Planck early results. VIII. ESZ sample. (Planck+, 2011)

Collaboration Planck; P A R Ade; N Aghanim; M Arnaud; M Ashdown; J Aumont; C Baccigalupi; M Baker; A Balbi; A J Banday; R B Barreiro; J G Bartlett; E Battaner; K Benabed; K Bennett; A Benoit; J P Bernard; M Bersanelli; R Bhatia; J J Bock; A Bonaldi; J R Bond; J Borrill; F R Bouchet; T Bradshaw; M Bremer; M Bucher; C Burigana; R C Butler; P Cabella; C M Cantalupo; B Cappellini; J F Cardoso; R Carr; M Casale; A Catalano; L Cayon; A Challinor; A Chamballu; J Charra; R R Chary; L Y Chiang; C Chiang; P R Christensen; D L Clements; S Colombi; F Couchot; A Coulais; B P Crill; G Crone; M Crook; F Cuttaia; L Danese; O D'Arcangelo; R D Davies; R J Davis; P de Bernardis; J de Bruin; G de Gasperis; A de Rosa; G de Zotti; J Delabrouille; J M Delouis; F X Desert; J Dick; C Dickinson; K Dolag; H Dole; S Donzelli; O Dore; U Doerl; M Douspis; X Dupac; G Efstathiou; T A Ensslin; H K Eriksen; F Finelli

Planck early results. VIII. ESZ sample. (Planck+, 2011)

Collaboration Planck, P A R Ade, N Aghanim, M Arnaud, M Ashdown, J Aumont, C Baccigalupi, M Baker, A Balbi, A J Banday, R B Barreiro, J G Bartlett, E Battaner, K Benabed, K Bennett, A Benoit, J P Bernard, M Bersanelli, R Bhatia, J J BockA Bonaldi, J R Bond, J Borrill, F R Bouchet, T Bradshaw, M Bremer, M Bucher, C Burigana, R C Butler, P Cabella, C M Cantalupo, B Cappellini, J F Cardoso, R Carr, M Casale, A Catalano, L Cayon, A Challinor, A Chamballu, J Charra, R R Chary, L Y Chiang, C Chiang, P R Christensen, D L Clements, S Colombi, F Couchot, A Coulais, B P Crill, G Crone, M Crook, F Cuttaia, L Danese, O D'Arcangelo, R D Davies, R J Davis, P de Bernardis, J de Bruin, G de Gasperis, A de Rosa, G de Zotti, J Delabrouille, J M Delouis, F X Desert, J Dick, C Dickinson, K Dolag, H Dole, S Donzelli, O Dore, U Doerl, M Douspis, X Dupac, G Efstathiou, T A Ensslin, H K Eriksen, F Finelli

Research output: Contribution to journal › Article › peer-review

Abstract

We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ (ESZ) sample is comprised of 189 candidates, which have a high signal-to-noise ratio ranging from 6 to 29. Its high reliability (purity above 95%) is further ensured by an extensive validation process based on Planck internal quality assessments and by external cross-identification and follow-up observations. Planck provides the first measured SZ signal for about 80% of the 169 previously-known ESZ clusters. Planck furthermore releases 30 new cluster candidates, amongst which 20 meet the ESZ signal-to-noise selection criterion. At the submission date, twelve of the 20 ESZ candidates were confirmed as new clusters, with eleven confirmed using XMM-Newton snapshot observations, most of them with disturbed morphologies and low luminosities. The ESZ clusters are mostly at moderate redshifts (86% with z below 0.3) and span more than a decade in mass, up to the rarest and most massive clusters with masses above 1x10¹⁵M_âŠ™. (1 data file).

Original language	English
Journal	VizieR Online Data Catalog
Volume	353
Publication status	Published - 2012

Keywords

Clusters: galaxy
Redshifts

Access to Document

http://adsabs.harvard.edu/abs/2012yCat..35369008P

Cite this

Planck, C., Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Baker, M., Balbi, A., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Battaner, E., Benabed, K., Bennett, K., Benoit, A., Bernard, J. P., Bersanelli, M., Bhatia, R., ... Finelli, F. (2012). Planck early results. VIII. ESZ sample. (Planck+, 2011). VizieR Online Data Catalog, 353. http://adsabs.harvard.edu/abs/2012yCat..35369008P

