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researcher

A. Jordán

96 papers hereh-index 478.1k citations227 works total

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

author position
  • first author6
  • middle author69
  • last author6

Across the 81 of 96 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP28
  • astro-ph26
  • astro-ph.CO16
  • astro-ph.GA13
  • astro-ph.HE5
  • astro-ph.SR5
same name
  • A. Jordán — 6 papers, h 5
  • A. Jordán — 5 papers, h 5
  • A. Jordán — 5 papers, h 4
  • A. Jordán — 4 papers, h 1
  • A. Jordán — 3 papers, h 3
  • A. Jordán — 2 papers, h 2

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
20032023
most citedThe ACS Virgo Cluster Survey. XIII. SBF Distance Catalog and the Three-Dimensional Structure of the Virgo Cluster

731 citations · 9.1k across the 96 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.EP2021★ 74 cited

ACCESS & LRG-BEASTS: a precise new optical transmission spectrum of the ultrahot Jupiter WASP-103b

James Kirk, Ben Rackham, Ryan MacDonald +17

We present a new ground-based optical transmission spectrum of the ultrahot Jupiter WASP-103b (Teq​=2484K). Our transmission spectrum is the result of combining five new tran…

astro-ph.EP2021★ 43 cited

Warm Jupiters in TESS Full-Frame Images: A Catalog and Observed Eccentricity Distribution for Year 1

Jiayin Dong, Chelsea X. Huang, Rebekah I. Dawson +57

Warm Jupiters -- defined here as planets larger than 6 Earth radii with orbital periods of 8--200 days -- are a key missing piece in our understanding of how planetary systems form…

astro-ph.EP2021★ 37 cited

Precise transit and radial-velocity characterization of a resonant pair: a warm Jupiter TOI-216c and eccentric warm Neptune TOI-216b

Rebekah I. Dawson, Chelsea X. Huang, Rafael Brahm +53

TOI-216 hosts a pair of warm, large exoplanets discovered by the TESS Mission. These planets were found to be in or near the 2:1 resonance, and both of them exhibit transit timing…

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