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Title: Planck intermediate results: XL. The Sunyaev-Zeldovich signal from the Virgo cluster

Abstract

The Virgo cluster is the largest Sunyaev-Zeldovich (SZ) source in the sky, both in terms of angular size and total integrated flux. Planck’s wide angular scale and frequency coverage, together with its high sensitivity, enable a detailed study of this big object through the SZ effect. Virgo is well resolved by Planck, showing an elongated structure that correlates well with the morphology observed from X-rays, but extends beyond the observed X-ray signal. We find good agreement between the SZ signal (or Compton parameter, yc) observed by Planck and the expected signal inferred from X-ray observations and simple analytical models. Owing to its proximity to us, the gas beyond the virial radius in Virgo can be studied with unprecedented sensitivity by integrating the SZ signal over tens of square degrees. In this paper, we study the signal in the outskirts of Virgo and compare it with analytical models and a constrained simulation of the environment of Virgo. Planck data suggest that significant amounts of low-density plasma surround Virgo, out to twice the virial radius. We find the SZ signal in the outskirts of Virgo to be consistent with a simple model that extrapolates the inferred pressure at lower radii, while assumingmore » that the temperature stays in the keV range beyond the virial radius. The observed signal is also consistent with simulations and points to a shallow pressure profile in the outskirts of the cluster. This reservoir of gas at large radii can be linked with the hottest phase of the elusivewarm/hot intergalactic medium. Taking the lack of symmetry of Virgo into account, we find that a prolate model is favoured by the combination of SZ and X-ray data, in agreement with predictions. In conclusion, based on the combination of the same SZ and X-ray data, we constrain the total amount of gas in Virgo. Under the hypothesis that the abundance of baryons in Virgo is representative of the cosmic average, we also infer a distance for Virgo of approximately 18 Mpc, in good agreement with previous estimates.« less

Authors:
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; « less
Publication Date:
Research Org.:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
Contributing Org.:
Planck Collaboration
OSTI Identifier:
1398448
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 596; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; ISM; galaxies; Virgo cluster; intracluster medium; cosmic background radiation; large-scale structure of Universe

