Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck

J. Sánchez; Y. Omori; C. Chang; L. E. Bleem; T. Crawford; A. Drlica-Wagner; S. Raghunathan; G. Zacharegkas; T. M. C. Abbott; M. Aguena; A. Alarcon; S. Allam; O. Alves; A. Amon; S. Avila; E. Baxter; K. Bechtol; B. A. Benson; G. M. Bernstein; E. Bertin; S. Bocquet; D. Brooks; D. L. Burke; A. Campos; J. E. Carlstrom; A. Carnero Rosell; M. Carrasco Kind; J. Carretero; F. J. Castander; R. Cawthon; C. Chang; A. Chen; A. Choi; R. Chown; M. Costanzi; A. T. Crites; M. Crocce; L. N. da Costa; M. E. S. Pereira; T. de Haan; J. De Vicente; J. DeRose; S. Desai; H. T. Diehl; M. A. Dobbs; S. Dodelson; P. Doel; J. Elvin-Poole; W. Everett; S. Everett; I. Ferrero; B. Flaugher; P. Fosalba; J. Frieman; J. García-Bellido; M. Gatti; E. M. George; D. W. Gerdes; G. Giannini; D. Gruen; R. A. Gruendl; J. Gschwend; G. Gutierrez; N. W. Halverson; S. R. Hinton; G. P. Holder; D. L. Hollowood; W. L. Holzapfel; K. Honscheid; J. D. Hrubes; D. J. James; L. Knox; K. Kuehn; N. Kuropatkin; O. Lahav; A. T. Lee; D. Luong-Van; N. MacCrann; J. L. Marshall; J. McCullough; J. J. McMahon; P. Melchior; J. Mena-Fernández; F. Menanteau; R. Miquel; L. Mocanu; J. J. Mohr; J. Muir; J. Myles; T. Natoli; S. Padin; A. Palmese; S. Pandey; F. Paz-Chinchón; A. Pieres; A. A. Plazas Malagón; A. Porredon; C. Pryke; M. Raveri; C. L. Reichardt; M. Rodriguez-Monroy; A. J. Ross; J. E. Ruhl; E. Rykoff; C. Sánchez; E. Sanchez; V. Scarpine; K. K. Schaffer; I. Sevilla-Noarbe; E. Sheldon; E. Shirokoff; M. Smith; M. Soares-Santos; Z. Staniszewski; A. A. Stark; E. Suchyta; M. E. C. Swanson; G. Tarle; D. Thomas; M. A. Troxel; D. L. Tucker; J. D. Vieira; M. Vincenzi; N. Weaverdyck; R. Williamson; B. Yanny; B. Yin; (DES Collaborations) SPT

doi:10.1093/mnras/stad1167

Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck

J. Sánchez^*, Y. Omori, C. Chang, L. E. Bleem, T. Crawford, A. Drlica-Wagner, S. Raghunathan, G. Zacharegkas, T. M. C. Abbott, M. Aguena, A. Alarcon, S. Allam, O. Alves, A. Amon, S. Avila, E. Baxter, K. Bechtol, B. A. Benson, G. M. Bernstein, E. BertinS. Bocquet, D. Brooks, D. L. Burke, A. Campos, J. E. Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, R. Cawthon, C. Chang, A. Chen, A. Choi, R. Chown, M. Costanzi, A. T. Crites, M. Crocce, L. N. da Costa, M. E. S. Pereira, T. de Haan, J. De Vicente, J. DeRose, S. Desai, H. T. Diehl, M. A. Dobbs, S. Dodelson, P. Doel, J. Elvin-Poole, W. Everett, S. Everett, I. Ferrero, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, M. Gatti, E. M. George, D. W. Gerdes, G. Giannini, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, N. W. Halverson, S. R. Hinton, G. P. Holder, D. L. Hollowood, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, D. J. James, L. Knox, K. Kuehn, N. Kuropatkin, O. Lahav, A. T. Lee, D. Luong-Van, N. MacCrann, J. L. Marshall, J. McCullough, J. J. McMahon, P. Melchior, J. Mena-Fernández, F. Menanteau, R. Miquel, L. Mocanu, J. J. Mohr, J. Muir, J. Myles, T. Natoli, S. Padin, A. Palmese, S. Pandey, F. Paz-Chinchón, A. Pieres, A. A. Plazas Malagón, A. Porredon, C. Pryke, M. Raveri, C. L. Reichardt, M. Rodriguez-Monroy, A. J. Ross, J. E. Ruhl, E. Rykoff, C. Sánchez, E. Sanchez, V. Scarpine, K. K. Schaffer, I. Sevilla-Noarbe, E. Sheldon, E. Shirokoff, M. Smith, M. Soares-Santos, Z. Staniszewski, A. A. Stark, E. Suchyta, M. E. C. Swanson, G. Tarle, D. Thomas, M. A. Troxel, D. L. Tucker, J. D. Vieira, M. Vincenzi, N. Weaverdyck, R. Williamson, B. Yanny, B. Yin, (DES Collaborations) SPT

