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Constraining the baryon–dark matter relative velocity with the large-scale three-point correlation function of the SDSS BOSS DR12 CMASS galaxies

Authors :
Anže Slosar
Hee-Jong Seo
Chia-Hsun Chuang
Héctor Gil-Marín
Graziano Rossi
Will J. Percival
Francisco-Shu Kitaura
Shirley Ho
Ashley J. Ross
Mariana Vargas-Magaña
Daniel J. Eisenstein
Zachary Slepian
Jonathan Blazek
Joseph E. McEwen
Joel R. Brownstein
Institut Lagrange de Paris
Sorbonne Universités
Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585))
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Sorbonne Université (SU)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE )
Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS )
Source :
Mon.Not.Roy.Astron.Soc., Mon.Not.Roy.Astron.Soc., 2018, 474 (2), pp.2109-2115. ⟨10.1093/mnras/stx2723⟩, Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 474 (2), pp.2109-2115. ⟨10.1093/mnras/stx2723⟩, Slepian, Z, Eisenstein, D J, Blazek, J A, Brownstein, J R, Chuang, C-H, Gil-marín, H, Ho, S, Kitaura, F, Mcewen, J E, Percival, W J, Ross, A J, Rossi, G, Seo, H-J, Slosar, A & Vargas-Magaña, M 2018, ' Constraining the baryon–dark matter relative velocity with the large-scale three-point correlation function of the SDSS BOSS DR12 CMASS galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 474, no. 2, pp. 2109-2115 . https://doi.org/10.1093/mnras/stx2723, Mon.Not.Roy.Astron.Soc., 2018, 474 (2), pp.2109-2115. 〈10.1093/mnras/stx2723〉
Publication Year :
2018
Publisher :
HAL CCSD, 2018.

Abstract

International audience; We search for a galaxy clustering bias due to a modulation of galaxy number with the baryon–dark matter relative velocity resulting from recombination-era physics. We find no detected signal and place the constraint

Details

Language :
English
ISSN :
00358711 and 13652966
Database :
OpenAIRE
Journal :
Mon.Not.Roy.Astron.Soc., Mon.Not.Roy.Astron.Soc., 2018, 474 (2), pp.2109-2115. ⟨10.1093/mnras/stx2723⟩, Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 474 (2), pp.2109-2115. ⟨10.1093/mnras/stx2723⟩, Slepian, Z, Eisenstein, D J, Blazek, J A, Brownstein, J R, Chuang, C-H, Gil-marín, H, Ho, S, Kitaura, F, Mcewen, J E, Percival, W J, Ross, A J, Rossi, G, Seo, H-J, Slosar, A & Vargas-Magaña, M 2018, ' Constraining the baryon–dark matter relative velocity with the large-scale three-point correlation function of the SDSS BOSS DR12 CMASS galaxies ', Monthly Notices of the Royal Astronomical Society, vol. 474, no. 2, pp. 2109-2115 . https://doi.org/10.1093/mnras/stx2723, Mon.Not.Roy.Astron.Soc., 2018, 474 (2), pp.2109-2115. 〈10.1093/mnras/stx2723〉
Accession number :
edsair.doi.dedup.....cccca59e5f0499487ad83b04ba426bfb
Full Text :
https://doi.org/10.1093/mnras/stx2723⟩