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Authors

Davide Bianchi

Name variants: D. Brooks · D. Bianchi

Last known institution:
Mylan (Switzerland)
ORCID:
0000-0001-9712-0006
8
h-index
6
i10-index
225
Citations
47
Works
Trends over time

Performance over time

Citation overview

Publications (bars) and citations (line) by year

  • Publications
  • Citations
013253850050100150200201520162017202220232024202520262015: Publications 1, Citations 02016: Publications 1, Citations 02017: Publications 1, Citations 02022: Publications 1, Citations 02023: Publications 1, Citations 02024: Publications 12, Citations 112025: Publications 29, Citations 2002026: Publications 1, Citations 14

Citation history

050100150200201520162017202220232024202520262015: Citations 02016: Citations 02017: Citations 02022: Citations 02023: Citations 02024: Citations 112025: Citations 2002026: Citations 14

Publication history

013253850201520162017202220232024202520262015: Publications 12016: Publications 12017: Publications 12022: Publications 12023: Publications 12024: Publications 122025: Publications 292026: Publications 1

h-index evolution

Cumulative h-index by year

035810201520162017202220232024202520262015: h-index 02016: h-index 02017: h-index 02022: h-index 02023: h-index 02024: h-index 22025: h-index 82026: h-index 8

Most-cited works

  1. DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations202526 citations
  2. DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman alpha forest202520 citations
  3. DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements20259 citations
  4. DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics20258 citations
  5. DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars20246 citations
  6. DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars20246 citations
  7. Characterization of DESI fiber assignment incompleteness effect on 2-point clustering and mitigation methods for DR1 analysis20254 citations
  8. Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples20254 citations
  9. Mitigating imaging systematics for DESI 2024 emission Line Galaxies and beyond20254 citations
  10. SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos20242 citations