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Title: Planck intermediate results: XI. The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies

Abstract

We present the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Survey (SDSS). These are predominantly the central galaxies of their dark matter halos. We calibrate the stellar-to-halo mass conversion using realistic mock catalogues based on the Millennium Simulation. Applying a multi-frequency matched filter to the Planck data for each LBG, and averaging the results in bins of stellar mass, we measure the mean SZ signal down to M* ∼ 2 × 1011 M, with a clear indication of signal at even lower stellar mass. We derive the scaling relation between SZ signal and halo mass by assigning halo properties from our mock catalogues to the real LBGs and simulating the Planck observation process. This relation shows no evidence for deviation from a power law over a halo mass range extending from rich clusters down to M500 ~ 2 × 1013 M, and there is a clear indication of signal down to M500 ~ 4 × 1012 M. Planck's SZ detections in such low-mass halos imply that about a quarter of all baryons have now been seen in the form of hot halo gas, and thatmore » this gas must be less concentrated than the dark matter in such halos in order to remain consistent with X-ray observations. At the high-mass end, the measured SZ signal is 20% lower than found from observations of X-ray clusters, a difference consistent with the magnitude of Malmquist bias effects that were previously estimated for the X-ray sample.« less

Authors:
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; « less
Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE
Contributing Org.:
Planck Collaboration
OSTI Identifier:
1523875
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 557; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Barrena, R., Bartlett, J. G., Battaner, E., Benabed, K., Bernard, J. -P., Bersanelli, M., Bikmaev, I., Bock, J. J., Böhringer, H., Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bourdin, H., Burenin, R., Burigana, C., Butler, R. C., Cabella, P., Chamballu, A., Chary, R. -R., Chiang, L. -Y, Chon, G., Christensen, P. R., Clements, D. L., Colafrancesco, S., Colombi, S., Colombo, L. P. L., Comis, B., Coulais, A., Crill, B. P., Cuttaia, F., Da Silva, A., Dahle, H., Davis, R. J., de Bernardis, P., de Gasperis, G., de Rosa, A., de Zotti, G., Delabrouille, J., Démoclès, J., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Finelli, F., Flores-Cacho, I., Forni, O., Frailis, M., Franceschi, E., Frommert, M., Galeotta, S., Ganga, K., Génova-Santos, R. T., Giard, M., Giraud-Héraud, Y., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Hansen, F. K., Harrison, D., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, T. R., Jaffe, A. H., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Khamitov, I., Kisner, T. S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Lawrence, C. R., Le Jeune, M., Leonardi, R., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Luzzi, G., Macías-Pérez, J. F., MacTavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Maris, M., Marleau, F., Marshall, D. J., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Mazzotta, P., Mei, S., Melchiorri, A., Melin, J. -B., Mendes, L., Mennella, A., 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., Nørgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., Osborne, S., Oxborrow, C. A., Pajot, F., Paoletti, D., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Piffaretti, R., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Poutanen, T., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Ristorcelli, I., Rocha, G., Roman, M., Rosset, C., Rossetti, M., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Savini, G., Scott, D., Spencer, L., Starck, J. -L., Stolyarov, V., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Valenziano, L., Van Tent, B., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Wang, W., Welikala, N., Weller, J., White, S. D. M., White, M., Yvon, D., Zacchei, A., and Zonca, A. Planck intermediate results: XI. The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies. United States: N. p., 2013. Web. doi:10.1051/0004-6361/201220941.
