Can CMB surveys help the AGN community?

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dc.contributor Aalto-yliopisto fi
dc.contributor Aalto University en
dc.contributor.author Partridge, Bruce
dc.contributor.author Bonavera, Laura
dc.contributor.author López-Caniego, Marcos
dc.contributor.author Datta, Rahul
dc.contributor.author Gonzalez-Nuevo, Joaquin
dc.contributor.author Gralla, Megan
dc.contributor.author Herranz, Diego
dc.contributor.author Lähteenmäki, Anne
dc.contributor.author Mocanu, Laura
dc.contributor.author Prince, Heather
dc.contributor.author Vieira, Joaquin
dc.contributor.author Whitehorn, Nathan
dc.contributor.author Zhang, Lizhong
dc.date.accessioned 2017-11-21T13:38:59Z
dc.date.available 2017-11-21T13:38:59Z
dc.date.issued 2017-08-30
dc.identifier.citation Partridge , B , Bonavera , L , López-Caniego , M , Datta , R , Gonzalez-Nuevo , J , Gralla , M , Herranz , D , Lähteenmäki , A , Mocanu , L , Prince , H , Vieira , J , Whitehorn , N & Zhang , L 2017 , ' Can CMB surveys help the AGN community? ' Galaxies , vol 5 , no. 3 , 47 . DOI: 10.3390/galaxies5030047 en
dc.identifier.issn 2075-4434
dc.identifier.other PURE UUID: c6dfd75c-1df9-4b33-8660-87923a15465c
dc.identifier.other PURE ITEMURL: https://research.aalto.fi/en/publications/can-cmb-surveys-help-the-agn-community(c6dfd75c-1df9-4b33-8660-87923a15465c).html
dc.identifier.other PURE LINK: http://www.scopus.com/inward/record.url?scp=85031004462&partnerID=8YFLogxK
dc.identifier.other PURE FILEURL: https://research.aalto.fi/files/15870396/partridge_et_al_galaxies_05_00047_v2.pdf
dc.identifier.uri https://aaltodoc.aalto.fi/handle/123456789/28860
dc.description.abstract Contemporary projects to measure anisotropies in the cosmic microwave background (CMB) are now detecting hundreds to thousands of extragalactic radio sources, most of them blazars. As a member of a group of CMB scientists involved in the construction of catalogues of such sources and their analysis, I wish to point out the potential value of CMB surveys to studies of AGN jets and their polarization. Current CMB projects, for instance, reach mJy sensitivity, offer wide sky coverage, are "blind" and generally of uniform sensitivity across the sky (hence useful statistically), make essentially simultaneous multi-frequency observations at frequencies from 30 to 857 GHz, routinely offer repeated observations of sources with interesting cadences and now generally provide polarization measurements. The aim here is not to analyze in any depth the AGN science already derived from such projects, but rather to heighten awareness of their promise for the AGN community. en
dc.format.extent 6
dc.format.mimetype application/pdf
dc.language.iso en en
dc.relation.ispartofseries Galaxies en
dc.relation.ispartofseries Volume 5, issue 3 en
dc.rights openAccess en
dc.subject.other Astronomy and Astrophysics en
dc.subject.other 115 Astronomy and space science en
dc.title Can CMB surveys help the AGN community? en
dc.type A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä fi
dc.description.version Peer reviewed en
dc.contributor.department Haverford College
dc.contributor.department University of Oviedo
dc.contributor.department European Space Astronomy Centre
dc.contributor.department NASA Goddard Space Flight Center
dc.contributor.department University of Arizona
dc.contributor.department Universidad de Cantabria
dc.contributor.department Metsähovi Radio Observatory
dc.contributor.department University of Chicago
dc.contributor.department Princeton University
dc.contributor.department University of Illinois at Urbana-Champaign
dc.contributor.department University of California at Los Angeles
dc.subject.keyword Active galactic nuclei
dc.subject.keyword Cosmic microwave background
dc.subject.keyword Extragalactic radio sources
dc.subject.keyword Polarized emission
dc.subject.keyword Astronomy and Astrophysics
dc.subject.keyword 115 Astronomy and space science
dc.identifier.urn URN:NBN:fi:aalto-201711217681
dc.identifier.doi 10.3390/galaxies5030047
dc.type.version publishedVersion


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