Citation Formats

Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartolo, N., Battaner, E., Benabed, K., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., Churazov, E., Clements, D. L., Colombo, L. P. L., Combet, C., Comis, B., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Hansen, F. K., Harrison, D. L., Helou, G., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Leonardi, R., Levrier, F., Liguori, M., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maffei, B., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marcos-Caballero, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mennella, A., Migliaccio, M., Mitra, S., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Oxborrow, C. A., Pagano, L., Pajot, F., Paoletti, D., Pasian, F., Pearson, T. J., Perdereau, O., Perotto, L., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Savini, G., Schaefer, B. M., Scott, D., Soler, J. D., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Weller, J., Yvon, D., Zacchei, A., and Zonca, A. Planck intermediate results: XL. The Sunyaev-Zeldovich signal from the Virgo cluster. United States: N. p., 2016. Web. doi:10.1051/0004-6361/201527743.
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Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartolo, N., Battaner, E., Benabed, K., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., Churazov, E., Clements, D. L., Colombo, L. P. L., Combet, C., Comis, B., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Hansen, F. K., Harrison, D. L., Helou, G., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Leonardi, R., Levrier, F., Liguori, M., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maffei, B., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marcos-Caballero, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mennella, A., Migliaccio, M., Mitra, S., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Oxborrow, C. A., Pagano, L., Pajot, F., Paoletti, D., Pasian, F., Pearson, T. J., Perdereau, O., Perotto, L., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Savini, G., Schaefer, B. M., Scott, D., Soler, J. D., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Weller, J., Yvon, D., Zacchei, A., & Zonca, A. Planck intermediate results: XL. The Sunyaev-Zeldovich signal from the Virgo cluster. United States. https://doi.org/10.1051/0004-6361/201527743
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Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartolo, N., Battaner, E., Benabed, K., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., Churazov, E., Clements, D. L., Colombo, L. P. L., Combet, C., Comis, B., Couchot, F., Coulais, A., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Dolag, K., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Gudmundsson, J. E., Hansen, F. K., Harrison, D. L., Helou, G., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Leonardi, R., Levrier, F., Liguori, M., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maffei, B., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Marcos-Caballero, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Mazzotta, P., Meinhold, P. R., Melchiorri, A., Mennella, A., Migliaccio, M., Mitra, S., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Oxborrow, C. A., Pagano, L., Pajot, F., Paoletti, D., Pasian, F., Pearson, T. J., Perdereau, O., Perotto, L., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Savini, G., Schaefer, B. M., Scott, D., Soler, J. D., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Weller, J., Yvon, D., Zacchei, A., and Zonca, A. Mon . "Planck intermediate results: XL. The Sunyaev-Zeldovich signal from the Virgo cluster". United States. https://doi.org/10.1051/0004-6361/201527743. https://www.osti.gov/servlets/purl/1398448.
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@article{osti_1398448,
title = {Planck intermediate results: XL. The Sunyaev-Zeldovich signal from the Virgo cluster},
author = {Ade, P. A. R. and Aghanim, N. and Arnaud, M. and Ashdown, M. and Aumont, J. and Baccigalupi, C. and Banday, A. J. and Barreiro, R. B. and Bartolo, N. and Battaner, E. and Benabed, K. and Benoit-Lévy, A. and Bernard, J. -P. and Bersanelli, M. and Bielewicz, P. and Bonaldi, A. and Bonavera, L. and Bond, J. R. and Borrill, J. and Bouchet, F. R. and Burigana, C. and Butler, R. C. and Calabrese, E. and Cardoso, J. -F. and Catalano, A. and Chamballu, A. and Chiang, H. C. and Christensen, P. R. and Churazov, E. and Clements, D. L. and Colombo, L. P. L. and Combet, C. and Comis, B. and Couchot, F. and Coulais, A. and Crill, B. P. and Curto, A. and Cuttaia, F. and Danese, L. and Davies, R. D. and Davis, R. J. and de Bernardis, P. and de Rosa, A. and de Zotti, G. and Delabrouille, J. and Dickinson, C. and Diego, J. M. and Dolag, K. and Dole, H. and Donzelli, S. and Doré, O. and Douspis, M. and Ducout, A. and Dupac, X. and Efstathiou, G. and Elsner, F. and Enßlin, T. A. and Eriksen, H. K. and