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C. Robinson

33 papers hereh-index 13481 citations40 works total

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

author position
  • first author4
  • middle author24
  • last author4

Across the 32 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR25
  • astro-ph.EP6
  • astro-ph.IM2
same name
  • C. Robinson — 21 papers, h 45
  • C. Robinson — 15 papers, h 11
  • C. Robinson — 11 papers
  • C. Robinson — 7 papers, h 7
  • C. Robinson — 4 papers, h 4
  • C. Robinson — 4 papers, h 3

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
20142026
most citedMiniature Exoplanet Radial Velocity Array (MINERVA) I. Design, Commissioning, and First Science Results

87 citations · 587 across the 32 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.EP2025

JWST-TST High Contrast: Medium-resolution spectroscopy reveals a carbon-rich circumplanetary disk around the young accreting exoplanet Delorme 1 AB b

Mathilde Mâlin, Kimberly Ward-Duong, Sierra L. Grant +21

Young accreting planetary-mass objects are thought to draw material from a circumplanetary disk (CPD) composed of gas and dust. While the gas within the disk is expected to dispers…

astro-ph.SR2025★ 1 cited

The ODYSSEUS Survey. Using accretion and stellar rotation to reveal the star-disk connection in T Tauri stars

Caeley V. Pittman, C. C. Espaillat, Zhaohuan Zhu +4

Classical T Tauri stars (CTTS) exhibit strong variability over timescales of minutes to decades. However, much theoretical work assumes that CTTS are in stable spin states. Here, w…

astro-ph.SR2025

The ODYSSEUS Survey. Characterizing magnetospheric geometries and hotspot structures in T Tauri stars

Caeley V. Pittman, C. C. Espaillat, Connor E. Robinson +20

Magnetospheric accretion is a key process that shapes the inner disks of T Tauri stars, controlling mass and angular momentum evolution. It produces strong ultraviolet and optical…

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