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Barrena, R., Bartlett, J. G., Battaner, E., Benabed, K., Bernard, J. -P., Bersanelli, M., Bikmaev, I., Bock, J. J., Böhringer, H., Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bourdin, H., Burenin, R., Burigana, C., Butler, R. C., Cabella, P., Chamballu, A., Chary, R. -R., Chiang, L. -Y, Chon, G., Christensen, P. R., Clements, D. L., Colafrancesco, S., Colombi, S., Colombo, L. P. L., Comis, B., Coulais, A., Crill, B. P., Cuttaia, F., Da Silva, A., Dahle, H., Davis, R. J., de Bernardis, P., de Gasperis, G., de Rosa, A., de Zotti, G., Delabrouille, J., Démoclès, J., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Finelli, F., Flores-Cacho, I., Forni, O., Frailis, M., Franceschi, E., Frommert, M., Galeotta, S., Ganga, K., Génova-Santos, R. T., Giard, M., Giraud-Héraud, Y., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Hansen, F. K., Harrison, D., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, T. R., Jaffe, A. H., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Khamitov, I., Kisner, T. S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Lawrence, C. R., Le Jeune, M., Leonardi, R., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Luzzi, G., Macías-Pérez, J. F., MacTavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Maris, M., Marleau, F., Marshall, D. J., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Mazzotta, P., Mei, S., Melchiorri, A., Melin, J. -B., Mendes, L., Mennella, A., 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., Nørgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., Osborne, S., Oxborrow, C. A., Pajot, F., Paoletti, D., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Piffaretti, R., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Poutanen, T., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Ristorcelli, I., Rocha, G., Roman, M., Rosset, C., Rossetti, M., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Savini, G., Scott, D., Spencer, L., Starck, J. -L., Stolyarov, V., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Valenziano, L., Van Tent, B., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Wang, W., Welikala, N., Weller, J., White, S. D. M., White, M., Yvon, D., Zacchei, A., & Zonca, A. Planck intermediate results: XI. The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies. United States. doi:10.1051/0004-6361/201220941.
Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., Barreiro, R. B., Barrena, R., Bartlett, J. G., Battaner, E., Benabed, K., Bernard, J. -P., Bersanelli, M., Bikmaev, I., Bock, J. J., Böhringer, H., Bonaldi, A., Bond, J. R., Borrill, J., Bouchet, F. R., Bourdin, H., Burenin, R., Burigana, C., Butler, R. C., Cabella, P., Chamballu, A., Chary, R. -R., Chiang, L. -Y, Chon, G., Christensen, P. R., Clements, D. L., Colafrancesco, S., Colombi, S., Colombo, L. P. L., Comis, B., Coulais, A., Crill, B. P., Cuttaia, F., Da Silva, A., Dahle, H., Davis, R. J., de Bernardis, P., de Gasperis, G., de Rosa, A., de Zotti, G., Delabrouille, J., Démoclès, J., Diego, J. M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T. A., Finelli, F., Flores-Cacho, I., Forni, O., Frailis, M., Franceschi, E., Frommert, M., Galeotta, S., Ganga, K., Génova-Santos, R. T., Giard, M., Giraud-Héraud, Y., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Hansen, F. K., Harrison, D., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, T. R., Jaffe, A. H., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Khamitov, I., Kisner, T. S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lähteenmäki, A., Lamarre, J. -M., Lasenby, A., Lawrence, C. R., Le Jeune, M., Leonardi, R., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Luzzi, G., Macías-Pérez, J. F., MacTavish, C. J., Maffei, B., Maino, D., Mandolesi, N., Maris, M., Marleau, F., Marshall, D. J., Martínez-González, E., Masi, S., Massardi, M., Matarrese, S., Mazzotta, P., Mei, S., Melchiorri, A., Melin, J. -B., Mendes, L., Mennella, A., 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., Nørgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., Osborne, S., Oxborrow, C. A., Pajot, F., Paoletti, D., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Piffaretti, R., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Poutanen, T., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Ristorcelli, I., Rocha, G., Roman, M., Rosset, C., Rossetti, M., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Savini, G., Scott, D., Spencer, L., Starck, J. -L., Stolyarov, V., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Valenziano, L., Van Tent, B., Vielva, P., Villa, F., Vittorio, N., Wade, L. A., Wandelt, B. D., Wang, W., Welikala, N., Weller, J., White, S. D. M., White, M., Yvon, D., Zacchei, A., and Zonca, A. Wed . "Planck intermediate results: XI. The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies". United States. doi:10.1051/0004-6361/201220941. https://www.osti.gov/servlets/purl/1523875.
@article{osti_1523875,
title = {Planck intermediate results: XI. The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies},