^*Corresponding author for this work

Australian Astronomical Optics

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

8 Citations (Scopus)

Abstract

We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-y maps generated using data from the South Pole Telescope (SPT) and the Planck mission. We model this cross-correlation measurement together with the galaxy autocorrelation to constrain the distribution of gas in the Universe. We measure the hydrostatic mass bias or, equivalently, the mean halo bias-weighted electron pressure <b_h P_e>, using large-scale information. We find <b_h P_e> to be [0.16^+0.03_-0.04, 0.28^+0.04_-0.05, 0.45^+0.06_-0.10, 0.54^+0.08_-0.07, 0.61^+0.08_-0.06, 0.63^+0.07_-0.08] meV cm⁻³ at redshifts z ∼ [0.30, 0.46, 0.62, 0.77, 0.89, 0.97]. These values are consistent with previous work where measurements exist in the redshift range. We also constrain the mean gas profile using small-scale information, enabled by the high-resolution of the SPT data. We compare our measurements to different parametrized profiles based on the cosmo-OWLS hydrodynamical simulations. We find that our data are consistent with the simulation that assumes an AGN heating temperature of 10^8.5 K but are incompatible with the model that assumes an AGN heating temperature of 10^8.0 K. These comparisons indicate that the data prefer a higher value of electron pressure than the simulations within r_500c of the galaxies’ haloes.

Original language	English
Pages (from-to)	3163-3182
Number of pages	20
Journal	Monthly Notices of the Royal Astronomical Society
Volume	522
Issue number	2
DOIs	https://doi.org/10.1093/mnras/stad1167
Publication status	Published - Jun 2023

Keywords

galaxies: structure
large-scale structure of Universe
cosmology: observations

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Sánchez, J., Omori, Y., Chang, C., Bleem, L. E., Crawford, T., Drlica-Wagner, A., Raghunathan, S., Zacharegkas, G., Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Avila, S., Baxter, E., Bechtol, K., Benson, B. A., Bernstein, G. M., ... (DES Collaborations) SPT (2023). Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck. Monthly Notices of the Royal Astronomical Society, 522(2), 3163-3182. https://doi.org/10.1093/mnras/stad1167

@article{1f3fa2f1b6a44750853d88f253934528,

title = "Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck",

abstract = "We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-y maps generated using data from the South Pole Telescope (SPT) and the Planck mission. We model this cross-correlation measurement together with the galaxy autocorrelation to constrain the distribution of gas in the Universe. We measure the hydrostatic mass bias or, equivalently, the mean halo bias-weighted electron pressure h Pe>, using large-scale information. We find h Pe> to be [0.16+0.03-0.04, 0.28+0.04-0.05, 0.45+0.06-0.10, 0.54+0.08-0.07, 0.61+0.08-0.06, 0.63+0.07-0.08] meV cm−3 at redshifts z ∼ [0.30, 0.46, 0.62, 0.77, 0.89, 0.97]. These values are consistent with previous work where measurements exist in the redshift range. We also constrain the mean gas profile using small-scale information, enabled by the high-resolution of the SPT data. We compare our measurements to different parametrized profiles based on the cosmo-OWLS hydrodynamical simulations. We find that our data are consistent with the simulation that assumes an AGN heating temperature of 108.5 K but are incompatible with the model that assumes an AGN heating temperature of 108.0 K. These comparisons indicate that the data prefer a higher value of electron pressure than the simulations within r500c of the galaxies{\textquoteright} haloes.",