Finelli, F. and Forni, O. and Frailis, M. and Fraisse, A. A. and Franceschi, E. and Galeotta, S. and Galli, S. and Ganga, K. and Giard, M. and Giraud-Héraud, Y. and Gjerløw, E. and González-Nuevo, J. and Górski, K. M. and Gregorio, A. and Gruppuso, A. and Gudmundsson, J. E. and Hansen, F. K. and Harrison, D. L. and Helou, G. and Hernández-Monteagudo, C. and Herranz, D. and Hildebrandt, S. R. and Hivon, E. and Hobson, M. and Hornstrup, A. and Hovest, W. and Huffenberger, K. M. and Hurier, G. and Jaffe, A. H. and Jaffe, T. R. and Jones, W. C. and Keihänen, E. and Keskitalo, R. and Kisner, T. S. and Kneissl, R. and Knoche, J. and Kunz, M. and Kurki-Suonio, H. and Lagache, G. and Lamarre, J. -M. and Lasenby, A. and Lattanzi, M. and Lawrence, C. R. and Leonardi, R. and Levrier, F. and Liguori, M. and Lilje, P. B. and Linden-Vørnle, M. and López-Caniego, M. and Lubin, P. M. and Macías-Pérez, J. F. and Maffei, B. and Maggio, G. and Maino, D. and Mandolesi, N. and Mangilli, A. and Marcos-Caballero, A. and Maris, M. and Martin, P. G. and Martínez-González, E. and Masi, S. and Matarrese, S. and Mazzotta, P. and Meinhold, P. R. and Melchiorri, A. and Mennella, A. and Migliaccio, M. and Mitra, S. and Miville-Deschênes, M. -A. and Moneti, A. and Montier, L. and Morgante, G. and Mortlock, D. and Munshi, D. and Murphy, J. A. and Naselsky, P. and Nati, F. and Natoli, P. and Noviello, F. and Novikov, D. and Novikov, I. and Oppermann, N. and Oxborrow, C. A. and Pagano, L. and Pajot, F. and Paoletti, D. and Pasian, F. and Pearson, T. J. and Perdereau, O. and Perotto, L. and Pettorino, V. and Piacentini, F. and Piat, M. and Pierpaoli, E. and Plaszczynski, S. and Pointecouteau, E. and Polenta, G. and Ponthieu, N. and Pratt, G. W. and Prunet, S. and Puget, J. -L. and Rachen, J. P. and Reinecke, M. and Remazeilles, M. and Renault, C. and Renzi, A. and Ristorcelli, I. and Rocha, G. and Rosset, C. and Rossetti, M. and Roudier, G. and Rubiño-Martín, J. A. and Rusholme, B. and Sandri, M. and Santos, D. and Savelainen, M. and Savini, G. and Schaefer, B. M. and Scott, D. and Soler, J. D. and Stolyarov, V. and Stompor, R. and Sudiwala, R. and Sunyaev, R. and Sutton, D. and Suur-Uski, A. -S. and Sygnet, J. -F. and Tauber, J. A. and Terenzi, L. and Toffolatti, L. and Tomasi, M. and Tristram, M. and Tucci, M. and Umana, G. and Valenziano, L. and Valiviita, J. and Van Tent, B. and Vielva, P. and Villa, F. and Wade, L. A. and Wandelt, B. D. and Wehus, I. K. and Weller, J. and Yvon, D. and Zacchei, A. and Zonca, A.},
abstractNote = {The Virgo cluster is the largest Sunyaev-Zeldovich (SZ) source in the sky, both in terms of angular size and total integrated flux. Planck’s wide angular scale and frequency coverage, together with its high sensitivity, enable a detailed study of this big object through the SZ effect. Virgo is well resolved by Planck, showing an elongated structure that correlates well with the morphology observed from X-rays, but extends beyond the observed X-ray signal. We find good agreement between the SZ signal (or Compton parameter, yc) observed by Planck and the expected signal inferred from X-ray observations and simple analytical models. Owing to its proximity to us, the gas beyond the virial radius in Virgo can be studied with unprecedented sensitivity by integrating the SZ signal over tens of square degrees. In this paper, we study the signal in the outskirts of Virgo and compare it with analytical models and a constrained simulation of the environment of Virgo. Planck data suggest that significant amounts of low-density plasma surround Virgo, out to twice the virial radius. We find the SZ signal in the outskirts of Virgo to be consistent with a simple model that extrapolates the inferred pressure at lower radii, while assuming that the temperature stays in the keV range beyond the virial radius. The observed signal is also consistent with simulations and points to a shallow pressure profile in the outskirts of the cluster. This reservoir of gas at large radii can be linked with the hottest phase of the elusivewarm/hot intergalactic medium. Taking the lack of symmetry of Virgo into account, we find that a prolate model is favoured by the combination of SZ and X-ray data, in agreement with predictions. In conclusion, based on the combination of the same SZ and X-ray data, we constrain the total amount of gas in Virgo. Under the hypothesis that the abundance of baryons in Virgo is representative of the cosmic average, we also infer a distance for Virgo of approximately 18 Mpc, in good agreement with previous estimates.},
doi = {10.1051/0004-6361/201527743},
journal = {Astronomy and Astrophysics},
number = ,
volume = 596,
place = {United States},
year = {Mon Dec 12 00:00:00 EST 2016},
month = {Mon Dec 12 00:00:00 EST 2016}
}
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    Statistical properties of Galactic CMB foregrounds: dust and synchrotron
    journal, June 2018