author = {Ade, P. A. R. and Aghanim, N. and Arnaud, M. and Ashdown, M. and Atrio-Barandela, F. and Aumont, J. and Baccigalupi, C. and Balbi, A. and Banday, A. J. and Barreiro, R. B. and Barrena, R. and Bartlett, J. G. and Battaner, E. and Benabed, K. and Bernard, J. -P. and Bersanelli, M. and Bikmaev, I. and Bock, J. J. and Böhringer, H. and Bonaldi, A. and Bond, J. R. and Borrill, J. and Bouchet, F. R. and Bourdin, H. and Burenin, R. and Burigana, C. and Butler, R. C. and Cabella, P. and Chamballu, A. and Chary, R. -R. and Chiang, L. -Y and Chon, G. and Christensen, P. R. and Clements, D. L. and Colafrancesco, S. and Colombi, S. and Colombo, L. P. L. and Comis, B. and Coulais, A. and Crill, B. P. and Cuttaia, F. and Da Silva, A. and Dahle, H. and Davis, R. J. and de Bernardis, P. and de Gasperis, G. and de Rosa, A. and de Zotti, G. and Delabrouille, J. and Démoclès, J. and Diego, J. M. and Dole, H. and Donzelli, S. and Doré, O. and Douspis, M. and Dupac, X. and Efstathiou, G. and Enßlin, T. A. and Finelli, F. and Flores-Cacho, I. and Forni, O. and Frailis, M. and Franceschi, E. and Frommert, M. and Galeotta, S. and Ganga, K. and Génova-Santos, R. T. and Giard, M. and Giraud-Héraud, Y. and González-Nuevo, J. and Górski, K. M. and Gregorio, A. and Gruppuso, A. and Hansen, F. K. and Harrison, D. and Hernández-Monteagudo, C. and Herranz, D. and Hildebrandt, S. R. and Hivon, E. and Hobson, M. and Holmes, W. A. and Hornstrup, A. and Hovest, W. and Huffenberger, K. M. and Hurier, G. and Jaffe, T. R. and Jaffe, A. H. and Jones, W. C. and Juvela, M. and Keihänen, E. and Keskitalo, R. and Khamitov, I. and Kisner, T. S. and Kneissl, R. and Knoche, J. and Kunz, M. and Kurki-Suonio, H. and Lähteenmäki, A. and Lamarre, J. -M. and Lasenby, A. and Lawrence, C. R. and Le Jeune, M. and Leonardi, R. and Lilje, P. B. and Linden-Vørnle, M. and López-Caniego, M. and Lubin, P. M. and Luzzi, G. and Macías-Pérez, J. F. and MacTavish, C. J. and Maffei, B. and Maino, D. and Mandolesi, N. and Maris, M. and Marleau, F. and Marshall, D. J. and Martínez-González, E. and Masi, S. and Massardi, M. and Matarrese, S. and Mazzotta, P. and Mei, S. and Melchiorri, A. and Melin, J. -B. and Mendes, L. and Mennella, A. 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 Nørgaard-Nielsen, H. U. and Noviello, F. and Novikov, D. and Novikov, I. and Osborne, S. and Oxborrow, C. A. and Pajot, F. and Paoletti, D. and Perotto, L. and Perrotta, F. and Piacentini, F. and Piat, M. and Pierpaoli, E. and Piffaretti, R. and Plaszczynski, S. and Pointecouteau, E. and Polenta, G. and Popa, L. and Poutanen, T. and Pratt, G. W. and Prunet, S. and Puget, J. -L. and Rachen, J. P. and Rebolo, R. and Reinecke, M. and Remazeilles, M. and Renault, C. and Ricciardi, S. and Ristorcelli, I. and Rocha, G. and Roman, M. and Rosset, C. and Rossetti, M. and Rubiño-Martín, J. A. and Rusholme, B. and Sandri, M. and Savini, G. and Scott, D. and Spencer, L. and Starck, J. -L. and Stolyarov, V. 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 Valenziano, L. and Van Tent, B. and Vielva, P. and Villa, F. and Vittorio, N. and Wade, L. A. and Wandelt, B. D. and Wang, W. and Welikala, N. and Weller, J. and White, S. D. M. and White, M. and Yvon, D. and Zacchei, A. and Zonca, A.},
abstractNote = {We present the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Survey (SDSS). These are predominantly the central galaxies of their dark matter halos. We calibrate the stellar-to-halo mass conversion using realistic mock catalogues based on the Millennium Simulation. Applying a multi-frequency matched filter to the Planck data for each LBG, and averaging the results in bins of stellar mass, we measure the mean SZ signal down to M* ∼ 2 × 1011 M⊙, with a clear indication of signal at even lower stellar mass. We derive the scaling relation between SZ signal and halo mass by assigning halo properties from our mock catalogues to the real LBGs and simulating the Planck observation process. This relation shows no evidence for deviation from a power law over a halo mass range extending from rich clusters down to M500 ~ 2 × 1013 M⊙, and there is a clear indication of signal down to M500 ~ 4 × 1012 M⊙. Planck's SZ detections in such low-mass halos imply that about a quarter of all baryons have now been seen in the form of hot halo gas, and that this gas must be less concentrated than the dark matter in such halos in order to remain consistent with X-ray observations. At the high-mass end, the measured SZ signal is 20% lower than found from observations of X-ray clusters, a difference consistent with the magnitude of Malmquist bias effects that were previously estimated for the X-ray sample.},
doi = {10.1051/0004-6361/201220941},
journal = {Astronomy and Astrophysics},
number = ,
volume = 557,
place = {United States},
year = {2013},
month = {8}
}