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title = "Planck early results. VIII. ESZ sample. (Planck+, 2011)",

abstract = "We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ (ESZ) sample is comprised of 189 candidates, which have a high signal-to-noise ratio ranging from 6 to 29. Its high reliability (purity above 95%) is further ensured by an extensive validation process based on Planck internal quality assessments and by external cross-identification and follow-up observations. Planck provides the first measured SZ signal for about 80% of the 169 previously-known ESZ clusters. Planck furthermore releases 30 new cluster candidates, amongst which 20 meet the ESZ signal-to-noise selection criterion. At the submission date, twelve of the 20 ESZ candidates were confirmed as new clusters, with eleven confirmed using XMM-Newton snapshot observations, most of them with disturbed morphologies and low luminosities. The ESZ clusters are mostly at moderate redshifts (86% with z below 0.3) and span more than a decade in mass, up to the rarest and most massive clusters with masses above 1x1015M{\^a}{\v S}{\texttrademark}. (1 data file).",

keywords = "Clusters: galaxy, Redshifts",

author = "Collaboration Planck and Ade, {P A R} and N Aghanim and M Arnaud and M Ashdown and J Aumont and C Baccigalupi and M Baker and A Balbi and Banday, {A J} and Barreiro, {R B} and Bartlett, {J G} and E Battaner and K Benabed and K Bennett and A Benoit and Bernard, {J P} and M Bersanelli and R Bhatia and Bock, {J J} and A Bonaldi and Bond, {J R} and J Borrill and Bouchet, {F R} and T Bradshaw and M Bremer and M Bucher and C Burigana and Butler, {R C} and P Cabella and Cantalupo, {C M} and B Cappellini and Cardoso, {J F} and R Carr and M Casale and A Catalano and L Cayon and A Challinor and A Chamballu and J Charra and Chary, {R R} and Chiang, {L Y} and C Chiang and Christensen, {P R} and Clements, {D L} and S Colombi and F Couchot and A Coulais and Crill, {B P} and G Crone and M Crook and F Cuttaia and L Danese and O D'Arcangelo and Davies, {R D} and Davis, {R J} and {de Bernardis}, P and {de Bruin}, J and {de Gasperis}, G and {de Rosa}, A and {de Zotti}, G and J Delabrouille and Delouis, {J M} and Desert, {F X} and J Dick and C Dickinson and K Dolag and H Dole and S Donzelli and O Dore and U Doerl and M Douspis and X Dupac and G Efstathiou and Ensslin, {T A} and Eriksen, {H K} and F Finelli",

note = "tablea1.dat 189x98 *The Early Sunyaev-Zeldovich (ESZ) sample",

year = "2012",

language = "English",

volume = "353",

journal = "VizieR Online Data Catalog",

}

Planck, C, Ade, PAR, Aghanim, N, Arnaud, M, Ashdown, M, Aumont, J, Baccigalupi, C, Baker, M, Balbi, A, Banday, AJ, Barreiro, RB, Bartlett, JG, Battaner, E, Benabed, K, Bennett, K, Benoit, A, Bernard, JP, Bersanelli, M, Bhatia, R, Bock, JJ, Bonaldi, A, Bond, JR, Borrill, J, Bouchet, FR, Bradshaw, T, Bremer, M, Bucher, M, Burigana, C, Butler, RC, Cabella, P, Cantalupo, CM, Cappellini, B, Cardoso, JF, Carr, R, Casale, M, Catalano, A, Cayon, L, Challinor, A, Chamballu, A, Charra, J, Chary, RR, Chiang, LY, Chiang, C, Christensen, PR, Clements, DL, Colombi, S, Couchot, F, Coulais, A, Crill, BP, Crone, G, Crook, M, Cuttaia, F, Danese, L, D'Arcangelo, O, Davies, RD, Davis, RJ, de Bernardis, P, de Bruin, J, de Gasperis, G, de Rosa, A, de Zotti, G, Delabrouille, J, Delouis, JM, Desert, FX, Dick, J, Dickinson, C, Dolag, K, Dole, H, Donzelli, S, Dore, O, Doerl, U, Douspis, M, Dupac, X, Efstathiou, G, Ensslin, TA, Eriksen, HK & Finelli, F 2012, 'Planck early results. VIII. ESZ sample. (Planck+, 2011)', VizieR Online Data Catalog, vol. 353. <http://adsabs.harvard.edu/abs/2012yCat..35369008P>

