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1by Sun, M., Sehgal, N., Voit, G. M., Donahue, M., Jones, C., Forman, W., Vikhlinin, A., Sarazin, C.“... pressure content for a sample of local galaxy groups from Sun et al. (2009). The group Y_{sph, 500} - M_500...”
Published 2010
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2by Sun, M., Sehgal, N., Voit, G. M., Donahue, M., Jones, C., Forman, W., Vikhlinin, A., Sarazin, C.“... pressure content for a sample of local galaxy groups from Sun et al. (2009). The group Y_{sph, 500} - M_500...”
Published in The Astrophysical Journal (2010)
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3by Marc Davis, Brian F. Gerke, Alison L. Coil, Michael C. Cooper, Renbin Yan, Jeffrey A. Newman, S. M. Faber, David Koo, Puragra Guhathakurta“... and the Red-Sequence Cluster Survey. The specific study discussed here detects clusters and smaller galaxy...”
Published 2008
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4Subjects: “...galaxies: kinematics and dynamics—galaxies: distances and redshifts— galaxies: groups...”
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5by Raouf, Mojtaba, Smith, Rory, Khosroshahi, Habib G., van de Sande, Jesse, Bryant, Julia J., Cortese, Luca, Brough, S., Croom, Scott M., Hwang, Ho Seong, Driver, Simon, López-Sánchez, Ángel R., Ko, Jongwan, Kim, Jae-Woo, Shin, Jihye, Scott, Nicholas, Bland-Hawthorn, Joss, Richards, Samuel N., Owers, Matt, Lawrence, J. S., Konstantopoulos, Iraklis S.“... relaxed and unrelaxed galaxy groups for a sample of 154 galaxies in the SAMI galaxy survey. We...”
Published in The Astrophysical Journal (2020)
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6by Davis, M., Gerke, B. F., Coil, A. L., Cooper, M. C., Yan, R., Newman, J. A., Faber, S. M., Koo, D., Guhathakurta, P.“... and the Red-Sequence Cluster Survey. The specific study discussed here detects clusters and smaller galaxy...”
Published 2005
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7by Wang, Di, Lagos, Claudia D. P., Croom, Scott M., Wright, Ruby J., Bahé, Yannick M., Bryant, Julia J., van de Sande, Jesse, Vaughan, Sam P.“... at $z=0$. We focus on satellite galaxies in galaxy groups and clusters ($10^{12}\,\rm M_{\odot...”
Published 2023
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8by Bleem, L. E., Crawford, T. M., Ansarinejad, B., Benson, B. A., Bocquet, S., Carlstrom, J. E., Chang, C. L., Chown, R., Crites, A. T., de Haan, T., Dobbs, M. A., Everett, W. B., George, E. M., Gualtieri, R., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Knox, L., Lee, A. T., Luong-Van, D., Marrone, D. P., McMahon, J. J., Meyer, S. S., Millea, M., Mocanu, L. M., Mohr, J. J., Natoli, T., Omori, Y., Padin, S., Pryke, C., Raghunathan, S., Reichardt, C. L., Ruhl, J. E., Schaffer, K. K., Shirokoff, E., Staniszewski, Z., Stark, A. A., Vieira, J. D., Williamson, R.“... of astrophysical and cosmological analyses, including studies of the gas properties of galaxies, groups...”
Published in The Astrophysical Journal Supplement Series (2021)
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9“... by the astrophysical uncertainties in modeling the gas pressure profile in galaxy groups and clusters. In this paper we...”
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10by Ramos-Ceja, M. E., Basu, K., Pacaud, F., Bertoldi, F.“... by the astrophysical uncertainties in modeling the gas pressure profile in galaxy groups and clusters. In this paper we...”
Published in Astronomy & Astrophysics (2014)
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11by Ansarinejad, B., Murphy, D. N. A., Shanks, T., Metcalfe, N.“... ATLAS survey, we construct a new catalogue of photometrically selected galaxy groups and clusters using...”
Published in Monthly Notices of the Royal Astronomical Society (2022)
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12by Wang, Di, Lagos, Claudia D. P., Croom, Scott M., Wright, Ruby J., Bahé, Yannick M., Bryant, Julia J., van de Sande, Jesse, Vaughan, Sam P.“... at $z=0$. We focus on satellite galaxies in galaxy groups and clusters ($10^{12}\,\rm M_{\odot...”
Published in Monthly Notices of the Royal Astronomical Society (2023)
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13“..., low-surface-density elliptical galaxies and star clusters, and diffuse galaxy groups. They can also...”
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14by Grandis, S., Mohr, J. J., Costanzi, M., Saro, A., Bocquet, S., Klein, M., Aguena, M., Allam, S., Annis, J., Ansarinejad, B., Bacon, D., Bertin, E., Bleem, L., Brooks, D., Burke, D. L., Rosel, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Choi, A., da Costa, L. N., De Vincente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Everett, S., Ferrero, I., Floyd, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gupta, N., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Lahav, O., Lidman, C., Lima, M., Maia, M. A. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Myles, J., Ogando, R., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Reichardt, C. L., Romer, A. K., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Singh, P., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Weller, J., Wilkinson, R. D., Wu, H.“...) measurements suggests that these low mass contaminants are galaxy groups with masses $\sim3$-$5\times 10^{13...”
Published in Monthly Notices of the Royal Astronomical Society (2021)
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