Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey
We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field I...
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Gespeichert in:
| Autor*in: |
L.E. Bleem [verfasserIn] M. Klein [verfasserIn] T. M. C. Abbott [verfasserIn] P. A. R. Ade [verfasserIn] M. Aguena [verfasserIn] O. Alves [verfasserIn] A. J. Anderson [verfasserIn] F. Andrade-Oliveira [verfasserIn] B. Ansarinejad [verfasserIn] M. Archipley [verfasserIn] M. L. N. Ashby [verfasserIn] J. E. Austermann [verfasserIn] D. Bacon [verfasserIn] J. A. Beall [verfasserIn] A. N. Bender [verfasserIn] B. A. Benson [verfasserIn] F. Bianchini [verfasserIn] S. Bocquet [verfasserIn] D. Brooks [verfasserIn] D. L. Burke [verfasserIn] M. Calzadilla [verfasserIn] J. E. Carlstrom [verfasserIn] A. Carnero Rosell [verfasserIn] J. Carretero [verfasserIn] C. L. Chang [verfasserIn] P. Chaubal [verfasserIn] H. C. Chiang [verfasserIn] T-L. Chou [verfasserIn] R. Citron [verfasserIn] C. Corbett Moran [verfasserIn] M. Costanzi [verfasserIn] T. M. Crawford [verfasserIn] A. T. Crites [verfasserIn] L. N. da Costa [verfasserIn] T. de Haan [verfasserIn] J. De Vicente [verfasserIn] S. Desai [verfasserIn] M. A. Dobbs [verfasserIn] P. Doel [verfasserIn] W. Everett [verfasserIn] I. Ferrero [verfasserIn] B. Flaugher [verfasserIn] B. Floyd [verfasserIn] D. Friedel [verfasserIn] J. Frieman [verfasserIn] J. Gallicchio [verfasserIn] J. Garc'ia-Bellido [verfasserIn] M. Gatti [verfasserIn] E. M. George [verfasserIn] G. Giannini [verfasserIn] S. Grandis [verfasserIn] D. Gruen [verfasserIn] R. A. Gruendl [verfasserIn] N. Gupta [verfasserIn] G. Gutierrez [verfasserIn] N. W. Halverson [verfasserIn] S. R. Hinton [verfasserIn] G. P. Holder [verfasserIn] D. L. Hollowood [verfasserIn] W. L. Holzapfel [verfasserIn] K. Honscheid [verfasserIn] J. D. Hrubes [verfasserIn] N. Huang [verfasserIn] J. Hubmayr [verfasserIn] K. D. Irwin [verfasserIn] J. Mena-Fernández [verfasserIn] D. J. James [verfasserIn] F. Kéruzoré [verfasserIn] L. Knox [verfasserIn] K. Kuehn [verfasserIn] O. Lahav [verfasserIn] A. T. Lee [verfasserIn] S. Lee [verfasserIn] D. Li [verfasserIn] A. Lowitz [verfasserIn] J. L. Marshal [verfasserIn] M. McDonald [verfasserIn] J. J. McMahon [verfasserIn] F. Menanteau [verfasserIn] S. S. Meyer [verfasserIn] R. Miquel [verfasserIn] J. J. Mohr [verfasserIn] J. Montgomery [verfasserIn] J. Myles [verfasserIn] T. Natoli [verfasserIn] J. P. Nibarger [verfasserIn] G. I. Noble [verfasserIn] V. Novosad [verfasserIn] R. L. C. Ogando [verfasserIn] S. Padin [verfasserIn] S. Patil [verfasserIn] M. E. S. Pereira [verfasserIn] A. Pieres [verfasserIn] A. A. Plazas Malag'on [verfasserIn] C. Pryke [verfasserIn] C. L. Reichardt [verfasserIn] M. Rodr'iguez-Monroy [verfasserIn] A. K. Romer [verfasserIn] J. E. Ruhl [verfasserIn] B. R. Saliwanchik [verfasserIn] L. Salvati [verfasserIn] E. Sanchez [verfasserIn] A. Saro [verfasserIn] K. K. Schaffer [verfasserIn] T. Schrabback [verfasserIn] I. Sevilla-Noarbe [verfasserIn] C. Sievers [verfasserIn] G. Smecher [verfasserIn] M. Smith [verfasserIn] T. Somboonpanyakul [verfasserIn] B. Stalder [verfasserIn] A. A. Stark [verfasserIn] E. Suchyta [verfasserIn] M. E. C. Swanson [verfasserIn] G. Tarle [verfasserIn] C. To [verfasserIn] C. Tucker [verfasserIn] T. Veach [verfasserIn] J. D. Vieira [verfasserIn] M. Vincenzi [verfasserIn] G. Wang [verfasserIn] J. Weller [verfasserIn] N. Whitehorn [verfasserIn] P. Wiseman [verfasserIn] W. L. K. Wu [verfasserIn] V. Yefremenko [verfasserIn] J. A. Zebrowski [verfasserIn] Y. Zhang [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2024 |
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| Übergeordnetes Werk: |
In: The Open Journal of Astrophysics - Maynooth Academic Publishing, 2020, 7(2024) |
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| Übergeordnetes Werk: |
volume:7 ; year:2024 |
| Links: |
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| DOI / URN: |
10.21105/astro.2311.07512 |
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| Katalog-ID: |
DOAJ095791493 |
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| 024 | 7 | |a 10.21105/astro.2311.07512 |2 doi | |
| 035 | |a (DE-627)DOAJ095791493 | ||
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| 050 | 0 | |a QB1-991 | |
| 050 | 0 | |a QB460-466 | |
| 100 | 0 | |a L.E. Bleem |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey |
| 264 | 1 | |c 2024 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 520 | |a We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. | ||
| 653 | 0 | |a Astronomy | |
| 653 | 0 | |a Astrophysics | |
| 700 | 0 | |a M. Klein |e verfasserin |4 aut | |
| 700 | 0 | |a T. M. C. Abbott |e verfasserin |4 aut | |
| 700 | 0 | |a P. A. R. Ade |e verfasserin |4 aut | |
| 700 | 0 | |a M. Aguena |e verfasserin |4 aut | |
| 700 | 0 | |a O. Alves |e verfasserin |4 aut | |
| 700 | 0 | |a A. J. Anderson |e verfasserin |4 aut | |
| 700 | 0 | |a F. Andrade-Oliveira |e verfasserin |4 aut | |
| 700 | 0 | |a B. Ansarinejad |e verfasserin |4 aut | |
| 700 | 0 | |a M. Archipley |e verfasserin |4 aut | |
| 700 | 0 | |a M. L. N. Ashby |e verfasserin |4 aut | |
| 700 | 0 | |a J. E. Austermann |e verfasserin |4 aut | |
| 700 | 0 | |a D. Bacon |e verfasserin |4 aut | |
| 700 | 0 | |a J. A. Beall |e verfasserin |4 aut | |
| 700 | 0 | |a A. N. Bender |e verfasserin |4 aut | |
| 700 | 0 | |a B. A. Benson |e verfasserin |4 aut | |
| 700 | 0 | |a F. Bianchini |e verfasserin |4 aut | |
| 700 | 0 | |a S. Bocquet |e verfasserin |4 aut | |