    • Kandel, D.; Lazarian, A.; Pogosyan, D.
    • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 1
    • DOI: 10.1093/mnras/sty1115

    Planck's view on the spectrum of the Sunyaev–Zeldovich effect
    journal, February 2018

    • Erler, Jens; Basu, Kaustuv; Chluba, Jens
    • Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 3
    • DOI: 10.1093/mnras/sty327

    Probing galaxy cluster and intra-cluster gas with luminous red galaxies
    journal, May 2019

    • Gong, Yan; Ma, Yin-Zhe; Tanimura, Hideki
    • Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 4
    • DOI: 10.1093/mnras/stz1177

    Statistical properties of polarized CMB foreground maps
    journal, June 2019

    • von Hausegger, Sebastian; Gammelgaard Ravnebjerg, Aske; Liu, Hao
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
    • DOI: 10.1093/mnras/stz1582

    Searching for H i imprints in cosmic web filaments with 21-cm intensity mapping
    journal, August 2019

    • Tramonte, Denis; Ma, Yin-Zhe; Li, Yi-Chao
    • Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 1
    • DOI: 10.1093/mnras/stz2146

    The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
    journal, November 2019

    • Davies, Jonathan J.; Crain, Robert A.; Oppenheimer, Benjamin D.
    • Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 3
    • DOI: 10.1093/mnras/stz3201

    The impact of the observed baryon distribution in haloes on the total matter power spectrum
    journal, December 2019

    • Debackere, Stijn N. B.; Schaye, Joop; Hoekstra, Henk
    • Monthly Notices of the Royal Astronomical Society, Vol. 492, Issue 2
    • DOI: 10.1093/mnras/stz3446

    Probing primordial gravitational waves: Ali CMB Polarization Telescope
    journal, February 2018

    • Li, Hong; Li, Si-Yu; Liu, Yang
    • National Science Review, Vol. 6, Issue 1
    • DOI: 10.1093/nsr/nwy019

    Strategies for detecting the missing hot baryons in the universe
    journal, October 2015

    • Bregman, Joel N.; Alves, Guilherme Camargo; Miller, Matthew J.
    • Journal of Astronomical Telescopes, Instruments, and Systems, Vol. 1, Issue 4
    • DOI: 10.1117/1.jatis.1.4.045003

    The FABLE simulations: A feedback model for galaxies, groups and clusters
    text, January 2019

    • Henden, Nicholas; Puchwein, Ewald; Shen, Sijing
    • Apollo - University of Cambridge Repository
    • DOI: 10.17863/cam.43228

    The COS-Halos Survey: Metallicities in the Low-redshift Circumgalactic Medium
    journal, March 2017

    • Prochaska, J. Xavier; Werk, Jessica K.; Worseck, Gábor
    • The Astrophysical Journal, Vol. 837, Issue 2
    • DOI: 10.3847/1538-4357/aa6007

    A Measurement of the Cosmic Microwave Background B -mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data
    journal, October 2017

    Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
    journal, September 2019

    • Golovich, N.; Dawson, W. A.; Wittman, D. M.
    • The Astrophysical Journal, Vol. 882, Issue 1
    • DOI: 10.3847/1538-4357/ab2f90

    Relieving tensions related to the lensing of the cosmic microwave background temperature power spectra
    journal, January 2017

    THE STACKED THERMAL SUNYAEV–ZEL’DOVICH SIGNAL OF LOCALLY BRIGHTEST GALAXIES IN PLANCK FULL MISSION DATA: EVIDENCE FOR GALAXY FEEDBACK?
    journal, July 2015

    Exploring cosmic origins with CORE: B -mode component separation
    journal, April 2018

    • Remazeilles, M.; Banday, A. J.; Baccigalupi, C.
    • Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 04
    • DOI: 10.1088/1475-7516/2018/04/023