TY - JOUR

T1 - Planck early results. VIII. ESZ sample. (Planck+, 2011)

AU - Planck, Collaboration

AU - Ade, P A R

AU - Aghanim, N

AU - Arnaud, M

AU - Ashdown, M

AU - Aumont, J

AU - Baccigalupi, C

AU - Baker, M

AU - Balbi, A

AU - Banday, A J

AU - Barreiro, R B

AU - Bartlett, J G

AU - Battaner, E

AU - Benabed, K

AU - Bennett, K

AU - Benoit, A

AU - Bernard, J P

AU - Bersanelli, M

AU - Bhatia, R

AU - Bock, J J

AU - Bonaldi, A

AU - Bond, J R

AU - Borrill, J

AU - Bouchet, F R

AU - Bradshaw, T

AU - Bremer, M

AU - Bucher, M

AU - Burigana, C

AU - Butler, R C

AU - Cabella, P

AU - Cantalupo, C M

AU - Cappellini, B

AU - Cardoso, J F

AU - Carr, R

AU - Casale, M

AU - Catalano, A

AU - Cayon, L

AU - Challinor, A

AU - Chamballu, A

AU - Charra, J

AU - Chary, R R

AU - Chiang, L Y

AU - Chiang, C

AU - Christensen, P R

AU - Clements, D L

AU - Colombi, S

AU - Couchot, F

AU - Coulais, A

AU - Crill, B P

AU - Crone, G

AU - Crook, M

AU - Cuttaia, F

AU - Danese, L

AU - D'Arcangelo, O

AU - Davies, R D

AU - Davis, R J

AU - de Bernardis, P

AU - de Bruin, J

AU - de Gasperis, G

AU - de Rosa, A

AU - de Zotti, G

AU - Delabrouille, J

AU - Delouis, J M

AU - Desert, F X

AU - Dick, J

AU - Dickinson, C

AU - Dolag, K

AU - Dole, H

AU - Donzelli, S

AU - Dore, O

AU - Doerl, U

AU - Douspis, M

AU - Dupac, X

AU - Efstathiou, G

AU - Ensslin, T A

AU - Eriksen, H K

AU - Finelli, F

N1 - tablea1.dat 189x98 *The Early Sunyaev-Zeldovich (ESZ) sample

PY - 2012

Y1 - 2012

N2 - We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ (ESZ) sample is comprised of 189 candidates, which have a high signal-to-noise ratio ranging from 6 to 29. Its high reliability (purity above 95%) is further ensured by an extensive validation process based on Planck internal quality assessments and by external cross-identification and follow-up observations. Planck provides the first measured SZ signal for about 80% of the 169 previously-known ESZ clusters. Planck furthermore releases 30 new cluster candidates, amongst which 20 meet the ESZ signal-to-noise selection criterion. At the submission date, twelve of the 20 ESZ candidates were confirmed as new clusters, with eleven confirmed using XMM-Newton snapshot observations, most of them with disturbed morphologies and low luminosities. The ESZ clusters are mostly at moderate redshifts (86% with z below 0.3) and span more than a decade in mass, up to the rarest and most massive clusters with masses above 1x1015MâŠ™. (1 data file).

AB - We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ (ESZ) sample is comprised of 189 candidates, which have a high signal-to-noise ratio ranging from 6 to 29. Its high reliability (purity above 95%) is further ensured by an extensive validation process based on Planck internal quality assessments and by external cross-identification and follow-up observations. Planck provides the first measured SZ signal for about 80% of the 169 previously-known ESZ clusters. Planck furthermore releases 30 new cluster candidates, amongst which 20 meet the ESZ signal-to-noise selection criterion. At the submission date, twelve of the 20 ESZ candidates were confirmed as new clusters, with eleven confirmed using XMM-Newton snapshot observations, most of them with disturbed morphologies and low luminosities. The ESZ clusters are mostly at moderate redshifts (86% with z below 0.3) and span more than a decade in mass, up to the rarest and most massive clusters with masses above 1x1015MâŠ™. (1 data file).

KW - Clusters: galaxy

KW - Redshifts

M3 - Article

VL - 353

JO - VizieR Online Data Catalog

JF - VizieR Online Data Catalog

ER -

Planck early results. VIII. ESZ sample. (Planck+, 2011)

Abstract

Keywords

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