<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2021-06-18T08:29:20Z" 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>SuperBoRG: search HST parallel imaging data</title><shortName>J/ApJS/253/4</shortName><identifier>ivo://CDS.VizieR/J/ApJS/253/4</identifier><altIdentifier>doi:10.26093/cds/vizier.22530004</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Morishita T.</name></creator><date role="Updated">2021-09-29T08:58:05Z</date><date role="Created">2021-06-18T08:29:20Z</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>hst-photometry</subject><subject>surveys</subject><description>The Hubble Space Telescope (HST) has been providing tremendous survey efficiency via its pure-parallel mode by observing another field in parallel with the primary instrument in operation for the primary observation. In this study, we present a new archival project, SuperBoRG, which aims at compiling data taken in extragalactic parallel programs of HST with the Wide Field Camera 3 in the past decade, including pure-parallel (BoRG, HIPPIES, and COS-GTO) and coordinated-parallel (CLASH and RELICS) programs. The total effective area reaches ~0.41deg^2^ from 4.1Ms, or 47days, of observing time, which is the largest collection of optical-to-near-infrared imaging data of HST for extragalactic science. We reduce all data in a consistent manner with an updated version of our data reduction pipeline, including a new sky background subtraction step. When available, imaging data from the Spitzer Space Telescope are also included in photometric analyses. The data set consists of 316 independent sight lines and is highly effective for identification of high-z luminous sources (M_UV_&lt;~-20mag) at z~7-12, helping to minimize the effects of cosmic variance. As a demonstration, we present three new z&gt;~7 source candidates, including one luminous galaxy candidate at z_phot_~10.4 with M_UV_~-21.9mag; the best-fit spectral energy distribution implies a large amount of stellar mass (logM_*_/M_{sun}_~10) and moderate dust attenuation (A_V_~1.4mag), though the possibility of it being a low-z interloper cannot be completely rejected (~23%) with the current data set. The data set presented in this study is also suited for intermediate- and low-z science cases.</description><source format="bibcode">2021ApJS..253....4M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/253/4</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/120/2747">J/AJ/120/2747 : HDF-South WFPC2 observations (Casertano+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/926">J/AJ/132/926 : Galaxies in the Hubble Ultra Deep Field (Coe+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/418/2074">J/MNRAS/418/2074 : Robust sample of galaxies at 6.0&lt;z&lt;8.7 (Mclure+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/25">J/ApJS/199/25 : CLASH sources for MACS1149.6+2223 (Postman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/203/24">J/ApJS/203/24 : Structural param. of galaxies in CANDELS (van der Wel+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/427/1666">J/MNRAS/427/1666 : Massive galaxies in CANDELS-UDS field (Bruce+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/440/2810">J/MNRAS/440/2810 : Galaxy luminosity function at z =~ 7 (Bowler+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/77">J/ApJ/788/77 : MW L/T/M-dwarfs identified in BoRG survey (Holwerda+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/803/34">J/ApJ/803/34 : z~4-10 galaxies from HST legacy fields (Bouwens+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/71">J/ApJ/810/71 : UV mag of candidate galaxies at 3~&lt;z~&lt;8.5 (Finkelstein+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/812/114">J/ApJ/812/114 : Grism Lens-Amplified Survey from Space. I. (Treu+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/590/A31">J/A+A/590/A31 : ASTRODEEP Frontier Fields Catalogues (Merlin+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/33">J/ApJS/224/33 : CLASH-VLT: the FF cluster MACS J0416.1-2403 (Balestra+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/254">J/ApJ/835/254 : GLASS. IX. Data from HFF &amp; GLASS (Morishita+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/619/A136">J/A+A/619/A136 : VLT/X-SHOOTER spectrum of COLA1 (Matthee+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/884/85">J/ApJ/884/85 : RELICS: Reionization Lensing Cluster Survey (Coe+, 2019)</relatedResource><relatedResource>http://www.stsci.edu/~tmorishita/superborg/ : SuperBoRG home page</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/253/4</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/253/4</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/253/4</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/253/4</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/253/4</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/253/4</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJS/253/4/table1 (Limiting magnitudes for the SuperBORG fields)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/253/4/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/253/4/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/253/4/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>84.88</ra><dec>-64.15</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/0 97 134 158 524 1171 2240 2335 2488 2519 2737 4103 4107 4373 4376 4394 4821 4824 4964 4966 4989 5099 5119 5200-5201 5203 5246 5274 5283 5353 5363 5414 5420 5437 5502 5529 5551 5613 5639 5669 5715 5811 5817 5820 5831 5881 5884 5974 6020-6021 6081 6219 6223 6235 6383 6438 6441 6459 6488 6492 6539 6620 7252 7280 7309 7387 7456 7768 7902 7904 7998 8205 8282 8303-8304 8340 8486 8755 8921 8952 9019 9052 9201 9260 9457 9459 9476 9498 9604 9628 9643 9660 9717 9943 10055 10265 10401 10433 10548 10654-10655 10659 10664 10707 10764 10854 10873 10940 11209 11398 11435 11456 12047 12380 12644 13026 16702 16712 16836 16947 17125 17457 17502 17518 17730 18021 18409 18496 18581 18666-18667 18726 18770 18777 18786 18800 18976 19036 19097 19147 19700 20735 21126 22289 22309 22330 22771 23078 23173 25132 25188 25194 25451 25472 25673 25675 25885 25926 25932 25954 25979 26024 26036 26090 26177 26214 26287 26452-26453 26555 26858-26859 26929 26973 26975 26977 27075 27115 27158 27305 27409 27436 27513 27607 27648 27719 27788 27924 27965 27975 28065 28141 28164 28201 28346 28395 28400 28426 28517 28535 28548 28571 28583 28622 28641 31216 31546 31649 31663 31679 32335 32948 33192 33297 33304 33317 33586 33795-33796 33813 33950 33966 34533 34793 35147 35164 35483 35576 35631 36554 36700 36846 37382 38380 38464 38916 40274 41014 42704 44208 44245 44470 44658 44817 44920 45669 46076 46130 46363 46418 46474 46566 46647 47353 47919 48076 48178 48423 48434 48933 48965 49012</spatial><spectral>3.9193497546148093e-20 4.780735699255511e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/253/4?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJS/253/4/table1</name><description>Limiting magnitudes for the SuperBORG fields</description><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>Survey</name><description>Survey identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Field</name><description>Field identifier (HHMM+DDMM)</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>F350LP</name><description>[24.5/28]? HST/WFC3 F350LP band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F600LP</name><description>[25.2/27.3]? HST/WFC3 F600LP band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F606W</name><description>[25.8/28.3]? HST/WFC3 F606W band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>[24.5/26.6]? HST/WFC3 F814W band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F098M</name><description>[25.2/28.2]? HST/WFC3 F098M band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F105W</name><description>[24/27.7]? HST/WFC3 F105W band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F125W</name><description>[24/28.1]? HST/WFC3 F125W band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F140W</name><description>[24.1/27.5]? HST/WFC3 F140W band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F160W</name><description>[23.9/27.6] HST/WFC3 F160W band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>IRAC1</name><description>[22.8/24.4]? Spitzer/IRAC 3.6 micron band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>IRAC2</name><description>[22.8/24.4]? Spitzer/IRAC 4.5 micron band 5{sigma}-limiting magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>