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researcher

C. D'Andrea

159 papers hereh-index 6219.9k citations269 works total

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

author position
  • first author4
  • middle author107
  • last author4

Across the 115 of 159 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO88
  • astro-ph.GA28
  • astro-ph.HE15
  • astro-ph.IM12
  • astro-ph11
  • astro-ph.SR3
same name
  • C. D'Andrea — 6 papers, h 35
  • C. D'Andrea — 5 papers, h 3
  • C. D'Andrea — 1 paper, h 4
  • C. D'Andrea — 1 paper, h 1

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
20002021
most citedImproved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

1.9k citations · 19.1k across the 159 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2019★ 23 cited

Identification of RR Lyrae stars in multiband, sparsely-sampled data from the Dark Energy Survey using template fitting and Random Forest classification

K. M. Stringer, J. P. Long, L. M. Macri +75

Many studies have shown that RR Lyrae variable stars (RRL) are powerful stellar tracers of Galactic halo structure and satellite galaxies. The Dark Energy Survey (DES), with its de…

astro-ph.SR2017★ 49 cited

Chemical Abundance Analysis of Three α-Poor, Metal-Poor Stars in the Ultra-Faint Dwarf Galaxy Horologium I

D. Q. Nagasawa, J. L. Marshall, J. D. Simon +68

We present chemical abundance measurements of three stars in the ultra-faint dwarf galaxy Horologium I, a Milky Way satellite discovered by the Dark Energy Survey. Using high resol…

astro-ph.SR2016★ 100 cited

DES14X3taz: A Type I Superluminous Supernova Showing a Luminous, Rapidly Cooling Initial Pre-Peak Bump

M. Smith, M. Sullivan, C. B. D'Andrea +81

We present DES14X3taz, a new hydrogen-poor super luminous supernova (SLSN-I) discovered by the Dark Energy Survey (DES) supernova program, with additional photometric data provided…

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