First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations
International audience We report results from an analysis aimed at detecting the trispectrum of the kinematic Sunyaev-Zel'dovich (kSZ) effect by combining data from the South Pole Telescope (SPT) and {\it Herschel}-SPIRE experiments over a 100 ${\rm deg}^{2}$ field. The SPT observations combine...
Published in: | Physical Review Letters |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Other Authors: | , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
HAL CCSD
2024
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Subjects: | |
Online Access: | https://hal.science/hal-04510904 https://doi.org/10.1103/PhysRevLett.133.121004 |
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ftsorbonneuniv:oai:HAL:hal-04510904v1 |
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HAL Sorbonne Université |
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English |
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[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
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[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Raghunathan, S Ade, P.A.R Anderson, A.J Ansarinejad, B Archipley, M Austermann, J.E Balkenhol, L Beall, J.A Benabed, K Bender, A.N Benson, B.A Bianchini, F Bleem, L.E Bock, J Bouchet, F.R Bryant, L Camphuis, E Carlstrom, J.E Cecil, T.W Chang, C.L Chaubal, P Chiang, H.C Chichura, P.M Chou, T.-L Citron, R Coerver, A Crawford, T.M Crites, A.T Cukierman, A Daley, C Dibert, K.R Dobbs, M.A Doussot, A Dutcher, D Everett, W Feng, C Ferguson, K.R Fichman, K Foster, A Galli, S Gallicchio, J Gambrel, A.E Gardner, R.W Ge, F George, E.M Goeckner-Wald, N Gualtieri, R Guidi, F Guns, S Gupta, N de Haan, T Halverson, N.W Hivon, E Holder, G.P Holzapfel, W.L Hood, J.C Hrubes, J.D Hryciuk, A Huang, N Hubmayr, J Irwin, K.D Kéruzoré, F Knox, L Korman, M Kornoelje, K Kuo, C.-L Lee, A.T Levy, K Li, D Lowitz, A.E Lu, C Maniyar, A Mcmahon, J.J Menanteau, F Millea, M Montgomery, J Moran, C. Corbett Nakato, Y Natoli, T Nibarger, J.P Noble, G.I Novosad, V Omori, Y Padin, S Pan, Z Paschos, P Patil, S Phadke, K.A Prabhu, K Pryke, C Quan, W Rahimi, M Rahlin, A Reichardt, C.L Rouble, M Ruhl, J.E Saliwanchik, B.R Schaffer, K.K Schiappucci, E Sievers, C Smecher, G Sobrin, J.A Stark, A.A Stephen, J Suzuki, A Tandoi, C Thompson, K.L Thorne, B Trendafilova, C Tucker, C Umilta, C Veach, T Vieira, J.D Viero, M.P Wan, Y Wang, G Whitehorn, N Wu, W.L.K Yefremenko, V Young, M.R Zebrowski, J.A Zemcov, M First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations |
topic_facet |
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience We report results from an analysis aimed at detecting the trispectrum of the kinematic Sunyaev-Zel'dovich (kSZ) effect by combining data from the South Pole Telescope (SPT) and {\it Herschel}-SPIRE experiments over a 100 ${\rm deg}^{2}$ field. The SPT observations combine data from the previous and current surveys, namely SPTpol and SPT-3G, to achieve depths of 4.5, 3, and 16 $\mu {\rm K-arcmin}$ in bands centered at 95, 150, and 220 GHz. For SPIRE, we include data from the 600 and 857 GHz bands. We reconstruct the velocity-induced large-scale correlation of the small-scale kSZ signal with a quadratic estimator that uses two cosmic microwave background (CMB) temperature maps, constructed by optimally combining data from all the frequency bands. We reject the null hypothesis of a zero trispectrum at $10.3\sigma$ level. However, the measured trispectrum contains contributions from both the kSZ and other undesired components, such as CMB lensing and astrophysical foregrounds, with kSZ being sub-dominant. We use the \textsc{Agora} simulations to estimate the expected signal from CMB lensing and astrophysical foregrounds. After accounting for the contributions from CMB lensing and foreground signals, we do not detect an excess kSZ-only trispectrum and use this non-detection to set constraints on reionization. By applying a prior based on observations of the Gunn-Peterson trough, we obtain an upper limit on the duration of reionization of $\Delta z_{\rm re, 50} < 4.5$ (95% C.L). We find these constraints are fairly robust to foregrounds assumptions. This trispectrum measurement is independent of, but consistent with, {\it Planck}'s optical depth measurement. This result is the first constraint on the epoch of reionization using the non-Gaussian nature of the kSZ signal. |