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Fig. 1 Fig. 1: Distributions in colour (left) and redshift (right) of our locally brightest galaxies and of the SDSS/DR7 population from which they were drawn. Black histograms refer to the parent sample and red histograms to the locally brightest galaxies. The panels in each set correspond to five disjoint ranges ofmore » log10 $M$/$M$ , as indicated in the labels. In the left-hand set, additional labels give the number of galaxies contributing to the parent (black) and locally brightest (red) histograms. Dashed vertical lines in these same panels indicate the colour we use to separate red and blue galaxies in Fig. 3 below.« less

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Galaxy cluster X-ray luminosity scaling relations from a representative local sample (REXCESS)
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Breaking the hierarchy of galaxy formation
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The impact of galaxy formation on the X-ray evolution of clusters
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Planck pre-launch status: The Planck -LFI programme
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Sunyaev-Zel’dovich signal of the maxBCG SDSS galaxy clusters in WMAP
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The 10 Meter South Pole Telescope
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Scaling relations for galaxy clusters in the Millennium-XXL simulation: Scaling relations for clusters in the MXXL
journal, October 2012


Galaxy Clusters Selected with the Sunyaev-Zel'Dovich Effect from 2008 South pole Telescope Observations
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Galaxy Clusters Discovered with a Sunyaev-Zel'Dovich Effect Survey
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Modeling galaxy formation in evolving dark matter halos
journal, January 1991


Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the Sloan Digital Sky Survey: stellar mass, luminosity, morphology and environment dependencies
journal, May 2006


Revisiting the cosmic cooling crisis
journal, October 2001

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Quasar Feedback on the Intracluster Medium
journal, December 2002

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K -Corrections and Filter Transformations in the Ultraviolet, Optical, and Near-Infrared
journal, January 2007

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Constraints on the Relationship Between Stellar mass and halo mass at low and high Redshift
journal, January 2010

