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S. Salimbeni

Identifiers

  • name variant S. Salimbeni 0.60 · backfill

Papers (17)

  1. The evolution of the AGN content in groups up to z~1 astro-ph.CO · 2013 · author #4
  2. The evolving slope of the stellar mass function at 0.6 <= z < 4.5 from deep WFC3 data astro-ph.CO · 2011 · author #4
  3. An X-ray underluminous cluster of galaxies in the 4Ms CDFS observations astro-ph.CO · 2011 · author #6
  4. The bright end of the z ~ 7 UV Luminosity Function from a wide and deep HAWK-I survey astro-ph.CO · 2010 · author #25
  5. The Morphology of Passively Evolving Galaxies at z ~ 2 from HST/WFC3 Deep Imaging in the Hubble Ultradeep Field astro-ph.CO · 2009 · author #8
  6. Evidence for a fast evolution of the UV luminosity function beyond redshift 6 from a deep HAWK-I survey of the GOODS-S field astro-ph.CO · 2009 · author #22
  7. A Comprehensive Study of Large Scale Structures in the GOODS-SOUTH Field up to z \sim 2.5 astro-ph.CO · 2009 · author #1
  8. Uncertainties and Systematic Effects on the estimate of stellar masses in high z galaxies astro-ph.CO · 2009 · author #1
  9. The Fraction of Quiescent Massive Galaxies in the Early Universe astro-ph.GA · 2009 · author #9
  10. The physical properties of Lyalpha emitting galaxies: not just primeval galaxies? astro-ph · 2008 · author #6
  11. Large Scale Structures at High Redshift in the GOODS Field astro-ph · 2008 · author #2
  12. A Photometrically Detected Forming Cluster of Galaxies at Redshift 1.6 in the GOODS Field astro-ph · 2007 · author #2
  13. Physical properties of z~4 LBGs: differences between galaxies with and without Ly-alpha emission astro-ph · 2007 · author #4
  14. The Abundance of Distant and Extremely Red Galaxies: The Role of AGN Feedback in Hierarchical Models astro-ph · 2006 · author #5
  15. The B-Band Luminosity Function of Red and Blue Galaxies up to z=3.5 astro-ph · 2004 · author #2
  16. The K20 survey. VI. The Distribution of the Stellar Masses in Galaxies up to z~2 astro-ph · 2004 · author #12
  17. The evolution of the galaxy luminosity function in the rest frame blue band up to z=3.5 astro-ph · 2003 · author #10

Mentions

  • 1007.5396 #25 · backfill · confidence 0.70 S. Salimbeni
  • 0911.1158 #8 · backfill · confidence 0.70 S. Salimbeni
  • 0909.2853 #22 · backfill · confidence 0.70 S. Salimbeni
  • 0903.3952 #1 · backfill · confidence 0.70 S. Salimbeni
  • 0901.3540 #1 · backfill · confidence 0.70 S. Salimbeni
  • 0901.2898 #9 · backfill · confidence 0.70 S. Salimbeni
  • 0811.1861 #6 · backfill · confidence 0.70 S. Salimbeni
  • 0801.3557 #2 · backfill · confidence 0.70 S. Salimbeni
  • 0707.1783 #2 · backfill · confidence 0.70 S. Salimbeni

Frequent Coauthors