keywords = "galaxies: structure, large-scale structure of Universe, cosmology: observations",

author = "J. S{\'a}nchez and Y. Omori and C. Chang and Bleem, {L. E.} and T. Crawford and A. Drlica-Wagner and S. Raghunathan and G. Zacharegkas and Abbott, {T. M. C.} and M. Aguena and A. Alarcon and S. Allam and O. Alves and A. Amon and S. Avila and E. Baxter and K. Bechtol and Benson, {B. A.} and Bernstein, {G. M.} and E. Bertin and S. Bocquet and D. Brooks and Burke, {D. L.} and A. Campos and Carlstrom, {J. E.} and Rosell, {A. Carnero} and Kind, {M. Carrasco} and J. Carretero and Castander, {F. J.} and R. Cawthon and C. Chang and A. Chen and A. Choi and R. Chown and M. Costanzi and Crites, {A. T.} and M. Crocce and {da Costa}, {L. N.} and Pereira, {M. E. S.} and {de Haan}, T. and {De Vicente}, J. and J. DeRose and S. Desai and Diehl, {H. T.} and Dobbs, {M. A.} and S. Dodelson and P. Doel and J. Elvin-Poole and W. Everett and S. Everett and I. Ferrero and B. Flaugher and P. Fosalba and J. Frieman and J. Garc{\'i}a-Bellido and M. Gatti and George, {E. M.} and Gerdes, {D. W.} and G. Giannini and D. Gruen and Gruendl, {R. A.} and J. Gschwend and G. Gutierrez and Halverson, {N. W.} and Hinton, {S. R.} and Holder, {G. P.} and Hollowood, {D. L.} and Holzapfel, {W. L.} and K. Honscheid and Hrubes, {J. D.} and James, {D. J.} and L. Knox and K. Kuehn and N. Kuropatkin and O. Lahav and Lee, {A. T.} and D. Luong-Van and N. MacCrann and Marshall, {J. L.} and J. McCullough and McMahon, {J. J.} and P. Melchior and J. Mena-Fern{\'a}ndez and F. Menanteau and R. Miquel and L. Mocanu and Mohr, {J. J.} and J. Muir and J. Myles and T. Natoli and S. Padin and A. Palmese and S. Pandey and F. Paz-Chinch{\'o}n and A. Pieres and Malag{\'o}n, {A. A. Plazas} and A. Porredon and C. Pryke and M. Raveri and Reichardt, {C. L.} and M. Rodriguez-Monroy and Ross, {A. J.} and Ruhl, {J. E.} and E. Rykoff and C. S{\'a}nchez and E. Sanchez and V. Scarpine and Schaffer, {K. K.} and I. Sevilla-Noarbe and E. Sheldon and E. Shirokoff and M. Smith and M. Soares-Santos and Z. Staniszewski and Stark, {A. A.} and E. Suchyta and Swanson, {M. E. C.} and G. Tarle and D. Thomas and Troxel, {M. A.} and Tucker, {D. L.} and Vieira, {J. D.} and M. Vincenzi and N. Weaverdyck and R. Williamson and B. Yanny and B. Yin and {(DES Collaborations) SPT}",

