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<ri:Resource created="2022-11-23T10:10:01Z" 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>Hubble Asteroid Hunter. II.</title><shortName>J/A+A/667/A141</shortName><identifier>ivo://CDS.VizieR/J/A+A/667/A141</identifier><altIdentifier>doi:10.26093/cds/vizier.36670141</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Garvin E.O.</name></creator><creator><name>Kruk S.</name></creator><creator><name>Cornen C.</name></creator><creator><name>Bhatawdekar R.</name></creator><creator><name>Canameras R.</name></creator><creator><name>Merin B.</name></creator><date role="Updated">2024-11-28T20:01:06Z</date><date role="Created">2022-11-23T10:10:01Z</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>gravitational-lensing</subject><subject>galaxies</subject><subject>catalogs</subject><description>The Hubble Space Telescope (HST) archives constitute a rich dataset of high-resolution images to mine for strong gravitational lenses. While many HST programmes specifically target strong lenses, they can also be present by coincidence in other HST observations. Our aim is to identify non-targeted strong gravitational lenses, without any prior selection on the lens properties, in almost two decades of images from the ESA Hubble Space Telescope archive (eHST). We used crowdsourcing on the Hubble Asteroid Hunter (HAH) citizen science project to identify strong lenses, along with asteroid trails, in publicly available large field-of-view HST images. We visually inspected 2 354 objects tagged by citizen scientists as strong lenses to clean the sample and identify the genuine lenses. We report the detection of 252 strong gravitational lens candidates, which were not the primary targets of the HST observations. A total of 198 of them are new, not previously reported by other studies, consisting of 45 A grades, 74 B grades and 79 C grades. The majority are galaxy-galaxy configurations. The newly detected lenses are, on average, 1.3 magnitudes fainter than previous HST searches. This sample of strong lenses with high-resolution HST imaging is ideal to follow up with spectroscopy for lens modelling and scientific analyses. This paper presents the unbiased search of lenses that enabled us to find a wide variety of lens configurations, including exotic lenses. We demonstrate the power of crowdsourcing in visually identifying strong lenses and the benefits of exploring large archival datasets. This study shows the potential of using crowdsourcing in combination with artificial intelligence for the detection and validation of strong lenses in future large-scale surveys such as ESA's Euclid mission or in JamesWebb Space Telescope (JWST) archival images.</description><source format="bibcode">2022A&amp;A...667A.141G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/667/A141</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/661/A85">J/A+A/661/A85 : Asteroid trails in HST images (Kruk+, 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(1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>ID</name><description>Internal lens ID from the paper, (2)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Grade</name><description>[ABC] The grade of the lens assigned by the authors (3)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>rarc</name><description>? Arc radius indicating the angular separation between the lens and the image of the source</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>q</name><description>? Axis ratio of the lens (measured with GALFIT)</description><ucd>phys.size.axisRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PA</name><description>[]? Position angle of the lens (measured with GALFIT), measured from North through East</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Class</name><description>The morphological class of the source images, with the following categories: Arc, Ring, Quad, Double, Triple, Cross</description><ucd>src.morph.type</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>z</name><description>? Redshift of the lens</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_z</name><description>[*] * indicates retrieved either from NED or from SDSS</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Inst</name><description>HST instrument and aperture (ACS/WFC3, WFC3/UVIS or WFC3/IR)</description><ucd>phys.angSize;instr.fov</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Filt</name><description>HST filter in which the lens was discovered and fitted with GALFIT</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>mag</name><description>? Magnitude of the lens (measured with GALFIT)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>re</name><description>? Effective radius of the lens (measured with GALFIT)</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_z</name><description>[SP] "S" indicates spectroscopic redshift, "P" is the photometric redshift</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>PropID</name><description>? The ID of the HST proposal in which the serendipitous strong lens was found (4)</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Ref</name><description>Reference to the article in which the lens was first reported (5)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Target</name><description>Name of the HST observation target in which the lens was found, if the target was a galaxy cluster</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="27*">char</dataType></column><column><name>DESI</name><description>? ID of candidate galaxy cluster from DESI (Zou et al, 2021, Cat. J/ApJS/253/56) found within 3 arcmin from the gravitational lens</description><ucd>meta.id</ucd><flag>nullable</flag></column><column><name>Ddesi</name><description>? Angular distance from the lens to the DESI cluster</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RedMap</name><description>ID of candidate galaxy cluster from SDSS RedMaPPer (Rykoff et al., Cat. J/ApJ/785/104) found within 3 arcmin from the gravitational lens</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>Dredmap</name><description>? Angular distance from the lens to the RedMaPPer cluster</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Name</name><description>IAU Name: Hubble Asteroid Hunter (HAH JHHMMSS.s+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column></table></schema></tableset></ri:Resource>