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B.C. Lemaux

Identifiers

  • name variant B.C. Lemaux 0.60 · backfill

Papers (15)

  1. The progeny of a Cosmic Titan: a massive multi-component proto-supercluster in formation at z=2.45 in VUDS astro-ph.CO · 2018 · author #2
  2. Evaluating Tests of Virialization and Substructure Using Galaxy Clusters in the ORELSE Survey astro-ph.GA · 2018 · author #2
  3. The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]-$\lambda$1908\AA ~emission 10.8 to 12.5 Gyr ago astro-ph.GA · 2017 · author #2
  4. The VIMOS Ultra Deep Survey: Emerging from the Dark, a Massive Proto-Cluster at z~4.57 astro-ph.GA · 2017 · author #1
  5. The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3 astro-ph.GA · 2017 · author #5
  6. Analogs of primeval galaxies two billion years after the Big Bang astro-ph.GA · 2017 · author #23
  7. New constraints on the average escape fraction of Lyman continuum radiation in z~4 galaxies from the VIMOS Ultra Deep Survey (VUDS) astro-ph.GA · 2016 · author #8
  8. Dust properties of Lyman break galaxies at $z\sim3$ astro-ph.GA · 2015 · author #14
  9. The Lyman Continuum escape fraction of galaxies at z=3.3 in the VUDS-LBC/COSMOS field astro-ph.GA · 2015 · author #27
  10. The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3 astro-ph.CO · 2014 · author #8
  11. The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS) astro-ph.CO · 2014 · author #8
  12. The evolving SFR-M_star relation and sSFR since z~5 from the VUDS spectroscopic survey astro-ph.GA · 2014 · author #7
  13. VIMOS Ultra-Deep Survey (VUDS): Witnessing the Assembly of a Massive Cluster at z~3.3 astro-ph.CO · 2014 · author #1
  14. Submillimetre Source Counts in the Fields of High-Redshift Galaxy Clusters astro-ph.CO · 2011 · author #11
  15. The Observations of Redshift Evolution in Large Scale Environments (ORELSE) Survey : I. The Survey Design and First Results on Cl 0023+0423 at z = 0.84 and RX J1821.6+6827 at z = 0.82 astro-ph · 2008 · author #3

Mentions

  • 1509.01101 #27 · backfill · confidence 0.70 B.C. Lemaux
  • 1412.5584 #8 · backfill · confidence 0.70 B.C. Lemaux
  • 1411.5688 #8 · backfill · confidence 0.70 B.C. Lemaux
  • 1411.5687 #7 · backfill · confidence 0.70 B.C. Lemaux
  • 1403.4230 #1 · backfill · confidence 0.70 B.C. Lemaux
  • 1109.5125 #11 · backfill · confidence 0.70 B.C. Lemaux
  • 0809.2092 #3 · backfill · confidence 0.70 B.C. Lemaux

Frequent Coauthors