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Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology
journal, October 2008

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Catalog extraction in SZ cluster surveys: a matched filter approach
journal, September 2006


Cooling and heating the intracluster medium in hydrodynamical simulations
journal, July 2003


Galaxy formation through hierarchical clustering
journal, September 1991

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  • The Astrophysical Journal, Vol. 379
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APEX-SZ first light and instrument status
journal, December 2006


SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
journal, January 2011

  • Komatsu, E.; Smith, K. M.; Dunkley, J.
  • The Astrophysical Journal Supplement Series, Vol. 192, Issue 2
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Planck early results. IV. First assessment of the High Frequency Instrument in-flight performance
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Galactic Stellar and Substellar Initial Mass Function
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  • Chabrier, Gilles
  • Publications of the Astronomical Society of the Pacific, Vol. 115, Issue 809
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Planck early results. XII. Cluster Sunyaev-Zeldovich optical scaling relations
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Planck early results. V. The Low Frequency Instrument data processing
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On the presence of thermal Sunyaev--Zel'dovich induced signal in the first-year WMAP temperature maps
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Planck early results. II. The thermal performance of Planck
journal, December 2011


THE ATACAMA COSMOLOGY TELESCOPE: SUNYAEV-ZEL'DOVICH-SELECTED GALAXY CLUSTERS AT 148 GHz IN THE 2008 SURVEY
journal, August 2011

  • Marriage, Tobias A.; Acquaviva, Viviana; Ade, Peter A. R.
  • The Astrophysical Journal, Vol. 737, Issue 2
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Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance
journal, December 2011


Simulations of AGN Feedback in Galaxy Clusters and Groups: Impact on Gas Fractions and the L X - T Scaling Relation
journal, October 2008

  • Puchwein, E.; Sijacki, D.; Springel, V.
  • The Astrophysical Journal, Vol. 687, Issue 2
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The Sunyaev–Zel'dovich effect
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Planck pre-launch status: High Frequency Instrument polarization calibration
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K ‐band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
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  • Lin, Yen‐Ting; Mohr, Joseph J.
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Simulations of the formation, evolution and clustering of galaxies and quasars
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The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
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  • Monthly Notices of the Royal Astronomical Society, Vol. 365, Issue 1
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Planck intermediate results : X. Physics of the hot gas in the Coma cluster
journal, June 2013


The Seventh data Release of the Sloan Digital sky Survey
journal, May 2009

  • Abazajian, Kevork N.; Adelman-McCarthy, Jennifer K.; Agüeros, Marcel A.
  • The Astrophysical Journal Supplement Series, Vol. 182, Issue 2
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Estimating the redshift distribution of photometric galaxy samples - II. Applications and tests of a new method
journal, July 2009


Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
journal, December 2011


Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample
journal, December 2011


X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation
journal, March 2004


On Foreground Removal from the Wilkinson Microwave Anisotropy Probe Data by an Internal Linear Combination Method: Limitations and Implications
journal, September 2004

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Planck    pre-launch status: Expected LFI polarisation capability
journal, September 2010


Planck early results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters
journal, December 2011


Planck intermediate results : V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect⋆
journal, February 2013


Planck pre-launch status: The HFI instrument, from specification to actual performance
journal, September 2010


Planck pre-launch status: Design and description of the Low Frequency Instrument
journal, September 2010


New York University Value-Added Galaxy Catalog: A Galaxy Catalog Based on New Public Surveys
journal, June 2005

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A SUNYAEV-ZEL'DOVICH-SELECTED SAMPLE OF THE MOST MASSIVE GALAXY CLUSTERS IN THE 2500 deg 2 SOUTH POLE TELESCOPE SURVEY
journal, August 2011


    Works referencing / citing this record:

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    The failure of stellar feedback, magnetic fields, conduction, and morphological quenching in maintaining red galaxies
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    Spectral Distortions in CMB by the Bulk Comptonization Due to Zeldovich Pancakes
    journal, July 2019