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<ri:Resource created="2018-12-03T14:15:21Z" 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>Bootes field deep LOFAR 150MHz imaging</title><shortName>J/A+A/620/A74</shortName><identifier>ivo://CDS.VizieR/J/A+A/620/A74</identifier><altIdentifier>doi:10.26093/cds/vizier.36200074</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Retana-Montenegro E.</name></creator><creator><name>Rottgering H.J.A</name></creator><creator><name>Shimwell T.W.</name></creator><creator><name>van Weeren R.J.,Prandoni I.</name></creator><creator><name>Brunetti G.</name></creator><creator><name>Best P.N</name></creator><creator><name>Bruggen M.</name></creator><date role="Updated">2019-01-07T09:20:25Z</date><date role="Created">2018-12-03T14:15:21Z</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>surveys</subject><subject>radio-galaxies</subject><subject>radio-continuum-emission</subject><description>We have conducted a deep survey (with a central rms of 55uJy) with the LOw Frequency ARray (LOFAR) at 120-168MHz of the Bootes field, with an angular resolution of 3.98"x6.45", and obtained a sample of 10091 radio sources (5{sigma} limit) over an area of 20deg^2^. The astrometry and flux scale accuracy of our source catalog is investigated. The resolution bias, incompleteness and other systematic effects that could affect our source counts are discussed and accounted for. The derived 150MHz source counts present a flattening below sub-mJy flux densities, that is in agreement with previous results from high- and low- frequency surveys. This flattening has been argued to be due to an increasing contribution of star-forming galaxies and faint active galactic nuclei. Additionally, we use our observations to evaluate the contribution of cosmic variance to the scatter in source counts measurements. The latter is achieved by dividing our Bootes mosaic into 10 non-overlapping circular sectors, each one with an approximate area of 2deg^2^. The counts in each sector are computed in the same way as done for the entire mosaic. By comparing the induced scatter with that of counts obtained from depth observations scaled to 150MHz, we find that the 1{sigma} scatter due to cosmic variance is larger than the Poissonian errors of the source counts, and it may explain the dispersion from previously reported depth source counts at flux densities S&lt;1mJy. This work demonstrates the feasibility of achieving deep radio imaging at low-frequencies with LOFAR.</description><source format="bibcode">2018A&amp;A...620A..74R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/620/A74</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/AJ/123/1784">J/AJ/123/1784 : 1.4GHz imaging of the Bootes field (de Vries+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/213">J/AJ/127/213 : LALA Bootes field X-ray source catalog (Wang+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/923">J/AJ/130/923 : Faint radio sources in the NOAO Bootes field (Wrobel+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/634/L1">J/ApJ/634/L1 : 16{mu}m sources in the NOAO Bootes field (Kasliwal+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/161/9">J/ApJS/161/9 : X-ray survey of the NDWFS Bootes field (Kenter+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/641/140">J/ApJ/641/140 : Optical counterparts in the NDWFS Bootes field (Brand+ 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/535/A38">J/A+A/535/A38 : Observations of NOAO Bootes field at 153MHz (Intema+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/793/82">J/ApJ/793/82 : LOFAR Bootes and 3C295 field sources (van Weeren+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/450/1477">J/MNRAS/450/1477 : VLA 352MHz image of the Bootes field. I. 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