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Galaxy groups in the COSMOS

Galaxy groups in the COSMOS. Alexis Finoguenov Max-Planck Institut fuer extraterrestrische Physik L. Guzzo, G. Hasinger, N. Scoville, A. Leauthaud, J.P. Kneib, H. Boehringer, & COSMOS collaboration. XMM COSMOS. PHOTO Z. COSMOS. 420 photo-z structures: z=0.1 z=0.3 z=0.5 z=0.7 z=1.

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Galaxy groups in the COSMOS

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  1. Galaxy groups in the COSMOS Alexis Finoguenov Max-Planck Institut fuer extraterrestrische Physik L. Guzzo,G. Hasinger, N. Scoville, A. Leauthaud, J.P. Kneib, H. Boehringer, & COSMOS collaboration

  2. XMMCOSMOS X-ray Scaling relation with lensing mass estimates

  3. PHOTOZ COSMOS 420 photo-z structures: z=0.1 z=0.3 z=0.5 z=0.7 z=1 X-ray Scaling relation with lensing mass estimates

  4. X-ray Scaling relation with lensing mass estimates

  5. X-ray cluster catalog X-ray Scaling relation with lensing mass estimates

  6. Redshift distribution X-ray Scaling relation with lensing mass estimates

  7. Log(N)-log(S) X-ray Scaling relation with lensing mass estimates

  8. Luminosity Function BCS (Ebeling et al. 1998) z<0.6 z>0.6 0<z<1.3 X-ray Scaling relation with lensing mass estimates

  9. COSMOS: X-ray selected clusters with weak lensing detection X-ray Scaling relation with lensing mass estimates

  10. Stacked lensing signal X-ray Scaling relation with lensing mass estimates

  11. M(lensing)-T relation AF et al. 2001 Vikhlinin et al. 2005 11 most luminous clusters at z~0.2 Bardeau et al. Stacked analysis • Merger clusters scatter more from the M-T relation • Luminosity selection is contaminated by the low-mass clusters mergers X-ray Scaling relation with lensing mass estimates

  12. X-ray Scaling relation with lensing mass estimates

  13. X-ray Scaling relation with lensing mass estimates

  14. X-ray Scaling relation with lensing mass estimates

  15. X-ray Scaling relation with lensing mass estimates

  16. X-ray Scaling relation with lensing mass estimates

  17. X-ray Scaling relation with lensing mass estimates

  18. X-ray Scaling relation with lensing mass estimates

  19. X-ray Scaling relation with lensing mass estimates

  20. X-ray Scaling relation with lensing mass estimates

  21. X-ray Scaling relation with lensing mass estimates

  22. X-ray Scaling relation with lensing mass estimates

  23. Conclusions • COSMOS survey explores the new regime of cluster fluxes • logN-logS is found to be similar yet somewhat higher then the predictions form the previous surveys • No evolution of the X-ray luminosity function is detected at probed luminosities • Lensing mass estimates extend to down to group regime X-ray Scaling relation with lensing mass estimates

  24. COSMOS -- team & collaborators Colin Norman Alexandre Refregier Alvio Renzini Jason Rhodes Mike Rich Dave Sanders Shunji Sasaki Dave Schminovich Eva Schinnerer Nick Scoville Marco Scodeggio Kartik Sheth Patrick Shopbell James Taylor Dave Thompson Neil Tyson Meg Urry Yoshi Taniguchi Ludovic Van Waerbeke Paolo Vettolani Simon White Lin Yan Alberto Franceschini Mauro Giavalisco Richard Griffiths Gigi Guzzo Gunther Hasinger Chris Impey Jean-Paul Kneib Karel Nel Jin Koda Anton Koekemoer Alexie Leauthaud Olivier LeFevre Ingo Lehmann Simon Lilly Thorsten Lisker Charles Liu Richard Massey Henry McCracken Yannick Mellier Satoshi Miyazaki Bahram Mobasher Takashi Murayama Roberto Abraham Masaru Ajiki Justin Alpert Herve Aussel Josh Barnes Marcella Brusa Daniela Calzetti Peter Capak John Carlstrom Chris Carilli Andrea Cimatti Andrea Comastri Marcella Corollo Emannuel Daddi Richard Ellis Martin Elvis Amr El Zant Shawn Ewald Mike Fall Alexis Finoguenov

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