<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2021-08-25T00:00:00" status="active" updated="2024-05-30T10:56:59" 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/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface-v1.0.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource-v1.1.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService-v1.1.xsd" xsi:type="vs:CatalogResource"><identifier>ivo://astron.nl/lotss_dr2/q/mosaics</identifier><curation><publisher>ASTRON</publisher><creator><name>Shimwell, T. W.</name></creator><creator><name>Hardcastle, M. J.</name></creator><creator><name>Tasse, C.</name></creator><creator><name>Best, P. N.</name></creator><creator><name>Röttgering, H. J. A.</name></creator><creator><name>Williams, W. L.</name></creator><creator><name>Botteon, A.</name></creator><creator><name>Drabent, A.</name></creator><creator><name>Mechev, A.</name></creator><creator><name>Shulevski, A.</name></creator><creator><name>van Weeren, R. J.</name></creator><creator><name>Bester, L.</name></creator><creator><name>Brüggen, M.</name></creator><creator><name>Brunetti, G.</name></creator><creator><name>Callingham, J. R.</name></creator><creator><name>Chyży, K.T.</name></creator><creator><name>Conway, J. E.</name></creator><creator><name>Dijkema, T. J.</name></creator><creator><name>Duncan, K.</name></creator><creator><name>de Gasperin, F.</name></creator><creator><name>Hale, C. L.</name></creator><creator><name>Haverkorn, M.</name></creator><creator><name>Hugo, B.</name></creator><creator><name>Jackson, N.</name></creator><creator><name>Mevius, M.</name></creator><creator><name>Miley, G. K.</name></creator><creator><name>Morabito, L. K.</name></creator><creator><name>Morganti, R.</name></creator><creator><name>Offringa, A.</name></creator><creator><name>Oonk, J. B. R.</name></creator><creator><name>Rafferty, D.</name></creator><creator><name>Sabater, J.</name></creator><creator><name>Smith, D. J. B.</name></creator><creator><name>Schwarz, D. J.</name></creator><creator><name>Smirnov, O.</name></creator><creator><name>O’Sullivan, S. P.</name></creator><creator><name>Vedantham, H.</name></creator><creator><name>White, G. J.</name></creator><creator><name>Albert, J. G.</name></creator><creator><name>Alegre, L.</name></creator><creator><name>Asabere, B.</name></creator><creator><name>Bacon, D. J.</name></creator><creator><name>Bonafede, A.</name></creator><creator><name>Bonnassieux, E.</name></creator><creator><name>Brienza, M.</name></creator><creator><name>Bilicki, M.</name></creator><creator><name>Bonato, M.</name></creator><creator><name>Calistro Rivera, G.</name></creator><creator><name>Cassano, R.</name></creator><creator><name>Cochrane, R.</name></creator><creator><name>Croston, J. H.</name></creator><creator><name>Cuciti, V.</name></creator><creator><name>Dallacasa, D.</name></creator><creator><name>Danezi, A.</name></creator><creator><name>Dettmar, R. J.</name></creator><creator><name>Di Gennaro, G.</name></creator><creator><name>Edler, H. W.</name></creator><creator><name>Enßlin, T. A.</name></creator><creator><name>Emig, K. L.</name></creator><creator><name>Franzen, T. M. O.</name></creator><creator><name>Garc\’ia-Vergara, C.</name></creator><creator><name>Grange, Y. G.</name></creator><creator><name>Gürkan, G.</name></creator><creator><name>Hajduk, M.</name></creator><creator><name>Heald, G.</name></creator><creator><name>Heesen, V.</name></creator><creator><name>Hoang, D. N.</name></creator><creator><name>Hoeft, M.</name></creator><creator><name>Horellou, C.</name></creator><creator><name>Iacobelli, M.</name></creator><creator><name>Jamrozy, M.</name></creator><creator><name>Jelić, V.</name></creator><creator><name>Kondapally, R.</name></creator><creator><name>Kukreti, P.</name></creator><creator><name>Kunert-Bajraszewska, M.</name></creator><creator><name>Magliocchetti, M.</name></creator><creator><name>Mahatma, V.</name></creator><creator><name>Małek, K.</name></creator><creator><name>Mandal, S.</name></creator><creator><name>Massaro, F.</name></creator><creator><name>Meyer-Zhao, Z.</name></creator><creator><name>Mingo, B.</name></creator><creator><name>Mostert, R. I. J.</name></creator><creator><name>Nair, D. G.</name></creator><creator><name>Nakoneczny, S. J.</name></creator><creator><name>Nikiel-Wroczyński, B.</name></creator><creator><name>Orrú, E.</name></creator><creator><name>Pajdosz-Śmierciak, U.</name></creator><creator><name>Pasini, T.</name></creator><creator><name>Prandoni, I.</name></creator><creator><name>van Piggelen, H. E.</name></creator><creator><name>Rajpurohit, K.</name></creator><creator><name>Retana-Montenegro, E.</name></creator><creator><name>Riseley, C. J.</name></creator><creator><name>Rowlinson, A.</name></creator><creator><name>Saxena, A.</name></creator><creator><name>Schrijvers, C.</name></creator><creator><name>Sweijen, F.</name></creator><creator><name>Siewert, T. M.</name></creator><creator><name>Timmerman, R.</name></creator><creator><name>Vaccari, M.</name></creator><creator><name>Vink, J.</name></creator><creator><name>West, J. L.</name></creator><creator><name>Wołowska, A.</name></creator><creator><name>Zhang, X.</name></creator><creator><name>Zheng, J.</name><logo>https://repository.surfsara.nl/api/objects/collection/lotss-dr2/thumbnail</logo></creator><date role="updated">2024-05-30T10:56:59</date><contact><name>Michael Sipior</name><address>Oude Hoogeveensedijk 4, 7991PD Dwingeloo, the Netherlands</address><email>vo@astron.nl</email></contact></curation><content><subject>radio continuum: general, techniques: image processing</subject><description> In this data release from the ongoing LOw-Frequency ARray (LOFAR)