| 700 | 0 | |a D. Brooks |e verfasserin |4 aut | |
| 700 | 0 | |a D. L. Burke |e verfasserin |4 aut | |
| 700 | 0 | |a M. Calzadilla |e verfasserin |4 aut | |
| 700 | 0 | |a J. E. Carlstrom |e verfasserin |4 aut | |
| 700 | 0 | |a A. Carnero Rosell |e verfasserin |4 aut | |
| 700 | 0 | |a J. Carretero |e verfasserin |4 aut | |
| 700 | 0 | |a C. L. Chang |e verfasserin |4 aut | |
| 700 | 0 | |a P. Chaubal |e verfasserin |4 aut | |
| 700 | 0 | |a H. C. Chiang |e verfasserin |4 aut | |
| 700 | 0 | |a T-L. Chou |e verfasserin |4 aut | |
| 700 | 0 | |a R. Citron |e verfasserin |4 aut | |
| 700 | 0 | |a C. Corbett Moran |e verfasserin |4 aut | |
| 700 | 0 | |a M. Costanzi |e verfasserin |4 aut | |
| 700 | 0 | |a T. M. Crawford |e verfasserin |4 aut | |
| 700 | 0 | |a A. T. Crites |e verfasserin |4 aut | |
| 700 | 0 | |a L. N. da Costa |e verfasserin |4 aut | |
| 700 | 0 | |a T. de Haan |e verfasserin |4 aut | |
| 700 | 0 | |a J. De Vicente |e verfasserin |4 aut | |
| 700 | 0 | |a S. Desai |e verfasserin |4 aut | |
| 700 | 0 | |a M. A. Dobbs |e verfasserin |4 aut | |
| 700 | 0 | |a P. Doel |e verfasserin |4 aut | |
| 700 | 0 | |a W. Everett |e verfasserin |4 aut | |
| 700 | 0 | |a I. Ferrero |e verfasserin |4 aut | |
| 700 | 0 | |a B. Flaugher |e verfasserin |4 aut | |
| 700 | 0 | |a B. Floyd |e verfasserin |4 aut | |
| 700 | 0 | |a D. Friedel |e verfasserin |4 aut | |
| 700 | 0 | |a J. Frieman |e verfasserin |4 aut | |
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| 700 | 0 | |a J. Garc'ia-Bellido |e verfasserin |4 aut | |
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| 700 | 0 | |a J. Hubmayr |e verfasserin |4 aut | |
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| 700 | 0 | |a A. T. Lee |e verfasserin |4 aut | |
| 700 | 0 | |a S. Lee |e verfasserin |4 aut | |
| 700 | 0 | |a D. Li |e verfasserin |4 aut | |
| 700 | 0 | |a A. Lowitz |e verfasserin |4 aut | |
| 700 | 0 | |a J. L. Marshal |e verfasserin |4 aut | |
| 700 | 0 | |a M. McDonald |e verfasserin |4 aut | |
| 700 | 0 | |a J. J. McMahon |e verfasserin |4 aut | |
| 700 | 0 | |a F. Menanteau |e verfasserin |4 aut | |
| 700 | 0 | |a S. S. Meyer |e verfasserin |4 aut | |
| 700 | 0 | |a R. Miquel |e verfasserin |4 aut | |
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| 700 | 0 | |a J. P. Nibarger |e verfasserin |4 aut | |
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| 700 | 0 | |a A. Saro |e verfasserin |4 aut | |
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| 700 | 0 | |a J. D. Vieira |e verfasserin |4 aut | |
| 700 | 0 | |a M. Vincenzi |e verfasserin |4 aut | |
| 700 | 0 | |a G. Wang |e verfasserin |4 aut | |
| 700 | 0 | |a J. Weller |e verfasserin |4 aut | |
| 700 | 0 | |a N. Whitehorn |e verfasserin |4 aut | |
| 700 | 0 | |a P. Wiseman |e verfasserin |4 aut | |
| 700 | 0 | |a W. L. K. Wu |e verfasserin |4 aut | |
| 700 | 0 | |a V. Yefremenko |e verfasserin |4 aut | |
| 700 | 0 | |a J. A. Zebrowski |e verfasserin |4 aut | |
| 700 | 0 | |a Y. Zhang |e verfasserin |4 aut | |
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10.21105/astro.2311.07512 doi (DE-627)DOAJ095791493 (DE-599)DOAJ2245da59b4b844f3b03f5152d7d18228 DE-627 ger DE-627 rakwb eng QB1-991 QB460-466 L.E. Bleem verfasserin aut Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. Astronomy Astrophysics M. Klein verfasserin aut T. M. C. Abbott verfasserin aut P. A. R. Ade verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut A. J. Anderson verfasserin aut F. Andrade-Oliveira verfasserin aut B. Ansarinejad verfasserin aut M. Archipley verfasserin aut M. L. N. Ashby verfasserin aut J. E. Austermann verfasserin aut D. Bacon verfasserin aut J. A. Beall verfasserin aut A. N. Bender verfasserin aut B. A. Benson verfasserin aut F. Bianchini verfasserin aut S. Bocquet verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut M. Calzadilla verfasserin aut J. E. Carlstrom verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut C. L. Chang verfasserin aut P. Chaubal verfasserin aut H. C. Chiang verfasserin aut T-L. Chou verfasserin aut R. Citron verfasserin aut C. Corbett Moran verfasserin aut M. Costanzi verfasserin aut T. M. Crawford verfasserin aut A. T. Crites verfasserin aut L. N. da Costa verfasserin aut T. de Haan verfasserin aut J. De Vicente verfasserin aut S. Desai verfasserin aut M. A. Dobbs verfasserin aut P. Doel verfasserin aut W. Everett verfasserin aut I. Ferrero verfasserin aut B. Flaugher verfasserin aut B. Floyd verfasserin aut D. Friedel verfasserin aut J. Frieman verfasserin aut J. Gallicchio verfasserin aut J. Garc'ia-Bellido verfasserin aut M. Gatti verfasserin aut E. M. George verfasserin aut G. Giannini verfasserin aut S. Grandis verfasserin aut D. Gruen verfasserin aut R. A. Gruendl verfasserin aut N. Gupta verfasserin aut G. Gutierrez verfasserin aut N. W. Halverson verfasserin aut S. R. Hinton verfasserin aut G. P. Holder verfasserin aut D. L. Hollowood verfasserin aut W. L. Holzapfel verfasserin aut K. Honscheid verfasserin aut J. D. Hrubes verfasserin aut N. Huang verfasserin aut J. Hubmayr verfasserin aut K. D. Irwin verfasserin aut J. Mena-Fernández verfasserin aut D. J. James verfasserin aut F. Kéruzoré verfasserin aut L. Knox verfasserin aut K. Kuehn verfasserin aut O. Lahav verfasserin aut A. T. Lee verfasserin aut S. Lee verfasserin aut D. Li verfasserin aut A. Lowitz verfasserin aut J. L. Marshal verfasserin aut M. McDonald verfasserin aut J. J. McMahon verfasserin aut F. Menanteau verfasserin aut S. S. Meyer verfasserin aut R. Miquel verfasserin aut