year = "2023",

month = jun,

doi = "10.1093/mnras/stad1167",

language = "English",

volume = "522",

pages = "3163--3182",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "2",

}

Sánchez, J, Omori, Y, Chang, C, Bleem, LE, Crawford, T, Drlica-Wagner, A, Raghunathan, S, Zacharegkas, G, Abbott, TMC, Aguena, M, Alarcon, A, Allam, S, Alves, O, Amon, A, Avila, S, Baxter, E, Bechtol, K, Benson, BA, Bernstein, GM, Bertin, E, Bocquet, S, Brooks, D, Burke, DL, Campos, A, Carlstrom, JE, Rosell, AC, Kind, MC, Carretero, J, Castander, FJ, Cawthon, R, Chang, C, Chen, A, Choi, A, Chown, R, Costanzi, M, Crites, AT, Crocce, M, da Costa, LN, Pereira, MES, de Haan, T, De Vicente, J, DeRose, J, Desai, S, Diehl, HT, Dobbs, MA, Dodelson, S, Doel, P, Elvin-Poole, J, Everett, W, Everett, S, Ferrero, I, Flaugher, B, Fosalba, P, Frieman, J, García-Bellido, J, Gatti, M, George, EM, Gerdes, DW, Giannini, G, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Halverson, NW, Hinton, SR, Holder, GP, Hollowood, DL, Holzapfel, WL, Honscheid, K, Hrubes, JD, James, DJ, Knox, L, Kuehn, K, Kuropatkin, N, Lahav, O, Lee, AT, Luong-Van, D, MacCrann, N, Marshall, JL, McCullough, J, McMahon, JJ, Melchior, P, Mena-Fernández, J, Menanteau, F, Miquel, R, Mocanu, L, Mohr, JJ, Muir, J, Myles, J, Natoli, T, Padin, S, Palmese, A, Pandey, S, Paz-Chinchón, F, Pieres, A, Malagón, AAP, Porredon, A, Pryke, C, Raveri, M, Reichardt, CL, Rodriguez-Monroy, M, Ross, AJ, Ruhl, JE, Rykoff, E, Sánchez, C, Sanchez, E, Scarpine, V, Schaffer, KK, Sevilla-Noarbe, I, Sheldon, E, Shirokoff, E, Smith, M, Soares-Santos, M, Staniszewski, Z, Stark, AA, Suchyta, E, Swanson, MEC, Tarle, G, Thomas, D, Troxel, MA, Tucker, DL, Vieira, JD, Vincenzi, M, Weaverdyck, N, Williamson, R, Yanny, B, Yin, B & (DES Collaborations) SPT 2023, 'Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck', Monthly Notices of the Royal Astronomical Society, vol. 522, no. 2, pp. 3163-3182. https://doi.org/10.1093/mnras/stad1167

TY - JOUR

T1 - Mapping gas around massive galaxies

T2 - cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck

AU - Sánchez, J.

AU - Omori, Y.

AU - Chang, C.

AU - Bleem, L. E.

AU - Crawford, T.

AU - Drlica-Wagner, A.

AU - Raghunathan, S.

AU - Zacharegkas, G.

AU - Abbott, T. M. C.

AU - Aguena, M.

AU - Alarcon, A.

AU - Allam, S.

AU - Alves, O.

AU - Amon, A.

AU - Avila, S.

AU - Baxter, E.

AU - Bechtol, K.

AU - Benson, B. A.

AU - Bernstein, G. M.

AU - Bertin, E.

AU - Bocquet, S.

AU - Brooks, D.

AU - Burke, D. L.

AU - Campos, A.

AU - Carlstrom, J. E.

AU - Rosell, A. Carnero

AU - Kind, M. Carrasco

AU - Carretero, J.

AU - Castander, F. J.

AU - Cawthon, R.

AU - Chang, C.

AU - Chen, A.

AU - Choi, A.

AU - Chown, R.

AU - Costanzi, M.

AU - Crites, A. T.

AU - Crocce, M.

AU - da Costa, L. N.

AU - Pereira, M. E. S.

AU - de Haan, T.

AU - De Vicente, J.

AU - DeRose, J.

AU - Desai, S.

AU - Diehl, H. T.

AU - Dobbs, M. A.

AU - Dodelson, S.

AU - Doel, P.

AU - Elvin-Poole, J.

AU - Everett, W.

AU - Everett, S.

AU - Ferrero, I.

AU - Flaugher, B.

AU - Fosalba, P.

AU - Frieman, J.

AU - García-Bellido, J.

AU - Gatti, M.

AU - George, E. M.

AU - Gerdes, D. W.

AU - Giannini, G.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Gschwend, J.

AU - Gutierrez, G.

AU - Halverson, N. W.

AU - Hinton, S. R.

AU - Holder, G. P.

AU - Hollowood, D. L.

AU - Holzapfel, W. L.

AU - Honscheid, K.

AU - Hrubes, J. D.

AU - James, D. J.

AU - Knox, L.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lahav, O.

AU - Lee, A. T.

AU - Luong-Van, D.

AU - MacCrann, N.

AU - Marshall, J. L.

AU - McCullough, J.

AU - McMahon, J. J.

AU - Melchior, P.

AU - Mena-Fernández, J.

AU - Menanteau, F.

AU - Miquel, R.

AU - Mocanu, L.

AU - Mohr, J. J.

