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J. de Vicente

150 papers hereh-index 191.5k citations85 works total

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

author position
  • first author1
  • middle author96
  • last author3

Across the 100 of 150 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO77
  • astro-ph.GA41
  • astro-ph.IM12
  • astro-ph.HE9
  • astro-ph.EP6
  • astro-ph.SR3
same name
  • J. De Vicente — 10 papers
  • J. de Vicente — 6 papers, h 2
  • J. De Vicente — 2 papers
  • J. De Vicente — 1 paper
  • J. de Vicente — 1 paper, h 6
  • J. de Vicente — 1 paper, h 14

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
20082026
most citedDark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

1.2k citations · 8.6k across the 143 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2023★ 10 cited

Ultracool dwarfs candidates based on six years of the Dark Energy Survey data

M. dal Ponte, B. Santiago, A. Carnero Rosell +57

We present a sample of 19,583 ultracool dwarf candidates brighter than z ≤23 selected from the Dark Energy Survey DR2 coadd data matched to VHS DR6, VIKING DR5 and AllWISE co…

astro-ph.SR2020★ 35 cited

Chemical Analysis of the Ultra-Faint Dwarf Galaxy Grus~II. Signature of high-mass stellar nucleosynthesis

T. T. Hansen, J. L. Marshall, J. D. Simon +59

We present a detailed abundance analysis of the three brightest member stars at the top of the giant branch of the ultra-faint dwarf galaxy Grus~II. All stars exhibit a higher than…

astro-ph.SR2020★ 8 cited

Increasing the census of L and T dwarfs in wide binary and multiple systems using Dark Energy Survey DR1 and Gaia DR2 data

M. dal Ponte, B. Santiago, A. Carnero Rosell +57

We present the discovery of 255 binary and six multiple system candidates with wide > 5" separation composed by ultracool dwarfs companions to stars, plus nine double ultracool dwa…

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