J. J. Mohr verfasserin aut J. Montgomery verfasserin aut J. Myles verfasserin aut T. Natoli verfasserin aut J. P. Nibarger verfasserin aut G. I. Noble verfasserin aut V. Novosad verfasserin aut R. L. C. Ogando verfasserin aut S. Padin verfasserin aut S. Patil verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malag'on verfasserin aut C. Pryke verfasserin aut C. L. Reichardt verfasserin aut M. Rodr'iguez-Monroy verfasserin aut A. K. Romer verfasserin aut J. E. Ruhl verfasserin aut B. R. Saliwanchik verfasserin aut L. Salvati verfasserin aut E. Sanchez verfasserin aut A. Saro verfasserin aut K. K. Schaffer verfasserin aut T. Schrabback verfasserin aut I. Sevilla-Noarbe verfasserin aut C. Sievers verfasserin aut G. Smecher verfasserin aut M. Smith verfasserin aut T. Somboonpanyakul verfasserin aut B. Stalder verfasserin aut A. A. Stark verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut C. To verfasserin aut C. Tucker verfasserin aut T. Veach verfasserin aut J. D. Vieira verfasserin aut M. Vincenzi verfasserin aut G. Wang verfasserin aut J. Weller verfasserin aut N. Whitehorn verfasserin aut P. Wiseman verfasserin aut W. L. K. Wu verfasserin aut V. Yefremenko verfasserin aut J. A. Zebrowski verfasserin aut Y. Zhang verfasserin aut In The Open Journal of Astrophysics Maynooth Academic Publishing, 2020 7(2024) (DE-627)1683864301 25656120 nnns volume:7 year:2024 https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/article/2245da59b4b844f3b03f5152d7d18228 kostenfrei https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/toc/2565-6120 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 7 2024 |
| spelling |
10.21105/astro.2311.07512 doi (DE-627)DOAJ095791493 (DE-599)DOAJ2245da59b4b844f3b03f5152d7d18228 DE-627 ger DE-627 rakwb eng QB1-991 QB460-466 L.E. Bleem verfasserin aut Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. Astronomy Astrophysics M. Klein verfasserin aut T. M. C. Abbott verfasserin aut P. A. R. Ade verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut A. J. Anderson verfasserin aut F. Andrade-Oliveira verfasserin aut B. Ansarinejad verfasserin aut M. Archipley verfasserin aut M. L. N. Ashby verfasserin aut J. E. Austermann verfasserin aut D. Bacon verfasserin aut J. A. Beall verfasserin aut A. N. Bender verfasserin aut B. A. Benson verfasserin aut F. Bianchini verfasserin aut S. Bocquet verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut M. Calzadilla verfasserin aut J. E. Carlstrom verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut C. L. Chang verfasserin aut P. Chaubal verfasserin aut H. C. Chiang verfasserin aut T-L. Chou verfasserin aut R. Citron verfasserin aut C. Corbett Moran verfasserin aut M. Costanzi verfasserin aut T. M. Crawford verfasserin aut A. T. Crites verfasserin aut L. N. da Costa verfasserin aut T. de Haan verfasserin aut J. De Vicente verfasserin aut S. Desai verfasserin aut M. A. Dobbs verfasserin aut P. Doel verfasserin aut W. Everett verfasserin aut I. Ferrero verfasserin aut B. Flaugher verfasserin aut B. Floyd verfasserin aut D. Friedel verfasserin aut J. Frieman verfasserin aut J. Gallicchio verfasserin aut J. Garc'ia-Bellido verfasserin aut M. Gatti verfasserin aut E. M. George verfasserin aut G. Giannini verfasserin aut S. Grandis verfasserin aut D. Gruen verfasserin aut R. A. Gruendl verfasserin aut N. Gupta verfasserin aut G. Gutierrez verfasserin aut N. W. Halverson verfasserin aut S. R. Hinton verfasserin aut G. P. Holder verfasserin aut D. L. Hollowood verfasserin aut W. L. Holzapfel verfasserin aut K. Honscheid verfasserin aut J. D. Hrubes verfasserin aut N. Huang verfasserin aut J. Hubmayr verfasserin aut K. D. Irwin verfasserin aut J. Mena-Fernández verfasserin aut D. J. James verfasserin aut F. Kéruzoré verfasserin aut L. Knox verfasserin aut K. Kuehn verfasserin aut O. Lahav verfasserin aut A. T. Lee verfasserin aut S. Lee verfasserin aut D. Li verfasserin aut A. Lowitz verfasserin aut J. L. Marshal verfasserin aut M. McDonald verfasserin aut J. J. McMahon verfasserin aut F. Menanteau verfasserin aut S. S. Meyer verfasserin aut R. Miquel verfasserin aut J. J. Mohr verfasserin aut J. Montgomery verfasserin aut J. Myles verfasserin aut T. Natoli verfasserin aut J. P. Nibarger verfasserin aut G. I. Noble verfasserin aut V. Novosad verfasserin aut R. L. C. Ogando verfasserin aut S. Padin verfasserin aut S. Patil verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malag'on verfasserin aut C. Pryke verfasserin aut C. L. Reichardt verfasserin aut M. Rodr'iguez-Monroy verfasserin aut A. K. Romer verfasserin aut J. E. Ruhl verfasserin aut B. R. Saliwanchik verfasserin aut L. Salvati verfasserin aut E. Sanchez verfasserin aut A. Saro verfasserin aut K. K. Schaffer verfasserin aut T. Schrabback verfasserin aut I. Sevilla-Noarbe verfasserin aut C. Sievers verfasserin aut G. Smecher verfasserin aut M. Smith verfasserin aut T. Somboonpanyakul verfasserin aut B. Stalder verfasserin aut A. A. Stark verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut C. To verfasserin aut C. Tucker verfasserin aut T. Veach verfasserin aut J. D. Vieira verfasserin aut M. Vincenzi verfasserin aut G. Wang verfasserin aut J. Weller verfasserin aut N. Whitehorn verfasserin aut P. Wiseman verfasserin aut W. L. K. Wu verfasserin aut V. Yefremenko verfasserin aut J. A. Zebrowski verfasserin aut Y. Zhang verfasserin aut In The Open Journal of Astrophysics Maynooth Academic Publishing, 2020 7(2024) (DE-627)1683864301 25656120 nnns volume:7 year:2024 https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/article/2245da59b4b844f3b03f5152d7d18228 kostenfrei https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/toc/2565-6120 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 7 2024 |