    Impact of thermal diffusion and other abundance anomalies on cosmological uses of galaxy clusters
    journal, April 2014

    • Medvedev, P.; Gilfanov, M.; Sazonov, S.
    • Monthly Notices of the Royal Astronomical Society, Vol. 440, Issue 3
    • DOI: 10.1093/mnras/stu434

    Another shock for the Bullet cluster, and the source of seed electrons for radio relics
    journal, March 2015

    • Shimwell, Timothy W.; Markevitch, Maxim; Brown, Shea
    • Monthly Notices of the Royal Astronomical Society, Vol. 449, Issue 2
    • DOI: 10.1093/mnras/stv334

    Turbulence and particle acceleration in giant radio haloes: the origin of seed electrons
    journal, December 2016

    • Pinzke, Anders; Oh, S. Peng; Pfrommer, Christoph
    • Monthly Notices of the Royal Astronomical Society, Vol. 465, Issue 4
    • DOI: 10.1093/mnras/stw3024

    SZE observables, pressure profiles and centre offsets in Magneticum simulation galaxy clusters
    journal, April 2017

    • Gupta, N.; Saro, A.; Mohr, J. J.
    • Monthly Notices of the Royal Astronomical Society, Vol. 469, Issue 3
    • DOI: 10.1093/mnras/stx715

    A search for warm/hot gas filaments between pairs of SDSS Luminous Red Galaxies
    journal, November 2018

    • Tanimura, Hideki; Hinshaw, Gary; McCarthy, Ian G.
    • Monthly Notices of the Royal Astronomical Society, Vol. 483, Issue 1
    • DOI: 10.1093/mnras/sty3118

    The BAHAMAS project: the CMB–large-scale structure tension and the roles of massive neutrinos and galaxy formation
    journal, February 2018

    • McCarthy, Ian G.; Bird, Simeon; Schaye, Joop
    • Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 3
    • DOI: 10.1093/mnras/sty377

    The stellar halo of isolated central galaxies in the Hyper Suprime-Cam imaging survey
    journal, May 2019

    • Wang, Wenting; Han, Jiaxin; Sonnenfeld, Alessandro
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 2
    • DOI: 10.1093/mnras/stz1339

    Gaia-DR2 distance to the W3 Complex in the Perseus Arm
    journal, May 2019

    • Navarete, Felipe; Galli, Phillip A. B.; Damineli, Augusto
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 2
    • DOI: 10.1093/mnras/stz1442

    Manufacturing cosmic rays in the evolving dynamical states of galaxy clusters
    journal, July 2019

    • John, Reju Sam; Paul, Surajit; Iapichino, Luigi
    • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 1
    • DOI: 10.1093/mnras/stz1785

    A radio ridge connecting two galaxy clusters in a filament of the cosmic web
    journal, June 2019

    String Theory Explanation of Large-Scale Anisotropy and Anomalous Alignment
    journal, March 2018

    Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
    text, January 2017

    • Soergel, Bjoern; Giannantonio, Tommaso; Efstathiou, George
    • Apollo - University of Cambridge Repository
    • DOI: 10.17863/cam.10088

    Constraining ƒ(R) Gravity by the Large-Scale Structure
    journal, July 2015

    • de Martino, Ivan; De Laurentis, Mariafelicia; Capozziello, Salvatore
    • Universe, Vol. 1, Issue 2
    • DOI: 10.3390/universe1020123

    General Relativity and Cosmology: Unsolved Questions and Future Directions
    journal, September 2016

    Gas Contents of Galaxy Groups from Thermal Sunyaev–Zel’dovich Effects
    journal, February 2018

    Evidence for an X-Ray to Gamma-Ray Virial Shock Signal from the Coma Cluster
    journal, December 2018

    PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at 0.2 < z < 0.9
    journal, October 2019

    • Berti, Angela M.; Coil, Alison L.; Hearin, Andrew P.
    • The Astrophysical Journal, Vol. 884, Issue 1
    • DOI: 10.3847/1538-4357/ab3b5d
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