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<ri:Resource created="2022-03-29T06:36:25Z" 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>Evolution of C^IV^ absorbers. I. Absorber properties</title><shortName>J/ApJ/904/44</shortName><identifier>ivo://CDS.VizieR/J/ApJ/904/44</identifier><altIdentifier>doi:10.26093/cds/vizier.19040044</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hasan F.</name></creator><creator><name>Churchill C.W.</name></creator><creator><name>Stemock B.</name></creator><creator><name>Mathes N.L.</name></creator><creator><name>Nielsen N.M.,Finlator K.</name></creator><creator><name>Doughty C.</name></creator><creator><name>Croom M.</name></creator><creator><name>Kacprzak G.G.</name></creator><creator><name>Murphy M.T.</name></creator><date role="Updated">2022-06-13T09:48:40Z</date><date role="Created">2022-03-29T06:36:25Z</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>quasars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>infrared-astronomy</subject><subject>redshifted</subject><description>We present a large high-resolution study of the distribution and evolution of C^IV^ absorbers, including the weakest population with equivalent widths W_r_&lt;0.3{AA} . By searching 369 high-resolution, high signal-to-noise ratio spectra of quasars at 1.1&lt;=z_em_&lt;=5.3 from Keck/HIRES and VLT/UVES, we find 1268 C^IV^ absorbers with W_r_&gt;~0.05{AA} (our ~50% completeness limit) at redshifts 1.0&lt;=z&lt;=4.75. A Schechter function describes the observed equivalent width distribution with a transition from power-law to exponential decline at W_r_&gt;~0.5{AA} . The power-law slope {alpha} rises by ~7%, and the transition equivalent width W* falls by ~20% from &lt;z&gt;=1.7 to 3.6. We find that the comoving redshift path density, dN/dX, of W_r_&gt;=0.05{AA} absorbers rises by ~1.8 times from z~4.0 to 1.3, while the W_r_&gt;=0.6{AA} dN/dX rises by a factor of ~8.5. We quantify the observed evolution by a model in which dN/dX decreases linearly with increasing redshift. The model suggests that populations with larger W_r_ thresholds evolve faster with redshift and appear later in the universe. The cosmological Technicolor Dawn simulations at z=3-5 overproduce the observed abundance of absorbers with W_r_&lt;=0.3{AA} while yielding better agreement at higher W_r_. Our empirical linear model successfully describes C^IV^ evolution in the simulations and the observed evolution of W_r_&gt;=0.6{AA} C^IV^ for the past ~12Gyr. Combining our measurements with the literature gives us a picture of C^IV^ absorbing structures becoming more numerous and/or larger in physical size over the last ~13Gyr of cosmic time (z~6-0).</description><source format="bibcode">2020ApJ...904...44H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/904/44</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/J/A+A/283/759">J/A+A/283/759 : CIV QSO absorption systems (Petitjean+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/596/768">J/ApJ/596/768 : Optical depths in 19 QSOs (Schaye+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/473/791">J/A+A/473/791 : CIV absorption in DLAs and sub-DLAs systems (Fox+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/679/194">J/ApJ/679/194 : Low-z intergalactic medium. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>QSO</name><description>Quasar name in J2000 format (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType><flag>primary</flag></column><column><name>z</name><description>[1.16/5.3] Quasar emission redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Inst</name><description>Quasar spectrum observation facility</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>wmin</name><description>[2636/7648] Minimum wavelength CIV search space (2)</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>wmax</name><description>[3302/9578] Maximum wavelength CIV search space (3)</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nprop</name><description>Number of absorber properties (table2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Position from QSO identifier (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from QSO identifier (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/904/44/table2</name><description>Data of C^IV^ absorber properties</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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