| allfields_unstemmed |
10.21105/astro.2311.07512 doi (DE-627)DOAJ095791493 (DE-599)DOAJ2245da59b4b844f3b03f5152d7d18228 DE-627 ger DE-627 rakwb eng QB1-991 QB460-466 L.E. Bleem verfasserin aut Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. Astronomy Astrophysics M. Klein verfasserin aut T. M. C. Abbott verfasserin aut P. A. R. Ade verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut A. J. Anderson verfasserin aut F. Andrade-Oliveira verfasserin aut B. Ansarinejad verfasserin aut M. Archipley verfasserin aut M. L. N. Ashby verfasserin aut J. E. Austermann verfasserin aut D. Bacon verfasserin aut J. A. Beall verfasserin aut A. N. Bender verfasserin aut B. A. Benson verfasserin aut F. Bianchini verfasserin aut S. Bocquet verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut M. Calzadilla verfasserin aut J. E. Carlstrom verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut C. L. Chang verfasserin aut P. Chaubal verfasserin aut H. C. Chiang verfasserin aut T-L. Chou verfasserin aut R. Citron verfasserin aut C. Corbett Moran verfasserin aut M. Costanzi verfasserin aut T. M. Crawford verfasserin aut A. T. Crites verfasserin aut L. N. da Costa verfasserin aut T. de Haan verfasserin aut J. De Vicente verfasserin aut S. Desai verfasserin aut M. A. Dobbs verfasserin aut P. Doel verfasserin aut W. Everett verfasserin aut I. Ferrero verfasserin aut B. Flaugher verfasserin aut B. Floyd verfasserin aut D. Friedel verfasserin aut J. Frieman verfasserin aut J. Gallicchio verfasserin aut J. Garc'ia-Bellido verfasserin aut M. Gatti verfasserin aut E. M. George verfasserin aut G. Giannini verfasserin aut S. Grandis verfasserin aut D. Gruen verfasserin aut R. A. Gruendl verfasserin aut N. Gupta verfasserin aut G. Gutierrez verfasserin aut N. W. Halverson verfasserin aut S. R. Hinton verfasserin aut G. P. Holder verfasserin aut D. L. Hollowood verfasserin aut W. L. Holzapfel verfasserin aut K. Honscheid verfasserin aut J. D. Hrubes verfasserin aut N. Huang verfasserin aut J. Hubmayr verfasserin aut K. D. Irwin verfasserin aut J. Mena-Fernández verfasserin aut D. J. James verfasserin aut F. Kéruzoré verfasserin aut L. Knox verfasserin aut K. Kuehn verfasserin aut O. Lahav verfasserin aut A. T. Lee verfasserin aut S. Lee verfasserin aut D. Li verfasserin aut A. Lowitz verfasserin aut J. L. Marshal verfasserin aut M. McDonald verfasserin aut J. J. McMahon verfasserin aut F. Menanteau verfasserin aut S. S. Meyer verfasserin aut R. Miquel verfasserin aut J. J. Mohr verfasserin aut J. Montgomery verfasserin aut J. Myles verfasserin aut T. Natoli verfasserin aut J. P. Nibarger verfasserin aut G. I. Noble verfasserin aut V. Novosad verfasserin aut R. L. C. Ogando verfasserin aut S. Padin verfasserin aut S. Patil verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malag'on verfasserin aut C. Pryke verfasserin aut C. L. Reichardt verfasserin aut M. Rodr'iguez-Monroy verfasserin aut A. K. Romer verfasserin aut J. E. Ruhl verfasserin aut B. R. Saliwanchik verfasserin aut L. Salvati verfasserin aut E. Sanchez verfasserin aut A. Saro verfasserin aut K. K. Schaffer verfasserin aut T. Schrabback verfasserin aut I. Sevilla-Noarbe verfasserin aut C. Sievers verfasserin aut G. Smecher verfasserin aut M. Smith verfasserin aut T. Somboonpanyakul verfasserin aut B. Stalder verfasserin aut A. A. Stark verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut C. To verfasserin aut C. Tucker verfasserin aut T. Veach verfasserin aut J. D. Vieira verfasserin aut M. Vincenzi verfasserin aut G. Wang verfasserin aut J. Weller verfasserin aut N. Whitehorn verfasserin aut P. Wiseman verfasserin aut W. L. K. Wu verfasserin aut V. Yefremenko verfasserin aut J. A. Zebrowski verfasserin aut Y. Zhang verfasserin aut In The Open Journal of Astrophysics Maynooth Academic Publishing, 2020 7(2024) (DE-627)1683864301 25656120 nnns volume:7 year:2024 https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/article/2245da59b4b844f3b03f5152d7d18228 kostenfrei https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/toc/2565-6120 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 7 2024 |
| allfieldsGer |
10.21105/astro.2311.07512 doi (DE-627)DOAJ095791493 (DE-599)DOAJ2245da59b4b844f3b03f5152d7d18228 DE-627 ger DE-627 rakwb eng QB1-991 QB460-466 L.E. Bleem verfasserin aut Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. Astronomy Astrophysics M. Klein verfasserin aut T. M. C. Abbott verfasserin aut P. A. R. Ade verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut A. J. Anderson verfasserin aut F. Andrade-Oliveira verfasserin aut B. Ansarinejad verfasserin aut M. Archipley verfasserin aut M. L. N. Ashby verfasserin aut J. E. Austermann verfasserin aut D. Bacon verfasserin aut J. A. Beall verfasserin aut A. N. Bender verfasserin aut B. A. Benson verfasserin aut F. Bianchini verfasserin aut S. Bocquet verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut M. Calzadilla verfasserin aut J. E. Carlstrom verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut C. L. Chang verfasserin aut P. Chaubal verfasserin aut H. C. Chiang verfasserin aut T-L. Chou verfasserin aut R. Citron verfasserin aut C. Corbett Moran verfasserin aut M. Costanzi verfasserin aut T. M. Crawford verfasserin aut A. T. Crites verfasserin aut L. N. da Costa verfasserin aut T. de