Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Muldrew S"'
Autor:
Tholerus, E., Casson, F. J., Marsden, S. P., Wilson, T., Brunetti, D., Fox, P., Freethy, S. J., Hender, T. C., Henderson, S. S., Hudoba, A., Kirov, K. K., Koechl, F., Meyer, H., Muldrew, S. I., Olde, C., Patel, B. S., Roach, C. M., Saarelma, S., Xia, G.
STEP is a spherical tokamak prototype power plant that is being designed to demonstrate net electric power. The design phase involves the exploitation of plasma models to optimise fusion performance subject to satisfying various physics and engineeri
Externí odkaz:
http://arxiv.org/abs/2403.09460
Autor:
Penney, J. I., Blain, A. W., Wylezalek, D., Hatch, N. A., Lonsdale, C., Kimball, A., Assef, R. J., Condon, J. J., Eisenhardt, P. R. M., Jones, S. F., Kim, M., Lacy, M., Muldrew, S. I., Petty, S., Sajina, A., Silva, A., Stern, D., Diaz-Santos, T., Tsai, C-W., Wu, J.
We have observed the environments of a population of 33 heavily dust obscured, ultra-luminous, high-redshift galaxies, selected using WISE and NVSS at $z>$1.3 with the Infra-Red Array Camera on the $Spitzer$ Space Telescope over $\rm5.12\,'\times5.12
Externí odkaz:
http://arxiv.org/abs/1811.06818
Autor:
Hatch, N. A., Cooke, E. A., Muldrew, S. I., Hartley, W. G., Almaini, O., Conselice, C. J., Simpson, C. J.
We investigate the effects of dense environments on galaxy evolution by examining how the properties of galaxies in the z = 1.6 protocluster Cl 0218.3-0510 depend on their location. We determine galaxy properties using spectral energy distribution fi
Externí odkaz:
http://arxiv.org/abs/1609.08629
Autor:
Hatch, N. A., Muldrew, S. I., Cooke, E. A., Hartley, W. G., Almaini, O., Simpson, C. J., Conselice, C. J.
We present a comprehensive picture of the Cl0218.3-0510 protocluster at $z=1.623$ across 10 co-moving Mpc. Using filters that tightly bracket the Balmer and 4000 Angstrom breaks of the protocluster galaxies we obtain precise photometric redshifts res
Externí odkaz:
http://arxiv.org/abs/1603.03774
Autor:
Cooke, E. A., Hatch, N. A., Rettura, A., Wylezalek, D., Galametz, A., Stern, D., Brodwin, M., Muldrew, S. I., Almaini, O., Conselice, C. J., Eisenhardt, P. R., Hartley, W. G., Jarvis, M., Seymour, N., Stanford, S. A.
We use a sample of 37 of the densest clusters and protoclusters across $1.3 \le z \le 3.2$ from the Clusters Around Radio-Loud AGN (CARLA) survey to study the formation of massive cluster galaxies. We use optical $i'$-band and infrared 3.6$\mu$m and
Externí odkaz:
http://arxiv.org/abs/1507.00350
Autor:
Old, L., Wojtak, R., Mamon, G. A., Skibba, R. A., Pearce, F. R., Croton, D., Bamford, S., Behroozi, P., de Carvalho, R., Muñoz-Cuartas, J. C., Gifford, D., Gray, M. E., von der Linden, A., Merrifield, M. R., Muldrew, S. I., Müller, V., Pearson, R. J., Ponman, T. J., Rozo, E., Rykoff, E., Saro, A., Sepp, T., Sifón, C., Tempel, E.
This article is the second in a series in which we perform an extensive comparison of various galaxy-based cluster mass estimation techniques that utilise the positions, velocities and colours of galaxies. Our aim is to quantify the scatter, systemat
Externí odkaz:
http://arxiv.org/abs/1502.07347
Autor:
Old, L., Skibba, R. A., Pearce, F. R., Croton, D., Muldrew, S. I., Muñoz-Cuartas, J. C., Gifford, D., Gray, M. E., von der Linden, A., Mamon, G. A., Merrifield, M. R., Müller, V., Pearson, R. J., Ponman, T. J., Saro, A., Sepp, T., Sifón, C., Tempel, E., Tundo, E., Wang, Y. O., Wojtak, R.
This paper is the first in a series in which we perform an extensive comparison of various galaxy-based cluster mass estimation techniques that utilise the positions, velocities and colours of galaxies. Our primary aim is to test the performance of t
Externí odkaz:
http://arxiv.org/abs/1403.4610
We present results from a narrow-band survey of the field around the high redshift radio galaxy MRC 2104-242. We have selected Halpha emitters in a 7sq.arcmin field and compared the measured number density with that of a field sample at similar redsh
Externí odkaz:
http://arxiv.org/abs/1403.4259
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Akademický článek
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