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V. Zema

45 papers hereh-index 15636 citations72 works total

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

author position
  • first author2
  • middle author18
  • last author10

Across the 30 of 45 papers where every author was matched, so the position is known.

fields
  • physics.ins-det19
  • astro-ph.CO11
  • hep-ph9
  • astro-ph.IM3
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • V. Zema — 4 papers
  • V. Zema — 1 paper, h 0

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
20142026
most citedFirst results from the CRESST-III low-mass dark matter program

511 citations · 988 across the 44 of their papers we have counts for

collaborators
Showing 2026Show all

4 papers · 1 filter

physics.ins-det2026

Optimization studies of silicon remoTES cryogenic calorimeters

G. Angloher, M. R. Bharadwaj, A. Boehmer +42

The remoTES design, developed within the COSINUS experiment, enables a broader range of materials to be operated as cryogenic calorimeters read out with Transition Edge Sensors (TE…

physics.ins-det2026

The relative interfacial thermal contraction as a possible origin of the low-energy excess in cryogenic calorimeters

Vanessa Zema, Pasquale Pavone

Low threshold cryogenic calorimeters are a key technology for the advancement of rare-event searches. However, since a few years their sensitivity reach is challenged by the presen…

physics.ins-det2026

Optimisation of TES design for the CRESST experiment

G. Angloher, S. Banik, A. Bento +54

The CRESST experiment aims at the direct detection of sub-GeV dark matter particles via elastic scattering off nuclei in different target crystals at cryogenic temperatures. The ad…

hep-ph2026

Cosmic Ray Boosted Dark Matter in COSINUS: Modeling and Constraints

G. Angloher, M. R. Bharadwaj, A. Böhmer +41

Direct detection of nuclear recoils due to sub-GeV dark matter is challenging because of the small kinetic energy of the light dark matter particles. Although limits down to a few…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.