Two-metre Sky Survey (LoTSS) we present 120-168 MHz images covering
27% of the northern sky. Our coverage is split into two regions
centred at approximately 12h45m +44°30′ and 1h00m +28°00′ and spanning
4178 and 1457 square degrees respectively. The images were derived
from 3,451 hrs (7.6 PB) of LOFAR High Band Antenna data which were
corrected for the direction-independent instrumental properties as
well as direction-dependent ionospheric distortions during extensive,
but fully automated, data processing. A catalogue of 4,395,448 radio
sources is derived from our total intensity (Stokes I) maps, where the
majority of these have never been detected at radio wavelengths
before. At 6′′ resolution, our full bandwidth Stokes I continuum maps
with a central frequency of 144 MHz have: a median rms sensitivity of
83 μ Jy/beam; a flux density scale accuracy of approximately 10%; an
astrometric accuracy of 0.2′′; and we estimate the point-source
completeness to be 90% at a peak brightness of 0.8 mJy/beam. By
creating three 16 MHz bandwidth images across the band we are able to
measure the in-band spectral index of many sources, albeit the error
on the derived spectral index is &gt; ±0.2 which is a consequence of our
flux-density scale accuracy and small fractional bandwidth. Our
circular polarisation (Stokes V) 20′′ resolution 120-168 MHz continuum
images have a median rms sensitivity of 95 μ Jy/beam, and we estimate
a Stokes I to Stokes V leakage of 0.056%. Our linear polarisation
(Stokes Q and Stokes U) image cubes consist of 480 97.6 kHz wide
planes and have a median rms sensitivity per plane of 10.8mJy/beam at
4′ and 2.2mJy/beam at 20′′; we estimate the Stokes I to Stokes Q/U
leakage to be approximately 0.2%. Here we characterise and publicly
release our Stokes I, Q, U and V images in addition to the calibrated
uv-data to facilitate the thorough scientific exploitation of this
unique dataset.</description><source 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58884.8</temporal><spectral>7.95129e-26 1.1132e-25</spectral><waveband>Radio</waveband></coverage><tableset><schema><name>lotss_dr2</name><description> In this data release from the ongoing LOw-Frequency ARray (LOFAR)
Two-metre Sky Survey (LoTSS) we present 120-168 MHz images covering
27% of the northern sky. Our coverage is split into two regions
centred at approximately 12h45m +44°30′ and 1h00m +28°00′ and spanning
4178 and 1457 square degrees respectively. The images were derived
from 3,451 hrs (7.6 PB) of LOFAR High Band Antenna data which were
corrected for the direction-independent instrumental properties as
well as direction-dependent ionospheric distortions during extensive,
but fully automated, data processing. A catalogue of 4,395,448 radio
sources is derived from our total intensity (Stokes I) maps, where the
majority of these have never been detected at radio wavelengths
before. At 6′′ resolution, our full bandwidth Stokes I continuum maps
with a central frequency of 144 MHz have: a median rms sensitivity of
83 μ Jy/beam; a flux density scale accuracy of approximately 10%; an
astrometric accuracy of 0.2′′; and we estimate the point-source
completeness to be 90% at a peak brightness of 0.8 mJy/beam. By
creating three 16 MHz bandwidth images across the band we are able to
measure the in-band spectral index of many sources, albeit the error
on the derived spectral index is &gt; ±0.2 which is a consequence of our
flux-density scale accuracy and small fractional bandwidth. Our
circular polarisation (Stokes V) 20′′ resolution 120-168 MHz continuum
images have a median rms sensitivity of 95 μ Jy/beam, and we estimate
a Stokes I to Stokes V leakage of 0.056%. Our linear polarisation
(Stokes Q and Stokes U) image cubes consist of 480 97.6 kHz wide
planes and have a median rms sensitivity per plane of 10.8mJy/beam at
4′ and 2.2mJy/beam at 20′′; we estimate the Stokes I to Stokes Q/U
leakage to be approximately 0.2%. Here we characterise and publicly
release our Stokes I, Q, U and V images in addition to the calibrated
uv-data to facilitate the thorough scientific exploitation of this
unique dataset.</description><table><name>lotss_dr2.mosaics</name><description> In this data release from the ongoing LOw-Frequency ARray (LOFAR)
Two-metre Sky Survey (LoTSS) we present 120-168 MHz images covering
27% of the northern sky. Our coverage is split into two regions
centred at approximately 12h45m +44°30′ and 1h00m +28°00′ and spanning
4178 and 1457 square degrees respectively. The images were derived
from 3,451 hrs (7.6 PB) of LOFAR High Band Antenna data which were
corrected for the direction-independent instrumental properties as
well as direction-dependent ionospheric distortions during extensive,
but fully automated, data processing. A catalogue of 4,395,448 radio
sources is derived from our total intensity (Stokes I) maps, where the
majority of these have never been detected at radio wavelengths