Haan verfasserin aut J. De Vicente verfasserin aut S. Desai verfasserin aut M. A. Dobbs verfasserin aut P. Doel verfasserin aut W. Everett verfasserin aut I. Ferrero verfasserin aut B. Flaugher verfasserin aut B. Floyd verfasserin aut D. Friedel verfasserin aut J. Frieman verfasserin aut J. Gallicchio verfasserin aut J. Garc'ia-Bellido verfasserin aut M. Gatti verfasserin aut E. M. George verfasserin aut G. Giannini verfasserin aut S. Grandis verfasserin aut D. Gruen verfasserin aut R. A. Gruendl verfasserin aut N. Gupta verfasserin aut G. Gutierrez verfasserin aut N. W. Halverson verfasserin aut S. R. Hinton verfasserin aut G. P. Holder verfasserin aut D. L. Hollowood verfasserin aut W. L. Holzapfel verfasserin aut K. Honscheid verfasserin aut J. D. Hrubes verfasserin aut N. Huang verfasserin aut J. Hubmayr verfasserin aut K. D. Irwin verfasserin aut J. Mena-Fernández verfasserin aut D. J. James verfasserin aut F. Kéruzoré verfasserin aut L. Knox verfasserin aut K. Kuehn verfasserin aut O. Lahav verfasserin aut A. T. Lee verfasserin aut S. Lee verfasserin aut D. Li verfasserin aut A. Lowitz verfasserin aut J. L. Marshal verfasserin aut M. McDonald verfasserin aut J. J. McMahon verfasserin aut F. Menanteau verfasserin aut S. S. Meyer verfasserin aut R. Miquel verfasserin aut J. J. Mohr verfasserin aut J. Montgomery verfasserin aut J. Myles verfasserin aut T. Natoli verfasserin aut J. P. Nibarger verfasserin aut G. I. Noble verfasserin aut V. Novosad verfasserin aut R. L. C. Ogando verfasserin aut S. Padin verfasserin aut S. Patil verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malag'on verfasserin aut C. Pryke verfasserin aut C. L. Reichardt verfasserin aut M. Rodr'iguez-Monroy verfasserin aut A. K. Romer verfasserin aut J. E. Ruhl verfasserin aut B. R. Saliwanchik verfasserin aut L. Salvati verfasserin aut E. Sanchez verfasserin aut A. Saro verfasserin aut K. K. Schaffer verfasserin aut T. Schrabback verfasserin aut I. Sevilla-Noarbe verfasserin aut C. Sievers verfasserin aut G. Smecher verfasserin aut M. Smith verfasserin aut T. Somboonpanyakul verfasserin aut B. Stalder verfasserin aut A. A. Stark verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut C. To verfasserin aut C. Tucker verfasserin aut T. Veach verfasserin aut J. D. Vieira verfasserin aut M. Vincenzi verfasserin aut G. Wang verfasserin aut J. Weller verfasserin aut N. Whitehorn verfasserin aut P. Wiseman verfasserin aut W. L. K. Wu verfasserin aut V. Yefremenko verfasserin aut J. A. Zebrowski verfasserin aut Y. Zhang verfasserin aut In The Open Journal of Astrophysics Maynooth Academic Publishing, 2020 7(2024) (DE-627)1683864301 25656120 nnns volume:7 year:2024 https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/article/2245da59b4b844f3b03f5152d7d18228 kostenfrei https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/toc/2565-6120 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 7 2024 |
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10.21105/astro.2311.07512 doi (DE-627)DOAJ095791493 (DE-599)DOAJ2245da59b4b844f3b03f5152d7d18228 DE-627 ger DE-627 rakwb eng QB1-991 QB460-466 L.E. Bleem verfasserin aut Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. Astronomy Astrophysics M. Klein verfasserin aut T. M. C. Abbott verfasserin aut P. A. R. Ade verfasserin aut M. Aguena verfasserin aut O. Alves verfasserin aut A. J. Anderson verfasserin aut F. Andrade-Oliveira verfasserin aut B. Ansarinejad verfasserin aut M. Archipley verfasserin aut M. L. N. Ashby verfasserin aut J. E. Austermann verfasserin aut D. Bacon verfasserin aut J. A. Beall verfasserin aut A. N. Bender verfasserin aut B. A. Benson verfasserin aut F. Bianchini verfasserin aut S. Bocquet verfasserin aut D. Brooks verfasserin aut D. L. Burke verfasserin aut M. Calzadilla verfasserin aut J. E. Carlstrom verfasserin aut A. Carnero Rosell verfasserin aut J. Carretero verfasserin aut C. L. Chang verfasserin aut P. Chaubal verfasserin aut H. C. Chiang verfasserin aut T-L. Chou verfasserin aut R. Citron verfasserin aut C. Corbett Moran verfasserin aut M. Costanzi verfasserin aut T. M. Crawford verfasserin aut A. T. Crites verfasserin aut L. N. da Costa verfasserin aut T. de Haan verfasserin aut J. De Vicente verfasserin aut S. Desai verfasserin aut M. A. Dobbs verfasserin aut P. Doel verfasserin aut W. Everett verfasserin aut I. Ferrero verfasserin aut B. Flaugher verfasserin aut B. Floyd verfasserin aut D. Friedel verfasserin aut J. Frieman verfasserin aut J. Gallicchio verfasserin aut J. Garc'ia-Bellido verfasserin aut M. Gatti verfasserin aut E. M. George verfasserin aut G. Giannini verfasserin aut S. Grandis verfasserin aut D. Gruen verfasserin aut R. A. Gruendl verfasserin aut N. Gupta verfasserin aut G. Gutierrez verfasserin aut N. W. Halverson verfasserin aut S. R. Hinton verfasserin aut G. P. Holder verfasserin aut D. L. Hollowood verfasserin aut W. L. Holzapfel verfasserin aut K. Honscheid verfasserin aut J. D. Hrubes verfasserin aut N. Huang verfasserin aut J. Hubmayr verfasserin aut K. D. Irwin verfasserin aut J. Mena-Fernández verfasserin aut D. J. James verfasserin aut F. Kéruzoré verfasserin aut L. Knox verfasserin aut K. Kuehn verfasserin aut O. Lahav verfasserin aut A. T. Lee verfasserin aut S. Lee verfasserin aut D. Li verfasserin aut A. Lowitz verfasserin aut J. L. Marshal verfasserin aut M. McDonald verfasserin aut J. J. McMahon verfasserin aut F. Menanteau verfasserin aut S. S. Meyer verfasserin aut R. Miquel verfasserin aut J. J. Mohr verfasserin aut J. Montgomery