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researcher

D. A. García-Hernández

112 papers hereh-index 417.8k citations225 works total

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

author position
  • sole author5
  • first author21
  • middle author63
  • last author4

Across the 93 of 112 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR66
  • astro-ph.GA31
  • astro-ph12
  • astro-ph.EP2
  • astro-ph.IM1
same name
  • D. A. García-Hernández — 25 papers, h 20
  • D. A. García-Hernández — 19 papers, h 19
  • D. A. García-Hernández — 12 papers, h 3
  • D. A. García-Hernández — 9 papers, h 3
  • D. A. García-Hernández — 4 papers, h 5
  • D. A. García-Hernández — 4 papers, h 5

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
20022023
most citedThe Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment

681 citations · 7k across the 112 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.SR2023★ 15 cited

An Investigation of Non-Canonical Mixing in Red Giant Stars Using APOGEE 12C/13C Ratios Observed in Open Cluster Stars

Caroline McCormick, Steven R. Majewski, Verne V. Smith +9

Standard stellar evolution theory poorly predicts the surface abundances of chemical species in low-mass, red giant branch (RGB) stars. Observations show an enhancement of p-p chai…

astro-ph.SR2023★ 11 cited

The carbon star DY Persei may be a cool R Coronae Borealis variable

D. A. Garcia-Hernandez, N. Kameswara Rao, D. L. Lambert +3

Optical and near-IR photometry suggests that the carbon star DY Persei exhibits fadings similar to those of R Coronae Borealis (RCB) variables. Photometric surveys of the Galaxy an…

astro-ph.SR2023

The messy death of a multiple star system and the resulting planetary nebula as observed by JWST

Orsola De Marco, Muhammad Akashi, Stavros Akras +66

Planetary nebulae (PNe), the ejected envelopes of red giant stars, provide us with a history of the last, mass-losing phases of 90 percent of stars initially more massive than the…

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