The XMM Cluster Survey: The Stellar Mass Assembly of Fossil Galaxies

Autor: Harrison, Craig D., Miller, Christopher J., Richards, Joseph W., Lloyd-Davies, E. J., Hoyle, Ben, Romer, A. Kathy, Mehrtens, Nicola, Hilton, Matt, Stott, John P., Capozzi, Diego, Collins, Chris A., Deadman, Paul-James, Liddle, Andrew R., Sahlén, Martin, Stanford, S. Adam, Viana, Pedro T. P.

This paper presents both the result of a search for fossil systems (FSs) within the XMM Cluster Survey and the Sloan Digital Sky Survey and the results of a study of the stellar mass assembly and stellar populations of their fossil galaxies. In total

Externí odkaz: http://arxiv.org/abs/1202.4450

The XMM Cluster Survey: Optical analysis methodology and the first data release

Autor: Mehrtens, Nicola, Romer, A. Kathy, Lloyd-Davies, E. J., Hilton, Matt, Miller, Christopher J., Stanford, S. A., Hosmer, Mark, Hoyle, Ben, Collins, Chris A., Liddle, Andrew R., Viana, Pedro T. P., Nichol, Robert C., Stott, John P., Dubois, E. Naomi, Kay, Scott T., Sahlen, Martin, Young, Owain, Short, C. J., Christodoulou, L., Watson, William A., Davidson, Michael, Harrison, Craig D., Baruah, Leon, Smith, Mathew, Burke, Claire, Deadman, Paul-James, Rooney, Philip J., Edmondson, Edward M., West, Michael, Campbell, Heather C., Edge, Alastair C., Mann, Robert G., Wake, David, Benoist, Christophe, da Costa, Luiz, Maia, Marcio A. G., Ogando, Ricardo

The XMM Cluster Survey (XCS) is a serendipitous search for galaxy clusters using all publicly available data in the XMM-Newton Science Archive. Its main aims are to measure cosmological parameters and trace the evolution of X-ray scaling relations. I

Externí odkaz: http://arxiv.org/abs/1106.3056

Mapping the Galactic Halo with blue horizontal branch stars from the 2dF quasar redshift survey

Autor: De Propris, Roberto, Harrison, Craig D., Mares, Peter J., CTIO, University, Cornell

Publikováno v: ApJ, 719, 1582 (2010)

We use 666 blue horizontal branch (BHB) stars from the 2Qz redshift survey to map the Galactic halo in four dimensions (position, distance and velocity). We find that the halo extends to at least 100 kpc in Galactocentric distance, and obeys a single

Externí odkaz: http://arxiv.org/abs/1007.0013

The XMM Cluster Survey: X-ray analysis methodology

Autor: Lloyd-Davies, E. J., Romer, A. Kathy, Mehrtens, Nicola, Hosmer, Mark, Davidson, Michael, Sabirli, Kivanc, Mann, Robert G., Hilton, Matt, Liddle, Andrew R., Viana, Pedro T. P., Campbell, Heather C., Collins, Chris A., Dubois, E. Naomi, Freeman, Peter, Harrison, Craig D., Hoyle, Ben, Kay, Scott T., Kuwertz, Emma, Miller, Christopher J., Nichol, Robert C., Sahlen, Martin, Stanford, S. A., Stott, John P.

Publikováno v: Lloyd-davies, E J, Romer, A K, Mehrtens, N, Hosmer, M, Davidson, M, Sabirli, K, Mann, R G, Hilton, M, Liddle, A R, Viana, P T P, Campbell, H C, Collins, C A, Dubois, E N, Freeman, P, Harrison, C D, Hoyle, B, Kay, S T, Kuwertz, E, Miller, C J, Nichol, R C, Sahlén, M, Stanford, S A & Stott, J P 2011, ' The XMM Cluster Survey: X-ray analysis methodology ', Monthly Notices of the Royal Astronomical Society, vol. 418, no. 1, pp. 14-53 . https://doi.org/10.1111/mnr.2011.418.issue-1

The XMM Cluster Survey (XCS) is a serendipitous search for galaxy clusters using all publicly available data in the XMM-Newton Science Archive. Its main aims are to measure cosmological parameters and trace the evolution of X-ray scaling relations. I

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f9970e3895bd736ec22896b3359974cc
http://sro.sussex.ac.uk/id/eprint/41525/1/XMMCluster.x.pdf

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