verfasserin aut J. Myles verfasserin aut T. Natoli verfasserin aut J. P. Nibarger verfasserin aut G. I. Noble verfasserin aut V. Novosad verfasserin aut R. L. C. Ogando verfasserin aut S. Padin verfasserin aut S. Patil verfasserin aut M. E. S. Pereira verfasserin aut A. Pieres verfasserin aut A. A. Plazas Malag'on verfasserin aut C. Pryke verfasserin aut C. L. Reichardt verfasserin aut M. Rodr'iguez-Monroy verfasserin aut A. K. Romer verfasserin aut J. E. Ruhl verfasserin aut B. R. Saliwanchik verfasserin aut L. Salvati verfasserin aut E. Sanchez verfasserin aut A. Saro verfasserin aut K. K. Schaffer verfasserin aut T. Schrabback verfasserin aut I. Sevilla-Noarbe verfasserin aut C. Sievers verfasserin aut G. Smecher verfasserin aut M. Smith verfasserin aut T. Somboonpanyakul verfasserin aut B. Stalder verfasserin aut A. A. Stark verfasserin aut E. Suchyta verfasserin aut M. E. C. Swanson verfasserin aut G. Tarle verfasserin aut C. To verfasserin aut C. Tucker verfasserin aut T. Veach verfasserin aut J. D. Vieira verfasserin aut M. Vincenzi verfasserin aut G. Wang verfasserin aut J. Weller verfasserin aut N. Whitehorn verfasserin aut P. Wiseman verfasserin aut W. L. K. Wu verfasserin aut V. Yefremenko verfasserin aut J. A. Zebrowski verfasserin aut Y. Zhang verfasserin aut In The Open Journal of Astrophysics Maynooth Academic Publishing, 2020 7(2024) (DE-627)1683864301 25656120 nnns volume:7 year:2024 https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/article/2245da59b4b844f3b03f5152d7d18228 kostenfrei https://doi.org/10.21105/astro.2311.07512 kostenfrei https://doaj.org/toc/2565-6120 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 7 2024 |
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L.E. Bleem @@aut@@ M. Klein @@aut@@ T. M. C. Abbott @@aut@@ P. A. R. Ade @@aut@@ M. Aguena @@aut@@ O. Alves @@aut@@ A. J. Anderson @@aut@@ F. Andrade-Oliveira @@aut@@ B. Ansarinejad @@aut@@ M. Archipley @@aut@@ M. L. N. Ashby @@aut@@ J. E. Austermann @@aut@@ D. Bacon @@aut@@ J. A. Beall @@aut@@ A. N. Bender @@aut@@ B. A. Benson @@aut@@ F. Bianchini @@aut@@ S. Bocquet @@aut@@ D. Brooks @@aut@@ D. L. Burke @@aut@@ M. Calzadilla @@aut@@ J. E. Carlstrom @@aut@@ A. Carnero Rosell @@aut@@ J. Carretero @@aut@@ C. L. Chang @@aut@@ P. Chaubal @@aut@@ H. C. Chiang @@aut@@ T-L. Chou @@aut@@ R. Citron @@aut@@ C. Corbett Moran @@aut@@ M. Costanzi @@aut@@ T. M. Crawford @@aut@@ A. T. Crites @@aut@@ L. N. da Costa @@aut@@ T. de Haan @@aut@@ J. De Vicente @@aut@@ S. Desai @@aut@@ M. A. Dobbs @@aut@@ P. Doel @@aut@@ W. Everett @@aut@@ I. Ferrero @@aut@@ B. Flaugher @@aut@@ B. Floyd @@aut@@ D. Friedel @@aut@@ J. Frieman @@aut@@ J. Gallicchio @@aut@@ J. Garc'ia-Bellido @@aut@@ M. Gatti @@aut@@ E. M. George @@aut@@ G. Giannini @@aut@@ S. Grandis @@aut@@ D. Gruen @@aut@@ R. A. Gruendl @@aut@@ N. Gupta @@aut@@ G. Gutierrez @@aut@@ N. W. Halverson @@aut@@ S. R. Hinton @@aut@@ G. P. Holder @@aut@@ D. L. Hollowood @@aut@@ W. L. Holzapfel @@aut@@ K. Honscheid @@aut@@ J. D. Hrubes @@aut@@ N. Huang @@aut@@ J. Hubmayr @@aut@@ K. D. Irwin @@aut@@ J. Mena-Fernández @@aut@@ D. J. James @@aut@@ F. Kéruzoré @@aut@@ L. Knox @@aut@@ K. Kuehn @@aut@@ O. Lahav @@aut@@ A. T. Lee @@aut@@ S. Lee @@aut@@ D. Li @@aut@@ A. Lowitz @@aut@@ J. L. Marshal @@aut@@ M. McDonald @@aut@@ J. J. McMahon @@aut@@ F. Menanteau @@aut@@ S. S. Meyer @@aut@@ R. Miquel @@aut@@ J. J. Mohr @@aut@@ J. Montgomery @@aut@@ J. Myles @@aut@@ T. Natoli @@aut@@ J. P. Nibarger @@aut@@ G. I. Noble @@aut@@ V. Novosad @@aut@@ R. L. C. Ogando @@aut@@ S. Padin @@aut@@ S. Patil @@aut@@ M. E. S. Pereira @@aut@@ A. Pieres @@aut@@ A. A. Plazas Malag'on @@aut@@ C. Pryke @@aut@@ C. L. Reichardt @@aut@@ M. Rodr'iguez-Monroy @@aut@@ A. K. Romer @@aut@@ J. E. Ruhl @@aut@@ B. R. Saliwanchik @@aut@@ L. Salvati @@aut@@ E. Sanchez @@aut@@ A. Saro @@aut@@ K. K. Schaffer @@aut@@ T. Schrabback @@aut@@ I. Sevilla-Noarbe @@aut@@ C. Sievers @@aut@@ G. Smecher @@aut@@ M. Smith @@aut@@ T. Somboonpanyakul @@aut@@ B. Stalder @@aut@@ A. A. Stark @@aut@@ E. Suchyta @@aut@@ M. E. C. Swanson @@aut@@ G. Tarle @@aut@@ C. To @@aut@@ C. Tucker @@aut@@ T. Veach @@aut@@ J. D. Vieira @@aut@@ M. Vincenzi @@aut@@ G. Wang @@aut@@ J. Weller @@aut@@ N. Whitehorn @@aut@@ P. Wiseman @@aut@@ W. L. K. Wu @@aut@@ V. Yefremenko @@aut@@ J. A. Zebrowski @@aut@@ Y. Zhang @@aut@@ |
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Brooks</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">D. L. Burke</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. Calzadilla</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. E. Carlstrom</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. Carnero Rosell</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Carretero</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">C. L. Chang</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">P. Chaubal</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">H. C. Chiang</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T-L. Chou</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">R. Citron</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">C. Corbett Moran</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. Costanzi</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T. M. Crawford</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. T. Crites</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">L. N. da Costa</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T. de Haan</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. De