author2 |
Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) SPT-3G SPTpol |
format |
Article in Journal/Newspaper |
author |
Raghunathan, S Ade, P.A.R Anderson, A.J Ansarinejad, B Archipley, M Austermann, J.E Balkenhol, L Beall, J.A Benabed, K Bender, A.N Benson, B.A Bianchini, F Bleem, L.E Bock, J Bouchet, F.R Bryant, L Camphuis, E Carlstrom, J.E Cecil, T.W Chang, C.L Chaubal, P Chiang, H.C Chichura, P.M Chou, T.-L Citron, R Coerver, A Crawford, T.M Crites, A.T Cukierman, A Daley, C Dibert, K.R Dobbs, M.A Doussot, A Dutcher, D Everett, W Feng, C Ferguson, K.R Fichman, K Foster, A Galli, S Gallicchio, J Gambrel, A.E Gardner, R.W Ge, F George, E.M Goeckner-Wald, N Gualtieri, R Guidi, F Guns, S Gupta, N de Haan, T Halverson, N.W Hivon, E Holder, G.P Holzapfel, W.L Hood, J.C Hrubes, J.D Hryciuk, A Huang, N Hubmayr, J Irwin, K.D Kéruzoré, F Knox, L Korman, M Kornoelje, K Kuo, C.-L Lee, A.T Levy, K Li, D Lowitz, A.E Lu, C Maniyar, A Mcmahon, J.J Menanteau, F Millea, M Montgomery, J Moran, C. Corbett Nakato, Y Natoli, T Nibarger, J.P Noble, G.I Novosad, V Omori, Y Padin, S Pan, Z Paschos, P Patil, S Phadke, K.A Prabhu, K Pryke, C Quan, W Rahimi, M Rahlin, A Reichardt, C.L Rouble, M Ruhl, J.E Saliwanchik, B.R Schaffer, K.K Schiappucci, E Sievers, C Smecher, G Sobrin, J.A Stark, A.A Stephen, J Suzuki, A Tandoi, C Thompson, K.L Thorne, B Trendafilova, C Tucker, C Umilta, C Veach, T Vieira, J.D Viero, M.P Wan, Y Wang, G Whitehorn, N Wu, W.L.K Yefremenko, V Young, M.R Zebrowski, J.A Zemcov, M |
author_facet |
Raghunathan, S Ade, P.A.R Anderson, A.J Ansarinejad, B Archipley, M Austermann, J.E Balkenhol, L Beall, J.A Benabed, K Bender, A.N Benson, B.A Bianchini, F Bleem, L.E Bock, J Bouchet, F.R Bryant, L Camphuis, E Carlstrom, J.E Cecil, T.W Chang, C.L Chaubal, P Chiang, H.C Chichura, P.M Chou, T.-L Citron, R Coerver, A Crawford, T.M Crites, A.T Cukierman, A Daley, C Dibert, K.R Dobbs, M.A Doussot, A Dutcher, D Everett, W Feng, C Ferguson, K.R Fichman, K Foster, A Galli, S Gallicchio, J Gambrel, A.E Gardner, R.W Ge, F George, E.M Goeckner-Wald, N Gualtieri, R Guidi, F Guns, S Gupta, N de Haan, T Halverson, N.W Hivon, E Holder, G.P Holzapfel, W.L Hood, J.C Hrubes, J.D Hryciuk, A Huang, N Hubmayr, J Irwin, K.D Kéruzoré, F Knox, L Korman, M Kornoelje, K Kuo, C.-L Lee, A.T Levy, K Li, D Lowitz, A.E Lu, C Maniyar, A Mcmahon, J.J Menanteau, F Millea, M Montgomery, J Moran, C. Corbett Nakato, Y Natoli, T Nibarger, J.P Noble, G.I Novosad, V Omori, Y Padin, S Pan, Z Paschos, P Patil, S Phadke, K.A Prabhu, K Pryke, C Quan, W Rahimi, M Rahlin, A Reichardt, C.L Rouble, M Ruhl, J.E Saliwanchik, B.R Schaffer, K.K Schiappucci, E Sievers, C Smecher, G Sobrin, J.A Stark, A.A Stephen, J Suzuki, A Tandoi, C Thompson, K.L Thorne, B Trendafilova, C Tucker, C Umilta, C Veach, T Vieira, J.D Viero, M.P Wan, Y Wang, G Whitehorn, N Wu, W.L.K Yefremenko, V Young, M.R Zebrowski, J.A Zemcov, M |
author_sort |
Raghunathan, S |
title |
First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations |
title_short |
First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations |
title_full |
First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations |
title_fullStr |
First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations |
title_full_unstemmed |
First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations |
title_sort |
first constraints on the epoch of reionization using the non-gaussianity of the kinematic sunyaev-zel'dovich effect from the south pole telescope and {\it herschel}-spire observations |
publisher |
HAL CCSD |
publishDate |
2024 |
url |
https://hal.science/hal-04510904 https://doi.org/10.1103/PhysRevLett.133.121004 |
long_lat |
ENVELOPE(160.700,160.700,-76.867,-76.867) |
geographic |
Gunn South Pole |
geographic_facet |
Gunn South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Phys.Rev.Lett. https://hal.science/hal-04510904 Phys.Rev.Lett., 2024, 133 (12), pp.121004. ⟨10.1103/PhysRevLett.133.121004⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2403.02337 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevLett.133.121004 ARXIV: 2403.02337 doi:10.1103/PhysRevLett.133.121004 INSPIRE: 2765125 |
op_doi |
https://doi.org/10.1103/PhysRevLett.133.121004 |
