ad4e-45fb-80aa-857092cb2690/resource/696daf96-c920-4f8e-969a-723221be4d8d> a dcat:Distribution ;
    dct:format "BIN" ;
    dct:issued "2025-08-30T05:09:20.536326"^^xsd:dateTime ;
    dct:modified "2025-09-23T15:37:36.021611"^^xsd:dateTime ;
    dct:title "Data Information (Unknown Format)" ;
    dcat:accessURL <https://heasarc.gsfc.nasa.gov/xamin/vo/cone?showoffsets&table=cbfgrxecxo&> ;
    dcat:mediaType "application/octet-stream" .

<https://data.amerigeoss.org/dataset/02b7ab37-ad4e-45fb-80aa-857092cb2690/resource/ffcf3eab-2b82-4c75-a0d7-c5b502796869> a dcat:Distribution ;
    dct:description "cbfgrxecxo.html" ;
    dct:format "HTML" ;
    dct:issued "2025-08-30T05:09:20.536323"^^xsd:dateTime ;
    dct:modified "2025-09-23T15:37:36.020761"^^xsd:dateTime ;
    dct:title "Data Information (HTML)" ;
    dcat:accessURL <https://heasarc.gsfc.nasa.gov/W3Browse/all/cbfgrxecxo.html> ;
    dcat:mediaType "text/html" .

<https://data.amerigeoss.org/organization/727dbdd5-3f98-4ac0-9d28-5e344558139b> a foaf:Agent ;
    foaf:name "US Migrating" .