Vicente</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Desai</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. A. Dobbs</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">P. Doel</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">W. Everett</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">I. Ferrero</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">B. Flaugher</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">B. Floyd</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">D. Friedel</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Frieman</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Gallicchio</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Garc'ia-Bellido</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. Gatti</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">E. M. George</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">G. Giannini</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Grandis</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">D. Gruen</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">R. A. Gruendl</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">N. Gupta</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">G. Gutierrez</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">N. W. Halverson</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. R. Hinton</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">G. P. Holder</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">D. L. Hollowood</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">W. L. Holzapfel</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">K. Honscheid</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. D. Hrubes</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">N. Huang</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Hubmayr</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">K. D. Irwin</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Mena-Fernández</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">D. J. James</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">F. 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Li</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. Lowitz</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. L. Marshal</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. McDonald</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. J. McMahon</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">F. Menanteau</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. S. Meyer</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">R. Miquel</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. J. Mohr</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Montgomery</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Myles</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T. Natoli</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. P. Nibarger</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">G. I. Noble</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">V. Novosad</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">R. L. C. Ogando</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Padin</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Patil</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. E. S. Pereira</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. Pieres</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. A. Plazas Malag'on</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">C. Pryke</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">C. L. Reichardt</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. Rodr'iguez-Monroy</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. K. Romer</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. E. Ruhl</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">B. R. Saliwanchik</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">L. Salvati</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">E. 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Sievers</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">G. Smecher</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. Smith</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T. Somboonpanyakul</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">B. Stalder</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. A. Stark</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">E. 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L.E. Bleem M. Klein T. M. C. Abbott P. A. R. Ade M. Aguena O. Alves A. J. Anderson F. Andrade-Oliveira B. Ansarinejad M. Archipley M. L. N. Ashby J. E. Austermann D. Bacon J. A. Beall A. N. Bender B. A. Benson F. Bianchini S. Bocquet D. Brooks D. L. Burke M. Calzadilla J. E. Carlstrom A. Carnero Rosell J. Carretero C. L. Chang P. Chaubal H. C. Chiang T-L. Chou R. Citron C. Corbett Moran M. Costanzi T. M. Crawford A. T. Crites L. N. da Costa T. de Haan J. De Vicente S. Desai M. A. Dobbs P. Doel W. Everett I. Ferrero B. Flaugher B. Floyd D. Friedel J. Frieman J. Gallicchio J. Garc'ia-Bellido M. Gatti E. M. George G. Giannini S. Grandis D. Gruen R. A. Gruendl N. Gupta G. Gutierrez N. W. Halverson S. R. Hinton G. P. Holder D. L. Hollowood W. L. Holzapfel K. Honscheid J. D. Hrubes N. Huang J. Hubmayr K. D. Irwin J. Mena-Fernández D. J. James F. Kéruzoré L. Knox K. Kuehn O. Lahav A. T. Lee S. Lee D. Li A. Lowitz J. L. Marshal M. McDonald J. J. McMahon F. Menanteau S. S. Meyer R. Miquel J. J. Mohr J. Montgomery J. Myles T. Natoli J. P. Nibarger G. I. Noble V. Novosad R. L. C. Ogando S. Padin S. Patil M. E. S. Pereira A. Pieres A. A. Plazas Malag'on C. Pryke C. L. Reichardt M. Rodr'iguez-Monroy A. K. Romer J. E. Ruhl B. R. Saliwanchik L. Salvati E. Sanchez A. Saro K. K. Schaffer T. Schrabback I. Sevilla-Noarbe C. Sievers G. Smecher M. Smith T. Somboonpanyakul B. Stalder A. A. Stark E. Suchyta M. E. C. Swanson G. Tarle C. To C. Tucker T. Veach J. D. Vieira M. Vincenzi G. Wang J. Weller N. Whitehorn P. Wiseman W. L. K. Wu V. Yefremenko J. A. Zebrowski Y. Zhang |
