J/ApJ/900/55ivo://CDS.VizieR/J/ApJ/900/55doi:10.26093/cds/vizier.19000055CDSEverett W.B.Zhang L.Crawford T.M.Vieira J.D.Aravena M.,Archipley M.A.Austermann J.E.Benson B.A.Bleem L.E.Carlstrom J.E.,Chang C.L.Chapman S.Crites A.T.de Haan T.Dobbs M.A.George E.M.,Halverson N.W.Harrington N.Holder G.P.Holzapfel W.L.Hrubes J.D.,Knox L.Lee A.T.Luong-Van D.Mangian A.C.Marrone D.P.McMahon J.J.,Meyer S.S.Mocanu L.M.Mohr J.J.Natoli T.Padin S.Pryke C.,Reichardt C.L.Reuter C.A.Ruhl J.E.Sayre J.T.Schaffer K.K.,Shirokoff E.Spilker J.S.Stalder B.Staniszewski Z.Stark A.A.,Story K.T.Switzer E.R.Vanderlinde K.Weiss A.Williamson R.2022-03-21T09:29:14Z2022-01-12T08:42:00ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmillimeter-astronomyphotometrysubmillimeter-astronomyradio-galaxiesredshiftedsurveysWe present a catalog of emissive point sources detected in the SPT-SZ survey, a contiguous 2530 square degree area surveyed with the South Pole Telescope (SPT) from 2008-2011 in three bands centered at 95, 150, and 220GHz. The catalog contains 4845 sources measured at a significance of 4.5{sigma} or greater in at least one band, corresponding to detections above approximately 9.8, 5.8, and 20.4mJy in 95, 150, and 220GHz, respectively. The spectral behavior in the SPT bands is used for source classification into two populations based on the underlying physical mechanisms of compact, emissive sources that are bright at millimeter wavelengths: synchrotron radiation from active galactic nuclei and thermal emission from dust. The latter population includes a component of high-redshift sources often referred to as submillimeter galaxies (SMGs). In the relatively bright flux ranges probed by the survey, these sources are expected to be magnified by strong gravitational lensing. The survey also contains sources consistent with protoclusters, groups of dusty galaxies at high redshift undergoing collapse. We cross-match the SPT-SZ catalog with external catalogs at radio, infrared, and X-ray wavelengths and identify available redshift information. The catalog splits into 3980 synchrotron-dominated and 865 dust-dominated sources, and we determine a list of 506 SMGs. Ten sources in the catalog are identified as stars. We calculate number counts for the full catalog, and synchrotron and dusty components, using a bootstrap method and compare our measured counts with models. This paper represents the third and final catalog of point sources in the SPT-SZ survey.2020ApJ...900...55Ehttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/900/55CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/156 : IRAS Faint Source Catalog, |b|>10, Version 2.0 (Moshir+ 1989)VIII/38 : The Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996)IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)IX/29 : ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000)VII/221 : PSCz catalog (Saunders+, 2000)VIII/78 : Sydney University Molonglo Sky Survey (SUMSS) (Mauch+ 2006)VIII/81 : Sydney University Molonglo Sky Survey (SUMSS V2.1) (Mauch+ 2008)II/297 : AKARI/IRC mid-IR all-sky Survey (ISAS/JAXA, 2010)II/298 : AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010)II/311 : WISE All-Sky Data Release (Cutri+ 2012)II/328 : AllWISE Data Release (Cutri+ 2013)J/A+A/363/887 : High frequency peakers. I. Bright sample (Dallacasa+, 2000)J/MNRAS/372/1621 : SCUBA Half-Degree Extragalactic Survey. II (Coppin+, 2006)J/MNRAS/380/199 : SCUBA Half-Degree Extragalactic Survey. III (Ivison+, 2007)J/ApJS/178/280 : Compendium of ISO far-IR extragalactic data (Brauher+, 2008)J/AN/330/223 : High frequency peakers. Faint sample (Stanghellini+, 2009)J/MNRAS/401/160 : AzTEC survey of the SHADES