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Resource Record Summary

Catalog Service:
SPT-SZ survey point sources at 95, 150 & 220GHz

Short name: J/ApJ/779/61
IVOA Identifier: ivo://CDS.VizieR/J/ApJ/779/61
DOI (Digital Object Identifier): 10.26093/cds/vizier.17790061
Publisher: CDSivo://CDS[Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/779/61
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2015 Jun 09 15:38:11Z
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Description


We present a point-source catalog from 771deg^2^ of the South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) survey at 95, 150, and 220GHz. We detect 1545 sources above 4.5{sigma} significance in at least one band. Based on their relative brightness between survey bands, we classify the sources into two populations, one dominated by synchrotron emission from active galactic nuclei, and one dominated by thermal emission from dust-enshrouded star-forming galaxies. We find 1238 synchrotron and 307 dusty sources. We cross-match all sources against external catalogs and find 189 unidentified synchrotron sources and 189 unidentified dusty sources. The dusty sources without counterparts are good candidates for high-redshift, strongly lensed submillimeter galaxies. We derive number counts for each population from 1Jy down to roughly 11, 4, and 11mJy at 95, 150, and 220GHz. We compare these counts with galaxy population models and find that none of the models we consider for either population provide a good fit to the measured counts in all three bands. The disparities imply that these measurements will be an important input to the next generation of millimeter-wave extragalactic source population models.

More About this Resource

About the Resource Providers

This section describes who is responsible for this resource

Publisher: CDSivo://CDS[Pub. ID]

Creators:
Mocanu L.M.Crawford T.M.Vieira J.D.Aird K.A.Aravena M.Austermann J.E.Benson B.A.Bethermin M.Bleem L.E.Bothwell M.Carlstrom J.E.Chang C.L.Chapman S.Cho H.-M.Crites A.T.de Haan T.Dobbs M.A.Everett W.B.George E.M.Halverson N.W.Harrington N.Hezaveh Y.Holder G.P.Holzapfel W.L.Hoover S.Hrubes J.D.Keisler R.Knox L.Lee A.T.Leitch E.M.Lueker M.Luong-Van D.Marrone D.P.McMahon J.J.Mehl J.Meyer S.S.Mohr J.J.Montroy T.E.Natoli T.Padin S.Plagge T.Pryke C.Rest A.Reichardt C.L.Ruhl J.E.Sayre J.T.Schaffer K.K.Shirokoff E.Spieler H.G.Spilker J.S.Stalder B.Staniszewski Z.Stark A.A.Story K.T.Switzer E.R.Vanderlinde K.Williamson R.

Contact Information:
X CDS support team
Email: cds-question at unistra.fr
Address: CDS
Observatoire de Strasbourg
11 rue de l'Universite
F-67000 Strasbourg
France

Status of This Resource

This section provides some status information: the resource version, availability, and relevant dates.

Version: n/a
Availability: This is an active resource.
  • This service provides only public data.
Relevant dates for this Resource:
  • Updated: 2017 Dec 22 05:32:55Z
  • Created: 2015 Jun 09 15:38:11Z

This resource was registered on: 2015 Jun 09 15:38:11Z
This resource description was last updated on: 2021 Oct 21 00:00:00Z

What This Resource is About

This section describes what the resource is, what it contains, and how it might be relevant.

Resource Class: CatalogService
This resource is a service that provides access to catalog data. You can extract data from the catalog by issuing a query, and the matching data is returned as a table.
Resource type keywords:
  • Catalog
Subject keywords:
  • Millimeter astronomy
  • Submillimeter astronomy
  • Radio astronomy
  • Radio sources
  • Surveys
Intended audience or use:
  • Research: This resource provides information appropriate for supporting scientific research.
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/779/61 Literature Reference: 2013ApJ...779...61M

Related Resources:

Other Related Resources
TAP VizieR generic service(IsServedBy) ivo://CDS.VizieR/TAP [Res. ID]
Conesearch service(IsServedBy)
VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013) ivo://CDS.VizieR/VIII/91 [Res. ID]

Data Coverage Information

This section describes the data's coverage over the sky, frequency, and time.

Wavebands covered:

  • Radio

Rights and Usage Information

This section describes the rights and usage information for this data.

Rights:

Available Service Interfaces

Custom Service

This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.

VO Compliance: Level 2: This is a VO-compliant resource.
Available endpoints for this service interface:
Custom Service

This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.

VO Compliance: Level 2: This is a VO-compliant resource.
Available endpoints for this service interface:
  • URL-based interface: http://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/779/61
Table Access Protocol - Auxiliary ServiceXX

This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.

VO Compliance: Level 2: This is a VO-compliant resource.
Available endpoints for the standard interface:
  • http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Simple Cone SearchXXSearch Me

This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.

VO Compliance: Level 2: This is a VO-compliant resource.
Description:
Cone search capability for table J/ApJ/779/61/table4 (SPT-SZ 771-square-degree point source catalog)
Available endpoints for the standard interface:
  • http://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/779/61/table4?
Maximum search radius accepted: 180.0 degrees
Maximum number of matching records returned: 50000
This service supports the VERB input parameter:
Use VERB=1 to minimize the returned columns or VERB=3 to maximize.


Developed with the support of the National Science Foundation
under Cooperative Agreement AST0122449 with the Johns Hopkins University
The NAVO project is a member of the International Virtual Observatory Alliance

This NAVO Application is hosted by the Space Telescope Science Institute

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