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Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey |
| abstract |
We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. |
| abstractGer |
We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. |
| abstract_unstemmed |
We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu. |
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M. Klein T. M. C. Abbott P. A. R. Ade M. Aguena O. Alves A. J. Anderson F. Andrade-Oliveira B. Ansarinejad M. Archipley M. L. N. Ashby J. E. Austermann D. Bacon J. A. Beall A. N. Bender B. A. Benson F. Bianchini S. Bocquet D. Brooks D. L. Burke M. Calzadilla J. E. Carlstrom A. Carnero Rosell J. Carretero C. L. Chang P. Chaubal H. C. Chiang T-L. Chou R. Citron C. Corbett Moran M. Costanzi T. M. Crawford A. T. Crites L. N. da Costa T. de Haan J. De Vicente S. Desai M. A. Dobbs P. Doel W. Everett I. Ferrero B. Flaugher B. Floyd D. Friedel J. Frieman J. Gallicchio J. Garc'ia-Bellido M. Gatti E. M. George G. Giannini S. Grandis D. Gruen R. A. Gruendl N. Gupta G. Gutierrez N. W. Halverson S. R. Hinton G. P. Holder D. L. Hollowood W. L. Holzapfel K. Honscheid J. D. Hrubes N. Huang J. Hubmayr K. D. Irwin J. Mena-Fernández D. J. James F. Kéruzoré L. Knox K. Kuehn O. Lahav A. T. Lee S. Lee D. Li A. Lowitz J. L. Marshal M. McDonald J. J. McMahon F. Menanteau S. S. Meyer R. Miquel J. J. Mohr J. Montgomery J. Myles T. Natoli J. P. Nibarger G. I. Noble V. Novosad R. L. C. Ogando S. Padin S. Patil M. E. S. Pereira A. Pieres A. A. Plazas Malag'on C. Pryke C. L. Reichardt M. Rodr'iguez-Monroy A. K. Romer J. E. Ruhl B. R. Saliwanchik L. Salvati E. Sanchez A. Saro K. K. Schaffer T. Schrabback I. Sevilla-Noarbe C. Sievers G. Smecher M. Smith T. Somboonpanyakul B. Stalder A. A. Stark E. Suchyta M. E. C. Swanson G. Tarle C. To C. Tucker T. Veach J. D. Vieira M. Vincenzi G. Wang J. Weller N. Whitehorn P. Wiseman W. L. K. Wu V. Yefremenko J. A. Zebrowski Y. Zhang |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">DOAJ095791493</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240413122632.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">240413s2024 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.21105/astro.2311.07512</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)DOAJ095791493</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)DOAJ2245da59b4b844f3b03f5152d7d18228</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="050" ind1=" " ind2="0"><subfield code="a">QB1-991</subfield></datafield><datafield tag="050" ind1=" " ind2="0"><subfield code="a">QB460-466</subfield></datafield><datafield tag="100" ind1="0" ind2=" "><subfield code="a">L.E. Bleem</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Galaxy Clusters Discovered via the Thermal Sunyaev-Zel'dovich Effect in the 500-square-degree SPTpol Survey</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2024</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We present a catalog of 689 galaxy cluster candidates detected at significance $\xi<4$ via their thermal Sunyaev-Zel'dovich (SZ) effect signature in 95 and 150 GHz data from the 500-square-degree SPTpol survey. We use optical and infrared data from the Dark Energy Camera and the Wide-field Infrared Survey Explorer (WISE) and Spitzer satellites, to confirm 544 of these candidates as clusters with $\sim94\%$ purity. The sample has an approximately redshift-independent mass threshold at redshift $z<0.25$ and spans $1.5 \times 10^{14} < M_{500c} < 9 \times 10^{14}$ $M_\odot/h_{70}$ and $0.03<z\lesssim1.6$ in mass and redshift, respectively; 21% of the confirmed clusters are at $z<1$. We use external radio data from the Sydney University Molonglo Sky Survey (SUMSS) to estimate contamination to the SZ signal from synchrotron sources. The contamination reduces the recovered $\xi$ by a median value of 0.032, or $\sim0.8\%$ of the $\xi=4$ threshold value, and $\sim7\%$ of candidates have a predicted contamination greater than $\Delta \xi = 1$. With the exception of a small number of systems $(<1\%)$, an analysis of clusters detected in single-frequency 95 and 150 GHz data shows no significant contamination of the SZ signal by emission from dusty or synchrotron sources. This cluster sample will be a key component in upcoming astrophysical and cosmological analyses of clusters. The SPTpol millimeter-wave maps and associated data products used to produce this sample are available at https://pole.uchicago.edu/public/data/sptpol_500d_clusters/index.html, and the NASA LAMBDA website. An interactive sky server with the SPTpol maps and Dark Energy Survey data release 2 images is also available at NCSA https://skyviewer.ncsa.illinois.edu.</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Astronomy</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Astrophysics</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. 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