fields. I. (Austermann+, 2010)J/MNRAS/402/2403 : Australia Telescope 20GHz Survey Cat., AT20G (Murphy+, 2010)J/ApJ/719/763 : Millimeter-wave sources in the SPT survey (Vieira+, 2010)J/ApJ/779/61 : SPT-SZ point sources at 95, 150 & 220GHz (Mocanu+, 2013)J/ApJS/216/27 : Galaxy clusters in the SPT-SZ survey (Bleem+, 2015)J/A+A/594/A26 : 2nd Planck Cat. of Compact Sources (PCCS2) (Planck+, 2016)J/MNRAS/465/1789 : SCUBA-2 Cosmology Legacy Survey (Geach+, 2017)J/A+A/619/A94 : Planck Multi-frequences Non-thermal Sources (Planck+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/900/55https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/900/55http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/900/55https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/900/55https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/900/55http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/900/55GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/900/55/table4 (*The SPT-SZ multiband catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/900/55/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/900/55/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/900/55/table4?GETtext/xml+votable180.050000true0.101-45.2250.0055555555555555564/2097 2116 2442 2882 2886-2888 5/8285-8286 8301 8303 8305-8307 8310-8311 8313 8315 8317 8349-8350 8365 8368-8369 8373 8375-8376 8379-8381 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11654-11655 11657 11664-11665 11667 11681-11682 11686 11690 11696 11840 11845 11847 11853-11855 11860 11866 12032 6/16385 16392 20481 33116-33117 33133-33135 33137 33139 33148 33150-33151 33181 33183 33191 33197-33199 33201-33203 33208 33210-33211 33217-33218 33232-33234 33237-33239 33249-33251 33256 33258-33259 33265-33267 33272-33273 33279 33372 33375 33390-33391 33393 33395 33405-33407 33437 33439 33447 33454-33456 33458-33459 33464 33466-33468 33471 33481-33485 33488-33489 33491 33497-33498 33509 33511-33512 33514-33515 33528 33530 33533-33535 33548-33549 33551 33569-33571 33573-33575 33580 33582-33586 33592 33594 33596 33598-33599 33604 33606 33609-33611 33618-33619 33621-33622 33629 33631 33640 33642-33643 33652 33654 33669-33671 33677-33681 33683-33684 33687 33692-33693 33697-33700 33702-33703 33710-33712 33714-33715 33717 33719-33720 33722-33724 33726 33733-33736 33738-33742 33744-33745 33752 33754-33756 33758-33762 33764 33766-33769 33771 33776-33777 33779 33784 33787 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45496-45498 45505-45507 45509-45511 45521-45523 45525 45527-45529 45531 45534-45535 45540 45542-45543 45545-45547 45553 45555-45556 45558 45560-45562 45663 45677 45681 45683-45684 45686-45690 45693-45695 45776-45777 45779 45787 45821 45826-45827 45836-45837 45839 45846-45847 45849-45851 45861-45864 45866 45869-45870 45872 45874-45878 45884-45885 45887 45889-45891 45895 45900 45902-45903 45912 45914-45915 45917-45919 45921-45923 45928 45930-45933 45935 45941-45943 45950 45960-45962 45964-45966 45968-45969 45971-45973 45984-45985 45987 45989 45991-45993 46008-46009 46011-46013 46015 46020-46021 46023-46024 46029-46033 46035-46036 46039 46044 46048-46049 46052 46054-46055 46057-46059 46064-46065 46067-46068 46070 46074-46075 46081-46083 46085 46087 46097 46099 46101-46103 46105-46107 46128-46130 46136-46138 46144-46146 46160-46162 46224-46226 46228 46230-46232 46234 46240 46242 46244 46246-46247 46252-46254 46261 46268-46269 46271-46273 46275 46281-46283 46288-46290 46293-46295 46297-46299 46301 46304 46306 46310-46312 46314-46315 46320-46321 46323-46324 46326-46327 46332 46334-46338 46340-46342 46345-46348 46350-46351 46356-46358 46360 46362-46364 46366-46367 46373-46375 46385-46387 