The XMM-LSS survey: the Class 1 cluster sample over the initial 5 deg2 and its cosmological modelling★
Article first published online: 21 NOV 2007
Monthly Notices of the Royal Astronomical Society
Volume 382, Issue 3, pages 1289–1308, December 2007
How to Cite
Pacaud, F., Pierre, M., Adami, C., Altieri, B., Andreon, S., Chiappetti, L., Detal, A., Duc, P.-A., Galaz, G., Gueguen, A., Le Fèvre, J.-P., Hertling, G., Libbrecht, C., Melin, J.-B., Ponman, T. J., Quintana, H., Refregier, A., Sprimont, P.-G., Surdej, J., Valtchanov, I., Willis, J. P., Alloin, D., Birkinshaw, M., Bremer, M. N., Garcet, O., Jean, C., Jones, L. R., Le Fèvre, O., Maccagni, D., Mazure, A., Proust, D., Röttgering, H. J. A. and Trinchieri, G. (2007), The XMM-LSS survey: the Class 1 cluster sample over the initial 5 deg2 and its cosmological modelling. Monthly Notices of the Royal Astronomical Society, 382: 1289–1308. doi: 10.1111/j.1365-2966.2007.12468.x
- Issue published online: 21 NOV 2007
- Article first published online: 21 NOV 2007
- Accepted 2007 September 12. Received 2007 September 12; in original form 2007 March 7
Figure B2. Images of the C1 clusters (sorted by right ascension). Left: X-ray/Z-band overlay of the central 7 arcmin. Right: true colour (g, r, i) image with X-ray contours and measured redshift in the central 1.5 Mpc.
Figure C1. Images of the C1 nearby galaxies. Left: 7 arcmin wide L-band image overlayed with X-ray contours. Right: 5 arcmin wide true colour (g, r, i) image overlayed with X-ray contours.
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