pith. sign in

H. Bohringer

Identifiers

  • name variant H. Bohringer 0.60 · backfill

Papers (15)

  1. Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum astro-ph.CO · 2026 · author #187
  2. Optical validation and characterization of Planck PSZ1 sources at the Canary Islands observatories. I. First year of ITP13 observations astro-ph.CO · 2018 · author #12
  3. The far-infrared view of M87 as seen by the Herschel Space Observatory astro-ph.CO · 2010 · author #13
  4. Cluster galaxies in XMMU J2235-2557: galaxy population properties in most massive environments at z~1.4 astro-ph.CO · 2010 · author #14
  5. Feedback under the microscope: thermodynamic structure and AGN driven shocks in M87 astro-ph.CO · 2010 · author #7
  6. The Evolution of Galaxy Clusters Across Cosmic Time astro-ph.CO · 2009 · author #2
  7. X-ray Properties of Intermediate-Redshift Groups of Galaxies astro-ph · 2006 · author #5
  8. Filaments, Bubbles, and Weak Shocks in the Gaseous Atmosphere of M87 astro-ph · 2006 · author #8
  9. Radio and X-ray diffuse emission in six clusters of galaxies astro-ph · 2001 · author #4
  10. SDSS-RASS: Next Generation of Cluster-Finding Algorithms astro-ph · 2000 · author #12
  11. An XMM-Newton study of the sub-structure in M87's halo astro-ph · 2000 · author #3
  12. XEUS - The X-ray Evolving Universe Spectroscopy Mission astro-ph · 1999 · author #9
  13. X-ray/Optical analysis of the cluster of galaxies Abell 1300: Indications of a post-merger at z = 0.31 astro-ph · 1997 · author #6
  14. Dynamics of Abell 2218 from optical and near-IR imagery of arc(let)s and ROSAT/HRI X-ray map astro-ph · 1995 · author #6
  15. Cooling flows, central galaxy--cluster alignments, X-ray absorption and dust astro-ph · 1995 · author #4

Mentions

  • 2605.21436 #187 · arxiv_oai · confidence 0.70 H. Bohringer
  • 1010.0787 #13 · backfill · confidence 0.70 H. Bohringer
  • 1009.1423 #14 · backfill · confidence 0.70 H. Bohringer
  • 1006.5484 #7 · backfill · confidence 0.70 H. Bohringer
  • 0902.4890 #2 · backfill · confidence 0.70 H. Bohringer

Frequent Coauthors