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<ri:Resource created="2020-11-17T06:00:38Z" status="active" updated="2025-06-13T15:25:00Z" 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>J-PLUS Ly{alpha}-emitting candidates</title><shortName>J/A+A/643/A149</shortName><identifier>ivo://CDS.VizieR/J/A+A/643/A149</identifier><altIdentifier>doi:10.26093/cds/vizier.36430149</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Spinoso D.</name></creator><creator><name>Orsi A.</name></creator><creator><name>Lopez-Sanjuan C.</name></creator><creator><name>Bonoli S.</name></creator><creator><name>Viironen K.,Izquierdo-Villalba D.</name></creator><creator><name>Sobral D.</name></creator><creator><name>Gurung-Lopez S.</name></creator><creator><name>Hernan-Caballero A.,Ederoclite A.</name></creator><creator><name>Varela J.</name></creator><creator><name>Overzier R.</name></creator><creator><name>Miralda-Escude J.</name></creator><creator><name>Muniesa D.J.,Vilchez J.M.</name></creator><creator><name>Alcaniz J.</name></creator><creator><name>Angulo R.E.</name></creator><creator><name>Cenarro A.J.</name></creator><creator><name>Cristobal-Hornillos D.,Dupke R.A.</name></creator><creator><name>Hernandez-Monteagudo C.</name></creator><creator><name>Marin-Franch A.</name></creator><creator><name>Moles M.</name></creator><creator><name>Sodre L.Jr,Vazquez-Ramio H.</name></creator><date role="Updated">2021-05-04T13:09:09Z</date><date role="Created">2020-11-17T06:00:38Z</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>catalogs</subject><subject>ultraviolet-astronomy</subject><subject>line-intensities</subject><description>We present the photometric determination of the bright-end of the Ly{alpha} luminosity function (at L_Ly{alpha}_&gt;~10^43.5^erg/s) within four redshifts windows ({Delta}z&lt;0.16) in the interval 2.2&lt;~z&lt;~3.3. Our work is based on the Javalambre Photometric Local Universe Survey (J-PLUS) first data-release, which provides multiple narrow-band measurements over ~1000deg^2^, with limiting magnitude ~22. Theanalysis of high-z Ly{alpha}-emitting sources over such a wide area is unprecedented, and allows to select a total of ~14500 hyper-bright(L_Ly{alpha}_&gt;10^43.3^erg/s) Ly{alpha}-emitting candidates. We test our selection with two spectroscopic follow-up programs at the GTC telescope,which confirm as line-emitting sources ~89% of the targets, with ~64% being genuine z~2.2 QSOs. We extend the 2.2&lt;~z&lt;~3.3 Ly{alpha} luminosity function for the first time above L_Ly{alpha}_~10^44^erg/s and down to densities of ~10^-8^Mpc^-3^. Our results unveil with high detail the Schechter exponential-decay of the brightest-end of the Ly{alpha} LF, complementing the power-law component of previous LF determinations at 43.3&lt;~Log10(L_Ly{alpha}_/(erg/s))&lt;~44. We measure {PHI}*=(3.33+/-0.19)x10^-6^, Log(L*)=44.65+/-0.65 and {alpha}=-1.35+/-0.84 as an average over the redshifts we probe. These values are significantly different than the typical Schechter parameters measured for the Ly{alpha} LF of high-z star-forming LAEs. This suggests that z&gt;2 AGN/QSOs (likely dominant in our samples) are described by a structurally different LF than z&gt;2 star-forming LAEs, namely with L*_QSOs_~100 L*_LAEs_ and {PHI}*_QSOs_~10^-3^{PHI}*_LAEs_. Finally, our method identifies very efficiently as high-z line-emitters sources without previous spectroscopic confirmation, currently classified as stars (~2000 objects in each redshift bin, on average). 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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>TileId</name><description>Identifier of the Tile image where the object was detected (TILE_ID)</description><ucd>obs.image</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Id</name><description>Number identifier assigned by Sextractor for the object in the image (NUMBER)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000) (ALPHA_J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000) (DELTA_J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>FLya</name><description>Photometric estimate of the integrated line-flux in Ly{alpha}, corrected for filter-width losses (LYA_FLUX)</description><unit>mW.m**-2</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FLya</name><description>Error on FLya (LYA_FLUX_ERR)</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LLya</name><description>? 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Ly{alpha} luminosity computed from the sources FLya and redshift (LYA_LUM)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.UV</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_z</name><description>? Redshift error (Z_ERR) (3)</description><ucd>stat.error;src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Error on LLya (LYA_LUM_ERR)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EWLya</name><description>Ly{alpha} equivalent width (LYA_EW) (1)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>z</name><description>Sources redshift assuming detection at the narrow-band central wavelength (Z) (2)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>SDSS-QSO</name><description>[0/1] Flag identifying the presence of SDSS QSOs counterparts (at any z) (SDSS_QSO) (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SDSS-QSORz</name><description>[0/1] Flag identifying the presence of SDSS QSOs counterparts (at the redshift sampled by the NB used to select the candidates) (SDSS_RIGHTz_QSO) (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LQAC-QSO</name><description>[0/1] Flag identifying the presence of LQAC (Souchay et al., 2015, Cat. 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