46398-46400 46402 46404-46405 46407 46409-46412 46414 46416 46418-46419 46421-46425 46427 46429 46444-46445 46448-46450 46464 46466-46468 46470 46472-46473 46476-46477 46479 46481 46483 46485-46486 46492-46493 46496 46499 46505-46507 46509-46510 46512-46514 46529-46530 46536 46592 46594-46595 46604 46607 46612-46613 46615 46624 46626-46627 46632-46634 46636 46638-46639 46641-46642 46644 46646-46647 46650-46651 46653-46654 46664-46665 46672-46674 46676 46679 46682-46683 46685-46687 46689 46691-46693 46696 46698-46699 46701-46702 46705 46720-46721 46723 46732 46734 46736 46738-46741 46743 46749 46752 46754 46756-46757 46764-46766 46769-46770 46788 46848 46850 46852 47366 47369 47372-47373 47375-47376 47378 47385-47386 47396-47398 47405 47407-47408 47411 47424 47427-47428 47430-47433 47436 47439 47444-47446 47449-47451 47453-47454 47456-47458 47461-47463 47468-47470 47473 47476 47480 47504-47505 47507-47510 47513 47517 47519 475536.294766091792609e-23 1.4577353054677622e-22https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/900/55?format=asciiMillimeterRadiodefaultJ/ApJ/900/55/table4*The SPT-SZ multiband catalogCtptsCross-match flag(s) (4)meta.codecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSPT-SSource identification (JHHMMSS+DDMM.m)meta.id;meta.maincharRAJ2000Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[-65.31/-39.7] Declination (J2000)degpos.eq.dec;meta.mainSN95[0/2313] Raw signal-to-noise in 95GHzstat.snrfloatS95-raw[-8.3/5952] Raw flux in 95GHzmJyphot.flux.density;em.mm.50-100GHzfloatS95-best[0.03/5959] Deboosted flux in 95GHz (1)mJyphot.flux.density;em.mm.50-100GHzfloatB_S95-best[0.09/6049] Upper 1{sigma} confidence interval on S95-bestmJystat.fit.paramfloatb_S95-best[0.02/5870] Lower 1{sigma} confidence interval on S95-bestmJystat.fit.paramfloatSN150[0.0/3399] Raw signal-to-noise in 150GHzstat.snrfloatS150-raw[-2.8/4827] Raw flux in 150GHzmJyphot.flux.density;em.mm.100-200GHzfloatS150-best[0.03/4843] Deboosted flux in 150GHz (1)mJyphot.flux.density;em.mm.100-200GHzfloatB_S150-best[0.2/4933] Upper 1{sigma} confidence interval on S150-bestmJystat.fit.paramfloatb_S150-best[0.03/4710] Lower 1{sigma} confidence interval on S150-bestmJystat.fit.paramfloatSN220[0/808] Raw signal-to-noise in 220GHzstat.snrfloatS220-raw[-12.6/3915] Raw flux in 220GHzmJyphot.flux.density;em.mm.200-400GHzfloatS220-best[0.09/3906] Deboosted flux in 220GHz (1)mJyphot.flux.density;em.mm.200-400GHzfloatB_S220-best[0.3/4129] Upper 1{sigma} confidence interval on S220-bestmJystat.fit.paramfloatb_S220-best[0.03/3638] Lower 1{sigma} confidence interval on S220-bestmJystat.fit.paramfloatalpha1-raw[-34.2/34.1] Spectral index between 95GHz and 150GHz, raw fluxesspect.indexfloatalpha1-best[-3/4.4] Spectral index between 95GHz and 150GHz, deboosted fluxes (1)spect.indexfloatB_alpha1-best[-2.9/4.8] Upper 1{sigma} confidence interval on alpha1-beststat.fit.paramfloatb_alpha1-best[-3/3.8] Lower 1{sigma} confidence interval on alpha1-beststat.fit.paramfloatalpha2-raw[-46.5/47.7] Spectral index between 150GHz and 220GHz, raw fluxesspect.indexfloatalpha2-best[-2.6/4.9] Spectral index between 150GHz and 220GHz, deboosted fluxes (1)spect.indexfloatB_alpha2-best[-2/5] Upper 1{sigma} confidence interval on alpha2-beststat.fit.paramfloatb_alpha2-best[-2.9/4.8] Lower 1{sigma} confidence interval on alpha2-beststat.fit.paramfloatPpdf[0/1] Spectral index posterior probability distribution above threshold (2)stat.fit.goodnessfloatTypeSource Classification (3)src.classcharExtdExtended source flag ("yes": 122 occurrences) (5)meta.codecharz[1.7e-05/6.9]? Cross-matched redshift from NED, if availablesrc.redshiftfloatnullableCutSource cut flag(s) (6)meta.codechar