before. At 6′′ resolution, our full bandwidth Stokes I continuum maps
with a central frequency of 144 MHz have: a median rms sensitivity of
83 μ Jy/beam; a flux density scale accuracy of approximately 10%; an
astrometric accuracy of 0.2′′; and we estimate the point-source
completeness to be 90% at a peak brightness of 0.8 mJy/beam. By
creating three 16 MHz bandwidth images across the band we are able to
measure the in-band spectral index of many sources, albeit the error
on the derived spectral index is &gt; ±0.2 which is a consequence of our
flux-density scale accuracy and small fractional bandwidth. Our
circular polarisation (Stokes V) 20′′ resolution 120-168 MHz continuum
images have a median rms sensitivity of 95 μ Jy/beam, and we estimate
a Stokes I to Stokes V leakage of 0.056%. Our linear polarisation
(Stokes Q and Stokes U) image cubes consist of 480 97.6 kHz wide
planes and have a median rms sensitivity per plane of 10.8mJy/beam at
4′ and 2.2mJy/beam at 20′′; we estimate the Stokes I to Stokes Q/U
leakage to be approximately 0.2%. Here we characterise and publicly
release our Stokes I, Q, U and V images in addition to the calibrated
uv-data to facilitate the thorough scientific exploitation of this
unique dataset.</description><column><name>accref</name><description>Access key for the data</description><utype>Access.Reference</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>owner</name><description>Owner of the data</description><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>embargo</name><description>Date the data will become/became public</description><unit>a</unit><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>mime</name><description>MIME type of the file served</description><ucd>meta.code.mime</ucd><utype>Access.Format</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>accsize</name><description>Size of the data in 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reference frame</description><ucd>VOX:STC_CoordRefFrame</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>wcs_equinox</name><description>Equinox of the given coordinates</description><unit>yr</unit><ucd>VOX:STC_CoordEquinox</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>wcs_projection</name><description>FITS WCS projection type</description><ucd>VOX:WCS_CoordProjection</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>wcs_refpixel</name><description>WCS reference pixel</description><unit>pix</unit><ucd>VOX:WCS_CoordRefPixel</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>wcs_refvalues</name><description>World coordinates at WCS reference pixel</description><unit>deg</unit><ucd>VOX:WCS_CoordRefValue</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>wcs_cdmatrix</name><description>FITS WCS CDij matrix</description><unit>deg/pix</unit><ucd>VOX:WCS_CDMatrix</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>bandpassid</name><description>Freeform name of the bandpass used</description><ucd>VOX:BandPass_ID</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>bandpassunit</name><description>Unit of bandpass specifications (always m).</description><ucd>VOX:BandPass_Unit</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>bandpassrefval</name><description>Characteristic quantity for the bandpass of the image</description><unit>m</unit><ucd>VOX:BandPass_RefValue</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>bandpasshi</name><description>Upper limit of the bandpass (in BandPass_Unit units)</description><unit>m</unit><ucd>VOX:BandPass_HiLimit</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>bandpasslo</name><description>Lower limit of the bandpass (in BandPass_Unit units)</description><unit>m</unit><ucd>VOX:BandPass_LoLimit</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pixflags</name><description>Flags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display only</description><ucd>VOX:Image_PixFlags</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>coverage</name><description>Field covered by the image</description><unit>deg</unit><dataType arraysize="*" extendedType="polygon" xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>mosaic_id</name><description>The name of the mosaic.</description><ucd>meta.id;meta.main</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>related_products</name><description>Link related products for the observation</description><ucd>meta.ref.url</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>lofar_obsids</name><description>ObsID(s) of the LOFAR observation(s) used for imaging the central pointing.</description><ucd>meta.id;obs</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>data_pid</name><description>EPIC PID of the data product (for citation).</description><ucd>meta.bib</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>adler32</name><description>Adler32 checksum of the file</description><ucd>meta.fits;meta.number</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column></table></schema><schema><name>ivoa</name><description>Definition and support code for the ObsCore data model and table.</description><table><name>ivoa.obscore</name><description>This data collection is queriable in The VO @ ASTRON's obscore table.</description></table></schema></tableset></ri:Resource>