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M. B. Bayliss

Identifiers

  • name variant M. B. Bayliss 0.60 · backfill

Papers (12)

  1. Galaxy populations in the most distant SPT-SZ clusters - I. Environmental quenching in massive clusters at $1.4\lesssim z\lesssim1.7$ astro-ph.GA · 2018 · author #6
  2. Galaxy Kinematics and Mass Calibration in Massive SZE Selected Galaxy Clusters to z=1.3 astro-ph.CO · 2017 · author #9
  3. Sunyaev-Zel'dovich Effect and X-ray Scaling Relations from Weak-Lensing Mass Calibration of 32 SPT Selected Galaxy Clusters astro-ph.CO · 2017 · author #8
  4. The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MEGaSaURA) II: Stacked Spectra astro-ph.GA · 2017 · author #2
  5. The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MEGaSaURA) I: The Sample and the Spectra astro-ph.GA · 2017 · author #2
  6. SPT-GMOS: A Gemini/GMOS-South Spectroscopic Survey of Galaxy Clusters in the SPT-SZ Survey astro-ph.CO · 2016 · author #1
  7. Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters astro-ph.CO · 2015 · author #7
  8. Time Delay Measurements for the Cluster-lensed Sextuple Quasar SDSS J2222+2745 astro-ph.CO · 2015 · author #4
  9. On the lack of correlation between Mg II 2796, 2803 Angstrom and Lyman alpha emission in lensed star-forming galaxies astro-ph.GA · 2014 · author #2
  10. SPT-CLJ2040-4451: An SZ-Selected Galaxy Cluster at z = 1.478 With Significant Ongoing Star Formation astro-ph.CO · 2013 · author #1
  11. SDSSJ2222+2745 A Gravitationally Lensed Sextuple Quasar with Maximum Image Separation of 15.1" Discovered in the Sloan Giant Arcs Survey astro-ph.CO · 2012 · author #4
  12. Early-Time Chromatic Variations in the Wind-Swept Medium of GRB 021211 and the Faintness of its Afterglow astro-ph · 2005 · author #21

Mentions

  • 1505.06187 #4 · backfill · confidence 0.70 M. B. Bayliss
  • 1406.3356 #2 · backfill · confidence 0.70 M. B. Bayliss
  • 1307.2903 #1 · backfill · confidence 0.70 M. B. Bayliss
  • 1211.1091 #4 · backfill · confidence 0.70 M. B. Bayliss

Frequent Coauthors