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researcher

C. Robinson

3 papers here

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

author position
  • first author1
  • middle author1
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
ORCID 0000-0003-1639-510X
same name
  • C. Robinson — 11 papers
  • C. Robinson — 9 papers, h 45
  • C. Robinson — 7 papers, h 11
  • C. Robinson — 2 papers, h 2
  • C. Robinson — 1 paper, h 7
  • C. Robinson — 1 paper, h 4

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

most citedMulti-epoch Ultraviolet HST Observations of Accreting Low-mass Stars

56 citations · 93 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2019★ 15 cited

Revealing the Star-Disk-Jet Connection in GM Aur using Multiwavelength Variability

C. C. Espaillat, E. Macias, J. Hernandez +1

Here we analyze the first simultaneous X-ray, ultraviolet, optical, infrared, and centimeter observations of a T Tauri star (TTS). We present three epochs of simultaneous Spitzer a…

astro-ph.SR2019★ 22 cited

Using Multiwavelength Variability to Explore the Connection between X-ray Emission, the Far-Ultraviolet H2 Bump, and Accretion in T Tauri Stars

C. C. Espaillat, C. Robinson, S. Grant +1

The high-energy radiation fields of T Tauri stars (TTS) should affect the surrounding circumstellar disk, having implications for disk transport and heating. Yet, observational evi…

astro-ph.SR2019★ 56 cited

Multi-epoch Ultraviolet HST Observations of Accreting Low-mass Stars

Connor Robinson, Catherine Espaillat

Variability is a defining characteristic of young low-mass stars that are still accreting material from their primordial protoplanetary disk. Here we present the largest \textit{HS…

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