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researcher

B. Schmidt

67 papers hereh-index 273.1k citations151 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author26
  • last author1

Across the 28 of 67 papers where every author was matched, so the position is known.

fields
  • physics.ins-det28
  • nucl-ex20
  • hep-ex8
  • astro-ph.CO5
  • astro-ph.IM3
  • cond-mat.supr-con1
same name
  • B. Schmidt — 240 papers
  • B. Schmidt — 143 papers
  • B. Schmidt — 46 papers, h 61
  • B. Schmidt — 42 papers, h 61
  • B. Schmidt — 39 papers, h 32
  • B. Schmidt — 35 papers, h 31

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20122025
most citedA search for low-mass WIMPs with EDELWEISS-II heat-and-ionization detectors

127 citations · 636 across the 43 of their papers we have counts for

collaborators
Showing 2016 · astro-ph.COShow all

3 papers · 2 filters

astro-ph.CO2016★ 5 cited

Measurement of the cosmogenic activation of germanium detectors in EDELWEISS-III

The EDELWEISS Collaboration, E. Armengaud, Q. Arnaud +46

We present a measurement of the cosmogenic activation in the germanium cryogenic detectors of the EDELWEISS III direct dark matter search experiment. The decay rates measured in de…

astro-ph.CO2016★ 66 cited

Improved EDELWEISS-III sensitivity for low-mass WIMPs using a profile likelihood approach

EDELWEISS Collaboration, L. Hehn, E. Armengaud +46

We report on a dark matter search for a Weakly Interacting Massive Particle (WIMP) in the mass range mχ​∈[4,30]GeV/c2 with the EDELWEISS-III experiment. A 2D prof…

astro-ph.CO2016

Constraints on low-mass WIMPs from the EDELWEISS-III dark matter search

EDELWEISS Collaboration, E. Armengaud, Q. Arnaud +63

We present the results of a search for elastic scattering from galactic dark matter in the form of Weakly Interacting Massive Particles (WIMPs) in the 4-30 GeV/c2 mass range. We…

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