container_title |
Physical Review Letters |
container_volume |
133 |
container_issue |
12 |
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1812818338197274624 |
spelling |
ftsorbonneuniv:oai:HAL:hal-04510904v1 2024-10-13T14:10:49+00:00 First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel'dovich Effect from the South Pole Telescope and {\it Herschel}-SPIRE Observations Raghunathan, S Ade, P.A.R Anderson, A.J Ansarinejad, B Archipley, M Austermann, J.E Balkenhol, L Beall, J.A Benabed, K Bender, A.N Benson, B.A Bianchini, F Bleem, L.E Bock, J Bouchet, F.R Bryant, L Camphuis, E Carlstrom, J.E Cecil, T.W Chang, C.L Chaubal, P Chiang, H.C Chichura, P.M Chou, T.-L Citron, R Coerver, A Crawford, T.M Crites, A.T Cukierman, A Daley, C Dibert, K.R Dobbs, M.A Doussot, A Dutcher, D Everett, W Feng, C Ferguson, K.R Fichman, K Foster, A Galli, S Gallicchio, J Gambrel, A.E Gardner, R.W Ge, F George, E.M Goeckner-Wald, N Gualtieri, R Guidi, F Guns, S Gupta, N de Haan, T Halverson, N.W Hivon, E Holder, G.P Holzapfel, W.L Hood, J.C Hrubes, J.D Hryciuk, A Huang, N Hubmayr, J Irwin, K.D Kéruzoré, F Knox, L Korman, M Kornoelje, K Kuo, C.-L Lee, A.T Levy, K Li, D Lowitz, A.E Lu, C Maniyar, A Mcmahon, J.J Menanteau, F Millea, M Montgomery, J Moran, C. Corbett Nakato, Y Natoli, T Nibarger, J.P Noble, G.I Novosad, V Omori, Y Padin, S Pan, Z Paschos, P Patil, S Phadke, K.A Prabhu, K Pryke, C Quan, W Rahimi, M Rahlin, A Reichardt, C.L Rouble, M Ruhl, J.E Saliwanchik, B.R Schaffer, K.K Schiappucci, E Sievers, C Smecher, G Sobrin, J.A Stark, A.A Stephen, J Suzuki, A Tandoi, C Thompson, K.L Thorne, B Trendafilova, C Tucker, C Umilta, C Veach, T Vieira, J.D Viero, M.P Wan, Y Wang, G Whitehorn, N Wu, W.L.K Yefremenko, V Young, M.R Zebrowski, J.A Zemcov, M Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) SPT-3G SPTpol 2024 https://hal.science/hal-04510904 https://doi.org/10.1103/PhysRevLett.133.121004 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2403.02337 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevLett.133.121004 ARXIV: 2403.02337 doi:10.1103/PhysRevLett.133.121004 INSPIRE: 2765125 Phys.Rev.Lett. https://hal.science/hal-04510904 Phys.Rev.Lett., 2024, 133 (12), pp.121004. ⟨10.1103/PhysRevLett.133.121004⟩ [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2024 ftsorbonneuniv https://doi.org/10.1103/PhysRevLett.133.121004 2024-09-23T14:19:19Z International audience We report results from an analysis aimed at detecting the trispectrum of the kinematic Sunyaev-Zel'dovich (kSZ) effect by combining data from the South Pole Telescope (SPT) and {\it Herschel}-SPIRE experiments over a 100 ${\rm deg}^{2}$ field. The SPT observations combine data from the previous and current surveys, namely SPTpol and SPT-3G, to achieve depths of 4.5, 3, and 16 $\mu {\rm K-arcmin}$ in bands centered at 95, 150, and 220 GHz. For SPIRE, we include data from the 600 and 857 GHz bands. We reconstruct the velocity-induced large-scale correlation of the small-scale kSZ signal with a quadratic estimator that uses two cosmic microwave background (CMB) temperature maps, constructed by optimally combining data from all the frequency bands. We reject the null hypothesis of a zero trispectrum at $10.3\sigma$ level. However, the measured trispectrum contains contributions from both the kSZ and other undesired components, such as CMB lensing and astrophysical foregrounds, with kSZ being sub-dominant. We use the \textsc{Agora} simulations to estimate the expected signal from CMB lensing and astrophysical foregrounds. After accounting for the contributions from CMB lensing and foreground signals, we do not detect an excess kSZ-only trispectrum and use this non-detection to set constraints on reionization. By applying a prior based on observations of the Gunn-Peterson trough, we obtain an upper limit on the duration of reionization of $\Delta z_{\rm re, 50} < 4.5$ (95% C.L). We find these constraints are fairly robust to foregrounds assumptions. This trispectrum measurement is independent of, but consistent with, {\it Planck}'s optical depth measurement. This result is the first constraint on the epoch of reionization using the non-Gaussian nature of the kSZ signal. Article in Journal/Newspaper South pole HAL Sorbonne Université Gunn ENVELOPE(160.700,160.700,-76.867,-76.867) South Pole Physical Review Letters 133 12 |