AU - Muir, J.

AU - Myles, J.

AU - Natoli, T.

AU - Padin, S.

AU - Palmese, A.

AU - Pandey, S.

AU - Paz-Chinchón, F.

AU - Pieres, A.

AU - Malagón, A. A. Plazas

AU - Porredon, A.

AU - Pryke, C.

AU - Raveri, M.

AU - Reichardt, C. L.

AU - Rodriguez-Monroy, M.

AU - Ross, A. J.

AU - Ruhl, J. E.

AU - Rykoff, E.

AU - Sánchez, C.

AU - Sanchez, E.

AU - Scarpine, V.

AU - Schaffer, K. K.

AU - Sevilla-Noarbe, I.

AU - Sheldon, E.

AU - Shirokoff, E.

AU - Smith, M.

AU - Soares-Santos, M.

AU - Staniszewski, Z.

AU - Stark, A. A.

AU - Suchyta, E.

AU - Swanson, M. E. C.

AU - Tarle, G.

AU - Thomas, D.

AU - Troxel, M. A.

AU - Tucker, D. L.

AU - Vieira, J. D.

AU - Vincenzi, M.

AU - Weaverdyck, N.

AU - Williamson, R.

AU - Yanny, B.

AU - Yin, B.

AU - (DES Collaborations) SPT

PY - 2023/6

Y1 - 2023/6

N2 - We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-y maps generated using data from the South Pole Telescope (SPT) and the Planck mission. We model this cross-correlation measurement together with the galaxy autocorrelation to constrain the distribution of gas in the Universe. We measure the hydrostatic mass bias or, equivalently, the mean halo bias-weighted electron pressure h Pe>, using large-scale information. We find h Pe> to be [0.16+0.03-0.04, 0.28+0.04-0.05, 0.45+0.06-0.10, 0.54+0.08-0.07, 0.61+0.08-0.06, 0.63+0.07-0.08] meV cm−3 at redshifts z ∼ [0.30, 0.46, 0.62, 0.77, 0.89, 0.97]. These values are consistent with previous work where measurements exist in the redshift range. We also constrain the mean gas profile using small-scale information, enabled by the high-resolution of the SPT data. We compare our measurements to different parametrized profiles based on the cosmo-OWLS hydrodynamical simulations. We find that our data are consistent with the simulation that assumes an AGN heating temperature of 108.5 K but are incompatible with the model that assumes an AGN heating temperature of 108.0 K. These comparisons indicate that the data prefer a higher value of electron pressure than the simulations within r500c of the galaxies’ haloes.

AB - We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-y maps generated using data from the South Pole Telescope (SPT) and the Planck mission. We model this cross-correlation measurement together with the galaxy autocorrelation to constrain the distribution of gas in the Universe. We measure the hydrostatic mass bias or, equivalently, the mean halo bias-weighted electron pressure h Pe>, using large-scale information. We find h Pe> to be [0.16+0.03-0.04, 0.28+0.04-0.05, 0.45+0.06-0.10, 0.54+0.08-0.07, 0.61+0.08-0.06, 0.63+0.07-0.08] meV cm−3 at redshifts z ∼ [0.30, 0.46, 0.62, 0.77, 0.89, 0.97]. These values are consistent with previous work where measurements exist in the redshift range. We also constrain the mean gas profile using small-scale information, enabled by the high-resolution of the SPT data. We compare our measurements to different parametrized profiles based on the cosmo-OWLS hydrodynamical simulations. We find that our data are consistent with the simulation that assumes an AGN heating temperature of 108.5 K but are incompatible with the model that assumes an AGN heating temperature of 108.0 K. These comparisons indicate that the data prefer a higher value of electron pressure than the simulations within r500c of the galaxies’ haloes.

KW - galaxies: structure

KW - large-scale structure of Universe

KW - cosmology: observations

UR - http://www.scopus.com/inward/record.url?scp=85161516546&partnerID=8YFLogxK

UR - http://purl.org/au-research/grants/arc/DP200101068

U2 - 10.1093/mnras/stad1167

DO - 10.1093/mnras/stad1167

M3 - Article

AN - SCOPUS:85161516546

SN - 0035-8711

VL - 522

SP - 3163

EP - 3182

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-y maps from SPT and Planck

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